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The president of the Chicago Teachers Union explains how climate change became a pillar of the union’s contract demands

A Satellite for Optimal Control and Imaging (SOC-i) CubeSat awaits integration at Firefly’s Payload Processing Facility at Vandenberg Space Force Base, California on Thursday, June 6, 2024. SOC-i, along with several other CubeSats, will launch to space on an Alpha rocket during NASA’s Educational Launch of Nanosatellites (ELaNa) 43 mission as part of the agency’s CubeSat Launch Initiative and Firefly’s Venture-Class Launch Services Demonstration 2 contract.Photo credit: NASA

Eight CubeSats that are part of NASA’s CubeSat Launch Initiative have been integrated into Firefly Aerospace’s deployment hardware and are ready to be encapsulated into the payload fairing of Firefly’s Alpha rocket. The launch, named “Noise of Summer,” will lift off early this summer from Space Launch Complex 2 at Vandenberg Space Force Base in California. 

University students from several schools, along with some technicians from NASA, brought their small satellites to Firefly for integration with the rocket. The satellites are designed to perform a range of scientific experiments and technical demonstrations including high-speed communications, cosmic ray detection, climate monitoring, and new de-orbiting techniques. 

The CubeSats on the ELaNa 43 (Educational Launch of a Nanosatellite) manifest are: 

• CatSat – University of Arizona, Tucson, Arizona 
• KUbe-Sat-1 – University of Kansas, Lawrence, Kansas 
• MESAT1 – University of Maine, Orono, Maine 
• R5-S4 – NASA’s Johnson Space Center, Houston, Texas 
• R5-S2-2.0 – NASA’s Johnson Space Center, Houston 
• SOC-i – University of Washington, Seattle, Washington 
• TechEdSat-11 – NASA’s Ames Research Center, California’s Silicon Valley 
• Serenity – Teachers in Space  

Students are heavily involved in all aspects of their mission from developing, assembling, and testing payloads to working with NASA and the launch vehicle integration teams. The CubeSats are held to rigorous standards like that of the primary spacecraft.  

Firefly Aerospace is one of three companies selected under NASA’s Launch Services Program Venture-Class Launch Services Demonstration 2 (VCLS Demo 2) contract awarded in December 2020. These VCLS Demo 2 missions can tolerate a higher level of risk and help create opportunities for new launch vehicles, helping grow the launch vehicle market while increasing access to space for small spacecraft and science missions. 

2 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater) In developing its flow battery, ESS drew from groundbreaking research and development conducted by the space agency more than 40 years ago. Pictured here, a 200-watt demonstration unit of the flow battery NASA built in the 1970s and 1980s.Credit: NASA

Solar power is abundant – when the Sun is shining. Wind power is steady – when the wind is blowing. However, creating a steady electricity supply from intermittent power sources is a challenge. NASA was focused on this problem more than 45 years ago when the agency designed a new type of liquid battery during the energy price shocks of the 1970s. While engineers continued over the following decades to develop flow batteries, as they’re now called, the technology has drawn even more attention in recent years, with the urgency of climate change powering a larger-scale transition to renewables like solar and wind.

It’s fair to say that flow batteries today owe something to the major push the technology received in the 1970s when a NASA team of chemical, electrical, and mechanical engineers developed an iron-chromium flow battery at Lewis Research Center – now Glenn Research Center – in Cleveland.

The NASA system involved two tanks of liquid electrolyte solutions, one infused with iron chloride and the other with chromium chloride. These electrolytes were pumped through the battery cell, triggering a chemical reaction through a membrane that separated the two solutions inside the battery. During charge, electrical energy was converted to chemical energy and stored in the electrolyte liquid. To discharge the energy, the process was reversed.

ESS flow batteries enable a steady supply of electricity from intermittent energy sources, such as wind and solar. They store up to 12 hours of energy and discharge it when needed. They can be built in shipping containers, like the one being installed in the picture here, or larger installations can be housed in a building.Credit: ESS Inc.

