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APOD: 2026 September 17 – A Treasure Chest in the Carina Nebula

17 September 2026 at 05:05

APOD

Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

A colorful nebula resembles an open treasure chest on a field of stars

A Treasure Chest in the Carina Nebula

Explanation: This treasure chest is full of stars. The featured image was obtained with NASAβ€˜s James Webb Space Telescope and shows a dust pillar in the Carina Nebula inside our Galaxy, roughly 7500 light-years away. It is formed by interstellar gas and dust, and shaped by powerful stellar winds and radiation from neighboring stars like the nearby Eta Carinae stellar system which is more luminous than 5 million suns. The star formation inside the pillar is excavating its head, creating the open lid of the chest. Astronomers estimate that there are about 70 stars in a compact cluster inside the pillar. This cluster is now thought to be only around 1.3 million years old. Its bounty of young stars includes a massive star approximately 19 times as massive as the Sun. More massive stars are rarer, shine brighter and evolve faster than less massive stars. They are the shiniest jewels in the treasure chest.

APOD’s main NASA site is moving : From apod.nasa.gov to science.nasa.gov/apod
Tomorrow’s picture: what’s next?

Date September 17, 2026
Credit ESA/Webb, NASA & CSA, M. Reiter; Acknowledgement: M. H. Γ–zsaraΓ§
Authors & editors: Cecilia Chirenti, Robert Nemiroff, Jerry Bonnell, Keighley Rockcliffe
A service of: ASD at NASA / GSFC,
NASA Science Activation & Michigan Tech. U.

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Summer Goes Out With a Heat Dome

17 September 2026 at 05:01
Air temperatures in the United States are depicted in white to light blue (cooler) and orange to red (warmer). An area of red, indicating temperatures around 100 degrees Fahrenheit, covers Texas and several states to the east and northeast.
An area of high pressure over the south-central U.S. produced unseasonable and, in some places, record-breaking warmth on September 15, 2026, as shown in this map of modeled air temperatures from GEOS (Goddard Earth Observing System).
NASA Earth Observatory/Michala Garrison

While the calendar indicated that astronomical summer was winding down, a swath of the south-central United States was sweltering under a heat dome in mid-September 2026.

This map shows air temperatures in the contiguous U.S. on September 15, 2026, at 4 p.m. Central Time (21:00 Universal Time), modeled at 2 meters (6.5 feet) above the ground. It was produced by combining satellite observations with temperatures predicted by a version of theΒ GEOSΒ (Goddard Earth Observing System) model, which uses mathematical equations to represent physical processes in the atmosphere. The darkest reds indicate areas where temperatures approached or exceeded 40 degrees Celsius (104 degrees Fahrenheit).

More than 41 million people in the U.S.β€”about 12 percent of the populationβ€”were under a National Weather Service extreme heat advisory, extreme heat watch, or extreme heat warning on September 15. The high temperatures spanned large portions of several states, such as Texas, Oklahoma, Arkansas, Missouri, and Tennessee. Meteorologists warned that high humidity, limited cloud cover, and light winds could make temperatures feel higher than thermometer readings and increase the risk of heat-related illnesses.

Several locations set new daily high temperature records on September 15. These included Dallas, Texas, at 101ΒΊF (38ΒΊC), Memphis, Tennessee, at 99ΒΊF (37ΒΊC), and Nashville, Tennessee, at 100ΒΊF (38ΒΊC). The cities were all at least 12ΒΊF warmer than normal that day, with Nashville breaking its daily-high record from 1927. The day before, Nashville also set a record-high minimum temperature of 75ΒΊF (24ΒΊC).

A weather phenomenon meteorologists call a heat dome was responsible for driving temperatures up across the region. A heat dome develops when an area of high pressure in the upper atmosphere pushes hot air toward the surface and traps it there. Heat domes put the brakes on convection and suppress clouds and precipitation. This allows sunlight to reach Earth’s surface relatively unhindered and further elevate air temperatures.

The stretch of unseasonable temperatures follows the warmest June through August in the contiguous United States in a 132-year record, according to NOAA. The three-month period in 2026 was 0.4ΒΊF warmer than the previous records, set in 1936 and 2021.

NASA Earth Observatory image by Michala Garrison,Β usingΒ GEOS-FPΒ data from theΒ Global Modeling and Assimilation OfficeΒ at NASA GSFC. Story by Lindsey Doermann.

Downloads

Air temperatures in the United States are depicted in white to light blue (cooler) and orange to red (warmer). An area of red, indicating temperatures around 100 degrees Fahrenheit, covers Texas and several states to the east and northeast.

September 15, 2026

JPEG (1.22 MB)

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Passion Meets Precision at NASA’s Flight Research Lab

16 September 2026 at 22:06

4 min read

Passion Meets Precision at NASA’s Flight Research Lab

One man communicates with a hand-held radio, as two other men wait to the side for the go-ahead command to fly an experiment on a drone.
Derek Abramson, Dale Reed Subscale Flight Research Laboratory chief engineer, left, communicates with the Edwards Air Force Base air traffic control tower for approval to fly the Alta-X drone near NASA’s Armstrong Flight Research Center in Edwards, California, on Thursday, Aug. 27, 2026. Justin Link, small uncrewed aircraft pilot, second from left, and laboratory chief pilot Justin Hall await flight clearance. Researchers at NASA’s Johnson Space Center in Houston developed the advanced guidance and navigation system known as the Safe and Precise Landing – Integrated Capabilities Evolution (SPLICE) experiment, which is installed on the Alta-X. SPLICE will help spacecraft land precisely and detect and avoid potential hazards, which is critical for NASA missions to the Moon and to Mars.
NASA/Ryan Kline

Long before they helped shape NASA’s future aerospace breakthroughs, Derek Abramson, Justin Hall, and Justin Link were in their garages and homes building radio‑controlled aircraft, testing new ideas, and flying their creations at hobby events. That early passion now fuels the work of NASA’s Dale Reed Subscale Flight Research Laboratory at the agency’s Armstrong Flight Research Center in Edwards, California.

At NASA Armstrong’s subscale flight lab, the team turns that lifelong enthusiasm into mission-focused innovation. The laboratory supports research that ranges from advanced navigation systems for future landings on the Moon and Mars to emerging aeronautics concepts that need quick, low-cost evaluation. NASA’s small, remotely piloted and autonomous aircraft allow engineers to explore ideas that could be difficult, risky or expensive to test at full scale.

Skilled team

Abramson, Hall, and Link play key roles in that work. Abramson serves as the laboratory’s chief engineer. Hall is the chief pilot. Link is a drone pilot. Together, they integrate emerging aerospace technologies with the lab’s subscale aircraft fleet and, when needed, design and build aircraft or flight experiments to evaluate new concepts.

A boy holds a large radio-controlled black-and-yellow helicopter.
Derek Abramson, chief engineer at the Dale Reed Subscale Flight Research Laboratory at NASA’s Armstrong Flight Research Center in Edwards, California, is shown with his Kalt Cyclone radio-controlled helicopter in the mid-1980s. Abramson loved flying this aircraft as a child, and he has been an aviation enthusiast for as long as he can remember.
Derek Abramson

Abramson’s expertise, built through service in the U.S. Navy and the aerospace industry, centers on technical oversight, management, and system design. Hall is known for creative approaches to problem solving and uses practical methods to address technical challenges and maintain flight safety. Link specializes in designing and fabricating research vehicles and draws on extensive hands-on experience to understand what works, and what does not, in flight.Β 

On weekends, the team often tinkers in their garages or hangars building radio-control aircraft, researching hobby trends, or exploring new technologies. You might see them flying their creations at hobby events or attending trade shows. Their passion for flight brought Abramson, Hall, and Link together years before they one-by-one joined NASA more than a decade ago, though each discovered that spark in a different way.

Early influences

Abramson’s interest began as a child with rubber-band powered stick and tissue aircraft and radio-controlled models. His early aviation pursuits led to his first solo flight while in high school and a pilot’s license. In the Navy, he worked on multiple aircraft, including EA-6B and the F-18, as an avionics technician. As an engineer, he supported the B-1 and CV-22 Osprey aircraft flight tests. As an intern at NASA Armstrong, he used his operational and engineering experience on remotely piloted and autonomous aircraft.

Hall’s interest grew after seeing historic aircraft including the Mach 3 SR-71 fly over his elementary school playground and watching Space Shuttle Challenger land from above his dad’s shoulders. He has built and flown model and remotely piloted aircraft for as long as he can remember. His reputation flying radio-controlled hobby aircraft at fly-ins and trade events led to an offer to fly subscale aircraft at NASA.

