NASA News
NASA Receives 10 Nominations for the 29th Annual Webby Awards
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) This ultra high-definition video featuring an orange tabby cat named Taters, was streamed from nearly 19 million miles away via laser by NASA’s Deep Space Optical Communications (DSOC) experiment, marking a historic milestone for space communications.Jet Propulsion LaboratorySince it began in 1958, NASA has been charged by law with spreading the word about its work to the widest extent practicable. From typewritten press releases to analog photos and film, the agency has effectively moved into social media and other online communications. NASA’s broad reach across digital platforms has been recognized by the International Academy of Digital Arts and Sciences (IADAS), with 10 nominations across multiple categories for the academy’s 29th annual Webby Awards.
The 2025 Webby nominations demonstrate NASA's dedication to sharing the wonders of space through digital platforms. We believe in the power of digital storytelling to inspire the next generation of explorers.Michelle R. Jones
Deputy Associate Administrator for Communications
Public Voting OpportunitiesVoting for the Webby People’s Voice Awards—chosen by the public—is open now through Thursday, April 17. Voting links for each category are listed below.
29th Annual Webby Award Nominees AI, Immersive & GamesNASA’s Snap It! An Eclipse Photo Adventure
NASA
Kids and Family
NASA Instagram
NASA
Education and Science
Matt Dominick’s X Account: A Visual Journey from Space
NASA
Best Photography & Design
NASA’s 2024 Total Solar Eclipse Campaign
NASA
Events and Livestreams
NASA’s Webb Telescope: Unfolding a Universe of Wonders
NASA Goddard
Education and Science
2024 Total Solar Eclipse: Through the Eyes of NASA
NASA
Events and Live
NASA Streams Historic Cat Video From Deep Space
NASA’s Jet Propulsion Laboratory
Events and Livestreams
NASA Website
NASA
Government & Associations
NASA+ Streaming Service
NASA
Television, Film & Streaming
NASA Newsletter
NASA
Business, News and Technology
Established in 1996 during the web’s infancy, The Webbys is presented by the IADAS—a 3000+ member judging body. The Academy is comprised of Executive Members—leading Internet experts, business figures, luminaries, visionaries, and creative celebrities—and associate members who are former Webby winners, nominees and other internet professionals.
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. In the spirit of the open web, the Webby People’s Voice is chosen by the voting public, and garners millions of votes from all over the world.
NASA’s SPHEREx Takes First Images, Preps to Study Millions of Galaxies
5 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA’s SPHEREx, which will map millions of galaxies across the entire sky, captured one of its first exposures March 27. The observatory’s six detectors each captured one of these uncalibrated images, to which visible-light colors have been added to represent infrared wavelengths. SPHEREx’s complete field of view spans the top three images; the same area of the sky is also captured in the bottom three images. NASA/JPL-CaltechProcessed with rainbow hues to represent a range of infrared wavelengths, the new pictures indicate the astrophysics space observatory is working as expected.
NASA’s SPHEREx (short for Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) has turned on its detectors for the first time in space. Initial images from the observatory, which launched March 11, confirm that all systems are working as expected.
Although the new images are uncalibrated and not yet ready to use for science, they give a tantalizing look at SPHEREx’s wide view of the sky. Each bright spot is a source of light, like a star or galaxy, and each image is expected to contain more than 100,000 detected sources.
There are six images in every SPHEREx exposure — one for each detector. The top three images show the same area of sky as the bottom three images. This is the observatory’s full field of view, a rectangular area about 20 times wider than the full Moon. When SPHEREx begins routine science operations in late April, it will take approximately 600 exposures every day.
Each image in this uncalibrated SPHEREx exposure contains about 100,000 light sources, including stars and galaxies. The two insets at right zoom in on sections of one image, showcasing the telescope’s ability to capture faint, distant galaxies. These sections are processed in grayscale rather than visible-light color for ease of viewing.NASA/JPL-Caltech“Our spacecraft has opened its eyes on the universe,” said Olivier Doré, SPHEREx project scientist at Caltech and NASA’s Jet Propulsion Laboratory, both in Southern California. “It’s performing just as it was designed to.”
The SPHEREx observatory detects infrared light, which is invisible to the human eye. To make these first images, science team members assigned a visible color to every infrared wavelength captured by the observatory. Each of the six SPHEREx detectors has 17 unique wavelength bands, for a total of 102 hues in every six-image exposure.
Breaking down color this way can reveal the composition of an object or the distance to a galaxy. With that data, scientists can study topics ranging from the physics that governed the universe less than a second after its birth to the origins of water in our galaxy.
“This is the high point of spacecraft checkout; it’s the thing we wait for,” said Beth Fabinsky, SPHEREx deputy project manager at JPL. “There’s still work to do, but this is the big payoff. And wow! Just wow!”
During the past two weeks, scientists and engineers at JPL, which manages the mission for NASA, have executed a series of spacecraft checks that show all is well so far. In addition, SPHEREx’s detectors and other hardware have been cooling down to their final temperature of around minus 350 degrees Fahrenheit (about minus 210 degrees Celsius). This is necessary because heat can overwhelm the telescope’s ability to detect infrared light, which is sometimes called heat radiation. The new images also show that the telescope is focused correctly. Focusing is done entirely before launch and cannot be adjusted in space.
“Based on the images we are seeing, we can now say that the instrument team nailed it,” said Jamie Bock, SPHEREx’s principal investigator at Caltech and JPL.
How It WorksWhere telescopes like NASA’s Hubble and James Webb space telescopes were designed to target small areas of space in detail, SPHEREx is a survey telescope and takes a broad view. Combining its results with those of targeted telescopes will give scientists a more robust understanding of our universe.
The observatory will map the entire celestial sky four times during its two-year prime mission. Using a technique called spectroscopy, SPHEREx will collect the light from hundreds of millions of stars and galaxies in more wavelengths any other all-sky survey telescope.
Track SPHEREx with NASA's Eyes on the Solar SystemWhen light enters SPHEREx’s telescope, it’s directed down two paths that each lead to a row of three detectors. The observatory’s detectors are like eyes, and set on top of them are color filters, which are like color-tinted glasses. While a standard color filter blocks all wavelengths but one, like yellow- or rose-tinted glasses, the SPHEREx filters are more like rainbow-tinted glasses: The wavelengths they block change gradually from the top of the filter to the bottom.
“I’m rendered speechless,” said Jim Fanson, SPHEREx project manager at JPL. “There was an incredible human effort to make this possible, and our engineering team did an amazing job getting us to this point.”
More About SPHERExThe SPHEREx mission is managed by JPL for the agency’s Astrophysics Division within the Science Mission Directorate at NASA Headquarters. BAE Systems (formerly Ball Aerospace) built the telescope and the spacecraft bus. The science analysis of the SPHEREx data will be conducted by a team of scientists located at 10 institutions in the U.S., two in South Korea, and one in Taiwan. Caltech managed and integrated the instrument. Data will be processed and archived at IPAC at Caltech. The mission’s principal investigator is based at Caltech with a joint JPL appointment. The SPHEREx dataset will be publicly available at the NASA-IPAC Infrared Science Archive. Caltech manages JPL for NASA.
For more about SPHEREx, visit:
https://science.nasa.gov/mission/spherex/
News Media ContactCalla Cofield
Jet Propulsion Laboratory, Pasadena, Calif.
626-808-2469
calla.e.cofield@jpl.nasa.gov
2025-045
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Studying Ice for the Future of Flight
Thomas Ozoroski, a researcher at NASA’s Glenn Research Center in Cleveland, takes icing accretion measurements in October 2024 as part of transonic truss-braced wing concept research.
In the future, aircraft with long, thin wings supported by aerodynamic braces could help airlines save on fuel costs – but those same wings could be susceptible to ice buildup. In the historic Icing Research Tunnel at NASA Glenn, scientists and engineers are testing a concept for a transonic truss-braced wing. Their goal: to collect important data to inform the design of these potential efficient aircraft of the future.
NASA Glenn can simulate icing conditions in its Icing Research Tunnel to identify potential challenges for new aircraft designs. These tests provide valuable information about how ice builds up on wings and can help identify the most critical icing conditions for safety.
Read more about icing testing at NASA Glenn.
Image credit: NASA/Jordan Cochran
What’s Up: April 2025 Skywatching Tips from NASA
Enjoy observing planets in the morning and evening sky, look for Lyrid meteors, and hunt for the “faint fuzzy” wonder that is the distant and ancient city of stars known as globular cluster M3.
Skywatching HighlightsAll Month – Planet Visibility:
- Mercury: Visible for a few days in the second half of April, extremely low in the east before sunrise.
- Venus: Rising low in the east in the hour before dawn.
- Mars: Bright and easy to view after dark all month. Setting a couple of hours after midnight.
- Jupiter: Bright and easy to spot in the west after dark, setting a couple of hours after sunset.
- Saturn: Visible low in the east below Venus, before dawn in the last two weeks of April.
Daily Highlights:
April 1 & 30 – Jupiter & Crescent Moon: Find the charming pair in the west as the sky darkens, setting about 3 hours after sunset.
April 4 & 5 – Mars & Moon: The Moon, around its first quarter phase, appears near Mars in the sky for two nights.
April 24-25 – Grouping of the Moon & Three Planets: Find Venus, Saturn, and the crescent moon gathered low in the east as dawn warms the morning sky. Mercury is also visible below them for those with a clear view to the horizon.
All month – Venus: Earth’s hothouse twin planet has made the shift from an evening object to a morning sight. You’ll notice it rising low in the east before dawn, looking a little higher each morning through the month.
All month – Mars: Looking bright and reddish in color, Mars is visible high overhead after dark all month. At the start of the month it lies along a line with bright stars Procyon and Pollux, but you’ll notice it moves noticeably over the course of April (~12 degrees or the width of your outstretched fist at arm’s length).
TranscriptWhat’s Up for April? Planets at dusk and dawn, April showers, and observing a distant city of stars.
Sky chart showing Jupiter and the crescent Moon on April 1. A similar scene repeats on April 30, but with the Moon appearing above Jupiter. NASA/JPL-CaltechFirst up, in the evening sky, we begin and end the month with Jupiter and the crescent Moon shining brightly together in the western sky as sunset fades. On both April 1st and 30th, you can find the charming pair about half an hour after sunset, setting about 3 hours later.
