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NASA Wins 6 Webby Awards, 8 Webby People’s Voice Awards
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)NASA’s broad reach across digital platforms has been recognized by the International Academy of Digital Arts and Sciences (IADAS), which awarded NASA 6 Webbys in the 28th Annual Webby Awards.
Editor’s Note: This article has been updated to add Hubble’s Inside the Image to the list of Webby Award wins.
NASA was recognized today by the 28th Annual Webby Awards with six Webby Awards and eight Webby People’s Voice Awards, the latter of which are awarded by the voting public. The Webbys honors excellence in nine major media types: websites and mobile sites, video, advertising, media and public relations, apps and software, social media, podcasts, games, the metaverse, and virtual and artificial intelligence (AI).
“We’re thrilled that the Webbys have recognized the breadth of NASA’s digital communications,” said Marc Etkind, associate administrator for communications. “To have a podcast, a virtual exhibit, live streaming, social and web all honored shows how our skilled and accomplished our team is. We’re especially pleased to see awards recognizing our reinvigorated digital platforms, including the NASA website and NASA+ streaming service. Together with the science website and NASA app, they are the core of our digital communications.”
The broad scope of the awards also highlights the agency’s enterprise approach to communications. For example, live streams are produced and led by the Office of Communications at NASA Headquarters in Washington. Each program, however, originates from within projects at NASA centers and represents many months of logistical preparation, rehearsals and constant review and adjustment. Once the TV streams are set, they are hosted on NASA’s website and fed to NASA’s social media channels, where the agency team engages with the live audience, providing background context and answering questions. All the while, agency photographers are documenting the effort and posting pictures to digital platforms while NASA’s audio team is gather sound and interviews to continue telling the story via podcasts.
Since 1998, NASA has been nominated for more than 100 Webby Awards, winning 37 Webbys and 53 People’s Voice Awards.
Full List of NASA’s 28th Annual Webby Award WinsNASA.gov
Webby Winner, People’s Voice Winner
Websites and Mobile Sites-General Desktop & Mobile Sites | Government & Associations
This is the fifth Webby Award and the 12th People’s Voice Award for the agency’s website
NASA’s Curious Universe: Suiting Up for Space
Webby Winner, People’s Voice Winner
Best Podcasts-Individual Episodes | Science & Education
NASA’s Immersive Earth
Webby Winner, People’s Voice Winner
Artificial Intelligence (AI), Metaverse & Virtual-General Virtual Experiences | Science & Education
NASA: Message in a Bottle
NASA Jet Propulsion Laboratory
Webby Winner, People’s Voice Winner
Advertising, Media & PR-PR Campaigns | Best Community Engagement
OSIRIS-REx Asteroid Sample Return (Official 4K NASA Live Stream)
People’s Voice Winner
Video-General Video | Events & Live Streams
NASA’s First Asteroid Sample Return Mission
Webby Winner, People’s Voice Winner
Social-Social Campaigns | Education & Science
NASA+ Streaming Service
Webby Winner
Websites and Mobile Sites-General Desktop & Mobile Sites | Television, Film & Streaming
Annular Solar Eclipse
People’s Voice Winner
Social-Social Campaigns | Events & Live Streams
Hubble’s Inside the Image
NASA, Origin Films
People’s Voice Winner
Video-Video Series & Channels | Science & Education
Established in 1996, The Webby Awards are presented by the International Academy of Digital Arts and Sciences (IADAS)—a judging body comprised of more than 3,000 leading Internet experts, business figures, luminaries, visionaries and creative celebrities. The Webbys honor excellence in nine major media types: websites and mobile sites, video, advertising, media and public relations, apps and software, social, podcasts, games and Metaverse, virtual and artificial Intelligence (AI).
The Webby Awards presents two honors in every category—The Webby Award and The Webby People’s Voice Award. Members of the International Academy of Digital Arts and Sciences (IADAS) select the nominees for both awards in each category, as well as the winners of The Webby Awards. The Webby People’s Voice is awarded by the voting public.
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Sols 4164-4165: What’s Around the Ridge-bend?
2 min read
Sols 4164-4165: What’s Around the Ridge-bend? This image was taken by the Left Navigation Camera and looks towards the deposits that make up the bend in Gediz Vallis ridge between “Pinnacle Ridge” and “Fascination Turret”. In the background is the layered stratigraphy that makes up the butte “Texoli”. NASA/JPL-CaltechEarth planning date: Monday, April 22, 2024
Curiosity succeeded on a ~14 m drive along a bend in upper Gediz Vallis ridge (uGVR) to park next to “Pinnacle Ridge,” an outcrop of uGVR to the north. Benefitting from a surplus in power, Curiosity’s already substantial targeted science block was extended to 2 hours. This allowed for the perfect imaging opportunity to look back and investigate the ridge deposits between “Pinnacle Ridge” and “Fascination Turret,” an outcrop of uGVR to the south. In other words, most of the imaging opportunities in this two-sol plan will be spent documenting what’s just around the ridge-bend with a detailed Mastcam stereo-mosaic and two ChemCam Long Distance RMI mosaics.
Today I served as Keeper of the Plan for the Geology and Mineralogy Theme Group, where I was kept busy recording all of the geology related requests from the instrument teams. The first sol involved planning contact science on a nearby dark-toned float block, “Sluggo Pass,” possibly originating from Gediz Vallis ridge. The composition and sedimentary textures of “Sluggo Pass” will be investigated with the Alpha Particle X-Ray Spectrometer (APXS), a ChemCam passive raster, and the Mars Hand Lens Imager (MAHLI). While constraints prevented brushing “Sluggo Pass” with the Dust Removal Tool (DRT), the target appeared to be relatively dust-free. The rest of the science plan on the first sol includes a ChemCam Laser-Induced Breakdown Spectroscopy (LIBS) targeting a dark-toned coating on light-toned bedrock, dubbed ‘South Lake,’ and two small Mastcam mosaics on blocks possibly associated with “Pinnacle Ridge.”
After a planned ~31 m drive from our current location, the focus of the second sol of the plan will be on untargeted remote science. This includes one of ChemCam’s automated AEGIS (Autonomous Exploration for Gathering Increased Science) activities where geological targets are automatically selected from the rover’s navigation cameras for analysis with ChemCam. Additionally, environmental activities were also planned, including tau observations to assess the amount of dust in the atmosphere and Mastcam deck monitoring activities to assess the amount of dust accumulated on the rover deck.
Written by Amelie Roberts, Graduate Student at Imperial College London
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First NASA Mars Analog Crew Nears End of Mission
The first crew to take part in a yearlong NASA Mars analog mission reached the 300-day mark of its mission on April 20.
The team of four volunteers entered the CHAPEA (Crew Health and Performance Exploration Analog) habitat at NASA’s Johnson Space Center in Houston on June 25, 2023, and is expected to complete the mission on July 6, 2024.
During their 300 days in the ground-based habitat, the crew engaged in multiple simulated “Marswalks,” grew and harvested several salad crops to occasionally supplement their shelf-stable food, and took part in habitat and equipment maintenance.
NASA is leading a return to the Moon for long-term science and exploration. Through Artemis missions, NASA will land the first woman, first person of color, and first international partner astronaut on the Moon, using innovative technologies to explore more of the lunar surface than ever before. Lessons learned on and around the Moon and activities like CHAPEA on the ground will prepare NASA for the next giant leap: sending astronauts to Mars.