Two men stand by a yellow and black radio-controlled aircraft.
Justin Hall, chief pilot at the Dale Reed Subscale Flight Research Laboratory at NASA’s Armstrong Flight Research Center in Edwards, California, stands in front of a radio-controlled aircraft with his dad, David Hall, in August 2020. David Hall built the Gee Bee aircraft years earlier but was unable to fly it due to his health. He asked his son to fly the aircraft so he could see it in the air, which Justin did the day of this photo. Shortly afterward, David Hall passed away.
Justin Hall
Two men hold a large radio-controlled aircraft. The aircraft is red with white and black stripes.
Justin link, drone pilot at the Dale Reed Subscale Flight Research Laboratory at NASA’s Armstrong Flight Research Center in Edwards, California, and his dad, Don Link, hold a Firebird radio-controlled aircraft on the day of its first flight in September 2023. It was a project they worked on together. Don Link reduced the dimensions of the original larger-scale model aircraft and drew the plans, while Justin Link manufactured composite molds and built the aircraft from scratch.
Justin Link

Link was five years old when he built balsa-wood aircraft with his dad and flew them in a field near their home. As he grew older, his hobby expanded to include radio-controlled cars, boats, helicopters, and aircraft. Aviation runs deep in Link’s family. His great grandfather served in the U.S. Army Air Corps, his grandfathers served in the U.S. Air Force, and his dad was an Air Force avionics technician. Link raced sailplanes, competed with scaled warbird aircraft, and was encouraged by family and friends to pursue an aviation profession. He has worked with large drones for more than 11 years, focusing on research and development, composite materials, and specialized fabrication methods.

Together, the team applies its experience and knowledge in rapid design, fabrication, integration and flight testing to bring new ideas to flight. Their work continues to support NASA’s missions across aeronautics, science, and exploration.

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Amendment 74: A.14 Atmosphere Research Program Due Date Delay and Clarification Regarding the use of Generative AI

16 September 2026 at 21:28

Through ROSES-25 A.14 Atmosphere NASA is soliciting proposals for data analysis and modeling of NASA supported airborne campaign data. NASA’s Earth Science Division has supported numerous airborne campaigns during the last few years, see Section 2 of the program element text.

A.14 Atmosphere required a mandatory Notice of Intent (NOI) to propose. Proposers who have not already submitted a compliant NOI are not eligible to submit a proposal.

ROSES-2025 Amendment 74 delays the due date for A.14 Atmosphere to December 2, 2026. Also, Section 4.3.3 β€œUse of Generative AI” now mentions a related NSPIRES cover page question on the use of AI. An updated FAQ has been posted under β€œOther Documents” on the NSPIRES page for this program element.

Questions concerning A.14 Atmosphere may be directed to Ken Jucks at kenneth.w.jucks@nasa.gov, Emma Knowland atΒ  k.e.knowland@nasa.gov, and the other points of contact that appear in Section 4 of the text.

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IRIS Stories

16 September 2026 at 21:07
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Cargo Mission and Crew-13 Updates; Station Research, Maintenance Continue

16 September 2026 at 20:40
NASA's SpaceX Crew-12 members (from left), Andrey Fedyaev of Roscosmos, Jack Hathaway and Jessica Meir of NASA, and Sophie Adenot of ESA speak to journalists on the ground during a news conference on Wednesday, Sept. 16.
NASA’s SpaceX Crew-12 members (from left), Andrey Fedyaev of Roscosmos, Jack Hathaway and Jessica Meir of NASA, and Sophie Adenot of ESA speak to journalists on the ground during a news conference on Wednesday, Sept. 16.

New supplies are on their way to the International Space Station after launching aboard a Progress 96 cargo spacecraft at 9:33 a.m. EDT on Wednesday. Progress 96 will arrive Saturday for an automated docking to the Poisk module at 9:46 a.m. EDT bringing nearly three tons of food, fuel, and cargo to the Expedition 75 crew members.

NASA and SpaceX are now targeting as soon as early October for the launch of the Crew-13 mission to allow for completion of prelaunch activities, readiness reviews, and coordination of space station operations. The team successfully replaced an oxidizer valve in Dragon’s propulsion system after a leak was detected earlier in processing.

In the meantime, the seven residents aboard the orbiting outpost stayed focused on ongoing microgravity research, cargo operations, and lab maintenance throughout Wednesday.

Station commander Jessica Meir of NASA began her shift documenting her sleep quality, collecting a saliva sample, and downloading biomedical data collected from her smart watch to a computer tablet. Researchers will analyze Meir’s health metrics for the RelaxPro investigation to help reduce stress and improve sleep for astronauts. Next, she transferred cargo in and out of Northrop Grumman’s Cygnus XL cargo spacecraft which has been berthed to the Unity module’s Earth-facing port since April 14.

NASA flight engineer Anil Menon once again soldered components on a circuit board in the Harmony module using lead-free soldering techniques to demonstrate the safe manufacturing and repairing of electronics in microgravity. The space-soldered samples will be returned to Earth and compared to identical ground-soldered samples. Results may lead to reduced reliance on costly resupply missions.

NASA flight engineer Jack Hathaway spent his shift inside the Destiny laboratory module installing new water filter cartridges in the oxygen generation system. The filters remove fluoride ions keeping water pure and clean as it passes through the spacecraft’s systems.

Flight engineer Sophie Adenot of ESA (European Space Agency) worked out on the new European Enhanced Exploration Exercise Device (E4D) installed inside the Columbus laboratory module. Controller software on the E4D tracked her performance helping researchers evaluate its effectiveness for use onΒ future long-duration missions.

The three cosmonauts from Roscosmos, flight engineers Pyotr Dubrov, Anna Kikina, and Andrey Fedyaev, spent their shift on station maintenance. Dubrov tested power systems and cleaned vents in the Zvezda service module. Kikina serviced Zvezda’s Elektron oxygen generator and cleaned fan screens in the Rassvet module. Fedyaev inspected and photographed laptop computers and their power supplies.

Fedyaev and his SpaceX Crew-12 crewmates Meir, Hathaway, and Adenotβ€”who have been aboard the space station since February 14β€”also participated in a news conference with journalists on the ground. Meir commented on her recent spacewalk when she rode the Canadarm2 robotic arm, β€œI felt like I was just there levitating above the Earth. I think that was the biggest eureka moment for me.”

Learn more about station activities by following the space station blog, @space_station on X, as well as the ISS Facebook and ISS Instagram accounts.

Get the latest from NASA delivered every week. Subscribe here.

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Educator’s Guide – Exploring Magnetism

16 September 2026 at 19:07

In this teacher’s magnetism activity guide, β€œExploring Magnetism,” students are given the opportunity to act as scientists discovering magnetic fields and electromagnetism through inquiry and measurement.

Included at the beginning of each session is a summary of the session, a list of national education standards that the session covers, and a list of materials required for the session. Each session is broken into several activities, with each activity outlined for the teacher. In the Background Material section, you can find science background for the lessons. A glossary can be found after the background section, and at the very end we recommend different resources finding materials to purchase and for learning more about magnetism.

The activities in this guide are meant as primers for supplementary guides that allow students to learn about the importance of magnetic fields in space science, which are studied by NASA scientists. For example, in Exploring Magnetism in the Solar Wind, students learn about the stream of charged particles emanating from the Sunβ€”called the Solar Windβ€” and how NASA scientists are designing a mission called STEREO to study it and its magnetic field. The other guides, Exploring Magnetism in Solar Flares and Exploring Magnetism in the Aurorae, allow students to learn about magnetism in the Sun-Earth System with more hands-on lessons.

Credit: University of California, Berkeley

Find the resource here β†—

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NASA’s Moon Orbiter Spots New, β€˜Once-in-Century’ Moon Crater

16 September 2026 at 19:06
6 Min Read

NASA’s Moon Orbiter Spots New, β€˜Once-in-Century’ Moon Crater

Black-and-white image of a textured, cratered surface. Two black arrows near the center point inward toward a small, dark, circular feature.
A zoomed-in view of the Moon made from images from NASA’s Lunar Reconnaissance Orbiter Camera. (More information at the bottom of article.)
Credits: NASA Goddard/Intuitive Machines/Robert Wagner

It started as a routine data-quality check. But as Robert Wagner, a scientist with NASA’s Lunar Reconnaissance Orbiter (LRO), scanned a giant Moon map on his computer screen, an unusually large bright spot circled by a dark halo caught his eye, as it implied that surface material in that area had been shaken up.

