Feed aggregator
LSAH Newsletter
1 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Reid Wiseman finds a little peace and quiet in the station’s Destiny lab.NASA
The Lifetime Surveillance of Astronaut Health (LSAH) program collects, analyzes, and interprets medical, physiological, hazard exposure, and environmental data for the purpose of maintaining astronaut health and safety as well as preventing occupationally induced injuries or disease related to space flight or space flight training. It allows NASA to effectively understand and mitigate the long-term health risks of human spaceflight, as well as support the physical and mental well-being of astronauts during future exploration missions.
The LSAH Newsletter serves to inform and update former astronauts on how their medical data is being utilized by the LSAH team. It is published and distributed bi-annually.
+ October 2025 | Vol 30 Issue 2 – LSAH Newsletter
+ Past LSAH Newsletters and Publications
TREAT Astronauts Act Share Details Last Updated Nov 25, 2025 EditorRobert E. LewisLocationJohnson Space Center Related Terms Explore More 9 min read Medical Examination Requirements (MER) for Former Astronauts Article 3 years ago 1 min read Historical Resources Article 3 years ago 1 min read March Updates for Interim Final Rule, NID, and TAAB Article 3 years ago Keep Exploring Discover More Topics From NASAHumans In Space
Missions
International Space Station
Solar System
LSAH Newsletter
1 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Reid Wiseman finds a little peace and quiet in the station’s Destiny lab.NASAThe Lifetime Surveillance of Astronaut Health (LSAH) program collects, analyzes, and interprets medical, physiological, hazard exposure, and environmental data for the purpose of maintaining astronaut health and safety as well as preventing occupationally induced injuries or disease related to space flight or space flight training. It allows NASA to effectively understand and mitigate the long-term health risks of human spaceflight, as well as support the physical and mental well-being of astronauts during future exploration missions.
The LSAH Newsletter serves to inform and update former astronauts on how their medical data is being utilized by the LSAH team. It is published and distributed bi-annually.
+ October 2025 | Vol 30 Issue 2 – LSAH Newsletter
+ Past LSAH Newsletters and Publications
TREAT Astronauts Act Share Details Last Updated Nov 25, 2025 EditorRobert E. LewisLocationJohnson Space Center Related Terms Explore More 9 min read Medical Examination Requirements (MER) for Former Astronauts Article 3 years ago 1 min read Historical Resources Article 3 years ago 1 min read March Updates for Interim Final Rule, NID, and TAAB Article 3 years ago Keep Exploring Discover More Topics From NASAHumans In Space
Missions
International Space Station
Solar System
NASA & GLOBE Connect People, Land, and Space
4 min read
NASA & GLOBE Connect People, Land, and Space The GLOBE Land Cover satellite comparison table is generated weekly for every GLOBE Land Cover observation. GLOBE volunteers receive an email with a link to the table. Information about the table may be found on the GLOBE Observer website.
A group of elementary-aged students gather outside of Oldham County Public Library in La Grange, Kentucky, United States to look at clouds in the sky. “If anyone asks what you are doing, tell them, ‘I am a citizen scientist and I am helping NASA,’” Children’s Programming Librarian, Cheri Grinnell, tells the kids. Grinnell supports an afterschool program called Leopard Spot where she engages K-5 students in collecting environmental data with the GLOBE (Global Learning & Observations to Benefit the Environment) Program.
“One little boy really got excited about that, and I heard him tell his mom he was working for NASA as they were leaving,” says Grinnell. That idea is reinforced when the program receives an email from NASA with satellite data that align with the cloud data the students submitted. “I forwarded the NASA satellite response to the after-school coordinator, and she read it to them. That really excited them because it was evidence this is the real deal.”
This experience is one the GLOBE Observer Team (part of the NASA Science Activation program’s NASA Earth Science Education Collaborative, NESEC) hears often: GLOBE volunteers of all ages love getting an email from NASA that compares satellite data with their cloud observations. “Feedback from NASA is huge. It’s the hook,” says Tina Rogerson, the programmer at NASA Langley Research Center who manages the satellite comparison emails. “It ties NASA science into what they saw when they did the observation.”
Now, volunteers will have more opportunities to receive a satellite comparison email from NASA. GLOBE recently announced that, in addition to sending emails about satellite data that align with the cloud observations made by learners, they will now also be sending emails that compare the GLOBE Observer Land Cover observations made by learners with satellite data. The new satellite comparison for land cover builds on the system used to create cloud comparisons at NASA Langley Research Center.
When a volunteer receives the email, they will see a link for each observation they have submitted. The link will open a website with a satellite comparison table. Their observation is at the top, followed by a satellite-based assessment of the land cover at that location. The last row of the table shows the most recent Landsat and Sentinel-2 satellite images of the observation site. Rogerson pulls GLOBE land cover data from the public GLOBE database to generate and send the comparison tables on a weekly basis. While users may opt out of receiving these emails, most participants will be excited to review their data from the space perspective.
These new collocated land cover observations are expected to raise greater awareness of how NASA and its interagency partners observe our changing home planet from space in order to inform societal needs. They will help every GLOBE volunteer see how their observations of the land fit in with the wider space-based view and how they are participating in the process of science. Based on the response to cloud satellite emails, seeing that bigger, impactful perspective via the satellite comparison email is motivating. The hope is to encourage volunteers to continue being NASA citizen scientists, collecting Earth system observations for GLOBE’s long-term environmental record.
“I’m excited that land cover is finally becoming part of the operational satellite comparison system,” says Rogerson. This means that GLOBE volunteers will routinely receive satellite data for both land cover and clouds. “We are bringing real science right into your world.”
