NASA
NASA Selects BAE Systems to Develop Air Quality Instrument for NOAA
NASA, on behalf of the National Oceanic and Atmospheric Administration (NOAA), has selected BAE Systems (formerly known as Ball Aerospace & Technologies Corporation) of Boulder, Colorado, to develop an instrument to monitor air quality and provide information about the impact of air pollutants on Earth for NOAA’s Geostationary Extended Observations (GeoXO) satellite program.
This cost-plus-award-fee contract is valued at approximately $365 million. It includes the development of one flight instrument as well as options for additional units. The anticipated period of performance for this contract includes support for 10 years of on-orbit operations and five years of on-orbit storage, for a total of 15 years for each flight model. The work will take place at BAE Systems, NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and the agency’s Kennedy Space Center in Florida.
The GeoXO Atmospheric Composition (ACX) instrument is a hyperspectral spectrometer that measures a wide spectrum of light from ultraviolet to visible. The instrument will provide hourly observations of air pollutants emitted by transportation, power generation, industry, oil and gas extraction, volcanoes, and wildfires as well as secondary pollutants generated from these emissions once they are in the atmosphere. By providing continuous observations and measurements of atmospheric composition, ACX data will improve air quality forecasting and monitoring and mitigate health impacts from severe pollution and smoke events, such as asthma, cardiovascular disease, and neurological disorders. Data from ACX also will help scientists better understand linkages between weather, air quality and climate.
The contract scope includes the tasks and deliverables necessary to design, analyze, develop, fabricate, integrate, test, verify, evaluate, support launch, supply and maintain the instrument ground support equipment, and support mission operations at the NOAA Satellite Operations Facility in Suitland, Maryland.
The GeoXO program is the follow-on to the Geostationary Operational Environmental Satellites – R (GOES-R) Series Program.
The GeoXO satellite system will advance Earth observations from geostationary orbit. The mission will supply vital information to address major environmental challenges of the future in support of weather, ocean, and climate operations in the United States. Advanced capabilities from GeoXO will help address our changing planet and the evolving needs of NOAA’s data users. NOAA and NASA are working to ensure these critical observations are in place by the early 2030s when the GOES-R Series nears the end of its operational lifetime.
Together, NOAA and NASA will oversee the development, launch, testing, and operation of all the satellites in the GeoXO program. NOAA funds and manages the program, operations, and data products. On behalf of NOAA, NASA and commercial partners develop and build the instruments and spacecraft and launch the satellites.
For more information on the GeoXO program, visit:
https://www.nesdis.noaa.gov/geoxo
-end-
Liz Vlock
Headquarters, Washington
202-358-1600
elizabeth.a.vlock@nasa.gov
Jeremy Eggers
Goddard Space Flight Center, Greenbelt, Md.
757-824-2958
jeremy.l.eggers@nasa.gov
John Leslie
NOAA’s National Environmental Satellite, Data, and Information Service
202-527-3504
nesdis.pa@noaa.gov
ScienceCraft for Outer Planet Exploration (SCOPE)
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Artist’s depiction of ScienceCraft, which integrates the science instrument with the spacecraft by printing a quantum dot spectrometer directly on the solar sail to form a monolithic, lightweight structure.Mahmooda SultanaMahmooda Sultana
NASA Goddard Space Flight Center
Missions to the outer solar system are an important part of NASA’s goals because these scarcely visited worlds, particularly the ice giants Neptune and Uranus, hold secrets about the formation and evolution of our solar system and countless others. However, due to the high cost, long travel time and narrow window for mission implementation, outer solar system exploration has been extremely limited in more than 60 years of space exploration. In this NIAC, we are developing a mission architecture that addresses all of these challenges by using a ScienceCraft and enables science missions at the outer planet system. Sciencraft integrates a science instrument and spacecraft into one monolithic and lightweight structure. By printing an ultra-lightweight quantum dot-based spectrometer, developed by the PI Sultana, directly on the solar sail we create a breakthrough spacecraft architecture allowing an unprecedented parallelism and throughput of data collection, and rapid travel across the solar system. Unlike conventional solar sails that serve only to propel small cubesats, ScienceCraft puts its area at use for spectroscopy, pushing the boundary of scientific exploration of the outer solar system. ScienceCraft offers an attractive low resource platform that can enable
science missions at a significantly lower cost and provide a large number of launch opportunities as a secondary payload. By leveraging these benefits, we propose a mission concept to Triton, a unique planetary body in our solar system, within the short window that closes around 2045 to answer compelling science questions about Triton’s atmosphere, ionosphere, plumes and internal structure. In Phase I, we performed an end-to-end feasibility study for a Neptune-Triton mission using a ScienceCraft, as well as identifying the key technologies needed for such a mission and tall poles that we need to address. As part of phase II, we plan to further mature the mission concept, develop and demonstrate some of the key technologies, address the tall poles identified in phase I and develop a roadmap for implementing SCOPE.
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Flexible Levitation on a Track (FLOAT)
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Artist concept of novel approach proposed by a 2024 NIAC Phase II awardee for possible future missions depicting lunar surface with planet Earth on the horizon.Credit: Ethan SchalerEthan Schaler
NASA Jet Propulsion Laboratory
We want to build the first lunar railway system, which will provide reliable, autonomous, and efficient payload transport on the Moon. A durable, long-life robotic transport system will be critical to the daily operations of a sustainable lunar base in the 2030’s, as envisioned in NASA’s Moon to Mars plan and mission concepts like the Robotic Lunar Surface Operations 2 (RLSO2), to:
— Transport regolith mined for ISRU consumables (H2O, LOX, LH2) or construction
— Transport payloads around the lunar base and to / from landing zones or other outposts
We propose developing FLOAT — Flexible Levitation on a Track — to meet these transportation needs.
The FLOAT system employs unpowered magnetic robots that levitate over a 3-layer flexible film track: a graphite layer enables robots to passively float over tracks using diamagnetic levitation, a flex-circuit layer generates electromagnetic thrust to controllably propel
robots along tracks, and an optional thin-film solar panel layer generates power for the base when in sunlight. FLOAT robots have no moving parts and levitate over the track to minimize lunar dust abrasion / wear, unlike lunar robots with wheels, legs, or tracks.
FLOAT tracks unroll directly onto the lunar regolith to avoid major on-site construction — unlike conventional roads, railways, or cableways. Individual FLOAT robots will be able to transport payloads of varying shape / size (>30 kg/m^2) at useful speeds (>0.5m/s), and a large-scale FLOAT system will be capable of moving up to 100,000s kg of regolith / payload multiple kilometers per day. FLOAT will operate autonomously in the dusty, inhospitable lunar environment with minimal site preparation, and its network of tracks can be rolled-up / reconfigured over time to match evolving lunar base mission requirements.
