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This landscape of “mountains” and “valleys” speckled with glittering stars is actually the edge of a nearby, young, star-forming region called NGC 3324 in the Carina Nebula. Captured in infrared light by NASA’s new James Webb Space Telescope, this image reveals for the first time previously invisible areas of star birth. NASA, ESA, CSA, and STScITracking Spring Flooding
Ural River levels peak in this April 13, 2024, enhanced color image from Landsat 9; here, vegetation appears red, while water is blue-green. After heavy rain and rapid snowmelt, rivers in southern Russia and northern Kazakhstan swelled, flooding homes and displacing thousands of people.
Landsat 9, the latest satellite in the Landsat series, contributes a critical component to the international strategy for monitoring the health and state of the Earth, allowing more frequent observations. Data from Landsat 9 can be used to inform decisions in key areas like urban expansion, coral reef degradation, and natural disasters.
Image Credit: NASA/Michala Garrison, USGS
NASA’s Chandra Releases Doubleheader of Blockbuster Hits
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These two movies of the Cassiopeia A and Crab Nebula supernova remnants show Chandra’s capabilities of documenting changes in astronomical objects over human timeframes. Dramatic changes are apparent in the debris and radiation remaining after the explosion of these two massive stars in our galaxy. Such time-lapse movies would not be possible without Chandra’s archives that serve as public repositories for the data collected over Chandra’s nearly 25 years of operations.New movies of two of the most famous objects in the sky — the Crab Nebula and Cassiopeia A — are being released from NASA’s Chandra X-ray Observatory. Each includes X-ray data collected by Chandra over about two decades. They show dramatic changes in the debris and radiation remaining after the explosion of two massive stars in our galaxy.
The Crab Nebula, the result of a bright supernova explosion seen by Chinese and other astronomers in the year 1054, is 6,500 light-years from Earth. At its center is a neutron star, a super-dense star produced by the supernova. As it rotates at about 30 times per second, its beam of radiation passes over the Earth every orbit, like a cosmic lighthouse.
As the young pulsar slows down, large amounts of energy are injected into its surroundings. In particular, a high-speed wind of matter and anti-matter particles plows into the surrounding nebula, creating a shock wave that forms the expanding ring seen in the movie. Jets from the poles of the pulsar spew X-ray emitting matter and antimatter particles in a direction perpendicular to the ring.
Over 22 years, Chandra has taken many observations of the Crab Nebula. With this long runtime, astronomers see clear changes in both the ring and the jets in the new movie. Previous Chandra movies showed images taken from much shorter time periods — a 5-month period between 2000 and 2001 and over 7 months between 2010 and 2011 for another. The longer timeframe highlights mesmerizing fluctuations, including whip-like variations in the X-ray jet that are only seen in this much longer movie. A new set of Chandra observations will be conducted later this year to follow changes in the jet since the last Chandra data was obtained in early 2022.
Crab Nebula TimelapseTo view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
This video begins with a composite version of the Crab Nebula, combining Chandra X-ray data with infrared data from the James Webb Space Telescope. Over 22 years, Chandra has taken many observations of the Crab Nebula. With this long runtime, astronomers see clear changes in both the ring and the jets in the new movie. Previous Chandra movies showed images taken from much shorter time periods — a 5-month period between 2000 and 2001 and over 7 months between 2010 and 2011 for another. The longer timeframe highlights mesmerizing fluctuations, including whip-like variations in the X-ray jet that are only seen in this much longer movie. A new set of Chandra observations will be conducted later this year to follow changes in the jet since the last Chandra data was obtained in early 2022. (Credit: X-ray: NASA/CXC/SAO; Image processing: NASA/CXC/SAO/J. Schmidt, J. Major, A. Jubett, K. Arcand)The second billing in this doubleheader is just as spectacular. Cassiopeia A (Cas A for short) is the remains of a supernova that is estimated to have exploded about 340 years ago in Earth’s sky. While other Chandra movies of Cas A have previously been released, including one with data extending from 2000 to 2013, this new movie is substantially longer featuring data from 2000 through to 2019.
The outer region of Cas A shows the expanding blast wave of the explosion. The blast wave is composed of shock waves, similar to the sonic booms generated by a supersonic aircraft. These expanding shock waves are sites where particles are being accelerated to energies that are higher than the most powerful accelerator on Earth, the Large Hadron Collider. As the blast wave travels outwards it encounters surrounding material and slows down, generating a second shock wave that travels backwards relative to the blast wave, analogous to a traffic jam travelling backwards from the scene of an accident on a highway.