Wilsonville, Oregon-based ESS Inc. built on NASA’s early work as the company developed its own flow batteries using only iron, salt, and water.  When the ESS team began developing its battery in 2011, the company founders wanted to use iron as NASA had. They found they could pair iron with a simple salt solution, which was cheaper to obtain and easier to work with than the chromium mixture NASA had used.

ESS flow batteries are designed for power grids that are increasingly powered by intermittent wind and solar generation. The company’s systems store up to 12 hours of energy and are used to provide backup power to critical community facilities.

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Details Last Updated Jun 20, 2024 Related Terms

• Spinoffs
• Glenn History
• Glenn Research Center
• NASA History
• Technology Transfer
• Technology Transfer & Spinoffs

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Technology

NASA is very interested in developing a propulsion method to allow spacecraft to go faster. We’ve reported several times on different ideas to support that goal, and most of the more successful have utilized the Sun’s gravity well, typically by slingshotting around it, as is commonly done with Jupiter currently. But, there are still significant hurdles when doing so, not the least of which is the energy radiating from the Sun simply vaporizing anything that gets close enough to utilize a gravity assist. That’s the problem a project supported by NASA’s Institute for Advanced Concepts (NIAC) and run by Jason Benkoski, now of Lawrence Livermore National Laboratory, is trying to solve.

The project was awarded a NIAC Phase I grant in 2022, focused on combining two separate systems – a heat shield and a thermal propellant system. According to the project’s final report, combining those two technologies could allow a spacecraft to perform what is known as an Oberth maneuver around the Sun. In this orbital mechanics trick, a spacecraft uses the Sun’s gravity well to slingshot itself at high speeds in the direction it aims. It’s similar to the Sundiver technology discussed in other articles.

So, what makes this project unique? One thing is the heat shield – Dr. Benkoski and his team developed a material that is capable of withstanding up to 2700 K. While that is still not anywhere near the temperature of the Sun’s surface, which can reach up to 5800 K, its enough to get pretty close, and thereby unlock a spacecraft’s ability to use an Oberth maneuver in the first place. 

Image of the test set-up for the thermal shield.
Credit – Benkoski et al.

Samples of the material with these thermal properties have already been produced. However, further research is needed to understand whether they’re cut out for space flight. And a heat shield alone isn’t enough to perform the maneuver – a spacecraft also must have a propulsion system that can withstand those temperatures. 

A solar thermal propulsion system could potentially do so. These systems use the Sun’s energy to pressurize their own propellant and then expel those propellants out to gain thrust, which is a necessary component of an Oberth maneuver. There are several different types of fuels that could work for such a system, and a large chunk of the research in the Phase I project looked at the different costs/benefits of each.

Hydrogen is one of the more common fuels considered for a solar thermal propulsion system. Though it is lightweight, it requires a bulky cryogenic system to store the hydrogen because it is heated to the point of being used as thrust. In the end, its trade-offs made it the least effective of the propellants considered during the project.

Graphic depicting the development path for the solar thermal propulsion system.
Credit – Benkoski et al.

Lithium hydride was the surprise winner for the fuel that allows for the fastest escape velocity. Calculations show it could result in a velocity of over 12 AU / yr. However, there are constraints with the fuel’s storage and handling.

Dr. Benkoski settled on a more mundane fuel as the overall winner of the modeling he did – methane. While it generally results in a slower final velocity than lithium hydride, its final speed is still respectable at over 10 AU / yr. It also eliminates many storage hassles of other propellants, such as the cryogenics required to store hydrogen.

There are some drawbacks, though – the calculated maximum speed is only about 1.7 times faster than what could already be done with a gravitational assist from Jupiter, which wouldn’t require all the fancy thermal shielding. There are other downsides to that, though, such as the direction the spacecraft can travel in being limited by where Jupiter is in relation to other objects of interest. Orbiting the Sun, on the other hand, it is possible to reach pretty much anywhere in the solar system and beyond with the right controlled burn.

