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Early Career Faculty (ECF) 2025 Awards
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Preparations for Next Moonwalk Simulations Underway (and Underwater)Advanced Diagnostics for High-Enthalpy Test Facilities Simulating Spacecraft Atmospheric Entry
- Damiano Baccarella
University of Tennessee, Knoxville
Application of Resonance Enhanced Multi-Photon Ionization Diagnostics to the Characterization of Arcjet Flows - Ciprian Dumitrache
Colorado State University
Ultrafast Laser Diagnostics for Nonequilibrium Flowfields Characterization in Atmospheric Entry Studies - Dan Fries
University of Kentucky, Lexington
Multiplexed Polarization Spectroscopy for Single-Shot Multi-Species Diagnostics in High-Enthalpy Flows - Yi Mazumdar
Georgia Institute of Technology
Simultaneous Temperature, Species, and Velocity Measurements using Ultrafast Laser Diagnostics for Ground Testing of Spacecraft Atmospheric Entry Systems
Planning for Autonomous Spacecraft Using Machine Learning Methods to Enable Onboard Guidance, Navigation, and Control
- Glen Chou
Georgia Institute of Technology
Robust Real-Time Hierarchical Neural Planning and Control with System-Level Guarantees - Roshan Eapen
Pennsylvania State University
Hamilton-Jacobi aided Planning and Reasoning for Intelligent Spacecraft Maneuvers (HJ-PRISM) - Bin Hu
University of Houston
Safety-Enabled and Efficient Onboard Planning for Autonomous Spacecraft via Physics-Informed Reinforcement Learning
NASA Volunteers Help Zooniverse Reach 1 Billion Classifications
The Zooniverse, a NASA grantee that runs the world’s largest platform for online people-powered research, has reached an extraordinary milestone: 1 billion classifications contributed by volunteers around the world. This milestone is a celebration of everyone who has marked a dip in a light curve, confirmed the presence of a moving object in a short video, or identified species in a camera trap image. Each of these small contributions collectively advances our understanding of the universe.
A total of 31 NASA-sponsored citizen science projects have been hosted on Zooniverse, accounting for 120 million classifications by 324 thousand volunteers since 2020. Through projects like Planet Hunters TESS, Daily Minor Planet, Backyard Worlds: Planet 9, Space Umbrella, and Snapshot Wisconsin, volunteers help discover exoplanets, identify near-Earth objects and asteroids, search for brown dwarfs and planetary systems, analyze effects of the solar wind, and inform wildlife management decisions. These projects have led to 96 scientific publications, and 56 of these articles feature NASA citizen scientists as co-authors to recognize the significance of their research contributions. These efforts demonstrate how public participation can accelerate discovery by combining human curiosity and pattern recognition with data from NASA missions and observatories. Collaboration between volunteers, scientists, and computing technology will be even more important in the future as we tackle enormous and complex datasets, like those from NASA’s upcoming Nancy Grace Roman Space Telescope.
“One billion classifications represent far more than a number; it’s one billion moments of curiosity transformed into meaningful contributions to research,” said Laura Trouille, principal investigator of Zooniverse and vice president of Science Engagement at the Adler Planetarium. “Every classification on Zooniverse brings us one step closer to new discoveries and a deeper understanding of our universe, our world, and ourselves.”
Zooniverse is the world’s largest platform for people-powered research. Co-founded by the Adler Planetarium and the University of Oxford, with the University of Minnesota serving as a key institutional partner, Zooniverse enables anyone, anywhere to contribute directly to real scientific research. Through its six-year collaboration with NASA, Zooniverse provides science-enabling infrastructure to NASA researchers through tools and a community of more than 3 million registered volunteers.
Facebook logo @nasascience_ @nasascience_ Instagram logo @nasascience_ Linkedin logo @nasascience_NASA Photographer Captures Images from F-18 Over Washington
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Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA photographer Jim Ross flies above the Washington Monument in Washington on Saturday, July 4, 2026, in an F-18 aircraft, as part of a flyover to celebrate America’s 250th birthday. This aircraft is from NASA’s Armstrong Flight Research Center in Edwards, California, and it joined other NASA aircraft for the flyover.NASA/Jim RossNASA flight photographers capture history from a perspective few ever experience, getting a rare bird’s-eye view of the agency’s missions in action. Their photos document key NASA research and give the public a front-row seat to the work happening behind the scenes.