Cas A has been one of the most highly observed targets and publicly released images from the Chandra mission. It was Chandra’s official first-light image in 1999 after the Space Shuttle Columbia launched into orbit and quickly discovered a point source of X-rays in Cas A’s center for the first time, later confirmed to be a neutron star. Over the years, astronomers have used Chandra to discover evidence for “superfluid” inside Cas A’s neutron star, to reveal that the original massive star may have turned inside out as it exploded and to take an important step in pinpointing how giant stars explode. Chandra has also mapped the elements forged inside the star, which are now moving into space to help seed the next generation of stars and planets. More recently, Chandra data was combined with data from NASA’s James Webb Space Telescope to help determine the origin of mysterious structures within the remnant.
Cassiopeia A TimelapseTo view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
This video begins with a composite version of the Cassiopeia A, combining Chandra X-ray data with infrared data from the James Webb Space Telescope. Cassiopeia A (Cas A for short) is the remains of a supernova that is estimated to have exploded about 340 years ago in Earth’s sky. This new Cas A movie features data from 2000 through to 2019. The images used in the latest Cas A movie have been processed using a state-of-the-art processing technique, led by Yusuke from Rikkyo University in Japan, to fully capitalize on Chandra's sharp X-ray vision. (Credit: X-ray: NASA/CXC/SAO; Optical: NASA/STScI; Image Processing: NASA/CXC/SAO/J. Major, A. Jubett, K. Arcand)The images used in the latest Cas A movie have been processed using a state-of-the-art processing technique, led by Yusuke from Rikkyo University in Japan, to fully capitalize on Chandra’s sharp X-ray vision. The paper describing their work was published in The Astrophysical Journal and is available online.
These two movies show Chandra’s capabilities of documenting changes in astronomical objects over human timeframes. Such movies would not be possible without Chandra’s archives that serve as public repositories for the data collected over Chandra’s nearly 25 years of operations.
NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science from Cambridge Massachusetts and flight operations from Burlington, Massachusetts.
Read more from NASA’s Chandra X-ray Observatory.
For more Chandra images, multimedia and related materials, visit:
https://www.nasa.gov/mission/chandra-x-ray-observatory/
News Media ContactMegan Watzke
Chandra X-ray Center
Cambridge, Mass.
617-496-7998
Jonathan Deal
Marshall Space Flight Center
Huntsville, Ala.
256-544-0034
Kiyun Kim: From Intern to Accessibility Advocate
Kiyun Kim began at Goddard as a summer intern. Impressed by the center’s community bonds, Kim is now co-chair of a center resource group that champions accessibility and inclusivity.
Name: Kiyun Kim
Title: Software Engineer
Organization: Ground Software Systems Branch (Code 583)
What do you do at Goddard Space Flight Center?
I’m a software engineer on the ground software systems branch. We do all the software work that stays on the ground and does not go up into space. We do things like software that helps us coordinate stuff on the ground, helps us contact with the satellites, do scheduling, process data, all sorts of things like that. What I do at any given time depends on what project I’m under.
The main thing that I’ve been working on lately is a tool for database checkouts. There are different versions of the database for each satellite and what we want to be able to do is validate those databases and also to look at the changes between databases and compare them to each other.
In the past, I’ve also worked on a contact scheduling tool — when you have a bunch of different satellites, they’re kind of staggered in orbit, so normally, their signals wouldn’t run into each other, so to speak, when you’re getting the downlinks from them. But when you have a project that is sharing ground resources with other projects, other organizations, the way that Joint Polar Satellite System is, you sometimes have to work to prevent conflicts between satellites. What we’re trying to do is maximize the amount of downlinks for each mission in line with what they need.
Prior to that I was on Goddard Mission Services Evolution Center, or GMSEC. It’s a framework so that missions can take care of all the communication between all the different parts of their systems. So for example, each mission can use GMSEC and take the built in components that GMSEC offers or build their own components and just plug them into GMSEC and they’ll all talk to each other using GMSEC.
Specifically, I worked on the web interface for that and made a countdown clock for it, modeled after the Magnetospheric Multiscale Mission (MMS).
What led you to working at NASA?