In Phase 2, we will continue to retire risks related to the manufacture, deployment, control, and long-term operation of meter-scale robots / km-scale tracks that support human exploration (HEO) activities on the Moon, by accomplishing the following key tasks:
— Design, manufacture, and test a series of sub-scale robot / track prototypes, culminating with a demonstration in a lunar-analog testbed (that includes testing various site preparation and track deployment strategies)
— Investigate impacts of environmental effects (e.g. temperature, radiation, charging, lunar regolith simulant contamination, etc.) on system performance and longevity
— Investigate / define a technology roadmap to address technology gaps and mature manufacturing capability for critical hardware (e.g. large-area magnetic arrays with mm-scale magnetic domains, and large-area flex-circuit boards)
— Continue refining simulations of FLOAT system designs with increased fidelity, to provide improved performance estimates under the RLSO2 mission concept We will also leverage these sub-scale prototypes to explore opportunities for follow-on technology demonstrations on sub-orbital flights (via Flight Opportunities / TechFlights) or lunar technology demos (via LSII / CLPS landers)
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Radioisotope Thermoradiative Cell Power Generator
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Artist’s depiction of Radioisotope Thermoradiative Cell Power GeneratorStephen PollyStephen Polly
Rochester Institute of Technology
In this project we will continue our Phase I efforts to develop and demonstrate the feasibility of a revolutionary power source for missions to the outer planets utilizing a new paradigm in thermal power conversion, the thermoradiative cell (TRC). Operating like a solar cell in reverse, the TRC converts heat from a radioisotope source into infrared light which is sent off into the cold universe. In this process, electricity is generated. In our Phase I study, we showed 8 W of electrical power is possible from the 62.5 W Pu-238 pellet from a general purpose heat source using a 0.28 eV bandgap TRC operating at 600 K. The necessary array includes 1,125 cm² of TRC emitters, or just over 50% of the surface area of a 6U cubesat. With a mass (heat source + TRC) of 622 g, a mass specific power of 12.7 W/kg is possible, over a 4.5x improvement from heritage multi-mission radioisotope thermoelectric generator (MMRTG) was shown. Building on our results from Phase I, we believe there is much more potential to unlock here.
Using low-bandgap III-V materials such as InAsSb in nanostructured arrays to limit potential loss mechanisms, a 25x improvement in mass specific power and a four order of magnitude decrease in volume from a MMRTG is an early estimate, with higher performance possible depending on operating conditions. TRC technology will allow a proliferation of small versatile spacecraft with power requirements not met by photovoltaic arrays or bulky, inefficient MMRTG systems. This will directly enable small-sat missions to the outer planets as well as operations in permanent shadow such as polar lunar craters.
This study will investigate the thermodynamics and feasibility of the development of a radioisotope enabled thermoradiative power source focusing on system size, weight, power (SWaP) while continuing to integrate the effects of potential power and efficiency loss mechanisms developed in Phase I. Experimentally, materials and TRC devices will be grown including InAsSb-based type-II superlattices by metalorganic vapor phase epitaxy (MOVPE) to target low-bandgap materials with suppressed Auger recombination. Metal-semiconductor contacts capable of surviving the required elevated temperatures will be investigated. TRC devices will be tested for performance at elevated temperature facing a cold ambient under vacuum in a modified cryostat testing apparatus developed in Phase I.
We will analyze a radioisotope thermoradiative converter to power a cubesat mission operating at Uranus. This will include an engineering design study of our reference mission with the Compass engineering team at NASA Glenn Research Center with expertise on the impact of new technologies on spacecraft design in the context of an overall mission, incorporating all engineering disciplines and combining them at a system level. Finally, we will develop a technological roadmap for the necessary components of the TRC to power a future mission.
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The Great Observatory for Long Wavelengths (GO-LoW)
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Artist’s depiction of The Great Observatory for Long Wavelengths (GO-LoW)Mary KnappMary Knapp
MIT
Humankind has never before seen the low frequency radio sky. It is hidden from ground-based telescopes by the Earth’s ionosphere and challenging to access from space with traditional missions because the long wavelengths involved (meter- to kilometer-scale)
require infeasibly massive telescopes to see clearly. Electromagnetic radiation at these low frequencies carries crucial information about exoplanetary and stellar magnetic fields (a key ingredient to habitability), the interstellar/intergalactic medium, and the earliest
stars and galaxies.
The Great Observatory for Long Wavelengths (GO-LoW) proposes an interferometric array of thousands of identical SmallSats at an Earth-Sun Lagrange point (e.g. L5) to measure the magnetic fields of terrestrial exoplanets via detections of their radio emissions at
frequencies between 100 kHz and 15 MHz. Each spacecraft will carry an innovative Vector Sensor Antenna, which will enable the first survey of exoplanetary magnetic fields within 5 parsecs.
In a departure from the traditional approach of a single large and expensive spacecraft (i.e. HST, Chandra, JWST) with many single points of failure, we propose an interferometric Great Observatory comprised of thousands of small, cheap, and easily-replaceable
nodes. Interferometry, a technique that combines signals from many spatially separated receivers to form a large ‘virtual’ telescope, is ideally suited to long wavelength astronomy. The individual antenna/receiver systems are simple, no large structures are required, and the very large spacing between nodes provides high spatial resolution.
In our Phase I study, we found that a hybrid constellation architecture was most efficient. Small and simple “listener” nodes (LNs) collect raw radio data using a deployable vector sensor antenna. A small number of larger, more capable “communication and computation” nodes (CCNs) collect data from LNs via a local radio network, perform beamforming processing to reduce the data volume, and then transmit the data to Earth via free space optics (lasercomm). Cross correlation of the beamformed data is performed on Earth, where computational resources are not tightly constrained. The CCNs are also responsible for constellation management, including timing distribution and ranging. The Phase I study also showed that the LN-CCN architecture optimizes packing efficiency, allowing a small number of super-heavy lift launch vehicles (e.g. Starship) to deploy the entire constellation to L4.
The Phase I study showed that the key innovation for GO-LoW is the “system of systems.” The technology needed for each individual piece of the observatory (e.g. lasercomm, CubeSats, ranging, timing, data transfer, data processing, orbit propagation) is not a big leap from current state of the art, but the coordination of all these physical elements, data products, and communications systems is novel and challenging, especially at scale.
In the proposed study, we will (1) develop a real-time, multi-agent simulation of the GO-LoW constellation that demonstrates the autonomous operations architecture required to achieve a
large (up to 100k) constellation outside of Earth’s orbit, (2) continue to refine the science case and requirements by simulating science output from the constellation and assessing major error sources informed by the real-time simulation, (3) develop appropriate orbital modeling to assess propulsion requirements for stationkeeping at a stable Lagrange point, and (4) further refine the technology roadmap required to make GO-LoW feasible in the next 10-20 years. GO-LoW represents a disruptive new paradigm for space missions. It achieves reliability through massive redundancy rather than extensive testing. It can evolve and grow with new technology rather than being bound to a fixed point in hardware/software development. Finally, it promises to open a new spectral window on the universe where unforeseen discoveries surely await.
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Pulsed Plasma Rocket (PPR): Shielded, Fast Transits for Humans to Mars
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Simplified image of the PPR system. Brianna ClementsBrianna Clements
Howe Industries
The future of a space-faring civilization will depend on the ability to move both cargo and humans efficiently and rapidly. Due to the extremely large distances that are involved in space travel, the spacecraft must reach high velocities for reasonable mission transit times. Thus, a propulsion system that produces a high thrust with a high specific impulse is essential. However, no such technologies are currently available.