Jim Ross, a photographer at NASA’s Armstrong Flight Research Center in Edwards, California, flew over Washington during the Fourth of July celebration to document a NASA flyover commemorating America’s 250th birthday. He’s captured some of the agency’s most exhilarating milestones, like early SR-71 flights, the delivery flight of Space Shuttle Endeavour to Los Angeles, and first flights of NASA’s X-59 quiet supersonic research aircraft.
“I grew up in Bozeman, Montana, when it was still considered a small town, so if someone told that little kid that he would be flying in a F-18 over the National Mall, he would have never believed it,” Ross said. “I love documenting history, and having the opportunity to capture flights and launches has kept me doing it for almost 37 years.”
Ross began his aviation photography career in 1989 when he joined the staff at NASA Armstrong (then Dryden). He became the photo lead in 1997, a title he retains.
Check out his images from the flyover here: https://www.nasa.gov/gallery/freedom-250/
NASA photographer Jim Ross takes a selfie from the rear seat of a NASA F/A‑18 during a cross‑country flight from Spokane, Washington, to Washington, D.C., on Thursday, July 2, 2026. The agency’s F‑15, flying alongside the aircraft, is visible through the window. Both aircraft, from NASA’s Armstrong Flight Research Center in Edwards, California, participated in the Freedom 250 flyover with other NASA and military aircraft on Saturday, July 4, 2026.NASA/Jim Ross NASA photographer Jim Ross flies above Washington on Saturday, July 4, 2026, in an F-18 aircraft, as part of a flyover to celebrate America’s 250th birthday. This aircraft is from NASA’s Armstrong Flight Research Center in Edwards, California, and it joined other NASA aircraft for the flyover. A NASA F-15 is seen flying to the side of the NASA F-18.NASA/Jim Ross Share Details Last Updated Jul 10, 2026 EditorDede DiniusContactTeresa Whitingteresa.whiting@nasa.gov Related Terms Explore More 3 min read A Day of Flight Testing at NASA Armstrong Article 1 week ago 5 min read NASA’s Newest Wind Tunnel Builds on Legacy of Innovation Article 2 weeks ago 3 min read This is How NASA Flight Tests New Technology Article 2 weeks ago Keep Exploring Discover More Topics From NASAArmstrong Flight Research Center
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Waxing Gibbous Moon
The waxing gibbous moon is nestled in the darkness of space in this June 26, 2026, image from the International Space Station. The space station was 264 miles above the Indian Ocean southeast of Madagascar at the time.
The waxing gibbous phase comes before the full moon phase. During this time, the Moon appears brighter in the night sky to viewers on Earth.
Image credit: NASA
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NASA Sets Coverage for Astronaut Anil Menon Launch to Space Station
NASA astronaut Anil Menon will launch aboard the Roscosmos Soyuz MS-29 spacecraft to the International Space Station on Tuesday, July 14, accompanied by cosmonauts Pyotr Dubrov and Anna Kikina, where they will join the Expedition 74 crew advancing scientific research.
Menon, Dubrov, and Kikina will lift off at 10:47 a.m. EDT (7:47 p.m. Baikonur time) from the Baikonur Cosmodrome in Kazakhstan. Live launch and docking coverage is available on NASA+, Amazon Prime, and the agency’s YouTube channel. Learn how to watch NASA content through a variety of online platforms, including social media.
After a two-orbit, three-hour trip to the station, the spacecraft will automatically dock at 1:56 p.m. to the Prichal module. Shortly afterward, hatches will open between the Soyuz and the orbiting laboratory.
Once aboard, the trio will join NASA astronauts Jessica Meir, Jack Hathaway, and Chris Williams, ESA (European Space Agency) astronaut Sophie Adenot, and Roscosmos cosmonauts Sergey Kud-Sverchkov, Sergei Mikaev, and Andrey Fedyaev.
NASA’s coverage schedule is as follows (all times Eastern and subject to change based on real-time operations):
Tuesday, July 14
9:45 a.m. – Launch coverage begins on NASA+, Amazon Prime, and YouTube.