β€œI just stopped, dropped everything, and started looking into what that spot was,” said Wagner, an image-processing specialist from Intuitive Machines who works with data from the Lunar Reconnaissance Orbiter Camera (LROC) system.

By comparing before and after images of the Moon, Wagner realized he had discovered the largest, newly formed crater ever found in the solar system, as scientists reported Wednesday in Science Advances. This discovery highlights the value of NASA’s Moon orbiter data in studying a dynamic landscape as the agency advances a sustained human presence and expanded scientific and commercial activity on the Moon.

Two nearly identical black-and-white images appear side by side, separated by a vertical black line. Each shows a dark, uneven surface with scattered small circular depressions and several larger round formations with bright, raised rims. In the left image, a thin white circle marks a small, white spot near the center; there is no circled, white spot in the the corresponding area in the right image.
A zoomed-in view of McGetchin crater, circled on the left, next to a β€œbefore” image on the right. The panel on the left is made from images captured by NASA’s Lunar Reconnaissance Orbiter Wide-Angle Camera in summer 2025; the right panel was made from images taken in spring 2011. The white spot is not the crater itself, but rather material flung out of the crater, which formed when a rock, possibly this size of a three- to six‑story building, crashed into the Moon between April 11 and May 22, 2024 – a once-in-a-century event, as scientists reported on Sept. 15, 2026, in a pair of papers in Science Advances. The area shown in the images is 38 miles wide.
NASA Goddard/Intuitive Machines/Robert Wagner

Officially named McGetchin after pioneering lunar scientist Tom McGetchin, the crater formed on the Moon’s eastern edge sometime between April 11 and May 22, 2024, after a comet or asteroid the size of a three- to six-story building hit the surface.
Β 
The crash left a crater, 728 feet wide, that spans the length of two football fields. And at 141 feet deep, the crater could fit three vertically stacked yellow school buses.
Β 
Scientists estimate that an impact of this magnitude happens on the Moon about once in a century or even longer.

Moon takes some hits

For more than 17 years, LRO has been circling the Moon and using its seven instruments to map the topography, surface composition, temperature, and radiation environment there. The spacecraft’s team has identified at least 1,000 new impact craters throughout the mission and flagged 100,000 more surface changes from an object smashing into the Moon or from the debris that flung out after.

With no atmosphere to slow them or burn them up, space rocks and other objects easily reach the lunar surface. Most are much smaller compared to the object that carved out McGetchin crater. The smallest craters scientists can distinguish from LRO images are about 30 feet wide, the length of a three-story building laid on its side, made by rocks about 43 inches wide, the size of a monster-truck tire. Scientists estimate that impacts of this scale produce about 140 new craters across the Moon each year. But most new ones are made by microscopic projectiles that leave holes too small to identify in orbital images.

With its numerous instruments, the spacecraft can observe changes to the lunar surface that aren’t apparent in the LROC images alone. After the crater was discovered, scientists working with LRO’s thermal instrument, Diviner, made follow-up observations of the site. They found a 4-mile-wide area around the crater that is about 16 degrees Fahrenheit cooler at night than its surroundings.

Animated temperature map that alternates between two images. A vertical strip through the center blinks on and off, revealing a dark blue circular area surrounding a small white spot near the middle. The pale blue map also contains scattered yellow, orange, and red spots and rings, including a large, curved red-and-yellow feature near the lower center. A 5-kilometer scale bar appears at lower left, and a color key ranges from 90 kelvin in dark blue to 130 kelvin in dark red.
This animated image set shows an area on the eastern limb of the Moon before and after McGetchin crater formed there sometime between April 11 and May 22, 2024. The post-impact image was constructed using data taken by NASA’s Lunar Reconnaissance Orbiter (LRO) thermal instrument, Diviner, between Nov. 15, 2025, and Feb. 18, 2026, after scientists discovered the crater in visible-light images taken by LRO’s Wide-Angle Camera. Pre-impact temperatures are from the Diviner Global High-Resolution Mosaics (GHRM). The crater formed on the Moon after a comet or asteroid, possibly the size of a six-story building, hit the surface in a rare, once-in-a-century collision. The dark blue strip that flashes into view reveals a 4-mile-wide β€œcold spot” around the crater that is about 16 degrees Fahrenheit cooler at night than its surroundings. This cooling happens because an impact fluffs up regolith around a crater, making it less dense and therefore less able to retain heat. Scientists on the Diviner team reported this finding in a paper published on Sept. 16, 2026, in Science Advances. The red and yellow spots indicate areas typically associated with rocks excavated by long-ago impacts which, though still at cryogenic temperatures like their surroundings, remain slightly warmer at night.
NASA Goddard/UCLA/JHU APL

Reporting in a second paper Wednesday in the same journal, researchers say that the cooling happens because the impact fluffs up the regolith around the crater, making it less dense and therefore less able to retain heat.

The large extent of this β€œcold spot” is striking, scientists say, because it shows that impacts can modify the Moon’s surface far beyond the crater itself. These physical changes could affect how rover wheels interact with the surface, for instance.

Wide black-and-white image of a rough, uneven surface densely covered with circular depressions and raised areas. The upper and lower edges are especially rugged, while the center is smoother and divided by subtle vertical bands. A black arrow left of center points toward a faint, narrow vertical mark.
A global view of the Moon made by stitching together hundreds of images from the Wide-Angle Camera aboard NASA’s Lunar Reconnaissance Orbiter (LRO). Robert Wagner, image processing specialist for LRO, made this map using two sets of mages taken several years apart. He used a software designed to highlight any changes between the two sets. Anything that stayed the same turned gray; anything different showed up as bright or dark patches. A black arrow just left of center points to McGetchin crater.
NASA Goddard/Intuitive Machines/Robert Wagner

Road to discovery

The LROC system collects images from about 60 miles above the Moon as LRO loops from pole to pole. The system includes two cameras that capture high‑resolution black‑and‑white images and one camera for moderate‑resolution multispectral images. Over the years and thousands of passes, scientists have built maps detailed enough to spot not only new craters, but also landslides, landers, seismic faults, and even hints of lava tubes.

LROC scientists regularly analyze close-up images of small portions of the Moon’s surface taken by the Narrow-Angle Camera. Using these images, they look for changes that are typically less than 30 feet across. But every few years the team searches for large (wider than 150 feet) features by creating global Moon maps and comparing them to older versions.

Square black-and-white image of a dark, uneven surface. At the center is a dark, roughly circular depression surrounded by a bright irregular area, with long streaks of lighter material radiating outward in all directions.
An overhead, close-up view of McGetchin crater that was taken on Dec. 5, 2025, by NASA’s Lunar Reconnaissance Orbiter (LRO) Narrow-Angle Camera (NAC). After the crater was discovered on Oct. 24, 2025, in global images from LRO’s Wide-Angle Camera, which captures broad views with pixels the size of American football fields, scientists turned to the NAC, which takes much sharper views at about 3 feet per pixel. The NAC images, taken as LRO flew over the impact site again, revealed the crater size, shape, and how the surrounding terrain was affected by the impact that carved McGetchin. The image covers an area that’s ΒΎ mile wide.
NASA Goddard/Intuitive Machines
Square black-and-white image of a dark, gently uneven surface scattered with small circular depressions. Near the center is a small oval crater with a bright raised rim and dark interior. Fine, bright streaks radiate outward from the crater across the surrounding surface.
This view from the side (55Β° away from straight down) towards the east, covers an area of the Moon that’s about 1.5 miles wide. It was taken by NASA’s Lunar Reconnaissance Orbiter Narrow-Angle Camera on March 3, 2026.
NASA Goddard/Intuitive Machines

That’s what Wagner was doing on Oct.β€―24,β€―2025, when he came across McGetchin. Using images from LROC’s Wide-Angle Camera, which captures broad views with pixels the size of football fields, he stacked hundreds of β€œbefore” and β€œafter” frames with software designed to highlight change. Anything that stayed the same turned gray while anything different showed up as bright or dark patches.

While the process sounds straightforward, spotting real craters requires a lot of manual work. The software flags every tiny shift in lighting or shadow, generating hundreds of false alarms. For this reason, Wagner typically verifies the software, looking for small fuzzy halos around pixel‑wide bright points, which indicate splashes of regolith around a new crater.

Spanning hundreds of pixels, McGetchin stood out immediately. β€œIt was by far the most obvious impact debris pattern I’ve ever seen in one of these images,” Wagner said.