Mars is high overhead in the south on April evenings. At the start of the month, it’s directly in between bright stars Procyon and Pollux, but it moves noticeably during the month. You’ll find the first-quarter moon right next to Mars on April 4th and 5th.
Moving to the morning sky, Venus has now made the switch from an evening object to a morning one. You may start to notice it rising low in the east before dawn, looking a little higher each morning through the month.
Sky chart showing the eastern sky 45 minutes before sunrise on April 24, with Venus, Saturn and the crescent Moon forming a grouping low in the sky. Mercury might also be visible for those with a completely clear view to the horizon. NASA/JPL-CaltechAround April 24th and 25th, you’ll find Venus, Saturn, and the crescent moon gathered low in the east as dawn warms up the morning sky. Those with a clear view to the horizon might also pick out Mercury looking bright, but very low in the sky.
April brings shooting stars as Earth passes through one the streams of comet dust that create our annual meteor showers. The Lyrids are a modest meteor shower that peaks overnight on April 21st and into the morning of the 22nd. You can expect up to 15 meteors per hour near the peak under dark skies.
The Lyrids are best observed from the Northern Hemisphere, but can be seen from south of the equator as well. View them after about 10:30pm local time until dawn, with the best viewing around 5 a.m. The waning crescent moon will rise around 3:30am, but at only 27% full, it shouldn’t interfere too much with your meteor watching. For the best experience, face roughly toward the east, lie down in a safe, dark place away from bright lights, and look straight overhead. Meteors can appear anywhere in the sky, and some Lyrids can leave bright trails that last for a few seconds after they’ve passed.
NASA studies meteors from the ground, in the air, and from orbit to forecast meteor activity and protect spacecraft, and to understand the composition of comets and asteroids throughout our solar system.
Sky chart facing east around 9pm in April 2025 showing the location of globular cluster M3. The chart depicts the cluster’s position relative to the Big Dipper and bright stars Arcturus and Cor Caroli. The Big Dipper star Megrez serves as an indicator for the brightness of Cor Caroli. For easy visibility, M3 is depicted brighter and larger than its actual appearance. NASA/JPL-CaltechApril offers a chance to observe a truly distant wonder – a globular cluster known as “M3.” It’s a vast collection of stars that lies 34,000 light-years from Earth in our galaxy’s outer reaches. Astronomer Charles Messier discovered this object in 1764, while searching for new comets. Realizing it wasn’t one, he added it to his list of interesting objects that were not comets, which today we know as Messier’s catalog.
Through binoculars, Messier 3, or M3, appears as a small, fuzzy, star-like patch of light. With a small telescope, you’ll see a more defined glow with a slightly grainy texture. And with telescopes 8 inches or larger, the cluster begins to resolve into hundreds of individual stars.
Now, globular clusters contain some of the oldest stars in the universe, often over 10 billion years old. Unlike open clusters like the Pleiades, which sit within the Milky Way’s spiral arms, globular clusters are found in the galaxy’s halo, orbiting far above and below the Milky Way’s disk. Our galaxy has around 150 confirmed globular clusters. M3 itself is probably 11 to 13 billion years old and contains around half a million stars. And it’s relatively easy to spot in April under dark skies with binoculars or a small telescope.
Finding M3 starts with the Big Dipper. Facing east, use the Dipper’s handle to “arc to Arcturus,” the fourth-brightest star in the night sky. From there, look higher in the sky to find the star Cor Caroli located here to the west of the Dipper’s handle. It’s about as bright as this star in the Dipper’s cup. M3 is located roughly a third of the way from Arcturus to Cor Caroli. With binoculars or a finder scope, sweep within this area until you spot a faint, round glow.
M3 is an excellent target for beginners and seasoned observers alike. Whether using binoculars or a telescope, you’ll be rewarded with a view of one of the oldest objects in our galaxy.
The phases of the Moon for April 2025. NASA/JPL-CaltechAbove are the phases of the Moon for April.
Stay up to date on all of NASA’s missions exploring the solar system and beyond at NASA Science. I’m Preston Dyches from NASA’s Jet Propulsion Laboratory, and that’s What’s Up for this month.
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NASA History News and Notes–Spring 2025
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Preparations for Next Moonwalk Simulations Underway (and Underwater)The NASA History Office brings you the new Spring 2025 issue of NASA History News & Notes reflecting on some of the transitional periods in NASA’s history, as well as the legacies of past programs. Topics include NASA’s 1967 class of astronauts, historic experiments in airborne astronomy, NASA’s aircraft consolidation efforts in the 1990s, lightning observations from space, the founding of the NACA, the DC-8 airborne science laboratory, and more!
Volume 42, Number 1
Spring 2025
By Brian Odom
In the first few months of 2025, NASA will celebrate several significant anniversaries, including the 110th anniversary of the National Advisory Committee for Aeronautics (NACA) (March 3), the 55th anniversary of the launch of Apollo 13 (April 11), and the 35th anniversary of the launch of the Hubble Space Telescope (April 24). Celebrating these important milestones is a way for us as an agency and for the public to reflect upon where we have been and what we have accomplished and to think about what we might accomplish next. Continue Reading
The XS-11 and the Transition Away from Mandatory Jet Pilot Training for NASA AstronautsBy Jennifer Ross-Nazzal
Flying in space has been associated with pilots ever since 1959, when NASA announced its first class of astronauts, known as the Mercury 7. Part of being a professional astronaut meant you were a certified jet pilot. Even the scientist-astronauts, so named to differentiate them from the astronauts assigned to the Mercury and Gemini missions, selected in 1965 and in 1967, received pilot training. Until NASA better understood the impact of weightlessness on the human body, Robert R. Gilruth, head of the Manned Spacecraft Center (MSC) in Houston, believed all astronauts should meet this qualification. But when five scientist-astronauts from the 1967 class had a rocky transition, leading them to resign—due to their disinterest in flying at the cost of their scientific training and no spaceflight opportunities—it eventually led NASA to rethink their idea of having all astronauts become jet pilots. Continue Reading
Portrait of NASA’s 1967 group of astronauts. Seated at the table, left to right, are Philip K. Chapman, Robert A. R. Parker, William E. Thornton, and John A. Llewellyn. Standing, left to right, are Joseph P. Allen IV, Karl G. Henize, Anthony W. England, Donald L. Holmquest, Story Musgrave, William B. Lenoir, and Brian T. O’Leary.NASA The High-Flying Legacy of Airborne Observation: How Experimental Aircraft Contributed to Astronomy at NASABy Lois Rosson
In June 2011, the Stratospheric Observatory for Infrared Astronomy (SOFIA) chased down Pluto’s occultation of a far-away star. … SOFIA’s 2011 observation of Pluto followed up on a historic 1988 observation made by the airborne Kuiper Airborne Observatory (KAO) that proved that Pluto had an atmosphere at all. The technical versatility of both flights, conducted from aircraft hurtling stabilized telescopes through the air, speaks to the legacy of airborne astronomical observation at NASA. But how did this idiosyncratic format emerge in the first place? Airborne astronomy, in which astronomical observations are made from a moving aircraft, was attempted almost as soon as airplanes themselves were developed. Continue Reading
NASA’s Tortuous Effort to Consolidate its AircraftBy Robert Arrighi
Thirty years ago, on January 6, 1995, NASA Administrator Dan Goldin announced, “We’ve started a revolution at NASA. It’s real. We have a road map for change. We’ve already begun.” Thus began one of the agency’s most daunting endeavors, a top-to-bottom reassessment of NASA’s processes, programmatic assignments, and staffing levels. One of the most controversial aspects of this effort was the proposal to transfer nearly all of the agency’s research aircraft to Dryden Flight Research Center (today known as Armstrong). Continue Reading
Three ER-2 Aircraft in formation over Golden Gate Bridge, San Francisco, CA on their final flight out of NASA Ames Research Center before redeployment to NASA’s Dryden Flight Research Center, now known as NASA Armstrong.NASA/Eric James The Space Between: Mesoscale Lightning Observations and Weather Forecasting, 1965–82By Brad Massey
Skylab astronaut Edward G. Gibson looked down at Earth often during his 84 days on NASA’s first space station. From his orbital vantage point, Gibson took in the breathtaking views of our planet’s diverse landscapes. He also noted the interesting behavior of the planet’s most powerful electrical force: lightning. … Gibson’s words were of great interest to the lightning researchers affiliated with NASA’s Severe Storms and Local Research Program and others who believed observing Earth’s lightning from low Earth orbit generated valuable data that meteorologists could use to better forecast dangerous storm characteristics and behavior. With these motivations in mind, researchers created new Earth- and space-based experiments from the mid-1960s to the first Space Shuttle missions in the early 1980s that observed lightning on a regional level. Continue Reading
Adding Color to the Moon: Jack Kinzler’s Oral History InterviewsBy Sandra Johnson
Manned Spacecraft Center (MSC) Director Robert R. Gilruth placed a call to Jack Kinzler less than four months before the Apollo 11 launch. Gilruth asked him to attend a meeting with a high-level group of individuals from both MSC and NASA Headquarters to discuss ideas for celebrating the first lunar landing. Kinzler, in his capacity as the chief of the Technical Services Division, arrived ready to present his suggestions for commemorating the achievement. Continue Reading
Apollo 11 astronaut Edwin E. “Buzz” Aldrin Jr. poses for a photograph beside the deployed United States flag during the mission’s extravehicular activity (EVA) on the lunar surface.NASA The Founding of the NACABy James Anderson
One hundred ten years ago this month, NASA’s predecessor organization, the National Advisory Committee for Aeronautics (NACA), was founded. The date of the anniversary marks the passage of a rider to a naval appropriations bill that established the NACA for the modest sum of $5,000 annually. Telling the story of the NACA’s founding in this manner—using March 3, 1915, as the moment in time to represent the NACA’s beginning—is true, but it overlooks two crucial aspects of the founding. The founding was both a culmination and a turning point for science and aeronautics in the United States. Continue Reading
Remembering the DC-8 Airborne Science Laboratory at NASABy Bradley Lynn Coleman
The NASA History Office and NASA Earth Science Division cohosted a workshop on the recently retired NASA DC-8 Airborne Science Laboratory (1986–2024) at the Mary W. Jackson NASA Headquarters Building in Washington, DC, October 24 and 25, 2024. The workshop celebrated the history of the legendary aircraft; documented DC-8–enabled scientific, engineering, education, and outreach activities; and captured lessons of the past for future operators. Continue Reading
The DC-8 in flight near Lone Pine, California. NASA/Jim Ross Download the Spring 2025 Edition More Issues of NASA History News and Notes Share Details Last Updated Apr 01, 2025 Related Terms Keep Exploring Discover Related TopicsNASA History
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Ways Community College Students Can Get Involved With NASA
For many students, the path to a NASA career begins at a community college. These local, two-year institutions offer valuable flexibility and options to those aspiring to be part of the nation’s next generation STEM workforce. NASA offers several opportunities for community college students to expand their horizons, make connections with agency experts, add valuable NASA experiences to their resumes, and home in on the types of STEM roles that best fit their skills and interests. Below are some of the exciting NASA activities and experiences available to community college students.