10:47 a.m. – Launch
1:10 p.m. – Rendezvous and docking coverage begins on NASA+, Amazon Prime, and YouTube.
1:56 p.m. – Docking
3:30 p.m. – Hatch opening and welcome coverage begins on NASA+, Amazon Prime, and YouTube.
3:55 p.m. – Hatch opening
Menon, Dubrov, and Kikina will spend about eight months aboard the orbital complex as International Space Station Expedition 74/75 crew members before returning to Earth in April 2027. This will be Menon’s first spaceflight and the second for both Dubrov and Kikina.
During his stay on the station, Menon will conduct scientific research and technology demonstrations aimed at advancing human space exploration and benefiting life on Earth. He will continue research to refine in-space production of semiconductor crystals to enable the large-scale manufacturing of components needed for high-performance computers, artificial intelligence, and improved medical devices. Menon also will perform ultrasound using augmented reality and artificial intelligence methods that could eliminate the need for medical support from Earth on future space missions. He will be a test subject helping researchers understand how blood flow is affected in space to protect future astronauts. He also will test bioprinting vascular constructs in microgravity to improve understanding of the aging process to advance therapeutic developments.
For more than 25 years, people have lived and worked continuously aboard the International Space Station, advancing scientific knowledge and making research breakthroughs not possible on Earth. The space station helps NASA understand and overcome the challenges of human spaceflight, expand commercial opportunities in low Earth orbit, and build on the foundation for long-duration missions to the Moon, as part of the Artemis program, and to Mars.
To learn more about International Space Station research, operations, and its crews, visit:
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NASA Space Telescope Maps Magnetic Fields of ‘Lighthouse’ Pulsar
For the first time, scientists have used NASA’s IXPE (Imaging X-ray Polarimetry Explorer) to directly measure the magnetic fields of PSR J1101−6101, a pulsar located within what is often referred to as the Lighthouse Nebula. The results provide new insight into the structure of some of the most extreme objects in the cosmos, as NASA continues to explore the secrets of how the universe works. A paper describing the results published Thursday in the Astrophysical Journal.
Scientists have successfully measured the magnetic field of the Lighthouse pulsar’s nebula using NASA’s IXPE. Their measurements confirm the theory that high-energy particles escape along the galaxy’s magnetic field lines. This composite image contains X-ray data from IXPE in blue (highlighted in the inset), the Chandra X-ray Observatory in purple, and radio data from CSIRO in green. The starfield is optical data from the 2MASS optical survey. X-ray: Chandra: NASA/CXC/Stanford Univ./J.T. Dinsmore et al.; IXPE: NASA/MSFC/J.T. Dinsmore et al., Radio: CSIRO/ATNF/ATCA; Optical: 2MASS/UMass/IPAC-Caltech/NASA/NSF; Image processing: NASA/CXC/SAO/L. Frattare Fast facts- A pulsar is a type of neutron star with a strong magnetic field that spins incredibly fast. The pulsar at the center of the Lighthouse Nebula is rotating 16 times per second.
- Neutron stars are the leftover cores of massive stars, formed at the end of their life cycles, that possess more mass than the Sun. They are condensed down to the size of a city, making them natural laboratories for studying extreme physics.
- Polarization is a property of light that describes the direction of its electric field vibrations. The polarization degree is a measurement of how aligned those vibrations are with each other.
In June 2025, IXPE spent nearly 18 days focused on the Lighthouse Nebula.
Astronomers studied two narrow X-ray offshoots extending from the pulsar to better understand how electrons at nearly the speed of light interact with this energetic system. The longer offshoot is known as the “filament,” and the shorter one is the “trail.”
When high-energy particles from the pulsar collide with the gas of interstellar space, they form a bow shock, like the bow wave formed at the front of a speeding boat. Most particles become trapped behind this bow shock, forming the turbulent trail behind the pulsar.
Researchers have suspected since 2008 that the highest-energy particles escape through this bow shock into interstellar space, flowing along the galaxy’s magnetic field lines to create the nebula’s long, thin filament.
“We wanted to test that theory,” said Jack Dinsmore, undergraduate student at Stanford University, who led the study. “The ‘smoking gun’ would come by measuring the polarization of the light, which indicates the magnetic field direction. If the magnetic field points along the filament, that confirms that the filament’s particles are flowing along the field.”