As Dr. Benkoski notes in the final report, he made plenty of assumptions when doing his modeling calculations, including that the system would only be able to use already-developed technologies rather than speculative ones that could dramatically impact the results. For now, it doesn’t seem NASA has selected this project to move on to Phase II, and it’s unclear what future work is planned for further development. If nothing else, it is a step toward understanding what would be necessary to truly send spacecraft past the Sun and into deep space at a speed much faster than anything else has gone before. Given NASA’s continual attention to this topic, undoubtedly, someday, one of the missions will succeed in doing so.

Learn More:
Benkoski et al – Combined Heat Shield and Solar Thermal Propulsion System for an Oberth Maneuver
UT – Tiny Spacecraft Using Solar Sails Open Up a Solar System of Opportunity
UT – Want the Fastest Solar Sail? Drop it Into the Sun First
UT – A Mission to Reach the Solar Gravitational Lens in 30 Years

Lead Image:
Graphic of a solar thermal propulsion system undergoing a Oberth maneuver around the Sun.
Credit – Jason Benkoski

The post Slingshotting Around the Sun Would Make a Spacecraft the Faster Ever appeared first on Universe Today.

Reducing the size of the microphone in electronic devices would allow manufacturers to include more of them, increasing the capability for noise cancellation

Reducing the size of the microphone in electronic devices would allow manufacturers to include more of them, increasing the capability for noise cancellation

In its fourth episode, "The Acolyte" has a bigger sense of urgency, delivers a surprising Star Wars prequels cameo, and twists the plot once again.

Check out the new prologue video for the upcoming sci-fi RPG title, "Exodus."

4 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater) Danielle Koch, an aerospace engineer at NASA’s Glenn Research Center in Cleveland, was honored by the Girl Scouts of North East Ohio as a 2024 Woman of Distinction. She accepted the award during a ceremony on May 16. Credit: Girl Scouts of North East Ohio/Andrew Jordan

You’d think a NASA aerospace engineer who spends her days inside a giant dome researching how to make plane engines quieter and spacecraft systems more efficient would have a pretty booked schedule. Still, advocacy and mentoring, especially for women and girls in STEM, is something Danielle Koch always tries to say yes to.

For decades, Koch has tutored students, volunteered as a mentor for engineering challenges, and engaged Pre-K through Ph.D. classes with stories from her career at NASA’s Glenn Research Center in Cleveland. Koch also works to recruit women and others from underrepresented groups to the field and find ways to remove barriers to their advancement.

For her efforts, Koch was recently recognized by the Girl Scouts of North East Ohio as a 2024 Woman of Distinction. The award, presented to Koch during a ceremony on May 16, celebrates women whose leadership contributes to the community, providing girls with positive role models. Koch says that diverse people and programs have similarly shaped her own career path.

“None of this is anything I’ve done myself; there are huge groups of people who are making change and making things better for all of us,” Koch said. “Every story I tell about me being a woman at NASA is really a story about them.”

Danielle Koch (right) is an aerospace engineer in the Acoustics Branch at NASA’s Glenn Research Center in Cleveland, where she works to make flight quieter and spacecraft systems more efficient.Credit: NASA/Jef Janis

A Pittsburgh native and graduate of Case Western Reserve University, Koch began her career as a test engineer at NASA Glenn in 1990 as the only woman in her work group. While there were women around her, Koch says she did not see many senior-level female engineers or scientists “working ahead of her.” With determination and the “rock-solid” support of colleagues, family, and friends, Koch forged ahead, becoming a research aerospace engineer in NASA Glenn’s Acoustics Branch in 1998.

“She’s somebody that goes above and beyond almost all of the time, while using her knowledge and career to bring others up to her level,” said John Lucero, Koch’s supervisor and the chief of the Acoustics Branch at NASA Glenn.

