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NASA Wallops to Launch Three Sounding Rockets During Solar Eclipse
Three Black Brant IX sounding rockets for the Atmospheric Perturbations around Eclipse Path (APEP) mission are scheduled to launch from NASA’s Wallops Flight Facility launch range in Virginia. The launch window opens April 8, 2024, at 2:40 p.m. EDT.
Launching approximately 45 minutes before, during, and after the peak local eclipse, the APEP sounding rockets will study how Earth’s upper atmosphere is affected when sunlight momentarily dims over a portion of the planet. Targeted launch times for the three rockets are 2:40 p.m., 3:20 p.m., and 4:05 p.m. but may be subject to change.
The launches will be livestreamed on Wallops’ YouTube beginning at 2:30 p.m.
Weather permitting, the launches may be visible in the mid-Atlantic region. Remember to always wear solar safety or “eclipse” glasses when looking at the Sun to protect your eyes. For the Wallops area, the eclipse will begin around 2:06 p.m. The Moon will block 81.4% of the Sun’s light at peak local eclipse at 3:23 p.m. and conclude at 4:34 p.m.
Launch viewing map forAtmospheric Perturbations around Eclipse Path mission are scheduled to launch from NASA’s launch range at Wallops Flight Facility in Virginia on April 8, 2024.Credit: NASAMembers of the public are invited to the NASA Wallops Visitor Center on Monday, April 8, to view the sounding rocket launches and the partial eclipse. Gates to the visitor center will open from 1-5 p.m. and will close once parking lot capacity is reached. For those traveling to our visitor center, all vehicles MUST fit within a standard parking spot for this event; no large, oversized vehicles or buses will be allowed for entry.
The visitor center will offer solar-related activities, have NASA sounding rocket experts onsite to answer questions, and host Globe Program expert Brian Campbell, who will be showing people how to collect data during the eclipse using the Observer app. Eclipse glasses and pinhole viewers will be available during this event while supplies last. Food trucks will be onsite serving food and drinks, including empanadas, crab cakes, hamburgers, hot dogs, barbecue, water ice, and more.
While this combined viewing event is exciting for some, it may not be ideal for all. A designated sensory-friendly quiet area will be available at the Wallops Visitor Center for guests. This supervised quiet area will include dimmed lighting, seating, a reflection area, and touch items for guests to explore.
Prepare for safe solar viewing during this year’s eclipse by checking out NASA’s Eclipse Safety page.
Media Contact
Amy Barra
NASA’s Wallops Flight Facility, Wallops Island, Virginia
NASA will launch three sounding rockets during the total solar eclipse on April 8, 2024,…
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Article 3 days agoAdvances in Understanding COPV Structural Life
The Structures Technical Discipline Team (TDT) was involved in numerous investigations this past year, but composites, fracture mechanics, and pressure vessels dominate the list. All three of these specialties are important to composite overwrapped pressure vessels (COPV). One of the TDT’s most important findings this year was the exposure of an inherent vulnerability that underpredicts structural life, driven by current specifications and testing standards for COPVs. This NESC work and its recommendations will significantly improve safety and mission success for all current and future COPV operations throughout the aerospace community.
Dr. David Dawicki employs digital image correlation to evaluate strain in metallic coupons.Damage Tolerance Analysis Standard Can Be Unconservative for COPVs
COPVs consist of a metallic liner that contains the fluid or gas and a composite overwrap that provides strength (Figure 1). The operational pressure cycles for a spaceflight COPV generally starts with an initial overpressure, called an autofrettage cycle, that yields the metallic liner, while the stronger composite overwrap remains elastic. Liner yielding during autofrettage results in a small amount of liner growth, resulting in liner compression when the COPV is depressurized after autofrettage. The subsequent operational cycles can be either elastic (elastically responding COPV) or elastic-plastic (plastically responding COPV).
Figure 1.Illustration of COPV major components.The damage tolerance life evaluation of spaceflight COPVs is governed by the ANSI/AIAA-S-081B, Space Systems–Composite Overwrapped Pressure Vessels. This standard provides the baseline requirements for damage tolerance analyses (DTA) of COPVs with elastically responding liners. The standard allows the DTA to consider the influence of the elastic-plastic autofrettage cycle independently of the elastically responding cycles. The elastically responding cycles are permitted to be analyzed using linear elastic fracture mechanics (LEFM) tools like the NASGRO crack-growth analysis software. The standard states that the DTA must not consider any beneficial influences of the autofrettage cycle on the subsequent elastically responding cycles but does not consider the possibility of detrimental influences of the autofrettage cycle.
In the study, Unconservatism of Linear-Elastic Fracture Mechanics Analysis Post Autofrettage (NASA/TM-20230013348), an NESC team conducted a combined experimental and analytical investigation into the influence of the autofrettage cycle on subsequent elastic cycles. Tests were conducted on coupons with part-through surface cracks that were subjected to cyclic loading that was representative of the operational cycles of a COPV liner. Half of the tests were conducted with the full loading history (including the autofrettage cycle) and the other half were identical except that the autofrettage cycle was omitted. Cracks in the tests with the autofrettage cycle grew faster than cracks in the identical tests that excluded the autofrettage cycle, as shown by the fracture surfaces in the photomicrographs (Figure 2). The distance between the mark left by the autofrettage cycle and the ductile fracture region was the amount of crack growth (Δa=0.0077 inch) due to the LEFM cycles. Crack growth due to the LEFM cycles in the LEFM-only test was Δa=0.0022 inch, more than three times slower than that in the identical autofrettage plus LEFM test.
Figure 2. Fracture surfaces from two identical tests showing crack growth (Δa), with and without an initial autofrettage cycle.
A validated finite element analysis and experimental measurements were used to evaluate the influence of the autofrettage cycle. The elastic-plastic autofrettage cycle was found to create a large region of plastic deformation ahead of the crack and blunted the crack tip. Previous fracture mechanics tests and analytical studies in the literature examined elastic overloads and found that plastic deformation ahead of the crack developed residual stresses that closed the crack surfaces, reducing the subsequent crack growth rate. However, the crack blunting allowed the crack to remain open for the entire loading, as illustrated by the finite element simulations of the crack surfaces at peak and minimum stress (Figure 3). The differences between the tests with and without the autofrettage cycle that were observed experimentally and simulated with a validated finite element analysis indicate that the damage tolerance analysis approach allowed by the standard can be unconservative. The NESC proposed an alternative damage tolerance analysis approach and recommended that the AIAA Aerospace Pressure Vessel Committee on standards update the ANSI/AIAA S-081B standard to address COPV liners with compressive stresses following the peak autofrettage stress.
Figure 3. Abaqus finite element analysis of crack growth with and without an autofrettage cycle. Y-axis indicates crack opening displacement and x-axis indicates crack length.
A Brief Introduction to Damage Tolerance for COPVs
ANSI/AIAA S-081B standard, Space Systems–Composite Overwrapped Pressure Vessels, is a compilation of accepted practices for COPVs used in space applications developed as a collaboration of industry, government, and universities. The standard covers many aspects of COPVs including damage tolerance life analyses that are used for flight qualification overseen by fracture control boards. The standard for damage tolerance requires that the COPV “…survive four operational lifetimes with the largest crack in the metallic liner that can be missed by a nondestructive evaluation (NDE) subjected to bounding stresses representative of what the COPV experiences in its life (manufacturing, integration, operational including thermal and residual).” The operational life of a COPV liner typically includes an initial elastic-plastic cycle (autofrettage or proof) followed by other cycles that may be elastic (elastically responding liners) or elastic-plastic (plastically responding liners). A representative load spectrum is shown at right. During autofrettage, the COPV is pressurized to at least proof pressure to compress the liner inner surface, making it less susceptible to operational stresses. COPVs with elastically responding liners may be damage-tolerance qualified using LEFM analysis tools, but plastically responding liners must be damage-tolerance qualified by testing. Guidance on evaluating the appropriateness of LEFM tools for COPV damage tolerance was provided in NESC Technical Bulletin No. 21-04, Evaluating Appropriateness of LEFM Tools for COPV and Metal Pressure Vessel Damage Tolerance Life Verification Tolerance Life Verification and NASA/TM-2020-5006765/Volumes 1/2.
A COPV consists of a metallic liner with an exterior composite wrap. The composite provides strength, and the liner contains the compressed fluid or gas. Results of a failure test. COPVs contain high pressure gases or fluids that can have tremendous explosive energy.Future of the Structures Discipline
As the Agency moves more toward forming strategic industry partnerships with commercial contracts for new programs, the Structures TDT has highlighted the need for proper focus on appropriate requirements as the Team’s strategic vector. Although NASA Standards are often provided for reference, their prescriptive nature is not necessarily appropriate for use with commercial contracts. Industry partners and/or NASA team members create alternative standards, unique for each program, but there is inconsistency across different programs with respect to detailed requirements in these standards. Emerging technologies such as soft goods, large-scale deployable structures, inflatables, probabilistic analysis techniques, and additive manufactured hardware all drive unique requirements. The TDT identified the need for a tailoring guide, tied to mission priorities and risk postures, to assist with insight/oversight strategies for NASA programs. Using industry partners also means less NASA-owned hardware, which can lead to a loss of institutional knowledge.
Representative loading spectrum for an elastically responding COPV liner with an initial elastic-plastic cycle.Its imperative that Engineering Directorates at each center proactively look for in-house projects so the next generation of engineers have opportunities for hands-on experience developing, designing, and testing (DDT) flight hardware. This experience is the foundation necessary for NASA engineers to guide the commercial partners through their own DDT processes and to be able to provide appropriate verification and validation of NASA requirements. Structures TDT members form a diverse team crossing all centers and programs, facilitating good collaboration on requirement interpretation, which ultimately ensures safety of NASA crew and mission success of operations in these new commercial programs.
Computed tomography scan of a metallic liner detecting a part-through crack.Harnessing the 2024 Eclipse for Ionospheric Discovery with HamSCI
3 min read
Harnessing the 2024 Eclipse for Ionospheric Discovery with HamSCIAs the total solar eclipse on April 8, 2024, draws closer, a vibrant community of enthusiastic amateur radio operators, known as “hams,” is gearing up for an exciting project with the Ham Radio Science Citizen Investigation (HamSCI) group. Our goal is clear and ambitious: to use the Moon’s shadow as a natural laboratory to uncover the intricacies of the ionosphere, a layer of Earth’s atmosphere crucial for radio communication.
This rare event offers an unmatched opportunity to observe the ionosphere’s response to the temporary absence of solar radiation during the eclipse. HamSCI, a collective of citizen scientists and professional researchers, plans to seize this opportunity by conducting radio experiments across North America.
This image captures the Moon passing in front of the Sun during an eclipse on Jan. 30, 2014, seen in space by NASA’s Solar Dynamics Observatory. NASA/SDOOur mission centers on two main activities: the Solar Eclipse QSO Party (SEQP) and the Gladstone Signal Spotting Challenge. For the SEQP, amateur radio operators across the continent will aim to establish as many radio contacts (called QSOs) as possible before, during, and after the eclipse, creating a lively scene filled with radio signals. This effort will generate a vast network of observations on radio wave behavior under the eclipse’s unique conditions. The SEQP, a competitive yet friendly event, encourages wide participation and adds an element of excitement.
The Gladstone Signal Spotting Challenge, named in honor of ham radio operator Philip Gladstone for his significant contributions to radio science, adopts a focused approach. Participants will use special equipment to monitor select radio frequencies, aiding in our observation of the ionosphere’s reaction to the eclipse. This crucial aspect of our project validates scientific models of the ionosphere and enriches our understanding of its interaction with solar radiation.
Amateur radio enthusiasts of all backgrounds and skill levels are invited to join these events, united by a shared enthusiasm for scientific exploration and a collective curiosity about the upper atmosphere. Through the support of the amateur radio community, HamSCI demonstrates the profound impact of citizen science in contributing to our scientific knowledge.
As the eclipse ends, our analytical work begins. We will delve into the collected data, interpret it, and publish our findings. These efforts are expected to significantly advance our understanding of the ionosphere and showcase the value of community involvement in scientific discovery.
HamSCI is an organization that aims to inspire wonder and encourage people to participate in scientific discovery. The community of citizen scientists associated with HamSCI believe that the seamless fusion of science and amateur radio is an excellent example of what can be achieved when people come together, driven by curiosity and a passion for exploration.
For more information about HamSCI and details on the SEQP and the Gladstone Signal Spotting Challenge, please visit:
- HamSCI’s Eclipse Information: https://hamsci.org/eclipse
- Contest Information: https://hamsci.org/contest-info
By McKenzie Denton
HamSCI Citizen Science Team Member
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How NASA’s Roman Telescope Will Measure Ages of Stars
Guessing your age might be a popular carnival game, but for astronomers it’s a real challenge to determine the ages of stars. Once a star like our Sun has settled into steady nuclear fusion, or the mature phase of its life, it changes little for billions of years. One exception to that rule is the star’s rotation period – how quickly it spins. By measuring the rotation periods of hundreds of thousands of stars, NASA’s Nancy Grace Roman Space Telescope promises to bring new understandings of stellar populations in our Milky Way galaxy after it launches by May 2027.
Stars are born spinning rapidly. However, stars of our Sun’s mass or smaller will gradually slow down over billions of years. That slowdown is caused by interactions between a stream of charged particles known as the stellar wind and the star’s own magnetic field. The interactions remove angular momentum, causing the star to spin more slowly, much like an ice skater will slow down when they extend their arms.
This effect, called magnetic braking, varies depending on the strength of the star’s magnetic field. Faster-spinning stars have stronger magnetic fields, which causes them to slow down more rapidly. Due to the influence of these magnetic fields, after about one billion years stars of the same mass and age will spin at the same rate. Therefore, if you know a star’s mass and rotation rate, you potentially can estimate its age. By knowing the ages of a large population of stars, we can study how our galaxy formed and evolved over time.
Measuring Stellar Rotation
How do astronomers measure the rotation rate of a distant star? They look for changes in the star’s brightness due to starspots. Starspots, like sunspots on our Sun, are cooler, darker patches on a star’s surface. When a starspot is in view, the star will be slightly dimmer than when the spot is on the far side of the star.
This image of our Sun was taken in August 2012 by NASA’s Solar Dynamics Observatory. It shows a number of sunspots. Other stars also experience starspots, which cause the star’s observed brightness to vary as the spots rotate in and out of view. By measuring those changes in brightness, astronomers can infer the star’s rotation period. NASA’s Nancy Grace Roman Space Telescope will collect brightness measurements for hundreds of thousands of stars located in the direction of the center of our Milky Way galaxy, yielding information about their rotation rates.Credit: NASAIf a star has a single, large spot on it, it would experience a regular pattern of dimming and brightening as the spot rotated in and out of view. (This dimming can be differentiated from a similar effect caused by a transiting exoplanet.) But a star can have dozens of spots scattered across its surface at any one time, and those spots vary over time, making it much more difficult to tease out periodic signals of dimming from the star’s rotation.
Applying Artificial Intelligence
A team of astronomers at the University of Florida is developing new techniques to extract a rotation period from measurements of a star’s brightness over time, through a program funded by NASA’s Nancy Grace Roman Space Telescope project.