After his discovery, scientists turned to the Narrow-Angle Camera, which takes much sharper views at about 3 feet per pixel. This camera’s close-up images, taken as LRO flew over the impact site again, revealed the crater size, shape, and how the surrounding terrain was affected. These images also helped researchers estimate the size and force of the rock fragment that formed the new crater, details that are expected to appear in a future paper.

Banner image caption: A zoomed-in view of the Moon, with debris around McGetchin crater visible as a white spot circled by a dark halo just right of center of the image (marked with black arrows). This is the view that Robert Wagner saw on Oct. 24, 2025, during a routine data-quality check. Wagner is an image processing specialist for NASA’s Lunar Reconnaissance Orbiter Camera, a system of three cameras. Using images from the Wide-Angle Camera (WAC), which captures broad views with pixels the size of American football fields, he stacked hundreds of images captured by WAC over the last several years with software designed to highlight change. Anything that stayed the same is gray; anything that changed showed up as bright or dark patches. The stripes in the image are due to slight changes in lighting between the older and newer images. This image composite shows an area of the Moon approximately 900 miles across.

About the Author

Lonnie Shekhtman

Lonnie Shekhtman

Senior Science Writer

Shekhtman helps communicate NASA planetary science to the world through news and feature stories on NASA.gov, videos for NASA+ and YouTube, and by working with the media. She reports on lunar and Mars science and exploration; NASA's search for life; missions to Venus, Titan, and Jupiter's Trojan asteroids; and many other topics related to NASA's exploration of our solar system and beyond.

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Simplified Summary

Scientists discovered a crater on the Moon that formed sometime between April 11 and May 22, 2024, after a comet or asteroid the size of a three- to six-story building hit the surface. Β  The crash left a crater, 728 feet wide, that spans the length of two football fields. And at 141 feet deep, the crater could fit three vertically stacked yellow school buses.

The post NASA’s Moon Orbiter Spots New, β€˜Once-in-Century’ Moon Crater appeared first on NASA Science.

SAVE THE DATE: 2026 Cosmic Origins Early Career Workshop, Oct 2026

16 September 2026 at 18:12

SAVE THE DATE: 2026 Cosmic Origins Early Career Workshop, October 20-22nd

16 September 2026

https://science.nasa.gov/astrophysics/programs/cosmic-origins/community/cosmic-origins-second-early-career-workshop-oct-2026

NASA’s Cosmic Origins Program is excited to invite you to the second Early Career Workshop, designed to support and empower the next generation of astrophysics leaders and PIs. The workshop aims to provide insights to early career scientists about the wide range of work done in the Cosmic Origins Program, to explain and demonstrate the tools and opportunities available to them, and to answer any questions they may have. This year we will have MORE early-career talks and panels to share your thoughts and ideas.

The workshop will take place virtually from October 20 – 22ndΒ 1:00-4:00pm ET. Registration and tentative agenda will be announced soon. Make sure you are subscribedΒ to both email lists to receiveΒ all updates!

Cosmic Pathfinders ProgramSend an email to Cosmic-Pathfinders-join@lists.nasa.govΒ with Subject=”join”
Cosmic Origins (COR) News & AnnouncementsSend an email to COR-News-join@lists.nasa.govΒ with Subject=”join”

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post SAVE THE DATE: 2026 Cosmic Origins Early Career Workshop, Oct 2026 appeared first on NASA Science.

REMINDER: 2027A NASA IRTF Call for Proposals

16 September 2026 at 18:11

REMINDER: 2027A NASA IRTF Call for Proposals | Due October 1st

16 September 2026

Solicitation Number: NN2027AOBSERV_IRTFΒ 

Proposals Due: 10/01/2026

Announcement Document:Β Call for Proposals

Other Documents:Β IRTF Home Page

The call for NASA Infrared Telescope Facility observing proposals for semester 2027A (February 1 to July 31, 2027) opened on September 1. The proposal Deadline is Thursday, October 1, 2026, 5PM Hawaii Standard Time. Available instruments are listed here. Remote observing is offered from any location with broadband Internet access for any project that utilizes IRTF facility instruments. Click hereΒ for information about IRTF Computer and Remote Observing Information. Please see the announcement for available instruments and for further information. Please review the information and use our Online Application Form. Β 

Questions may be directed to Warren Skidmore at warren.skidmore@hawaii.edu

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post REMINDER: 2027A NASA IRTF Call for Proposals appeared first on NASA Science.

Episode 182: Human Factors: Designing Systems with People in Mind – Part 1 of 2

16 September 2026 at 13:33

Cynthia Null: The knowledge of how human cognition systems work and how they’re evolved has led to a lot of misconceptions and oversimplifications in human performance. And miscalibration of how humans contribute to the system and system performance can be problematic. And so, it’s important that you actually understand how humans do what they do, so you can actually support their work.Β 

Host Andres Almeida: That’s Dr. Cynthia Null, talking about a scientific discipline important to mission success. It’s called human factors, and it’s about how people interact with the systems they design, build, and operate. As the NASA Technical Fellow for Human Factors, Dr. Null provides technical leadership and expertise on how human capabilities and performance are considered across the agency. Let’s dive in on this episode of Small Steps, Giant Leaps.Β 

[Intro music]Β 

Welcome to Small Steps, Giant Leaps, the podcast from NASA’s Academy of Program/Project & Engineering Leadership, or APPEL. I’m your host, Andres Almeida. I’m talking with Dr. Cynthia Null, who’s joining us from NASA’s Ames Research Center in Silicon Valley.Β 

Hi, Cynthia, thanks for joining us.Β 

Cynthia Null: Well, great to be here.

Host: Can you tell us a bit more about your role and what you do at NASA?Β 

Null: Yes, I’m the technical fellow for human factors at the NASA Engineering and Safety Center. The NASA Engineering and Safety Center was formed after the Columbia accident to create a ready team that’s independent of programs and projects and has deep expertise.Β 

And what we deliver is robust understanding of risk and possible risk mitigations for mission safety and success for any project or program mission across all of NASA.Β 

There are 21 different disciplines that have a Technical Fellow. And my job as a Technical Fellow, is to have insight into how human factors is used or not used across all missions, not just human spaceflight, but aeronautics, science missions, technology developments, whatever.Β 

Now, we don’t get involved in everything because we, we’re a limited size group, and we’re in workplaces where we can influence risk and mission success. So, part of my job is just general insight.Β 

Because what comes to the NESC are questions or issues or concerns that approach might be wrong, if a question comes in that might have human factors needs, then I would find someone with the right expertise to be on that team.Β 

Sometimes, the questions are just generally human factors questions at which point I would lead the team, but sometimes it’s a, it’s a software development project. But there’s [a] piece of it that human factors would have some influence in.Β 

Or, for example, we’ve looked at parachutes, and part of the problems with parachutes are actually just making them, not just designing them. And so, the making them, of course, is all done by hand. And so, we might do a human factors investigation of the processes and procedures, and those kind of things related to manufacturing, for example.Β 

Host: You’re talking about parachutes for spacecraft landing on other worlds, yeah?Β 

Null: Yes, spacecraft. Well, or landing back here. Orion comes down on a spacecraft. Dragon comes down on a chute. Or, yeah, it could be chutes for Mars or some other place we’ve landed, and so you want those things to work. They usually have some sort of redundancy, but not always.Β 

It’s really critical that you have all aspects of it, so you can go through all your materials and sizing and all that other kind of stuff, but if there’s a problem with manufacturing, then that could be change your risk posture. Then it wouldn’t come up in your analysis, but it could come up in flight. So, that would be a place where we could help.Β 

And we might just decide that actually it’s a brilliant process, and they’re doing everything they can to control it, or we might have recommendations.Β 

Host: Can you give a straightforward explanation of what human factors entails?Β 

Null: I’ll try!Β 

[Laughter]Β 

So, to start with, human factors is a scientific discipline. It’s based on the understanding of human capability as well as the interactions amidst humans and all other elements of the system and mission.Β 

So, work our discipline is based on actually started with the understanding of human sensory systems and the development of quantitative methods to describe them.Β 

This work was actually done by some very famous physicists in the 19th century, people you’ve probably heard of or studied. Hermann von Holtz [and] Ernst Mach are two of those people who actually not only did amazing discoveries related to physics, but also developed methodologies to understand eyes, ears. They discovered the vestibular system, which helps with balance. Those techniques that they developed to do quantitative descriptions are still used today, and they’ve been modified to deal with perception, not just sensation, and also how we think.Β 

So, human factors enhances mission safety, efficiency, success, and all those kind of things by developing requirements, tools, processes, and procedures to make the humans in the system successful.Β 