Howe Industries is currently developing a propulsion system that may generate up to 100,000 N of thrust with a specific impulse (Isp) of 5,000 seconds. The Pulsed Plasma Rocket (PPR) is originally derived from the Pulsed Fission Fusion concept, but is smaller, simpler, and more affordable. The exceptional performance of the PPR, combining high Isp and high thrust, holds the potential to revolutionize space exploration. The system’s high efficiency allows for manned missions to Mars to be completed within a mere two months. Alternatively, the PPR enables the transport of much heavier spacecraft that are equipped with shielding against Galactic Cosmic Rays, thereby reducing crew exposure to negligible levels. The system can also be used for other far range missions, such as those to the Asteroid Belt or even to the 550 AU location, where the Sun’s gravitational lens focuses can be considered. The PPR enables a whole new era in space exploration.
The NIAC Phase I study focused on a large, heavily shielded ship to transport humans and cargo to Mars for the development of a Martian base. The main topics included: assessing the neutronics of the system, designing the spacecraft, power system, and necessary subsystems, analyzing the magnetic nozzle capabilities, and determining trajectories and benefits of the PPR. Phase II will build upon these assessments and further the PPR concept.
In Phase II, we plan to:
- Optimize the engine design for reduced mass and higher Isp
- Perform proof-of-concept experiments of major components
- Complete a ship design for shielded human missions to Mars
Space Technology Mission Directorate
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Fluidic Telescope (FLUTE): Enabling the Next Generation of Large Space Observatories
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Artist’s depiction of the Fluidic Telescope (FLUTE)Edward BalabanEdward Balaban
NASA ARC
The future of space-based UV/optical/IR astronomy requires ever larger telescopes. The highest priority astrophysics targets, including Earth-like exoplanets, first generation stars, and early galaxies, are all extremely faint, which presents an ongoing challenge for current missions and is the opportunity space for next generation telescopes: larger telescopes are the primary way to address this issue.
With mission costs depending strongly on aperture diameter, scaling current space telescope technologies to aperture sizes beyond 10 m does not appear economically viable. Without a breakthrough in scalable technologies for large telescopes, future advances in
astrophysics may slow down or even completely stall. Thus, there is a need for cost-effective solutions to scale space telescopes to larger sizes.
The FLUTE project aims to overcome the limitations of current approaches by paving a path towards space observatories with largeaperture, unsegmented liquid primary mirrors, suitable for a variety of astronomical applications. Such mirrors would be created in
space via a novel approach based on fluidic shaping in microgravity, which has already been successfully demonstrated in a laboratory neutral buoyancy environment, in parabolic microgravity flights, and aboard the International Space Station (ISS). Theoretically
scale-invariant, this technique has produced optical components with superb, sub-nanometer (RMS) surface quality. In order to make the concept feasible to implement in the next 15-20 years with near-term technologies and realistic cost, we limit the diameter of the primary mirror to 50 meters.
In the Phase I study, we: (1) explored choices of mirror liquids, deciding to focus on ionic liquids, (2) conducted an extensive study of ionic liquids with suitable properties, (3) worked on techniques for ionic liquid reflectivity enhancement, (4) analyzed several alternative architectures for the main mirror frame, (5) conducted modeling of the effects of slewing maneuvers and temperature variations on the mirror surface, (6) developed a detailed mission concept for a 50-m fluidic mirror observatory, and (7) created a set of initial concepts for a subscale small spacecraft demonstration in low Earth orbit.
In Phase II, we will continue maturing the key elements of our mission concept. First, we will continue our analysis of suitable mirror frame architectures and modeling of their dynamic properties. Second, we will take next steps in our machine learning-based modeling and experimental work to develop reflectivity enhancement techniques for ionic liquids. Third, we will further advance the work of modeling liquid mirror dynamics. In particular, we will focus on modeling the effects from other types of external disturbances (spacecraft control accelerations, tidal forces, and micrometeorite impacts), as well as analyzing and modeling the impact of the thermal Marangoni effect on nanoparticle-infused ionic liquids. Fourth, we will create a model of the optical chain from the liquid mirror surface to the science instruments. Fifth, we will further develop the mission concept for a larger-scale, 50-m aperture observatory, focusing on its highest-risk elements. Finally, we will mature the concept for a small spacecraft technology demonstration mission in low Earth orbit, incorporating the knowledge gained in other parts of this work.
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Two Small NASA Satellites Will Measure Soil Moisture, Volcanic Gases
4 min read
Two Small NASA Satellites Will Measure Soil Moisture, Volcanic Gases NASA engineers Austin Tanner (left) and Manuel Vega stand beside SNoOPI, short for Signals of Opportunity P-Band Investigation, at the NanoRacks clean room facility in Houston. NASA / Denny HenryTwo NASA pathfinding missions were recently deployed into low-Earth orbit, where they are demonstrating novel technologies for observing atmospheric gases, measuring freshwater, and even detecting signs of potential volcanic eruptions.
The Signals of Opportunity P-Band Investigation (SNoOPI), a low-noise radio receiver, tests a new technique for measuring root-zone soil moisture by harnessing radio signals produced by commercial satellites — a big job for a 6U CubeSat the size of a shoebox.
Separately, the Hyperspectral Thermal Imager (HyTI) is measuring trace gases linked to volcanic eruptions. HyTI, also a 6U CubeSat, could pave the way for future missions dedicated to detecting volcanic eruptions weeks or months in advance.
Both instruments were launched on March 21 from NASA’S Cape Canaveral Space Force Station to the International Space Station aboard SpaceX’s Dragon cargo spacecraft as part of the company’s 30th commercial resupply mission. On April 21, the instruments were released into orbit from the station.
“Flying Ace” for Finding Freshwater in Soil and SnowAs a measurement technique, “signals of opportunity try to reutilize what already exists,” said James Garrison, professor of aeronautics and astronautics at Purdue University and principal investigator for SNoOPI.
Garrison and his team will try to collect the P-band radio signals produced by many commercial telecommunications satellites and repurpose them for science applications. The instrument maximizes the value of space-based assets already in orbit, transforming existing radio signals into research tools.
SNOOPI will prototype a new technique for measuring soil moisture.“By looking at what happens when satellite signals reflect off the surface of the Earth and comparing that to the signal that has not reflected, we can extract important properties about the surface where the signal reflects,” said Garrison.
P-band radio signals are powerful, penetrating Earth’s surface to a depth of about one foot (30 cm). This makes them ideal for studying root-zone soil moisture and snow water equivalent.
“By monitoring the amount of water in the soil, we get a good understanding of crop growth. We can also more intelligently monitor irrigation,” said Garrison. “Similarly, snow is very important because that’s also a place where water is stored. It has been hard to measure accurately on a global scale with remote sensing.”
High-time for HyTI and High-Resolution Thermal Imaging“I study volcanoes from space to try and work out when they’re going to start and stop erupting,” said Robert Wright, director of the Hawaii Institute of Geophysics and Planetology at the University of Hawaiʻi at Mānoa and the principal investigator for HyTI.
