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By NASA
NASA logo Chile will sign the Artemis Accords during a ceremony at 3 p.m. EDT on Friday, Oct. 25, at NASA’s Headquarters in Washington.
NASA Administrator Bill Nelson will host Aisén Etcheverry, Chile’s minister of science, technology, knowledge and innovation, and Juan Gabriel Valdés, ambassador of Chile to the United States, along with other officials from Chile and the U.S. Department of State.
This event is in-person only. U.S. media and U.S. citizens representing international media organizations interested in attending must RSVP no later than 5 p.m. on Thursday, Oct. 24, to hq-media@mail.nasa.gov. NASA’s media accreditation policy is online.
The signing ceremony will take place at the agency’s Glennan Assembly Room inside NASA Headquarters located at 300 E St. SW Washington.
NASA, in coordination with the U.S. Department of State and seven other initial signatory nations, established the Artemis Accords in 2020. With many countries and private companies conducting missions and operations around the Moon, the Artemis Accords provide a common set of principles to enhance the governance of the civil exploration and use of outer space.
The Artemis Accords reinforce the commitment by signatory nations to the Outer Space Treaty, the Registration Convention, the Rescue and Return Agreement, as well as best practices and norms of responsible behavior for civil space exploration and use.
Learn more about the Artemis Accords at:
https://www.nasa.gov/artemis-accords
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Meira Bernstein / Elizabeth Shaw
Headquarters, Washington
202-358-1600
meira.b.bernstein@nasa.gov / elizabeth.a.shaw@nasa.gov
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Last Updated Oct 21, 2024 LocationNASA Headquarters Related Terms
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By NASA
Microgravity had no immediate effect on a person’s ability to perceive the height of an object, indicating that astronauts can safely perform tasks that rely on accurate and precise height judgments soon after arrival in space.
We use the height and width of objects around us to complete tasks such as reaching for objects and deciding whether we can fit through an opening. VECTION, an investigation from the Canadian Space Agency, examined the effect of microgravity on an astronaut’s visual perception and how that ability may adapt during flight or upon return to Earth. Researchers conclude there is no need for countermeasures but suggest that space travelers be made aware of late-emerging and potentially long-lasting changes in the ability to perceive object height.
Canadian Space Agency astronaut David Saint-Jacques conducts a session for the VECTION experiment. NASA/Anne McClain Analysis of the genomes of five new species of bacteria found on the International Space Station identified specific adaptations to space, including the development of increased antibiotic resistance and a greater potential for causing diseases. The genes that facilitate these adaptations could serve as potential targets for drugs, helping to protect crew health on future missions.
Microbial Tracking-2 monitored viruses, bacteria, and fungi on the space station to catalog and characterize any with the potential to cause disease. Understanding the mechanisms behind adaptations to space could advance development of ways to protect crew member health as well as spacecraft and equipment on future missions. Microbial adaptations also have potential applications in biotechnology, such as engineering more resilient organisms for use in space and extraterrestrial environments.
A Microbial Tracking-2 sample collector on the International Space Station. NASA/Jack Fischer When NASA’s Airborne Lightning Observatory for Fly’s Eye and the space station’s ASIM instrument briefly passed over the same geographic area, the airborne instrument detected terrestrial gamma‐ray flashes (TGFs) that were not detected by ASIM. TGFs are short bursts of gamma‐rays produced by lightning in thunderclouds. This result suggests that a significant number of TGFs are too weak to be observed from space and that the percentage of lightning associated with these phenomena may be higher than previously thought.
ASIM, an investigation from the European Space Agency, studies high-altitude lightning in thunderstorms and the role it plays in Earth’s atmosphere and climate. Results could help scientists develop better atmospheric models to guide weather and climate prediction and response. The airborne instrument took measurements at an altitude of about 12 miles and ASIM at approximately 260 miles above Earth’s surface.
A view of ASIM mounted on the outside of the space station. NASAView the full article
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By NASA
NASA has selected four new crew members to participate in the final simulated mission to Mars in 2024 inside the agency’s Human Exploration Research Analog. From left are Kristen Magas, Anderson Wilder, Obaid Alsuwaidi, and Tiffany Snyder.Credit: C7M4 Crew NASA selected a crew of four research volunteers to participate in its last simulated mission to Mars in 2024 within a habitat at the agency’s Johnson Space Center in Houston.