NASA Community College Aerospace ScholarsGet an introduction to NASA, its missions, and its workplace culture through NASA Community College Aerospace Scholars (NCAS). This three-part series enables students to advance their knowledge of the agency, grow their STEM capabilities, interact with NASA experts, and learn about the different pathways to a NASA career.
Mission 1: Discover is a five-week, online orientation course that serves as an introduction to NASA.
Mission 2: Explore is a gamified mission to the Moon or Mars in which students develop a design solution while learning about the agency as a workplace.
Mission 3: Innovate is a three-week hybrid capstone project consisting of two weeks of online preparation and one week participating in a hands-on engineering design challenge at a NASA center.
NCAS begins with Mission 1 and students must complete each mission to be eligible for the next.
Members of a college student team monitor the performance of their robot during a NASA Community College Aerospace Scholars (NCAS) Mission 3: Innovate robotics competition.NASA Student Challenges
NASA’s student challenges and competitions invite students across a range of ages and education levels to innovate and build solutions to many of the agency’s spaceflight and aviation needs – and community college students across the U.S. are eligible for many of these opportunities. In NASA’s Student Launch challenge, each team designs, builds, and tests a high-powered rocket carrying a scientific or engineering payload. In the MUREP Innovation Tech Transfer Idea Competition (MITTIC)Teams from U.S.-designated Minority-Serving Institutions, including community colleges, have the opportunity to brainstorm and pitch new commercial products based on NASA technology.
NASA’s student challenges and competitions are active at varying times throughout the year – new challenges are sometimes added, and existing opportunities evolve – so we recommend students visit the NASA STEM Opportunities and Activities page and research specific challenges to enable planning and preparation for future participation.
NASA’s Student Launch tasks student teams from across the U.S. to design, build, test, and launch a high-powered rocket carrying a scientific or engineering payload. The annual challenge culminates with a final launch in Huntsville, Alabama, home of NASA’s Marshall Space Flight Center.NASA NASA RockOn! and RockSat Programs
Build an experiment and launch it aboard a sounding rocket! Through the hands-on RockOn! and RockSat programs, students gain experience designing and building an experiment to fly as a payload aboard a sounding rocket launched from NASA’s Wallops Flight Facility in Wallops Island, Virginia. In RockOn!, small teams get an introduction to creating a sounding rocket experiment, while RockSat-C and RockSat-X are more advanced experiment flight opportunities.
Students watch as their experiments launch aboard a sounding rocket for the RockSat-X program from NASA’s Wallops Flight Facility Aug. 11, 2022, at 6:09 p.m. EDT. The Terrier-Improved Malemute rocket carried the experiments to an altitude of 99 miles before descending via a parachute and landing in the Atlantic Ocean.NASA Wallops/Terry Zaperach NASA Internships
Be a part of the NASA team! With a NASA internship, students work side-by-side with agency experts, gaining authentic workforce experience while contributing to projects that align with NASA’s goals. Internships are available in a wide variety of disciplines in STEM and beyond, including communications, finance, and more. Each student has a NASA mentor to help guide and coach them through their internship.
NASA interns gain hands-on experience while contributing to agency projects under the guidance of a NASA mentor.NASA National Space Grant College and Fellowship Program
The National Space Grant College and Fellowship Project, better known as Space Grant, is a national network of colleges and universities working to expand opportunities for students and the public to participate in NASA’s aeronautics and space projects. Each state has its own Space Grant Consortium that may provide STEM education and training programs; funding for scholarships and/or internships; and opportunities to take part in research projects, public outreach, state-level student challenges, and more. Programs, opportunities, and offerings vary by state; students should visit their state’s Space Grant Consortium website to find out about opportunities available near them.
Students from the Erie Huron Ottawa Vocational Education Career Center are pictured at the 3KVA Mobile Photovoltaic Power Plant at NASA’s Glenn Research Center.NASA Additional Resources
Discovery Alert: Four Little Planets, One Big Step
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Four rocky planets much smaller than Earth orbit Barnard’s Star, the next closest to ours after the three-star Alpha Centauri system. Barnard’s is the nearest single star.
Key FactsBarnard’s Star, six light-years away, is notorious among astronomers for a history of false planet detections. But with the help of high-precision technology, the latest discovery — a family of four — appears to be solidly confirmed. The tiny size of the planets is also remarkable: Capturing evidence of small worlds at great distance is a tall order, even using state-of-the-art instruments and observational techniques.
DetailsWatching for wobbles in the light from a star is one of the leading methods for detecting exoplanets — planets orbiting other stars. This “radial velocity” technique tracks subtle shifts in the spectrum of starlight caused by the gravity of a planet pulling its star back and forth as the planet orbits. But tiny planets pose a major challenge: the smaller the planet, the smaller the pull. These four are each between about a fifth and a third as massive as Earth. Stars also are known to jitter and quake, creating background “noise” that potentially could swamp the comparatively quiet signals from smaller, orbiting worlds.
Astronomers measure the back-and-forth shifting of starlight in meters per second; in this case the radial velocity signals from all four planets amount to faint whispers — from 0.2 to 0.5 meters per second (a person walks at about 1 meter per second). But the noise from stellar activity is nearly 10 times larger at roughly 2 meters per second.
How to separate planet signals from stellar noise? The astronomers made detailed mathematical models of Barnard’s Star’s quakes and jitters, allowing them to recognize and remove those signals from the data collected from the star.
The new paper confirming the four tiny worlds — labeled b, c, d, and e — relies on data from MAROON-X, an “extreme precision” radial velocity instrument attached to the Gemini Telescope on the Maunakea mountaintop in Hawaii. It confirms the detection of the “b” planet, made with previous data from ESPRESSO, a radial velocity instrument attached to the Very Large Telescope in Chile. And the new work reveals three new sibling planets in the same system.
Fun FactsThese planets orbit their red-dwarf star much too closely to be habitable. The closest planet’s “year” lasts a little more than two days; for the farthest planet, it’s is just shy of seven days. That likely makes them too hot to support life. Yet their detection bodes well in the search for life beyond Earth. Scientists say small, rocky planets like ours are probably the best places to look for evidence of life as we know it. But so far they’ve been the most difficult to detect and characterize. High-precision radial velocity measurements, combined with more sharply focused techniques for extracting data, could open new windows into habitable, potentially life-bearing worlds.
Barnard’s star was discovered in 1916 by Edward Emerson Barnard, a pioneering astrophotographer.
The DiscoverersAn international team of scientists led by Ritvik Basant of the University of Chicago published their paper on the discovery, “Four Sub-Earth Planets Orbiting Barnard’s Star from MAROON-X and ESPRESSO,” in the science journal, “The Astrophysical Journal Letters,” in March 2025. The planets were entered into the NASA Exoplanet Archive on March 13, 2025.
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Sols 4495-4497: Yawn, Perched, and Rollin’
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Sols 4495-4497: Yawn, Perched, and Rollin’ NASA’s Mars rover Curiosity acquired this image of the upcoming “boxwork” structures to its west, using its Chemistry & Camera (ChemCam) Remote Micro-Imager (RMI). The ChemCam instrument studies the chemical composition of rocks and soil, using a laser to vaporize materials, then analyze their elemental composition using an on-board spectrograph. The ChemCam RMI is a high-resolution camera atop the rover’s mast. Curiosity captured this image on March 27, 2025 — Sol 4493, or Martian day 4,493 of the Mars Science Laboratory mission — at 15:35:21 UTC. NASA/JPL-Caltech/LANLWritten by Natalie Moore, Mission Operations Specialist at Malin Space Science Systems
Earth planning date: Friday, March 28, 2025
Womp, womp. Another SRAP (Slip Risk Assessment Process) issue due to wheels being perched on these massive layered sulfate rocks. With our winter power constraints as tight as they are, though, keeping the arm stowed freed up more time to check some lines off our rover’s weekend list. To do: SAM activity to exercise Oven 2 (check!), Navcam 360-degree “phase function” sky movie to monitor scattering of Martian clouds (check!), APXS atmospheric measurements of argon (check!), ChemCam passive sky measurements of oxygen (check!), and a drive of about 50 meters (about 164 feet) to the southwest (check!). Curiosity gets busy on the weekends so us PULs (Payload Uplink Leads) can do some lounging.
On the Mastcam team, we’ve been pretty busy in the layered sulfate unit. The rocks are rippled, layered, fractured, and surrounded by sandy troughs. Where did it all come from? What current and past processes are at play in this area? This weekend we’re collecting 70 images to help figure that out. ChemCam is helping by collecting chemistry measurements of the lowest block in this Navcam image, with two targets close by aptly named “Solana Beach” and “Del Mar.” To help conserve power, we’ve been trying to parallelize our activities as much as possible. Recently this means Mastcam has been taking images while ChemCam undergoes “TEC Cooling” (with the Thermo-Electric Cooler) to get as cold as possible before using their laser.
We’re all hoping the arm can come back from vacation next week.