A CHAPEA mission 1 crew member performs maintenance on hardware outside of the habitat during a simulated spacewalk in December 2023. NASA/CHAPEA Crew The CHAPEA mission 1 crew celebrates Christmas inside the habitat (from left: Ross Brockwell, Anca Selariu, Nathan Jones, Kelly Haston). NASA/CHAPEA Crew Inside the habitat, the CHAPEA mission 1 crew harvested tomatoes.NASA/CHAPEA Crew Explore More 2 min read First NASA Mars Analog Crew Passes Mission Halfway Mark Article 3 months ago 3 min read NASA Mars Analog Crew to Test Food Systems, Crop Growth Article 9 months ago 1 min read First CHAPEA Crew Begins 378-Day Mission Article 10 months agoNASA’s CloudSat Ends Mission Peering Into the Heart of Clouds
Over the course of nearly two decades, its powerful radar provided never-before-seen details of clouds and helped advance global weather and climate predictions.
CloudSat, a NASA mission that peered into hurricanes, tallied global snowfall rates, and achieved other weather and climate firsts, has ended its operations. Originally proposed as a 22-month mission, the spacecraft was recently decommissioned after almost 18 years observing the vertical structure and ice/water content of clouds.
As planned, the spacecraft — having reached the end of its lifespan and no longer able to make regular observations — was lowered into an orbit last month that will result in its eventual disintegration in the atmosphere.
When launched in 2006, the mission’s Cloud Profiling Radar was the first-ever 94 GHz wavelength (W-band) radar to fly in space. A thousand times more sensitive than typical ground-based weather radars, it yielded a new vision of clouds — not as flat images on a screen but as 3D slices of atmosphere bristling with ice and rain.
For the first time, scientists could observe clouds and precipitation together, said Graeme Stephens, the mission’s principal investigator at NASA’s Jet Propulsion Laboratory in Southern California. “Without clouds, humans wouldn’t exist, because they provide the freshwater that life as we know it requires,” he said. “We sometimes refer to them as clever little devils because of their confounding properties. Clouds have been an enigma in terms of predicting climate change.”
NASA’s CloudSat passed over Hurricane Bill near the U.S. East Coast in August 2009, capturing data from the Category 4 storm’s eye. This pair of images shows a view from the agency’s Aqua satellite (top) along with the vertical structure of the clouds measured by CloudSat’s radar (bottom).Jesse Allen, NASA Earth ObservatoryClouds have long held many secrets. Before CloudSat, we didn’t know how often clouds produce rain and snow on a global basis. Since its launch, we’ve also come a long way in understanding how clouds are able to cool and heat the atmosphere and surface, as well as how they can cause aircraft icing.
CloudSat data has informed thousands of research publications and continues to help scientists make key discoveries, including how much ice and water clouds contain globally and how, by trapping heat in the atmosphere, clouds accelerate the melting of ice in Greenland and at the poles.
Weathering the StormOver the years, CloudSat flew over powerful storm systems with names like Maria, Harvey, and Sandy, peeking beneath their swirling canopies of cirrus clouds. Its Cloud Profiling Radar excelled at penetrating cloud layers to help scientists explore how and why tropical cyclones intensify.
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In this animation, CloudSat’s radar slices into Hurricane Maria as it rapidly intensifies in the Atlantic Ocean in September 2017. Areas of high reflectivity, shown in red and pink, extend above 9 miles (15 kilometers) in height, indicating large amounts of water being drawn upward high into the atmosphere. Credit: NASA/JPL-Caltech/CIRAAcross the life of CloudSat, several potentially mission-ending issues occurred related to the spacecraft’s battery and to the reaction wheels used to control the satellite’s orientation. The CloudSat team developed unique solutions, including “hibernating” the spacecraft during nondaylight portions of each orbit to conserve power, and orienting it with fewer reaction wheels. Their solutions allowed operations to continue until the Cloud Profiling Radar was permanently turned off in December 2023.
“It’s part of who we are as a NASA family that we have dedicated and talented teams that can do things that have never before been done,” said Deborah Vane, CloudSat’s project manager at JPL. “We recovered from these anomalies with techniques that no one has ever used before.”
Sister SatellitesCloudSat was launched on April 28, 2006, in tandem with a lidar-carrying satellite called CALIPSO (short for the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation). The two spacecraft joined an international constellation of weather- and climate-tracking satellites in Earth orbit.
Radar and lidar are considered “active” sensors because they direct beams of energy at Earth — radio waves in the case of CloudSat and laser light in the case of CALIPSO — and measure how the beams reflect off the clouds and fine particles (aerosols) in the atmosphere. Other orbiting science instruments use “passive” sensors that measure reflected sunlight or radiation emitted from Earth or clouds.
Orbiting less than a minute apart, CloudSat and CALIPSO circled the globe in Sun-synchronous orbits from the North to the South Pole, crossing the equator in the early afternoon and after midnight every day. Their overlapping radar-lidar footprint cut through the vertical structure of the atmosphere to study thin and thick clouds, as well as the layers of airborne particles such as dust, sea salt, ash, and soot that can influence cloud formation.
The influence of aerosols on clouds remains a key question for global warming projections. To explore this and other questions, the recently launched PACE satellite and future missions in NASA’s Earth System Observatory will build upon CloudSat’s and CALIPSO’s legacies for a new generation.
“Earth in 2030 will be different than Earth in 2000,” Stephens said. “The world has changed, and the climate has changed. Continuing these measurements will give us new insights into changing weather patterns.”
More About the MissionsThe CloudSat Project is managed for NASA by JPL. JPL developed the Cloud Profiling Radar instrument with important hardware contributions from the Canadian Space Agency. Colorado State University provides science data processing and distribution. BAE Systems of Broomfield, Colorado, designed and built the spacecraft. The U.S. Space Force and U.S. Department of Energy contributed resources. U.S. and international universities and research centers support the mission science team. Caltech in Pasadena, California, manages JPL for NASA.
CALIPSO, which was a joint mission between NASA and the French space agency, CNES (Centre National d’Études Spatiales), ended its mission in August 2023.
News Media ContactsJane J. Lee / Andrew Wang
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-0307 / 626-379-6874
jane.j.lee@jpl.nasa.gov / andrew.wang@jpl.nasa.gov
Written by Sally Younger
2024-048
Share Details Last Updated Apr 23, 2024 Related Terms Explore More 3 min read NASA Data Helps Beavers Build Back Streams Article 4 days ago 6 min read NASA Selects New Aircraft-Driven Studies of Earth and Climate ChangeNASA has selected six new airborne missions that include domestic and international studies of fire-induced…
Article 4 days ago 4 min read Students Celebrate Rockets, Environment at NASA’s Kennedy Space Center Article 4 days agoHubble Spots the Little Dumbbell Nebula
To celebrate the 34th anniversary of the Hubble Space Telescope’s launch, the telescope captured an image of the Little Dumbbell Nebula, or M76. M76 is a planetary nebula, an expanding shell of glowing gases that were ejected from a dying red giant star that eventually collapses to an ultra-dense and hot white dwarf. It gets its descriptive name from its shape: a ring, seen edge-on as the central bar structure, and two lobes on either opening of the ring.
Since its launch in 1990 Hubble has made 1.6 million observations of over 53,000 astronomical objects. Most of Hubble’s discoveries were not anticipated before launch, such as supermassive black holes, the atmospheres of exoplanets, gravitational lensing by dark matter, the presence of dark energy, and the abundance of planet formation among stars.
Learn more about the Little Dumbbell Nebula and Hubble.
