NASA ORBIT Challenge 2026

NASA ORBIT Challenge 2026

NASA ORBIT graphic design imagery. The words "NASA ORBIT" are displayed encircled by an oval graphic design with a star at the bottom of the oval.

The NASA ORBIT (Opportunities in Research, Business, Innovation, and Technology for the Workforce) Challenge is a multi-phase, student-focused challenge designed to inspire and empower the next generation of innovators, engineers, entrepreneurs, and researchers.

Compete for cash prizes, receive mentorship from NASA experts, and present your work at an in-person showcase. Finalists gain access to an exclusive accelerator program designed to launch careers in STEM and entrepreneurship.

Award: $380,000 in total prizes

Registration Open Date: December 15, 2025

Registration Close Date: February 9, 2026

For more information, visit: https://nasaorbit.org/

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NASA’s Carruthers Geocorona Observatory Reveals ‘First Light’ Images

NASA’s Carruthers Geocorona Observatory Reveals ‘First Light’ Images

3 min read

NASA’s Carruthers Geocorona Observatory Reveals ‘First Light’ Images

NASA’s Carruthers Geocorona Observatory has captured its first images from space, revealing rare views of Earth and the Moon in ultraviolet light. Taken on Nov. 17 — still months before the mission’s science phase begins — these “first light” images confirm the spacecraft is healthy while hinting at the incredible views to come.

The initial images consist of two from Carruthers’ Wide Field Imager and two from its Narrow Field Imager. Each imager captured two different views: one showing a broad spectrum of far ultraviolet light, and one revealing light from Earth’s geocorona.

Comparison of wide field and narrow field images from NASA's Carruthers Geocorona Observatory: Each column shows far ultraviolet and Lyman-alpha views of Earth, with brightness color scales, using wide and narrow field imagers.
These four images constitute the “first light” for the Carruthers Geocorona Observatory mission. The images were taken on Nov. 17, 2025, from a location near the Sun-Earth Lagrange point 1 by the spacecraft’s Wide Field Imager (left column) and Narrow Field Imager (right column) in far ultraviolet light (top row) and the specific wavelength of light emitted by atomic hydrogen known as Lyman-alpha (bottom row). Earth is the larger, bright circle near the middle of each image; the Moon is the smaller circle below and to the left of it. The fuzzy “halo” around Earth in the images in the bottom row is the geocorona: the ultraviolet light emitted by Earth’s exosphere, or outermost atmospheric layer. The lunar surface still shines in Lyman-alpha because its rocky surface reflects all wavelengths of sunlight — one reason it is important to compare Lyman-alpha images with the broad ultraviolet filter. The far ultraviolet light imagery from the Narrow Field Imagery also captured two background stars, whose surface temperatures must be approximately twice as hot as the our Sun’s to be so bright in this wavelength of light.
NASA/Carruthers Geocorona Observatory

When Carruthers captured these images, the Moon was also in its field of view and slightly closer to the spacecraft than Earth was, making the Moon appear larger and closer to Earth than usual.

The specific wavelength Carruthers observed in two of the images, called Lyman-alpha, is light emitted by atomic hydrogen. The faint glow of Lyman-alpha from hydrogen in Earth’s outer atmosphere is called the “geocorona,” Latin for “Earth crown.”

In the broad-spectrum images, the Moon and Earth look similar: both are spheres with well-defined edges. However, in the Lyman-alpha filter, the Moon still appears as a crisp, sharp sphere while Earth appears surrounded by a bright “fuzz” extending out to space. This glow is the geocorona, the primary focus of the Carruthers mission. It is the only way to “see” Earth’s outermost atmospheric layer, although the light of the geocorona has only been photographed a handful of times in history. Carruthers will be the first mission to image it repeatedly, and from far enough away to see its great extent and discover how it changes over time.

These first images also offer a rare treat: sunlight reflected off the far side of the Moon, a view impossible to capture from Earth.