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ARMD Solicitations (ULI Proposals Invited)
7 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA / Lillian Gipson/Getty ImagesThis ARMD solicitations page compiles the opportunities to collaborate with NASA’s aeronautical innovators and/or contribute to their research to enable new and improved air transportation systems. A summary of available opportunities with key dates requiring action are listed first. More information about each opportunity is detailed lower on this page.
University Leadership Initiative
Step-A proposals due by June 26, 2025.
University Student Research Challenge
Proposals for Cycle 3 are due by June 26, 2025.
GENERAL ANNOUNCEMENT OF REQUEST FOR INFORMATION
Advanced Capabilities for Emergency Response Operations is using this request for information to identify technologies that address current challenges facing the wildland firefighting community. NASA is seeking information on data collection, airborne connectivity and communications solutions, unmanned aircraft systems traffic management, aircraft operations and autonomy, and more. This will support development of a partnership strategy for future collaborative demonstrations.
Interested parties were requested to respond to this notice with an information package no later than 4 pm ET, October 15, 2023, that shall be submitted via https://nari.arc.nasa.gov/acero-rfi. Any proprietary information must be clearly marked. Submissions will be accepted only from United States companies.
View the full RFI Announcement here.
Advanced Air Mobility MissionGENERAL ADVANCED AIR MOBILITY
ANNOUNCEMENT OF REQUEST FOR INFORMATION
This request for information (RFI) is being used to gather market research for NASA to make informed decisions regarding potential partnership strategies and future research to enable Advanced Air Mobility (AAM). NASA is seeking information from public, private, and academic organizations to determine technical needs and community interests that may lead to future solicitations regarding AAM research and development.
This particular RFI is just one avenue of multiple planned opportunities for formal feedback on or participation in NASA’s AAM Mission-related efforts to develop these requirements and help enable AAM.
The respond by date for this RFI closed on Feb. 1, 2025, at 6 p.m. EST.
View the full RFI announcement here.
NASA Research Opportunities in AeronauticsNASA’s Aeronautics Research Mission Directorate (ARMD) uses the NASA Research Announcement (NRA) process to solicit proposals for foundational research in areas where ARMD seeks to enhance its core capabilities.
Competition for NRA awards is open to both academia and industry.
The current open solicitation for ARMD Research Opportunities is ROA-2023 and ROA-2024.
Here is some general information to know about the NRA process.
- NRA solicitations are released by NASA Headquarters through the Web-based NASA Solicitation and Proposal Integrated Review and Evaluation System (NSPIRES).
- All NRA technical work is defined and managed by project teams within these four programs: Advanced Air Vehicles Program, Airspace Operations and Safety Program, Integrated Aviation Systems Program, and Transformative Aeronautics Concepts Program.
- NRA awards originate from NASA’s Langley Research Center in Virginia, Ames Research Center in California, Glenn Research Center in Cleveland, and Armstrong Flight Research Center in California.
- Competition for NRA awards is full and open.
- Participation is open to all categories of organizations, including educational institutions, industry, and nonprofits.
- Any updates or amendments to an NRA is posted on the appropriate NSPIRES web pages as noted in the Amendments detailed below.
- ARMD sends notifications of NRA updates through the NSPIRES email system. In order to receive these email notifications, you must be a Registered User of NSPIRES. However, note that NASA is not responsible for inadvertently failing to provide notification of a future NRA. Parties are responsible for regularly checking the NSPIRES website for updated NRAs.
Amendment 1
Amendment 1 to the NASA ARMD Research Opportunities in Aeronautics (ROA) 2024 NRA has been posted on the NSPIRES web site at https://nspires.nasaprs.com.
The announcement solicits proposals from accredited U.S. institutions for research training grants to begin the academic year. This NOFO is designed to support independently conceived research projects by highly qualified graduate students, in disciplines needed to help advance NASA’s mission, thus affording these students the opportunity to directly contribute to advancements in STEM-related areas of study. AAVP Fellowship Opportunities are focused on innovation and the generation of measurable research results that contribute to NASA’s current and future science and technology goals.
Research proposals are sought to address key challenges provided in Elements of Appendix A.8.
Notices of Intent (NOIs) are not required.
A budget breakdown for each proposal is required, detailing the allocation of the award funds by year. The budget document may adhere to any format or template provided by the applicant’s institution.
Proposals were due by April 30, 2024, at 5 PM ET.
Amendment 2
UPDATED ON MARCH 31, 2025
University Leadership Initiative (ULI) provides the opportunity for university teams to exercise technical and organizational leadership in proposing unique technical challenges in aeronautics, defining multi-disciplinary solutions, establishing peer review mechanisms, and applying innovative teaming strategies to strengthen the research impact.
Research proposals are sought in six ULI topic areas in Appendix D.4.
Topic 1: Safe, Efficient Growth in Global Operations (Strategic Thrust 1)
Topic 2: Innovation in Commercial High-Speed Aircraft (Strategic Thrust 2)
Topic 3: Ultra-Efficient Subsonic Transports (Strategic Thrust 3)
Topic 4: Safe, Quiet, and Affordable Vertical Lift Air Vehicles (Strategic Thrust 4)
Topic 5: In-Time System-Wide Safety Assurance (Strategic Thrust 5)
Topic 6: Assured Autonomy for Aviation Transformation (Strategic Thrust 6)
This NRA will utilize a two-step proposal submission and evaluation process. The initial step is a short mandatory Step-A proposal, which is due June 26, 2025. Those offerors submitting the most highly rated Step-A proposals will be invited to submit a Step-B proposal. All proposals must be submitted electronically through NSPIRES at https://nspires.nasaprs.com. An Applicant’s Workshop will be held on Thursday April 30, 2025; 1:00-3:00 p.m. ET (https://uli.arc.nasa.gov/applicants-workshops/workshop9) (Page will be live closer to the event.)
An interested partners list for this ULI is at https://uli.arc.nasa.gov/partners. To be listed as an interested lead or partner, please send electronic mail to hq-univpartnerships@mail.nasa.gov with “ULI Partnerships” in the subject line and include the information required for the table in that web page.
Amendment 3
Commercial Supersonic Technology seeks proposals for a fuel injector design concept and fabrication for testing at NASA Glenn Research Center.
The proposal for the fuel injector design aims to establish current state-of-the-art in low NOx supersonic cruise while meeting reasonable landing take-off NOx emissions. The technology application timeline is targeted for a supersonic aircraft with entry into service in the 2035+ timeframe.
These efforts are in alignment with activities in the NASA Aeronautics Research Mission Directorate as outlined in the NASA Aeronautics Strategic Implementation Plan, specifically Strategic Thrust 2: Innovation in Commercial High-Speed Aircraft.
Proposals were due by May 31, 2024 at 5 pm EDT.
Amendment 4
UPDATED ON JANUARY 16, 2025
University Student Research Challenge seeks to challenge students to propose new ideas/concepts that are relevant to NASA Aeronautics. USRC will provide students, from accredited U.S. colleges or universities, with grants for their projects and with the challenge of raising cost share funds through a crowdfunding campaign. The process of creating and implementing a crowdfunding campaign acts as a teaching accelerator – requiring students to act like entrepreneurs and raise awareness about their research among the public.
The solicitation goal can be accomplished through project ideas such as advancing the design, developing technology or capabilities in support of aviation, by demonstrating a novel concept, or enabling advancement of aeronautics-related technologies.
Notices of Intent are not required for this solicitation.
Proposals for Cycle 3 are due June 26, 2025.
Proposals can also be submitted later and evaluated in the second and third cycles.
The USRC Q&A/Info Session and Proposal Workshop will be held on the days/times below. Please join us on TEAMS using the Meeting Link, or call in via +1 256-715-9946,,317928116#.
USRC CycleInformation Session/Q&A DateProposal Due DateCycle 1Sept. 20, 2024 at 2 pm ETNov. 7, 2024Cycle 2Jan. 27, 2025 at 2 pm ETMarch 13, 2025Cycle 3May 12, 2024 at 2 pm ETJune 26, 2025 Keep Exploring See More About NASA AeronauticsAeronautics STEM
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Share Details Last Updated Mar 31, 2025 EditorJim BankeContactJim Bankejim.banke@nasa.gov Related TermsNASA Trains for Orion Water Recovery Ahead of Artemis II Launch
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) The Crew Module Test Article (CMTA), a full scale mockup of the Orion spacecraft, is seen in the Pacific Ocean as teams practice Artemis recovery operations during Underway Recovery Test-12 onboard USS Somerset off the coast of California, Saturday, March 29, 2025. NASA/Bill IngallsPreparations for NASA’s next Artemis flight recently took to the seas as a joint NASA and Department of Defense team, led by NASA’s Exploration Ground Systems Program, spent a week aboard the USS Somerset off the coast of California practicing procedures for recovering the Artemis II spacecraft and crew.
Following successful completion of Underway Recovery Test-12 (URT-12) on Monday, NASA’s Landing and Recovery team and their Defense Department counterparts are certified to recover the Orion spacecraft as part of the upcoming Artemis II test flight that will send NASA astronauts Reid Wiseman, Victor Glover, and Christina Koch, as well as CSA (Canadian Space Agency) astronaut Jeremy Hansen, on a 10-day journey around the Moon.
“This will be NASA’s first crewed mission to the Moon under the Artemis program,” said Lili Villarreal, the landing and recovery director for Artemis II. “A lot of practice led up to this week’s event, and seeing everything come together at sea gives me great confidence that the air, water, ground, and medical support teams are ready to safely recover the spacecraft and the crew for this historic mission.”
A wave breaks inside the well deck of USS Somerset as teams work to recover the Crew Module Test Article (CMTA), a full scale replica of the Orion spacecraft, as they practice Artemis recovery operations during Underway Recovery Test-12 off the coast of California, Thursday, March 27, 2025.NASA/Joel KowskyOnce Orion reenters Earth’s atmosphere, the capsule will keep the crew safe as it slows from nearly 25,000 mph to about 325 mph. Then its system of 11 parachutes will deploy in a precise sequence to slow the capsule and crew to a relatively gentle 20 mph for splashdown off the coast of California. From the time it enters Earth’s atmosphere, the Artemis II spacecraft will fly 1,775 nautical miles to its landing spot in the Pacific Ocean. This direct approach allows NASA to control the amount of time the spacecraft will spend in extremely high temperature ranges.
