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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
Environmentalist and former Vice President Al Gore visited NASA’s Goddard Space Flight Center in Greenbelt, Maryland, on Oct. 16, 2024, to commemorate the upcoming 10th anniversary of the DSCOVR (Deep Space Climate Observatory) mission.
“The image of our Earth from space is the single most compelling iconic image that any of us have ever seen,” Gore said at a panel discussion for employees. “Now we have, thanks to DSCOVR, 50,000 ‘Blue Marble’ photographs … To date there are more than 100 peer-reviewed scientific publications that are based on the unique science gathered at the L1 point by DSCOVR. For all of the scientists who are here and those on the teams that are represented here, I want to say congratulations and thank you.”
To commemorate the upcoming 10th anniversary of the DSCOVR (Deep Space Climate Observatory) mission, NASA’s Goddard Space Flight Center in Greenbelt, Md., hosted environmentalist and former Vice President Al Gore, shown here addressing a crowd in the Building 3 Harry J. Goett Auditorium, on Oct. 16, 2024.NASA/Travis Wohlrab Following opening remarks from Gore, Goddard scientists participated in a panel discussion entitled “Remote Sensing and the Future of Earth Observations. From left to right: Dalia Kirschbaum, director, NASA Goddard Earth Sciences Division; Miguel Román, deputy director, atmospheres, NASA Goddard Earth Sciences Division; Lesley Ott, project scientist, U.S. Greenhouse Gas Center; John Bolten, chief, NASA Goddard Hydrological Sciences Laboratory.NASA/Travis Wohlrab Gore shakes hands with Kirschbaum following the panel discussion. Goddard Center Director Makenzie Lystrup stands between the two.NASA/Katy Comber Gore visits the overlook for the NASA Goddard clean room where the Roman Space Telescope is being assembled. Julie McEnery, Roman senior project scientist, stands at right.NASA/Katy Comber Christa Peters-Lidard, NASA Goddard’s Sciences and Exploration Directorate director (left), speaks with Gore in the lobby of Building 32, where the former vice president viewed the control room of NASA’s Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) mission.NASA/Katy Comber Following Gore’s talk on climate monitoring, Goddard scientists participated in a panel discussion, “Remote Sensing and the Future of Earth Observations,” which explored the latest advancements in technology that allow for the monitoring of the atmosphere from space and showcased how Goddard’s research drives the future of Earth science.
Gore’s visit also entailed a meeting with the DSCOVR science team, a view into the clean room where Goddard is assembling the Roman Space Telescope, and a stop at the control center for PACE: NASA’s Plankton, Aerosol, Cloud, ocean Ecosystem mission.
Launched Feb. 11, 2015, DSCOVR is a space weather station that monitors changes in the solar wind, providing space weather alerts and forecasts for geomagnetic storms that could disrupt power grids, satellites, telecommunications, aviation and GPS.
DSCOVR is a joint mission among NASA, the National Oceanic and Atmospheric Administration (NOAA), and the U.S. Air Force. The project originally was called Triana, a mission conceived of by Gore in 1998 during his vice presidency.
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Last Updated Oct 17, 2024 EditorRob GarnerContactRob Garnerrob.garner@nasa.govLocationGoddard Space Flight Center Related Terms
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By NASA
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA’s C-130 Hercules is prepared for departure from NASA’s Wallops Flight Facility in Virginia, on October 15, 2024, for a cargo transport mission to India. The C-130 is supporting the NASA-ISRO Synthetic Aperture Radar (NISAR) mission.NASA/Madison Griffin NASA’s globetrotting C-130 Hercules team is carrying out a cargo transport mission to Bengaluru, India, in support of the NASA-ISRO Synthetic Aperture Radar (NISAR) mission.
The C-130 departed from NASA’s Wallops Flight Facility in Virginia, Tuesday, Oct. 15, to embark on the multi-leg, multi-day journey. The flight path will take the aircraft coast to coast within the United States, across the Pacific Ocean with planned island stops, and finally to its destination in India. The goal: safely deliver NISAR’s radar antennae reflector, one of NASA’s contributions to the mission, for integration on the spacecraft. NISAR is a joint mission between NASA and ISRO (Indian Space Research Organisation).
The cargo transport mission will encompass approximately 24,500 nautical miles and nearly 80 hours of flight time for the C-130 and crew. The flight plan includes strategic stops and rest days to service the aircraft and reduce crew fatigue from long-haul segments of the flight and multiple time zone changes.
The flight crew inspects the aircraft prior to departure from NASA Wallops.NASA/Madison Griffin The C-130’s cargo compartment has plenty of space to hold the more than 2,800-pound payload containing the radar antennae reflector once retrieved from California.NASA/Madison Griffin The first stop for the C-130 was March Air Reserve Base located in Riverside County, California, to retrieve the radar antennae reflector from NASA’s Jet Propulsion Laboratory in Southern California. Additional stops during the mission include Hickman Air Force Base, Hawaii; Andersen Air Force Base, Guam; Clark Air Base, Philippines; and Hindustan Aeronautics Limited Airport in Bengaluru, India.