They are using a type of artificial intelligence known as a convolutional neural network to analyze light curves, or plots of a star’s brightness over time. To do this, the neural network first must be trained on simulated light curves. University of Florida postdoctoral associate Zachary Claytor, the science principal investigator on the project, wrote a program called “butterpy” to generate such light curves.
A star can have dozens of spots scattered across its surface at any one time, causing irregular brightness fluctuations that make it difficult to tease out periodic signals of dimming due to the star’s rotation. This graph of data from the butterpy program shows how the observed brightness of a simulated star would vary over a single rotation period. NASA’s Roman Space Telescope will be able to measure the light curves, and therefore rotation rates, of hundreds of thousands of stars, bringing new insights into stellar populations in our galaxy.Credit: NASA, Ralf Crawford (STScI)“This program lets the user set a number of variables, like the star’s rotation rate, the number of spots, and spot lifetimes. Then it will calculate how spots emerge, evolve, and decay as the star rotates and convert that spot evolution to a light curve – what we would measure from a distance,” explained Claytor.
The team has already applied their trained neural network to data from NASA’s TESS (Transiting Exoplanet Survey Satellite). Systematic effects make it more challenging to accurately measure longer stellar rotation periods, yet the team’s trained neural network was able to accurately measure these longer rotation periods using the TESS data.
Roman’s Star Survey
The upcoming Roman Space Telescope will gather data from hundreds of millions of stars through its Galactic Bulge Time Domain Survey, one of three core community surveys it will conduct. Roman will look toward our galaxy’s center – a region crowded with stars – to measure how many of these stars change in brightness over time. These measurements will enable multiple science investigations, from searching for distant exoplanets to determining the stars’ rotation rates.
The specific survey design is still being developed by the astronomical community. The NASA-funded study on stellar rotation promises to help inform potential survey strategies.
“We can test which things matter and what we can pull out of the Roman data depending on different survey strategies. So when we actually get the data, we’ll already have a plan,” said Jamie Tayar, assistant professor of astronomy at the University of Florida and the program’s principal investigator.
“We have a lot of the tools already, and we think they can be adapted to Roman,” she added.
The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA’s Jet Propulsion Laboratory and Caltech/IPAC in Southern California, the Space Telescope Science Institute in Baltimore, and a science team comprising scientists from various research institutions. The primary industrial partners are BAE Systems, Inc. in Boulder, Colorado; L3Harris Technologies in Melbourne, Florida; and Teledyne Scientific & Imaging in Thousand Oaks, California.
By Christine Pulliam
Space Telescope Science Institute, Baltimore, Md.
Media Contact:
Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, Md.
301-286-1940
Christine Pulliam
Space Telescope Science Institute, Baltimore, Md.
NASA Achieves Milestone for Engines to Power Future Artemis Missions
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA conducted a full-duration RS-25 hot fire April 3 on the Fred Haise Test Stand at NASA’s Stennis Space Center near Bay St. Louis, Mississippi, achieving a major milestone for future Artemis flights of NASA’s SLS (Space Launch System) rocket. It marked the final test of a 12-test series to certify production of new RS-25 engines by lead contractor Aerojet Rocketdyne, an L3Harris Technologies company, to help power NASA’s SLS rocket on Artemis missions to the Moon and beyond, beginning with Artemis V. NASA/Danny Nowlin Crews transport RS-25 developmental engine E0525 to the Fred Haise Test Stand at NASA’s Stennis Space Center on Aug. 30, 2023, for the second and final certification test series.NASA/Danny Nowlin A crane lifts developmental engine E0525 onto the Fred Haise Test Stand at NASA’s Stennis Space Center on Aug. 30, 2023, in preparation for a series of 12 tests to collect performance data for lead SLS (Space Launch System) engines contractor Aerojet Rocketdyne, an L3Harris Technologies company, to produce engines that will help power the SLS rocket, beginning with Artemis V.NASA/Danny Nowlin Crews prepare to place RS-25 engine E0525 on the engine vertical installer on the Fred Haise Test Stand at NASA’s Stennis Space Center on Aug. 30, 2023. NASA/Danny Nowlin Team members ready RS-25 engine E0525 for full installation on the Fred Haise Test Stand at NASA’s Stennis Space Center on Aug. 30, 2023, for a second certification test series to collect data for the final RS-25 design certification review.NASA/Danny Nowlin The second – and final – RS-25 certification test series begins Oct. 17, 2023. When the liquid hydrogen and liquid oxygen propellants mix and ignite, an extremely high temperature exhaust, of up to 6,000-degrees Fahrenheit, mixes with water to form steam that exits the flame deflector and rises into the atmosphere, forming a cloud that subsequently cools.NASA/Danny Nowlin A cloud of steam is visible at NASA’s Stennis Space Center during an Oct. 17, 2023, hot fire that marks the first test in the critical series to support future SLS (Space Launch System) missions to deep space.NASA/Danny Nowlin An RS-25 hot fire at NASA’s Stennis Space Center on Nov. 15, 2023, marks the second test of a 12-test engine certification series. The NASA Stennis test team typically fires the certification engine for 500 seconds, the same amount of time engines must fire to help launch the SLS (Space Launch System) rocket to space with astronauts aboard the Orion spacecraft. NASA/Danny Nowlin Operators fire the RS-25 engine at NASA’s Stennis Space Center on Nov. 15, 2023, up to the 113% power level. The first four Artemis missions are using modified space shuttle main engines that can power up to 109% of their rated level. New RS-25 engines will power up to the 111% level to provide additional thrust, so testing up to the 113% power level provides a margin of operational safety.NASA/Danny Nowlin NASA demonstrates a key RS-25 engine capability necessary for flight of the SLS (Space Launch System) rocket during a hot fire on Nov. 29, 2023. Crews gimbaled, or pivoted, the RS-25 engine around a central point during the almost 11-minute (650 seconds) hot fire on the Fred Haise Test Stand at NASA’s Stennis Space Center.NASA/Danny Nowlin The first RS-25 engine test of 2024 takes place on Jan. 17, 2024, at NASA’s Stennis Space Center as crews complete a 500-second hot fire on the Fred Haise Test Stand. NASA/Danny Nowlin A remote field camera offers a head-on view of an RS-25 engine hot fire on the Fred Haise Test Stand at NASA’s Stennis Space Center on Jan. 23, 2024.NASA/Danny Nowlin NASA marks the halfway point of its second RS-25 certification series on Jan. 27, 2024, with the sixth test of the series on the Fred Haise Test Stand at NASA’s Stennis Space Center. For each Artemis mission, four RS-25 engines, along with a pair of solid rocket boosters, power the SLS (Space Launch System) rocket, producing more than 8.8 million pounds of thrust at liftoff. NASA/Danny Nowlin Teams at NASA’s Stennis Space Center install a second production nozzle, left, on Feb. 6, 2024, to gather additional performance data on the RS-25 certification engine at the Fred Haise Test Stand.NASA/Danny Nowlin A new RS-25 engine production nozzle is lifted on the Fred Haise Test Stand at NASA’s Stennis Space Center on Feb. 6, 2024. Crews used specially adapted procedures and tools to swap out the nozzles with the engine in place on the stand.NASA/Danny Nowlin Operators fire RS-25 engine E0525 for 550 seconds and up to a power level of 113% on the Fred Haise Test Stand at NASA’s Stennis Space Center on Feb. 23, 2024. The hot fire test was the first featuring a new engine nozzle, allowing engineers to collect and compare performance data on a second production unit.NASA/Danny Nowlin The third RS-25 hot fire of 600 seconds or more is conducted March 6, 2024, at NASA’s Stennis Space Center. The full-duration test on the Fred Haise Test Stand marked the ninth in a 12-test certification series for production of new engines to help power NASA’s SLS (Space Launch System) rocket on Artemis missions to the Moon and beyond, beginning with Artemis V. NASA/Danny Nowlin The test team at NASA’s Stennis Space Center conduct the first RS-25 hot fire of spring 2024 on March 22, powering the engine for a full duration 500 seconds and up to a power level of 113%.NASA/Danny Nowlin NASA closes in on a milestone for production of new RS-25 engines to help power future Artemis missions to the Moon and beyond following a successful full duration test on March 27, 2024, at NASA’s Stennis Space Center. The hot fire marked the 11th test of a 12-test series.NASA/Danny Nowlin NASA conducted a full-duration RS-25 hot fire April 3 on the Fred Haise Test Stand at NASA’s Stennis Space Center near Bay St. Louis, Mississippi.NASA/Danny NowlinNASA achieved a major milestone April 3 for production of new RS-25 engines to help power its Artemis campaign to the Moon and beyond with completion of a critical engine certification test series at NASA’s Stennis Space Center near Bay St. Louis, Mississippi.
The 12-test series represents a key step for lead engines contractor Aerojet Rocketdyne, an L3Harris Technologies company, to build new RS-25 engines, using modern processes and manufacturing techniques, for NASA’s SLS (Space Launch System) rockets that will power future lunar missions, beginning with Artemis V.
“The conclusion of the certification test series at NASA Stennis is just the beginning for the next generation of RS-25 engines that will help power human spaceflight for Artemis,” said Johnny Heflin, SLS liquid engines manager. “The newly produced engines on future SLS rockets will maintain the high reliability and safe flight operational legacy the RS-25 is known for while enabling more affordable high-performance engines for the next era of deep space exploration.”
Through Artemis, NASA will establish the foundation for long-term scientific exploration at the Moon; land the first woman, first person of color, and first international partner astronaut on the lunar surface; and prepare for human expeditions to Mars for the benefit of all.
Contributing to that effort, the NASA Stennis test team conducted a full-duration, 500-second hot fire to complete the 12-test series on developmental engine E0525, providing critical performance data for the final RS-25 design certification review. The April 3 hot fire completed a test series that began in October 2023.
RS-25 engines are evolved space shuttle main engines, upgraded with new components to produce the additional power needed to help launch NASA’s SLS rocket. The first four Artemis missions are using modified space shuttle main engines also tested at NASA Stennis. For each Artemis mission, four RS-25 engines, along with a pair of solid rocket boosters, power the SLS rocket, producing more than 8.8 million pounds of total combined thrust at liftoff.
“This was a critical test series, and credit goes to the entire test team for their dedication and unique skills that allowed us to meet the schedule and provide the needed performance data,” said Chip Ellis, project manager for RS-25 testing at NASA Stennis. “The tests conducted at NASA Stennis help ensure the safety of our astronauts and their future mission success. We are proud to be part of the Artemis mission.”
The E0525 developmental engine featured new key components – including a nozzle, hydraulic actuators, flex ducts, and turbopumps – that matched design features of those used during an initial certification test series completed at NASA Stennis last summer.
The two certification test series helped verify the new engine components meet all Artemis flight requirements moving forward. Aerojet Rocketdyne is using techniques such as 3D printing to produce new RS-25 engines more efficiently, while maintaining high performance and reliability. NASA has awarded the company contracts to provide 24 new engines, supporting SLS launches for Artemis V through Artemis IX.
“Successfully completing this rigorous test series is a testament to the outstanding work done by the team to design, implement and test this upgraded version of the RS-25 that reduces the cost by 30% from the space shuttle program,” said Mike Lauer, RS-25 program director at Aerojet Rocketdyne. “We tested the new RS-25 engines to the extreme limits of operation to ensure the engines can operate at a higher power level needed for SLS and complete the mission with margin.”
RS-25 Final Certification Test Series by the NumbersAll RS-25 engines are tested and proven flightworthy at NASA Stennis prior to use on Artemis missions. RS-25 tests at the center are conducted by a diverse team of operators from NASA, Aerojet Rocketdyne, and Syncom Space Services, prime contractor for site facilities and operations.
Facebook logo @NASASTENNIS @NASASTENNIS Instagram logo @NASASTENNIS Share Details Last Updated Apr 04, 2024 EditorNASA Stennis CommunicationsContactC. Lacy Thompsoncalvin.l.thompson@nasa.gov / (228) 688-3333LocationStennis Space Center Related Terms Explore More 3 min read NASA to Continue Testing for New Artemis Moon Rocket Engines Article 1 month ago 2 min read NASA Marks Halfway Point for Artemis Moon Rocket Engine Certification Series Article 2 months ago 3 min read NASA Stennis Continues Preparations for Future Artemis Testing Article 4 months ago Keep Exploring Discover More Topics from NASA StennisDoing Business with NASA Stennis
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Eclipses Near and Far
On April 8, 2024, North America will witness its last total solar eclipse for more than twenty years. Other parts of the world will experience the rare celestial event in the coming decade. A total solar eclipse occurs when the Moon passes directly between the Sun and the Earth, blocking its disk from view but making its corona visible in a dazzling display. Although spectacular when seen from the ground, observed from space, solar eclipses appear as large shadows moving across the face of the Earth. The unique geometry of the Earth-Sun-Moon system allows total solar eclipses to occur. Eclipses also occur outside the Earth-Moon system, although the geometries of those worlds rarely if ever produce the stunning display visible on Earth. Spacecraft exploring other worlds have documented these extraterrestrial eclipses.
Left: Schematic geometry of a solar eclipse; sizes and distances not to scale. Right: Path of the April 8, 2024, total solar eclipse. Image credit: courtesy Sky & Telescope.
A solar eclipse occurs when the Moon passes between the Sun and the Earth, with the Moon casting its shadow on its home planet. Although the Sun is much larger than the Moon, it is also much farther away. As seen from Earth, the Sun and Moon have roughly the same angular diameter and appear roughly the same size in the sky. A total eclipse occurs when the Moon blocks out the Sun’s disk entirely. Because the Moon does not orbit in a perfect circle around the Earth, it appears smaller at its farthest point thus creating annular eclipses. Moons around other planets can also create eclipses although their different sizes relative to the Sun do not create our familiar eclipses. Planets with multiple moons can have more than one eclipse occur at the same time.
Left: Gemini XII astronauts photograph the total solar eclipse from Earth orbit in November 1966. Middle: Surveyor 3 observes a solar eclipse from the Moon in April 1967. Right: In November 1969, Apollo 12 astronauts returning from Moon experienced a solar eclipse as the Earth blocked the Sun shortly before splashdown.
Gemini XII astronauts James A. Lovell and Edwin E. “Buzz” Aldrin for the first time photographed a solar eclipse from Earth orbit on Nov. 12, 1966. Sixteen hours into their flight, the nearly total eclipse came into view as they flew over the Galapagos Islands and Aldrin took several photographs and a short film clip. Calculations showed that Gemini XII passed within 3.4 miles of the center of the eclipse’s path that traversed South America. The Surveyor 3 spacecraft observed the first solar eclipse from the Moon on April 24, 1967. Unlike solar eclipses observed on Earth, this time the Earth itself blocked the Sun – observers on Earth saw the event as a lunar eclipse as the Moon passed through the Earth’s shadow. In November 1969, as Apollo 12 astronauts Charles “Pete” Conrad, Richard F. Gordon, and Alan L. Bean neared Earth on their return from the second lunar landing – during which they visited Surveyor 3 – orbital mechanics had a show in store for them. Their trajectory passed through Earth’s shadow, treating them to a total solar eclipse. From their perspective, the Earth appeared about 15 times larger than the Sun. Gordon radioed Mission Control, “We’re getting a spectacular view at eclipse,” and Bean proclaimed it a “fantastic sight.” Conrad reported on the rapidly changing scenery, with the Sun illuminating the Earth’s atmosphere in a 360-degree ring with ever-changing colors while the planet remained pitch black. In the darkness, they could see flashes of lightning in thunderstorms appearing as fireflies. As their eyes adapted to the dark portion of the Earth, they saw landmasses such as India and even city lights. In the center of the Earth’s dark disc they reported seeing a large bright circle that turned out to be the glint of the full Moon reflecting off the Indian Ocean.