Original
Annotated

An interactive slider image allowing the user to swipe between two versions of an image, one with annotations and one without. The image shows a spacecraft’s view of Earth (at center) and the Moon (lower left) in ultraviolet light. The image includes a circular heatmap with a bright yellow center (Earth) fading to green and blue at the edges, showing Earth’s geocorona. A smaller bright spot appears near the bottom edge (the Moon). A vertical color bar labeled

An interactive slider image allowing the user to swipe between two versions of an image, one with annotations and one without. The image shows a spacecraft’s view of Earth (at center) and the Moon (lower left) in ultraviolet light. The image includes a circular heatmap with a bright yellow center (Earth) fading to green and blue at the edges, showing Earth’s geocorona. A smaller bright spot appears near the bottom edge (the Moon). A vertical color bar labeled

An interactive slider image allowing the user to swipe between two versions of an image, one with annotations and one without. The image shows a spacecraft’s view of Earth (at center) and the Moon (lower left) in ultraviolet light. The image includes a circular heatmap with a bright yellow center (Earth) fading to green and blue at the edges, showing Earth’s geocorona. A smaller bright spot appears near the bottom edge (the Moon). A vertical color bar labeled
An interactive slider image allowing the user to swipe between two versions of an image, one with annotations and one without. The image shows a spacecraft’s view of Earth (at center) and the Moon (lower left) in ultraviolet light. The image includes a circular heatmap with a bright yellow center (Earth) fading to green and blue at the edges, showing Earth’s geocorona. A smaller bright spot appears near the bottom edge (the Moon). A vertical color bar labeled

Original

Annotated

Carruthers Geocorona ObservatorY

A View of Earth’s Geocorona

Narrow Field Imager/Lyman-alpha filter


This view of the Earth, Moon, and Earth’s geocorona was captured by the Carruthers Geocorona Observatory’s Narrow Field Imager on Nov. 17, 2025. Move the slider to switch between the original version and one with overlaid annotations. In the annotated version, labels for Earth, the Moon, and Earth’s geocorona are overlaid on the image. The circle around Earth represents Earth’s surface, and the arc around Earth’s middle represents the orientation of Earth’s equator. The arrow pointing up and slightly to the left from Earth represents Earth’s rotational axis. The arrow pointing out to the right from Earth represents the direction to the Sun. The color scale indicates brightness, with brighter light appearing more yellow and dimmer light appearing more blue. The ‘glow’ that extends beyond Earth’s surface and out into space is Earth’s geocorona, which is emitted by hydrogen atoms in Earth’s exosphere in a wavelength of ultraviolet light known as Lyman-alpha.

These initial images were taken with short, five-minute exposures — just long enough to confirm that the instrument is performing well. During the main science phase, Carruthers will take 30-minute exposures, allowing it to reveal even fainter details of the geocorona and trace how Earth’s outer atmosphere responds to the changing Sun.

Carruthers launched on Sept. 24 and is just a few weeks from completing its journey to the Sun-Earth Lagrange point 1, a point of gravitational balance roughly 1 million miles closer to the Sun than Earth is. Carruthers will begin its primary science phase in March 2026, when it will begin sending back a steady stream of ultraviolet portraits of our planet’s ever-shifting outer atmosphere.

By Miles Hatfield
NASA’s Goddard Space Flight Center, Greenbelt, Md.

About the Author

Miles Hatfield

Miles Hatfield

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NASA’s IMAP Mission Captures ‘First Light,’ Looks Back at Earth 

NASA’s IMAP Mission Captures ‘First Light,’ Looks Back at Earth 

3 min read

NASA’s IMAP Mission Captures ‘First Light,’ Looks Back at Earth 

All 10 instruments aboard NASA’s newly launched IMAP (Interstellar Mapping and Acceleration Probe) mission have successfully recorded their first measurements in space. With these “first light” observations, the spacecraft is now collecting preliminary science data as it journeys to its observational post at Lagrange point 1 (L1), about 1 million miles from Earth toward the Sun. 

“We are extremely pleased with the initial in-flight performance of the IMAP mission. All instruments have successfully powered on and our commissioning remains on track. We have already collected useful data including exercising our near-real-time space weather data stream,” said Brad Williams, IMAP program executive at NASA Headquarters in Washington. “This successful milestone is quickly setting the stage for the start of our primary science operations.”