Obaid Alsuwaidi, Kristen Magas, Tiffany Snyder, and Anderson Wilder will step into the 650-square-foot HERA (Human Exploration Research Analog) facility on Friday, Nov. 1. Once inside, the team will live and work like astronauts for 45 days. The crew will exit the facility on Monday, Dec. 16, after simulating their return to Earth. Jordan Hundley and Robert Wilson also were named as alternate crew members.
Scientists use HERA studies to examine how crew members adapt to isolation, confinement, and remote conditions before NASA sends astronauts on deep space missions to the Moon, Mars, and beyond. The studies provide data about human health and performance in an enclosed environment over time with crews facing different challenges and tasks.
The four volunteers will carry out scientific research and operational tasks throughout their simulated mission, including raising shrimp, growing vegetables, and “walking” on the surface of Mars using virtual reality. They will also experience communication delays lasting up to five minutes as they “near” Mars, allowing researchers to see how crews may respond to the type of delays astronauts will encounter in deep space. Astronauts traveling to the Red Planet may encounter one-way communication delays lasting as long as 20 minutes.
As with the previous HERA missions, crew members will conduct 18 human health studies during the mission through NASA’s Human Research Program. Collectively, the work helps scientists understand how a spaceflight-like environment contributes to the physiological, behavioral, and psychological health of crew members. Insights gleaned from the studies will allow researchers to develop and test strategies aimed at helping astronauts overcome obstacles on deep space missions.
Primary Crew
Obaid Alsuwaidi
Obaid Alsuwaidi serves as captain engineer for the United Arab Emirates’ (UAE) Ministry of Defense. In this role, he provides guidance in civil and marine engineering and addresses challenges facing the organization. Previously, Alsuwaidi worked as a project manager for the defense ministry, helping to streamline productivity, establish high standards of professionalism, and build a team of experts to serve the UAE’s needs.
Alsuwaidi earned a bachelor’s degree in Engineering from Western Sydney University in Australia, followed by a master’s degree in Civil and Environmental Engineering from George Washington University in Washington.
In his free time, Alsuwaidi enjoys horseback riding, swimming, and running.
Kristen Magas
Kristen Magas is an educator and engineer, currently teaching at Tri-County Regional Vocational Technical High School in Franklin, Massachusetts. She also mentors students involved in a NASA design and prototyping program, helping them develop and fabricate products to improve life in space on both International Space Station and Artemis missions. Magas was a finalist for the 2025 Massachusetts State Teacher of the Year.
Magas received bachelor’s and master’s degrees in Civil and Environmental Engineering from Cornell University in Ithaca, New York. She also holds a master’s degree in Vocational Education from Westfield State University in Massachusetts. She has worked as a community college professor as well as a design engineer in municipal water and wastewater treatment.
In her spare time, Magas enjoys coaching robotics and track and field, hiking, biking, and staying connected with her community. She has two children and resides in North Attleboro, Massachusetts with her husband of 25 years.
Tiffany Snyder
Tiffany Snyder is a supervisor for the Cybersecurity Mission Integration Office at NASA, helping to ensure agency missions are shielded against cybersecurity threats. She has more than 20 years of information technology and cybersecurity experience, working with the Air National Guard and as a special agent with the Defense Counterintelligence Security Agency. She joined NASA in 2018 as an IT specialist, and later served as the deputy chief information security officer at NASA’s Kennedy Space Center in Florida, providing cybersecurity oversight.
Snyder holds a bachelor’s degree in Earth Science from the State University of New York at Buffalo and a master’s degree in Digital Forensics from the University of Central Florida in Orlando.
In her spare time, she enjoys playing with her dogs — Artemis and Apollo, gardening, running, and visiting the beach with her family.
Anderson Wilder
Anderson Wilder is a Florida Institute of Technology graduate student working on his doctorate in Psychology. His research focuses on team resiliency and human-machine interactions. He also works in the campus’s neuroscience lab, investigating how spaceflight contributes to neurobehavioral changes in astronauts.