Left: The Moon’s shadow photographed from Mir during the August 1999 eclipse. Image credit: courtesy French space agency CNES. Middle: NASA astronaut Donald R. Pettit observed the first solar eclipse from the International Space Station during Expedition 6 in December 2002. Right: Pettit’s second eclipse during Expedition 31 in May 2012.
The credit belongs to French astronaut Jean-Pierre Haigneré for taking the first photograph from Earth orbit of the Moon’s shadow during a solar eclipse. He photographed the Aug. 11, 1999, total eclipse pass over England while onboard the Russian space station Mir as an Expedition 27 flight engineer. NASA astronaut Donald R. Pettit claims the title as the first person to photograph an eclipse from the International Space Station when he observed the Dec. 2, 2002, total eclipse during Expedition 6. As an additional claim, on May 20, 2012, Pettit observed his second eclipse from the space station during Expedition 31, this one an annular eclipse over the Western Pacific Ocean.
Left: Expedition 12 image of the March 2006 total eclipse over the eastern Mediterranean Sea. Middle: Expedition 52 image of the August 2017 total eclipse over North America. Right: Expedition 63 image of the June 2020 annular eclipse.
Left and middle: Two views of the eclipse over Antarctica in December 2021, from the Expedition 66 crew aboard the space station, left, and from the Deep Space Climate Observatory (DSCOVR) satellite. Right: DSCOVR image of the October 2023 annular solar eclipse over North America.
Space station crews have observed and documented a number of solar eclipses in addition to Pettit’s two sightings, their ability to see the Moon’s shadow as it traverses the Earth’s surface determined by their orbital trajectory. Expedition 12 observed the total eclipse on March 29, 2006, Expedition 43 documented the total eclipse on March 25, 2015, Expedition 52 observed the most recent total eclipse visible from North America on Aug. 21, 2017, Expedition 61 observed the annular eclipse on Dec. 26, 2019, Expedition 63 saw the annular eclipse on June 21, 2020, Expedition 66 imaged the total eclipse over Antarctica on Dec. 4, 2021, and Expedition 70 viewed the annular eclipse visible in North America on Oct. 14, 2023. Positioned nearly one million miles away at the L1 Earth-Sun Lagrange point, the National Oceanic and Atmospheric Administration’s Deep Space Climate Observatory (DSCOVR) satellite keeps a watchful eye on Earth’s climate. NASA’s Earth Polychromatic Imaging Camera (EPIC), a camera and telescope aboard DSCOVR, has taken stunning images of the Moon’s shadow during eclipses as well as the Moon transiting across the face of the Earth.
Mars
Beyond the Earth-Moon system, eclipses do not occur on Mercury and Venus since they lack natural satellites to block out the Sun. Mars has two small satellites, Phobos and Deimos, both too small to fully eclipse the Sun, even though it appears only half as big as on Earth. Several rovers have captured Phobos and Deimos as they form annular eclipses. Some astronomers contend that due to the small sizes of the Martian satellites, especially Deimos, compared to the Sun, these are technically transits, not eclipses, but no formal definition exists. The Mars Exploration Rover Opportunity imaged the first eclipses from the surface of Mars shortly after its arrival on the planet, first of Deimos on March 4, 2004, followed by Phobos three days later. More recently, the Mars 2020 Perseverance rover imaged the annular eclipse of Phobos on April 20, 2022, and the eclipse (or transit) of Deimos on Jan. 22, 2024.
Left: Mars Exploration Rover Opportunity images of Deimos, left, and Phobos crossing in front of the Sun. Middle: Perseverance image of a Phobos annular eclipse in April 2022. Right: Perseverance image of a Deimos eclipse (or transit) in January 2024.
Jupiter
Left: Hubble Space Telescope infrared image of a triple eclipse on Jupiter on March 28, 2004, with moons Ganymede, Io, and Callisto casting shadows on the planet. Middle: Hubble Space Telescope image of the Jan. 24, 2015, multiple eclipse on Jupiter, with five of its moons – Callisto, Io, Europa, Amalthea, and Thebe – casting shadows on the planet. Right: Europa eclipses Io in December 2014, as observed through an Earth-based telescope. Image credit: courtesy Jen Miller and Joy Chavez, Gemini Observatory.
Since the outer gas giant planets do not have solid surfaces, no spacecraft has imaged an actual eclipse by one of the multitude of moons orbiting these worlds. What we can observe, through ground-based and orbiting telescopes and spacecraft are the shadows cast by the moons on their home planets. Eclipses on Jupiter are not exceptionally rare given the planet’s large size compared to its many moons and greater distance from the Sun. Only five of Jupiter’s moons, Amalthea, Io, Europe, Ganymede, and Callisto are either large enough or close enough to the planet to completely occult the Sun. And given the low tilts of the moons’ orbits, they cast a shadow on every revolution. Double, triple and multiple simultaneous eclipses are not uncommon. The Hubble Space Telescope has observed numerous such events. Given the number of Jupiter’s moons, especially the four large Galilean moons, and that their orbits all lie very close to Jupiter’s equatorial plane, they occasionally eclipse each other, with the outer moons passing between the Sun and the inner moons. When Earth passes through Jupiter’s equatorial plane, fortunate observers can capture these rare events using ground-based telescopes, sometimes accidentally as they observe the Galilean moons for other reasons.
Left: Juno image of Io’s shadow on Jupiter in September 2019. Right: Juno image of Jupiter’s moon Ganymede casting its shadow on the planet in February 2022.
The Juno spacecraft, in orbit around Jupiter since 2016, has returned stunning images of Jupiter’s cloud patterns. On Sept. 11, 2019, it captured a spectacular image of Io’s shadow on Jupiter’s colorful cloud tops. On Feb. 25, 2022, Juno imaged the largest moon Ganymede’s shadow.
Saturn and beyond
Left: As it orbited Saturn, in November 2009 Cassini imaged eclipses of moons Titan, center, and Enceladus, lower right of Titan, and the planet’s rings. Middle: Titan casts its shadow, elongated by the planet’s curvature, on Saturn in this November 2009 image from the Cassini orbiter. Right: Sequential Hubble Space Telescope February 2009 images of a quadruple eclipse, as Saturn’s moons Enceladus, Dione, Titan, and Mimas cast their shadows on the planet.
Like Jupiter, dozens of moons orbit around the ringed planet Saturn, providing ample opportunities for telescopes and spacecraft to observe them passing in front of and casting their shadows onto the planet. The Cassini spacecraft, in orbit around Saturn between 2004 and 2017, captured thousands of images of the planet, its rings, and its moons. On many occasions, Cassini passed behind the planet and its moons, creating artificial eclipses, while at other times the spacecraft imaged the moons’ shadows on the planet’s cloud tops. The Hubble Space Telescope captured a series of images of a rare quadruple eclipse on Feb. 24, 2009, as Saturn’s moons Enceladus, Dione, Titan, and Mimas transited across the planet, casting their shadows on the cloud tops.
The Cassini spacecraft created this artificial eclipse of Saturn in November 2013 as it traveled beyond Saturn during one of its orbits, with many objects, including Earth, made visible.
On July 19, 2013, Cassini took a series of images from a distance of about 750,000 miles as Saturn eclipsed the Sun. In the event dubbed The Day the Earth Smiled, people on Earth received notification in advance that Cassini would be taking their picture from 900 million miles away, and were encouraged to smile at its camera. In addition to the Earth and Moon, Cassini captured Venus, Mars, and seven of Saturn’s satellites in the photograph.
Left: Composite image showing the relative apparent sizes of the Sun and a selection of planetary moons. Image credit: courtesy sdoisgo.blogspot.com. Middle: July 2006 Hubble Space Telescope image of Uranus and its moon Ariel casting a shadow on the planet. Right: The New Horizons spacecraft created an artificial eclipse as it flew behind Pluto during its July 2015 flyby, the Sun’s rays highlighting its tenuous atmosphere.
The Earth occupies a unique position with the nearly equal apparent diameters of the Moon and the Sun, providing opportunities for annular and total solar eclipses. As viewed from planets farther in the solar system, the Sun’s apparent diameter diminishes, with the apparent sizes of the moons orbiting those planets either larger or smaller than the Sun. Eclipses as we know them do not exist elsewhere in the solar system. Spacecraft exploring those remote worlds easily create artificial eclipses by passing through the planets’ shadows, often revealing important information, such as New Horizons imaging the tenuous atmosphere surrounding Pluto.
Paths of solar eclipses between 2021 and 2030. Image credit: courtesy Greatamericaneclipse.com.
The next total solar eclipse visible in North America will not occur until 2044, but over the next few years, several eclipses visible in other parts of the world will no doubt be targets of opportunity for astronauts’ cameras aboard the space station. And spacecraft exploring planets in the solar system will continue to document eclipses in those faraway places.
Explore More 7 min read 65 Years Ago: NASA Selects America’s First Astronauts Article 2 days ago 6 min read 45 Years Ago: Space Shuttle Columbia Arrives at NASA’s Kennedy Space Center Article 2 weeks ago 21 min read 55 Years Ago: Four Months Until the Moon Landing Article 2 weeks agoThe Marshall Star for April 3, 2024
By Celine Smith
On April 8 between 1 and 3 p.m., the Moon will pass between the Sun and Earth to create a total solar eclipse for 15 states. While Alabama will experience a partial eclipse, area residents can enjoy some fun-filled festivities to celebrate the event.
The U.S. Space & Rocket Center in Huntsville, in collaboration with the Alabama Space Grant Consortium and NASA’s Marshall Space Flight Center, will host a family-friendly eclipse watch party. There will be children’s activities in the Spark!Lab, starting at 10 a.m. Dennis Gallagher, a plasma physicist within the Heliophysics and Planetary Science branch at Marshall, will give eclipse presentations at 11:30 a.m. and 12:30 p.m. in the National Geographic Theater at the center. Those attending the eclipse watch party will receive a pair of eclipse glasses with their ticket, which is included in the price of general admission to the rocket center. Civil servants can receive free admission for themselves and family members with their ID badge, while Marshall contractors can gain admission with their badge.
Joe Matus, an engineer at NASA’s Marshall Space Flight Center, captured this image of the total solar eclipse Aug. 21, 2017, near Hopkinsville, Kentucky. NASA/Joe MatusMarshall team members don’t have to leave the arsenal to enjoy the solar eclipse. Food trucks will be staying at the food corral during the eclipse, so viewers can enjoy lunch while witnessing the natural phenomenon.
Meanwhile, experts from NASA and Marshall have collaborated with the city of Russellville, Arkansas, to provide educational outreach opportunities and panel discussions. The public is invited to this free event, with more than 100,000 tourists expected to visit Russellville for the rare experience.
Due to the length of the eclipse totality in Russellville, NASA is planning to host part of the agency’s live television broadcast from the city, as well as conduct several scientific presentations and public events for visitors. There, the total eclipse will last for four minute and 11 seconds.
Everyone is invited to experience the eclipse through NASA’s live coverage on NASA+ and the NASA app. NASA also will stream the broadcast live on its Facebook, X, YouTube, and Twitch social media accounts, as well as a telescope-only feed of eclipse views on the NASA TV media channel and YouTube.
Those viewing the eclipse should take proper precautions to protect their eyes. Without protective eyewear during a partial eclipse, viewers are susceptible to eye damage. It’s also highly recommended that eclipse viewers wear a hat, use sunscreen, and avoid exposing a lot of skin.
According to Gallagher, the Sun’s magnetic field is affected by its rotation. When the Sun rotates enough, the magnetic field can no longer hold its energy releasing solar flares. There are even some instances where bundles of the Sun’s magnetic field and ionized gas are ejected together from the Sun’s surface, creating a coronal mass ejection. These arches and arcs may be visible during the eclipse.
“Luminous tendrils of ionized gas reaching two to three solar radii in all directions away from the Sun’s surface will be revealed in graceful loops and sweeping arches off into the distance,” Gallagher said.
“Coronal mass ejections and solar flare emissions are a direct hazard to humans and human made systems. Coronal mass ejections specifically interact with Earth’s magnetic field to create additional hazards in space and on Earth’s surface. While the Sun seems a steady life-giving companion, uninvolved with Earthly travails, a total solar eclipse offers everyone, including scientists, the chance to get a closer look at what goes on at the Sun behind the blinding glare of its nuclear heart.”
Read more about the 2024 total solar eclipse from NASA.
Smith, a Media Fusion employee, supports the Marshall Office of Communications.
Hi-C Rocket Experiment Could Provide New Look at Solar FlaresBy Jessica Barnett
For a brief moment in April, team members with NASA’s Marshall Space Flight Center could get their best opportunity yet to study a solar flare using a combination of new technologies in the first-ever Solar Flare Sounding Rocket Campaign.
Teams are planning to launch two rocket experiments within a minute of each other during an active solar flare. The High-resolution Coronal Flare mission (Hi-C Flare) led by Marshall and the fourth Focusing Optics X-ray Solar Imager mission (FOXSI-4), led by the University of Minnesota, have complementary instrumentation designed to study the extreme energies involved with solar flares.
From left, NASA test engineer William Hogue, Hi-C principal investigator Sabrina Savage, and NASA systems scientist Ken Kobayashi stand in front of the Hi-C flare instrument section after it has been packaged and prepared for shipping from White Sands to Alaska. NASA“This is a pioneering campaign,” said Sabrina Savage, principal investigator for Hi-C Flare. “Launching sounding rockets to observe the Sun to test new technologies optimized for flare observations has not even been an option until now.”
Following a month of integration and testing at White Sands Missile Range in New Mexico, the Hi-C Flare team is completing two weeks of launch site integration at the Poker Flat Research Range in Alaska. The planned campaign window will be open for two weeks, beginning April 5. Each morning, the teams will spend about five hours preparing the experiment for launch, followed by up to four hours of monitoring solar data for the right flare that meets the mission study criteria. If none occurs, the rockets will be restowed in shelters overnight, and the launch will be reattempted the next day.
But if the right one does appear, the experiments will launch on Black Brant IX sounding rockets. Hi-C Flare is equipped with the third iteration of the High-Resolution Coronal Imager, or Hi-C 3. This will be the fourth flight for Hi-C, but its first with such ride-along instruments as COOL-AID (COronal OverLapagram – Ancillary Imaging Diagnostics), CAPRI-SUN (high-Cadence low-energy Passband x-Ray detector with Integrated full-SUN field of view), and SSAXI (Swift Solar Activity X-ray Imager). With these new tools, the team hopes to further solar research by capturing data at flare energies in higher-than-ever resolution and cadence.