HyTI, short for Hyperspectral Thermal Imager, is testing a novel instrument for measuring thermal radiation.Hyperspectral imagers like HyTI measure a broad spectrum of thermal radiation signatures, and they’re particularly useful for characterizing gases in low concentrations. Wright and his team hope HyTI will help them quantify concentrations of sulfur dioxide in the atmosphere around volcanoes.
Weeks or even months before they erupt, volcanoes often emit increased amounts of sulfur dioxide and other trace gases. Measuring those gases could indicate an impending eruption HyTI’s sensitivity to thermal radiation will also be useful for observing water vapor and convection.
“There are two science objectives for HyTI. We want to try and improve how we can predict when a volcano will erupt and when a volcanic eruption is going to end,” said Wright. “And we’re also going to be measuring soil moisture content as it pertains to drought.”
Setting the Stage for Future Science MissionsThrough its Earth Science Technology Office (ESTO), NASA worked closely with both Garrison and Wright to help transform their research into fully-functioning, space-ready prototypes.
“The ESTO program allows for scientists to have interesting ideas and actually turn them into reality,” said Wright. Garrison agreed. “ESTO’s been a great partner.”
For more information about collaborating with NASA to create new technologies for Earth observation, visit ESTO’s homepage here.
Related Link: SNoOPI: A Flying Ace for Soil Moisture and Snow Measurements
By Gage Taylor
NASA’s Goddard Space Flight Center, Greenbelt, Md.
About the Author Gage TaylorShare
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By Their Powers Combined
By Their Powers Combined
This April 20, 2024, image shows a first: all six radio frequency antennas at the Madrid Deep Space Communication Complex, part of NASA’s Deep Space Network (DSN), carried out a test to receive data from the agency’s Voyager 1 spacecraft at the same time.
Combining the antennas’ receiving power, or arraying, lets the DSN collect the very faint signals from faraway spacecraft. Voyager 1 is over 15 billion miles (24 billion kilometers) away, so its signal on Earth is far fainter than any other spacecraft with which the DSN communicates. It currently takes Voyager 1’s signal over 22 ½ hours to travel from the spacecraft to Earth. To better receive Voyager 1’s radio communications, a large antenna – or an array of multiple smaller antennas – can be used. A five-antenna array is currently needed to downlink science data from the spacecraft’s Plasma Wave System (PWS) instrument. As Voyager gets further way, six antennas will be needed.
Image Credit: MDSCC/INTA, Francisco “Paco” Moreno
May’s Night Sky Notes: Stargazing for Beginners
3 min read
May’s Night Sky Notes: Stargazing for Beginnersby Kat Troche of the Astronomical Society of the Pacific
Millions were able to experience the solar eclipse on April 8, 2024, inspiring folks to become amateur astronomers – hooray! Now that you’ve been ‘bitten by the bug’, and you’ve decided to join your local astronomy club, here are some stargazing tips!
The Bortle ScaleBefore you can stargaze, you’ll want to find a site with dark skies. It’s helpful learn what your Bortle scale is. But what is the Bortle scale? The Bortle scale is a numeric scale from 1-9, with 1 being darkest and 9 being extremely light polluted; that rates your night sky’s darkness. For example, New York City would be a Bortle 9, whereas Cherry Springs State Park in Pennsylvania is a Bortle 2.
The Bortle scale helps amateur astronomers and stargazers to know how much light pollution is in the sky where they observe. International Dark Sky AssociationDetermining the Bortle scale of your night sky will help narrow down what you can expect to see after sunset. Of course, other factors such as weather (clouds namely) will impact seeing conditions, so plan ahead. Find Bortle ratings near you here: www.lightpollutionmap.info
No Equipment? No Problem!There’s plenty to see with your eyes alone. Get familiar with the night sky by studying star maps in books, or with a planisphere. These are great to begin identifying the overall shapes of constellations, and what is visible during various months.
A full view of the northern hemisphere night sky in mid-May. Stellarium WebInteractive sky maps, such as Stellarium Web, work well with mobile and desktop browsers, and are also great for learning the constellations in your hemisphere. There are also several astronomy apps on the market today that work with the GPS of your smartphone to give an accurate map of the night sky.
Keep track of Moon phases. Both the interactive sky maps and apps will also let you know when planets and our Moon are out! This is especially important because if you are trying to look for bright deep sky objects, like the Andromeda Galaxy or the Perseus Double Cluster, you want to avoid the Moon as much as possible. Moonlight in a dark sky area will be as bright as a streetlight, so plan accordingly! And if the Moon is out, check out this Skywatcher’s Guide to the Moon: bit.ly/MoonHandout
Put On That Red LightIf you’re looking at your phone, you won’t be able to see as much. Our eyes take approximately 30 minutes to get dark sky adapted, and a bright light can ruin our night vision temporarily. The easiest way to stay dark sky adapted is to avoid any bright lights from car headlights or your smartphone. To avoid this, simply use red lights, such as a red flashlight or headlamp.
The reason: white light constricts the pupils of your eyes, making it hard to see in the dark, whereas red light allows your pupils to stay dilated for longer. Most smartphones come with adaptability shortcuts that allow you to make your screen red, but if you don’t have that feature, use red cellophane on your screen and flashlight.
Up next: why binoculars can sometimes be the best starter telescope, with Night Sky Network’s upcoming mid-month article through NASA’s website!
How NASA Continues Inspiring Engineer’s Future
Work at NASA’s Stennis Space Center near Bay St. Louis, Mississippi, takes one site engineer back to a childhood memory, where a dream of being a member of the NASA team began. Now, Briou Bourgeois is working to launch a career with even bigger aspirations.
A lot of the work we do at NASA Stennis … I think is going to be beneficial to the agency’s focus of establishing the first long-term presence on the MoonBriou Bouregois
NASA Stennis Mechanical Test Operations Engineer
The Bay St. Louis native recalls childhood watching the Apollo 13 movie with his dad. He became fascinated with the story of how astronauts overcame challenges when NASA attempted the third lunar landing in 1970.
Even as the lunar portion of the mission was aborted due to the rupture of a service module oxygen tank, Bourgeois was fascinated by how everybody on the ground at NASA’s Johnson Space Center in Houston fought through challenges to come up with solutions.
Bourgeois said he did not understand the gravity of the situation he was watching unfold, but he was not short of questions. He wanted to learn more.
“That probably spurred me into wanting to become part of the NASA team but, even more so, to become an astronaut and be sort of the tip of the spear when it comes to space exploration and doing the hard things that allow humanity to further understand the universe and space in general,” Bourgeois said.
Now in his seventh year at NASA Stennis, the Mississippi State University graduate said the wide range of testing capabilities at the south Mississippi site, coupled with working alongside a variety of people “highly specialized in the aerospace operations realm” is what he enjoys most.
He currently works at the versatile E Test Complex, where the mechanical test operations engineer supports research and development testing as NASA collaborates with commercial companies pursuing a future in space.
The Pass Christian, Mississippi, resident is the mechanical operations lead for the Relativity Space thrust chamber assembly test project and the Blue Origin pre-burner project. In those roles, he has written test procedures and developed a thorough knowledge of test operations.