The Artemis II astronauts trained during URT-11 in February 2024, when they donned Orion Crew Survival System suits and practiced a range of recovery operations at sea using the Crew Module Test Article, a stand -in for their spacecraft.
For the 12th training exercise, NASA astronauts Deniz Burnham and Andre Douglas, along with ESA (European Space Agency) astronaut Luca Parmitano, did the same, moving from the simulated crew module to USS Somerset, with helicopters, a team of Navy divers in small boats, NASA’s open water lead – a technical expert and lead design engineer for all open water operations – as well as Navy and NASA medical teams rehearsing different recovery scenarios.
Grant Bruner, left, and Gary Kirkendall, right, Orion suit technicians, are seen with ESA (European Space Agency) astronaut Luca Parmitano, second from left, and NASA astronauts Deniz Burnham, center, and Andre Douglas, as they prepare to take part in Artemis recovery operations as part of Underway Recovery Test-12 onboard USS Somerset off the coast of California, Thursday, March 27, 2025. NASA/Joel Kowsky“Allowing astronauts to participate when they are not directly involved in a mission gives them valuable experience by exposing them to a lot of different scenarios,” said Glover, who will pilot Artemis II. “Learning about different systems and working with ground control teams also broadens their skillsets and prepares them for future roles. It also allows astronauts like me who are assigned to the mission to experience other roles – in this case, I am serving in the role of Joe Acaba, Chief of the Astronaut Office.”
NASA astronaut and Artemis II pilot Victor Glover, right, speaks to NASA astronauts Andre Douglas and Deniz Burnham as they prepare to take part in practicing Artemis recovery procedures during Underway Recovery Test-12 onboard USS Somerset off the coast of California, Friday, March 28, 2025.NASA/Joel Kowsky NASA astronaut Deniz Burnham smiles after landing in a Navy helicopter onboard USS Somerset during Underway Recovery Test-12 off the coast of California, Thursday, March 27, 2025.NASA/Bill IngallsAs the astronauts arrive safely at the ship for medical checkouts, recovery teams focus on returning the spacecraft and its auxiliary ground support hardware to the amphibious transport dock.
Navy divers attach a connection collar to the spacecraft and an additional line to a pneumatic winch inside the USS Somerset’s well deck, allowing joint NASA and Navy teams to tow Orion toward the ship. A team of sailors and NASA recovery personnel inside the ship manually pull some of the lines to help align Orion with its stand, which will secure the spacecraft for its trip to the shore. Following a safe and precise recovery, sailors will drain the well deck of water, and the ship will make its way back to Naval Base San Diego.
The Artemis II test flight will confirm the foundational systems and hardware needed for human deep space exploration, taking another step toward missions on the lunar surface and helping the agency prepare for human missions to Mars.
About the AuthorAllison TankersleyPublic Affairs Specialist Share Details Last Updated Mar 31, 2025 Related Terms Explore More 5 min read NASA’s SPHEREx Takes First Images, Preps to Study Millions of Galaxies Article 7 hours ago 5 min read Old Missions, New Discoveries: NASA’s Data Archives Accelerate ScienceEvery NASA mission represents a leap into the unknown, collecting data that pushes the boundaries…
Article 1 day ago 5 min read 20-Year Hubble Study of Uranus Yields New Atmospheric InsightsThe ice-giant planet Uranus, which travels around the Sun tipped on its side, is a…
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Artemis II Core Stage Integration – Complete!
Technicians from NASA and primary contractor Amentum join the SLS (Space Launch System) rocket with the stacked solid rocket boosters for the Artemis II mission at NASA’s Kennedy Space Center in Florida on March 23, 2025. The core stage is the largest component of the rocket, standing 212 feet tall and weighing about 219,000 pounds with its engines. The stage is the backbone of the rocket, supporting the launch vehicle stage adapter, interim cryogenic propulsion stage, Orion stage adapter, and the Orion spacecraft.
Artemis II is the first crewed test flight under NASA’s Artemis campaign and is another step toward missions on the lunar surface and helping the agency prepare for future human missions to Mars.
Image credit: NASA/Frank Michaux
Career Spotlight: Technologist (Ages 14-18)
Technologists are professionals who research, develop, and test emerging technologies. They also find useful ways to put new technologies to work. A technologist is an expert in a specific type of technology, often within a specific field. Many industries rely on innovations developed by technologists. Some of these include aerospace, research, manufacturing, healthcare, and information technology.
NASA technologists make use of technological advancements to improve NASA’s capabilities and better meet the needs of its missions. They also oversee how technologies developed by NASA can improve life on Earth through commercial products. These products are called spinoffs. For examples of how NASA shows up in your everyday life, visit: https://spinoff.nasa.gov.
What are some technology careers at NASA?Instrument scientist: Works to improve or develop instruments that collect data. In aerospace, an instrument is a sensor or other device that takes measurements or gathers scientific information. This role may include working with other specialties to design, create, and test scientific instruments.
Data scientist: Uses computer science to create tools that manage data. Some of the tasks a data scientist might perform include developing predictive models, machine learning algorithms, or software to extract useful information from large sets of data.
Information technology (IT) specialist: Designs, maintains, implements, and protects IT systems across the agency. Develops software, manages IT projects, and develops applications to support both organizational and mission operations.
One of three small lunar rovers that are part of a NASA technology demonstration called CADRE (Cooperative Autonomous Distributed Robotic Exploration) is prepared for shipping in a clean room at the agency’s Jet Propulsion Laboratory in Southern California.NASA/JPL-Caltech How can I become a technologist?There are many different types of careers in technology, and the requirements vary. While you’re in high school, explore the possibilities and learn about the specialties and roles that will fit your interests. Then, investigate the academic path and experience you’ll need to eventually be hired into those roles. Current job openings, guidance counselors, and mentors can shed light on the types of certifications or degrees required. With this information, you can begin planning for the skills and education you’ll need.
It’s important to remember that technology is always advancing. Even after you’ve launched your technologist career, a “lifelong learning” mindset will help you keep up with new innovations and skills.
How can I start preparing today to become a technologist?Start growing your technology skills today with hands-on activities created by NASA STEM. Looking for something more involved? Many of NASA’s student challenges, competitions, and activities offer authentic experience in aerospace technology, computer science, and more.
Students aged 16 and up who are U.S. citizens are eligible to apply for a paid NASA internship. Interns work on real projects with the guidance of a NASA mentor. Internship sessions are held each year in spring, summer, and fall; visit NASA’s Internships website to learn about important deadlines and current opportunities.
Frank Pena, test director, checks on the 10-foot Mock Truss-Braced Wing at NASA’s Armstrong Flight Research Center in Edwards, California. The aircraft concept involves a wing braced on an aircraft using diagonal struts that also add lift and could result in significantly improved aerodynamics.NASA Advice from NASA technologists“Think about your personal interests and passions, and also the impact you’d like your work to have. What do you feel personally interested in when it comes to science and technology? Is there a problem that you think is very important for our society to solve? Often there is a research or technology field that can combine those two things!” – Olivia Tyrrell, NASA research engineer
What do you feel personally interested in when it comes to science and technology?Olivia Tyrrell
NASA Research Engineer
“If you like to create things or find solutions to problems, working in technology is a great choice. Scientists identify problems, engineers solve problems, but ultimately, we need to create new technologies, new things, new gadgets. Technologists are building the next generation toolbox for engineers and scientists to pull from, enabling everyone to solve problems in more effective and innovative ways. (Technologists invent things… what’s cooler than that?!)” – Kristen John, technical integration manager for lunar dust mitigation
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Career Spotlight: Scientist (Ages 14-18)
Science is about exploring answers to questions. A scientist uses research and evidence to form hypotheses, test variables, and then share their findings.
NASA scientists conduct groundbreaking research to answer some of humanity’s most profound questions. Most scientists start as project scientists in their early careers. They spend a lot of time publishing their peer-reviewed literature and presenting scientific research. Senior-level scientists provide leadership in the NASA community, actively publish research group work, and take on management roles.
What are some of the different types of scientists that work at NASA?Many types of scientists work at NASA to support its wide variety of missions. The agency’s scientists research the foods we send to space, the habitability of other planets, the weather in space, and so much more. Here are a few examples of types of scientists at NASA.
Planetary scientist: Discovers and studies the planetary objects in our solar system. These efforts shed light on the history of the solar system and the distribution of life within it.
Astrobiologist: Studies the origins of life, how life evolves, and where it might be found in the universe.
Astrophysicist: Studies the physical and chemical structures of stars, planets, and other natural objects found in space.
Biological/physical scientist: Studies how biological and physical processes work in challenging environments like space. This information helps NASA design longer human space missions and also benefits life on Earth.
Earth scientist: Uses observations and data from satellites and other sources to study Earth’s atmosphere, oceans, land cover, and land use.
Heliophysicist: Studies the Sun and its behaviors, such as magnetic fields, solar wind, and space weather. This knowledge helps us better understand and predict the Sun’s effects on Earth and in space.
How can I become a scientist?Focus on building your scientific knowledge and skills. You can do this by taking challenging academic courses, participating in science fairs, and joining extracurricular activities that have a scientific focus. This is also a good time to research what types of sciences you’re most interested in, possible careers in those fields, and academic degrees required for those jobs.
Scientists typically need at least a four-year degree. Most pursue a master’s degree or even a doctorate (Ph.D.) to become experts in their field.
How can I start preparing today to become a scientist?Interested in applying some science skills right away? NASA provides a variety of hands-on activities for a range of skill levels. The space agency also offers student challenges, competitions, and activities that provide authentic experience in a variety of science fields. For up-to-date opportunities, visit:
NASA also offers paid internships for U.S. citizens aged 16 and up. Interns work on real projects with the guidance of a NASA mentor. Internship sessions are held each year in spring, summer, and fall; visit NASA’s Internships website to learn about important deadlines and current opportunities.