NESEC, led by the Institute for Global Environmental Strategies (IGES) and supported by NASA under cooperative agreement award number NNX16AE28A, is part of NASA’s Science Activation Portfolio. Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn/about-science-activation/.
Share Details Last Updated Nov 25, 2025 Editor NASA Science Editorial Team Related Terms Explore More 3 min read New NASA HEAT and My NASA Data Resources Bring Space Weather Science into ClassroomsArticle
1 day ago
2 min read NASA Citizen Science Toolkit for Librarians
NASA’s Toolkit for Librarians can help you share NASA citizen science opportunities with your patrons…
Article
1 day ago
3 min read 10 Years of Students Helping NASA Grow Space Food with Growing Beyond Earth
Article
4 days ago
Keep Exploring Discover More Topics From NASA James Webb Space Telescope
Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
Perseverance Rover
This rover and its aerial sidekick were assigned to study the geology of Mars and seek signs of ancient microbial…
Parker Solar Probe
On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona…
Juno
NASA’s Juno spacecraft entered orbit around Jupiter in 2016, the first explorer to peer below the planet’s dense clouds to…
NASA & GLOBE Connect People, Land, and Space
4 min read
NASA & GLOBE Connect People, Land, and Space The GLOBE Land Cover satellite comparison table is generated weekly for every GLOBE Land Cover observation. GLOBE volunteers receive an email with a link to the table. Information about the table may be found on the GLOBE Observer website.A group of elementary-aged students gather outside of Oldham County Public Library in La Grange, Kentucky, United States to look at clouds in the sky. “If anyone asks what you are doing, tell them, ‘I am a citizen scientist and I am helping NASA,’” Children’s Programming Librarian, Cheri Grinnell, tells the kids. Grinnell supports an afterschool program called Leopard Spot where she engages K-5 students in collecting environmental data with the GLOBE (Global Learning & Observations to Benefit the Environment) Program.
“One little boy really got excited about that, and I heard him tell his mom he was working for NASA as they were leaving,” says Grinnell. That idea is reinforced when the program receives an email from NASA with satellite data that align with the cloud data the students submitted. “I forwarded the NASA satellite response to the after-school coordinator, and she read it to them. That really excited them because it was evidence this is the real deal.”
This experience is one the GLOBE Observer Team (part of the NASA Science Activation program’s NASA Earth Science Education Collaborative, NESEC) hears often: GLOBE volunteers of all ages love getting an email from NASA that compares satellite data with their cloud observations. “Feedback from NASA is huge. It’s the hook,” says Tina Rogerson, the programmer at NASA Langley Research Center who manages the satellite comparison emails. “It ties NASA science into what they saw when they did the observation.”
Now, volunteers will have more opportunities to receive a satellite comparison email from NASA. GLOBE recently announced that, in addition to sending emails about satellite data that align with the cloud observations made by learners, they will now also be sending emails that compare the GLOBE Observer Land Cover observations made by learners with satellite data. The new satellite comparison for land cover builds on the system used to create cloud comparisons at NASA Langley Research Center.
When a volunteer receives the email, they will see a link for each observation they have submitted. The link will open a website with a satellite comparison table. Their observation is at the top, followed by a satellite-based assessment of the land cover at that location. The last row of the table shows the most recent Landsat and Sentinel-2 satellite images of the observation site. Rogerson pulls GLOBE land cover data from the public GLOBE database to generate and send the comparison tables on a weekly basis. While users may opt out of receiving these emails, most participants will be excited to review their data from the space perspective.
These new collocated land cover observations are expected to raise greater awareness of how NASA and its interagency partners observe our changing home planet from space in order to inform societal needs. They will help every GLOBE volunteer see how their observations of the land fit in with the wider space-based view and how they are participating in the process of science. Based on the response to cloud satellite emails, seeing that bigger, impactful perspective via the satellite comparison email is motivating. The hope is to encourage volunteers to continue being NASA citizen scientists, collecting Earth system observations for GLOBE’s long-term environmental record.
“I’m excited that land cover is finally becoming part of the operational satellite comparison system,” says Rogerson. This means that GLOBE volunteers will routinely receive satellite data for both land cover and clouds. “We are bringing real science right into your world.”
NESEC, led by the Institute for Global Environmental Strategies (IGES) and supported by NASA under cooperative agreement award number NNX16AE28A, is part of NASA’s Science Activation Portfolio. Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn/about-science-activation/.
Share Details Last Updated Nov 25, 2025 Editor NASA Science Editorial Team Related Terms Explore More 3 min read New NASA HEAT and My NASA Data Resources Bring Space Weather Science into ClassroomsArticle
1 day ago
2 min read NASA Citizen Science Toolkit for Librarians
NASA’s Toolkit for Librarians can help you share NASA citizen science opportunities with your patrons…
Article
1 day ago
3 min read 10 Years of Students Helping NASA Grow Space Food with Growing Beyond Earth
Article
4 days ago
Keep Exploring Discover More Topics From NASA James Webb Space Telescope
Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
Perseverance Rover
This rover and its aerial sidekick were assigned to study the geology of Mars and seek signs of ancient microbial…
Parker Solar Probe
On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona…
Juno
NASA’s Juno spacecraft entered orbit around Jupiter in 2016, the first explorer to peer below the planet’s dense clouds to…
Skipping Meals before Thanksgiving Dinner Can Be Bad for Gut Health
Skipping meals before a big holiday feast probably isn’t the best idea for gut health, experts say. Here’s how to prevent overeating on an empty stomach—and tips for if you do
NASA’s Roman Observatory Passes Spate of Key Tests
NASA’s nearly complete Nancy Grace Roman Space Telescope has made another set of critical strides toward launch. This fall, the outer portion passed two tests — a shake test and an intense sound blast — to ensure its successful launch. The inner portion of the observatory underwent a major 65-day thermal vacuum test, showing that it will function properly in space. As NASA’s next flagship space telescope, Roman will address essential questions in the areas of dark energy, planets outside our solar system, and astrophysics.