One challenge with these measurements is that the Lighthouse Nebula is relatively faint. To address this, IXPE scientists developed advanced analysis methods that use every bit of data, avoiding simplifying steps that could limit information. With these new tools and the new observations of the Lighthouse, the science team successfully measured the filament’s polarization. These techniques also gave a polarization measurement of the trail, and the pulsar’s emission signal.
Their analysis confirmed with more than 99% confidence that the magnetic field does indeed align with the particles’ flow.
While the parallel direction confirms models for the particle’s motion, the polarization degree was high enough to raise new questions.
“Many of the models for filaments assume strong magnetic turbulence,” said Roger Romani, a Stanford University professor who co-authored this paper. “The high polarization degree we measured indicates lower turbulence than such models require.”
The IXPE observations also showed that the magnetic field responsible for X-ray emission had to be parallel to the trail. However, the authors collected radio frequency observations showing a magnetic field pointing almost exactly perpendicular.
“The striking divergence in magnetic field orientations observed between radio and X-ray wavelengths provides compelling evidence for the highly structured nature of these objects,” said Niccolò Bucciantini of the Italian National Institute for Astrophysics and co-author of the study. “This marks the first clear indication that particles of different energies occupy distinct regions within the system, hinting at the presence of multiple, and potentially very different, acceleration mechanisms at work.”
More about IXPEThe IXPE mission, which continues to provide unprecedented data enabling groundbreaking discoveries about celestial objects across the universe, is a joint NASA and Italian Space Agency mission with partners and science collaborators in 12 countries. It is led by NASA’s Marshall Space Flight Center in Huntsville, Alabama, and BAE Systems, Inc. manages spacecraft operations together with the University of Colorado’s Laboratory for Atmospheric and Space Physics in Boulder.
Learn more about IXPE’s ongoing mission here:
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Details Last Updated Jul 09, 2026 Editor Lee Mohon Contact Joel Wallace Location Marshall Space Flight Center Related Terms Explore More 3 min read NASA’s IXPE Measures White Dwarf Star for First TimeBy Michael Allen For the first time, scientists have used NASA’s IXPE (Imaging X-ray Polarimetry…
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Principal Investigator and Quality Assessment Reports Evaluate Umbra Synthetic Aperture Radar Data
Two new reports from NASA’s Commercial Satellite Data Acquisition (CSDA) program evaluate data from the Umbra X-band Synthetic Aperture Radar (SAR) satellite constellation for the NASA Earth science research and applications community. The results of these evaluations help to inform NASA program management and the user community about the quality of these commercial data for use in NASA science.
NASA’s CSDA program released the Umbra SAR Principal Investigator Evaluation Summary and Umbra SAR Quality Assessment Reports in May 2026. (The cover of the Quality Assessment Report is shown at left.) The results of these evaluations help inform NASA program management about the quality of this commercial data for use in NASA science. At right, a collage of synthetic aperture radar images from Umbra. Credit: NASA CSDA program / © Umbra Lab Inc., 2026. All Rights ReservedThe CSDA Umbra Synthetic Aperture Radar SAR Principal Investigator Evaluation Summary documents the findings of evaluation teams. The teams were given access to the Umbra archive as well as the ability to task the Umbra constellation for new acquisitions. The tasking capability allowed evaluation teams to test the utility of Umbra data in time-sensitive workflows and to monitor areas experiencing rapid change and/or emergent environmental conditions, such as harmful algal blooms.
Although the Principal Investigator Evaluation Summary supports the use of Umbra SAR data for NASA Earth science research and applications overall, it noted several strengths and weaknesses of the Umbra X-band data. Strengths included access to a very high spatial resolution X-band SAR satellite constellation; taskable access to high temporal repeat opportunities with quick turnaround; imaging flexibility with a range of azimuth and incidence angles; and the company’s Open Data Program. Conversely, the PI teams reported weaknesses, including issues with Umbra geolocation (noting large and small geolocation errors), limited software compatibility, metadata, and some missing technical documentation.