Austin Bumbalough, an electronics engineer at NASA’s Marshall Space Flight Center, waves from behind the Hi-C payload in front of the Vehicle Assembly Building in White Sands, New Mexico, in February 2024. The payload will be used in the Hi-C rocket experiment planned to take place sometime in April.NASA“It’s a different wavelength from previous Hi-C flights, there are different features that we expect to see on the Sun’s corona, and there’s a slightly different temperature range of features that we expect to see,” said Adam Kobelski, institutional principal investigator for the SSAXI instrument.
The Sun is currently experiencing the “solar maximum” phase of its activity cycle, which increases the chances of a solar flare occurring during the campaign window. The study requires a specific type of flare, one that registers as a C5-class or higher with a duration longer than the rocket flight. While it isn’t yet possible to precisely predict when a solar flare will occur or how long it will be, the team has developed algorithms to provide alerts and predictive diagnostics using data from solar telescopes in orbit, factoring in the complexity of active regions and real-time changes to X-ray and extreme ultraviolet solar output.
The alert won’t be instant, however. In fact, it could take several minutes for the information to get from a telescope in space to the team on the ground to the team members who launch the rocket – and even then, due to the science requirements for the two missions, Hi-C Flare is planning to launch after FOXSI-4 takes flight. The flare may have progressed by up to 10 minutes by the time Hi-C Flare begins making observations.
The Hi-C flare instrument sits inside a clean tent for integration testing at White Sands Missile Range in February 2024. NASA“That’s why we’re requiring a long-duration flare, so we can guarantee ourselves that we will see it,” said Genevieve Vigil, technical and camera lead for Hi-C and COOL-AID.
Once in air, sensors on the rocket will point the cameras toward the Sun and stabilize the instrumentation. Then, a shutter door will open and allow the cameras to acquire data for about five minutes before the door closes and the rocket falls back to Earth. Vigil said the rocket will land somewhere in the Alaskan tundra, where it will stay until weather conditions are safe enough for it to be retrieved via helicopter and for the team to begin fully processing the data.
Kobelski is hoping to see small-scale heating in the corona.
“It’s a very unique thing that only this set of instrumentation can do, since it has the high resolution and can see very hot things,” he said. “I would like to see actual structure in the heating that occurs in the corona.”
The Hi-C Flare experiment and rocket subsystems are staged on the launch rail and prepared for integration with the rocket motors in April 2024.NASAFor Vigil, it’s about testing the equipment and the process.
“I want to show that this method – of catching a flare in action, then launching a rocket to go take pictures of it – is an effective way to study flares,” she said. “That would open a lot of doors to a lot of other kinds of instruments that you could build and specifically design for flare studies, that you could then test.”
Marshall Space Flight Center leads the Hi-C Flare experiment in partnership with the Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, and Montana State University in Bozeman. Launch support is provided at Poker Flat Research Range by the University of Alaska Fairbanks and NASA’s Sounding Rocket Program at the agency’s Wallops Flight Facility on Wallops Island, Virginia, which is managed by NASA’s Goddard Space Flight Center. NASA’s Heliophysics Division manages the sounding-rocket program for the agency’s Science Mission Directorate.
Barnett, a Media Fusion employee, supports the Marshall Office of Communications.
‘Hooray for SLS!’ Children’s Book Launches on NASA.gov“Hooray for SLS!” – the first in a series of illustrated children’s books designed to introduce the youngest members of the Artemis Generation ages 3 to 8 to the unique elements that make NASA’s Artemis campaign possible – is now publicly available on NASA’s website.
“Hooray for SLS!” is a NASA product written by Lane Polak and illustrated by Heather Legge-Click.NASAIn addition to a downloadable version of the book, coloring sheets, and student activities online, parents and educators can also watch and listen to a read aloud version of the book on YouTube.
“Hooray for SLS!”is a NASA product written by Lane Polak and illustrated by Heather Legge-Click. Learn more about SLS (Space Launch System) and check out the book here.
NASA’s Marshall Space Flight Center manages the SLS Program.
I Am Artemis: Mat BevillSignificant events in history keep finding Mat Bevill. As the associate chief engineer for NASA’s SLS (Space Launch System) Program, Bevill assists the program chief engineer by interfacing with each of the element chief engineers and helping make critical decisions for the development and flight of the SLS mega rocket that will power NASA’s Artemis campaign. With the launch of Artemis II, the first crewed test flight of SLS and the Orion spacecraft, Bevill’s technical leadership and support for the SLS Chief Engineer’s Office will place him, once again, at a notable moment in time.
Mat Bevill, the associate chief engineer for NASA’s SLS (Space Launch System) Program, stands in front of a four-segment solid rocket booster that powered the space shuttle at NASA’s Marshall Space Flight Center.NASA/Brandon Hancock“Think of me as the assistant coach. While the head coach is on the front line leading the team, I’m on the sidelines providing feedback and advising those efforts,” said Bevill. As a jack-of-all-trades, he enables progress in any way that he can, something he’s familiar with after 37 years with NASA. And, on Nov. 16, 2022, as the SLS rocket roared to life for the first time with the Artemis I test flight, Bevill couldn’t help but reflect on a lifetime of experiences and lessons that led to that moment.
Bevill began his NASA career while he was still attending the University of Tennessee at Chattanooga. During his sophomore year as a mechanical engineer student, he applied for the agency’s internship program at NASA’s Marshall Space Flight Center.
Just a few months before Bevill began his journey with NASA, the Challenger accident occurred, taking the lives of all seven crewmembers in January 1986. Bevill joined the Solid Motor Branch at Marshall as teams across the agency worked to understand the cause of the accident. It was a fast-paced environment, and Bevill had to learn quickly about the solid rocket boosters.
“It was a surreal experience, but I was privileged to work with those people. We were figuring out tough lessons together and working toward a common goal,” Bevill recalls.
Those tough lessons provided Bevill with tremendous hands-on experience related to the solid rocket booster hardware that would not only shape his career, but, later, the SLS rocket. The five-segment solid rocket boosters that provide more than 75% of thrust for SLS to go to the Moon are based on the same four-segment design that powered 135 shuttle missions to low Earth orbit. His experience from his time with the shuttle led him to deputy chief engineer for the SLS Boosters Office.
Just as for Artemis I, Bevill will be standing by and serving as the “assistant coach” for Artemis II as the SLS rocket, once again, takes flight and sends the first crewed Artemis mission around the Moon. “SLS has been the crowning jewel of my career, and I consider myself blessed to be a part of NASA’s history,” Bevill said.
SLS is part of NASA’s backbone for deep space exploration, along with the Orion spacecraft, advanced spacesuits and rovers, the Gateway in orbit around the Moon, and commercial human landing systems. SLS is the only rocket that can send Orion, astronauts, and supplies to the Moon in a single launch.
NASA Names Finalists to Help Deal with Dust in Human Lander ChallengeNASA selected 12 finalist teams to compete in the next round of the Human Lander Challenge (HuLC) competition. In 2023, NASA invited undergraduate and graduate students from accredited colleges and universities in the United States to propose innovative solutions to manage the lunar dust a spacecraft stirs up when landing on the Moon.
NASA’s Artemis campaign will establish a long-term human presence on and around the Moon for the benefit of all, and one of the challenges the agency and its partners must address is the particularly dusty aspect of landing on the lunar surface. These university-level teams will spend the next several months continuing to develop their concepts for managing or preventing the cloud of dust created when using rocket engines to land on unprepared surfaces like the Moon. This effect is called plume surface interaction and can damage assets NASA plans to establish on the Moon’s surface, like habitats and scientific experiments.
“Each team brings a unique perspective and I’m excited to see the cumulation of each team’s extensive research and concept development at the 2024 Forum,” said Jamshid Samareh, lead for the technology identification and assessment team at NASA’s Langley Research Center. “Their proposed system-level designs showcase the brilliance and dedication of the Artemis Generation to our collective mission. I am confident their work will propel us closer to the Moon and hopefully inspire future advancements in space exploration.”
The 2024 HuLC Finalist Teams are:
- Colorado School of Mines
- “Prudent Landers – FAST”
- Advisor: Mark Florida, Dr. Angel Abbud-Madrid, David Purcell
- Embry-Riddle Aeronautical University
- “Plume Additive for Reducing Surface Ejecta and Cratering (PARSEC)”
- Advisor: Dr. Siwei Fan
- Embry-Riddle Aeronautical University
- “Ceramic Research Advancement Technology at Embry-Riddle (C.R.A.T.E.R.)”
- Advisor: Seetha Raghavan
- Ohio Northern University
- “HuLC Smash”
- Dr. Louis DiBerardino
- Texas A&M University
- “Maroon Moon: Preliminary Surface Stabilization to Mitigate Lunar Plume Surface Interaction”
- Advisor: John F. Connolly, Dr. Jean-Louis Briaud
- Texas A&M University
- “Synthetic Orbital Landing Area for Crater Elimination (SOLACE)”
- Advisor: Dr. Helen Reed
- Texas State University
- “Numerical Simulation and Physical Validation of Regolith Ejecta During Plume Surface Interaction”
- Advisor: Dr. Bin Xiao
- The College of New Jersey
- “TCNJ Adaptable Regolith Retention Program (TARRP)”
- Advisor: Mohammed Alabsi
- University of California San Diego
- “Microwave Lunar Sintering of Nanophase Iron Enriched Lunar Regolith for the Creation of a Lunar Landing Pad”
- Advisor: Dr. Amy Eguchi, Dr. Zahra Sadeghizadeh, Dr. Ross Turner
- University of Colorado Boulder (Graduate Team)
- “Lunar Surface Assessment Tool (LSAT): A Simulation of Lunar Dust Dynamics for Risk Analysis”
- Advisor: James Nabity
- University of Illinois Urbana-Champaign
- “HINDER: Holistic Integration of Navigational Dynamics for Erosion Reduction”
- Advisor: Laura Villafane Roca
- University of Michigan
- “ARC-LIGHT: Algorithm for Robust Characterization of Lunar surface Imaging for Ground Hazards and Trajectory”
- Advisor: Mirko Gamba, Chris Ruf
The finalist selection process involved a rigorous assessment of each team’s proposal package submission, consisting of a 5–7-page concept proposal and a two-minute summary video. The judging panel made up of subject matter experts from NASA’s Human Landing System Program considered factors such as feasibility, innovation, and adherence to NASA’s safety standards. Each team will receive a $7,000 stipend award to facilitate further development of their proposed concept and their full participation in the 2024 HuLC Forum in Huntsville in June. The 12 finalists will make final presentations to a panel of NASA and industry experts at the onsite HuLC Forum. The top three winning teams will share a prize purse of $18,000.
The Human Lander Challenge is sponsored by NASA’s Human Landing System Program and managed by the National Institute of Aerospace.
NASA’s Marshall Space Flight Center manages the Human Landing System Program.
Through Artemis, NASA will land the first woman, first person of color, and its first international partner astronaut on the Moon, paving the way for a long-term, sustainable lunar presence to explore more of the lunar surface than ever before and prepare for future astronaut missions to Mars.
For full competition details, visit the Human Lander Challenge website.
Chandra: Stunning Echo of 800-year-old ExplosionIn the year 1181 a rare supernova explosion appeared in the night sky, staying visible for 185 consecutive days. Historical records show that the supernova looked like a temporary ‘star’ in the constellation Cassiopeia shining as bright as Saturn.
Ever since, scientists have tried to find the supernova’s remnant. At first it was thought that this could be the nebula around the pulsar – the dense core of a collapse star – named 3C 58. However closer investigations revealed that the pulsar is older than supernova 1181.
Pa 30 is a nearly circular nebula with a central star in the constellation Cassiopeia. It is pictured here combining images from several telescopes. This composite image uses data across the electromagnetic spectrum and shows a spectacular new view of the supernova remnant.X-ray: (Chandra) NASA/CXC/U. Manitoba/C. Treyturik, (XMM-Newton) ESA/C. Treyturik; Optical: (Pan-STARRS) NOIRLab/MDM/Dartmouth/R. Fesen; Infrared: (WISE) NASA/JPL/Caltech/; Image Processing: Univ. of Manitoba/Gilles Ferrand and Jayanne EnglishIn the last decade, another contender was discovered; Pa 30 is a nearly circular nebula with a central star in the constellation Cassiopeia. It is pictured here combining images from several telescopes. This composite image uses data across the electromagnetic spectrum and shows a spectacular new view of the supernova remnant. This allows us to marvel at the same object that appeared in our ancestors’ night sky more than 800 years ago.
X-ray observations by ESA’s XMM-Newton (blue) show the full extent of the nebula and NASA’s Chandra X-ray Observatory (cyan) pinpoints its central source. The nebula is barely visible in optical light but shines bright in infrared light, collected by NASA’s Wide-field Infrared Space Explorer (red and pink). Interestingly, the radial structure in the image consists of heated sulfur that glows in visible light, observed with the ground-based Hiltner 2.4 m telescope at the MDM Observatory (green) in Arizona, USA, as do the stars in the background by Pan-STARRS (white) in Hawaii, USA.
Studies of the composition of the different parts of the remnant have led scientists to believe that it was formed in a thermonuclear explosion, and more precisely a special kind of supernova called a sub-luminous Type Iax event. During this event two white dwarf stars merged, and typically no remnant is expected for this kind of explosion. But incomplete explosions can leave a kind of ‘zombie’ star, such as the massive white dwarf star in this system. This very hot star, one of the hottest stars in the Milky Way (about 200 000 degrees Celsius), has a fast stellar wind with speeds up to 16,000 km/h. The combination of the star and the nebula makes it a unique opportunity for studying such rare explosions.
NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.
Read more from NASA’s Chandra X-ray Observatory.
Europa Clipper Survives and Thrives in ‘Outer Space’ on EarthIn less than six months, NASA is set to launch Europa Clipper on a 1.6-billion-mile voyage to Jupiter’s ocean moon Europa. From the wild vibrations of the rocket ride to the intense heat and cold of space to the punishing radiation of Jupiter, it will be a journey of extremes. The spacecraft was recently put through a series of hard-core tests at the agency’s Jet Propulsion Laboratory to ensure it’s up to the challenge.
Called environmental testing, the battery of trials simulates the environment that the spacecraft will face, subjecting it to shaking, chilling, airlessness, electromagnetic fields, and more.
Europa Clipper is seen in the 25-Foot Space Simulator at JPL in February, before the start of thermal vacuum testing. A battery of tests ensures that the NASA spacecraft can withstand the extreme hot, cold, and airless environment of space. NASA/JPL-Caltech“These were the last big tests to find any flaws,” said JPL’s Jordan Evans, the mission’s project manager. “Our engineers executed a well-designed and challenging set of tests that put the system through its paces. What we found is that the spacecraft can handle the environments that it will see during and after launch. The system performed very well and operates as expected.”
The most recent environmental test for Europa Clipper was also one of the most elaborate, requiring 16 days to complete. The spacecraft is the largest NASA has ever built for a planetary mission and one of the largest ever to squeeze into JPL’s historic 85-foot-tall, 25-foot-wide thermal vacuum chamber (TVAC). Known as the 25-foot Space Simulator, the chamber creates a near-perfect vacuum inside to mimic the airless environment of space.
At the same time, engineers subjected the hardware to the high temperatures it will experience on the side of Europa Clipper that faces the Sun while the spacecraft is close to Earth. Beams from powerful lamps at the base of the Space Simulator bounced off a massive mirror at its top to mimic the heat the spacecraft will endure.