Image Credit: NASA, ESA, STScI
Explore the Universe with the First E-Book from NASA’s Fermi
4 min read
Explore the Universe with the First E-Book from NASA’s FermiTo commemorate a milestone anniversary for NASA’s Fermi spacecraft, the mission team has published an e-book called “Our High-Energy Universe: 15 Years with the Fermi Gamma-ray Space Telescope.”
Readers can download the e-book in PDF and EPUB formats. The e-book is aimed at general audiences with an interest in space.
Cover for the e-book “Our High-Energy Universe: 15 Years with the Fermi Gamma-ray Space Telescope.” NASA PDFApr 22, 2024
PDF (44.03 MB)
EPUB
Apr 22, 2024
EPUB+ZIP (804.49 MB)
Launched on June 11, 2008, Fermi detects gamma rays, the highest-energy form of light, from Earth’s atmosphere to far-flung galaxies and cosmic phenomena in between. Its research has uncovered details on topics ranging from solar flares to star formation and the mysteries at the center of our Milky Way.
Through images, fun facts, and launch-day memories, the e-book tells Fermi’s story from conceptualization to launch and recounts some of the mission’s groundbreaking discoveries. By delving into high-energy astrophysics topics like gamma-ray bursts and blazars, readers can explore Fermi’s universe and what questions remain open for investigation in its next chapter.
Fermi was originally called the Gamma-ray Large Area Space Telescope but was renamed after Italian physicist Enrico Fermi in August 2008.
“Enrico Fermi’s science has been important for understanding the sources that the Fermi telescope sees,” said Elizabeth Hays, the mission’s project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “The gamma-ray sky is powered by particle acceleration mechanisms he theorized about.”
The satellite has two gamma-ray detectors: the Large Area Telescope (LAT) and the Gamma-ray Burst Monitor (GBM).
The LAT observes a fifth of the gamma-ray sky at any time, detecting high-energy light with energies ranging from 20 million to over 300 billion electron volts. (The energy of visible light is 2 to 3 electron volts.) The GBM views about 70% of the sky at a time at lower energies, searching for brief flashes of gamma-ray light.
The result of this carefully crafted duo is the most sensitive gamma-ray observatory in orbit, equipped to study the universe’s highest-energy phenomena near and far.
By peering through Fermi’s gamma-ray eyes, we can better understand our solar system. Within its first eight years of operation, Fermi detected gamma-ray emissions from 40 solar flares — bursts of energy from the Sun. Some even originated on the Sun’s far side, allowing scientists to analyze how charged particles fired by solar flares can arc from one side of the Sun to produce gamma rays on the other.
In studying our Milky Way, Fermi found two lobes of high-energy gamma rays — called the Fermi Bubbles — extending above and below the galaxy’s center. Each bubble stands 25,000 light-years tall. Astronomers think the bubbles formed following an ancient burst of activity from the Milky Way’s central supermassive black hole.
Fermi helps scientists understand black holes in other galaxies, too.
“As a black hole forms, either from the death of a massive star or the collision of two neutron stars, it creates a brief flash of light called a gamma-ray burst,” said Judith Racusin, Fermi’s deputy project scientist at Goddard. “Fermi detects about one burst a day and has helped revolutionize our understanding of these phenomena.”
Even after 15 years of accomplishments, however, many mysteries remain for Fermi to tackle. One of the telescope’s ongoing objectives is to study the composition of dark matter — the mysterious substance that makes up about 25% of the universe.
Because dark matter doesn’t reflect, absorb, or emit light, scientists remain unsure of its composition. One popular theory suggests, though, that dark matter particles create gamma rays when they interact. If Fermi can spot this high-energy signature, it might help scientists learn more about dark matter’s makeup.
If there’s one thing Fermi has taught us, it’s to expect the unexpected. Gamma-ray research has yielded unprecedented breakthroughs in our understanding of the Milky Way’s central black hole, our flaring Sun, and merging neutron stars. As much as we anticipate the next gamma-ray revelation, only time will tell what exactly Fermi has in store.
Fermi is an astrophysics and particle physics partnership managed by Goddard. Fermi was developed in collaboration with the U.S. Department of Energy, with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the United States.
By Jenna Ahart
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Media Contact:
Claire Andreoli
301-286-1940
claire.andreoli@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Hubble Celebrates 34th Anniversary with a Look at the Little Dumbbell Nebula
5 min read
Hubble Celebrates 34th Anniversary with a Look at the Little Dumbbell NebulaIn celebration of the 34th anniversary of the launch of NASA’s legendary Hubble Space Telescope on April 24, astronomers took a snapshot of the Little Dumbbell Nebula (also known as Messier 76, M76, or NGC 650/651) located 3,400 light-years away in the northern circumpolar constellation Perseus. The photogenic nebula is a favorite target of amateur astronomers.
In celebration of the 34th anniversary of the launch of NASA’s legendary Hubble Space Telescope, astronomers took a snapshot of the Little Dumbbell Nebula, also known as Messier 76, or M76, located 3,400 light-years away in the northern circumpolar constellation Perseus. The name ‘Little Dumbbell’ comes from its shape that is a two-lobed structure of colorful, mottled, glowing gases resembling a balloon that’s been pinched around a middle waist. Like an inflating balloon, the lobes are expanding into space from a dying star seen as a white dot in the center. Blistering ultraviolet radiation from the super-hot star is causing the gases to glow. The red color is from nitrogen, and blue is from oxygen. NASA, ESA, STScIDownload this image (3MB)
Download this image (33MB)
M76 is classified as a planetary nebula, an expanding shell of glowing gases that were ejected from a dying red giant star. The star eventually collapses to an ultra-dense and hot white dwarf. A planetary nebula is unrelated to planets, but have that name because astronomers in the 1700s using low-power telescopes thought this type of object resembled a planet.
M76 is composed of a ring, seen edge-on as the central bar structure, and two lobes on either opening of the ring. Before the star burned out, it ejected the ring of gas and dust. The ring was probably sculpted by the effects of the star that once had a binary companion star. This sloughed off material created a thick disk of dust and gas along the plane of the companion’s orbit. The hypothetical companion star isn’t seen in the Hubble image, and so it could have been later swallowed by the central star. The disk would be forensic evidence for that stellar cannibalism.
The primary star is collapsing to form a white dwarf. It is one of the hottest stellar remnants known at a scorching 250,000 degrees Fahrenheit, 24 times our Sun’s surface temperature. The sizzling white dwarf can be seen as a pinpoint in the center of the nebula. A star visible in projection beneath it is not part of the nebula.
Pinched off by the disk, two lobes of hot gas are escaping from the top and bottom of the “belt,” along the star’s rotation axis that is perpendicular to the disk. They are being propelled by the hurricane-like outflow of material from the dying star, tearing across space at two million miles per hour. That’s fast enough to travel from Earth to the Moon in a little over seven minutes! This torrential “stellar wind” is plowing into cooler, slower-moving gas that was ejected at an earlier stage in the star’s life, when it was a red giant. Ferocious ultraviolet radiation from the super-hot star is causing the gases to glow. The red color is from nitrogen, and blue is from oxygen.
Given our solar system is 4.6 billion years old, the entire nebula is a flash in the pan by cosmological timekeeping. It will vanish in about 15,000 years.
Hubble’s Star Trekking
Since its launch in 1990 Hubble has made 1.6 million observations of over 53,000 astronomical objects. To date, the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute in Baltimore, Maryland holds 184 terabytes of processed data that is science-ready for astronomers around the world to use for research and analysis. Since 1990, 44,000 science papers have been published from Hubble observations. The space telescope is the most scientifically productive space astrophysics mission in NASA history. The demand for using Hubble is so high it is currently oversubscribed by a factor of six-to-one.