Even as Bourgeois continues adding to his experience, he also has applied to become a NASA astronaut. Thanks, to his work at NASA Stennis, he feels equipped to make the split-second decisions needed during highly critical and hazardous moments. In addition, his NASA Stennis experience has taught him greatly about the importance of teamwork.
“A lot of the work we do at NASA Stennis with propellant transfers, managing cryogenic systems, pneumatic systems, hydraulic systems, and just having the hands-on experience and operational knowledge of those systems, I think is going to be beneficial to the agency’s focus of establishing the first long-term presence on the Moon,” Bourgeois said.
Whether Bourgeois’ future is at NASA Stennis or beyond, the NASA employee looks forward to helping the agency explore the secrets of the universe for the benefit of all.
Learn more about the people who work at NASA StennisU.S. Department of State Open House at NASA Headquarters
This event was part of Space Diplomacy Week, focused on deepening bilateral relationships, specifically how international partnerships are strengthened by space exploration.
NASA Ames Astrogram – March/April 2024
On April 23, the Advanced Composite Solar Sail System CubeSat mission launched successfully aboard an Electron rocket launched by Rocket Lab and carried Ames’ payload from Māhia, New Zealand. The CubeSat was subsequently delivered to a Sun-synchronous orbit around Earth.
Ames has pioneered the use of CubeSats and small satellites to run innovative, cost-effective missions and test technologies in space, providing leadership in cost-effective spaceflight missions for NASA.
An artist’s concept of NASA’s Advanced Composite Solar Sail System spacecraft in orbit.NrediASA/Aero Animation/Ben SchweighartUnder the auspices of STMD’s Small Spacecraft Technology Program, the Advanced Composite Solar Sail System mission demonstrates next-generation solar sail technology for small interplanetary spacecraft. It will test a new way of navigating our solar system when the mission’s CubeSat hoists its sail into space – not to catch the wind, but the propulsive power of sunlight. This technology could advance future space travel and expand our understanding of our Sun and solar system.
NASA, FAA Partner to Develop New Wildland Fire TechnologiesRecently, NASA and the Federal Aviation Administration (FAA) established a research transition team to guide the development of wildland fire technology.
Wildland fires are occurring more frequently and at a larger scale than in past decades, according to the U.S. Forest Service. Emergency responders will need a broader set of technologies to prevent, monitor, and fight these growing fires more effectively. Under this Wildland Fire Airspace Operations research transition team, NASA and the FAA will develop concepts and test new technologies to improve airspace integration.
Artist’s rendering of remotely piloted aircraft providing fire suppression, monitoring and communications capabilities during a wildland fire.Credit: NASACurrent aerial firefighting operations are limited to times when aircraft have clear visibility – otherwise pilots run the risk of flying into terrain or colliding with other aircraft. Drones could overcome this limitation by enabling responders to remotely monitor and suppress these fires during nighttime and low visibility conditions, such as periods of heavy smoke. However, advanced airspace management technologies are needed to enable these uncrewed aircraft to stay safely separated and allow aircraft operators to maintain situational awareness during wildland fire management response operations.
Over the next four years, NASA’s Advanced Capabilities for Emergency Response Operations (ACERO) project, in collaboration with the FAA, will work to develop new airspace access and traffic management concepts and technologies to support wildland fire operations. These advancements will help inform a concept of operations for the future of wildland fire management under development by NASA and other government agencies. The team will test and validate uncrewed aircraft technologies for use by commercial industry and government agencies, paving the way for integrating them into future wildland fire operations.
ACERO is led out of NASA’s Ames Research Center in Silicon Valley under the agency’s Aeronautics Research Mission Directorate.
Studying the Ocean with NASA Computer Simulations A tool developed at NASA Ames’ Advanced Supercomputing division provides researchers with a global view of their ocean simulation in high resolution. In this part of the global visualization, the Gulf Stream features prominently. Surface water speeds are shown ranging from 0 meters per second (dark blue) to 1.25 meters (about 4 feet) per second (cyan). The video is running at one simulation day per second. The data used comes from the Estimating the Circulation and Climate of the Ocean (ECCO) consortium.Credit: NASA/Bron Nelson, David Ellsworth“Every time I help with visualizing [ocean] simulation data, I learn about an entirely new area of ocean or climate research, and I’m reminded of how vast and rich this area of research is. And…the real magic happens at the intersection and interaction of simulated and observed data.
It is a great honor – and a thrill – to collaborate with devoted, world-class scientists doing such important, cutting-edge research and sometimes to even help them learn something new about their science.”
—Dr. Nina McCurdy, a data visualization scientist with the NASA Advanced Supercomputing division at NASA’s Ames Research Center in California’s Silicon Valley
Luxembourg Leaders Focus on Lunar Exploration During Visit to NASA Amesby Abigail Tabor
The challenges of working on the surface of the Moon are at the center of a facility at NASA’s Ames Research Center in California’s Silicon Valley. The Lunar Lab and Regolith Testbeds help scientists and engineers – from NASA and industry alike – study how well science instruments, robots, and people might be able to safely work, manipulate, navigate, and traverse the tough lunar terrain. On March 7, three visitors from the Grand Duchy of Luxembourg – Deputy Prime Minister Xavier Bettel, Minister of the Economy Lex Delles, and Ambassador to the United States Nicole Bintner – learned more about the work happening here.
Left to right: Ames Deputy Center Director David Korsmeyer, Ames Center Director Eugene Tu, Deputy Prime Minister of Luxembourg Xavier Bettel, Luxembourg Minister of Economy Lex Delles, and Ambassador Nicole Bintner meet at Ames on March 7, 2024.Credit: NASA Ames/Brandon TorresDuring the visit, lunar rock and crater features crafted from lunar soil, or regolith, simulant were lit by harsh, low-angle illumination to simulate sunlight conditions at the Moon’s poles. Members of the VIPER mission (Volatiles Investigating Polar Exploration Rover) discussed their work testing optical sensors at the lab for NASA’s water-hunting Moon rover. Engineering versions of VIPER’s hazard-avoidance cameras and lighting system, tested in the facility, were also on display. The lab is managed by NASA’s Solar System Exploration Research Virtual Institute (SSERVI).
The Regolith Testbeds enable research applicable to places beyond our Moon as well, including Mercury, asteroids, and regolith-covered moons like Mars’ Phobos.
Luxembourg was one of the first nations to sign the Artemis Accords and has taken steps to enable commercial space exploration. At Ames, the visitors learned about the center’s support of NASA’s Artemis exploration goals, including with VIPER, agency supercomputing resources, and the development of advanced tools for lunar operations.
AI, Robots, Autonomy Software Discussed at Star Trek Convention Above: Left to right are Abigail Tabor of the Office of Communications Division, J. Benton, computer science researcher; and Dr. Jennifer Blank, senior scientist in the Space Science and Astrobiology Directorate speaking on a panel at the March Star Trek Convention held in Hyatt Regency SFO, Burlingham, California. They spoke about artificial intelligence for a future space station that will orbit the Moon and the use of legged robot technology, autonomy software, and remote science operations in a volcanic cave. At least 7,000 attended the Star Trek Convention. Majoring in Liberal Studies: Giving Back, Honoring Culture, and Working at NASAChoosing a major can be intimidating, so finding Liberal Studies was perfect for community-centered Maria Lopez, deputy operations manager for the NASA Ames Exchange. Maria was interviewed by the Puente Project, a mission to increase the number of educationally underrepresented students who enroll in four-year colleges and universities, as part of the “Puente Major 2 Career Video Series.” The Major 2 Career video series, which is on YouTube, focuses on different majors. The project highlights various professionals’ journey from college to their career. The premise is to feature two professionals who earned the same bachelor’s degrees but following different professions to show the range and opportunities to first-generation college bound students currently at the middle school, high school, and community college levels.