Advice from NASA scientists“Take advantage of opportunities in different fields like attending summer classes, volunteering on the weekends, visiting museums, attending community lectures, and reading introductory books at the library. These are a few ways to expand your scope of possibility within the sciences, while simultaneously narrowing your focus in a field.” – Angela Garcia, exploration geologist
“The key to being a scientist is to love asking questions. If you are fascinated about how and why things work — you are already a scientist.”Nicola Fox
NASA Associate Administrator, Science Mission Directorate
“One general skill that is often overlooked is the ability to write well and clearly. There’s a misconception that being a scientist means using big words and writing in ways that no one understands, when it’s actually the opposite. The ability to communicate your thoughts and ideas so that a child can understand is not easy, but it’s essential for good scientific writing.” – Matt Mickens, NASA horticulturist
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20-Year Hubble Study of Uranus Yields New Atmospheric Insights
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NASA, ESA, Erich Karkoschka (LPL)
The ice-giant planet Uranus, which travels around the Sun tipped on its side, is a weird and mysterious world. Now, in an unprecedented study spanning two decades, researchers using NASA’s Hubble Space Telescope have uncovered new insights into the planet’s atmospheric composition and dynamics. This was possible only because of Hubble’s sharp resolution, spectral capabilities, and longevity.
The team’s results will help astronomers to better understand how the atmosphere of Uranus works and responds to changing sunlight. These long-term observations provide valuable data for understanding the atmospheric dynamics of this distant ice giant, which can serve as a proxy for studying exoplanets of similar size and composition.
When Voyager 2 flew past Uranus in 1986, it provided a close-up snapshot of the sideways planet. What it saw resembled a bland, blue-green billiard ball. By comparison, Hubble chronicled a 20-year story of seasonal changes from 2002 to 2022. Over that period, a team led by Erich Karkoschka of the University of Arizona, and Larry Sromovsky and Pat Fry from the University of Wisconsin used the same Hubble instrument, STIS (the Space Telescope Imaging Spectrograph), to paint an accurate picture of the atmospheric structure of Uranus.
Uranus’ atmosphere is mostly hydrogen and helium, with a small amount of methane and traces of water and ammonia. The methane gives Uranus its cyan color by absorbing the red wavelengths of sunlight.
The Hubble team observed Uranus four times in the 20-year period: in 2002, 2012, 2015, and 2022. They found that, unlike conditions on the gas giants Saturn and Jupiter, methane is not uniformly distributed across Uranus. Instead, it is strongly depleted near the poles. This depletion remained relatively constant over the two decades. However, the aerosol and haze structure changed dramatically, brightening significantly in the northern polar region as the planet approaches its northern summer solstice in 2030.
The image columns show the change of Uranus for the four years that STIS observed Uranus across a 20-year period. Over that span of time, the researchers watched the seasons of Uranus as the south polar region darkened going into winter shadow while the north polar region brightened as northern summer approaches. NASA, ESA, Erich Karkoschka (LPL)Uranus takes a little over 84 Earth years to complete a single orbit of the Sun. So, over two decades, the Hubble team has only seen mostly northern spring as the Sun moves from shining directly over Uranus’ equator toward shining almost directly over its north pole in 2030. Hubble observations suggest complex atmospheric circulation patterns on Uranus during this period. The data that are most sensitive to the methane distribution indicate a downwelling in the polar regions and upwelling in other regions.
The team analyzed their results in several ways. The image columns show the change of Uranus for the four years that STIS observed Uranus across a 20-year period. Over that span of time, the researchers watched the seasons of Uranus as the south polar region (left) darkened going into winter shadow while the north polar region (right) brightened as it began to come into a more direct view as northern summer approaches.
The top row, in visible light, shows how the color of Uranus appears to the human eye as seen through even an amateur telescope.
In the second row, the false-color image of the planet is assembled from visible and near-infrared light observations. The color and brightness correspond to the amounts of methane and aerosols. Both of these quantities could not be distinguished before Hubble’s STIS was first aimed at Uranus in 2002. Generally, green areas indicate less methane than blue areas, and red areas show no methane. The red areas are at the limb, where the stratosphere of Uranus is almost completely devoid of methane.
The two bottom rows show the latitude structure of aerosols and methane inferred from 1,000 different wavelengths (colors) from visible to near infrared. In the third row, bright areas indicate cloudier conditions, while the dark areas represent clearer conditions. In the fourth row, bright areas indicate depleted methane, while dark areas show the full amount of methane.
At middle and low latitudes, aerosols and methane depletion have their own latitudinal structure that mostly did not change much over the two decades of observation. However, in the polar regions, aerosols and methane depletion behave very differently.
In the third row, the aerosols near the north pole display a dramatic increase, showing up as very dark during early northern spring, turning very bright in recent years. Aerosols also seem to disappear at the left limb as the solar radiation disappeared. This is evidence that solar radiation changes the aerosol haze in the atmosphere of Uranus. On the other hand, methane depletion seems to stay quite high in both polar regions throughout the observing period.
Astronomers will continue to observe Uranus as the planet approaches northern summer.
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, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.
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University High Triumphs at JPL-Hosted Ocean Sciences Bowl
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) This team from University High School in Irvine, California, won the 2025 regional Oceans Science Bowl, hosted by NASA’s Jet Propulsion Laboratory. From left: Nethra Iyer, Joanne Chen, Matthew Feng, Avery Hexun, Angelina Yan, and coach David Knight.NASA/JPL-CaltechThe annual regional event puts students’ knowledge of ocean-related science to the test in a fast-paced academic competition.
A team of students from University High School in Irvine earned first place at a fast-paced regional academic competition focused on ocean science disciplines and hosted by NASA’S Jet Propulsion Laboratory in Southern California.
Eight teams from Los Angeles and Orange counties competed at the March 29 event, dubbed the Los Angeles Surf Bowl. It was the last of about 20 regional competitions held across the U.S. this year in the lead-up to the virtual National Ocean Sciences Bowl finals event in mid-May.
Santa Monica High School earned second place; Francisco Bravo Medical Magnet High School in Los Angeles came in third. With its victory, University repeated its winning performance from last year. The school also won the JPL-hosted regional Science Bowl earlier this month.
Teams from all eight schools that participated in the JPL-hosted 2025 regional Ocean Sciences Bowl pose alongside volunteers and coaches.NASA/JPL-CaltechFor the Ocean Sciences Bowl, teams are composed of four to five students and a coach. To prepare for the event, team members spend months answering multiple-choice questions with a “Jeopardy!”-style buzzer in just five seconds. Questions come in several categories, including biology, chemistry, geology, and physics along with related geography, technology, history, policy, and current events topics.
A question in the chemistry category might be “What chemical is the principal source of energy at many of Earth’s hydrothermal vent systems?” (It’s hydrogen sulfide.) Other questions can be considerably more challenging.
When a team member buzzes in and gives the correct answer to a multiple-choice question, the team earns a bonus question, which allows teammates to consult with one another to come up with an answer. More complicated “team challenge questions” prompt students to work together for a longer period. The theme of this year’s competition is “Sounding the Depths: Understanding Ocean Acoustics.”
University High junior Matthew Feng, a return competitor, said the team’s success felt like a payoff for hours of studying together, including on weekends. He keeps coming back to the competition partly for the sense of community and also for the personal challenge, he said. “It’s nice to compete and meet people, see people who were here last year,” Matthew added. “Pushing yourself mentally — the first year I was shaking so hard because I wasn’t used to that much adrenaline.”
Since 2000, JPL’s Public Services Office has coordinated the Los Angeles regional contest with the help of volunteers from laboratory staff and former Ocean Sciences Bowl participants in the local community. JPL is managed for NASA by Caltech.
The National Ocean Sciences Bowl is a program of the Center for Ocean Leadership at the University Corporation for Atmospheric Research, a nonprofit consortium of colleges and universities focused in part on Earth science-related education.
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Share Details Last Updated Mar 31, 2025 Related Terms Explore More 6 min read NASA’s Curiosity Rover Detects Largest Organic Molecules Found on MarsResearchers analyzing pulverized rock onboard NASA’s Curiosity rover have found the largest organic compounds on…
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El X-59 de la NASA completa la prueba de ‘control de crucero’ mantenimiento automático de velocidad del motor
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Preparations for Next Moonwalk Simulations Underway (and Underwater) El avión de investigación supersónico silencioso X-59 de la NASA se encuentra en una rampa de Lockheed Martin Skunk Works en Palmdale, California, durante el atardecer. Esta aeronave única en su tipo es propulsada por un motor General Electric F414, una variante de los motores utilizados en los aviones F/A-18. El motor está montado sobre el fuselaje para reducir la cantidad de ondas de choque que llegan al suelo. El X-59 es la pieza central de la misión Quesst de la NASA, que busca demostrar el vuelo supersónico silencioso y permitir futuros viajes comerciales sobre tierra – más rápidos que la velocidad del sonido.Lockheed Martin Corporation/Garry Tice El avión de investigación supersónico silencioso X-59 de la NASA se encuentra en una rampa de Lockheed Martin Skunk Works en Palmdale, California, durante el atardecer. Esta aeronave única en su tipo es propulsada por un motor General Electric F414, una variante de los motores utilizados en los aviones F/A-18. El motor está montado sobre el fuselaje para reducir la cantidad de ondas de choque que llegan al suelo. El X-59 es la pieza central de la misión Quesst de la NASA, que busca demostrar el vuelo supersónico silencioso y permitir futuros viajes comerciales sobre tierra – más rápidos que la velocidad del sonido.Lockheed Martin Corporation/Garry TiceRead this story in English here.
El equipo detrás del X-59 de la NASA completó en marzo otra prueba crítica en tierra, garantizando que el silencioso avión supersónico será capaz de mantener una velocidad específica durante su funcionamiento. Esta prueba, conocida como mantenimiento automático de velocidad del motor, es el más reciente marcador de progreso a medida que el X-59 se acerca a su primer vuelo este año.
“El mantenimiento automático de la velocidad del motor es básicamente la versión de control de crucero de la aeronave,” explicó Paul Dees, jefe adjunto de propulsión de la NASA del X-59 en el Centro de Investigación de Vuelo Armstrong de la agencia en Edwards, California. “El piloto activa el control de velocidad a su velocidad actual y luego puede aumentarla o ajustarla gradualmente según sea necesario.”