The inner portion of NASA’s Nancy Grace Roman Space Telescope (which consists of the telescope, instrument carrier, two instruments, and spacecraft) recently passed thermal vacuum testing. In this photo, the assembly is being lifted out of the Space Environment Simulator after completing 65 days of assessments. Credit: NASA/Jolearra Tshiteya
“We want to make sure Roman will withstand our harshest environments,” said Rebecca Espina, a deputy test director at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “From a mechanical standpoint, our heaviest loads and stresses come from launch, so we use testing to mimic the launch environment.”
The vibration and acoustic testing were the final round of launch simulations for the outer portion of the Roman observatory, which consists of the outer barrel assembly, deployable aperture cover, and recently installed flight solar panels.
During acoustic testing, a large chamber with gigantic horns emulated the launch’s thunderous sounds, which cause high-frequency vibrations. Test operators outfitted the chamber and assembly with various sensors to monitor the hardware’s response to the sound, which gradually ramped up to a full minute at 138 decibels — louder than a jet plane’s takeoff at close range!
After moving to a massive shaker table, Roman’s outer assembly went through testing to replicate the rocket launch’s lower-frequency vibrations. Each individual test lasts only about a minute, sweeping from 5 to 50 hertz (the lowest note on a grand piano vibrates at 27.5 hertz), but NASA engineers tested three axes of movement over several weeks, breaking up the tests with on-the-spot data analysis.
Like in acoustic testing, the team installed sensors to capture the assembly’s response to the shaking. Structural analysts and test operators use this information not only to evaluate success but also to improve models and subsequent assessments.
“There’s a real sense of accomplishment when you get a piece of hardware this large through this test program,” said Shelly Conkey, lead structural analyst for this assembly at NASA Goddard. “I am proud of the work that our team of people has done.”
The outer portion of NASA’s Nancy Grace Roman Space Telescope (which consists of the outer barrel assembly, deployable aperture cover, and solar panels) recently passed vibration and acoustic testing. The structure is shown here in the acoustic testing chamber at NASA’s Goddard Space Flight Center in Greenbelt, Md., where it was blasted with intense sound to simulate launch conditions.Credit: NASA/Jolearra Tshiteya
The core portion of the observatory (the telescope, instrument carrier, two instruments, and spacecraft bus) moved into the Space Environment Simulator test chamber at NASA Goddard in August. There, it was subjected to extreme temperatures to mimic the chill of space and heat from the Sun. A team of more than 200 people ran simulations continuously for more than two months straight, assessing the telescope’s optics and the assembly’s overall mission readiness.
“The thermal vacuum test marked the first time the telescope and instruments were used together,” said Dominic Benford, Roman’s program scientist at NASA Headquarters in Washington. “The next time we turn everything on will be when the observatory is in space!”
Following extensive assessments, the core portion of NASA’s Nancy Grace Roman Space Telescope was removed from the test chamber (as shown in this gif) and returned to the largest clean room at NASA’s Goddard Space Flight Center in Greenbelt, Md. Next, it will be prepped for final integration.Credit: NASA/Sophia Roberts
The team expects to connect Roman’s two major parts in November, resulting in a complete observatory by the end of the year. Following final tests, Roman will move to the launch site at NASA’s Kennedy Space Center in Florida for launch preparations in summer 2026. Roman remains on schedule for launch by May 2027, with the team aiming for as early as fall 2026.
The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA’s Jet Propulsion Laboratory in Southern California; Caltech/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a science team comprising scientists from various research institutions. The primary industrial partners are BAE Systems Inc. in Boulder, Colorado; L3Harris Technologies in Rochester, New York; and Teledyne Scientific & Imaging in Thousand Oaks, California.
For more information about the Roman Space Telescope, visit:
By Laine Havens and Ashley Balzer
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Media contact:
Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, Md.
301-286-1940
NASA’s Roman Observatory Passes Spate of Key Tests
NASA’s nearly complete Nancy Grace Roman Space Telescope has made another set of critical strides toward launch. This fall, the outer portion passed two tests — a shake test and an intense sound blast — to ensure its successful launch. The inner portion of the observatory underwent a major 65-day thermal vacuum test, showing that it will function properly in space. As NASA’s next flagship space telescope, Roman will address essential questions in the areas of dark energy, planets outside our solar system, and astrophysics.
The inner portion of NASA’s Nancy Grace Roman Space Telescope (which consists of the telescope, instrument carrier, two instruments, and spacecraft) recently passed thermal vacuum testing. In this photo, the assembly is being lifted out of the Space Environment Simulator after completing 65 days of assessments. Credit: NASA/Jolearra Tshiteya“We want to make sure Roman will withstand our harshest environments,” said Rebecca Espina, a deputy test director at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “From a mechanical standpoint, our heaviest loads and stresses come from launch, so we use testing to mimic the launch environment.”
The vibration and acoustic testing were the final round of launch simulations for the outer portion of the Roman observatory, which consists of the outer barrel assembly, deployable aperture cover, and recently installed flight solar panels.