To simulate the journey away from the Sun, the lamps were dimmed and liquid nitrogen filled tubes in the chamber walls to chill them to temperatures replicating space. The team then gauged whether the spacecraft could warm itself, monitoring it with about 500 temperature sensors, each of which had been attached by hand.
TVAC marked the culmination of environmental testing, which included a regimen of tests to ensure the electrical and magnetic components that make up the spacecraft don’t interfere with one another.
NASA’s Europa Clipper is seen being lifted into the Space Simulator at JPL in February. Thermal vacuum testing, which lasted 16 days, ensures that the spacecraft will withstand the harsh conditions of space.NASA/JPL-CaltechThe orbiter also underwent vibration, shock, and acoustics testing. During vibration testing, the spacecraft was shaken repeatedly – up and down and side to side – the same way it will be jostled aboard the SpaceX Falcon Heavy rocket during liftoff. Shock testing involved pyrotechnics to mimic the explosive jolt the spacecraft will get when it separates from the rocket to fly its mission. Finally, acoustic testing ensured that Europa Clipper can withstand the noise of launch, when the rumbling of the rocket is so loud it can damage the spacecraft if it’s not sturdy enough.
“There still is work to be done, but we’re on track for an on-time launch,” Evans said. “And the fact that this testing was so successful is a huge positive and helps us rest more easily.”
Later this spring, the spacecraft will be shipped to NASA’s Kennedy Space Center. There, teams of engineers and technicians will carry out final preparations with eyes on the clock. Europa Clipper’s launch period opens Oct. 10.
After liftoff, the spacecraft will zip toward Mars, and in late February 2025, it will be close enough to use the Red Planet’s gravitational force for added momentum. From there, the solar-powered spacecraft will swing back toward Earth to get another slingshot boost – from our own planet’s gravitational field – in December 2026.
Then it’s on to the outer solar system, where Europa Clipper is set to arrive at Jupiter in 2030. The spacecraft will orbit the gas giant while it flies by Europa 49 times, dipping as close as 16 miles from the moon’s surface to gather data with its powerful suite of science instruments. The information gathered will tell scientists more about the moon’s watery interior.
A timelapse video shows engineers and technicians moving NASA’s Europa Clipper spacecraft into the 85-foot-tall Space Simulator at the agency’s Jet Propulsion Laboratory in Southern California. The spacecraft underwent thermal vacuum testing in the chamber in February 2024 and passed with flying colors.Credit: NASA/JPL-Caltech
Europa Clipper’s main science goal is to determine whether there are places below the surface of Jupiter’s icy moon, Europa, that could support life. The mission’s three main science objectives are to determine the thickness of the moon’s icy shell and its surface interactions with the ocean below, to investigate its composition, and to characterize its geology. The mission’s detailed exploration of Europa will help scientists better understand the astrobiological potential for habitable worlds beyond our planet.
Managed by Caltech in Pasadena, California, JPL leads the development of the Europa Clipper mission in partnership with the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland, for NASA’s Science Mission Directorate. APL designed the main spacecraft body in collaboration with JPL and NASA’s Goddard Space Flight Center.
The Planetary Missions Program Office at NASA’s Marshall Space Flight Center executes program management of the Europa Clipper mission.
Learn more about Europa.
NASA Sets Coverage for Astronaut Loral O’Hara, Crewmates ReturnThree crew members are scheduled to begin their return to Earth on April 5, from the International Space Station. NASA will provide live coverage of their departure from the orbital complex and landing.
NASA astronaut and Expedition 70 Flight Engineer Loral O’Hara uses a portable glovebag to replace components on a biological printer, the BioFabrication Facility, that is testing the printing of organ-like tissues in microgravity.NASANASA astronaut Loral O’Hara, Roscosmos cosmonaut Oleg Novitskiy, and spaceflight participant Marina Vasilevskaya of Belarus will depart from the station’s Rassvet module in the Roscosmos Soyuz MS-24 spacecraft at 10:55 p.m. CDT April 5, and will head for a parachute-assisted landing on the steppe of Kazakhstan, southeast of the town of Dzhezkazgan, at 2:18 a.m. April 6.
Coverage will begin at 7 p.m. on April 5 with farewells and the Soyuz hatch closure on NASA+, NASA Television, the NASA app, YouTube, and the agency’s website. Learn how to stream NASA TV through a variety of platforms including social media.
O’Hara is completing a mission spanning 204 days in space that covered 3,264 orbits of the Earth and 86.5 million miles. Novitskiy and Vasilevskaya launched with NASA astronaut Tracy C. Dyson to the station aboard the Soyuz MS-25 spacecraft on March 23. Dyson will remain aboard the station for a six-month research mission.
After landing, the three crew members will fly on a helicopter from the landing site to the recovery staging city of Karaganda, Kazakhstan. O’Hara then will depart back to Houston.
The HOSC (Huntsville Operations Support Center) at NASA’s Marshall Space Flight Center provides engineering and mission operations support for the space station, the Commercial Crew Program, and Artemis missions, as well as science and technology demonstration missions. The Payload Operations Integration Center within the HOSC operates, plans, and coordinates the science experiments onboard the space station 365 days a year, 24 hours a day.
NASA Selects Companies to Advance Moon Mobility for Artemis Missions
NASA has selected Intuitive Machines, Lunar Outpost, and Venturi Astrolab to advance capabilities for a lunar terrain vehicle (LTV) that Artemis astronauts will use to travel around the lunar surface, conducting scientific research during the agency’s Artemis campaign at the Moon and preparing for human missions to Mars.
The awards leverage NASA’s expertise in developing and operating rovers to build commercial capabilities that support scientific discovery and long-term human exploration on the Moon. NASA intends to begin using the LTV for crewed operations during Artemis V.
“We look forward to the development of the Artemis generation lunar exploration vehicle to help us advance what we learn at the Moon,” said Vanessa Wyche, director of NASA’s Johnson Space Center in Houston. “This vehicle will greatly increase our astronauts’ ability to explore and conduct science on the lunar surface while also serving as a science platform between crewed missions.”
NASA will acquire the LTV as a service from industry. The indefinite-delivery/indefinite-quantity, milestone-based Lunar Terrain Vehicle Services contract with firm-fixed-price task orders has a combined maximum potential value of $4.6 billion for all awards.
Artist concept of Lunar Outpost’s Lunar Dawn lunar terrain vehicle.Credit: Lunar Outpost Artist concept of Intuitive Machines’ Moon RACER lunar terrain vehicle.Credit: Intuitive Machines Artist concept of Venturi Astrolab’s FLEX lunar terrain vehicle.Credit: AstrolabEach provider will begin with a feasibility task order, which will be a year-long special study to develop a system that meets NASA’s requirements through the preliminary design maturity project phase. The agency will issue a subsequent request for task order proposal to eligible provider(s) for a demonstration mission to continue developing the LTV, deliver it to the surface of the Moon, and validate its performance and safety ahead of Artemis V. NASA anticipates making an award to only one provider for the demonstration. NASA will issue additional task orders to provide unpressurized rover capabilities for the agency’s moonwalking and scientific exploration needs through 2039.
The LTV will be able to handle the extreme conditions at the Moon’s South Pole and will feature advanced technologies for power management, autonomous driving, and state of the art communications and navigation systems. Crews will use the LTV to explore, transport scientific equipment, and collect samples of the lunar surface, much farther than they could on foot, enabling increased science returns.
Between Artemis missions, when crews are not on the Moon, the LTV will operate remotely to support NASA’s scientific objectives as needed. Outside those times, the provider will have the ability to use their LTV for commercial lunar surface activities unrelated to NASA missions.
“We will use the LTV to travel to locations we might not otherwise be able to reach on foot, increasing our ability to explore and make new scientific discoveries,” said Jacob Bleacher, chief exploration scientist in the Exploration Systems Development Mission Directorate at NASA Headquarters in Washington. “With the Artemis crewed missions, and during remote operations when there is not a crew on the surface, we are enabling science and discovery on the Moon year around.”
NASA provided technical requirements, capabilities, and safety standards needed for LTV development and operations, and the selected companies have agreed to meet the key agency requirements. The contract request for proposal required each provider to propose a solution to provide end-to-end services, including LTV development, delivery to the Moon, and execution of operations on the lunar surface.
Through Artemis, NASA will send astronauts – including the first woman, first person of color, and its first international partner astronaut – to explore the Moon for scientific discovery, technology evolution, economic benefits, and to build the foundation for crewed missions to Mars. Advanced rovers, along with the agency’s SLS (Space Launch System) rocket and Orion spacecraft, commercial human landing systems and next-generation spacesuits, and Gateway are NASA’s foundation for deep space exploration.
Learn more about NASA’s Artemis campaign at:
-end-
Kathryn Hambleton
Headquarters, Washington
202-358-1100
kathryn.a.hambleton@nasa.gov
Victoria Ugalde / Nilufar Ramji
Johnson Space Center, Houston
281-483-5111
victoria.d.ugalde@nasa.gov / nilufar.ramji@nasa.gov
Scientists Pursue the Total Solar Eclipse with NASA Jet Planes
5 min read
Scientists Pursue the Total Solar Eclipse with NASA Jet PlanesThe April 8, 2024, total solar eclipse will produce stunning views across North America. While anyone along the eclipse path with a clear sky will see the spectacular event, the best view might be 50,000 feet in the air, aboard NASA’s WB-57 jet planes. That’s where a trio of NASA-funded teams are sending their scientific instruments to take measurements of the eclipse.
Two teams will image the Sun’s outer atmosphere – the corona – and a third will measure the ionosphere, the upper electrically charged layer of Earth’s atmosphere. This information will help scientists better understand the structure and temperature of the corona, the effects of the Sun on Earth’s atmosphere, and even aid in the search of asteroids that may orbit near the Sun.
The April 8, 2024 total solar eclipse will produce stunning views across North America. While anyone along the eclipse path with a clear sky will see the spectacular event, the best view might be 50,000 feet in the air, aboard NASA’s WB-57 jet planes. That’s where a trio of NASA-funded teams are sending their scientific instruments to take measurements of the eclipse. Credit: NASADuring a total solar eclipse, the Moon perfectly blocks the bright face of the Sun, casting a small swath of Earth in darkness. With the Sun’s main light masked, the much dimmer solar corona becomes visible to the naked eye. This provides scientists a unique opportunity to study this mysterious region of the Sun. The brief blocking of sunlight also allows scientists to study how the Sun’s light affects Earth’s atmosphere.
In the past, solar eclipses have driven numerous scientific discoveries. For this solar eclipse, NASA is funding several scientific experiments – including the three using the WB-57s – to make measurements during the eclipse. NASA’s WB-57s fly much higher than commercial aircraft. This altitude allows the jets to fly above clouds – meaning no chance of missing the eclipse due to bad weather. Additionally, the height puts the jets above most of Earth’s atmosphere, which allows for the cameras to take crisper images and capture wavelengths, such as infrared light, that don’t make it to the ground. Since the planes can travel at 460 miles per hour, they’re also able to extend the time they spend in the Moon’s shadow. While the eclipse will last no more than four and a half minutes at any point on the ground, the planes will see an eclipse that lasts about 25 percent longer, over 6 minutes and 22 seconds.
This map shows the path of the 2024 total solar eclipse. The dark path across the continent is the path of totality. By flying along this path, the WB-57s will extend the amount of time they spend in totality.NASA/Scientific Visualization Studio/Michala Garrison; Eclipse Calculations By Ernie Wright, NASA Goddard Space Flight Center“By extending the duration of totality, we’re increasing the duration of how much data we can acquire,” said Shadia Habbal, a researcher at the University of Hawaii who leads of one of the WB-57 eclipse experiments.
Habbal’s experiment will fly spectrometers – which record specific wavelengths of light and cameras. The instruments will measure the temperature and chemical composition of the corona and coronal mass ejections, which are large bursts of solar material. With this data, scientists aim to better understand the structure of the corona and identify the source of the solar wind, the constant stream of particles emitted by the Sun.
Habbal hopes the results of their study will help differentiate between different competing models of how the corona is heated. “This light is our best probe short of sticking a thermometer in the corona,” Habbal said.
NASA/ESA’s Solar and Heliospheric Observatory (SOHO) captured this video of a coronal mass ejection on March 13, 2023. NASA/ESA/SOHOFor another team, led by Amir Caspi at the Southwest Research Institute in Boulder, Colorado, it’s not their first time chasing eclipses by plane. Caspi led a previous trailblazing experiment with the WB-57s during the 2017 total solar eclipse that crossed America from sea to sea. Images taken from the jet were used to study the structure of the corona.
That time was the first the jets had ever been used to study an eclipse. This time, an improved camera setup will allow measurements in more wavelengths from infrared to visible light that will hopefully reveal new information about structures in the middle and lower corona. The observations, taken with a high-resolution, high-speed camera, could also help study a dust ring that circles the Sun and help search for asteroids that may orbit near the Sun.
“There isn’t a lot of data of the Sun at some of the wavelengths we’ll be studying,” Caspi said. “We don’t know what we’ll find, so it’s extra exciting to be making these measurements.”
A third experiment will study the effects of the Moon’s shadow on the ionosphere using an instrument called an ionosonde, which was designed at JHU APL. An ionosonde functions like a simple radar. The device sends out high-frequency radio signals and listens for their echoes rebounding off the ionosphere, which allows the researchers to measure how charged the ionosphere is.
“The eclipse basically serves as a controlled experiment,” said Bharat Kunduri, leader of the ionosphere project and a research assistant professor at Virginia Tech in Blacksburg, Virginia. “It gives us an opportunity to understand how changes in solar radiation can impact the ionosphere, which can in turn impact some of these technologies like radar and GPS that we rely on in our daily lives.”
By Mara Johnson-Groh
NASA’s Goddard Space Flight Center, Greenbelt, Md.
A spectacular eclipse will sweep across North America on April 8, 2024! Enjoy these free…
Article 2 days ago Keep Exploring Discover Related TopicsMissions
Humans in Space
Climate Change
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Carving a Path
These aren’t highways in this picture taken on Aug. 15, 2023; they’re paths carved by glaciers as they move through the Karakoram mountain range north of the Himalayas.
Crew aboard the International Space Station take photos of Earth, recording how the planet changes over time due to human activity and natural events. This allows scientists to monitor disasters and direct response on the ground and study a number of phenomena, from the movement of glaciers to urban wildlife.
Image Credit: NASA/Woody Hoburg
NASA Receives 13 Nominations for the 28th Annual Webby Awards
6 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)Since it began in 1958, NASA has been charged by law with spreading the word about its work “to the widest extent practicable.” From typewritten press releases to analog photos and film, NASA has effectively moved into social media and other online communications. NASA’s broad reach across digital platforms has been recognized by the International Academy of Digital Arts and Sciences (IADAS), which gave NASA 13 nominations for the academy’s Webby Awards this year.
At NASA, we share the secrets of the universe through every platform and media there is. These nominations—for websites, podcasts, social media, apps and virtual experiences—showcase the breadth and depth of the NASA digital team, as they inspire the next generation to reach for the stars.Marc Etkind
NASA Associate Administrator for Communications
Public Voting OpportunitiesVoting for the Webby People’s Voice Awards—chosen by the public—is open now through Thursday, April 18. Voting links for each category are listed below.