Most of Hubble’s discoveries were not anticipated before launch, such as supermassive black holes, the atmospheres of exoplanets, gravitational lensing by dark matter, the presence of dark energy, and the abundance of planet formation among stars.
Hubble will continue research in those domains and capitalize on its unique ultraviolet-light capability on such topics as solar system phenomena, supernovae outbursts, composition of exoplanet atmospheres, and dynamic emission from galaxies. And Hubble investigations continue to benefit from its long baseline of observations of solar system objects, stellar variable phenomena and other exotic astrophysics of the cosmos.
NASA’s James Webb Space Telescope was designed to be meant to be complementary to Hubble, and not a substitute. Future Hubble research also will take advantage of the opportunity for synergies with Webb, which observes the universe in infrared light. The combined wavelength coverage of the two space telescopes expands on groundbreaking research in such areas as protostellar disks, exoplanet composition, unusual supernovae, cores of galaxies and chemistry of the distant universe.
Hubble’s Senior Project Scientist Dr. Jennifer Wiseman takes us on a tour of this stunning new image, describes the telescope’s current health, and summarizes some of Hubble’s contributions to astronomy during its 34-year career.Credit: NASA’s Goddard Space Flight Center; Lead Producer: Paul Morris
The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, Colorado, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, Maryland, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.
Media Contact:
Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov
Ray Villard
Space Telescope Science Institute, Baltimore, MD
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
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Pushing the Limits of Sub-Kilowatt Electric Propulsion Technology to Enable Planetary Exploration and Commercial Mission Concepts
NASA has developed an advanced propulsion technology to facilitate future planetary exploration missions using small spacecraft. Not only will this technology enable new types of planetary science missions, one of NASA’s commercial partners is already preparing to use it for another purpose—to extend the lifetimes of spacecraft that are already in orbit. Identifying the opportunity for industry to use this new technology not only advances NASA’s goal of technology commercialization, it could potentially create a path for NASA to acquire this important technology from industry for use in future planetary missions.
The New TechnologyPlanetary science missions using small spacecraft will be required to perform challenging propulsive maneuvers—such as achieving planetary escape velocities, orbit capture, and more—that require a velocity change (delta-v) capability well in excess of typical commercial needs and the current state-of-the-art. Therefore, the #1 enabling technology for these small spacecraft missions is an electric propulsion system that can execute these high-delta-v maneuvers. The propulsion system must operate using low power (sub-kilowatt) and have high-propellant throughput (i.e., the capability to use a high total mass of propellant over its lifetime) to enable the impulse required to execute these maneuvers.
After many years of research and development, researchers at NASA Glenn Research Center (GRC) have created a small spacecraft electric propulsion system to meet these needs—the NASA-H71M sub-kilowatt Hall-effect thruster. In addition, the successful commercialization of this new thruster will soon provide at least one such solution to enable the next generation of small spacecraft science missions requiring up to an amazing 8 km/s of delta-v. This technical feat was accomplished by the miniaturization of many advanced high-power solar electric propulsion technologies developed over the last decade for applications such as the Power and Propulsion Element of Gateway, humanity’s first space station around the Moon.
Left: NASA-H71M Hall-effect thruster on the Glenn Research Center Vacuum Facility 8 thrust stand. Right: Dr. Jonathan Mackey tuning the thrust stand prior to closing and pumping down the test facility. Benefits of This Technology for Planetary ExplorationSmall spacecraft using the NASA-H71M electric propulsion technology will be able to independently maneuver from low-Earth orbit (LEO) to the Moon or even from a geosynchronous transfer orbit (GTO) to Mars. This capability is especially remarkable because commercial launch opportunities to LEO and GTO have become routine, and the excess launch capacity of such missions is often sold at low cost to deploy secondary spacecraft. The ability to conduct missions that originate from these near-Earth orbits can greatly increase the cadence and lower the cost of lunar and Mars science missions.
This propulsion capability will also increase the reach of secondary spacecraft, which have been historically limited to scientific targets that align with the primary mission’s launch trajectory. This new technology will enable secondary missions to substantially deviate from the primary mission’s trajectory, which will facilitate exploration of a wider range of scientific targets.
In addition, these secondary spacecraft science missions would typically have only a short period of time to collect data during a high-speed flyby of a distant body. This greater propulsive capability will allow deceleration and orbital insertion at planetoids for long-term scientific study.
Furthermore, small spacecraft outfitted with such significant propulsive capability will be better equipped to manage late-stage changes to the primary mission’s launch trajectory. Such changes are frequently a top risk for small spacecraft science missions with limited onboard propulsive capability that depend on the initial launch trajectory to reach their science target.
Commercial ApplicationsThe megaconstellations of small spacecraft now forming in low-Earth orbits have made low-power Hall-effect thrusters the most abundant electric propulsion system used in space today. These systems use propellant very efficiently, which allows for orbit insertion, de-orbiting, and many years of collision avoidance and re-phasing. However, the cost-conscious design of these commercial electric propulsion systems has inevitably limited their lifetime capability to typically less than a few thousand hours of operation and these systems can only process about 10% or less of a small spacecraft’s initial mass in propellant.
By contrast, planetary science missions benefiting from the NASA-H71M electric propulsion system technology could operate for 15,000 hours and process over 30% of the small spacecraft’s initial mass in propellant. This game-changing capability is well beyond the needs of most commercial LEO missions and comes at a cost premium that makes commercialization for such applications unlikely. Therefore, NASA sought and continues to seek partnerships with companies developing innovative commercial small spacecraft mission concepts with unusually large propellant throughput requirements.
One partner that will soon use the licensed NASA electric propulsion technology in a commercial small spacecraft application is SpaceLogistics, a wholly owned subsidiary of Northrop Grumman. The Mission Extension Pod (MEP) satellite servicing vehicle is equipped with a pair of Northrop Grumman NGHT-1X Hall-effect thrusters, whose design is based on the NASA-H71M. The small spacecraft’s large propulsive capability will allow it to reach geosynchronous Earth orbit (GEO) where it will be mounted on a far larger satellite. Once installed, the MEP will serve as a “propulsion jet pack” to extend the life of its host spacecraft for at least six years.
Northrop Grumman is currently conducting a long duration wear test (LDWT) of the NGHT-1X in GRC’s Vacuum Facility 11 to demonstrate its full lifetime operational capability. The LDWT is funded by Northrop Grumman through a fully reimbursable Space Act Agreement. The first MEP spacecraft are expected to launch in 2025, where they will extend the life of three GEO communication satellites.
Collaborating with U.S. industry to find small spacecraft applications with propulsive requirements similar to future NASA planetary science missions not only supports U.S. industry in remaining a global leader in commercial space systems but creates new commercial opportunities for NASA to acquire these important technologies as planetary missions require them.
Northrop Grumman NGHT-1X engineering model Hall-effect thruster operating in Glenn Research Center Vacuum Facility 8. The design of the NGHT-1X is based on the NASA-H71M Hall-effect thruster. Credit: Northrop GrummanNASA continues to mature the H71M electric propulsion technologies to expand the range of data and documentation available to U.S. industry for the purpose of developing similarly advanced and highly capable low-power electric propulsion devices.