During acoustic testing, a large chamber with gigantic horns emulated the launch’s thunderous sounds, which cause high-frequency vibrations. Test operators outfitted the chamber and assembly with various sensors to monitor the hardware’s response to the sound, which gradually ramped up to a full minute at 138 decibels — louder than a jet plane’s takeoff at close range!
After moving to a massive shaker table, Roman’s outer assembly went through testing to replicate the rocket launch’s lower-frequency vibrations. Each individual test lasts only about a minute, sweeping from 5 to 50 hertz (the lowest note on a grand piano vibrates at 27.5 hertz), but NASA engineers tested three axes of movement over several weeks, breaking up the tests with on-the-spot data analysis.
Like in acoustic testing, the team installed sensors to capture the assembly’s response to the shaking. Structural analysts and test operators use this information not only to evaluate success but also to improve models and subsequent assessments.
“There’s a real sense of accomplishment when you get a piece of hardware this large through this test program,” said Shelly Conkey, lead structural analyst for this assembly at NASA Goddard. “I am proud of the work that our team of people has done.”
The outer portion of NASA’s Nancy Grace Roman Space Telescope (which consists of the outer barrel assembly, deployable aperture cover, and solar panels) recently passed vibration and acoustic testing. The structure is shown here in the acoustic testing chamber at NASA’s Goddard Space Flight Center in Greenbelt, Md., where it was blasted with intense sound to simulate launch conditions.Credit: NASA/Jolearra TshiteyaThe core portion of the observatory (the telescope, instrument carrier, two instruments, and spacecraft bus) moved into the Space Environment Simulator test chamber at NASA Goddard in August. There, it was subjected to extreme temperatures to mimic the chill of space and heat from the Sun. A team of more than 200 people ran simulations continuously for more than two months straight, assessing the telescope’s optics and the assembly’s overall mission readiness.
“The thermal vacuum test marked the first time the telescope and instruments were used together,” said Dominic Benford, Roman’s program scientist at NASA Headquarters in Washington. “The next time we turn everything on will be when the observatory is in space!”
Following extensive assessments, the core portion of NASA’s Nancy Grace Roman Space Telescope was removed from the test chamber (as shown in this gif) and returned to the largest clean room at NASA’s Goddard Space Flight Center in Greenbelt, Md. Next, it will be prepped for final integration.Credit: NASA/Sophia RobertsThe team expects to connect Roman’s two major parts in November, resulting in a complete observatory by the end of the year. Following final tests, Roman will move to the launch site at NASA’s Kennedy Space Center in Florida for launch preparations in summer 2026. Roman remains on schedule for launch by May 2027, with the team aiming for as early as fall 2026.
The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA’s Jet Propulsion Laboratory in Southern California; Caltech/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a science team comprising scientists from various research institutions. The primary industrial partners are BAE Systems Inc. in Boulder, Colorado; L3Harris Technologies in Rochester, New York; and Teledyne Scientific & Imaging in Thousand Oaks, California.
For more information about the Roman Space Telescope, visit:
By Laine Havens and Ashley Balzer
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Media contact:
Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, Md.
301-286-1940
We may need a fourth law of thermodynamics for living systems
We may need a fourth law of thermodynamics for living systems
Trump Orders Genesis Mission to Advance AI Breakthroughs
A new federal initiative aims to accelerate scientific discovery by uniting artificial intelligence with large federal datasets
Red Spider Nebula
Red Spider Nebula
Using its Near-InfraRed Camera (NIRCam), NASA’s James Webb Space Telescope captured never-before-seen details of the Red Spider Nebula, a planetary nebula, in this image released on Oct. 26, 2025. NIRCam is Webb’s primary near-infrared imager, providing high-resolution imaging and spectroscopy for a wide variety of investigations.
Webb’s new view of the Red Spider Nebula reveals for the first time the full extent of the nebula’s outstretched lobes, which form the ‘legs’ of the spider. These lobes, shown in blue, are traced by light emitted from H2 molecules, which contain two hydrogen atoms bonded together. Stretching over the entirety of NIRCam’s field of view, these lobes are shown to be closed, bubble-like structures that each extend about 3 light-years. Outflowing gas from the center of the nebula has inflated these massive bubbles over thousands of years.
Image credit: ESA/Webb, NASA & CSA, J. H. Kastner (Rochester Institute of Technology)
Red Spider Nebula
Using its Near-InfraRed Camera (NIRCam), NASA’s James Webb Space Telescope captured never-before-seen details of the Red Spider Nebula, a planetary nebula, in this image released on Oct. 26, 2025. NIRCam is Webb’s primary near-infrared imager, providing high-resolution imaging and spectroscopy for a wide variety of investigations.
Webb’s new view of the Red Spider Nebula reveals for the first time the full extent of the nebula’s outstretched lobes, which form the ‘legs’ of the spider. These lobes, shown in blue, are traced by light emitted from H2 molecules, which contain two hydrogen atoms bonded together. Stretching over the entirety of NIRCam’s field of view, these lobes are shown to be closed, bubble-like structures that each extend about 3 light-years. Outflowing gas from the center of the nebula has inflated these massive bubbles over thousands of years.
Image credit: ESA/Webb, NASA & CSA, J. H. Kastner (Rochester Institute of Technology)
NASA Crater Detection Challenge
Crater rims are vital landmarks for planetary science and navigation. Yet detecting them in real imagery is tough, with shadows, lighting shifts, and broken edges obscuring their shape.
This project invites you to develop methods that can reliably fit ellipses to crater rims, helping advance future space exploration.