As a modern-day celestial cartographer, IMAP will chart the boundaries of the heliosphere — a huge bubble created by the Sun’s wind that encapsulates our entire solar system — and study how the heliosphere interacts with the local galactic neighborhood beyond.

To map the heliosphere’s boundaries, IMAP is equipped with three instruments that measure energetic neutral atoms: IMAP-Lo, IMAP-Hi, and IMAP-Ultra. These uncharged particles, called ENAs for short, are cosmic messengers formed at the heliosphere’s edge that allow scientists to study the boundary region and its variability from afar. 

An animated GIF shows a large oval that is initially filled with large rectangular pixels of different colors from dark blue, light blue, green, yellow, orange, red, and pink. The pixels change color rapidly. The oval then goes from filled to only having two large vertical bands of colored pixels and then two thinner vertical bands of pixels, with the rest of the oval becoming gray, with no data. At the center of the oval a white dot is labeled
These partial maps of the heliosphere’s boundaries were compiled from first-light data from the IMAP-Hi, IMAP-Lo, and IMAP-Ultra instruments. These initial looks offer a first glimpse at the detail NASA’s IMAP (Interstellar Mapping and Acceleration Probe) will be able to capture. The warmer colors show regions with more energetic neutral atoms (ENAs).
NASA

“It’s just astounding that within the first couple weeks of observations, we see such clear and consistent ENA data across the factor of 10,000 in energy covered collectively by the three imagers,” said David McComas, Princeton University professor and principal investigator for the IMAP mission. “This, plus excellent first light data from all seven of the other instruments, makes for a 10 out of 10, A-plus start to the mission.”

As IMAP travelled away from Earth, the IMAP-Ultra instrument looked back at the planet and picked up ENAs created by Earth’s magnetic environment. These terrestrially made ENAs, which overwhelm ENAs coming from the heliosphere in sheer numbers, is a reason why IMAP will be stationed at L1. There the spacecraft will have an unobstructed view of ENAs coming from the heliosphere’s boundaries.

An elongated, horizontal colorized map shows rectangular pixels of different colors, mostly blue and green but dominated by a large circular feature in red, orange, and yellow on the far left. The background is mostly blue but two large swatches of green appear near the top center and bottom center.
Earth’s magnetic environment can be seen glowing bright in this image taken by the IMAP-Ultra instrument, which includes ENA data as well as noise. Earth sits at the center of the red donut-shaped structure. This image was taken as IMAP left Earth for its post at Lagrange point 1.
NASA

The mission will also study the solar wind, a continuous flow of charged particles coming from the Sun. Solar wind observations from five of IMAP’s instruments will be used by the IMAP Active Link for Real-Time (I-ALiRT) system to provide roughly a half hour’s warning to voyaging astronauts and spacecraft near Earth about harmful space weather and radiation coming their way. The IMAP instruments are already making near-real-time solar wind measurements that can be used to support space weather forecasts. The I-ALiRT network is being exercised and will be ready for space weather forecasters when IMAP starts its regular science mission at L1.

With all of IMAP’s instruments up and running, the mission has nearly completed its commissioning stage and will arrive at L1 in early January. The mission is now working to complete the final commissioning steps and instrument calibration with the goal of being ready to take operational science data starting Saturday, Feb. 1, 2026. 

Here’s a look at IMAP’s instruments and what they’ve seen in their first-light observations.

By Mara Johnson-Groh
NASA’s Goddard Space Flight Center, Greenbelt, Md.

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NASA, Partners Share First Data From New US-European Sea Satellite

NASA, Partners Share First Data From New US-European Sea Satellite

5 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

A map showing a portion of the North Atlantic Ocean, with the U.S. Eastern seaboard along the left side of the frame, is covered with wide yellow lines criss-crossing in X shapes. Written on the lines in black ink is either “S6MF” for Sentinel-6 Michael Freilich or “S6B” for Sentinel-6B, showing the orbital paths of each satellite. On the left side of the image, a legend labeled “sea level anomaly (cm)” shows a vertical, rainbow-hued graph ranging from dark blue at the bottom to dark red at the top; the colors correspond to blobs of each shade that cover the ocean on the map.
Sentinel-6B and Sentinel-6 Michael Freilich captured data on Nov. 26 of sea levels across a vast stretch of the Atlantic. Within the crisscrossing bands, red indicates higher water relative to the long-term average; blue indicates lower water. The tracks are layered atop the combined observations of other sea-level satellites.
EUMETSAT

Launched in November, Sentinel-6B will track ocean height with ultraprecision to advance marine forecasting, national security, and more.