The knowledge of how human cognition systems work and how they’re evolved has led to a lot of misconceptions and oversimplifications in human performance. And miscalibration of how humans contribute to the system and system performance can be problematic. And so, it’s important that you actually understand how humans do what they do, so you can actually support their work.Β 

Host: Is it important for human factors to be considered early in mission development? Is that something that you feel strongly about?Β 

Null: Very strongly. So, the thing is, when you’re, when you’re conceiving a mission, you’re also conceiving what humans will do and what they won’t do. And so, you can early on decide that you’re going to have a fully autonomous mission, and you can, and you can design it without the considering having human crew. And whether it’s crew on the ground or crew in space, that’s a decision you can make.Β 

But when you then can’t actually make everything work without real-time human decision-making, then you sort of have to step back and start all over again to figure out what their roles are really going to be.Β 

So, defining the human role and understanding what that role is and what you need to support that role is really critical.Β 

Host: Was human factors, as a discipline, shaped by lessons learned?Β 

Null: Well, yeah, it might look like that, but people were doing human factors and doing proactive human factors starting as early as World War II.Β 

So, one of the big problems in World War II, and it may have been problems before that, but I guess probably with communication systems and all these other kind of things, maybe it was less apparent. But a big problem for, for in World War II was just keeping planes in the air, keeping them and repairing them when they came back, and so maintenance became a huge issue.Β 

And one of the problems with maintenance can be: Have you actually designed for maintainability? So, if you can’t access the part of the engine you need to repair, then you have to actually take the engine off. If you have to take the engine off, okay, that plane is going to be in the repair area much longer than if you can repair it in place. And so, access becomes a very, very important thing.Β 

So, in the very, just after World War II, the field of human factors hadn’t been named yet, but people who had been involved in solving problems in World War II for the military came from major universities on the East Coast: Harvard, Penn, probably Yale, a few others, and those people were then contracted to the government to develop guidance on how to do designs for future mission systems. And right in those design books, right in the lectures about those designs, they started with, β€œWe need to design for the mission from the beginning.”

So, the first book that was a guidance book on how to write human factors, the first chapter is called β€œThe System.” The first bullet, it just says you have you, all of our contractors as well as the – this is written this, is written in the early β€˜50s – all of our contractors, as well as all of our in-house designers, believe that you have to do designs starting at the system level.Β 

So, the notion of systems engineering is written, is the first paragraph in this human factors book. And paragraph 1.1 is entitled β€œThe Human in the System” and how you have to work on designing for all the roles the human is going to have in the system, which could be engineer, like design engineer. It could be manufacturing. It could be maintenance. It could be operations. It could be the crew member, right? It could be anyone, right?

And all of those people are valuable assets to the mission, and they all need to be counted for. And you have to make sure that they have the information they need, the tools that they need, and that they have everything else that they need, like access, for example. And so, all of those things were actually talked about from the beginning in human factors.

Now, that doesn’t necessarily mean that’s the role we had in every system design once we said that’s what we needed. But it has been the mantra of human factors from the beginning that you actually had to think about the design, and that when we weren’t patching stuff that people forgot about that we were actually actively working on design.Β 

And in the early ’50s, people were asking questions, all sorts of questions at all sorts of different levels about how you should do human factors. So, one of the simple, simple questions is, if you need somebody to respond to something really quickly, like hit the off button, or hit the escape button, or something like that. And the question was, how big does the button have to be so you can find it and hit it quickly?Β 

And what they decided was that there was a tradeoff between speed and accuracy, and there was also a tradeoff between size and distance. So, if the button was far away, it had to be much bigger because you’re just sort of trying to hit it with your hand. And so, if it’s small, then you can’t get to it.Β 

Β Β 

And so, there’s actually a law called Fitts’s Law, named after a military human factors person from the, this is early β€˜50s, where he actually described an equation: If the button’s close, like on your armrest, then it doesn’t have to be very big. But if it’s going to be out in front of you on the on the front displays on say an airplane or wherever, then it has to be big enough that you can just jam your hand in some direction and you won’t miss it.Β 

Now, we also said, β€œBut if you don’t put a cover on it, they could accidentally bump into it.” And so, the other thing we said is, β€œImportant things like aborts should have a cover on them so you don’t elbow into them accidentally because you don’t really want to do that unless it’s intended.” So, what you have to be going for if it’s far away, [it] has to be big, but it also has to be protected from just being bumped into accidentally.Β Β 

Host: You just made me think of an everyday example. I go to a gym where there’s a treadmill that has an emergency stop button in the center. And I’m moving my arms and I frequently hit it. It’s a large red button. I frequently hit it and I stop.Β 

Null: Exactly. So, what we would do in safety critical systems is we would put a cover on that. Or we might have, you know, you have to hit it twice, or you have to do something so that it takes two actions instead of one.Β 

But yes, I’ve been on those treadmills, and I do realize that it, yeah, it’s easy to hit them off. But it’s also good to have that there because if you are actually falling, you really do want that off instead of being thrown to the back.Β 

[Laughter]Β 

And usually in a gym, those treadmills, the rows between them are not that far. You could hit your head on the one behind you if you’re not careful. So, it’s good that it’s there, but you’re right. If it’s too easy to hit, that’s a problem. And so, those are actually how human factors thinks about everything, okay? And so, so that’s the, that’s sort of the problem.Β 

But people then say, β€œOh, I can think like a human factors person. I’m a human.” So, there are lots of misconceptions about how humans actually work.Β 

Host: I bet there are. What are some?

Null: Well, so, one of them is that humans are maybe sort of bad at sort of probability or understanding risk or making decisions that are involved like that.Β 

And so, a long time ago, people interested in this topic actually did some research, and their subjects were either novices or actually experts in the field, and one of the studies was done with medical decision-making.Β 

And they gave a scenario, and half of the people got a scenario that was about a particular treatment for a disease, and it described this treatment, and then it said the survival rate was 90 percent.Β 

For another treatment, they described this treatment (entirely different treatment) and they described it in terms of its mortality rate, as opposed to its survival rate. And they said its mortality rate was 10 percent. And so, they asked both novices and doctors, β€œWould you prefer treatment A or treatment B?” Now, notice that 90% survival and 10% mortality are actually the same risk.Β Β 

Host: Right.

Null: But almost everyone picked the survival, and this was seen as being emotional, sort of, tagging, right? That you were having emotional response instead of a perceptual response.Β Β 

So, some people who actually know a little bit more about how the brain works decided to redo the experiment, and the only thing they changed was how they represented the survival rate and the mortality rate. And in the new experiment, they said that nine out of 10 people would survive in the first, and one out of 10 people would die in the second.Β 

And the bias towards survive, the survival metric went away, so that it wasn’t actually in the main,Β the emotional tagging. It was actually that humans are actually better at frequency than probability. So, let’s just think about this.Β 

I have a favorite meal that I like to have on Sundays at my house, and it’s fresh fish. And you don’t want to buy that several days in advance. And so, when I’m running errands on Sunday, I try to drive by a grocery store or a place where I’ve been before that I think the fish might be good, and buy some fish on my way home. So, it’s been, it’s been properly chilled until I get it to my kitchen and then I can cook it.Β Β 

So, over time, I’ve noticed that there are stores when I go into I often don’t have fish, so maybe once I’ve gotten fish there, and another place I’ve gotten fish, like, five or six times in a row. It appears that people think that way, as opposed to saying, β€œOh, the probability I get fish from this market is…” and so that since we live our lives more like on frequency basis and not on, on collecting all the data and running a probability theory, it might be more natural for us to understand things presented in the way that we run our lives (in frequency, as opposed to changing into probability).Β 

Now, that doesn’t mean you can’t get people to be sophisticated about both the same representation of the facts. But if you’re just asking for a quick response or you’re doing a quick analysis, it may be actually better to present data as frequency data than as probabilistic data because that’s sort of a capability we have that we’ve had probably since the Serengeti.Β 

[Laughter]Β 

Because knowing where predators were or food was (one to avoid and one to find) would have been very, very important, and you probably weren’t thinking of it as a risk probability, but more of an experience that would be that way. And so, I think that gives you a little bit of an example of how it’s completely counterintuitive to expect that someone would interpret 90% and nine out of 10 as different, right?Β 

But actually, it takes less training to get people to do it without with, with having it as a frequency than it would be having it as a probability. And so, if you’re trying to have safe, reliable, quick, resilient performance, then it’s important to match human capability. And we always don’t understand what our capability is.Β 

Host: Right.