Maria highlighted how she landed on Liberal Studies after trying a few majors, the challenges she faced along the way, and her unexpected and exciting career with NASA. She started out in STEM education and has supported the NASA mission in different roles with the technical publications office, international office, protocol office, and the office of diversity and equal opportunity. Maria shares an array of mission enabling positions with NASA and how NASA fuels her passion for celebrating culture and community outreach. In the video, she demonstrates by example that NASA is within reach and inspires students to pursue their dreams.
Watch and learn more about Maria’s journey!
Maria on detail with the Protocol Office supporting a presidential visit in 2023.Credit: photo by Lisa Lockyer Ames Engineer Natasha Schatzman Excites Kids about the Mars Helicopter On April 13, the Sunnyvale Public Library hosted “Space Camp 2024” with space-themed activities for kids, such as crafts, scavenger hunts, speakers, and more. Apollo 16 lunar samples were displayed at the event and Ames engineer Dr. Natasha Schatzman of Code AV gave a presentation to an enthusiastic crowd of a few hundred people about her NASA journey, her work on the Mars helicopter efforts, and led a Mars paper helicopter activity with the children. Students young and old enjoyed the fun of learning about vertical flight. Mayor Larry Klein attended the event and did a reading for the kids. Ames Staff Shares NASA Mission Info with Cal Academy Nightlife AttendeesAmes Office of Communications (OComm) supported a NASA exhibits booth at the California Academy of Sciences Nightlife festivities on the evening of Feb. 29, in Golden Gate Park, San Francisco. About a third of the 2,000 plus attendees interacted with the NASA booth and presenters, experiencing many high-quality interactions with many of the attendees. The QUESST (NASA’s mission to demonstrate how the X-59 can fly supersonic without generating loud sonic booms), VIPER (Volatiles Investigating Polar Exploration Rover), Artemis, Orion missions were discussed and many attendees were asked if they’d like to send their names with VIPER on its upcoming launch. Hillary Smith of OComm is seen below interacting with visitors at the event.
Hillary Smith at Academy of Sciences in San Francisco interacting with event attendees. Lego Exhibit Brings Out the Engineering Creativity with the KidsOn April 13 and 14, the Office of Communications team members facilitated VIPER’s (Volatiles Investigating Polar Exploration Rover) subject matter experts Vandana Jay and Hans Thomas who interacted with audiences at LEGOLand Bay Area in Miliptas, California. The experts worked alongside “master builders” supplied by LEGOLand to help younger engineers design and test moon rovers of their own creation, creating a fun engineering challenge. During the day, the team interacted with about 80 families and close to 500 individual attendees. See below for photos from the event.
Kids enjoying making their own little lego Moon rovers. Building rovers at the April 13 LegoLand Bay Area event. Moon rovers built by students at the April 13 LegoLand Bay Area event. Building model lego rovers. Ames Space Biology and Astrobiology Teams Engage Kids with Science Demos Tri-Valley Innovation Fair at Alameda County Fairgrounds was held April 18 – 19 and is an annual event featuring STEM (science, technology, engineering, and math) providers and vendors across the Bay Area. The Ames booth highlighted the Space Biology and Astrobiology groups. The space biology team highlighted how model organisms, such as tardigrades, drosophila, yeast and C. elegans give researchers insights into the effects of space on living organisms and the astrobiology team highlighted the search for life in the universe and Earth’s extremophiles. Attendees to the event enjoyed posing with the astronaut cutouts and learning about the electromagnetic spectrum and the James Webb Space Telescope with an interactive infrared demo. Close to 1,000 interactions occurred during the event. SJCU Research Week Event Highlights its Partnerships with NASA Ames San Jose State University (SJSU) Research Week, April 15 – 19, consists of a series of events at the campus that highlight the university’s engagement in research with partners such as NASA Ames. The Ames booth at Paseo de Cesar Chavez on campus on April 15 featured the TechEdSat small sat project, the Ames Aeronautics directorate and OSTEM. Marcus Murbac and his team comprised of many SJSU alumni, showed off their latest iteration of the TechEdSat and Zach Roberts spoke about Ames aeronautics projects as well as a couple of drones. Francesa Bura, an intern at Ames, talked about internship and OSTEM resources. Information about Ames Atmospheric Sciences and NASA jobs also were shared. About 200 students visited the display and the event supported the activities that Ames has with the university. PASIFIKA STEM Fair Provides Engaging Hands-on STEM Experience The Bay Area PASIFIKA STEM Fair is an annual event organized by the Pacific Islander Encouraging Fun Engineering Science and Technology (PIEFEST) organization dedicated to improving Pacific Islander representation and access to STEM (Science, Technology, Engineering and Math) related careers. The event brings STEM organization and enthusiasts in the Bay Area together to provide Pacific Islander students and families an Interactive, hands-on STEM experience. The NASA booth featured a new VIPER mission demo, permanently shadowed craters of the Nobile region, and emissions spectra of various elements and molecules, the astronaut cutouts, as well as an electromagnetic spectrum demo. More than 1,000 students of varying grade levels and their parents and families attended the event, with more than 20 vendors participating with hands-on activities and demonstrations. Interacting with the exhibits at the Bay Area PASIFIKA STEM Fair. Jonas Dino of the Ames Office of Communications Division at the Bay Area PASIFIKA STEM fair, connecting with and inspiring kids of all ages as to the wonders of science. Kids enjoying the interactive exhibits at the NASA booth during the Bay Area PASIFIKA STEM Fair. Future Aspirations, the Importance of STEM Discussed at Grimmer Career Day Jonas Dino from the Ames Public Engagement team was the featured speaker at the Grimmer Elementary Career Day on April 26. He presented to the entire school body of more than 300 TK to 5th grade students, teachers and administrators talking about careers at NASA and the need for the students to be STEM literate and possibly entering the NASA workforce pipeline in the future. He also interacted with the students at lunch talking to them about their future aspirations and answering specific questions they had about NASA. The career day featured members of the Fremont community including fire, police, engineers and medical personnel visiting classrooms talking about their careers. Starling Stuns at Golden Gate Park Planetarium Show Bay Area audiences got a unique look at a NASA Ames CubeSat mission during a full-dome planetarium show as part of the Benjamin Dean lecture series at the Morrison Planetarium at the California Academy of Sciences in Golden Gate Park, San Francisco, on March 4. NASA Ames aerospace flight systems engineer and Starling mission deputy project manager Scott Miller shared Ames’ legacy in CubeSats and swarms and how technologies used in NASA’s Starling mission aims to tackle crowding in low Earth orbit and enhance how we study deep space, in his presentation, “NASA Spacecraft Swarms for Low Earth Orbit and Beyond.” Credit: photos by Josh Roberts In Memoriam …Dr. Anna McHargue (Colonel, USAF, Ret.) passed away peacefully on March 26, 2024, at the Veterans Administration Medical Center in Palo Alto, California. Hospital staff honored her with a brief ceremony for passing veterans, which her close friends attended.
