NASA’s New Astronaut Candidates

NASA’s New Astronaut Candidates

Ten people in blue jumpsuits link arms. The two women on either end wave at the audience, who is not visible.
NASA/James Blair

NASA’s 2025 astronaut candidate class greets the crowd in this Sept. 22, 2025, image. The group was introduced Monday following a competitive selection process of more than 8,000 applicants from across the United States. The class now will complete nearly two years of training before becoming eligible for flight assignments supporting future science and exploration missions to low Earth orbit, the Moon, and Mars.

After graduation, the 2025 class will join the agency’s active astronaut corps. Active astronauts are conducting science research aboard the space station while preparing for the transition to commercial space stations and the next great leaps in human exploration at the Moon and Mars. The candidates’ operational expertise, scientific knowledge, and technical backgrounds are essential to advancing NASA’s deep space exploration goals and sustaining a long-term human presence beyond low Earth orbit.

Image credit: NASA/James Blair

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Jessica Taveau

The Need to Bake Out Silicone Based Thermal Control Coatings

The Need to Bake Out Silicone Based Thermal Control Coatings

Background
The NASA Engineering and Safety Center (NESC) has reviewed flight, ground test, and published data on ultraviolet-induced degradation of silicone based thermal control coatings. Analysis has shown, for at least one silicone coating, that bake-out plays an important role in ultraviolet (UV) degradation, indicating that UV interaction with paint volatiles, and not the structural material, is the primary source of coating discoloration.

Discussion
Spacecraft temperature is primarily determined by the absorptivity and emissivity of the vehicle’s coating. Absorptivity is the fraction of the sun’s irradiance that is absorbed, and emissivity determines the amount of infrared power that is emitted. The combination of these properties, along with additional heat from internal sources and other external radiation sources, determines the spacecraft’s thermal environment. Choosing an appropriate coating, referred to as a thermal control coating, is key to keeping the vehicle within a desired temperature range. However, these coatings can degrade, (i.e., darken), in low earth orbit (LEO), primarily due to solar UV exposure, complicating the choice of coating. Zinc-oxide (ZnO) scatterers in a silicate binder are among the most stable white coatings but suffer from poor adherence. Replacing the silicate with organic silicone improves paint mechanical properties, but optical property measurements of UV exposure stability for ZnO-silicone coatings have been widely divergent. This led to a request that the NESC resolve the variations to better predict the stability of specific ZnO-silicone coatings in LEO. Testing of coupons began in FY25 and will complete in FY26.

Many silicone-based thermal control coatings have been evaluated in ground simulation chambers and tested in space since the mid-1960s [ref 1, 2], demonstrating a wide range of UV degradation rates, sometimes for the same formulation. Ground testing a particular ZnO-silicone coating in two different facilities yielded degradation rates that differed by more than a factor of 6. This is similar to variations seen in a round-robin test of ground UV exposure facilities in the 1960s [ref. 2] and casts doubt as to the usefulness of ground testing to predict flight performance. In this case, consideration of the differences between the two ground tests along with partial retesting, pointed to the presence of volatiles as the source of the difference. In one facility, the samples were baked out prior to testing, removing most of the volatiles in the paint, but in the other facility the samples were not baked out. This indicated that the primary source of absorptivity change was UV interaction, not with the silicone substrate material, nor with the ZnO scatterers, but with the volatiles. In addition, the two facilities had different UV irradiance spectra, which may have contributed to the large degradation variation [ref.3].

A literature search was conducted and, surprisingly, only one paper was found that tested ZnO-silicone paint degradation with and without a prebake [ref. 1]. In this publication, paint S-31 without a bake-out was exposed to 1780 equivalent solar hours (ESH) of UV and saw a change in absorptivity of 0.02, but a sample that was baked at 260°C (500°F) for 1 hour and then exposed to 1780 ESH saw only a change of 0.006. In a second case, two S-33 samples were exposed to 4170 ESH, both with a one hour 150°C prebake out and one with an additional one hour 260°C prebake. The one with the single bake-out saw an absorptivity change of 0.02 and the one with the additional bake-out saw a change of only 0.011, comparable to the “best zinc oxide…silicate paint.”

Testing of ZnO-silicone paints has been conducted on the Materials International Space Station experiment (MISSE), [ref. 4], showing a similar reduction in UV degradation for samples that were baked out prior to flight and those that were not. In MISSE-19, a sample of a ZnO-silicone paint that was baked out showed a net change in absorptivity of 0.011 (Wake position) versus 0.27 for a sample of the same paint in the Zenith position that was not baked out. There is positional variation that may have contributed to this difference, but the removal of volatiles is a likely contributor.