Project LeadDr. Gabriel F. Benavides, NASA Glenn Research Center (GRC)
Sponsoring OrganizationsPlanetary Science Division – Planetary Exploration Science Technology Office (PESTO); Space Operations Mission Directorate – Commercial Space Capabilities Office (CSCO); Space Technology Mission Directorate – Game Changing Development (GCD) program; Space Technology Mission Directorate – Small Spacecraft Technology (SST) program
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Sols 4161-4163: Double Contact Science
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Sols 4161-4163: Double Contact Science This image was taken by Mast Camera (Mastcam) onboard NASA’s Mars rover Curiosity on Sol 4159 (2024-04-18 13:24:29 UTC). NASA/JPL-Caltech/MSSSEarth planning date: Friday, April 19, 2024
Curiosity has a three-sol weekend plan coming up as it makes progress along the edge of upper Gediz Vallis ridge. We have observations planned to investigate multiple bedrock targets with interesting rippled textures, dark-toned float, and the ridge. With two contact science targets, lots of targeted and untargeted remote observations, and a drive scheduled, Curiosity will have a busy three-sol plan ahead!
On the first sol of the plan, we have two contact science bedrock targets for MAHLI and APXS to analyze. MAHLI will image these targets up close, and APXS will acquire spectra from the targets for analysis of their elemental compositions. One of these bedrock targets (“Florence Lake”) is light-toned with laminations and will be brushed first to remove the dust on its surface. The other contact science target (“Mist Falls”) is a block of unbrushed, light-toned bedrock with a rippled texture. MAHLI also has a rotational stereo observation of “Castle Rock Spire” (a light-toned block of bedrock) and observations of the REMS UV sensor. In addition to bedrock observations by MAHLI and APXS, ChemCam has a LIBS observation of dark-toned float target “Silver Peak” on the first sol of this plan. ChemCam will also acquire long-distance RMIs of the rim of upper Gediz Vallis ridge and Fascination Turret to document stratigraphy. Mastcam will acquire mosaics to document exposed bedding, Kukenan butte, and Pinnacle Ridge.
Observations of Pinnacle Ridge by Mastcam will complement the ChemCam long-distance RMI observation of it on the second sol of the plan. This sol also has a ChemCam LIBS observation of “Needle Lake” to document different degrees of erosion of bedrock across laminations and a ChemCam passive dark test. Mastcam will image the two LIBS targets and will also acquire several mosaics of “Pahoa Island”, “Quail Flat”, and “The Nose” to document light-toned laminated bedrock, ripple structures, and characteristics of a dark float rock, respectively. On the second sol Curiosity will drive away. The third sol of the plan features untargeted remote observations, including ChemCam Passive Sky activities, dust devil observations, and Mastcam tau measurements.
Written by Abigail Knight, Graduate Student at Washington University
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NASA Astronaut to Inspire Artemis Generation in Boston
April 22, 2024
NASA astronaut Stephen Bowen, along with representatives from NASA and the International Space Station National Laboratory, will visit Boston on Wednesday, April 24, and Thursday, April 25, as part of the agency’s Destination Station to highlight research opportunities aboard the station.
Destination Station was created to educate the public and engage prospective researchers about the benefits, capabilities, and opportunities to use the space station. The space station has been continuously inhabited for more than 23 years, enabling more than 5,000 researchers to conduct more than 3,500 innovative experiments in the areas of biology and biotechnology, human health, space and physical science, and technology.
Throughout the week, NASA and the ISS National Lab will meet with a variety of academic institutions, business incubators, and private-sector companies with ties to the Boston community. During the visits, Bowen will provide perspectives on living and working in space.
Media who wish interview Bowen during the outreach events in Boston, should contact Kara Slaughter at kara.c.slaughter@nasa.gov or 281-483-5111.
Bowen was the first submarine officer selected to be a NASA astronaut. He most recently served as commander of NASA’s SpaceX Crew-6 mission to the station where he was part of a six-month research mission, Expedition 69. He is a veteran of three space shuttle flights to the station, including STS-126, STS-132, and STS-133. Bowen has logged a total of 227 days in space and conducted 10 extravehicular activities in his career. His 10 spacewalks make him one of five humans who have conducted that many spacewalks and he is third on the all-time list for most cumulative spacewalking time. Bowen and the crews of Expedition 68 and 69 conducted more than 200 science experiments including tissue chip research, bioprinting human cells and tissues in space, and studying antibodies in microgravity. Bowen is a Massachusetts native and earned his bachelor’s degree from the United States Naval Academy in Annapolis, Maryland, and his master’s degree from the Massachusetts Institute of Technology in Cambridge.
Over the years, NASA’s Destination Station has led to research collaborations aboard the orbiting laboratory with a variety of academic and commercial companies. This visit also is a prelude to the 13th annual International Space Station Research and Development Conference at the Boston Marriott Copley Square from July 29 – Aug. 1, 2024.
Learn more about the International Space Station and its crews at:
Discover the International Space Station U.S. National Laboratory at:
https://www.issnationallab.org
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Kara Slaughter
Johnson Space Center, Houston
281-483-5111
NASA Invites Media to Learn About New Tech Mission Powered by the Sun
A new NASA mission is testing a new way to navigate our solar system by hoisting its sail into space – not to catch the wind, but the propulsive power of sunlight.
NASA’s Advanced Composite Solar Sail System is led by the agency’s Ames Research Center in California’s Silicon Valley. The microwave oven-sized CubeSat is scheduled to launch aboard a Rocket Lab Electron rocket from the company’s Launch Complex 1 on the Mahia Peninsula of New Zealand. The launch window opens at 3 p.m. PDT on Tuesday, April 23 (10 p.m. UTC). Successful deployment and operation of the solar sail’s lightweight composite booms will prove the capability and open the door to larger scale missions to the Moon, Mars, and beyond.
Once it arrives in its orbit, roughly 600 miles above Earth, the CubeSat will deploy a lightweight sunlight-powered composite solar sail system that measures more than 800 square feet. Much like a sailboat uses wind to traverse the ocean, the solar sail technology will use the pressure of sunlight to travel through space and perform a series of maneuvers to demonstrate orbit raising and lowering. Throughout the demonstration, the spacecraft may be visible to the naked eye in the night sky.
Media interested in scheduling an interview with one of the NASA Ames engineers involved with the development of the CubeSat should email the NASA Ames Office of Communications at arc-dl-newsroom@mail.nasa.gov.
A media resource reel including animated clips of the solar sail system is available here.
Get launch updates, breaking news, and images on the small satellites blog as well as NASA Ames’ Instagram, Facebook, and X.
For more information about NASA’s Ames Research Center, visit:
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Rachel Hoover
Ames Research Center, Silicon Valley, Calif.
650-604-4789
NASA Announces 30th Human Exploration Rover Challenge Winners
NASA announced the winners of the 30th Human Exploration Rover Challenge (HERC) April 22, with Parish Episcopal School, from Dallas, winning first place in the high school division, and the University of Alabama in Huntsville, capturing the college/university title.