Wilder previously served as an executive officer and engineer for an analog mission at the Mars Desert Research Station in Utah. There, he performed studies related to crew social dynamics, plant growth, and geology.
Wilder received his bachelor’s degrees in Linguistics and in Psychology from Ohio State University in Columbus. He also holds master’s degrees in Space Studies from International Space University in Strasbourg, France, and in Aviation Human Factors from the Florida Institute of Technology. He is completing another master’s degree in Cognitive Experimental Psychology at Cleveland State University in Ohio.
Outside of school, Wilder works as a parabolic flight coach, teaching people how to fly in reduced gravity environments. He also enjoys chess, reading, video games, skydiving, and scuba diving. On a recent dive, he explored a submerged section of the Great Wall of China.
Alternate Crew
Jordan Hundley
Jordan Hundley is a senior consultant at a professional services firm, offering federal agencies technical and programmatic support. Prior to his current position, he focused on U.S. Department of Defense clients, performing model-based system engineering and serving as a subject matter expert for related operations.
Hundley was commissioned into the U.S. Air Force through the Reserve Officers’ Training Corps program at the University of Central Florida in Orlando. While on active duty, he served as an intercontinental ballistic missile operations officer. He later joined the U.S. Air Force Reserve. Currently, he is a space operations officer with experience in space battle management and electromagnetic warfare.
Hundley earned a master’s degree in Engineering Management from Embry-Riddle Aeronautical University in Daytona Beach, Florida. He is currently pursuing a second master’s degree in Systems Engineering at the university.
Hundley holds a private pilot license and is a certified rescue diver. In his spare time, he enjoys hiking and camping, researching theology, and learning musical instruments.
Robert Wilson
Robert Wilson is a senior researcher and project manager at the Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland. He leads work enhancing human-machine collaborations, developing human prediction models, and integrating that technology into virtual reality and robotic systems designed to operate in isolated, constrained, and extreme environments. His human-machine teaming expertise also extends into responsible artificial intelligence development. He recently participated in a United Nations Roundtable discussion about artificial intelligence in security and defense.
Wilson received his bachelor’s and master’s degrees in Biomedical Engineering from Purdue University in 2013 and 2015, respectively. He earned his doctorate in Mechanical Engineering from the University of Colorado Boulder in 2020.
Outside of work, Wilson is an avid outdoors enthusiast. He enjoys scuba diving, winter camping, backcountry skiing, and hiking through the woods or mountains throughout the year. At home, he also likes to tinker in computer networking and self-hosted systems.
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NASA’s Human Research Program pursues the best methods and technologies to support safe, productive human space travel. Through science conducted in laboratories, ground-based analogs, commercial missions, and the International Space Station, the program scrutinizes how spaceflight affects human bodies and behaviors. Such research continues to drive NASA’s mission to innovate ways that keep astronauts healthy and mission-ready as human space exploration expands to the Moon, Mars, and beyond.
For more information about human research at NASA, visit:
https://www.nasa.gov/hrp
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Researchers think meltwater beneath Martian ice could support microbial life.
The white material seen within this Martian gully is believed to be dusty water ice. Scientists believe this kind of ice could be an excellent place to look for microbial life on Mars today. This image, showing part of a region called Dao Vallis, was captured by NASA’s Mars Reconnaissance Orbiter in 2009.NASA/JPL-Caltech/University of Arizona These holes, captured on Alaska’s Matanuska Glacier in 2012, are formed by cryoconite — dust particles that melt into the ice over time, eventually forming small pockets of water below the glacier’s surface. Scientists believe similar pockets of water could form within dusty water ice on Mars.Kimberly Casey CC BY-NC-SA 4.0 While actual evidence for life on Mars has never been found, a new NASA study proposes microbes could find a potential home beneath frozen water on the planet’s surface.
Through computer modeling, the study’s authors have shown that the amount of sunlight that can shine through water ice would be enough for photosynthesis to occur in shallow pools of meltwater below the surface of that ice. Similar pools of water that form within ice on Earth have been found to teem with life, including algae, fungi, and microscopic cyanobacteria, all of which derive energy from photosynthesis.