Finally, spacecraft testing of the same ZnO-silicone paint has shown very low UV degradation over extended periods in LEO which is interesting given that the paint on the spacecraft is not baked out. Aerodynamic heating on ascent is insufficient to remove the volatiles, however, surface temperatures while in orbit are sufficient. On the spacecraft, the paint covers an insulative, micrometeor protective layer allowing the paint to heat in sunlight (unlike the MISSE samples that are painted on aluminum disks mounted to an aluminum tray). This heating in orbit provides a nearly continuous bake-out, removing not only residual volatiles, but newly formed volatiles created by UV induced decomposition of longer chain molecules. Comparing outgassing data to the bake-out conditions further supports the proposition that volatiles within the paint, and not the binder or scatterers, discolor under solar UV exposure. Indicating that prebake or, in-flight continuous baking, is a key requirement for long duration performance of a specific family of ZnO-silicone based thermal control coatings.

A UV exposure facility at the Marshall Space Flight Center
Figure 1: A UV exposure facility at the Marshall Space Flight Center
Figure 2: A post exposure MISSE 2 sample tray [ref. 4]

References

1. Ref. Zerlaut, G. A., Y. Harada, and E. H. Tompkins. “41. Ultraviolet Irradiation of White Spacecraft Coatings.” In Symposium on Thermal Radiation of Solids, vol. 55, p. 391. Scientific and Technical Information Division, National Aeronautics andSpace Administration, 1965.

2. Arvesen, J. C., C. B. Neel, and C. C. Shaw. “44. Preliminary Results From a Round- Robin Study of Ultraviolet Degradation of Spacecraft.” In Symposium on Thermal Radiation of Solids, vol. 55, p. 443. Scientific and Technical Information Division, National Aeronautics and Space Administration, 1965.

3. ARVESEN, J. “Spectral dependence of ultraviolet-induced degradation of coatings for spacecraft thermal control.” In 2nd Thermophysics Specialist Conference, p. 340. 1967.

4. Kenny, Mike, Robert McNulty, and Miria Finckenor. “Further Analysis of Thermal Control Coatings on MISSE for Aerospace Applications.” In National Space and Missile Materials Symposium, no. M09-0535. 2009.

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Meagan Chappell

Crew Studies Cardiac Health and Unpacks Cygnus, Progress Spacecraft

Crew Studies Cardiac Health and Unpacks Cygnus, Progress Spacecraft

NASA astronauts Zena Cardman and Jonny Kim, both NASA astronauts, practice Canadarm2 robotic arm maneuvers on the Destiny laboratory module's robotics workstation. Kim commanded the Canadarm2 two days later to capture Northrop Grumman's Cygnus XL cargo craft with Cardman backing him up as the spacecraft arrived at the International Space Station.
NASA astronauts Zena Cardman and Jonny Kim practice Canadarm2 robotic arm maneuvers on the Destiny laboratory module’s robotics workstation. Kim commanded the Canadarm2 two days later to capture Northrop Grumman’s Cygnus XL cargo craft with Cardman backing him up as the spacecraft arrived at the International Space Station.
NASA

Expedition 73 kicked off the week with ultrasound scans for cardiac research and unloading new science experiments delivered last week aboard the Cygnus XL cargo craft. Spacesuit work and computer networking maintenance rounded out the day aboard the International Space Station.

NASA Flight Engineers Mike Fincke and Jonny Kim joined each other on Monday in the Columbus laboratory module to continue learning how living and working in space affects cardiovascular health. Fincke led the biomedical investigation scanning Kim’s chest with the Ultrasound 2 device to identify signs of space-caused plaque buildup or accelerated aging-like symptoms in the arteries. Kim also wore sensors that measured his cardiac activity during the scans for the CIPHER human research investigation. Doctors collect the health data from astronauts before, during, and after a spaceflight and compare it to data collected from other astronauts to gain clearer insights into crew health.

Earlier in the day, the duo partnered with NASA Flight Engineer Zena Cardman unpacking some of the 11,000 pounds of new science and supplies delivered last week aboard Northrop Grumman’s Cygnus XL resupply ship. A pair of portable science freezers containing research samples were removed from Cygnus and installed in an EXPRESS science rack ahead of upcoming experiment work. Cardman also installed new cloud computing hardware in the Destiny laboratory module then relocated air monitors from Destiny to the Tranquility module.

Flight Engineer Kimiya Yui of JAXA (Japan Aerospace Exploration Agency) spent his shift inside the Kibo laboratory module installing new computer networking gear. The ethernet hub upgrades will transmit data quicker and more efficiently throughout the orbital outpost.

Station Commander Sergey Ryzhikov of Roscosmos worked on an Orlan spacesuit in the Poisk module ahead of spacewalks planned for later this year. The three-time lab resident installed a variety of components inside the suit including a battery pack and a backup oxygen tank then conducted leak and pressure checks.