Dr. Anna McHargueDr. McHargue began her higher education at Murray State University in Kentucky, graduating in 1956 and eventually being selected as Distinguished Alumna. She pursued her medical degree at the University of Louisville School of Medicine in Kentucky, at a time when women were not very welcome in the field. She persevered and finished at the top of her class in 1962. She chose not to specialize in obstetrics and gynecology until later at the Stanford University Hospital, where she was a faculty member from 1974-1980. She practiced in the specialty for several years in Oakland and in Redwood City, California, and became a Fellow of the American College of Obstetricians and Gynecologists.
She served in the United States Air Force (USAF), joining in 1966, was promoted to colonel, and was trained as an aviation medical examiner qualified to perform Federal Aviation Administration flight physicals. She enjoyed flying all over the world with transport aircraft crews on military and humanitarian missions. In the USAF Reserves, she was named the 1999 and 2000 Flight Surgeon of the Year by the 312th Airlift Squadron. She retired in 2001 after 25 years of service.
From 1989-2020, she served as a part-time physician at the Health Unit at NASA’s Ames Research Center. Ultimately, she dedicated herself to the field of medicine for 58 years. Dr. McHargue was actively involved in the Church of the Advent as a deacon and on the Board of Trustees of Grace Cathedral in San Francisco.
Her funeral service and internment are planned at her hometown in Kentucky. Friends can donate and send condolences online to:
Equal Opportunity if the LawSols 4171-4172: Scoot Over!
3 min read
Sols 4171-4172: Scoot Over! This image was taken by Right Navigation Camera onboard NASA’s Mars rover Curiosity on Sol 4169 (2024-04-28 19:56:23 UTC). NASA/JPL-CaltechEarth planning date: Monday, April 29, 2024
On this two sol-planning day, the Curiosity science team logged in and found ourselves face to face with ‘Pinnacle Ridge’ (pictured above), part of the upper Gediz Vallis Ridge (uGVR). We saw two types of rocks in our workspace: light-toned layered rocks and darker toned rocks. Rocks that look this different are very exciting to a geologist’s eye – it means the rocks could have been formed in different environments, and could be made of different things… so how did these two types of rock end up next to each other? That’s for our clever team of scientists to work out, and we need our full suite of instruments to do that. Unfortunately, one of Curiosity’s wheels wasn’t on firm ground so we couldn’t safely unstow the arm, but these rocks are so exciting, we decided to scoot backwards about 15 cm to readjust the wheels so we can hopefully get full contact science on Wednesday.
However, we made the most of the time we have here taking lots of images. On the first sol, Curiosity has a massive 2.5 hours of science planned! This includes ChemCam Laser Induced Bedrock Spectroscopy (LIBS) and a Mastcam documentation image on one of the lighter toned rocks in the workspace named ‘Dawn Wall,’ as well as a passive observation on a darker toned rock named ‘Banner Peak.’ ChemCam will also take an RMI of ‘Pinnacle Ridge,’ and a long distance RMI of the base of ‘Kukenan’ butte. Team members interested in Mastcam are making the most of the science time scheduling a massive 37×2 mosaic of ‘Pinnacle Ridge’ to look at the distribution of the light and dark toned rocks we are seeing, as well as two smaller mosaics including within Pinnacle Ridge including a 9×1 of a scarp and a 4×1 of a possible basal contact. On this sol, Curiosity will then scoot over – a drive of ~15 cm – hopefully giving us a stable base to unstow the arm and get full contact science on these rocks later in the week.
On the second sol, Curiosity performs a ChemCam LIBS target on a rock in our new(ish) workspace. Curiosity will also take some environmental monitoring activities, including a 30 minute Navcam dust devil movie and a suprahorizon movie. We are also performing the SAM instrument’s electrical baseline test (EBT) that periodically occurs to monitor the instrument’s functioning. Curiosity will be kept very busy over the next few sols exploring Pinnacle Ridge here at uGVR.
Written by Emma Harris, Graduate Student at Natural History Museum
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NASA Balloons Head North of Arctic Circle for Long-Duration Flights
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Preparations for Next Moonwalk Simulations Underway (and Underwater)NASA is set to begin launch operations mid-May for the 2024 Sweden Long-Duration Scientific Balloon Campaign. Four stadium-sized, scientific balloons carrying science missions and technology demonstrations are scheduled to lift off from Swedish Space Corporation’s Esrange Space Center, situated north of the Arctic Circle near Kiruna, Sweden. The campaign will continue through early July.
Technicians attach the SUNRISE payload to its balloon and parachute from the launch site in Kiruna, Sweden, during the 2009 campaign. The mission returns for the 2024 Sweden Long-Duration Scientific Balloon Campaign as one of four primary missions set to launch between May and July.University Corporation for Atmospheric Research“NASA’s Balloon Program is excited to conduct our long-duration balloon campaign from Sweden this year,” said Andrew Hamilton, acting director of NASA’s Balloon Program Office. “Our partnership with the Swedish Space Corporation is valuable to NASA and the scientific community by allowing us to use their high-quality facilities at Esrange.”
Esrange, located in a vast unpopulated area in the northernmost part of Sweden, is an ideal location for the campaign. This area in Sweden’s polar region experiences constant daylight during summer. NASA’s zero-pressure balloons, used during the campaign, typically experience gas loss during the warming and cooling of the day to night cycle. However, they can perform long-duration flights in the constant sunlight of a polar region. “The location of the launch range and the stratospheric winds allow for excellent flight conditions to gather many days of scientific data as the balloons traverse from Sweden to northern Canada,” said Hamilton.
Four primary missions on deck for the Sweden campaign include:
- HELIX (High-Energy Light Isotope eXperiment): A balloon-borne experiment that features a powerful superconducting magnet designed to measure the flux of high-energy cosmic ray isotopes to energies that have not been explored. The measurements will help determine the age of cosmic rays in our galaxy.
- BOOMS (Balloon Observation of Microburst Scales): A high-resolution imager of X-rays from energetic electron microbursts that appear in the polar atmosphere. The mission will fly on a 60 million cubic feet balloon, a test flight set to qualify the balloon for reaching altitudes greater than 150,000 feet, which is higher than NASA’s current stratospheric inventory.
- SUNRISE-III: A solar observatory that takes high-resolution imaging and spectro-polarimetry of layers of the Sun called the solar photosphere and chromosphere, and active regions to measure magnetic field, temperature, and velocities with high height temporal resolution.
- XL-Calibur: A telescope that will observe a sample of galactic black hole and neutron star sources to gain new insight on how these objects accelerate electrons and emit X-rays.
Piggyback missions, or smaller payloads, sharing a ride on the XL-Calibur balloon flight include:
- IRCSP (Infrared Channeled Spectro-Polarimeter): A technology development mission for high-altitude spectro-polarimetric measurements of cloud tops to help improve measurements of the size and shape of ice particles, which are crucial in understanding weather and improving climate models.