Koch realized the landscape around her was evolving in 2016 when she sat down in one of NASA Glenn’s biggest conference rooms for the center’s annual Women Ignite workshop. It was the first time she’d seen the space entirely filled with women.

“It was striking,” Koch said. “Learning from each other and being visible to each other, it’s so huge.”

Koch points to insights gleaned from these workshops — which are focused on networking, skill-building, and empowerment — as propelling her forward, along with the center’s Women in STEM Leadership Development Program, launched to help the women of NASA Glenn connect and grow as leaders.

NASA Glenn Research Center aerospace engineer Danielle Koch gives a tour of the Aero-Acoustic Propulsion Laboratory to a group of students in 2017.Credit: NASA/Marvin Smith

Koch also spotlights the value of the Women at Glenn employee resource group, which organizes events and panels, shares job and volunteer opportunities, and provides a platform for addressing issues in the workplace.

“The employee resource group offers a great sense of community for women at the center,” said Women at Glenn co-chair and aerospace engineer Christine Pastor-Barsi. “When you feel like you’re unique, it’s good to know that there are others out there like you, even if you don’t always see them in the room.”

Koch says she’ll continue working as a mentor in the community and advocating for the diverse range of people who choose to take the leap into the STEM fields.

“It’s difficult to be the only one that’s visibly different in a room; it changes the way you communicate, the way you’re perceived,” Koch said. “It’s really important to reach out to people who are different from us and invite them to consider engineering as a career. We all benefit when we work with someone who’s different from ourselves.”

Get Involved + More Resources

• Learn about the Girls in STEM program at NASA Glenn, designed to inspire middle school students’ interest in STEM fields. The event features women working in STEM fields at NASA Glenn, an engaging STEM activity, and tours of NASA Glenn facilities.
• Continue celebrating International Women in Engineering Day with more inspiring stories of Women at NASA.
• Explore content from NASA’s observance of Women’s History Month.
• Discover how to engage with NASA experts.

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Supernova remnant 3C 58.X-ray: NASA/CXC/ICE-CSIC/A. Marino et al.; Optical: SDSS; Image Processing: NASA/CXC/SAO/J. Major

The supernova remnant 3C 58 contains a spinning neutron star, known as PSR J0205+6449, at its center. Astronomers studied this neutron star and others like it to probe the nature of matter inside these very dense objects. A new study, made using NASA’s Chandra X-ray Observatory and ESA’s XMM-Newton, reveals that the interiors of neutron stars may contain a type of ultra-dense matter not found anywhere else in the Universe.

In this image of 3C 58, low-energy X-rays are colored red, medium-energy X-rays are green, and the high-energy band of X-rays is shown in blue. The X-ray data have been combined with an optical image in yellow from the Digitized Sky Survey. The Chandra data show that the rapidly rotating neutron star (also known as a “pulsar”) at the center is surrounded by a torus of X-ray emission and a jet that extends for several light-years. The optical data shows stars in the field.

The team in this new study analyzed previously released data from neutron stars to determine the so-called equation of state. This refers to the basic properties of the neutron stars including the pressures and temperatures in different parts of their interiors.

The authors used machine learning, a type of artificial intelligence, to compare the data to different equations of state. Their results imply that a significant fraction of the equations of state — the ones that do not include the capability for rapid cooling at higher masses — can be ruled out.

The researchers capitalized on some neutron stars in the study being located in supernova remnants, including 3C 58. Since astronomers have age estimates of the supernova remnants, they also have the ages of the neutron stars that were created during the explosions that created both the remnants and the neutron stars. The astronomers found that the neutron star in 3C 58 and two others were much cooler than the rest of the neutron stars in the study.

The team thinks that part of the explanation for the rapid cooling is that these neutron stars are more massive than most of the rest. Because more massive neutron stars have more particles, special processes that cause neutron stars to cool more rapidly might be triggered.