In the pursuit of next generation, terrain-based optical navigation, NASA is developing a system that will use a visible-light camera on a spacecraft to capture orbital images of lunar terrain and process the imagery to:
- detect the crater rims in the images,
- identify the craters from a catalog, and
- estimate the camera/vehicle position based on the identified craters.
The focus of this project is the crater detection process.
Natural imagery varies significantly in lighting and will impact the completeness of crater rims in the images.
Award: $55,000 in total prizes
Open Date: November 25, 2025
Close Date: January 19, 2026
For more information, visit: https://www.topcoder.com/nasa-crater-detection
NASA Crater Detection Challenge
Crater rims are vital landmarks for planetary science and navigation. Yet detecting them in real imagery is tough, with shadows, lighting shifts, and broken edges obscuring their shape.
This project invites you to develop methods that can reliably fit ellipses to crater rims, helping advance future space exploration.
In the pursuit of next generation, terrain-based optical navigation, NASA is developing a system that will use a visible-light camera on a spacecraft to capture orbital images of lunar terrain and process the imagery to:
- detect the crater rims in the images,
- identify the craters from a catalog, and
- estimate the camera/vehicle position based on the identified craters.
The focus of this project is the crater detection process.
Natural imagery varies significantly in lighting and will impact the completeness of crater rims in the images.
Award: $55,000 in total prizes
Open Date: November 25, 2025
Close Date: January 19, 2026
For more information, visit: https://www.topcoder.com/nasa-crater-detection
CHAPEA Crew Begins Stay Inside NASA’s Mars Habitat for Second Mission
A crew of four research volunteers stepped inside NASA’s CHAPEA (Crew Health and Performance Exploration Analog) habitat on Oct. 19, marking the start of the agency’s second 378-day simulated Mars mission.
Ross Elder, Ellen Ellis, Matthew Montgomery, and James Spicer are living and working inside the roughly 1,700-square-foot 3D-printed habitat at the agency’s Johnson Space Center in Houston until Oct. 31, 2026.
“The information and lessons learned through CHAPEA will inform real-life mission planning, vehicle and surface habitat designs, and other resources NASA needs to support crew health and performance as we venture beyond low-Earth orbit,” said Sara Whiting, Human Research Program project scientist. “Through these lessons, NASA’s Human Research Program is reducing human health and performance risks of spaceflight to enable safe and successful crewed missions to the Moon, Mars, and beyond.”
The crew will face the challenges of a real Mars mission, and only leave to perform simulated “Marswalk” activities directly outside the habitat, wearing spacesuits, to traverse a simulated Mars environment filled with red sand. During these Marswalks, they will remain isolated within the building that houses CHAPEA at NASA Johnson.
“These crewmembers will help provide foundational data for mission planning and vehicle design and inform trades between resources, methods, and technologies that best support health and performance within the constraints of living on Mars,” said Grace Douglas, CHAPEA principal investigator. “The information gained from these simulated missions is critical to NASA’s goal of sending astronauts to explore Mars.”
During the year ahead, the crew will complete a variety of activities designed to replicate life and work on a long-duration mission on Mars, including high-tempo simulated Marswalks, robotic operations, habitat maintenance, physical exercise, and crop cultivation. The mission also aims to investigate how the crew adapts and responds to various environmental stressors that may arise during a real Martian mission, including limited access to resources, prolonged isolation, 22-minute communication delays, and equipment failures. Researchers will study how the team manages these conditions, which will inform future protocols and plans ahead of future crewed missions to Mars.
The first CHAPEA mission, which took place in the same habitat, concluded on July 6, 2024.
The CHAPEA mission 2 main crew and two alternate crew members are pictured in front of the Space Exploration Vehicle, the prototype pressurized rover that transported crew members to the habitat at the start of the mission. Credits: NASA/James Blair Ross Elder, CHAPEA mission 2 commander, waves to agency leaders and staff who are supporting the mission before he steps into the habitat. Credits: NASA/James Blair Suzanne Bell, CHAPEA Mission 2 Co-Principal Investigator, offers remarks to crew members Matthew Montgomery, James Spicer, Ross Elder, and Ellen Ellis directly before they enter the habitat for the 378-day mission. Credits: NASA/James Blair____
NASA’s Human Research Program
NASA’s Human Research Program pursues methods and technologies to support safe, productive human space travel. Through science conducted in laboratories, ground-based analogs, commercial missions, the International Space Station and Artemis missions, the program scrutinizes how spaceflight affects human bodies and behaviors. Such research drives the program’s quest to innovate ways that keep astronauts healthy and mission ready as human space exploration expands to the Moon, Mars, and beyond.
Explore More 5 min read NASA’s 2025 Astronaut Candidates: Shaping Artemis Exploration Article 6 days ago 4 min read The Overview Effect: Astronaut Perspectives from 25 Years in Low Earth Orbit Article 1 week ago 8 min read 25 Years of Scientific Discovery Aboard the International Space Station Article 1 week ago Keep Exploring Discover More Topics From NASALiving in Space
Artemis
Human Research Program
Space Station Research and Technology
CHAPEA Crew Begins Stay Inside NASA’s Mars Habitat for Second Mission
A crew of four research volunteers stepped inside NASA’s CHAPEA (Crew Health and Performance Exploration Analog) habitat on Oct. 19, marking the start of the agency’s second 378-day simulated Mars mission.
Ross Elder, Ellen Ellis, Matthew Montgomery, and James Spicer are living and working inside the roughly 1,700-square-foot 3D-printed habitat at the agency’s Johnson Space Center in Houston until Oct. 31, 2026.