- WALRUSS (Wallops Atmospheric Light Radiation and Ultraviolet Spectrum Sensor): A technology development mission for a sensor package capable of measuring the total ultraviolet (UV) − split among UVA, UVB, and UVC wavelengths − and ozone concentration.
NASA’s scientific balloons are a quick and cost-effective way to test, track, and recover scientific experiments for NASA and universities from all over the world. These heavy-lift balloons offer near-space access for suspended payloads weighing up to 8,000 pounds.
NASA’s Wallops Flight Facility in Virginia manages the agency’s scientific balloon flight program with 10 to 15 flights each year from launch sites worldwide. Peraton, which operates NASA’s Columbia Scientific Balloon Facility (CSBF) in Texas, provides mission planning, engineering services, and field operations for NASA’s scientific balloon program. The CSBF team has launched more than 1,700 scientific balloons over some 40 years of operations. NASA’s balloons are fabricated by Aerostar. The NASA Scientific Balloon Program is funded by the NASA Headquarters Science Mission Directorate Astrophysics Division.
For mission tracking, click here. For more information on NASA’s Scientific Balloon Program, visit: https://www.nasa.gov/scientificballoons.
NASA’s Wallops Flight Facility, Wallops Island, Va.
Share Details Last Updated Apr 30, 2024 EditorJamie AdkinsContactOlivia F. Littletonolivia.f.littleton@nasa.govLocationWallops Flight Facility Related Terms Explore More 3 min read NASA Wallops to Launch Three Sounding Rockets During Solar Eclipse Article 4 weeks ago 2 min read NASA, Salisbury U. Enact Agreement for Workforce Development Article 1 month ago 2 min read NRO Mission Launches from NASA Wallops on Electron Rocket Article 1 month agoNASA Showcases Innovations at the 2024 FIRST Robotics World Championships
NASA engaged with fans, student robotics teams, and industry leaders at the 2024 FIRST Robotics World Championships held April 17-20, at the George R. Brown Convention Center in Houston. The exhibit highlighted the future of technology and spaceflight, attracting over 50,000 participants from across the United States and worldwide.
The FIRST Robotics World Championships was established in 1992. Since relocating to Houston in 2017, the event has featured significant involvement from NASA, which annually supports and mentors more than 250 robotics teams, from elementary to high school levels.
Students and mentors explored NASA exhibits at the 2024 FIRST Robotics World Championships at the George R. Brown Convention Center from April 17-20. Credit: NASA/Joseph ZakrzewskiThe 2024 championships celebrated the integration of arts into STEM (science, technology, engineering, and math), empowering students to create a world of endless possibilities with big ideas, bold actions, and creativity.
Multiple NASA centers participated in the event including the Johnson Space Center, Armstrong Flight Research Center, Ames Research Center, Glenn Research Center, Goddard Space Flight Center, Katherine Johnson Independent Verification and Validation Facility, Kennedy Space Center, Jet Propulsion Laboratory, Langley Research Center, Michoud Assembly Facility, and Stennis Space Center.
The NASA exhibits offered a platform for engaging discussions about the agency’s latest projects, including the X-59 supersonic plane, the Automated Reconfigurable Mission Adaptive Digital Assembly Systems, the Volatiles Investigating Polar Exploration Rover, Mars Perseverance Rover and Ingenuity Helicopter, Cooperative Autonomous Distributed Robotic Exploration, Exobiology Extant Life Surveyor, and the Europa Clipper mission. These interactions provided a firsthand look at NASA’s groundbreaking science and technologies and their potential to benefit all humanity.
Attendees learn about NASA’s Europa Clipper mission at the 2024 FIRST Robotics World Championships. Credit: NASA/Joseph Zakrzewski“The energy during the event was phenomenal. It’s inspiring to see so many people passionate about robotics and eager to solve complex problems,” said Johnson Public Affairs Specialist Joseph Zakrzewski. “We are excited to unite tomorrow’s leaders from all corners of the world.”
The event also fostered discussions about STEM career opportunities, with many students expressing their aspirations to join the space industry.
As the championships drew to a close, the excitement was palpable, with students and mentors alike looking forward to the next season. With a successful turnout and the enthusiastic involvement of teams, sponsors, volunteers, and supporters, the future of STEM education appears brighter than ever.
Johnson Celebrates New Opportunities for Space Industry in Texas
NASA’s Johnson Space Center was recently involved in two major announcements with important implications for the future of space exploration and the aerospace industry.
On Feb. 29, 2024, NASA announced that the American Center for Manufacturing and Innovation (ACMI) signed an agreement to become a tenant at Johnson’s 240-acre Exploration Park. ACMI will lease a portion of the underutilized land to develop a Space Systems Campus that enables commercial and defense space manufacturing. The campus will incorporate an applied research facility partnered with multiple stakeholders across academia, state and local government, the Department of Defense, and regional economic development organizations.
NASA signed a separate lease with the Texas A&M University System earlier this year. Both agreements represent key achievements for Johnson’s Dare | Unite | Explore, with commitments focused on maintaining the center’s position as the hub of human spaceflight, developing strategic partnerships, and paving the way for a thriving space economy.
American Center for Manufacturing and Innovation Founder and CEO John Burer shakes hands with NASA’s Johnson Space Center Director Vanessa Wyche at the Bay Area Houston Economic Partnership’s aerospace advisory committee meeting on March 6, 2024. Photo Credit: NASA/Robert MarkowitzJohnson Center Director Vanessa Wyche shared the news at the Bay Area Houston Economic Partnership’s aerospace advisory committee meeting on March 6, emphasizing the agreement’s value to NASA, the State of Texas, and the nation. “At JSC, we have a vision to dare to expand frontiers and unite with our partners to explore for the benefit of all humanity. Today’s announcement is a significant component of bringing that vision to fruition,” she said. “The future of Texas’ legacy in aerospace is bright as Exploration Park will create an unparalleled aerospace, economic, business development, research and innovation region across the state.”
Texas’ role in space exploration and aerospace development was also highlighted during Governor Greg Abbott’s visit to Johnson on March 26. Abbott toured the Mission Control Center and spoke to native Texan and NASA astronaut Loral O’Hara aboard the International Space Station before joining Wyche and other state leaders to announce the launch of the Texas Space Commission and the Texas Aerospace Research and Space Economy Consortium. Speaking to media in Johnson’s Space Vehicle Mockup Facility, Abbott said that these new entities will promote innovation in the fields of space exploration and commercial aerospace, including by identifying research and development opportunities.
“We are so excited for what the Texas Space Commission will bring to the state of Texas and the flourishing aerospace industry here,” said Wyche. “With continued investment in the region, the Texas economy will benefit significantly from the ancillary job creation and growth resulting from new aerospace companies in the state.”
Several former NASA employees were named to the Commission’s inaugural board of directors and the Consortium’s first executive committee. They include Kathy Lueders, John Shannon, Kirk Shireman, Matt Ondler, Robert Ambrose, Brian Freedman, and former astronauts Nancy Currie-Gregg and Jack “2fish” Fischer.