Additionally, the CSDA Umbra Synthetic Aperture Radar SAR Quality Assessment Report documents the results of radiometric and geometric analyses performed by NASA subject matter experts (SMEs) enlisted to evaluate the fundamental quality of the Umbra data following the Joint NASA/European Space Agency (ESA) assessment guidelines (ESA-NASA, 2024).
Performed mainly on the single-look complex (SLC) Level 1 data products in Sensor Independent Complex Data (SICD) format, along with some additional Level 2 products used in science usability assessments by the evaluation team, the CSDA SMEs found the spatial resolution of the data agreed with Umbra’s specifications. However, the quality analysis results for geolocation accuracy did not universally align with the company’s specifications. Given these results, the SME’s concluded that “the overall positioning performance of the Umbra data did not meet the expected accuracy.
Regarding the radiometric performance of the data, which was assessed in terms of absolute accuracy, stability, and sensitivity, the SMEs found the data “underperform[ed] relative to that of well-calibrated reference SAR systems.”
About the CSDA ProgramThe CSDA program was established to identify, evaluate, and acquire data from commercial sources that support the NASA Earth science research and application goals. NASA’s Earth Science Division recognizes the potential impact commercial satellite constellations may have in encouraging/enabling efficient approaches to advancing Earth System Science and applications development for societal benefit. Commercially acquired data may also provide a cost-effective means to augment and/or complement the suite of Earth observations acquired by NASA, other U.S. government agencies, and international partners.
To read the reports in full, see the links under “Evaluation” heading on the CSDA’s Umbra commercial vendor webpage.
Curiosity Sees Martian Sulfur Up Close
This close-up view shows fragments of sulfur crystals — the first ever seen on the Red Planet. The crystals were found after NASA’s Curiosity Mars rover happened to drive over a rock and crush it on May 30, 2024. Several days later, Curiosity used a camera on the end of its robotic arm to take this image.
A recent paper in Science suggests that the sulfur formed when magma deep below the surface released fluids or gases that deposited sulfur on the Red Planet’s surface about 3 billion years ago.
Image credit: NASA/JPL-Caltech/MSSS
NASA Scientists Take to Air and Space to Study Arctic Sea Ice
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Preparations for Next Moonwalk Simulations Underway (and Underwater) These four views were captured from a World War II-era aircraft in April 2026, when scientists used instruments aboard the plane to study Arctic sea ice. Their flights were timed to coincide with satellites passing overhead so the airborne and orbital data could be combined.NASA/JPL-CaltechThis month, engineers at NASA’s Jet Propulsion Laboratory in Southern California are testing a spacecraft sensor that will help measure how quickly Arctic sea ice is disappearing. And while that instrument won’t launch for another year, scientists started preparing for its use during a recent field campaign in the Canadian wilderness.
Researchers spent two weeks in April flying above the Arctic Ocean, often watching sunrise from an altitude of 1,500 feet (457 meters) in a World War II-era plane. A variety of cutting-edge sensors used to measure the thickness of sea ice and snow were aboard the plane, including a stand-in for the microwave radiometer now undergoing testing at JPL. Measuring sea ice thickness is tricky, requiring a number of precise figures, including how high the sea ice rises above water, the depth of snow on top of that ice, and microwave emissions from the surface.
Flights were timed to the passage of satellites overhead so coordinated observations could be taken of the same features. Combining the airborne and satellite data will improve scientists’ ability to measure sea ice and understand how climate conditions are evolving across the Arctic.
In recent decades, the extent and thickness of Arctic sea ice have changed. Improving measurements of those changes helps scientists better understand the Arctic system while supporting navigation, weather and ocean research, and future satellite observations. As Arctic shipping activity increases, the region is also becoming strategically and economically more significant.
According to Sahra Kacimi of JPL, who served as the field campaign’s science lead, ongoing warming in the Arctic could potentially impact public safety and economic interests.
Find out what Arctic sea ice looked like as scientists studied it from the air — and using space-based instruments — during a field campaign this past April.Credit: NASA/JPL-Caltech Frequent flyers
Kacimi has spent years studying sea ice using satellite data, but the top-down view she gets from space is different than peering out a plane’s window.
The bewildering diversity of sea ice creates otherworldly landscapes. The ice can be attached to land or adrift in the ocean; it can be rough or smooth. Driven by winds and ocean currents, the ice is constantly shifting, breaking apart, and deforming. Cracks can open into long stretches of exposed ocean, and collisions between floes can push ice rubble into massive ridges that extend for miles.