28th Annual Webby Nominees AppsSpace Images
NASA, NASA Jet Propulsion Laboratory, Caltech
Apps & Software-General Apps | Education, Science & Reference
The Space Images app provides stunning new images of space, planets, Mars, asteroids, stars, galaxies, and cutting-edge space technology as they are released each week from NASA’s Jet Propulsion Laboratory.
CampaignsNASA: Message in a Bottle
NASA Jet Propulsion Laboratory
Advertising, Media & PR-PR Campaigns | Best Community Engagement
NASA’s Message in a Bottle campaign invited people around the world to sign their names to a poem written by the U.S. Poet Laureate Ada Limón. The poem connects the two water worlds — Earth, yearning to reach out and understand what makes a world habitable, and Europa, waiting with secrets yet to be explored. The campaign was a special collaboration, uniting art and science, by NASA, the U.S. Poet Laureate, and the Library of Congress.
PodcastsNASA’s Curious Universe
Podcasts-Shows | Science & Education
As an official NASA podcast, Curious Universe brings you mind-blowing science and space adventures you won’t find anywhere else. Explore the cosmos alongside astronauts, scientists, engineers, and other top NASA experts who are achieving remarkable feats in science, space exploration, and aeronautics. Learn something new about the wild and wonderful universe we share. All you need to get started is a little curiosity. NASA’s Curious Universe is an official NASA podcast hosted by Padi Boyd and Jacob Pinter.
NASA’s Curious Universe: Suiting Up for Space
Podcasts-Individual Episodes | Science & Education
Spacesuits are more than just garments – in the airless vacuum of space or on the freezing surface of the moon, they keep astronauts alive. In this episode of NASA’s Curious Universe podcast, we explore how NASA engineers like Amy Ross and Paromita Mitra contributed to the development of the next generation of spacesuits.
SocialHubble’s Servicing Mission 1
Social-Social Content Series | Education & Science
Shortly after its 1990 deployment, NASA discovered a flaw in the observatory’s primary mirror that affected the clarity of the telescope’s early images. Fortunately, Hubble’s design allowed astronauts to perform repairs, replace parts, and update its technology with new instruments while in orbit. Servicing Mission 1 was the first opportunity to install corrective optics that counteracted the primary mirror’s flaw, add new instruments, and conduct planned maintenance on the telescope.
NASA Social Media
Social-Features | Best Overall Social Presence, Brand
NASA’s flagship social media accounts host dynamic conversations about what’s new with America’s space agency, and why it matters. Spanning 15 social media platforms, these accounts reach more than 200 million people around the world.
NASA’s First Asteroid Sample Return Mission
Social-Social Campaigns | Education & Science
Science fiction became reality on Sept. 24, 2023 when NASA’s OSIRIS-REx spacecraft delivered rocks older than our own planet to the Utah desert, rocks that contain clues to the early solar system and the origins of life. The accompanying social media campaign and in-person, behind-the-scenes NASA Social event gave the public an inside look into NASA’s first mission to deliver an asteroid sample to Earth.
Annular Solar Eclipse
NASA, ADNET Systems Inc.
Social-Social Campaigns | Events & Live Streams
On Oct. 14, 2023, audiences across the web joined us live as a “ring of fire” eclipse. Visible in parts of the United States, Mexico, and many countries in South and Central America, millions of people in the Western Hemisphere experienced this eclipse.
VideoOSIRIS-REx Asteroid Sample Return (Official 4K NASA Live Stream)
Video-General Video | Events & Live Streams
Live coverage of OSIRIS-REx, the first U.S. mission to collect a sample from an asteroid, as it returned to Earth on Sept. 24, 2023, to drop off material from asteroid Bennu. The spacecraft didn’t land, but continued on to a new mission, OSIRIS-APEX, to explore asteroid Apophis. Meanwhile, scientists hope the Bennu sample OSIRIS-REx dropped into the Utah desert will offer clues to whether asteroids colliding with Earth billions of years ago brought water and other key ingredients for life here.
Virtual ExperiencesNASA’s Immersive Earth
Artificial Intelligence (AI), Metaverse & Virtual-General Virtual Experiences | Science & Education
NASA created the Earth Information Center with founding partners FEMA, EPA, NOAA, USAID, USDA and USGS. The Earth Information Center draws data from research conducted by NASA’s centers and government and industry partners. The interactive physical exhibit is located inside NASA Headquarters in Washington, where visitors are invited to see how our planet is changing in six key areas: sea level rise and coastal impacts, health and air quality, wildfires, greenhouse gases, sustainable energy, and agriculture.
WebsitesNASA.gov
Websites and Mobile Sites-General Desktop & Mobile Sites | Government & Associations
The new NASA web experience serves as an ever-expanding yet consolidated homebase for information about the agency’s missions and research, climate data, Artemis updates, and more. The updated nasa.gov and science.nasa.gov websites provide a connected, topic-driven experience, with a common search engine, integrated navigation, and optimized publishing capabilities in a modernized and secure set of web tools.
NASA+ Streaming Service
Websites and Mobile Sites-General Desktop & Mobile Sites | Television, Film & Streaming
Through the ad-free, no cost, and family-friendly streaming service, users gain access to the agency’s Emmy Award-winning live coverage and views into NASA’s missions through collections of original video series, including new series debuting on the streaming service. NASA+ also streams live event coverage, where people everywhere can watch in real-time as the agency launches science experiments and astronauts to space, and ultimately, the first woman and person of color to the Moon.
Hubble’s Inside the Image
NASA, Origin Films
Video-Video Series & Channels | Science & Education
In this ongoing series, astronomers explain the history and high-level science behind some of Hubble’s most beautiful, groundbreaking, and iconic images.
About the Webby AwardsEstablished in 1996, The Webbys is presented by the International Academy of Digital Arts and Sciences (IADAS)—a 3000+ member judging body comprised of leading Internet experts, business figures, luminaries, visionaries and creative celebrities. The Webbys honors excellence in nine major media types: websites and mobile sites, video, advertising, media and public relations, apps and software, social, podcasts, games and Metaverse, virtual and artificial Intelligence (AI).
The Webby Awards presents two honors in every category—The Webby Award and The Webby People’s Voice Award. Members of the International Academy of Digital Arts and Sciences (IADAS) select the nominees for both awards in each category, as well as the Winners of The Webby Awards. The Webby People’s Voice is awarded by the voting public.
Rock Sampled by NASA’s Perseverance Embodies Why Rover Came to Mars
The 24th sample taken by the six-wheeled scientist offers new clues about Jezero Crater and the lake it may have once held.
Analysis by instruments aboard NASA’s Perseverance Mars rover indicate that the latest rock core taken by the rover was awash in water for an extended period of time in the distant past, perhaps as part of an ancient Martian beach. Collected on March 11, the sample is the rover’s 24th – a tally that includes 21 sample tubes filled with rock cores, two filled with regolith (broken rock and dust), and one with Martian atmosphere.
“To put it simply, this is the kind of rock we had hoped to find when we decided to investigate Jezero Crater,” said Ken Farley, project scientist for Perseverance at Caltech in Pasadena, California. “Nearly all the minerals in the rock we just sampled were made in water; on Earth, water-deposited minerals are often good at trapping and preserving ancient organic material and biosignatures. The rock can even tell us about Mars climate conditions that were present when it was formed.”
The presence of these specific minerals is considered promising for preserving a rich record of an ancient habitable environment on Mars. Such collections of minerals are important for guiding scientists to the most valuable samples for eventual return to Earth with the Mars Sample Return campaign.
Edge of the Crater’s RimNicknamed “Bunsen Peak” for the Yellowstone National Park landmark, the rock – about 5.6 feet wide and 3.3 feet high (1.7 meters by 1 meter) – intrigued Perseverance scientists because the outcrop stands tall amid the surrounding terrain and has an interesting texture on one of its faces. They were also interested in Bunsen Peak’s vertical rockface, which offers a nice cross-section of the rock and, because it’s not flat-lying, is less dusty and therefore easier for science instruments to investigate.
Meet the 24th Martian sample collected by NASA’s Mars Perseverance rover – “Comet Geyser,” a sample taken from a region of Jezero Crater that is especially rich in carbonate, a mineral linked to habitability.Before taking the sample, Perseverance scanned the rock using the rover’s SuperCam spectrometers and the X-ray spectrometer PIXL, short for Planetary Instrument for X-ray Lithochemistry. Then the rover used the rotor on the end of its robotic arm to grind (or abrade) a portion of the surface and scanned the rock again. The results: Bunsen Peak looks to be composed of about 75% carbonate grains cemented together by almost pure silica.
“The silica and parts of the carbonate appear microcrystalline, which makes them extremely good at trapping and preserving signs of microbial life that might have once lived in this environment,” said Sandra Siljeström, a Perseverance scientist from the Research Institutes of Sweden (RISE) in Stockholm. “That makes this sample great for biosignature studies if returned to Earth. Additionally, the sample might be one of the older cores collected so far by Perseverance, and that is important because Mars was at its most habitable early in its history.” A potential biosignature is a substance or structure that could be evidence of past life but may also have been produced without the presence of life.
The Bunsen Peak sample is the third that Perseverance has collected while exploring the “Margin Unit,” a geologic area that hugs the inner edge of Jezero Crater’s rim.
This mosaic shows a rock called “Bunsen Peak” where NASA’s Perseverance Mars rover extracted its 21st rock core and abraded a circular patch to investigate the rock’s composition.NASA/JPL-Caltech/ASU/MSSS Perseverance’s CacheCam captured this image of the rover’s latest cored sample – taken from an intriguing rock called “Bunsen Peak” – on March 11. NASA/JPL-Caltech“We’re still exploring the margin and gathering data, but results so far may support our hypothesis that the rocks here formed along the shores of an ancient lake,” said Briony Horgan, a Perseverance scientist from Purdue University, in West Lafayette, Indiana. “The science team is also considering other ideas for the origin of the Margin Unit, as there are other ways to form carbonate and silica. But no matter how this rock formed, it is really exciting to get a sample.”
The rover is working its way toward the westernmost portion of the Margin Unit. At the base of Jezero Crater’s rim, a location nicknamed “Bright Angel” is of interest to the science team because it may offer the first encounter with the much older rocks that make up the crater rim. Once it’s done exploring Bright Angel, Perseverance will begin an ascent of several months to the rim’s top.
More About the MissionA key objective for Perseverance’s mission on Mars is astrobiology, including caching samples that may contain signs of ancient microbial life. The rover will characterize the planet’s geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith.
Subsequent NASA missions, in cooperation with ESA (European Space Agency), would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis.
The Mars 2020 Perseverance mission is part of NASA’s Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet.
NASA’s Jet Propulsion Laboratory, which is managed for the agency by Caltech, built and manages operations of the Perseverance rover.
For more about Perseverance:
https://mars.nasa.gov/mars2020/
News Media ContactsDC Agle
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-9011
agle@jpl.nasa.gov
Karen Fox / Charles Blue
NASA Headquarters, Washington
301-286-6284 / 202-802-5345
karen.c.fox@nasa.gov / charles.e.blue@nasa.gov
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Share Details Last Updated Apr 03, 2024 Related Terms Explore More 6 min read Scientists Pursue the Total Solar Eclipse with NASA Jet PlanesThe April 8, 2024, total solar eclipse will produce stunning views across North America. While…
Article 5 hours ago 4 min read How NASA Spotted El Niño Changing the Saltiness of Coastal Waters Article 8 hours ago 4 min read NASA Partnerships Bring 2024 Total Solar Eclipse to EveryoneOn Monday, April 8, NASA and its partners will celebrate the wonders of the total…
Article 1 day agoHow NASA Spotted El Niño Changing the Saltiness of Coastal Waters
New findings have revealed a coastal realm highly sensitive to changes in runoff and rainfall on land.
After helping stoke record heat in 2023 and drenching major swaths of the United States this winter, the current El Niño is losing steam this spring. Scientists have observed another way that the climate phenomenon can leave its mark on the planet: altering the chemistry of coastal waters.
A team at NASA’s Jet Propulsion Laboratory in Southern California used satellite observations to track the dissolved salt content, or salinity, of the global ocean surface for a decade, from 2011 to 2022. At the sea surface, salinity patterns can tell us a lot about how freshwater falls, flows, and evaporates between the land, ocean, and atmosphere – a process known as the water cycle.
The JPL team showed that year-to-year-variations in salinity near coastlines strongly correlate with El Niño Southern Oscillation (ENSO), the collective term for El Niño and its counterpart, La Niña. ENSO affects weather around the world in contrasting ways. El Niño, linked to warmer-than-average ocean temperatures in the equatorial Pacific, can lead to more rain and snowfall than normal in the southwestern U.S., as well as drought in Indonesia. These patterns are somewhat reversed during La Niña.
During the exceptional El Niño event of 2015, for example, the scientists traced a particularly distinct global water cycle effect: Less precipitation over land led to a decrease in river discharge on average, which in turn led to notably higher salinity levels in areas as far as 125 miles (200 kilometers) from shore.
Instruments in space can track how salinity varies by region and season. Using NASA satellite data, this map shows how monsoon rains and freshwater flowing into the Bay of Bengal keep it far less salty than the Arabian Sea to the west. (Areas of low and high salinity are shown in blue and yellow, respectively.)NASA’s Scientific Visualization Studio The Amazon River delivers millions of gallons of water to the ocean every second – enough to change global average surface salinity. A plume of low salinity water is shown here in dark blue, drifting away from the river mouth on ocean currents. The blue blob to the northwest is the Orinoco River plume.NASA’s Scientific Visualization StudioAt other times, the opposite was found: Areas with higher-than-normal rainfall over land saw increased river discharge, reducing salinity near those coasts.
“We’re able to show coastal salinity responding to ENSO on a global scale,” said lead author Severine Fournier, an ocean physicist at JPL.
The team found that salinity is at least 30 times more variable in these dynamic zones near coasts than in the open ocean. The link between rain, rivers, and salt is especially pronounced at the mouths of large river systems such as the Mississippi and Amazon, where freshwater plumes can be mapped from space as they gush into the ocean.
Salt as SignalWith global warming, researchers have been observing changes in the water cycle, including increases in extreme precipitation events and runoff. At the intersection of land and sea, coastal waters may be where the impacts are most detectable.
“Given the sensitivity to rainfall and runoff, coastal salinity could serve as a kind of bellwether, indicating other changes unfolding in the water cycle,” Fournier said.
She noted that some of the world’s coastal waters are not well studied, despite the fact that about 40% of the human population lives within about 60 miles (100 kilometers) of a coastline. One reason is that river gauges and other on-sitemonitors can be costly to maintain and cannot provide coverage of the whole planet, especially in more remote regions.
That’s where satellite instruments come in. Launched in 2011, the Aquarius mission made some of the first space-based global observations of sea surface salinity using extremely sensitive radiometers to detect subtle changes in the ocean’s microwave radiation emissions. Aquarius was a collaboration between NASA and Argentina’s space agency, CONAE (Comisión Nacional de Actividades Espaciales).
Today, two higher-resolution tools – the ESA (European Space Agency) Soil Moisture and Ocean Salinity (SMOS) mission and NASA’s Soil Moisture Active Passive (SMAP) mission – allow scientists to zoom to within 25 miles (40 kilometers) of coastlines.