One possibility for what is inside these neutron stars is a type of radioactive decay near their centers where neutrinos — low mass particles that easily travel through matter — carry away much of the energy and heat, causing rapid cooling.

Another possibility is that there are types of exotic matter found in the centers of these more rapidly cooling neutron stars.

The Nature Astronomy paper describing these results is available here. The authors of the paper are Alessio Marino (Institute of Space Sciences (ICE) in Barcelona, Spain), Clara Dehman (ICE), Konstantinos Kovlakas (ICE), Nanda Rea (ICE), J. A. Pons (University of Alicante in Spain), and Daniele Viganò (ICE).

NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science from Cambridge Massachusetts and flight operations from Burlington, Massachusetts.

Read more from NASA’s Chandra X-ray Observatory.

For more Chandra images, multimedia and related materials, visit:

https://www.nasa.gov/mission/chandra-x-ray-observatory/

Visual Description

This is an image of the leftovers from an exploded star called 3C 58, shown in X-ray and optical light. At the center of the remnant is a rapidly spinning neutron star, called a pulsar, that presents itself as a bright white object that’s somewhat elongated in shape.

Loops and swirls of material, in shades of blue and purple, extend outward from the neutron star in many directions, resembling the shape of an octopus and its arms.

Surrounding the octopus-like structure is a cloud of material in shades of red that is wider horizontally than it is vertically. A ribbon of purple material extends to the left edge of the red cloud, curling upward at its conclusion. Another purple ribbon extends to the right edge of the red cloud, though it is less defined than the one on the other side. Stars of many shapes and sizes dot the entire image.

News Media Contact

Megan Watzke
Chandra X-ray Center
Cambridge, Mass.
617-496-7998

Jonathan Deal
Marshall Space Flight Center
Huntsville, Ala.
256-544-0034

4 Min Read Next Generation NASA Technologies Tested in Flight Erin Rezich, Ian Haskin, QuynhGiao Nguyen, Jason Hill (Zero-G staff), and George Butt experience Lunar gravity while running test operations on the UBER payload. Credits: Zero-G

Teams of NASA researchers put their next-generation technologies to the microgravity test in a series of parabolic flights that aim to advance innovations supporting the agency’s space exploration goals.

These parabolic flights provide a gateway to weightlessness, allowing research teams to interact with their hardware in reduced gravity conditions for intervals of approximately 22 seconds. The flights, which ran from February to April, took place aboard Zero Gravity Corporation’s G-FORCE ONE aircraft and helped to advance several promising space technologies.

Under the Fundamental Regolith Properties, Handling, and Water Capture (FLEET) project, researchers tested an ultrasonic blade technology in a regolith simulant at lunar and Martian gravities. On Earth, vibratory tools reduce the forces between the tool and the soil, which also lowers the reaction forces experienced by the system. Such reductions indicate the potential for mass savings for tool systems used in space. 

This flight test aims to establish the magnitude of force reduction achieved by an ultrasonic tool on the Moon and Mars. Regolith interaction, including excavation, will be important to NASA’s resources to support long-duration lunar and Martian missions.

This experiment represents the success of an international effort three years in the making between NASA and Concordia University in Montreal, Quebec.

Erin Rezich

Project Principal Investigator

“This experiment represents the success of an international effort three years in the making between NASA and Concordia University in Montreal, Quebec. It was a NASA bucket list item for me to conduct a parabolic flight experiment, and it was even more special to do it for my doctoral thesis work. I’m very proud of my team and everyone’s effort to make this a reality,” said Erin Rezich, project principal investigator at NASA’s Glenn Research Center in Cleveland, Ohio. 

The FLEET project also has a separate payload planned for a future flight test on a suborbital rocket. The Vibratory Lunar Regolith Conveyor will demonstrate a granular material (regolith) transport system to study the vertical transport of lunar regolith simulants (soil) in a vacuum under a reduced gravity environment.