Some sea ice lasts only one season, while thicker ice can survive for several years (though multiyear sea ice is becoming less common in many parts of the Arctic). Entire ecosystems are affected by these changes, down to the arctic foxes and hares the scientists spotted throughout the trip.
Improving estimates of sea ice thickness helps scientists better understand how the region is changing and supports long-term observations of the Arctic environment. The NASA team logged about 50 hours in the air over the two-week campaign, conducting flights over drifting ice near the town of Inuvik before studying ice fixed to the shore of another location, a hamlet called Cambridge Bay.
For the Inuvik portion of the campaign, the team coordinated with the Surface Water and Ocean Topography (SWOT) mission, a satellite jointly developed by NASA and the French space agency, CNES (Centre National d’Études Spatiales), with JPL leading the United States component of the mission. Though it was designed to map the height of the globe’s sea and fresh water, SWOT can also measure the amount of sea ice above the waterline.
In Cambridge Bay, the NASA team joined researchers from ESA (European Space Agency), Germany’s Alfred Wegener Institute, and Canada’s University of Calgary. During this part of the campaign, coordinated flights soared over a field camp and under the tracks of satellite missions such as NASA’s Ice, Cloud, and Land Elevation Satellite-2 (ICESat-2) and ESA’s CryoSat-2.
To improve sea ice thickness estimates, ESA is developing, with cooperation from NASA, a new polar mission called Copernicus Polar Ice and Snow Topography Altimeter (CRISTAL). During the April airborne campaign, scientists flew instruments similar to what CRISTAL will carry, including the microwave radiometer now being tested at JPL.
“Combining observations from space, air, and ground surface instruments is essential for developing and validating algorithms for current and future missions,” Kacimi said.
For the scientists, it was also a chance to meet locals who see the Arctic’s changes up close. Kacimi spoke to community leaders and students at a STEM camp about how disappearing ice is affecting their communities.
“I’m used to looking at sea ice from space and thinking about its role in the global climate, but for people living in the Arctic, it carries a much deeper meaning,” Kacimi said.
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Students Connect NASA Science With Indigenous Knowledge to Study Coastal Erosion
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Students Connect NASA Science With Indigenous Knowledge to Study Coastal Erosion Students return from fieldwork and sit together in the classroom, examining NASA satellite images to learn about the changes to their community’s coastline.Story by Keri Moskowitz, Gulf of Maine Research Institute
For the Pleasant Point Passamaquoddy Reservation, or Sipayik, the ocean has always been a teacher. Situated in what is known as Downeast Maine, along the shores of Passamaquoddy Bay, generations of Indigenous people have lived along the coast, learning from the tides, the land, and their elders. But today, the shoreline is changing more rapidly. Coastal erosion is slowly taking land away. Land that already holds a history of loss.
In the summer of 2023, inspired by a trip to Fairbanks, AK to attend Climate Change in My Community – a workshop organized by the NASA Science Activation (SciAct) program’s Arctic and Earth Signs project – SciAct’s Learning Ecosystems Northeast (LENE) team began working with partners, including Indigenous leaders and scientists, to ask an important question: What does coastal erosion mean to people who have already lost land?
By November 2024, planning was underway at Sipayik Elementary School. The goal was to bring together Western science and Indigenous knowledge so students could understand the changes happening in their own community.
The lessons began in March 2025. For five weeks, nine 5th-grade students explored erosion in many ways. They visited local field sites and listened to elders share stories about how the coastline used to look. Learners used these accounts to measure the changes, both on the coast and via maps back in the classroom. They built erosion trays from simple materials to test how waves shape the land. They measured current high tide lines and compared them to historical ones. They studied old photographs and aerial images from 1942 to 2023 to see how much the shoreline had moved. They even compared 300-year-old tribal maps with future flood projections.
Students learned that science does not only live in textbooks. As one observer shared, “Our people were scientists without having to go to school.”
The students were curious, engaged, and proud. They saw that resilience is part of who they are. They have always adapted while holding on to culture.