I was looking for internships as a college student and my dad found the NASA summer internship program and encouraged me to apply. I got in and I had a really great time.
What have you enjoyed most about working at NASA?
One thing that I’ve really appreciated is the work-life balance aspect, and also the fact that I don’t have to give up learning new things in order to fulfill my job. Obviously if I have a deadline, I can’t go to the on-center talks and stuff, but the fact that there are all these talks on different subjects, I really like that I’m able to just go, and that I’m supported in doing that.
I still consider myself early in my career and there’s so much that I just don’t know about on center. I know of the kinds of things that I’ve been working on, obviously, but I don’t necessarily get exposed to everything else in my day-to-day work. Having the opportunity to see what else is going on on-center is also good for, beyond just sating my curiosity, it’s also good for helping me figure out what I want to do with my life.
Is there anything you didn’t expect when you started as an intern?
I was surprised by how warm people would be. I remember a very defining experience for me as an intern, was I was walking to get lunch one day from the cafeteria, and I ran into someone who I didn’t know and she stopped and because she saw my intern badge started talking with me. We ended up talking like out in the hot sun for like an hour. Later she invited me to lunch while I was still an intern, and she came to my intern presentation. She was actually from the Women’s Employee Resource Group. She wasn’t explicitly trying to recruit me, but she was just so excited to see a new face and reach out to me and make sure that I felt welcome. That was just like a really defining experience for me and I think it solidified that this was the kind of place I wanted to work at.
Kiyun Kim is one of the co-chairs of the Equal Accessibility Employee Resource Group at Goddard.Courtesy of Kiyun KimAre you involved in any groups on campus?
I’m one of the co-chairs of the Equal Accessibility Employee Resource Group. I admit that sometimes my own disabilities make it difficult for me to be as active as I would like, but I feel very strongly that the strong ERG presence on center is a blessing. It’s something that we should nurture.
The Equal Accessibility Employee Resource Group aims to create awareness around issues that face disabled folks in employment, as well as work to help alleviate some of the barriers that we face on center. It’s advocacy by and for the group that it represents. Obviously, you don’t need to be disabled to join and you also don’t have to disclose if you don’t want to. I think accessibility is something that we kind of take for granted until it’s not there for us. A lot of what we’re trying to do is to just make sure that the concerns of our constituents are bubbled up to leadership and make sure that accessibility is kept in mind as the center moves forward and continues to evolve.
Diversity in general contributes so much to the workforce. When we, intentionally or not, exclude entire groups of people from being able to work here and to thrive here we actually do lose a lot. Our goal is to prevent that from happening.
By Marta Hill
NASA’s Goddard Space Flight Center in Greenbelt, Md.
Conversations With Goddard is a collection of Q&A profiles highlighting the breadth and depth of NASA’s Goddard Space Flight Center’s talented and diverse workforce. The Conversations have been published twice a month on average since May 2011. Read past editions on Goddard’s “Our People” webpage.
Share Details Last Updated Apr 24, 2024 EditorMadison OlsonContactRob Garnerrob.garner@nasa.govLocationGoddard Space Flight Center Related Terms Explore More 5 min read Shawnta M. Ball Turns Obstacles into Opportunities in Goddard’s Education Office Article 2 weeks ago 9 min read Jennifer Krottinger: Designing Ways to Serve Article 2 months ago 4 min read Renee King: Ensuring Space for Everyone Article 2 months agoNASA Glenn Interactive Exhibit Earns Gold
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Preparations for Next Moonwalk Simulations Underway (and Underwater) A new interactive exhibit at the NASA Glenn Visitor Center replicates the Fluids and Combustion Facility on the International Space Station, enabling users to see how microgravity experiments operate. Credit: NASA/Christopher HartenstineThe Ohio Museums Association (OMA) presented NASA’s Glenn Research Center in Cleveland with two OMA 2023 Visual Communications Awards during its annual meeting in Sandusky, Ohio, on April 14. NASA Glenn and contractor Impact Inc. received the Gold Award (Level 2) and the Best in Show Award for the updated “Science in Space: Interactive International Space Station Exhibit” at the NASA Glenn Visitor Center, located in Great Lakes Science Center.