Using data from all three missions, the researchers found that surface salinity in coastal waters reached a maximum global average (34.50 practical salinity units, or PSU) each March and fell to a minimum global average (34.34 PSU) around September. (PSU is roughly equal to parts per thousand grams of water.) River discharge, especially from the Amazon, drives this timing.
In the open ocean, the cycle is different, with surface salinity reaching a global average minimum (34.95 PSU) from February to April and a global average maximum (34.97 PSU) from July to October. The open ocean does not show as much variability between seasons or years because it contains a significantly larger volume of water and is less sensitive to river discharge and ENSO. Instead, changes are governed by planet-scale precipitation minus total global evaporation, plus other factors like large-scale ocean circulation.
The study was published in the journal Geophysical Research Letters.
NASA Analysis Sees Spike in 2023 Global Sea Level Due to El Niño NASA Analysis Finds Strong El Niño Could Bring Extra Floods This Winter News Media ContactsJane J. Lee / Andrew Wang
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-0307 / 626-379-6874
jane.j.lee@jpl.nasa.gov / andrew.wang@jpl.nasa.gov
Written by Sally Younger
2024-035
Share Details Last Updated Apr 03, 2024 Related Terms Explore More 5 min read Rock Sampled by NASA’s Perseverance Embodies Why Rover Came to Mars Article 8 hours ago 9 min read Veronica T. Pinnick Put NASA’s PACE Mission through Its Paces Article 1 day ago 5 min read NASA’s Europa Clipper Survives and Thrives in ‘Outer Space’ on Earth Article 1 week agoNASA Invites Media to Annual FIRST Robotics Competition in Rocket City
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Students from the Power Struck Girls Team 5965 – an all-girls FIRST Robotics team from the Academy of Our Lady high school in Marrero, Louisiana, and sponsored by NASA’s Stennis Space Center – make final engineering adjustments to their robot during the 2023 Rocket City Regional FIRST Robotics tournaments in Huntsville.NASA/Joel WallaceThe Rocket City Regional – Alabama’s annual For Inspiration and Recognition of Science and Technology (FIRST) Robotics Competition – is scheduled for Friday, April 5, through Saturday, April 6, at the Von Braun Center South Hall in Huntsville, Alabama, known as the Rocket City. This event is free for the public.
FIRST Robotics is a global robotics competition for students in grades 9-12. Teams are challenged to raise funds, design a team brand, hone teamwork skills, and build and program industrial-sized robots to play a difficult field game against competitors.
More than 1,000 high school students on 47 teams from 10 states and 4 countries will compete in a new robotics game called, “CRESCENDO.”
Opening ceremonies begin at 8:30 a.m. CDT followed by qualification matches on April 5 and April 6. The Friday awards ceremony will begin at 6 p.m., while the Saturday awards ceremony will begin at 2:30 p.m.
District and regional competitions – such as the Rocket City Regional – are held across the country during March and April, providing teams a chance to qualify for the 2024 FIRST Robotics Competition Championship events held in late April in Houston.
NASA and its Robotics Alliance Project provide grants for high school teams and support for FIRST Robotics competitions to address the critical national shortage of students pursuing STEM (Science, Technology, Engineering, and Mathematics) careers. This FIRST Robotics Competition, The Rocket City Regional, is supported by NASA’s Marshall Space Flight Center in Huntsville, Alabama, and NASA’s Office of STEM Engagement.
News media interested in covering this event should respond no later than 4 p.m. on Thursday, April 4 by contacting Taylor Goodwin at 256-544-0034 or taylor.goodwin@nasa.gov.
Learn more about the Rocket City Regional event.
Find more information about Marshall’s support for education programs:
https://www.nasa.gov/marshall/marshall-stem-engagement/
Taylor Goodwin
256-544-0034
Marshall Space Flight Center, Huntsville, Alabama
taylor.goodwin@nasa.gov
On Monday, April 8, NASA and its partners will celebrate the wonders of the total…
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NASA’s Webb Probes an Extreme Starburst Galaxy
Amid a site teeming with new and young stars lies an intricate substructure.
A team of astronomers has used NASA’s James Webb Space Telescope to survey the starburst galaxy Messier 82 (M82). Located 12 million light-years away in the constellation Ursa Major, this galaxy is relatively compact in size but hosts a frenzy of star formation activity. For comparison, M82 is sprouting new stars 10 times faster than the Milky Way galaxy.
Led by Alberto Bolatto at the University of Maryland, College Park, the team directed Webb’s NIRCam (Near-Infrared Camera) instrument toward the starburst galaxy’s center, attaining a closer look at the physical conditions that foster the formation of new stars.
“M82 has garnered a variety of observations over the years because it can be considered as the prototypical starburst galaxy,” said Bolatto, lead author of the study. “Both NASA’s Spitzer and Hubble space telescopes have observed this target. With Webb’s size and resolution, we can look at this star-forming galaxy and see all of this beautiful, new detail.”
Image: M82 observed by the Hubble and Webb Telescopes On the left is the starburst galaxy M82 as observed by NASA’s Hubble Space Telescope in 2006. The small box at the galaxy’s core corresponds to the area captured so far by the NIRCam (Near-Infrared Camera) instrument on NASA’s James Webb Space Telescope. The red filaments as seen by Webb are the polycyclic aromatic hydrocarbon emission, which traces the shape of the galactic wind. In the Hubble image, light at .814 microns is colored red, .658 microns is red-orange, .555 microns is green, and .435 microns is blue (filters F814W, F658N, F555W, and F435W, respectively). In the Webb image, light at 3.35 microns is colored red, 2.50 microns is green, and 1.64 microns is blue (filters F335M, F250M, and F164N, respectively). NASA, ESA, CSA, STScI, A. Bolatto (University of Maryland) A Vibrant Community of StarsStar formation continues to maintain a sense of mystery because it is shrouded by curtains of dust and gas, creating an obstacle in observing this process. Fortunately, Webb’s ability to peer in the infrared is an asset in navigating these murky conditions. Additionally, these NIRCam images of the very center of the starburst were obtained using an instrument mode that prevented the very bright source from overwhelming the detector.
While dark brown tendrils of heavy dust are threaded throughout M82’s glowing white core even in this infrared view, Webb’s NIRCam has revealed a level of detail that has historically been obscured. Looking closer toward the center, small specks depicted in green denote concentrated areas of iron, most of which are supernova remnants. Small patches that appear red signify regions where molecular hydrogen is being lit up by a nearby young star’s radiation.
“This image shows the power of Webb,” said Rebecca Levy, second author of the study at the University of Arizona, Tucson. “Every single white dot in this image is either a star or a star cluster. We can start to distinguish all of these tiny point sources, which enables us to acquire an accurate count of all the star clusters in this galaxy.”
Finding Structure in Lively ConditionsLooking at M82 in slightly longer infrared wavelengths, clumpy tendrils represented in red can be seen extending above and below the galaxy’s plane. These gaseous streamers are a galactic wind rushing out from the core of the starburst.
One area of focus for this research team was understanding how this galactic wind, which is caused by the rapid rate of star formation and subsequent supernovae, is being launched and influencing its surrounding environment. By resolving a central section of M82, scientists could examine where the wind originates, and gain insight on how hot and cold components interact within the wind.
Webb’s NIRCam instrument was well-suited to trace the structure of the galactic wind via emission from sooty chemical molecules known as polycyclic aromatic hydrocarbons (PAHs). PAHs can be considered as very small dust grains that survive in cooler temperatures but are destroyed in hot conditions.
Much to the team’s surprise, Webb’s view of the PAH emission highlights the galactic wind’s fine structure – an aspect previously unknown. Depicted as red filaments, the emission extends away from the central region where the heart of star formation is located. Another unanticipated find was the similar structure between the PAH emission and that of hot, ionized gas.
“It was unexpected to see the PAH emission resemble ionized gas,” said Bolatto. “PAHs are not supposed to live very long when exposed to such a strong radiation field, so perhaps they are being replenished all the time. It challenges our theories and shows us that further investigation is required.”
Video: Tour of the M82 Image Credit: NASA’s Goddard Space Flight Center Lighting a Path ForwardWebb’s observations of M82 in near-infrared light spur further questions about star formation, some of which the team hopes to answer with additional data gathered with Webb, including that of another starburst galaxy. Two other papers from this team characterizing the stellar clusters and correlations among wind components of M82 are almost finalized.
In the near future, the team will have spectroscopic observations of M82 from Webb ready for their analysis, as well as complementary large-scale images of the galaxy and wind. Spectral data will help astronomers determine accurate ages for the star clusters and provide a sense of timing for how long each phase of star formation lasts in a starburst galaxy environment. On a broader scale, inspecting the activity in galaxies like M82 can deepen astronomers’ understanding of the early universe.
“Webb’s observation of M82, a target closer to us, is a reminder that the telescope excels at studying galaxies at all distances,” said Bolatto. “In addition to looking at young, high-redshift galaxies, we can look at targets closer to home to gather insight into the processes that are happening here – events that also occurred in the early universe.”
These findings have been accepted for publication in The Astrophysical Journal.The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and the Canadian Space Agency.
DownloadsRight click the images in this article to open a larger version in a new tab/window.
Download full resolution images for this article from the Space Telescope Science Institute.
These findings have been accepted for publication in The Astrophysical Journal.
Laura Betz – laura.e.betz@nasa.gov, Rob Gutro – rob.gutro@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Christine Pulliam – cpulliam@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
More about starburst galaxy M82
More Webb News – https://science.nasa.gov/mission/webb/latestnews/
More Webb Images – https://science.nasa.gov/mission/webb/multimedia/images/
Webb Mission Page – https://science.nasa.gov/mission/webb/
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Share Details Last Updated Apr 03, 2024 EditorStephen SabiaContactLaura Betzlaura.e.betz@nasa.gov Related Terms65 Years Ago: NASA Selects America’s First Astronauts
On Nov. 5, 1958, NASA, newly established to lead America’s civilian space program, formally established the Space Task Group (STG) at NASA’s Langley Research Center in Hampton, Virginia, to implement one of the nation’s top priorities – to develop a spacecraft capable of sending humans into space and returning them safely to Earth. In January 1959, the STG selected a contractor to build the spacecraft for Project Mercury and began the process of choosing who would fly the spacecraft. President Dwight D. Eisenhower directed NASA to choose its first astronauts from among the ranks of military pilots. The three-month rigorous process led to the selection on April 2, 1959, of seven men from among America’s military branches. The agency presented them to the world on April 9 as America’s Mercury 7 astronauts.
Left: The headquarters building for the Space Task Group at NASA’s Langley Research Center in Hampton, Virginia. Right: An early cutaway representation of the Mercury capsule.
President Eisenhower decided that military test pilots would make the most suitable astronauts. Choosing from among armed forces personnel would expedite the selection process since the government had access to their records and all had received prior security clearances and medical screening. On Jan. 5, 1959, NASA established the qualifications for the astronauts: less than 40 years of age; less than 5 feet 11 inches tall; excellent physical condition; bachelor’s degree or equivalent; graduate of test pilot school; and 1,500 hours of jet flight time. A screening in late January of the files of 508 graduates of the Navy and Air Force test pilot schools who met the basic age and flying requirements resulted in 110 qualified candidates. The selection committee ranked these candidates and divided them into three groups of about 35 each. The first two groups, comprising 69 candidates, received classified briefings at the Pentagon about the Mercury spacecraft and their potential participation. From this group, 53 volunteered for further evaluation and NASA decided not to call in the third group of candidates. Following an initial medical screening, 32 from this group advanced to undergo thorough medical evaluations at the Lovelace Foundation for Medical Education and Research, commonly known as the Lovelace Clinic, in Albuquerque, New Mexico. Beginning on Feb. 7, the candidates in six groups of five or six spent one week at Lovelace undergoing comprehensive medical examinations. From there, 31 of the 32 (one candidate failed a blood test at Lovelace) advanced to the Aero Medical Laboratory (AML) at Wright-Patterson Air Force Base in Dayton, Ohio, where weeklong testing of the six groups took place between Feb. 15 and March 28. Rather than simply examining them physically, testing at AML consisted of stressing the candidates in centrifuges, altitude chambers, and other devices to evaluate their reactions. The selection committee met at Langley in late March and based on all the available data selected seven candidates for Project Mercury. The 24 unsuccessful candidates received notification by telephone on April 1 with a follow up letter from Assistant STG Manager Charles J. Donlan on April 3, also advising them to apply for any possible future astronaut selections. Four of them did apply to the second selection in 1962, and NASA selected two of them. The seven chosen as Mercury astronauts received telephone calls from Donlan on April 2.
Group photo of the Mercury 7 astronauts at their first public appearance in April 1959: Walter M. Schirra, left, Alan B. Shepard, Virgil I. “Gus” Grissom, Donald K. “Deke” Slayton, John H. Glenn, M. Scott Carpenter, and L. Gordon Cooper.
On April 9, 1959, NASA formally introduced the men to the nation and the world. The event took place in the ballroom of the Dolley Madison House on Lafayette Square in Washington, D.C., the new space agency’s first headquarters. The astronauts took their seats at a long table on a makeshift stage, and NASA Administrator T. Keith Glennan introduced them in alphabetical order: “Malcolm S. Carpenter, Leroy G. Cooper, John H. Glenn, Virgil I. Grissom, Walter M. Schirra, Alan B. Shepard, and Donald K. Slayton … the nation’s Mercury astronauts!” After a brief photo session, for the next 90 minutes the new astronauts responded to numerous questions from the reporters gathered in the ballroom. For most of the men, meeting the press represented a new experience as they had little prior exposure to the media in their previous jobs as test pilots. By the time the event concluded, they clearly sensed that their lives had changed forever, with public attention as much a part of their jobs as training for and flying in space. They reported for work at Langley on April 27.
Mercury 7 astronauts M. Scott Carpenter, left, L. Gordon Cooper, John H. Glenn, and Virgil I. “Gus” Grissom.
Carpenter flew America’s second orbital flight, Mercury 7, in May 1962, after serving as backup to Glenn for his historic first orbital flight. He named his capsule Aurora 7. Due to late firing of his retrorockets for the deorbit burn, Carpenter landed 250 miles from the target, and he waited hours for rescue forces to recover him. Cooper served as Schirra’s backup before getting his flight assignment on Mercury 9. He spent 34 hours aboard his Faith 7 capsule, at the time the longest American spaceflight. He served as command pilot of the eight-day Gemini V mission in August 1965, setting another American record. As his last assignment, he served as backup commander for Apollo 10 in 1969. Glenn made history in February 1962 as the first American to orbit the Earth aboard Friendship 7. Although he retired from NASA in 1964 to pursue a career in politics, he flew again as a U.S. Senator in 1998 aboard STS-95 at age 77, still the record as the oldest person to orbit the Earth. Grissom flew the second suborbital mission, Mercury 4, aboard his Liberty Bell 7 capsule, in August 1961. Following splashdown, his spacecraft’s hatch accidentally blew off and seawater rapidly filled it, a recovery helicopter pulling him to safety at the last moment. As the first American to travel to space a second time, he commanded the first two-man spacecraft, Gemini 3, in March 1965. He received a third spaceflight assignment as the commander of Apollo 1, the first flight of the three-person spacecraft. He died tragically during a ground test fire of the spacecraft on Jan. 27, 1967.