In June of 2026, the students were invited to the Gulf of Maine Research Institute to present their work to scientists, staff, and REU (Research Experience for Undergraduate) interns. They traveled 3.5 hours for this opportunity, and the journey proved worthwhile. During the Q&A portion following their slideshow, someone asked whether learning to read the various maps was difficult. One student responded with a reminder: these were not merely maps but NASA satellite images.
Future goals for the project include inviting more elders and adding more field sites in the work, strengthening language and cultural connections, sharing student learning with other Native youth, and planning resilience strategies like marsh restoration in coordination with tribal leadership. When the students were asked if they planned to continue their studies and work on this cause after their time in the classroom ended, they all resoundingly stated “YES”.
In Sipayik, the story of erosion is not just about land washing away. It is about memory, knowledge, identity, and the strength of a community that continues to learn from the shore.
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Hubble Captures Star-Studded Cluster
This image from NASA’s Hubble Space Telescope showcases Messier 3 (M3), one of the Milky Way galaxy’s most massive globular clusters, or spherical collections of gravitationally bound stars. Globular clusters are made up of ancient stars that formed at roughly the same time from the same cloud of gas, giving those stars similar ages. Around 150 known globular clusters are sprinkled around the outer regions of the Milky Way.
Image credit: NASA, ESA, and A. Sarajedini (Florida Atlantic University); Processing: Gladys Kober (NASA/Catholic University of America)
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NASA Transfers ‘Hundred Acre Wood’ to Patuxent Research Refuge
NASA ceremonially transferred ownership of about 105 acres of wooded land at its Goddard Space Flight Center’s Greenbelt, Maryland, campus Tuesday to the adjoining Patuxent Research Refuge, managed by the U.S. Fish and Wildlife Service.
The property, formerly known as NASA Goddard’s Area 400, is now part of the largest block of unfragmented forest between Washington and Baltimore. The nearly 13,000-acre woodland is the nation’s only refuge specifically established to support wildlife research. The refuge also supports recreational uses, such as walking, biking, horseback riding, fishing, and hunting.
At a ceremony on July 7, 2026, U.S. Fish and Wildlife Service Director Brian Nesvik (left) and Jamie Dunn, center director, NASA’s Goddard Space Flight Center, Greenbelt, Md., sign certificates that ceremonially transfer a 105-acre parcel of property known as “Area 400” from NASA Goddard to the Service.NASA“For over six decades, NASA Goddard has helped shape humanity’s understanding of Earth,” said Jamie Dunn, center director, NASA Goddard. “We’re glad to present this land to our colleagues in the Fish and Wildlife Service, whose conservation and research helps do the real legwork in preserving our Blue Marble for future generations.”
NASA Goddard had used Area 400 for propellant research beginning in the 1960s. That work has largely since shifted to NASA facilities in other states or to commercial providers, and the property had long been a candidate for divestment. NASA and the Service began discussing a potential transfer in 2021.
Following remarks from attending dignitaries and the signing ceremony, assembled guests participated in a monarch butterfly release and milkweed seed dispersal.NASAPrior to the transfer, Area 400 was still almost entirely wooded aside from a two-and-a-half-acre clearing with 11 small structures. The interagency transfer was effective on Feb. 23, and NASA recently completed its final closeout activities at the property, deconstructing the buildings, roadway, and utility service.
This aerial photograph shows Area 400’s appearance in 1984. The surrounding forest has remained largely unchanged since NASA Goddard occupied the property in the 1960s.NASA“Through working with partners on the best use of land, as exemplified with this land transfer, we can continue to conserve America’s natural beauty and expand outdoor recreation opportunities for future generations,” said U.S. Fish and Wildlife Service Director Brian Nesvik.
Media contacts:
Rob Garner
News Chief, Office of Communications
NASA’s Goddard Space Flight Center
Keith Shannon
Regional Communications Lead – U.S. Fish and Wildlife Service Northeast Region
U.S. Department of the Interior
NASA’s New Horizons Spacecraft Wakes from Hibernation in Good Health
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NASA’s New Horizons Spacecraft Wakes from Hibernation in Good HealthFollowing its longest hibernation period ever of nearly a year, NASA’s New Horizons spacecraft has emerged in good health and is ready to begin transmitting science data gathered in the distant Kuiper Belt far beyond Pluto.