“The information and lessons learned through CHAPEA will inform real-life mission planning, vehicle and surface habitat designs, and other resources NASA needs to support crew health and performance as we venture beyond low-Earth orbit,” said Sara Whiting, Human Research Program project scientist. “Through these lessons, NASA’s Human Research Program is reducing human health and performance risks of spaceflight to enable safe and successful crewed missions to the Moon, Mars, and beyond.”
The crew will face the challenges of a real Mars mission, and only leave to perform simulated “Marswalk” activities directly outside the habitat, wearing spacesuits, to traverse a simulated Mars environment filled with red sand. During these Marswalks, they will remain isolated within the building that houses CHAPEA at NASA Johnson.
“These crewmembers will help provide foundational data for mission planning and vehicle design and inform trades between resources, methods, and technologies that best support health and performance within the constraints of living on Mars,” said Grace Douglas, CHAPEA principal investigator. “The information gained from these simulated missions is critical to NASA’s goal of sending astronauts to explore Mars.”
During the year ahead, the crew will complete a variety of activities designed to replicate life and work on a long-duration mission on Mars, including high-tempo simulated Marswalks, robotic operations, habitat maintenance, physical exercise, and crop cultivation. The mission also aims to investigate how the crew adapts and responds to various environmental stressors that may arise during a real Martian mission, including limited access to resources, prolonged isolation, 22-minute communication delays, and equipment failures. Researchers will study how the team manages these conditions, which will inform future protocols and plans ahead of future crewed missions to Mars.
The first CHAPEA mission, which took place in the same habitat, concluded on July 6, 2024.
The CHAPEA mission 2 main crew and two alternate crew members are pictured in front of the Space Exploration Vehicle, the prototype pressurized rover that transported crew members to the habitat at the start of the mission. Credits: NASA/James Blair Ross Elder, CHAPEA mission 2 commander, waves to agency leaders and staff who are supporting the mission before he steps into the habitat. Credits: NASA/James Blair Suzanne Bell, CHAPEA Mission 2 Co-Principal Investigator, offers remarks to crew members Matthew Montgomery, James Spicer, Ross Elder, and Ellen Ellis directly before they enter the habitat for the 378-day mission. Credits: NASA/James Blair____
NASA’s Human Research Program
NASA’s Human Research Program pursues methods and technologies to support safe, productive human space travel. Through science conducted in laboratories, ground-based analogs, commercial missions, the International Space Station and Artemis missions, the program scrutinizes how spaceflight affects human bodies and behaviors. Such research drives the program’s quest to innovate ways that keep astronauts healthy and mission ready as human space exploration expands to the Moon, Mars, and beyond.
Explore More 5 min read NASA’s 2025 Astronaut Candidates: Shaping Artemis Exploration Article 4 days ago 4 min read The Overview Effect: Astronaut Perspectives from 25 Years in Low Earth Orbit Article 5 days ago 8 min read 25 Years of Scientific Discovery Aboard the International Space Station Article 1 week ago Keep Exploring Discover More Topics From NASALiving in Space
Artemis
Human Research Program
Space Station Research and Technology
NASA Orbiter Shines New Light on Long-Running Martian Mystery
5 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) The European Space Agency’s Mars Express orbiter captured this view of Mars’ south polar ice cap Feb. 25, 2015. Three years later, the spacecraft detected a signal from the area to the right of the ice cap that scientists interpreted as an underground lake.ESA/DLR/FU Berlin, CC BY-SA 3.0 IGO
Results from an enhanced radar technique have demonstrated improvement to sub-surface observations of Mars.
NASA’s Mars Reconnaissance Orbiter (MRO) has revisited and raised new questions about a mysterious feature buried beneath thousands of feet of ice at the Red Planet’s south pole. In a recent study, researchers conclude from data obtained using an innovative radar technique that an area on Mars suspected of being an underground lake is more likely to be a layer of rock and dust.
The 2018 discovery of the suspected lake set off a flurry of scientific activity, as water is closely linked with life in the solar system. While the latest findings indicate this feature is not a lake below the Martian surface, it does suggest that the same radar technique could be used to check for subsurface resources elsewhere on Mars, supporting future explorers.
The paper, published in Geophysical Research Letters on Nov. 17, was led by two of MRO’s Shallow Radar (SHARAD) instrument scientists, Gareth Morgan and Than Putzig, who are based at the Planetary Science Institute in Tucson, Arizona, and Lakewood, Colorado, respectively.
The observations were made by MRO with a special maneuver that rolls the spacecraft 120 degrees. Doing so enhances the power of SHARAD, enabling the radar’s signal to penetrate deeper underground and provide a clearer image of the subsurface. These “very large rolls” have proved so effective that scientists are eager to use them at previously observed sites where buried ice might exist.
This map shows the approximate area where in 2018 ESA’s Mars Express detected a signal the mission’s scientists interpreted as an underground lake. The red lines show the path of NASA’s Mars Reconnaissance Orbiter, which flew both directly overhead as well as over an adjacent region. Credit: Planetary Science Institute
Morgan, Putzig, and fellow SHARAD team members had made multiple unsuccessful attempts to observe the area suspected of hosting a buried lake. Then the scientists partnered with the spacecraft’s operations team at NASA’s Jet Propulsion Laboratory in Southern California, which leads the mission, to develop the very large roll capability.
Because the radar’s antenna is at the back of MRO, the orbiter’s body obstructs its view and weakens the instrument’s sensitivity. After considerable work, engineers at JPL and Lockheed Martin Space in Littleton, Colorado, which built the spacecraft and supports its operations, developed commands for a 120-degree roll — a technique that requires careful planning to keep the spacecraft safe — to direct more of SHARAD’s signal at the surface.