These two FLEET payloads increase the understanding of excavation behavior and how the excavated soil will be transported in a reduced gravity environment.

QuynhGiao Nguyen takes experiment notes while Pierre-Lucas Aubin-Fournier and George Butt oversee experiment operations during a soil reset period between parabolas.Zero-G 3D Printed Technologies Take on Microgravity 

Under the agency’s On-Demand Manufacturing of Electronics (ODME) project, researchers tested 3D printing technologies to ease the use of electronics and tools aboard the International Space Station.

Flying its first microgravity environment test, the ODME Advanced Toolplate team evaluated a new set of substantially smaller 3D printed tools that provide more capabilities and reduce tool changeouts. The toolplate offers eight swappable toolheads so that new technologies can be integrated after it is sent up to the space station. The 3D printer component enables in-space manufacturing of electronics and sensors for structural and crew-monitoring systems and multi-material 3D printing of metals.

“The development of these critical 3D printing technologies for microelectronics and semiconductors will advance the technology readiness of these processes and reduce the risk for planned future orbital demonstrations on the International Space Station.

curtis hill

ODME Project Principal Investigator

Left to Right: Pengyu Zhang, Rayne Wolfe, and Jacob Kocemba (University of Wisconsin at Madison) control the Electrohydrodynamic (EHD) ink jet printer testing manufacturing processes that are relevant to semiconductors for the NASA On Demand Manufacturing of Electronics (ODME) project.Zero-G

NASA researchers tested another 3D printing technology developed under the agency’s ODME project for manufacturing flexible electronics in space. The Space Enabled Advanced Devices and Semiconductors team is developing electrohydrodynamic inkjet printer technology for semiconductor device manufacturing aboard the space station. The printer will allow for printing electronics and semiconductors with a single development cartridge, which could be updated in the future for various materials systems.

(Left to right) Paul Deffenbaugh (Sciperio), Cadré Francis (NASA MSFC), Christopher Roberts (NASA MSFC), Connor Whitley (Sciperio), and Tanner Corby (Redwire Space Technologies) operate the On Demand Manufacturing of Electronics (ODME) Advanced Toolplate printer in zero gravity to demonstrate the potential capability of electronics manufacturing in space.Zero-G The On Demand Manufacturing of Electronics (ODME) Advanced Toolplate printer mills a Fused Deposition Modeling (FDM) printed plastic substrate surface smooth in preparation for the further printing of electronic traces. Conducting this study in zero gravity allowed for analysis of Foreign Object Debris (FOD) capture created during milling.Zero-G Left to Right: Rayne Wolfe and Jacob Kocemba (University of Wisconsin at Madison) control the Electrohydrodynamic (EHD) ink jet printer testing manufacturing processes that are relevant to semiconductors for the NASA On Demand Manufacturing of Electronics (ODME) project.Zero-G Left to Right: Pengyu Zhang, Rayne Wolfe, and Jacob Kocemba (University of Wisconsin at Madison) control the Electrohydrodynamic (EHD) ink jet printer testing manufacturing processes that are relevant to semiconductors for the NASA On Demand Manufacturing of Electronics (ODME) project.Zero-G

NASA’s Flight Opportunities program supported testing various technologies in a series of parabolic flights earlier this year. These technologies are managed under NASA’s Game Changing Development program within the Space Technology Mission Directorate. Space Enabled Advanced Devices and Semiconductors technology collaborators included Intel Corp., Tokyo Electron America, the University of Wisconsin-Madison, Arizona State University, and Iowa State University. The Space Operations Mission Directorate’s In-Space Production Applications also supports this technology. Advanced Toolplate Technology collaborated with Redwire and Sciperio. The Ultrasonic Blade technology is a partnership with NASA’s Glenn Research Center in Cleveland, Ohio, and Concordia University in Montreal, Quebec, through an International Space Act Agreement.