From left, flight controllers Mark Lahr and Josh Albers, and Mission Operations Manager Alice Bowman, monitor telemetry streaming from NASA’s New Horizons spacecraft to the mission operations center at the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, on June 24, 2026. Now approximately 5.9 billion miles (9.5 billion kilometers) from Earth, New Horizons is ready to begin transmitting science data after being awakened from its longest ever, nearly yearlong hibernation period. NASA/Johns Hopkins APL/SwRI/Justin GladdenOn June 23, flight controllers at the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland, confirmed New Horizons, acting on stored commands uplinked to its main computer last July, had safely awakened from a 321‑day hibernation period that began Aug. 7. With the spacecraft now approximately 5.9 billion miles (9.5 billion kilometers) from Earth, the radio signals carrying that confirmation took about 8 hours and 52 minutes to reach the APL Mission Operations Center via NASA’s Deep Space Network station near Madrid, Spain.
The mission team typically places New Horizons in resource‑saving hibernation mode during long cruise periods. While the spacecraft is hibernating, operators do not send commands or retrieve data, but the spacecraft continues gathering and storing data around the clock from its heliospheric plasma sensors, Solar Wind at Pluto and the Pluto Energetic Particle Spectrometer Science Investigation, as well as its space dust detector, the Venetia Burney Student Dust Counter.
Alice Bowman, the New Horizons mission operations manager at APL, said the spacecraft reported back to Earth, via the Deep Space Network, with a weekly status beacon. “Every status report through this hibernation period was ‘green,’ meaning all was well aboard New Horizons each and every week,” she said.
As New Horizons resumes active operations, Bowman noted, the team will begin downlinking spacecraft health and safety data, followed by data from the three scientific instruments. In about three weeks, the spacecraft’s onboard Alice ultraviolet spectrograph will look at the hydrogen gas distribution in the outer heliosphere, while the Solar Wind at Pluto, the Pluto Energetic Particle Spectrometer Science Investigation, and the Venetia Burney Student Dust Counter instruments continue their measurements, and the ground team conducts a series of spacecraft and instrument checkouts.
The team also is completing upgrades to the ground‑system software that will make it easier to maintain operations of the spacecraft. Tests are already underway and are expected to continue through the year.
New Horizons is operating on updated autonomy logic designed for operations farther from the Sun and to accommodate the expected reduction in power and the naturally occurring increase in radio‑signal travel time.
The NASA spacecraft’s exploration of this distant region of the solar system marks the latest step in a journey that began in January 2006 with the fastest launch on record; a flyby of Jupiter in February 2007 that included stunning views of the gas giant and its moons; the first exploration through the Pluto system in July 2015; the first exploration of a Kuiper Belt object, Arrokoth, in January 2019, and unique studies of the Sun’s outer heliosphere and dozens of additional Kuiper Belt objects since then.
For more information on NASA’s New Horizons mission, visit:
https://science.nasa.gov/mission/new-horizons/
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Artemis II Crew and Apollo 14 Moon Tree
In this photograph, the Artemis II crew participates in the dedication of the Apollo 14 Moon tree at the Lunar Receiving Park at NASA’s Johnson Space Center on June 25, 2026. This tree is a second-generation Apollo Moon tree of the loblolly pine species. The original Apollo Moon trees were grown from seeds carried aboard Apollo 14 by NASA astronaut Stuart Roosa, a former U.S. Forest Service smoke jumper. Upon return to Earth, the seeds were germinated by the Forest Service, and the resulting seedlings were planted throughout the United States and around the world.
Image credit: NASA/James Blair
July 2026 Satellite Puzzler
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The World Cup From 250 Miles Up
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NASA Takes Flight For America’s 250th
NASA Administrator Jared Isaacman leads a flyover featuring his personally owned Northrop F-5 Tiger during the Great American State Fair on July 4, 2026, on the National Mall in Washington, D.C.
For 250 years, America has pushed the boundaries of what’s possible. From the earliest days of exploration, to the first steps on the Moon and the missions shaping our future, NASA represents the spirit of discovery that defines our nation.
As the United States celebrates its semiquincentennial, Freedom 250 highlights how innovation, courage, and scientific leadership have carried America forward — and how NASA continues to expand the frontier for the next generation.