El equipo del X-59 ya había realizado una prueba similar en el motor, pero sólo como un sistema aislado. La prueba de marzo verificó que la retención de velocidad funciona correctamente tras su integración en la aviónica de la aeronave.
“Necesitábamos verificar que el mantenimiento automático de velocidad funcionara no sólo dentro del propio motor, sino como parte de todo el sistema del avión,” explicó Dees. “Esta prueba confirmó que todos los componentes – software, enlaces mecánicos y leyes de control – funcionan juntos según lo previsto.”
El éxito de la prueba confirmó la habilidad de la aeronave para controlar la velocidad con precisión, lo cual será muy invaluable durante el vuelo. Esta capacidad aumentará la seguridad de los pilotos, permitiéndoles enfocarse en otros aspectos críticos de la operación de vuelo.
“El piloto va a estar muy ocupado durante el primer vuelo, asegurándose de que la aeronave sea estable y controlable,” dijo Dees. “Al tener la función del mantenimiento automático de velocidad, de reduce parte de esa carga de trabajo, lo que hace que el primer vuelo sea mucho más seguro.”
Inicialmente el equipo tenía planeado comprobar el mantenimiento automático de velocidad como parte de una próxima serie de pruebas en tierra donde alimentarían la aeronave con un sólido conjunto de datos para verificar su funcionalidad tanto en condiciones normales como de fallo, conocidas como pruebas de pájaro de aluminio (una estructura que se utiliza para probar los sistemas de una aeronave en un laboratorio, simulando un vuelo real). Sin embargo, el equipo se dio cuenta que había una oportunidad de probarlo antes.
“Fue un objetivo de oportunidad,” dijo Dees. “Nos dimos cuenta de que estábamos listos para probar el mantenimiento automático de velocidad del motor por separado mientras otros sistemas continuaban con la finalización de su software. Si podemos aprender algo antes, siempre es mejor.”
Con cada prueba exitosa, el equipo integrado de la NASA y Lockheed Martin acerca el X-59 al primer vuelo, y hacer historia en la aviación a través de su tecnología supersónica silenciosa.
Artículo Traducido por: Priscila Valdez
Share Details Last Updated Mar 31, 2025 EditorDede DiniusContactNicolas Cholulanicolas.h.cholula@nasa.gov Related Terms Keep Exploring Discover More Topics From NASAArmstrong Flight Research Center
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She Speaks for the Samples: Meet Dr. Juliane Gross, Artemis Campaign Sample Curation Lead
Based at NASA’s Johnson Space Center in Houston, the Astromaterials Research and Exploration Science Division, or ARES, curates the most extensive collection of extraterrestrial materials on Earth, ranging from microscopic cosmic dust particles to Apollo-era Moon rocks. Soon, ARES’ team of world-leading sample scientists hopes to add something new to its collection – lunar samples from the Moon’s South Pole region.
As the Artemis campaign sample curation lead, Dr. Juliane Gross is helping ARES and NASA prepare to collect and return those samples safely. “I’m responsible for representing the voice of the Moon rocks and advocating for their protection, preservation, and maintaining their integrity during the planning and execution of all stages of the different Artemis sample return missions,” she said.
Juliane Gross leads a geology lesson for Artemis II crew members as part of their field training in Iceland in 2024.NASAHer multifaceted role includes preparing the Johnson facility that will receive new lunar samples, developing curation strategies, and collaborating with mission teams to plan sampling operations, which encompass collection, handling, transport, and storage processes for all stages of Artemis missions. She trains program managers and engineers on the importance of sample return and teaches crew members how to identify lunar samples and collect them without contamination. She also works with the different programs and teams that oversee the vehicles used at different stages of lunar missions – collaborating with the human landing system team around tool storage and delivery to the lunar surface, the Orion Program to coordinate sample stowage for the return to Earth, and Exploration Ground Systems to plan sample recovery after splashdown.
Once samples are returned to Earth, Gross and the ARES curation team will conduct a preliminary examination of the materials and release a sample catalog from which members of the global scientific community may request loans to carry out their respective research.
Working across Artemis teams raised an unexpected but fun challenge for Gross – learning to communicate effectively with colleagues who have different academic and professional backgrounds. “Scientists like me speak a different language than engineers, and we all speak a different language than managers or the general public,” she said. “I have worked hard to find common vocabulary and to ‘translate’ science needs into the different types of languages that exist within the Artemis campaign. I’m trying to use our differences as strengths to enable mission success and to connect and build relationships with all these different teams through my love and passion for the Moon and rocks from the Moon.”
That passion emerged shortly after Gross completed her Ph.D. in geology, while working on lunar samples with the Lunar and Planetary Institute. She went on to become a research scientist with the American Museum of Natural History in New York, and then a tenured professor of planetary sciences at Rutgers University in Piscataway, New Jersey.
In 2019, NASA asked Gross to join the Apollo Next Generation Sample Analysis Program. Under the program, NASA preserved some of the 382 kilograms of lunar samples returned by Apollo missions, keeping them sealed for future generations to open and analyze. “NASA had the foresight to understand that technology would evolve and our level of sophistication for handling and examining samples would greatly increase,” Gross said.
She and two other scientists had the incredible opportunity to open and examine two samples returned by Apollo 17. Their work served as a practice run for Artemis sample returns while building upon the fundamental insights into the shared origin and history of Earth and the Moon that scientists previously derived from other Apollo samples. For example, the team extracted gas from one sample that will provide information about the volatiles that future lunar missions may encounter around the Moon’s South Pole.
“The Apollo Next Generation Sample Analysis Program linked the first generation of lunar explorers from Apollo with future explorers of the Moon with Artemis,” Gross said. “I’m very proud to have played such an important role in this initiative that now feeds forward to Artemis.”
Juliane Gross examines lunar samples returned by Apollo 17 in Johnson Space Center’s Lunar Sample Laboratory Facility. NASAGross’ connection with NASA began even earlier in her career. She was selected to join the agency-sponsored Antarctic Search for Meteorites team and lived in the deep ice fields of Antarctica for two months with seven other people. “We lived in tiny two-person tents without any support and recovered a total of 263 space rocks under challenging conditions,” she said. “I experienced the powerful forces of Antarctica and traveled 332 miles on skidoos. My body changed in the cold – I stuffed my face with enough butter, chocolate, and peanut M&Ms to last a lifetime and yet I lost weight.”
This formative experience taught Gross to find and celebrate beauty, even in her toughest moments. “I drank tea made with Antarctic glacier ice that is thousands to millions of years old. I will never forget the beautiful bell-like sounds that snow crystals make when being blown across the ice, the rainbow-sparkling ice crystals on a really cold day, the vast expanses of ice sheets looking like oceans frozen in eternity, and the icy bite of the wind on any unprotected skin that made me feel so alive and reminded me how vulnerable and precious life is,” she said. “And I will never ever forget the thrill and utter joy of finding a meteorite that you know no one on this planet has ever seen before you.”
Gross ultimately received the Antarctica Service Medal of the United States Armed Forces from the U.S. Department of Defense for her work.
Juliane Gross returns to McMurdo Station in Antarctica after working in the deep field for two months as part of the Antarctic Search for Meteorites team.Image courtesy of Juliane GrossTransitioning from full-time academia to her current position at NASA has been a big adjustment for Gross, but she has learned to love the change and the growth opportunities that come with it. “Being part of this incredible moment in history when we are about to return to the Moon with Artemis, our Apollo of today, feels so special and humbling that it made the transition easier,” she said.
The job has also increased Gross’ love and excitement for space exploration and reminds her every day why sample return missions are important. “The Moon is a museum of planetary history,” she said. “It has recorded and preserved the changes that affected the Earth-Moon system and is the best and most accessible place in the solar system to study planet-altering processes that have affected our corner of the universe.”
Still, “The Moon is only our next frontier,” she said. “Keep looking up and never give up. Ad astra!”
Watch below to learn about NASA’s rich history of geology training and hear how scientists and engineers are getting ready to bring back samples that will help us learn about the origins of our solar system.
NASA Awards Astrophysics Postdoctoral Fellowships for 2025
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NASA Awards Astrophysics Postdoctoral Fellowships for 2025The highly competitive NASA Hubble Fellowship Program (NHFP) recently named 24 new fellows to its 2025 class. The NHFP fosters excellence and leadership in astrophysics by supporting exceptionally promising and innovative early-career astrophysicists. Over 650 applicants vied for the 2025 fellowships. Each fellowship provides the awardee up to three years of support at a U.S. institution.
Once selected, fellows are named to one of three sub-categories corresponding to three broad scientific questions that NASA seeks to answer about the universe:
How does the universe work? – Einstein Fellows
How did we get here? – Hubble Fellows
Are we alone? – Sagan Fellows
“The 2025 class of the NASA Hubble Fellowship Program is comprised of outstanding NASA Astrophysics researchers,” said Shawn Domagal-Goldman, acting director of the Astrophysics Division at NASA Headquarters in Washington. “This class of competitively-selected fellows will inspire future generations through the products of their research, and by sharing the results of that work with the public. Their efforts will help NASA continue its worldwide leadership in space-based astrophysics research.”
The class of 2025 NHFP Fellows are shown in this photo montage (left to right, top to bottom): The Einstein Fellows (seen in the blue hexagons) are: Shi-Fan Chen, Nicolas Garavito Camargo, Jason Hinkle, Itai Linial, Kenzie Nimmo, Massimo Pascale, Elia Pizzati, Jillian Rastinejad and Aaron Tohuvavohu. The Hubble Fellows (seen in the red hexagons) are: Aliza Beverage, Anna de Graaff, Karia Dilbert, Emily Griffith, Viraj Karambelkar, Lindsey Kwok, Abigail Lee, Aaron Pearlman, Dominick Rowan, Nicholas Rui, Nadine Soliman, Bingjie Wang. The Sagan Fellows (seen in green hexagons) are: Kyle Franson, Caprice Phillips, and Keming Zhang.NASA, ESA, Megan Crane (Caltech/IPAC)The list below provides the names of the 2025 awardees, their fellowship host institutions, and their proposed research topics.