That’s the end of part 1 of our interview with Cynthia Null, NASA Technical Fellow for Human Factors. Stay tuned for part 2 of where Cynthia will detail more of the myths and misconceptions of how the human brain works.

For a transcript and to hear all other episodes, visit nasa.gov/podcasts. While you’re there, check out our other podcasts like Houston, We Have a Podcast, Curious Universe, and Universo curioso de la NASA. As always, thanks for listening.

Outro: Three. Two. One. This is an official NASA podcast.

The post Episode 182: Human Factors: Designing Systems with People in Mind – Part 1 of 2 appeared first on NASA Science.

APOD: 2026 September 16 – Webb’s View of M64

16 September 2026 at 05:05

APOD

Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

Hubble and JWST image of M64. A massive spiral galaxy glows with a yellow core, surrounded by arms full of orange-brown dust and pink and blue patches of star formation. Framed by a haze of dark dust, the galaxy shines against black space dotted with a few stars.Hubble image of M64. A massive spiral galaxy glows with a yellow core, surrounded by arms full of dark dust and pink and blue patches of star formation. Framed by a haze of dark dust, the galaxy shines against black space dotted with a few stars.

Webb's View of M64

Explanation: Sometimes where Hubble finds darkness, Webb sees light. An example is today’s composite images of Messier 64 (M64), a nearby spiral galaxy of many names. The dark band of dust partially blocking its bright core earned it the moniker β€œthe Black Eye Galaxy.” Webb’s Mid-InfraRed Instrument (MIRI) sees that dust, shown in red, as it absorbs and re-emits light from surrounding newborn stars. These young stars are embedded in pink star-forming regions in the Hubble-only image. M64’s inner and outer gas regions counter-rotate, creating regions of increased star formation where the two gas β€œcurrents” meet and compress. A merger between M64 and a smaller galaxy was likely the cause of the opposing motion of the outer gas. Spiral galaxies were once thought to have peaceful histories. M64 was key evidence that spiral galaxies, including the Milky Way, can and do experience mergers. Webb’s view of M64 will tell astronomers about the structure, motion, and composition of the galaxy’s dust and add context to the galaxy’s merger history and evolution.

APOD’s main NASA site is moving: From apod.nasa.gov to science.nasa.gov/apod
Tomorrow’s picture: treasure

Date: September 16, 2026
Credit: NASA, CSA, ESA, F. Belfiore (ESO), J. Lee (STScI), A. Leroy (OSU), and D. Thilker (JHU); Processing: G. Kober (NASA/Catholic University)
Authors & editors: Keighley Rockcliffe, Robert Nemiroff, Jerry Bonnell, Cecilia Chirenti
A service of: ASD at NASA / GSFC,
NASA Science Activation & Michigan Tech. U.

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Purple Haze Aurora

16 September 2026 at 05:01
Green and purple aurora and white airglow arc above Earth’s limb and the scattered city lights of Central Asia in a nighttime photo taken from the International Space Station.

One of the inspirations for Jimi Hendrix’s iconic 1967 hit β€œPurple Haze” is said to be the sci-fi novel Night of Light, about a distant planet in a binary star system. Every seven years, the story goes, the stars bathe the planet in a bizarre purple radiance with the power to rearrange physical reality in profound and unexpected ways. The atmosphere’s purple glow, for instance, turned some people into trees and brought statues to life.

It’s perhaps fitting, then, for an astronaut on the International Space Station to invoke the iconic song after witnessing the aurora illuminate Earth’s atmosphere with ethereal greens, reds, and purples. Hendrix would have β€œrejoiced” at the β€œbrilliant purple,” NASA astronaut Jessica Meir posted on September 8. It β€œmakes me want to kiss the sky,” she added in a nod to the lyrics of the Hendrix song.

The photograph above is one of many that the astronauts took on September 7, 2026, as they orbited an atmosphere quivering with color. The station was at an altitude of 255 miles (411 kilometers) and above Kyrgyzstan when the photo was taken. Stacking several of the photos also yielded a long-exposure series in which the aurora’s green glow mingles with star trails, moonlight, passing satellites, and city lights in a dazzling jumble of illumination.

Aurora is the Latin word for β€œdawn” and also the name of the Roman goddess of the dawn. Its use in reference to the atmospheric phenomenon likely comes from Europeans living far from the Arctic Circle, who would have experienced the aurora as a faint red glow to the north, resembling the reddish glow in the east at dawn.

The colorful phenomenon typically starts when the Sun sends charged particles toward Earth through solar flares, coronal mass ejections (CMEs), or an active solar wind. These particles interact with the magnetosphereβ€”the invisible, comet-shaped bubble of magnetic field lines surrounding the planetβ€”compressing and changing the configuration of the magnetic field. In the process, some particles within the field are drawn into Earth’s upper atmosphere, where they excite nitrogen and oxygen atoms and molecules, causing them to release photons.

The aurora Meir photographed occurred amid a disturbance associated with a high-speed stream of solar wind from a coronal hole and the lingering effects of multiple coronal mass ejections, according to updates from NOAA’s Space Weather Prediction Center. These solar wind disturbances interacted with Earth’s magnetosphere, causing minor (G1) geomagnetic storms.

The colors of auroras are influenced by the type of gas involved and the altitude at which they occur in the atmosphere. Oxygen excited to different energy levels can produce green and red. Green occurs roughly between 60 and 120 miles (100 and 200 kilometers) altitude, and red occurs above 120 miles (200 kilometers). Excited nitrogen gas, from about 60 to 120 miles (100 to 200 kilometers), glows blue or pink depending on the type and energy of the particles it interacts with. Sometimes, the light emitted by gases can appear to mix, making the auroras seem purple, pink, or even white.

While auroras can occur any time of the year, astronauts are especially likely to enjoy the light shows in the spring and fall, around the equinoxes. That’s because the geometry of Earth’s magnetic field relative to the solar wind makes it especially favorable for transferring solar-wind energy into the magnetosphere, a phenomenon known as the Russell-McPherron effect.

This isn’t the only example of Jimi Hendrix’s music making an impression beyond Earth. A selection of Hendrix’s music touched down on the Moon in 2024 with the Odysseus lander. Another Hendrix song, β€œVoodoo Chile,” made the list of wake-up songs for STS-110, according to a report from NASA’s History Division.

Astronaut photograph ISS075-E-88592Β was acquired on September 7, 2026, with a Nikon Z9 digital camera using a focal length of 15 millimeters. It is provided by the ISS Crew Earth Observations Facility and the Earth Science and Remote Sensing Unit at NASA Johnson Space Center. The image was taken by a member of theΒ Expedition 75 crew. The image has been cropped and enhanced to improve contrast, and lens artifacts have been removed. TheΒ International Space Station ProgramΒ supports the laboratory as part of theΒ ISS National LabΒ to help astronauts take pictures of Earth that will be of the greatest value to scientists and the public, and to make those images freely available on the internet. Additional images taken by astronauts and cosmonauts can be viewed at the NASA/JSCΒ Gateway to Astronaut Photography of Earth. Story by Adam Voiland.

Downloads

Green and purple aurora and white airglow arc above Earth’s limb and the scattered city lights of Central Asia in a nighttime photo taken from the International Space Station.

September 7, 2026

JPEG (6.20 MB)

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The post Purple Haze Aurora appeared first on NASA Science.

NASA Ames Stars of the Month: September 2026

16 September 2026 at 00:46
NASA Ames science stars of the month for September 20206. Pictured left to right is Steve Ormsby, Aphrodite Kostakis, Alejando Borlaff, Sarah Nickerson, Martina Caussi, Keiko Nomura, and Stephen Broccardo.

The NASA Ames Science Directorate recognizes the outstanding contributions of (pictured left to right) Steve Ormsby, Aphrodite Kostakis, Alejando Borlaff, Sarah Nickerson, Martina Caussi, Keiko Nomura, and Stephen Broccardo. Their commitment to the NASA mission represents the entrepreneurial spirit, technical expertise, and collaborative disposition needed to explore this world and beyond.

A portrait shot of Steve Ormsby in front of a NASA flag.

Space Biosciences Star: Steve OrmsbyΒ 

Steve Ormsby is a project engineer for the Space Biosciences Division with Amentum in the Center Operations Directorate. He is recognized for his perseverance, dedication and initiative in overseeing the safety of division facilities and infrastructure maintenance, as well as exceptional diligence as a property custodian.