This is the C-130 and crew’s third cargo transport to India in support of the NISAR mission, with prior flights in July 2023 and March 2024.
For more information, visit nasa.gov/wallops.
By Olivia Littleton
NASA’s Wallops Flight Facility, Wallops Island, Va.
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Last Updated Oct 17, 2024 EditorOlivia F. LittletonContactOlivia F. Littletonolivia.f.littleton@nasa.gov Related Terms
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By NASA
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
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.
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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
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Last Updated Oct 17, 2024 Related Terms
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4 min read New Team to Assess NASA’s Mars Sample Return Architecture Proposals
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Mars Sample Return MSR Home Mission Concept Overview Perseverance Rover Sample Retrieval Lander Mars Ascent Vehicle Sample Recovery Helicopters Earth Return Orbiter Science Overview Bringing Mars Samples to Earth Mars Rock Samples MSR Science Community Member Sign up News and Features Multimedia Images Videos Audio More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions The Solar System The Sun Mercury Venus Earth The Moon Mars Jupiter Saturn Uranus Neptune Pluto & Dwarf Planets Asteroids, Comets & Meteors The Kuiper Belt The Oort Cloud 4 min read
New Team to Assess NASA’s Mars Sample Return Architecture Proposals
NASA announced Wednesday a new strategy review team will assess potential architecture adjustments for the agency’s Mars Sample Return Program, which aims to bring back scientifically selected samples from Mars, and is a key step in NASA’s quest to better understand our solar system and help answer whether we are alone in the universe.
Earlier this year, the agency commissioned design studies from the NASA community and eight selected industry teams on how to return Martian samples to Earth in the 2030s while lowering the cost, risk, and mission complexity. The new strategy review team will assess 11 studies conducted by industry, a team across NASA centers, the agency’s Jet Propulsion Laboratory in Southern California, and the Johns Hopkins Applied Physics Laboratory. The team will recommend to NASA a primary architecture for the campaign, including associated cost and schedule estimates.
“Mars Sample Return will require a diversity of opinions and ideas to do something we’ve never done before: launch a rocket off another planet and safely return samples to Earth from more than 33 million miles away,” said NASA Administrator Bill Nelson. “It is critical that Mars Sample Return is done in a cost-effective and efficient way, and we look forward to learning the recommendations from the strategy review team to achieve our goals for the benefit of humanity.”
Returning samples from Mars has been a major long-term goal of international planetary exploration for more than three decades, and the Mars Sample Return Program is jointly planned with ESA (European Space Agency). NASA’s Perseverance rover is collecting compelling science samples that will help scientists understand the geological history of Mars, the evolution of its climate, and potential hazards for future human explorers. Retrieval of the samples also will help NASA’s search for signs of ancient life.
The team’s report is anticipated by the end of 2024 and will examine options for a complete mission design, which may be a composite of multiple studied design elements. The team will not recommend specific acquisition strategies or partners. The strategy review team has been chartered under a task to the Cornell Technical Services contract. The team may request input from a NASA analysis team that consists of government employees and expert consultants. The analysis team also will provide programmatic input such as a cost and schedule assessment of the architecture recommended by the strategy review team.
The Mars Sample Return Strategy Review Team is led by Jim Bridenstine, former NASA administrator, and includes the following members:
Greg Robinson, former program director, James Webb Space Telescope Lisa Pratt, former planetary protection officer, NASA Steve Battel, president, Battel Engineering; Professor of Practice, University of Michigan, Ann Arbor Phil Christensen, regents professor, School of Earth and Space Exploration, Arizona State University, Tempe Eric Evans, director emeritus and fellow, MIT Lincoln Lab Jack Mustard, professor of Earth, Environmental, and Planetary Science, Brown University Maria Zuber, E. A. Griswold professor of Geophysics and presidential advisor for science and technology policy, MIT The NASA Analysis Team is led by David Mitchell, chief program management officer at NASA Headquarters, and includes the following members:
John Aitchison, program business manager (acting), Mars Sample Return Brian Corb, program control/schedule analyst, NASA Headquarters Steve Creech, assistant deputy associate administrator for Technical, Moon to Mars Program Office, NASA Headquarters Mark Jacobs, senior systems engineer, NASA Headquarters Rob Manning, chief engineer emeritus, NASA JPL Mike Menzel, senior engineer, NASA Goddard Fernando Pellerano, senior advisor for Systems Engineering, NASA Goddard Ruth Siboni, chief of staff, Moon to Mars Program Office, NASA Headquarters Bryan Smith, director of Facilities, Test and Manufacturing, NASA Glenn Ellen Stofan, under secretary for Science and Research, Smithsonian For more information on NASA’s Mars Sample Return, visit:
https://science.nasa.gov/mission/mars-sample-return
Dewayne Washington
Headquarters, Washington
202-358-1100
dewayne.a.washington@nasa.gov
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Last Updated Oct 16, 2024 Related Terms
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