Flight Engineers Alexey Zubritsky and Oleg Platonov worked together throughout Monday unloading some of the nearly three tons of food, fuel, and supplies delivered aboard the Progress 93 cargo craft on Sept. 13. The duo also split up with Zubritsky working on the Roscosmos ventilation system and Platonov photographing landmarks in the Caspian Sea and the Amazon Delta.

Learn more about station activities by following the space station blog, @space_station on X, as well as the ISS Facebook and ISS Instagram accounts.

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Mark A. Garcia

Lettuce Find Healthy Space Food! Citizen Scientists Study Space Salads

Lettuce Find Healthy Space Food! Citizen Scientists Study Space Salads

Lettuce Find Healthy Space Food! Citizen Scientists Study Space Salads

Diagram illustrating research on lettuce grown in space stations and its effects on astronaut health. Lettuce nutritional content is linked to astronaut diet, potential diseases, and astronaut biological response. Missions including I4, JAXA, and NASA’s Twin Study are shown, with graphics of spacecraft, astronauts, the ISS, and biological diagrams.
Volunteer members of the OSDR-Analysis Working Groups examined the nutritional quality of crops grown in Low Earth Orbit and the physiological effects of space-induced nutrient deficiencies on astronauts. You can join the team here!
Credit: npj Microgravity/Barbero et al., 2025

Missions to the Moon and Mars pose nutritional challenges for astronauts. Now, a new paper on space-grown food iMissions to the Moon and Mars pose nutritional challenges for astronauts, but volunteers from NASA’s Open Science Data Repository Analysis Working Groups (OSDR-AWG) are working together to analyze data on astronaut health. The Analysis Working Groups examine biomedical data from NASA missions and space experiments collected in the NASA Open Science Data Repository. These teams use the data to answer questions in basic science, applied science, and health outcomes for space exploration.

For example, a recent paper on space-grown food examined data on lettuce grown on the International Space Station and the Tiangong II space station. It found that the crop contained 29-31% less calcium and 25% less magnesium than Earth lettuce, falling short of astronaut requirements.

Lettuce tell you more! The study revealed two further health challenges for astronauts relying on space grown veggies.

  • Disrupted calcium signaling: the analysis revealed that astronauts experienced changes in the expression of 163 calcium genes, which could accelerate bone loss. 
  • Leaky gut syndrome: data from the Japan Aerospace Exploration Agency (JAXA) show astronauts experienced compromised intestinal barriers due to altered protein production and regulation, likely disrupting their ability to absorb nutrients.

The researchers proposed a solution to these problems, too: bioengineered crops.! Perhaps plants could be developed that are enriched in calcium or therapeutic proteins to compensate for the deficiencies observed in the space-grown lettuce. 

This research was a collaboration between the ALSDA (Ames Life Sciences Data Archive), the Human Analysis and Plant Working Groups of the OSDR (the expansion of NASA Genelab centered at NASA Ames), along with BioAstra, a space life science non-profit. The data came primarily from OSDR with contributions from the Space Omics and Medical Atlas at Weill Cornell.

You can join the OSDR-Analysis Working Groups yourself and help plan the future of human space exploration. Dozens of project groups are active at any time. Learn more about the AWGs.

B Barbero Barcenilla, R Rivero, A Lynch, W Cromer, J Gong, B Harandi, M Stegmann, H Le, D Lundine, M Chung, J Puig, K Mikhailova, H Coker, A Marks, Rachel R. Gilbert, Ryan T. Scott, R Barker, P Glowe, EG Overbey, CE Mason. (2025) Feeding the cosmos: tackling personalized space nutrition and the leaky gut challenge. npj Microgravity 11, 45. https://doi.org/10.1038/s41526-025-00490-z

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Last Updated
Sep 22, 2025

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IC Stars

IC Stars

Material resembling a tangle of dark pink hair swirls dramatically across the image. The picture is dotted with dozens of colorful orbs in various sizes.
IC 348 is a star-forming region in our Milky Way galaxy.
X-ray: NASA/CXC/SAO; Infrared: NASA/ESA/CSA/STScI; Image Processing: NASA/CXC/SAO/J. Major

Data from NASA’s Chandra X-ray Observatory and NASA’s James Webb Space Telescope combine to reveal an otherworldly view of the star-forming region IC 348. In this image released on July 23, 2025, X-rays from Chandra are red, green, and blue, while infrared data from Webb are pink, orange, and purple.

The wispy structures that dominate the image are interstellar material that reflect the light from the cluster’s stars; this is known as a reflection nebula. The point-like sources in Chandra’s X-ray data are young stars in the cluster developing there.

Text credit: Megan Watzke

Image credit: X-ray: NASA/CXC/SAO; Infrared: NASA/ESA/CSA/STScI; Image Processing: NASA/CXC/SAO/J. Major

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Monika Luabeya