Portrait photo of Aphrodite Kostakis

Space Biosciences Star: Aphrodite Kostakis

Aphrodite Kostakis is the Facility Service Manager with Amentum for building N239 in the Space Biosciences Division. She is acknowledged for her exemplary work ethic in maintaining building safety, preparing for and leading VPP inspections with diligence and attention, and suggesting infrastructure improvements and ensuring they get implemented for everyone’s benefit.Β 

lejandro Serrano Borlaff speaks to media during the Artemis II splashdown event at Chabot Space & Science Center in Oakland, California.

Astrophysics Star: Alejandro Borlaff

Alejandro (Alex) Borlaff, a research scientist in the Astrophysics Division with the Bay Area Environmental Research Institute, is recognized for his leadership in pioneering and developing image reduction pipelines for the Hubble Space Telescope (HST) and the Roman Space Telescope’s Wide Field Instrument (WFI). These algorithms significantly advance the detection of ultra-low surface brightness features through rigorous modeling of background contamination, including scattered and zodiacal light, better maximizing the science derived from NASA flagship astrophysics missions.Β 

Portrait photo of Sarah Nickerson

Astrophysics Star: Sarah Nickerson

Sarah Nickerson, a research scientist in the Astrophysics Division with the Bay Area Environmental Research Institute, is recognized for exceptional work on the analysis and curation of data taken from the EXES instrument on NASA’s Stratospheric Observatory for Infrared Astronomy (SOFIA) observatory. This provides high-level data productsΒ  to the global astrophysics community for continued discovery and synergy with other NASA missions.

Portrait photo of Martina Caussi

Planetary Science and Exobiology Star: Martina Caussi

Martina Caussi is a NASA Postdoctoralβ€―Program Fellow in the Planetary Science and Exobiology Division. Martina is recognized for her outstanding work using finite element simulations to determine that topographic relaxation has played a significant role in shaping Tegid, an unusually shaped impact crater on Europa. This work represents valuable precursory science in anticipation of the Europa Clipper mission, which willβ€―refine our understanding of this ocean world.

Portrait of Keiko Nomura in a black shirt.

Earth Science Star: Keiko Nomura

Keiko Nomura is a research scientist for the NASA Earth Exchange (NEX) in the Earth Science Division with the Bay Area Environmental Research Institute. She is acknowledged for timely efforts in leadership, stakeholder engagement, coordination with NASA HQ management, and team building for the recently funded NEX-GeoAI project. This project is now being recognized as a key step forward to establishing NASA as the ground-truthing agency for federal and private sector GeoAI modeling activities for decision making.

Earth Science Star: Stephen Broccardo

Stephen Broccardo is a research scientist in the Earth Science Division with the Bay Area Environmental Research Institute. He is recognized for exceptional initiative and technical leadership in sustaining and advancing Ames’ atmospheric remote-sensing capabilities. Stephen has maintained critical observational capabilitiesΒ  and developed thoughtful technical milestones for future satellite-validation and science activities.

The post NASA Ames Stars of the Month: September 2026 appeared first on NASA Science.

NASA’s New X-59 Test Pilot Gets Behind Controls for Ground Test

16 September 2026 at 00:37
A man seated inside an aircraft cockpit adjusts a helmet, with the open canopy above him.
Mike Lippert, one of NASA’s X‑59 test pilots, sits in the cockpit of the agency’s X‑59 quiet supersonic research aircraft for the first time during an engine run at NASA’s Armstrong Flight Research Center in Edwards, California, on Thursday, Aug. 27, 2026. Lippert is the third X‑59 pilot supporting NASA’s Quesst mission, which will demonstrate quiet supersonic flight over U.S. communities and gather public feedback on the aircraft’s quieter sonic β€œthump.”
NASA/Carla Escamilla

This summer, NASA test pilotΒ Mike LippertΒ powered up theΒ X‑59Β cockpitΒ forΒ theΒ first time,Β running the aircraft’s engines on the groundΒ during a key step in hisΒ months of preparation and training to fly the experimentalΒ aircraft.Β 

β€œGetting into the cockpit of the X‑59 felt very comfortable,” saidΒ Lippert, the newest X-59 test pilot for NASA’sΒ QuesstΒ mission.Β β€œThe whole team has done a tremendous job of making sure I am trained and prepared.”

Lippert’sΒ first powered interaction with theΒ aircraftΒ demonstratedΒ howΒ mentorshipΒ worksΒ in NASA’s testΒ pilotΒ community.Β TheΒ X‑59’s two establishedΒ pilots,Β Nils Larson and Jim β€œClue” Less,Β guided him throughoutΒ theΒ test.Β LarsonΒ monitoredΒ Lippert’s coordination with the control room, whileΒ LessΒ answeredΒ questions and provided coaching.Β 

Their feedback,Β alongΒ with insights fromΒ experiencedΒ engineers,Β turnedΒ the startup sequence into aΒ detailedΒ trainingΒ exerciseΒ toΒ strengthenΒ Lippert’s understanding of the X‑59’s systems and theΒ pace of test operations.Β 

The X-59 is a revolutionary design, shaped to create a quiet thumpΒ instead of a sonic boom when flying faster than the speed of sound. TheΒ test pilots’ experience andΒ skill will allow NASA to safely test theΒ aircraft, then eventually fly it over U.S. communitiesΒ to gather data on how the public perceives theΒ sounds it makes.Β 

TheΒ engine run alsoΒ introducedΒ LippertΒ toΒ the X‑59’s maintenance crew.Β As theΒ test progressed, LippertΒ sawΒ howΒ theΒ cockpit and control roomΒ work togetherΒ during critical operations.Β Watching theΒ real-timeΒ rhythm, he said,Β providedΒ a betterΒ understandingΒ ofΒ how NASA’s flight testΒ teamsΒ align to ensure safety and precision.Β 

LippertΒ credited theΒ test team’s operating practicesΒ andΒ leadershipΒ forΒ helping him prepare for flight.Β HeΒ spent extensive timeΒ inΒ the X-59’s high-fidelityΒ simulatorΒ β€”Β designed to match the aircraft’s cockpitΒ β€”Β forΒ training,Β aircraftΒ familiarization, and mission rehearsal.Β TheΒ simulation team’sΒ members are absolute experts on theΒ aircraftΒ and have been key contributors toΒ hisΒ training and theΒ program as a whole, LippertΒ said.Β 

Lippert said he felt energized after powering on the aircraft’s systems for the first time, adding the milestone left him feeling ready for upcoming test flights. The X-59 will continue to progress through envelope expansion and test its performance under various flight conditions. In the coming months, it will advance toward acoustic validation flight tests to study the sonic thumps it is designed to make.

Learn more about theΒ QuesstΒ mission on NASA’s site.Β Β 

The post NASA’s New X-59 Test Pilot Gets Behind Controls for Ground Test appeared first on NASA Science.

NASA Field-Tests AI Fleet Capability for Science, Exploration

15 September 2026 at 21:43

NASA scientists and industry partners recently field-tested an artificial intelligence application that could make future solar system exploration missions more efficient, return more science data, and allow for faster scientific discoveries.

Team photo of twelve people standing on a road with trees behind them. In the foreground are four robots: two rovers and two drones.
Members of the ASTRA (Adaptive Sensing Technology for Responsive Autonomy) team with the fleet of robots they field-tested in July 2026. Left to right: Stephen Scarano, Karl Wunderlich, Zach Logan, Mohammad Goli, and James O’Hara of Noblis; James Marshall, Connor Firth, Leyton McKinney, Connor Williams, Steven Hard, Bethany Theiling, and Michael Monaghan of NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
Noblis/Sean Sullivan

This summer at the Virginia Tech Transportation Institute in Blacksburg, Virginia, a fleet of three robots worked together, and researchers assessed the fleet’s ability to act like an independent science team. To begin each test, a drone was assigned to choose an area of interest based on initial science goals provided by human experts. Then, the fleet’s programming weighed risks against potential science payoffs and calculated which robotic team member was best suited to investigate. As the fleet carried out its plan, it continually checked for environmental hazards, reassessed its strategy to adapt to new information, and reported back to its human managers, NASA’s Adaptive Sensing Technology for Responsive Autonomy (ASTRA) team.

Three robotic explorers in a grassy field: a drone parked between two rovers. The larger rover has a multi-jointed arm extending from it.
The ASTRA + Noblis fleet. The drone (center) uses environmental and scientific sensors to scout the area, identify places of interest, and collect data from overhead. The rover on the left uses lidar to map its surroundings in detail, help the fleet navigate obstacles, and gather context for scientific samples. The rover on the right uses a robotic arm to collect samples.
NASA/Bethany Theiling

The project’s ultimate goal is to provide a trustworthy extension of the human science team in situations where humans are too far away to give real-time instructions, like on uncrewed missions to the outer planets of our solar system, or where the risk to human explorers is unacceptably high, like in areas of the Moon and Mars that are difficult for astronauts to explore.