Mercury 7 astronauts Walter M. Schirra, left, Alan B. Shepard, and Donald K. “Deke” Slayton.
Schirra served as Carpenter’s backup before flying six orbits aboard his Sigma 7 spacecraft during the Mercury 8 mission in October 1962. He served as Grissom’s backup for Gemini 3 and flew as the command pilot for Gemini VI in December 1965, the first space rendezvous mission. Two months earlier, he showed his cool when on the first attempt to launch Gemini VI, the rocket’s engines shutdown just before liftoff. Before the Apollo 1 fire, he served as the commander of the Apollo 2 mission, then once again as Grissom’s backup for Apollo 1. After the fire, he flew as the commander of Apollo 7, the first crewed test of Command and Service Module in October 1968, the only astronaut to fly aboard all three of America’s first spacecraft. Shepard holds the honor as the first American in space for his suborbital flight aboard Freedom 7 during the Mercury 4 mission in May 1961. Grounded by an inner ear malady, Shepard went on to lead the astronauts as their chief until reinstated to flight duty in May 1969. He served as the commander of Apollo 14 in January-February 1971, the only Mercury 7 astronaut to walk on the Moon. Originally assigned to fly the Mercury 7 mission, in March 1962, flight surgeons grounded Slayton due to a heart irregularity just two months before his scheduled mission aboard Delta 7. While grounded, he served as chief of flight crew operations. Flight surgeons reinstated him to flying status in March 1972, and soon after NASA assigned him as the docking module pilot for the July 1975 Apollo-Soyuz Test Project joint mission with the Soviet Union.
Summary of spaceflights by the Mercury 7 astronauts. The highlighted boxes with flight names in italics represent astronauts who died before they could undertake the mission. Italics represent astronaut assigned to but did not fly the mission.
Astronaut biographies can be found at https://www.nasa.gov/astronauts
Read the JSC History Office oral histories with Carpenter, Cooper, Glenn, Schirra, and Shepard.
Explore More 6 min read 45 Years Ago: Space Shuttle Columbia Arrives at NASA’s Kennedy Space Center Article 2 weeks ago 21 min read 55 Years Ago: Four Months Until the Moon Landing Article 2 weeks ago 11 min read 20 Years Ago: First Image of Earth from Mars and Other Postcards of Home Article 4 weeks agoNASA Aeronautics Monthly STEM Newsletter
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Preparations for Next Moonwalk Simulations Underway (and Underwater)2024
NASA Aeronautics Monthly STEM Newsletter: Issue 35
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Share Details Last Updated Apr 02, 2024 EditorLillian GipsonContactJim Bankejim.banke@nasa.gov Related TermsA Home for Astronauts around the Moon
The Gateway space station’s HALO (Habitation and Logistics Outpost) module, one of two of Gateway’s habitation elements where astronauts will live, conduct science, and prepare for lunar surface missions, is one step closer to launch following welding completion in Turin, Italy.
HALO, shown in this image from Oct. 23, 2023, will next undergo a series of stress tests to ensure its safety. Upon successful completion, the future home for astronauts will travel to Gilbert, Arizona where Northrop Grumman will complete final outfitting ahead of launch to lunar orbit.
Gateway will be humanity’s first space station in lunar orbit as an essential element of the Artemis missions to return humans to the Moon for scientific discovery and chart a path for the first human missions to Mars.
Image Credit: Northrop Grumman/Thales Alenia Space
Veronica T. Pinnick Put NASA’s PACE Mission through Its Paces
To achieve the impossible, Veronica T. Pinnick, who put NASA’s PACE mission through its prelaunch paces, says you need to get comfortable with being uncomfortable.
Name: Dr. Veronica T. Pinnick
Title: Plankton Aerosol, Cloud and ocean Ecosystem (PACE) Integration and Test (I&T) manager
Formal Job Classification: Chemist
Organization: Integration and Test Branch, Electrical Engineering Division (Code 568)
Veronica Pinnick is an integration and test manager at NASA’s Goddard Space Flight Center in Greenbelt, Md.Credit: NASA/Dennis HenryWhat do you do and what is most interesting about your role here at Goddard?
As the PACE I&T manager, I managed the build-up of the entire observatory. Integration means we put the spacecraft together. Testing means we make sure it works within itself and that it will also work in space.
Why did you become a chemist? What is your educational background?
In third grade, we did a science experiment that involved pulling out the colors of a black maker, which turned out to be a mixture of many colors. It was the first time my little science brain exploded! I learned that maybe not everything was as it first appeared, it was so cool. Years later, I now do that same experiment (chromatography) on Mars, looking at dirt and pulling it apart to see what it is made of.
I have a B.A. in chemistry from Minot State University in North Dakota. I have a Ph.D. in analytical chemistry from Texas A&M University. I did a post-doctoral fellowship at Johns Hopkins School of Medicine in Maryland.
How did you come to Goddard?
My post-doctoral fellowship involved a Goddard project, designing an instrument to look for life on Mars. I thought that was an interesting application of my specialty! After my fellowship, I joined Goddard in 2010 working on that same project for 10 more years.
Towards the end of that project, I became the I&T manager responsible for building, testing, and delivery of that instrument to an ESA (European Space Agency) Mars rover. During those years, I realized that I wanted to change my career path more towards engineering.
Why did you merge science and engineering in your career?
Branching out to try new things can be scary. I think what I enjoy most about working at Goddard is that there are endless opportunities for people who are comfortable being uncomfortable. I really like both science and engineering. I think skills from my scientific background really help in building and testing instruments for other scientists.
When I started in college, I did not really understand the difference between science and engineering. When I arrived at Goddard, I learned the important difference between these two different roles. The scientist asks, “What do I want to measure?” The engineer asks, “How can I build an instrument to measure that?” Blending the two disciplines, you end up with an instrument that measures something in space!
We work at our best when we are cross-disciplinary, when scientists think like engineers and engineers think like scientists, when we can understand where each other is coming from. My passion is to try to return Goddard to my original mindset, that there should be full understanding of the goals of science and engineering by both disciplines.
Courtesy of Veronica PinnickAs a mentor, how do you encourage your people to be cross-disciplinary?
I encourage my mentees to think about their skill sets with an open mind and an open imagination. Sometimes people can get pigeon-holed in their skills and think they can only do one specific job. With the right mentorship and the right vision of what Goddard can do, and what gaps exist, we can fill the gaps with different skill sets.
So many times, junior scientists and engineers tell themselves they cannot do something because they lack the background or education. But in practice, what you really need are creative thinkers, creative problem solvers – your background does not matter. You must believe in your own potential. I try to show my mentees that I believe in them and their potential to branch out from their comfort zone. I tell them to push themselves to evolve. Again, you progress by being uncomfortable.
Goddard has the top minds in science and engineering. Everyone is always learning from their peers. Likewise, our mentees have so much to offer. The most junior people come at problems with a fresh perspective. Diverse perspectives always help bring new ideas to the table.
What is Goddard’s greatest challenge for new scientists and engineers?
When you are at a university, you do not always have a big budget, but you are unlimited in terms of the size or power of an instrument you want to build. When you send an instrument to space, the engineering challenges are to make it small, lightweight, and power efficient.
This is one of the hardest changes coming out of a university and joining Goddard. This is an adjustment that every person new to space has to think about and make.
What has made you proudest in your career?
I am proud of what I have built for space, but I am proudest of the people I have positively impacted along the way. I really think it is important to learn lessons from those who came before me and I am very grateful to them. I also want to help teach those coming up. We prepare lessons learned after each mission. I feel very strongly that it is important to pass these along to the next generation.
In addition to technical information, I focus a lot on people skills. To build a good team culture, you have to listen to and respect all the voices on your team. I hope to pass on the importance of teamwork and also having fun while doing our very important, very difficult work.
How does being comfortable being uncomfortable motivate you?
I have been drawn to a lot of flight missions and technology developments that are really, really challenging. That is what Goddard does best. It is unbelievable to do science on other planets! Each planet has its own unique challenges.
I started by working on ExoMars, the ESA Mars rover. I learned all about Mars and what makes doing science on Mars hard.
Then I worked on the proposal for Dragonfly, which is a flying drone that will explore Saturn’s moon Titan. I had to learn about why Titan is hard.
Now, I’ve finished building and launching a whole satellite for observing Earth, which included performing all the testing needed to make sure it will work on orbit.
Engineering instruments for different locations in the solar system requires a whole new set of engineering solutions. That is really fun, it allows me to be so creative. There are very few tried and true methods for some of these environments.
At Goddard, I am constantly challenged which makes me constantly uncomfortable but that is what I like. At first, it is intimidating. Then it is exciting!
Be comfortable being uncomfortable!
Why is working at Goddard like solving a puzzle?
At Goddard we work with some of the smartest people around. We are open to brainstorming together and coming up with solutions together.
Working on flight missions at Goddard, we work in teams which are inherently cross-disciplinary. When problems happen, it is not always easy to figure out what went wrong or how to fix the problem. Some of my most invigorating professional moments have been when things don’t go according to plan and I feel like a detective trying to figure out what exactly went wrong and how to fix it. That is where I have seen some of Goddard’s absolute best work.
Troubleshooting is like looking at 850 pieces of a 1,000 piece puzzle that you have to put together. You will never get all the pieces, but will have a pretty good idea of the big picture. It initially makes me frustrated, but I love it. It is so satisfying when your team solves the puzzle.
Why are education and outreach so important to you?
Being a good scientist means that a portion of your job is to communicate to the public what you are studying, why it is important, and what you found out. As a civil servant, the public is paying me to do this job, so I feel extremely responsible for bringing NASA’s mission to the public.
I have done education and public outreach with people of all ages. I really enjoy doing Mars rover activities with preschoolers. Three- and 4-year-olds helped me design the next Mars rover. Honestly, their ideas had great potential. I told them Mars was cold, so some of the kids put a blanket on the Rover model, which is almost exactly what we do. They were so excited to find out their solution really works in space!
People respond to knowing they can be a part of what we do. The public is so excited about what we do and want to know more. I feel inspired by their curiosity. Their excitement is infectious. They reinvigorate the joy in what we do and why we are doing what we do. I truly consider being an ambassador for NASA to the public a privilege, not a responsibility.
What do you do for fun?
I really like escape rooms; they involve all sorts of puzzles. I love the challenge of trying to figure something out under pressure. I play acoustic guitar and ukelele. We have a family band, but we only perform at home. I also like to travel and learn new languages. I am a total foodie and very much enjoy new creations made by my husband.
Who would you like to thank for encouraging you?
I absolutely thank my family, especially my husband and my son. Many of the missions we do at Goddard require a lot of personal sacrifice at times. Our missions often require long hours and extreme focus and concentration. We do it because we truly believe in and are inspired by Goddard’s mission. We are driven to build things and send them to space. That requires dedication not just from the people who work at Goddard, but also from their families. Their unending support means the world to me.
What is your “six-word memoir”? A six-word memoir describes something in just six words.
Always learning, giving back, being challenged.
By Elizabeth M. Jarrell
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Conversations With Goddard is a collection of Q&A profiles highlighting the breadth and depth of NASA’s Goddard Space Flight Center’s talented and diverse workforce. The Conversations have been published twice a month on average since May 2011. Read past editions on Goddard’s “Our People” webpage.
Share Details Last Updated Apr 02, 2024 Related TermsNASA Partnerships Bring 2024 Total Solar Eclipse to Everyone
Eclipses are an important contribution to NASA’s research into the Sun’s outer atmosphere, or corona, and the part of Earth’s atmosphere where space weather happens. They’re also an inspirational opportunity for the public to get involved, learn, and connect with our place in the universe.
Read More: 2024 Total Solar EclipseOn Monday, April 8, NASA and its partners will celebrate the wonders of the total solar eclipse as it passes over North America, with the path of totality in the United States, from Kerrville, Texas, to Houlton, Maine.
Our partners bring their creativity in sharing the excitement of the upcoming eclipse and help encourage everyone to safely enjoy this celestial event.Maureen O'Brien
Strategic alliances and partnerships manager for NASA's Office of Communications
Here are just some ways NASA is working with partners to engage the public in the upcoming total solar eclipse.
- NASA and the Major League Baseball Players Association are collaborating on the development of video and social content to emphasize eclipse awareness and safe viewing. NASA representatives also will throw out the first pitch in several games leading up to the eclipse.
- Indianapolis Motor Speedway is hosting an eclipse viewing event and live broadcast that will feature NASA exhibits, astronauts, INDY drivers, and STEM engagement talks and activities for visitors.
- Peanuts Worldwide is supporting educators with the release of new eclipse learning resources for elementary and middle school students and Snoopy is participating in events in Cleveland.
- Krispy Kreme introduced a new doughnut in honor of the eclipse and will share information about the eclipse and safe viewing.
- NASA is working with Google on new eclipse content on the Arts & Culture and other Google pages.
- Third Rock Radio (TRR) is sharing NASA podcast content and expert interviews, educational and safety messages, and a message from the International Space Station. TRR also will feature a Solar Songs listener request weekend leading up to eclipse day and live NASA TV audio coverage during the eclipse.
- Nasdaq will carry coverage of part of the NASA TV broadcast on its screen in Times Square.
Rob Lasalvia
Partnership manager for NASA’s Office of STEM Engagement
- Crayola Education released an eclipse-themed how-to video about the eclipse with a creative exercise for students.
- LEGO Education launched an eclipse education challenge to engage students and the public in learning more about the Sun and the eclipse.
- Microsoft will launch a quiz on eclipse safety with links to NASA resources.
- Discovery Education will get classrooms excited about space with eclipse resources on its PreK–12 learning platform.
- Canva released a series of free interactive eclipse courses and LabXchange released a new eclipse learning pathway for students.
- The Achievery will feature a collection of eclipse videos, share NASA’s live eclipse coverage, and host student events at AT&T locations across the country.
- NASA experts participated in a Game Jam hosted by the National Esports Association in February in which university students were challenged to create a game simulation of the Eclipse. The student-developed games will be featured during an online eclipse gaming event April 8.
- Jack and Jill of America, Inc. will host eclipse watch parties across the country for which NASA will provide viewing eclipse resources and educational materials.
- Girl Scouts of the USA is sharing NASA eclipse information and encouraging its chapters and troops to host watch parties or connect to local NASA events.
- NASA partnered with the National Park Service and Earth to Sky on activities, including the “Interpreting Eclipses” webinar series, to prepare interpreters and informal educators for the total eclipse and Heliophysics Big Year. Through this partnership, national parks hosting eclipse events also will provide elements designed especially for the blind and low vision, neurodivergent children, the physically impaired, and those with hearing impairments.
- NASA is providing eclipse resources and educational materials to local 4-H clubs along the path of totality through a partnership with the U.S. Department of Agriculture.
Anita Dey
Partnerships manager for outreach and engagement for NASA’s Science Mission Directorate
Learn more about NASA’s strategic partnerships and STEM engagement partnerships online. To learn more about where and how to safely view this year’s total solar eclipse, visit: https://go.nasa.gov/Eclipse2024.
Author: Gina Anderson, NASA Office of Communications
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