The annual engineering competition – one of NASA’s longest standing challenges – held its concluding event April 19 and April 20, at the U.S. Space & Rocket Center in Huntsville, Alabama, near NASA’s Marshall Space Flight Center. The complete list of 2024 award winners is provided below:
High School Division
- First Place: Parish Episcopal School, Dallas
- Second Place: Academy of Arts, Careers and Technology, Reno, Nevada
- Third Place: Escambia High School, Pensacola, Florida
College/University Division
- First Place: University of Alabama in Huntsville
- Second Place: Instituto Tecnológico de Santo Domingo, Dominican Republic
- Third Place: Campbell University, Buies Creek, North Carolina
Ingenuity Award
- University of West Florida, Pensacola, Florida
Phoenix Award
- High School Division: East Central High School, Moss Point, Mississippi
- College/University Division: North Dakota State University, Fargo, North Dakota
Task Challenge Award
- High School Division: Erie High School, Erie, Colorado
- College/University Division: South Dakota School of Mines and Technology, Rapid City, South Dakota
Project Review Award
- High School Division: Parish Episcopal School, Dallas
- College/University Division: University of Alabama in Huntsville
Featherweight Award
- Rhode Island School of Design, Providence, Rhode Island
Safety Award
- High School Division: NPS International School, Singapore
- College/University Division: Instituto Especializado de Estudios Superiores Loyola, San Cristobal, Dominican Republic
Crash and Burn Award
- KIET Group of Institutions, Delhi-NCR, India
Jeff Norris and Joe Sexton Memorial Pit Crew Award
- High School Division: Erie High School, Erie, Colorado
- College/University Division: Campbell University, Buies Creek, North Carolina
Team Spirit Award
- Instituto Tecnológico de Santo Domingo, Dominican Republic
Most Improved Performance Award
- High School Division: Jesco von Puttkamer School, Leipzig, Germany
- College/University Division: Universidad Católica Boliviana – San Pablo, La Paz, Bolivia
Social Media Award
- High School Division: Bledsoe County High School, Pikeville, Tennessee
- College/University Division: Universidad de Piura, Peru
STEM Engagement Award
- High School Division: Princess Margaret Secondary School, Surrey, British Columbia
- College/University Division: Trine University, Angola, Indiana
Artemis Educator Award
- Sadif Safarov from Istanbul Technical University, Turkey
Rookie of the Year
- Kanakia International School, Mumbai, India
More than 600 students with 72 teams from around the world participated as HERC celebrated its 30th anniversary as a NASA competition. Participating teams represented 42 colleges and universities and 30 high schools from 24 states, the District of Columbia, Puerto Rico, and 13 other nations from around the world. Teams were awarded points based on navigating a half-mile obstacle course, conducting mission-specific task challenges, and completing multiple safety and design reviews with NASA engineers.
“This student design challenge encourages the next generation of scientists and engineers to engage in the design process by providing innovative concepts and unique perspectives,” said Vemitra Alexander, HERC activity lead for NASA’s Office of STEM Engagement at Marshall. “While celebrating the 30th anniversary of the challenge, HERC also continues NASA’s legacy of providing valuable experiences to students who may be responsible for planning future space missions including crewed missions to other worlds.”
HERC is one of NASA’s eight Artemis Student Challenges reflecting the goals of the Artemis program, which seeks to land the first woman and first person of color on the Moon while establishing a long-term presence for science and exploration. NASA uses such challenges to encourage students to pursue degrees and careers in the fields of science, technology, engineering, and mathematics.
HERC is managed by NASA’s Southeast Regional Office of STEM Engagement at Marshall. Since its inception in 1994, more than 15,000 students have participated in HERC – with many former students now working at NASA, or within the aerospace industry.
To learn more about HERC, please visit:
https://www.nasa.gov/roverchallenge/home/index.html
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Gerelle Dodson
NASA Headquarters, Washington
202-358-4637
gerelle.q.dodson@nasa.gov
Taylor Goodwin
Marshall Space Flight Center, Huntsville, Ala.
256-544-0034
taylor.goodwin@nasa.gov
NASA Nurtures Promising Tech Ideas from Small Businesses
New space technology ideas emerge every day from innovators across the country, and NASA’s Small Business Innovation Research (SBIR) program on Monday selected more than 100 projects for funding. This program offers small businesses in the United States early-stage funding and support to advance the agency’s goals of exploring the unknown in air and space while returning benefits to Earth.
Specifically, NASA’s SBIR program awarded $93.5 million in Phase II contracts to bring 107 new ideas to life from 95 selected small businesses. Of these businesses, nearly 80% have less than 50 employees, and 21% are receiving their first Phase II award, valued at up to $850,000 each. Each small business was also eligible to apply for up to $50,000 in Technical and Business Assistance program funding to help find new market opportunities and shape their commercialization roadmap.
“We are thrilled to support this diverse set of companies as they work diligently to bring their technologies to market,” said Jenn Gustetic, director of Early Stage Innovation and Partnerships with NASA’s Space Technology Mission Directorate (STMD) at the agency’s headquarters in Washington. “Inclusive innovation is integral to mission success at NASA, and we’re excited to see that 29% of the awardees are from underrepresented groups, including 11% women-owned businesses.”
In Phase II, awardees will build on their success from the program’s first phase to bring their technologies closer to real-world use. The companies have 24 months to execute their plans, which focus on their technologies’ path to commercialization.
For example, NASA selected women-owned and first-time NASA Phase II awardee nou Systems, Inc. in Huntsville, Alabama, for its genetic testing instrument. While portable genetic sequencing already exists, field sequencing – that would allow DNA analysis anywhere on Earth or off planet – remains unfeasible as the preparation of the DNA Library remains an intensely manual process, needing a trained wet lab technician and several pieces of laboratory equipment. The Phase II technology takes advantage of several cross-enabling technologies, creating an instrument to automate the genetic sequencing process.
“Our program works directly with small businesses to forge innovative concepts and technologies that drive impact for NASA projects as well as a myriad of commercial endeavors,” said Jason L. Kessler, program executive for NASA’s SBIR and Small Business Technology Transfer (STTR) program at NASA Headquarters. “This collaboration results in realized opportunities not only for NASA but all of humanity.”
This includes technologies aiming to reduce astronaut workload and improve robotic scientific endeavors on the Moon and Mars. PickNik Inc. based in Boulder, Colorado, will use its Phase II award to continue developing a hardware-agnostic platform for supervised autonomy that empowers humans to command a remote robot to complete complex tasks with minimal input, which could support the Artemis program. Outside of NASA, PickNik’s software product may be of interest to commercial space customers working on low Earth orbit destinations, in-space servicing, and more, as well as on Earth in areas like warehouse management, oil rig maintenance, and deep-sea exploration.
The NASA SBIR program is open to U.S. small businesses to develop an innovation or technology. The program is part of STMD and managed by NASA’s Ames Research Center in California’s Silicon Valley.
To learn more about the NASA SBIR program, visit:
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Jimi Russell
Headquarters, Washington
james.j.russell@nasa.gov
202-358-1600
Our Beautiful Water World
This Jan. 30, 2012 image of Earth was created from photographs taken by the Visible/Infrared Imager Radiometer Suite (VIIRS) instrument aboard the Suomi NPP satellite. Many features of North America and the Western Hemisphere are particularly visible. The composite was created from the data collected during four orbits of the robotic satellite taken earlier in January 2012 and digitally projected onto the globe.
VIIRS collects visible and infrared imagery along with global observations of Earth’s land, atmosphere, cryosphere, and ocean, extending observational records collected by similar instruments aboard previously launched satellites, such as NASA’s Moderate Resolution Imaging Spectroradiometer (MODIS) and NOAA’s Advanced Very High Resolution Radiometer (AVHRR).
Help us celebrate Earth Day by sharing a #GlobalSelfie.
Image Credit: NASA
‘Vast and Rich:’ Studying the Ocean With NASA Computer Simulations
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A tool developed at NASA’s Advanced Supercomputing division provides researchers with a global view of their ocean simulation in high resolution. In this part of the global visualization, the Gulf Stream features prominently. Surface water speeds are shown ranging from 0 meters per second (dark blue) to 1.25 meters (about 4 feet) per second (cyan). The video is running at one simulation day per second. The data used comes from the Estimating the Circulation and Climate of the Ocean (ECCO) consortium. Credits: NASA/Bron Nelson, David Ellsworth“Every time I help with visualizing [ocean] simulation data, I learn about an entirely new area of ocean or climate research, and I’m reminded of how vast and rich this area of research is. And…the real magic happens at the intersection and interaction of simulated and observed data.