One of the questions the field test was designed to answer: Once the fleet has started working on a science objective, will it change tasks autonomously based on new information? In the testing, the fleet showed it could focus on its original objectives and follow up on new possibilities. When the lead drone found an additional area of interest in the course of its work, it didn’t abandon its current task, but it did pause to process the opportunity and pull in another robotic asset to investigate the new question.

A small robot on the move across pavement. In the background, people observe its progress and work on another robot.
Mohammad Goli, Zach Logan, and James O’Hara test communications on the sampling rover as Karl Wunderlich observes rover actions during a July 2026 field test in Blacksburg, Virginia. Noblis provided the robotic fleet’s ground capability (two rovers shown here).
Noblis/Sean Sullivan

Crucially, the fleet’s decision-making programs handled both objective and subjective information. What robotic assets are available? How far away are they, and how fast can each one move? How much does the science team want the knowledge that can be gained by mapping this area or by taking a sample of that material? Would the humans want to learn from a newly spotted point of interest more than they’d want the fleet to focus on its original task? How risky is each job for the robot attempting it, and is the danger acceptable to the mission planners?

β€œWe want to find a way for missions to do things that they could never do before because they didn’t have a decision-maker on board that can weigh all these criteria at the same time,” says Bethany Theiling, ASTRA principal investigator and field lead, of NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

This ability to consider subjective criteria alongside simple facts, then deliver decisions that satisfy the people behind the project, is what the ASTRA team is working to develop. The mission team will consider the robotic fleet to be successful if it can correctly act without direct instructions based on its physical capabilities and on the team’s priorities and risk assessments.

Theiling led the testing campaign in collaboration with Noblis, Aurora Engineering, and the University of Tulsa.

Similar Landscapes, Different Worlds

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A researcher in a clean suit kneels in the desert, collecting samples.
NASA scientist Mary Beth Wilhelm collects soil samples from Chile’s Atacama Desert. Studying ancient life in the driest places on Earth helps us to understand conditions on Mars.
NASA

The post NASA Field-Tests AI Fleet Capability for Science, Exploration appeared first on NASA Science.

AI/ML STIG Lecture Series, 21 Sept 2026

15 September 2026 at 21:20

AI/ML STIG Lecture Series

Artificial Intelligence & Machine Learning Science and Technology Interest Group

AI/ML STIG about AI/ML STIG Lecture Series

Location

Virtual

dates

21 September 2026
4:00pm ET

Community

AI/ML STIG

Type

Lecture

Hands-On Session I: Agentic Coding and Research Tools

Speaker

Christopher Stubbs, Harvard University

Meeting Connection

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post AI/ML STIG Lecture Series, 21 Sept 2026 appeared first on NASA Science.

Cosmic Origins Community Meeting, 22 Sept 2026

15 September 2026 at 21:20

Cosmic Origins Community Meeting

Location

Virtual

Dates

22 September 2026
12:00pm – 1:00pm ET

Community

Cosmic Origins

Type

Meeting

Post-Ad ASTRA Community Science Workshop Update

Hosted by the COPAG Leadership

This community meeting aims to provide you with an overview and explanation of the processes and plans for mission concepts submitted to the Ad ASTRA workshop. The meeting will include a description of how the NASA Astrophysics Division will use the information gathered at the workshop. Additionally, this meeting aims to collect feedback and questions that the COPAG community may have regarding the process and plans that further mission concept selections.Β 

Please use this form to submit any comments, questions, or feedback for the COPAG community meeting: https://forms.gle/puBBTk1mo34WiGwP7Β 

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post Cosmic Origins Community Meeting, 22 Sept 2026 appeared first on NASA Science.

AGN SIG Spotlight Series, 22 Sept 2026

15 September 2026 at 21:20

AGN SIG Spotlight Series

Active Galactic Nuclei Science Interest Group

Our Spotlight Series highlights recent advances in AGN science, with a strong emphasis on participation from early-career researchers, and includes plenty of time for community discussion following the presentations.Β 

AGN SIG about AGN SIG Spotlight Series

Location

Virtual

Dates

22 September 2026
1:00pm ET / 10:00am PT

Community

AGN SIG

Type

Seminar

Unveiling the Role of Multi-Phase AGN Outflows with MIRACLE

Speaker

Dr. Matteo Ceci (UniversitΓ  di Firenze)

Abstract

Galaxy evolution is tightly connected to Active Galactic Nuclei (AGN) through feedback processes in which gas accretion onto the supermassive black hole drives powerful multiphase outflows. Detailed studies in the local Universe are crucial to resolve the physical scales and gas phases involved, enabling a comprehensive view of AGN-host interactions. I will present first results from the MIRACLE (Mid-IR Activity of Circumnuclear Line Emission) program, combining JWST/MIRI, MUSE, and ALMA observations of seven nearby Seyfert galaxies. Thanks to JWST’s spatial resolution (50-150 pc), we probe atomic and molecular gas in the circumnuclear regions and assess the impact of AGN activity on their host galaxies. Focusing on NGC 1365, we trace the ionized outflow up to kiloparsec scales and constrain its energetics and effects on star formation (SF). By combining mid-IR diagnostics with advanced photoionization and kinematic models, we reproduce ~60 optical and mid-IR emission lines, disentangling AGN- and SF-driven components and providing robust estimates of gas density, ionization, extinction, and outflow mass. We show that classical methods commonly adopted in the literature can underestimate outflow masses by up to an order of magnitude.

Disk Reflection as the Origin of the X-ray Polarization of NGC 4151 with IXPE

Speaker

Dr. Elias Kammoun (California Institute of Technology)Β 

Abstract

The geometry of the X-ray emitting region around accreting supermassive black holes remains poorly constrained, but X-ray polarimetry now offers a new and direct perspective on it. I will present a spectro-polarimetric study of the nearby type-1 AGN NGC 4151, combining two long IXPE observations from 2022 and 2024 with simultaneous XMM-Newton and NuSTAR spectroscopy. IXPE reveals a polarization degree of 6–7% above 4 keV aligned with the radio jet, plus a distinct low-energy component at a different angle, providing evidence for at least two polarized components in the 2–8 keV band. While earlier work read the hard X-ray signal as a radially extended, slab-like corona, I will test an alternative: that the polarization is instead dominated by relativistic reflection from an accretion disk illuminated by a compact, lamp-post corona. Fitting the IXPE Stokes spectra with recently developed models, we find the data favor a low coronal height and a wide torus opening angle, with disk reflection supplying ~20% of the 2–8 keV flux. The same configuration reproduces the full 0.4–79 keV spectrum, showing that disk reprocessing by a compact corona can account for both the polarization and the broadband spectral properties of NGC 4151.

Seminar Connection

Zoom Registration, you will receive connection details by email after registration:Β 

https://alaska.zoom.us/meeting/register/V1okit8uSk2ql97gegbdzg

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post AGN SIG Spotlight Series, 22 Sept 2026 appeared first on NASA Science.

DGCE SIG Seminar, 24 Sept 2026

15 September 2026 at 21:20

DGCE SIG Seminar

Diffuse Gas in Cosmic Ecosystems Science Interest Group

DGCE SIG about DGCE SIG Seminar

Location

Virtual

Dates

24 September 2026
4:00pm ET / 1:00pm PT

Community

DGCE SIG

Type

Seminar

How the Faint Radio Sky is Changing Our Understanding of Star Formation and Galactic Outflows

Speaker

Allison Matthews (Carnegie Observatories)

Abstract

In the last decade, with the commissioning of high sensitivity radio telescopes, we have opened a new window into the faint radio sky. These novel facilities probe fundamental physical processes that regulate star formation and characterize star formation in normal galaxies like our Milky Way over nearly all cosmic time. Deep observations from MeerKAT and LOFAR have revealed that prior observations may have missed half the star formation at all cosmic times. This discrepancy has critical implications across astrophysics: estimates of gravitational wave events, the frequency of astrophysical transients, and the chemical evolution of galaxies. These same high-sensitivity radio facilities are simultaneously placing critical constraints on the physical drivers of galactic winds that we believe regulate star formation across all of cosmic time. In this talk, I will present these findings and outline programs with next generation radio facilities that will improve our observational constraints on the rate and regulation of star formation across cosmic time.

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post DGCE SIG Seminar, 24 Sept 2026 appeared first on NASA Science.

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