For more information about the Game Changing Development program, visit: nasa.gov/stmd-game-changing-development/

For more information about the Flight Opportunities program, visit: nasa.gov/stmd-flight-opportunities/ 

Testing In-Space Manufacturing Techs and More in Flight Facebook logo @NASATechnology @NASA_Technology Share

Details Last Updated Jun 20, 2024 EditorIvry Artis Related Terms

• Game Changing Development Program
• Flight Opportunities Program
• Space Technology Mission Directorate

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Researchers have confirmed a centuries-old rumour that leeches can jump, which they may do to land their next blood meal

Researchers have confirmed a centuries-old rumour that leeches can jump, which they may do to land their next blood meal

Prototype quantum photonic-dimer laser uses entanglement to bind photons and deliver a powerful beam of concentrated light that can shine through adverse weather like thick fog.

These cohousing communities are fighting an epidemic of loneliness with radical neighborliness.

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Preparations for Next Moonwalk Simulations Underway (and Underwater) Science in Space: June 2024

The Sun wields a huge influence on Earth. Its gravity holds our planet in its orbit, and solar energy drives the seasons, ocean currents, weather, climate, radiation belts, and auroras on Earth.

The solar wind, a flow of charged particles from the Sun, constantly bombards Earth’s magnetosphere, a vast magnetic shield around the planet. The Sun occasionally releases massive amounts of energy, creating solar geomagnetic storms that can interfere with communications and navigation and disrupt the electric power grid.

The colorful aurora borealis or Northern Lights and aurora australis or Southern Lights are created by the transfer of energy from solar electrons to molecules in Earth’s upper atmosphere. Those molecules then release that energy in the form of light. Different molecules create specific colors, such as green from oxygen.

Because Earth’s magnetic field directs solar electrons toward the poles, auroras typically are visible only at high latitudes, such as in Canada in the north and Australia in the south. But solar storms can send the lights into much lower latitudes. During a series of large solar eruptions in May 2024, for example, the display could be seen as far south as Texas and California.

Satellites captured auroras visible across the globe on May 11, 2024.NOAA

NASA has multiple missions studying how the Sun and solar storms affect Earth and space travel. The International Space Station contributes to this research in several ways. 

Improved Solar Energy Measurements

The station’s Total and Spectral Solar Irradiance Sensor (TSIS) measures solar irradiance, the solar energy Earth receives, and solar spectral irradiance, a measure of the Sun’s energy in individual wavelengths. Knowing the magnitude and variability of solar irradiance improves understanding of Earth’s climate, atmosphere, and oceans and enables more accurate predictions of space weather. Better predictions could in turn help protect humans and satellites in space and electric power transmission and radio communications on the ground. 

The first five years of TSIS observations demonstrated improved long-term spectral readings and lower uncertainties than measurements from a previous NASA mission, the Solar Radiation and Climate satellite. The accuracy of TSIS observations could improve models of solar irradiance variability and contribute to a long-term record of solar irradiance data. 

Earlier Sun Monitoring Installation of the Solar instruments on the space station during a spacewalk.NASA

The ESA (European Space Agency) Sun Monitoring on the External Payload Facility of Columbus, or Solar, collected data on solar energy output for more than a decade with three instruments covering most wavelengths of the electromagnetic spectrum. Different wavelengths emitted by the Sun are absorbed by and influence Earth’s atmosphere and contribute to our climate and weather. This monitoring helps scientists see how solar irradiance affects Earth and provides data to create models for predicting its influence. 

One instrument, the Solar Variable and Irradiance Monitor, covered the near-ultraviolet, visible, and thermal parts of the spectrum and helped improve the accuracy of these measurements.  

The SOLar SPECtral Irradiance Measurement instrument covered higher ranges of the solar spectrum. Its observations highlighted significant differences from previous solar reference spectra and models. Researchers also reported that repeated observations made it possible to determine a reference spectrum for the first year of the SOLAR mission, which corresponded to a solar minimum prior to Solar Cycle 24. 