“If we’re trying to find life anywhere in the universe today, Martian ice exposures are probably one of the most accessible places we should be looking,” said the paper’s lead author, Aditya Khuller of NASA’s Jet Propulsion Laboratory in Southern California.
Mars has two kinds of ice: frozen water and frozen carbon dioxide. For their paper, published in Nature Communications Earth & Environment, Khuller and colleagues looked at water ice, large amounts of which formed from snow mixed with dust that fell on the surface during a series of Martian ice ages in the past million years. That ancient snow has since solidified into ice, still peppered with specks of dust.
Although dust particles may obscure light in deeper layers of the ice, they are key to explaining how subsurface pools of water could form within ice when exposed to the Sun: Dark dust absorbs more sunlight than the surrounding ice, potentially causing the ice to warm up and melt up to a few feet below the surface.
The white edges along these gullies in Mars’ Terra Sirenum are believed to be dusty water ice. Scientists think meltwater could form beneath the surface of this kind of ice, providing a place for possible photosynthesis. This is an enhanced-color image; the blue color would not actually be perceptible to the human eye.NASA/JPL-Caltech/University of Arizona Mars scientists are divided about whether ice can actually melt when exposed to the Martian surface. That’s due to the planet’s thin, dry atmosphere, where water ice is believed to sublimate — turn directly into gas — the way dry ice does on Earth. But the atmospheric effects that make melting difficult on the Martian surface wouldn’t apply below the surface of a dusty snowpack or glacier.
Thriving Microcosms
On Earth, dust within ice can create what are called cryoconite holes — small cavities that form in ice when particles of windblown dust (called cryoconite) land there, absorb sunlight, and melt farther into the ice each summer. Eventually, as these dust particles travel farther from the Sun’s rays, they stop sinking, but they still generate enough warmth to create a pocket of meltwater around them. The pockets can nourish a thriving ecosystem for simple lifeforms..
“This is a common phenomenon on Earth,” said co-author Phil Christensen of Arizona State University in Tempe, referring to ice melting from within. “Dense snow and ice can melt from the inside out, letting in sunlight that warms it like a greenhouse, rather than melting from the top down.”
Christensen has studied ice on Mars for decades. He leads operations for a heat-sensitive camera called THEMIS (Thermal Emission Imaging System) aboard NASA’s 2001 Mars Odyssey orbiter. In past research, Christensen and Gary Clow of the University of Colorado Boulder used modeling to demonstrate how liquid water could form within dusty snowpack on the Red Planet. That work, in turn, provided a foundation for the new paper focused on whether photosynthesis could be possible on Mars.
In 2021, Christensen and Khuller co-authored a paper on the discovery of dusty water ice exposed within gullies on Mars, proposing that many Martian gullies form by erosion caused by the ice melting to form liquid water.
This new paper suggests that dusty ice lets in enough light for photosynthesis to occur as deep as 9 feet (3 meters) below the surface. In this scenario, the upper layers of ice prevent the shallow subsurface pools of water from evaporating while also providing protection from harmful radiation. That’s important, because unlike Earth, Mars lacks a protective magnetic field to shield it from both the Sun and radioactive cosmic ray particles zipping around space.
The study authors say the water ice that would be most likely to form subsurface pools would exist in Mars’ tropics, between 30 degrees and 60 degrees latitude, in both the northern and southern hemispheres.
Khuller next hopes to re-create some of Mars’ dusty ice in a lab to study it up close. Meanwhile, he and other scientists are beginning to map out the most likely spots on Mars to look for shallow meltwater — locations that could be scientific targets for possible human and robotic missions in the future.
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Andrew Good
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-2433
andrew.c.good@jpl.nasa.gov
Karen Fox / Molly Wasser
NASA Headquarters, Washington
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Last Updated Oct 17, 2024 Related Terms
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Jacquelyn Shuman visually assesses a prescribed fire at Ft. Stewart in Georgia, working with partner organizations as part of the Department of Defense Ft. Stewart 2024 Fire Research Campaign. USFS/Linda Chappell Jacquelyn Shuman, FireSense Project Scientist at NASA Ames Research Center, originally wanted to be a veterinarian. By the time she got to college, Shuman had switched interests to biology, which became a job teaching middle and high school science. Teaching pivoted to finance for a year, before Shuman returned to the science world to pursue a PhD.