The exhibit replicates the Fluids and Combustion Facility (FCF) on the International Space Station, which houses two research facilities — the Combustion Integrated Rack, or CIR, and the Fluids Integrated Rack, or FIR. Both were developed at NASA Glenn with prime contractor ZIN Technologies and are operated remotely from Glenn’s ISS Payloads Operation Center. The FCF supports physical and biological experiments to advance technology development while bringing many benefits back to Earth.
For more information about the exhibit, visit: https://www.nasa.gov/centers-and-facilities/glenn/new-nasa-glenn-exhibit-spotlights-microgravity-research/.
Explore More 1 min read NASA Participates in NCAA Women’s Championship Game Article 8 hours ago 1 min read NASA Glenn Teams Up with Cleveland Monsters Article 8 hours ago 1 min read NASA Glenn Joins Big Hoopla STEM Challenge Article 8 hours agoNASA Participates in NCAA Women’s Championship Game
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Preparations for Next Moonwalk Simulations Underway (and Underwater) Women scientists, engineers, and leaders from NASA stand at center court inside Rocket Mortgage FieldHouse in downtown Cleveland to hold a large American flag during the NCAA Women’s Championship Game opening ceremony. Credit: NASA/Jef JanisJust before tipoff at the live national broadcast of the NCAA Women’s Final Four Championship Game on April 7, 31 women scientists, engineers, and leaders from NASA stood at center court inside Rocket Mortgage FieldHouse in downtown Cleveland to hold a large American flag during the opening ceremony.
Women representing NASA carry a folded American flag off the court after the flag ceremony inside Rocket Mortgage FieldHouse in downtown Cleveland. Credit: NASA/Jef Janis
The crowd cheered as astronaut Jessica Watkins and professionals from NASA’s Glenn Research Center, NASA Headquarters, and other field centers opened the flag and waved it during the national anthem. Click here to see more images from this exciting outreach experience.
NASA participants, along with astronaut Jessica Watkins, pose at center court inside Rocket Mortgage FieldHouse in downtown Cleveland prior to the American flag opening ceremony. Credit: NASA/Michael Ahn Explore More 1 min read NASA Glenn Interactive Exhibit Earns Gold Article 8 hours ago 1 min read NASA Glenn Teams Up with Cleveland Monsters Article 8 hours ago 1 min read NASA Glenn Joins Big Hoopla STEM Challenge Article 8 hours agoNASA Glenn Teams Up with Cleveland Monsters
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Preparations for Next Moonwalk Simulations Underway (and Underwater)NASA’s Glenn Research Center joined the Cleveland Monsters to celebrate their total solar eclipse-themed game against the Rochester Americans at the Rocket Mortgage FieldHouse in Cleveland on March 30. NASA Glenn staff were on hand to discuss the total solar eclipse and NASA’s presence at Great Lakes Science Center’s Total Eclipse Fest 2024, April 6-8. NASA also provided a photobooth for guests to use, Eva the astronaut mascot made rounds, and Glenn showcased its Graphics and Visualization Lab through virtual reality glasses experiences and hands-on demos. The Monsters also showed a 2024 Eclipse Countdown Kickoff video during the game.
NASA Glenn’s Gretchen Morales-Valle, front left, and Daniel Phan, back left, share information about the total solar eclipse and viewing safety during the Cleveland Monsters game at Rocket Mortgage FieldHouse in Cleveland. Credit: NASA/John Oldham Explore More 1 min read NASA Glenn Interactive Exhibit Earns Gold Article 8 hours ago 1 min read NASA Participates in NCAA Women’s Championship Game Article 8 hours ago 1 min read NASA Glenn Joins Big Hoopla STEM Challenge Article 8 hours ago
NASA Glenn Joins Big Hoopla STEM Challenge
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Preparations for Next Moonwalk Simulations Underway (and Underwater) Sam Chamberlin, NASA Glenn Office of STEM Engagement, guides young guests in a hands-on activity demonstrating shape memory alloys during the Big Hoopla STEM Challenge. Credit: NASA/Catherine GravesNASA’s Glenn Research Center in Cleveland joined in the adventure of the Big Hoopla STEM Challenge held at the Dayton Convention Center on March 17. The free family event for kids (K-8) tied together the excitement of college basketball and the power of STEM education. NASA Glenn Deputy Center Director Dawn Schaible participated in the event, stressing NASA’s support for nurturing STEM education and careers.