Sentinel-6B, a joint mission by NASA and its U.S. and European partners to survey 90% of the world’s oceans for the benefit of communities and commerce, has started sending back its first measurements since launching in November. A newly published map of the data shows sea levels across a vast stretch of the Eastern Seaboard and Atlantic Ocean. 

About the size of a pickup truck, Sentinel-6B extends a decades-long effort led by the United States and Europe to track ocean height down to fractions of an inch using radar altimetry. Once its instruments and algorithms are fully calibrated next year, Sentinel-6B will return actionable data for ship crews, weather forecasters, national security, and the millions of people who live and work near coastlines.  

“NASA does incredible science using the unique vantage point of space every day to deliver life-saving data directly into the hands of decision-makers for storms, navigation, flooding, and more,” said Nicky Fox, associate administrator, Science Mission Directorate, NASA Headquarters in Washington. “The ocean measurements that Sentinel-6B collected during its first months in orbit benefit all, providing key insights to ensure the prosperity and security of coastal communities around the globe.” 

In addition to measuring sea level, instruments aboard the satellite will gather information on wind speeds, wave heights, atmospheric temperature, and humidity. In turn, that data can be used by U.S. agencies as well as to refine the Goddard Earth Observing System atmospheric forecast models, which the NASA Engineering and Safety Center relies on to plan safer re-entry of astronauts returning from Artemis missions.  

Mission teams in recent weeks have verified that Sentinel-6B and all its instruments are in good health. That includes the Poseidon-4 Synthetic Aperture Radar altimeter, the Advanced Microwave Radiometer for Climate, the Global Navigation Satellite System – Radio Occultation, and the Precise Orbit Determination Package. 

In the visualization above, featuring data captured by Sentinel-6B on Nov. 26, the crisscrossing bands trace the satellite’s path as it orbits Earth. The image also shows data collected on the same day by the satellite’s twin, Sentinel-6 Michael Freilich, which launched in 2020. The data in those bands is layered over the combined observations of other sea-level satellites across the region shown. Red indicates higher water relative to the long-term average; blue areas indicate lower water. Because the spacecraft’s instruments have not been fully calibrated, the data is considered preliminary but also quite promising. 

Together, Sentinel-6B and Sentinel-6 Michael Freilich make up the Copernicus Sentinel-6/Jason-CS (Continuity of Service) mission developed by NASA, ESA (European Space Agency), EUMETSAT (European Organisation for the Exploitation of Meteorological Satellites), and the National Oceanic and Atmospheric Administration (NOAA). 

“These first light images from Sentinel-6B underscore the value of Earth science observations in providing life-saving and economic-empowering data to communities along our world’s coastlines, where a third of the globe’s population lives,” said Karen St. Germain, director, NASA Earth Science Division at the agency’s headquarters. “This achievement also highlights the power of partnerships with ESA, EUMETSAT, and our sister science agency NOAA in advancing our collective understanding of Earth systems and putting that Earth science understanding to work for the benefit of humanity.” 

Sentinel-6/Jason-CS adds to a continuous sea level rise dataset that began in the early 1990s. Since then, the rate of sea level rise globally has doubled and currently averages about 0.17 inches (4.3 millimeters) per year. The rate differs between locations, with implications for coastal infrastructure, trade routes, and storm formation. 

“The accuracy and precision of this mission’s gold-standard dataset speaks to the foresight, more than 30 years ago, of investing in the technology and expertise that make it possible,” said Dave Gallagher, director, NASA’s Jet Propulsion Laboratory in Southern California. “We’re proud to continue partnering to collect these critical measurements into another decade, and even prouder of the teams behind this most recent milestone.” 