It is a great honor – and a thrill – to collaborate with devoted, world-class scientists doing such important, cutting-edge research and sometimes to even help them learn something new about their science.”
Dr. Nina McCurdy
Data visualization scientist with the NASA Advanced Supercomputing division at NASA’s Ames Research Center in California’s Silicon Valley
This Earth Day, learn more about the work of Nina and other Ames researchers studying our planet: Celebrating Our Ocean World at NASA in Silicon Valley.
Why is Methane Seeping on Mars? NASA Scientists Have New Ideas
Maksym Bocharov
The most surprising revelation from NASA’s Curiosity Mars Rover — that methane is seeping from the surface of Gale Crater — has scientists scratching their heads.
Living creatures produce most of the methane on Earth. But scientists haven’t found convincing signs of current or ancient life on Mars, and thus didn’t expect to find methane there. Yet, the portable chemistry lab aboard Curiosity, known as SAM, or Sample Analysis at Mars, has continually sniffed out traces of the gas near the surface of Gale Crater, the only place on the surface of Mars where methane has been detected thus far. Its likely source, scientists assume, are geological mechanisms that involve water and rocks deep underground.
If that were the whole story, things would be easy. However, SAM has found that methane behaves in unexpected ways in Gale Crater. It appears at night and disappears during the day. It fluctuates seasonally, and sometimes spikes to levels 40 times higher than usual. Surprisingly, the methane also isn’t accumulating in the atmosphere: ESA’s (the European Space Agency) ExoMars Trace Gas Orbiter, sent to Mars specifically to study the gas in the atmosphere, has detected no methane.
Why do some science instruments detect methane on the Red Planet while others don’t?
“It’s a story with a lot of plot twists,” said Ashwin Vasavada, Curiosity’s project scientist at NASA’s Jet Propulsion Laboratory in Southern California, which leads Curiosity’s mission.
Methane keeps Mars scientists busy with lab work and computer modeling projects that aim to explain why the gas behaves strangely and is detected only in Gale Crater. A NASA research group recently shared an interesting proposal.
Reporting in a March paper in the Journal of Geophysical Research: Planets, the group suggested that methane — no matter how it’s produced — could be sealed under solidified salt that might form in Martian regolith, which is “soil” made of broken rock and dust. When temperature rises during warmer seasons or times of day, weakening the seal, the methane could seep out.
Led by Alexander Pavlov, a planetary scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, the researchers suggest the gas also can erupt in puffs when seals crack under the pressure of, say, a rover the size of a small SUV driving over it. The team’s hypothesis may help explain why methane is detected only in Gale Crater, Pavlov said, given that’s it’s one of two places on Mars where a robot is roving and drilling the surface. (The other is Jezero Crater, where NASA’s Perseverance rover is working, though that rover doesn’t have a methane-detecting instrument.)
Pavlov traces the origin of this hypothesis to an unrelated experiment he led in 2017, which involved growing microorganisms in a simulated Martian permafrost (frozen soil) infused with salt, as much of Martian permafrost is.
Pavlov and his colleagues tested whether bacteria known as halophiles, which live in saltwater lakes and other salt-rich environments on Earth, could thrive in similar conditions on Mars.
The microbe-growing results proved inconclusive, he said, but the researchers noticed something unexpected: The top layer of soil formed a salt crust as salty ice sublimated, turning from a solid to a gas and leaving the salt behind.
Permafrost on Mars and Earth
“We didn’t think much of it at the moment,” Pavlov said, but he remembered the soil crust in 2019, when SAM’s tunable laser spectrometer detected a methane burst no one could explain.
“That’s when it clicked in my mind,” Pavlov said. And that’s when he and a team began testing the conditions that could form and crack hardened salt seals.
Pavlov’s team tested five samples of permafrost infused with varying concentrations of a salt called perchlorate that’s widespread on Mars. (There’s likely no permafrost in Gale Crater today, but the seals could have formed long ago when Gale was colder and icier.) The scientists exposed each sample to different temperatures and air pressure inside a Mars simulation chamber at NASA Goddard.
Periodically, Pavlov’s team injected neon, a methane analog, underneath the soil sample and measured the gas pressure below and above it. Higher pressure beneath the sample implied the gas was trapped. Ultimately, a seal formed under Mars-like conditions within three to 13 days only in samples with 5% to 10% perchlorate concentration.
This is a sample of mock Martian regolith, which is “soil” made of broken rock and dust. It’s one of five samples that scientists infused with varying concentrations of a salt called perchlorate that’s widespread on Mars. They exposed each sample to Mars-like conditions in the Mars simulation chamber at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The brittle clumps in the sample above show that a seal of salt did not form in this sample because the concentration of salt was too low. NASA/Alexander Pavlov This image is of another sample of mock Martian “soil” after it was removed from the Mars simulation chamber. The surface is sealed with a solid crust of salt. Alexander Pavlov and his team found that a seal formed after a sample spent three to 13 days under Mars-like conditions, and only if it had 5% to 10% perchlorate salt concentration. The color is lighter in the center where the sample was scratched with a metal pick. The light color indicates a drier soil underneath the top layer, which absorbed moisture from the air as soon as the sample was removed from the simulation chamber, turning brown. NASA/Alexander PavlovThat’s a much higher salt concentration than Curiosity has measured in Gale Crater. But regolith there is rich in a different type of salt minerals called sulfates, which Pavlov’s team wants to test next to see if they can also form seals.
Curiosity rover has arrived at a region believed to have formed as Mars’ climate was drying.
Improving our understanding of methane generation and destruction processes on Mars is a key recommendation from the 2022 NASA Planetary Mission Senior Review, and theoretical work like Pavlov’s is critical to this effort. However, scientists say they also need more consistent methane measurements.
SAM sniffs for methane only several times a year because it is otherwise busy doing its primary job of drilling samples from the surface and analyzing their chemical makeup.
In 2018, NASA announced that the Sample Analysis at Mars chemistry lab aboard the Curiosity Rover discovered ancient organic molecules that had been preserved in rocks for billions of years. Findings like this one help scientists understand the habitability of early Mars and pave the way for future missions to the Red Planet.Credit: NASA’s Goddard Space Flight Center
Download this video in HD formats from NASA Goddard’s Scientific Visualization Studio
“Methane experiments are resource intensive, so we have to be very strategic when we decide to do them,” said Goddard’s Charles Malespin, principal investigator for SAM.
Yet, to test how often methane levels spike, for instance, would require a new generation of surface instruments that measure methane continuously from many locations across Mars, scientists say.
“Some of the methane work will have to be left to future surface spacecraft that are more focused on answering these specific questions,” Vasavada said.
By Lonnie Shekhtman
NASA’s Goddard Space Flight Center, Greenbelt, Md.
NASA Sets Coverage of Roscosmos Spacewalk Outside Space Station
NASA will provide live coverage, beginning at 10:30 a.m. EDT Thursday, April 25, as two Roscosmos cosmonauts conduct a spacewalk outside the International Space Station. The spacewalk is expected to begin at 10:55 a.m. and could last up to seven hours.
NASA will stream the spacewalk on NASA+, NASA Television, the NASA app, YouTube, and the agency’s website. Learn how to stream NASA TV through a variety of platforms including social media.