Solar activity rises and falls over roughly 11-year cycles. The current Solar Cycle 25 began in December 2019, and scientists predicted a peak in solar activity between January and October of 2024, which included the May storms. 

The third instrument, SOLar Auto-Calibrating EUV/UV Spectrometers, measured the part of the solar spectrum between extreme ultraviolet and ultraviolet. Most of this highly energetic radiation is absorbed by the upper atmosphere, making it impossible to measure from the ground. Results suggested that these instruments could overcome the problem of degrading sensitivity seen with other solar measuring devices and provide more efficient data collection. 

Auroras from Space An aurora borealis display photographed from the International Space Station.NASA

Astronauts occasionally photograph the aurora borealis from the space station and post these images.  

For the CSA (Canadian Space Agency) AuroraMAX project, crew members photographed the aurora borealis over Yellowknife, Canada, between fall 2011 and late spring 2012. The space images, coordinated with a network of ground-based observatories across Canada, contributed to an interactive display at an art and science festival to inspire public interest in how solar activity affects Earth. The project also provides a live feed of the aurora borealis online every September through April.  

Student Satellites Deployment of the Miniature X-ray Solar Spectrometer and other CubeSats from the space station.NASA

The Miniature X-ray Solar Spectrometer CubeSat measured variation in solar X-ray activity to help scientists understand how it affects Earth’s upper atmosphere. Solar X-ray activity is enhanced during solar flares. Students at the University of Colorado Laboratory for Atmospheric Space Physics built the satellite, which deployed from the space station in early 2016. 

Better data help scientists understand how solar events affect satellites, crewed missions, and infrastructure in space and on the ground. Ongoing efforts to measure how Earth’s atmosphere responds to solar storms are an important part of NASA’s plans for Artemis missions to the Moon and for later missions to Mars. 

Melissa Gaskill 
International Space Station Research Communications Team 
NASA’s Johnson Space Center 

Search this database of scientific experiments to learn more about those mentioned above. 

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Latest News from Space Station Research

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Overview The Sun’s gravity holds the solar system together, keeping everything – from the biggest planets to the smallest particles…

NASA Heliophysics

Overview The Science Mission Directorate Heliophysics Division studies the nature of the Sun, and how it influences the very nature…

Station Science 101: Earth and Space Science

Video: 00:00:10

Summer officially begins in the Northern Hemisphere today 20 June, marking the longest day of the year. The summer solstice, which is when the Sun reaches the most northerly point in the sky, is set to occur tonight at 21:50 BST/22:50 CEST.

During the summer solstice, the Northern Hemisphere will experience the longest period of sunlight in a day or the longest day of the year. This is because of Earth’s position in orbit around the Sun and the way the North Pole is tilted towards the Sun during the solstice. 

The Sun’s rays hit the Northern Hemisphere at their most direct angle, resulting in the most extended period of daylight. Despite the long hours of daylight, it may not necessarily be the hottest day of the year. 

This animation shows one image per day captured by the Meteosat Second Generation from 20 June 2023 until 19 June 2024 captured at approximately 16:30 BST/17:30 CEST.

Access the related broadcast quality video material.

A new, official competition allows anyone to propose a mythology-based name for a "quasi-moon," an asteroid that orbits the Sun alongside Earth.

The post You Can Name a (Quasi) Moon! appeared first on Sky & Telescope.

The construction of the monument and another beside it more than 4,000 years ago corresponds to a time of bitter cold.

For the first time, a phenomenon astronomers have long hoped to image directly has been captured by the NASA/ESA/CSA James Webb Space Telescope’s Near-InfraRed Camera (NIRCam). In this stunning image of the Serpens Nebula, the discovery lies in the northern area of this young, nearby star-forming region.