NASA Glenn Research Center’s Deputy Center Director Dawn Schaible shares her excitement and support for STEM education during the Big Hoopla STEM Challenge. Credit: NASA/Scott BroemsenGlenn’s Office of STEM Engagement staff engaged over 200 students in hands-on STEM activities during the event. Students learned about the total solar eclipse, how to safely view the eclipse, and received eclipse glasses. They also participated in shape memory alloy demonstrations, experienced flight simulations using 360 Oculus goggles, and learned about solar energy by making ultraviolet bead bracelets.
Explore More 1 min read NASA Glenn Interactive Exhibit Earns Gold Article 8 hours ago 1 min read NASA Participates in NCAA Women’s Championship Game Article 8 hours ago 1 min read NASA Glenn Teams Up with Cleveland Monsters Article 8 hours agoNASA Mentors, Students Rock FIRST Buckeye Regional
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Preparations for Next Moonwalk Simulations Underway (and Underwater) The NASA-sponsored Magnificat MagnifiBots team from Magnificat High School in Rocky River, Ohio, earned the Rookie All-Star Award. Credit: NASA/Jef JanisNASA’s Glenn Research Center in Cleveland supported the 25th annual FIRST Robotics Buckeye Regional Competition, March 20 to 23, at Cleveland State University’s Wolstein Center.
The NASA-sponsored WorBots team from Thomas Worthington High School in Worthington, Ohio, and Worthington Kilbourne High School in Columbus, Ohio, received the Championship Qualifying Award and the Regional FIRST Impact Award. Credit: NASA/Jef JanisFifty-five teams of high school students competed in the robotics competition, which aims to inspire young people to be science and technology leaders and innovators by engaging them in mentor-based engineering.
The NASA-sponsored Argonauts team from Davis Aerospace and Maritime High School in Cleveland received the coveted Judges’ Award. Credit: NASA/Jef JanisNASA Glenn employees offered their time and expertise as mentors or volunteers supporting FIRST Robotics teams leading up to the event as well as on competition day. Glenn-sponsored teams took home key awards, and Sierra Lobo’s NASA Machine Shop earned the Volunteer of the Year Award.
The NASA-sponsored AstroCircuits team from John Marshall School of Information Technology in Cleveland ranked 14th out of 55 teams. Credit: NASA/Jef Janis Explore More 1 min read NASA Glenn Interactive Exhibit Earns Gold Article 8 hours ago 1 min read NASA Participates in NCAA Women’s Championship Game Article 8 hours ago 1 min read NASA Glenn Teams Up with Cleveland Monsters Article 8 hours agoCleveland School Students Learn About STEM Careers
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Preparations for Next Moonwalk Simulations Underway (and Underwater) Cleveland Metropolitan School District high school students learned about how a robotic dog named “Astro” serves as the eyes and ears for NASA employees conducting inspections in noisy facilities. Credit: NASA/Sara Lowthian-HannaNASA’s Glenn Research Center in Cleveland opened its doors to Cleveland Metropolitan School District (CMSD) students to explore various Science, Technology, Engineering, and Mathematics (STEM) careers.
NASA Glenn’s Office of STEM Engagement invited high school students onsite to explore center facilities and talk to NASA experts during NASA Career Exploration Day. Students learned about NASA internships, as well as paid STEM engagement learning experiences for CMSD students at NASA Glenn this summer.
“The career exploration day is two-fold,” said Glenn Education Project Specialist Clarence Jones. “We engage and inspire students to consider STEM careers, and we encourage them to participate in the summer CMSD Career Research Experience.”
During NASA Career Exploration Day, eleventh graders participated in hands-on STEM engagement activities and saw research demonstrations. They toured several facilities and engaged in a panel discussion with NASA scientists, engineers, and current NASA interns.
Cleveland Metropolitan School District high school students stand in front of an airplane in the Flight Research Building (hangar) at NASA’s Glenn Research Center in Cleveland. Credit: NASA/Jef Janis Explore More 1 min read NASA Glenn Interactive Exhibit Earns Gold Article 8 hours ago 1 min read NASA Participates in NCAA Women’s Championship Game Article 8 hours ago 1 min read NASA Glenn Teams Up with Cleveland Monsters Article 8 hours agoNASA Wins 6 Webby Awards, 8 Webby People’s Voice Awards
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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?
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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
-end-
Kara Slaughter
Johnson Space Center, Houston
281-483-5111