It was in a forest ecology class taught by her future PhD advisor, Herman “Hank” Shugart, that she first discovered a passion for ecosystems and dynamic vegetation that led her into the world of fire science, and eventually to NASA Ames.
While Shuman’s path into the world of fire science was not a direct one, she views her diverse experiences as the key to finding a fulfilling career. “Do a lot of different things and try a lot of different things, and if one thing isn’t connecting with you, then do something different,” Shuman said.
Diving into the World of Fire
Shuman’s PhD program focused on boreal forest dynamics across Russia, examining how the forest changes in response to climate change and wildfire. During her research, she worked mainly with scientists from Russia, Canada, and the US through the Northern Eurasia Earth Science Partnership Initiative (NEESPI), where Shugart served as the NEESPI Chief Scientist. “The experience of having a highly supportive mentor, being a part of the NEESPI community, and working alongside other inspiring female scientists from across the globe helped me to stay motivated within my own research,” Shuman said.
After completing her PhD, Shuman wanted to become involved in collaborative science with a global impact, which led her to the National Center for Atmospheric Research (NCAR). There, she spent seven years working as a project scientist on the Next Generation Ecosystem Experiment NGEE-Tropics) on a dynamic vegetation model project called FATES (Functionally Assembled Terrestrial Ecosystem Simulator). As part of the FATES team, Shuman used computer modeling to test vegetation structure and function in tropical and boreal forests after wildfires, and was the lead developer for updating the fire portion of the model.
This figure shows fire characteristics from an Earth system model that uses vegetation structure and interactive fire. The FATES model captures the fire intensity associated with burned land and grass growth in the Southern Hemisphere. Shuman et al. 2024 GMD Fire has also played a powerful role in Shuman’s personal life. In 2021, the Marshall Fire destroyed neighborhoods near her hometown of Boulder, Colorado, causing over $513 million of damage and securing its place as the state’s most destructive wildfire. Despite this, Shuman is determined to not live in fear. “Fire is part of our lives, it’s a part of the Earth system, and it’s something we can plan for. We can live more sustainably with fires.” The way to live safely in a fire-inclusive ecosystem, according to Shuman, is to develop ways to accurately track and forecast wildfires and smoke, and to respond to them efficiently: efforts the fire community is continuously working on improving.
The Fire Science Community
Collaboration is a critical element of wildland fire management. Fire science is a field that involves practitioners such as firefighters and land managers, but also researchers such as modelers and forecasters; the most effective efforts, according to Shuman, come when this community works together. “People in fire science might be out in the field and carrying a drip torch and marching along in the hilltops and the grasslands or be behind a computer and analyzing remote sensing data,” Shuman said. “We need both pieces.”
Protecting communities from wildfire impacts is one of the most fulfilling aspects of Shuman’s career, and a goal that unites this community. “Fire research poses tough questions, but the people who are thinking about this are the people who are acting on it,” Shuman said. “They are saying, ‘What can we do? How can we think about this? What information do we need? What are the questions?’ It’s a special community to be a part of.”
Looking to the Future of Fire
Currently at NASA Ames Research Center, Shuman is the Project Scientist for FireSense: a project focused on delivering NASA science and technology to practitioners and operational agencies. Shuman acts as the lead for the project office, identifying and implementing tools and strategies. Shuman still does ecosystem modeling work, including implementing vegetation models that forecast the impact of fire, but also spends time traveling to active fires across the country so she can help partners implement NASA tools and strategies in real time.
FireSense Project Scientist Jacquelyn Shuman stands with Roger Ottmar (United States Forest Service), surveying potential future locations for prescribed burns in Fishlake National Forest. NASA Ames/Milan Loiacono
“Right now, many different communities are all recognizing that we can partner to identify the best path forward,” Shuman said. “We have an opportunity to use everyone’s strengths and unique perspectives. It can be a devastating thing for a community and an ecosystem when a fire happens. Everyone is interested in using all this collective knowledge to do more, together.”
Written by Molly Medin, NASA Ames Research Center
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Last Updated Oct 17, 2024 Related Terms
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