The 2025 NHFP Einstein Fellows are:
- Shi-Fan Chen, Columbia University, Galaxies, Shapes and Weak Lensing in the Effective Field Theory of Large-Scale Structure
- Nicolas Garavito Camargo, University of Maryland, College Park, Local Group Galaxies in Disequilibrium; Building New Frameworks to Constrain the Nature of Dark Matter
- Jason Hinkle, University of Illinois, Urbana-Champaign, Nuclear Transients in the Golden Era of Time-Domain Astronomy
- Itai Linial, New York University, Repeating Nuclear Transients – Probes of Supermassive Black Holes and Their Environments
- Kenzie Nimmo, Northwestern University, From Glimmering Jewels to Cosmic Ubiquity: Unraveling the Origins of FRBs
- Massimo Pascale, University of California, Los Angeles, The Universe Seen Through Strong Gravitational Lensing
- Elia Pizzati, Harvard University, The Missing Link: Connecting Black Hole Growth and Quasar Light Curves in the Young Universe
- Jillian Rastinejad, University of Maryland, College Park, Illuminating the Explosive Origins of the Heavy Elements
- Aaron Tohuvavohu, California Institute of Technology, Ultraviolet Space Telescopes for the new era of Time Domain and Multi-Messenger Astronomy
The 2025 NHFP Hubble Fellows are:
- Aliza Beverage, Carnegie Observatories, Revealing Massive Galaxies Formation Using Chemical Abundances
- Anna de Graaff, Harvard University, Early giants in context: How could galaxies in the first billion years grow so rapidly?
- Karia Dibert, California Institute of Technology, Superconducting on-chip spectrometers for high-redshift astrophysics and cosmology
- Emily Griffith, University of Colorado, Boulder, Beyond Mg and Fe: Exploring Detailed Nucleosynthetic Patterns
- Viraj Karambelkar, Columbia University, The Anthropology of Merging Stars
- Lindsey Kwok, Northwestern University, Determining the Astrophysical Origins of White-Dwarf Supernovae with JWST Infrared Spectroscopy
- Abigail Lee, University of California, Berkeley, AGB Stars in the Era of NIR Astronomy: New Probes of Cosmology and Galaxy Evolution
- Aaron Pearlman, Massachusetts Institute of Technology, Pinpointing the Origins of Fast Radio Bursts and Tracing Baryons in the Cosmic Web
- Dominick Rowan, University of California, Berkeley, Fundamental Stellar Parameters Across the Hertzsprung-Russell Diagram
- Nicholas Rui, Princeton University, A seismic atlas of the stellar merger sky
- Nadine Soliman, Institute for Advanced Study, Micro Foundations, Macro Realities: Modeling the Multi-scale Physics Shaping Planets, Stars and Galaxies
- Bingjie Wang, Princeton University, Inference at the Edge of the Universe
The 2025 NHFP Sagan Fellows are:
- Kyle Franson, University of California, Santa Cruz, Mapping the Formation, Migration, and Thermal Evolution of Giant Planets with Direct Imaging and Astrometry
- Caprice Phillips, University of California, Santa Cruz, Aging in the Cosmos: JWST Insights into the Evolution of Brown Dwarf Atmospheres and Clouds
- Keming Zhang, Massachusetts Institute of Technology, Understanding the Origin and Abundance of Free-Floating Planets via Microlensing and Machine Learning
The class of 2025 NHFP Fellows are shown in this photo montage (left to right, top to bottom): The Einstein Fellows (seen in the blue hexagons) are: Shi-Fan Chen, Nicolas Garavito Camargo, Jason Hinkle, Itai Linial, Kenzie Nimmo, Massimo Pascale, Elia Pizzati, Jillian Rastinejad and Aaron Tohuvavohu.
The Hubble Fellows (seen in the red hexagons) are: Aliza Beverage, Anna de Graaff, Karia Dilbert, Emily Griffith, Viraj Karambelkar, Lindsey Kwok, Abigail Lee, Aaron Pearlman, Dominick Rowan, Nicholas Rui, Nadine Soliman, Bingjie Wang.
The Sagan Fellows (seen in green hexagons) are: Kyle Franson, Caprice Phillips, and Keming Zhang.
For short bios and photos, please visit the link at the end of the article.
An important part of the NHFP is the annual Symposium, which allows Fellows the opportunity to present results of their research, and to meet each other and the scientific and administrative staff who manage the program. The 2024 symposium was held at the NASA Exoplanet Science Institute (NExScI) in Pasadena, California. Science topics ranged through exoplanets, gravitational waves, fast radio bursts, cosmology and more. Non-science sessions included discussions about career paths and developing mentorship skills, as well as an open mic highlighting an array of talents other than astrophysics.
The Space Telescope Science Institute in Baltimore, Maryland, administers the NHFP on behalf of NASA, in collaboration with the Chandra X-ray Center at the Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, and the NASA Exoplanet Science Institute and the Jet Propulsion Laboratory, in Pasadena, California.
Short bios and photos of the 2025 NHFP Fellows can be found at:
https://www.stsci.edu/stsci-research/fellowships/nasa-hubble-fellowship-program/2025-nhfp-fellows
The class of 2025 NHFP Fellows are shown in this photo montage.
Share Details Last Updated Mar 31, 2025 EditorAndrea GianopoulosLocationNASA Goddard Space Flight Center Related TermsNASA Awards Launch Services Contract for SpaceX Starship
NASA has awarded SpaceX of Starbase, Texas, a modification under the NASA Launch Services (NLS) II contract to add Starship to their existing Falcon 9 and Falcon Heavy launch service offerings.
The NLS II contracts provide a broad range of commercial launch services for NASA’s planetary, Earth-observing, exploration, and scientific satellites. These high-priority, low and medium risk tolerant missions have full NASA technical oversight and mission assurance, resulting in the highest probability of launch success.
The NLS II contracts are multiple award, indefinite-delivery/indefinite-quantity, with an ordering period through June 2030 and an overall period of performance through December 2032. The contracts include an on-ramp provision that provides an opportunity annually for new launch service providers to add their launch service on an NLS II contract and compete for future missions and allows existing contractors to introduce launch services not currently on their NLS II contracts.
The contracts support the goals and objectives of the agency’s Science Mission Directorate, Space Operations Mission Directorate, Explorations Systems Development Mission Directorate, and the Space Technology Mission Directorate. Under the contracts, NASA also can provide launch services to other federal government agencies.
NASA’s Launch Services Program Office at the agency’s Kennedy Space Center in Florida manages the NLS II contracts. For more information about NASA and agency programs, visit:
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Patti Bielling
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NASA Boosts Efficiency with Custom X-66 Flooring
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Preparations for Next Moonwalk Simulations Underway (and Underwater) Eric Garza, an engineering technician in the Experimental Fabrication Shop at NASA’s Armstrong Flight Research Center in Edwards, California, cuts plywood to size for temporary floorboards for the X-66 experimental demonstrator aircraft on Aug. 26, 2024.NASA/Steve FreemanNASA designed temporary floorboards for the MD-90 aircraft to use while it is transformed into the X-66 experimental demonstrator aircraft. These floorboards will protect the original flooring and streamline the modification process.
Supporting the agency’s Sustainable Flight Demonstrator project, a small team in the Experimental Fabrication Shop at NASA’s Armstrong Flight Research Center in Edwards, California, built temporary floorboards to save the project time and resources. Repeated removal and installation of the original flooring during the modification process was time-consuming. Using temporary panels also ensures the original floorboards are protected and remain flightworthy for when modifications are complete, and the original flooring is reinstalled.
“The task of creating the temporary floorboards for the MD-90 involves a meticulous process aimed at facilitating modifications while maintaining safety and efficiency. The need for these temporary floorboards arises from the detailed procedure required to remove and reinstall the Original Equipment Manufacturer (OEM) floorboards,” said Jason Nelson, experimental fabrication lead. He is one of two members of the fabrication team – one engineering technician and one inspector – manufacturing about 50 temporary floorboards, which range in size from 20 inches by 36 inches to 42 inches by 75 inches.
A wood router cuts precise holes in plywood for temporary floorboards on Aug. 26, 2024, in the Experimental Fabrication Shop at NASA’s Armstrong Flight Research Center in Edwards, California. The flooring was designed for the X-66 experimental demonstrator aircraft. NASA/Steve FreemanNelson continued, “Since these OEM boards will be removed and reinstalled multiple times to accommodate necessary modifications, the temporary floorboards will save the team valuable time and resources. They will also provide the same level of safety and strength as the OEM boards, ensuring that the process runs smoothly without compromising quality.”
Designing and prototyping the flooring was a meticulous process, but the temporary solution plays a crucial role in optimizing time and resources as NASA works to advance safe and efficient air travel. The agency’s Sustainable Flight Demonstrator project seeks to inform the next generation of single-aisle airliners, the most common aircraft in commercial aviation fleets around the world. NASA partnered with Boeing to develop the X-66 experimental demonstrator aircraft.
NASA Armstrong’s Experimental Fabrication Shop carries out modifications and repair work on aircraft, ranging from the creation of something as small as an aluminum bracket to modifying wing spars, fuselage ribs, control surfaces, and other tasks to support missions.
Eric Garza, an engineering technician in the Experimental Fabrication Shop at NASA’s Armstrong Flight Research Center in Edwards, California, observes a wood router cut holes for temporary floorboards on Aug. 26, 2024. The flooring was designed for the X-66 experimental demonstrator aircraft. NASA/Steve Freeman Share Details Last Updated Mar 28, 2025 EditorDede DiniusContactSarah Mannsarah.mann@nasa.gov Related Terms Explore More 2 min read The Sky’s Not the Limit: Testing Precision Landing Tech for Future Space Missions Article 5 days ago 5 min read NASA Demonstrates New Wildland Fire Airspace Management System Article 6 days ago 3 min read New Aircraft Wing Undergoes Crucial NASA Icing Testing Article 6 days ago Keep Exploring Discover More Topics From NASAArmstrong Flight Research Center
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