Expedition 71 crewmates Oleg Kononenko and Nikolai Chub will venture outside the station’s Poisk airlock to complete the deployment of one panel on a synthetic radar system on the Nauka module.The two cosmonauts will also install equipment and experiments on the Poisk module to analyze the level of corrosion on station surfaces and modules.
The spacewalk will be the 270th in support of space station, and will be the seventh for Kononenko, who will wear the Orlan spacesuit with the red stripes, and the second for Chub, who will wear the spacesuit with the blue stripes.
Get breaking news, images, and features from the space station on the station blog, Instagram, Facebook, and X.
Learn more about International Space Station research and operations at:
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Joshua Finch / Claire O’Shea
Headquarters, Washington
202-358-1100
joshua.a.finch@nasa.gov / claire.a.o’shea@nasa.gov
Sandra Jones
Johnson Space Center, Houston
281-483-5111
sandra.p.jones@nasa.gov
Work Underway on Large Cargo Landers for NASA’s Artemis Moon Missions
Under NASA’s Artemis campaign, the agency and its partners will send large pieces of equipment to the lunar surface to enable long-term scientific exploration of the Moon for the benefit of all. NASA’s human landing system providers, SpaceX and Blue Origin, are beginning development of lunar landers for large cargo deliveries to support these needs.
NASA has contracted SpaceX and Blue Origin to provide landing systems to take astronauts to the Moon’s surface from lunar orbit, beginning with Artemis III. The agency has asked the two companies to develop cargo versions of their human lunar landers as an option under their existing contracts. These cargo variants are expected to land approximately 26,000 – 33,000 pounds (12 to 15 metric tons) of payload on the lunar surface and be in service no earlier than the Artemis VII mission.
“It’s essential that NASA has the capability to land not just astronauts, but large pieces of equipment, such as pressurized rovers, on the Moon for maximum return on science and exploration activities,” said Lisa Watson-Morgan, Human Landing System Program Manager at NASA’s Marshall Space Flight Center in Huntsville, Alabama. “Beginning this work now allows SpaceX and Blue Origin to leverage their respective human lander designs to provide cargo variants that NASA will need in the future.”
NASA expects the cargo versions of the companies’ landers to be modified versions of the human landing systems currently being developed for Artemis III, IV, and V. Modifications will include adjustments for payload interfaces and deployment mechanisms, and the cargo variants will not have human life support systems.
This initial work allows the companies to proceed with development for their cargo landers through a preliminary design review, the step that establishes the basis for proceeding with detailed design. SpaceX is conducting its work under the NextSTEP Appendix H contract, and Blue Origin is conducting its work under NextSTEP Appendix P. NASA officially exercised the options under those contracts in November 2023 to begin work on the large cargo landers.
With Artemis, NASA will explore more of the Moon than ever before, learn how to live and work away from home, and prepare for future human missions to the Red Planet. Artemis requires the best of international space agencies, private industry, and academia to establish the infrastructure for long-term scientific research and exploration. NASA’s SLS (Space Launch System) rocket, exploration ground systems, and Orion spacecraft, along with the human landing system, next-generation spacesuits and rovers, and Gateway lunar space station are the agency’s foundation for human exploration deep space.
For more information about Artemis, visit:
Slovenia Signs Artemis Accords, Joins Pursuit of Safer Space
NASA and Slovenia affirmed their cooperation in future space endeavors on Friday as Slovenia became the 39th country to sign the Artemis Accords. The signing certified Slovenia’s commitment to pursue safe and sustainable exploration of space for the benefit of humanity and took place during a U.S.-Slovenia strategic dialogue in Ljubljana, Slovenia, at the Ministry of Foreign Affairs Offices.
“NASA welcomes Slovenia to the Artemis Accords,” said NASA Administrator Bill Nelson. “Today, the partnership between the United States and Slovenia crosses a new frontier. We live in a golden era of exploring the stars. That era will be written by nations that explore the cosmos openly, responsibly, and in peace.”
State Secretary Matevž Frangež of the Ministry of the Economy, Tourism, and Sport signed the Accords on behalf of Slovenia, with James O’Brien, Assistant Secretary of State for European and Eurasian Affairs, participating in the signing event.
“Slovenia joins the principles, values, and rules on the peaceful use of space as a common good of humanity,” Frangež said.
Rebecca Bresnik, Associate General Counsel for International and Space Law, served as the senior NASA official at the ceremony, along with her husband, Randy Bresnik, who is a NASA astronaut of Slovenian descent.
“We are delighted to welcome Slovenia to the Artemis Accords family,” said Ambassador Jamie Harpootlian, the U.S. ambassador to Slovenia “We recognize Slovenia as a rising leader in space. We look forward to taking our collaborations with Slovenia on science, technology, and innovation to new frontiers.”
In 2020, the United States and seven other countries established the Artemis Accords to establish guidelines for the peaceful exploration and use of outer space. The Accords reinforce and implement key obligations in the 1967 Outer Space Treaty. They also strengthen the commitment by the United States and signatory nations to the Registration Convention, the Rescue and Return Agreement, as well as best practices NASA and its partners support, including the public release of scientific data.
Learn more about the Artemis Accords at:
https://www.nasa.gov/artemis-accords
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Lauren Low
Headquarters, Washington
202-358-1600
lauren.e.low@nasa.gov
NASA Data Helps Beavers Build Back Streams
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) A beaver family nibbles on aspen branches just up Logan Canyon from Utah State University, in Spawn Creek, Utah. Credit: Sarah KoenigsbergHumans aren’t the only mammals working to mitigate the effects of climate change in the Western United States. People there are also enlisting the aid of nature’s most prolific engineers – beavers. Using NASA-provided grants, two open-source programs from Boise State University in Idaho and Utah State University in Logan are making it possible for ranchers, land trust managers, nonprofits, and others to attract beavers to areas that need their help.
The Beaver Restoration Assessment Tool (BRAT) created by Utah State University uses data from satellites built at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, to identify areas that need restoration and would benefit from beavers’ dam-building abilities. The Boise State University Mesic Resource Restoration Monitoring Aid (MRRMaid) program, which also uses satellite data, monitors the areas over time. Both efforts are also supported by NASA’s Research Opportunities in Space and Earth Science program and the agency’s Applied Sciences’ Ecological Conservation program.
Once a site is chosen, program staffers and landowners begin to take measures to attract beavers, or the teams may relocate them from other areas. Either way, once on site, these semiaquatic builders get to work building and maintaining dams to create the ponds. The ponds help to retain water, including runoff from snowmelt and rainstorms, that would otherwise rush through the area, causing erosion and degrading the surrounding ecosystems.
Over time, these new ponds raise the water table, support wetlands that attract more wildlife and fish, and restore native plants to the ecosystem. Beaver dams can help ranchers improve water availability on their property, supporting their operations.
NASA Landsat data helps Utah State University identify streams where beavers can be reintroduced to help improve an ecosystem. Boise State University also uses Landsat data to show just how much beavers help. The vegetation in this satellite image indicates where streams or creeks are flowing and reveals the benefits of beaver activity.Credit: NASAIn addition to being beautiful and supporting the local ecology, these moisture-rich environments can limit wildfire damage with a barrier of healthy vegetation resistant to burning. When human infrastructure is nearby, a built-in leak or other interventions by humans can be added to control the water level, preventing floods that cause property damage.
As a restoration site’s health improves, MRRMaid and BRAT use NASA satellite data to monitor those changes and analyze how the beavers benefit the ecosystem in drought-stricken areas. Community leaders can use this information and the living examples of restored sites to build new parks and recreational areas and plan future restoration projects with their furry collaborators.
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