Flying 830 miles (1,336 kilometers) above Earth, Sentinel-6B is about 30 seconds behind its twin, Sentinel-6 Michael Freilich, currently the official reference satellite for sea level. Eventually, Sentinel-6B will take over that role, and Sentinel-6 Michael Freilich will move into a different orbit.

More about Sentinel-6B 

Copernicus Sentinel-6/Jason-CS was jointly developed by ESA, EUMETSAT, NASA, and NOAA, with funding support from the European Commission and technical support from CNES. The mission, starting with Sentinel-6 Michael Freilich, marked the first international involvement in Copernicus, the European Union’s Earth Observation Programme. 

Managed for NASA by Caltech in Pasadena, JPL contributed three science instruments for each Sentinel-6 satellite: the Advanced Microwave Radiometer, the Global Navigation Satellite System – Radio Occultation, and the laser retroreflector array. NASA also contributed launch services, ground systems supporting operation of the NASA science instruments, the science data processors for two of these instruments, and support for the international ocean surface topography community. 

For more about Sentinel-6B, visit: 

https://science.nasa.gov/mission/sentinel-6B/

News Media Contacts

Elizabeth Vlock
NASA Headquarters, Washington
202-358-1600
elizabeth.a.vlock@nasa.gov

Andrew Wang / Andrew Good
Jet Propulsion Laboratory, Pasadena, Calif.
626-379-6874 / 626-840-4291
andrew.wang@jpl.nasa.gov / andrew.c.good@jpl.nasa.gov

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A Subtle Return of La Niña 

A Subtle Return of La Niña 

A data visualization of Earth centered on the equatorial Pacific Ocean shows a strip of blue spanning part of the ocean basin’s middle, indicating where sea levels are lower than normal.
December 1, 2025

After a several-month hiatus, La Niña returned to the equatorial Pacific Ocean in September 2025 and has continued into December. However, this occurrence of El Niño’s cooler counterpart is relatively weak, and its influence on weather and climate over the next several months remains to be seen.  

Part of the El Niño-Southern Oscillation (ENSO) cycle, La Niña develops when strengthened easterly trade winds intensify the upwelling of cold, deep water in the eastern tropical Pacific. This process cools large swaths of the eastern and central equatorial Pacific while simultaneously pushing warm surface waters westward toward Asia and Australia. In a report published on December 11, the NOAA Climate Prediction Center confirmed that below-average sea surface temperatures associated with La Niña conditions were present and likely to continue for another month or two.

The shifting wind patterns and the movement of heat within the ocean have a direct impact on sea level. Because cooler water is denser and occupies less volume than warm water, sea levels in the central and eastern Pacific drop during La Niña events. The map above shows sea surface height observed on December 1, 2025. Shades of blue indicate below-normal sea levels, shades of red show above-normal levels, and white represents near-normal conditions.

Data for the map were acquired by the Sentinel-6 Michael Freilich satellite and processed by scientists at NASA’s Jet Propulsion Laboratory (JPL). Signals related to seasonal cycles and long-term trends have been removed to highlight sea level changes associated with ENSO and other short-term natural phenomena. The satellite’s twin successor, Sentinel-6B, launched in November 2025 and is expected to begin contributing to ENSO research and forecasts sometime in 2026.

This equatorial surface-water cooling alters the exchange of heat and moisture between the ocean and atmosphere, reshaping global atmospheric circulation patterns. La Niña’s coupling with the ocean and atmosphere can shift mid-latitude jet streams, intensifying rainfall in some regions while bringing drought to others.

Typically, La Niña years bring below-average rainfall to the American Southwest and above-average rainfall to the Northwest. But when the event is weak—whether El Niño or La Niña—the associated weather patterns can be “notoriously difficult to predict,” said Josh Willis, an oceanographer and Sentinel-6 Michael Freilich project scientist at JPL in Southern California.

“It still has the potential to tilt our winter toward the dry side in the American Southwest,” Willis said. “But it’s never a guarantee, especially with a mild event like this one.”

NASA Earth Observatory image by Lauren Dauphin, using modified Copernicus Sentinel data (2025) processed by the European Space Agency and further processed by Josh Willis and Kevin Marlis/NASA/JPL-Caltech. Story by Kathryn Hansen. 

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