Bright signalOn May 26, SHARAD performed a very large roll to finally pick up the signal in the target area, which spans about 12.5 miles (20 kilometers) and is buried under a slab of water ice almost 1 mile (1,500 meters) thick.
When a radar signal bounces off underground layers, the strength of its reflection depends on what the subsurface is made of. Most materials let the signal slip through or absorb it, making the return faint. Liquid water is special in that it produces a very reflective surface, sending back a very strong signal (imagine pointing a flashlight at a mirror).
That’s the kind of signal that was spotted from this area in 2018 by a team working with the Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) instrument aboard the ESA (European Space Agency) Mars Express orbiter. To explain how such a body of water could remain liquid under all that ice, scientists have hypothesized it could be a briny lake, since high salt content can lower water’s freezing temperature.
An antenna sticks out like whiskers from NASA’s Mars Reconnaissance Orbiter in this artist’s concept depicting the spacecraft, which has been orbiting the Red Planet since 2006. This antenna is part of SHARAD, a radar that peers below the Martian surface.NASA/JPL-Caltech
“We’ve been observing this area with SHARAD for almost 20 years without seeing anything from those depths,” said Putzig. But once MRO achieved a very large roll over the precise area, the team was able to look much deeper. And rather than the bright signal MARSIS received, SHARAD detected a faint one. A different very-large-roll observation of an adjacent area didn’t detect a signal at all, suggesting something unique is causing a quirky radar signal at the exact spot MARSIS saw a signal.
“The lake hypothesis generated lots of creative work, which is exactly what exciting scientific discoveries are supposed to do,” said Morgan. “And while this new data won’t settle the debate, it makes it very hard to support the idea of a liquid water lake.”
Alternative explanationsMars’ south pole has an ice cap sitting atop heavily cratered terrain, and most radar images of the area below the ice show lots of peaks and valleys. Morgan and Putzig said it’s possible that the bright signal MARSIS detected here may just be a rare smooth area — an ancient lava flow, for example.
Both scientists are excited to use the very large roll technique to reexamine other scientifically interesting regions of Mars. One such place is Medusae Fossae, a sprawling geologic formation on Mars’ equator that produces little radar return. While some scientists have suggested it’s composed of layers of volcanic ash, others have suggested the layers may include heaps of ice deep within.
“If it’s ice, that means there’s lots of water resources near the Martian equator, where you’d want to send humans,” said Putzig. “Because the equator is exposed to more sunlight, it’s warmer and ideal for astronauts to live and work.”
More about MRONASA’s Jet Propulsion Laboratory in Southern California manages MRO for the agency’s Science Mission Directorate in Washington as part of NASA’s Mars Exploration Program portfolio. Lockheed Martin Space in Denver built MRO and supports its operations. SHARAD was provided to the MRO mission by the Italian Space Agency (ASI).
News Media Contacts
Andrew Good
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-2433
andrew.c.good@jpl.nasa.gov
Karen Fox / Molly Wasser
NASA Headquarters, Washington
202-358-1600
karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov
2025-130
Share Details Last Updated Nov 25, 2025 Related Terms Explore More 6 min read NASA’s Mars Spacecraft Capture Images of Comet 3I/ATLAS Article 1 week ago 3 min read View Interstellar Comet 3I/ATLAS Through NASA’s Multiple LensesThis article was updated to include the full range of dates from the SOHO image.…
Article 1 week ago 4 min read What Would It Take to Say We Found Life? We Asked a NASA Expert: Episode 63 Article 3 months ago Keep Exploring Discover Related Topics Mars ExplorationMars is the only planet we know of inhabited entirely by robots. Learn more about the Mars Missions.
Mars Reconnaissance OrbiterNASA’s Mars Reconnaissance Orbiter (MRO) is the second longest-lived spacecraft to orbit Mars, after 2001 Mars Odyssey.
MRO ScienceOverview Among other ongoing achievements, data collected by Mars Reconnaissance Orbiter continues to help Mars scientists and engineers characterize potential…
Mars ExpressNASA Participation In partnership with their European colleagues, U.S. scientists are participating in the scientific instrument teams of the Mars…
NASA Orbiter Shines New Light on Long-Running Martian Mystery
5 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) The European Space Agency’s Mars Express orbiter captured this view of Mars’ south polar ice cap Feb. 25, 2015. Three years later, the spacecraft detected a signal from the area to the right of the ice cap that scientists interpreted as an underground lake.ESA/DLR/FU Berlin, CC BY-SA 3.0 IGOResults from an enhanced radar technique have demonstrated improvement to sub-surface observations of Mars.
NASA’s Mars Reconnaissance Orbiter (MRO) has revisited and raised new questions about a mysterious feature buried beneath thousands of feet of ice at the Red Planet’s south pole. In a recent study, researchers conclude from data obtained using an innovative radar technique that an area on Mars suspected of being an underground lake is more likely to be a layer of rock and dust.
The 2018 discovery of the suspected lake set off a flurry of scientific activity, as water is closely linked with life in the solar system. While the latest findings indicate this feature is not a lake below the Martian surface, it does suggest that the same radar technique could be used to check for subsurface resources elsewhere on Mars, supporting future explorers.
The paper, published in Geophysical Research Letters on Nov. 17, was led by two of MRO’s Shallow Radar (SHARAD) instrument scientists, Gareth Morgan and Than Putzig, who are based at the Planetary Science Institute in Tucson, Arizona, and Lakewood, Colorado, respectively.
The observations were made by MRO with a special maneuver that rolls the spacecraft 120 degrees. Doing so enhances the power of SHARAD, enabling the radar’s signal to penetrate deeper underground and provide a clearer image of the subsurface. These “very large rolls” have proved so effective that scientists are eager to use them at previously observed sites where buried ice might exist.
This map shows the approximate area where in 2018 ESA’s Mars Express detected a signal the mission’s scientists interpreted as an underground lake. The red lines show the path of NASA’s Mars Reconnaissance Orbiter, which flew both directly overhead as well as over an adjacent region. Credit: Planetary Science InstituteMorgan, Putzig, and fellow SHARAD team members had made multiple unsuccessful attempts to observe the area suspected of hosting a buried lake. Then the scientists partnered with the spacecraft’s operations team at NASA’s Jet Propulsion Laboratory in Southern California, which leads the mission, to develop the very large roll capability.
Because the radar’s antenna is at the back of MRO, the orbiter’s body obstructs its view and weakens the instrument’s sensitivity. After considerable work, engineers at JPL and Lockheed Martin Space in Littleton, Colorado, which built the spacecraft and supports its operations, developed commands for a 120-degree roll — a technique that requires careful planning to keep the spacecraft safe — to direct more of SHARAD’s signal at the surface.
Bright signalOn May 26, SHARAD performed a very large roll to finally pick up the signal in the target area, which spans about 12.5 miles (20 kilometers) and is buried under a slab of water ice almost 1 mile (1,500 meters) thick.
When a radar signal bounces off underground layers, the strength of its reflection depends on what the subsurface is made of. Most materials let the signal slip through or absorb it, making the return faint. Liquid water is special in that it produces a very reflective surface, sending back a very strong signal (imagine pointing a flashlight at a mirror).
That’s the kind of signal that was spotted from this area in 2018 by a team working with the Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) instrument aboard the ESA (European Space Agency) Mars Express orbiter. To explain how such a body of water could remain liquid under all that ice, scientists have hypothesized it could be a briny lake, since high salt content can lower water’s freezing temperature.
An antenna sticks out like whiskers from NASA’s Mars Reconnaissance Orbiter in this artist’s concept depicting the spacecraft, which has been orbiting the Red Planet since 2006. This antenna is part of SHARAD, a radar that peers below the Martian surface.NASA/JPL-Caltech“We’ve been observing this area with SHARAD for almost 20 years without seeing anything from those depths,” said Putzig. But once MRO achieved a very large roll over the precise area, the team was able to look much deeper. And rather than the bright signal MARSIS received, SHARAD detected a faint one. A different very-large-roll observation of an adjacent area didn’t detect a signal at all, suggesting something unique is causing a quirky radar signal at the exact spot MARSIS saw a signal.
“The lake hypothesis generated lots of creative work, which is exactly what exciting scientific discoveries are supposed to do,” said Morgan. “And while this new data won’t settle the debate, it makes it very hard to support the idea of a liquid water lake.”
Alternative explanationsMars’ south pole has an ice cap sitting atop heavily cratered terrain, and most radar images of the area below the ice show lots of peaks and valleys. Morgan and Putzig said it’s possible that the bright signal MARSIS detected here may just be a rare smooth area — an ancient lava flow, for example.
Both scientists are excited to use the very large roll technique to reexamine other scientifically interesting regions of Mars. One such place is Medusae Fossae, a sprawling geologic formation on Mars’ equator that produces little radar return. While some scientists have suggested it’s composed of layers of volcanic ash, others have suggested the layers may include heaps of ice deep within.
“If it’s ice, that means there’s lots of water resources near the Martian equator, where you’d want to send humans,” said Putzig. “Because the equator is exposed to more sunlight, it’s warmer and ideal for astronauts to live and work.”
More about MRONASA’s Jet Propulsion Laboratory in Southern California manages MRO for the agency’s Science Mission Directorate in Washington as part of NASA’s Mars Exploration Program portfolio. Lockheed Martin Space in Denver built MRO and supports its operations. SHARAD was provided to the MRO mission by the Italian Space Agency (ASI).
News Media Contacts
Andrew Good
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-2433
andrew.c.good@jpl.nasa.gov
Karen Fox / Molly Wasser
NASA Headquarters, Washington
202-358-1600
karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov
2025-130
Share Details Last Updated Nov 25, 2025 Related Terms Explore More 6 min read NASA’s Mars Spacecraft Capture Images of Comet 3I/ATLAS Article 1 week ago 3 min read View Interstellar Comet 3I/ATLAS Through NASA’s Multiple LensesThis article was updated to include the full range of dates from the SOHO image.…
Article 1 week ago 4 min read What Would It Take to Say We Found Life? We Asked a NASA Expert: Episode 63 Article 3 months ago Keep Exploring Discover Related Topics Mars ExplorationMars is the only planet we know of inhabited entirely by robots. Learn more about the Mars Missions.
Mars Reconnaissance OrbiterNASA’s Mars Reconnaissance Orbiter (MRO) is the second longest-lived spacecraft to orbit Mars, after 2001 Mars Odyssey.
MRO ScienceOverview Among other ongoing achievements, data collected by Mars Reconnaissance Orbiter continues to help Mars scientists and engineers characterize potential…
Mars ExpressNASA Participation In partnership with their European colleagues, U.S. scientists are participating in the scientific instrument teams of the Mars…
Scientists Identify Five Distinct Eras of Human Brain Aging
Human brains go through five distinct phases of life, each defined by its own set of characteristics, according to a new study