Wednesday, 24 June 2026

Playing the Moon Game 

A satellite image shows part of Alaska’s Katmai National Park. A chain of snowy mountain peaks stretches from the bottom left corner to the right side of the image. The Valley of Ten Thousand Smokes is a long, tan-colored feature runs toward the northwest in the upper-left.
September 29, 2025

In preparing to visit the Moon’s surface, soon-to-be lunar explorers in NASA’s Apollo program first ventured into a variety of unfamiliar landscapes on Earth. A couple of these trips, in the summers of 1965 and 1966, took astronauts to Alaska’s remote Katmai National Park for simulations of field geology in Moon-like environments.

In one exercise, which they called “playing the Moon game,” pairs of astronauts were placed at unfamiliar field sites and asked to pretend as if they were on the Moon. By the account of William Phinney, Apollo’s science training coordinator, they were tasked with collecting representative geologic samples and practicing how to communicate their observations to scientists.

A detailed satellite image centers on the Valley of Ten Thousand Smokes in Alaska. The tan-colored feature runs southeast-to-northwest. Snowy peaks appear on the right side of the image, and green, forested valleys fill the left side.
September 29, 2025

The Alaskan setting for the Moon game was an unusual volcanic landscape called the Valley of Ten Thousand Smokes. The valley is full of debris deposited by the 1912 eruption of Novarupta—the largest volcanic event on Earth in the 20th century.

The images above, acquired on September 29, 2025, with the OLI (Operational Land Imager) on Landsat 9, show the massive ash flow deposited by Novarupta. The layer measures up to 660 feet (200 meters) thick and was emplaced at a searing 1,380 degrees Fahrenheit (750 degrees Celsius). 

The Valley of Ten Thousand Smokes, shown in the 1917 photo below, is so named because of the abundance of fumaroles—gas and steam-emitting vents—that filled the valley for a decade after the eruption. A few hundred persisted more than 10 years, with some lasting until the 1990s.

Three people stand in the foreground of this black-and-white photo, silhouetted by steam coming from a fumarole. A dark, barren landscape dotted with plumes of rising steam extends into the background.
1917

Scientists initially suspected that the monster eruption occurred at Mount Katmai, a neighboring volcano with a large caldera located 6 miles (10 kilometers) east of Novarupta’s dome. However, they later determined that the eruption actually occurred at Novarupta—whose name means “new eruption”—after stealing magma from beneath Katmai. As the magma chamber emptied, Katmai collapsed, forming the 2.5-mile-wide (4-kilometer-wide) caldera present today.

The volcanic landscape in the Valley of Ten Thousand Smokes is far fresher than the ancient lava flows that formed the Moon’s volcanic features. But for the Apollo astronauts, it offered an “excellent opportunity to view volcanic materials and landforms in nearly pristine condition,” Phinney wrote. They studied evidence of fumaroles and examined vertical sections of the deposits where streams had eroded deep gorges.

This photo shows a broad valley filled with tan-colored volcanic material in the foreground and snowy mountains in the background. The ashy volcanic deposits create a mostly flat valley floor, except where steep-sided chasms formed by erosion run through it.
June 9, 1991

Researchers continue to visit this Alaskan wilderness in search of clues that could help decipher the geology of the Moon and Mars. In 2024, the Goddard Instrument Field Team (GIFT) trekked to the Valley of Ten Thousand Smokes to study its icy volcanic landscape. Like the valley, Mars contains glaciers and ice sheets layered with dust and ash, a dynamic and difficult-to-interpret environment.

Advancing lunar science, the GIFT team also collected samples from rock formations comparable to the Moon’s Gruithuisen Domes. These mysterious features are made of hardened lava with a different composition than the surrounding rock. With more to learn about our nearest celestial neighbor, the spirit of the Moon game lives on in the 21st century.

NASA Earth Observatory images by Lauren Dauphin, using Landsat data from the U.S. Geological Survey. Photos from National Geographic Society Katmai expeditions photographs, Archives and Special Collections, Consortium Library, University of Alaska Anchorage, and from the U.S. Geological Survey Volcano Hazards Program. Story by Lindsey Doermann. 

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A satellite image shows part of Alaska’s Katmai National Park. A chain of snowy mountain peaks stretches from the bottom left corner to the right side of the image. The Valley of Ten Thousand Smokes is a long, tan-colored feature runs toward the northwest in the upper-left.

September 29, 2025

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NASA Names Sean Gallagher as Chief Information Officer

Sean Gallagher
Official NASA portrait of Sean Gallagher
Credit: NASA

NASA has selected Sean Gallagher as the agency’s chief information officer (CIO). In this role, he is responsible for the agency’s entire portfolio of Information Technology products and services. Gallagher has been serving in an acting capacity since January and his permanent role is effective immediately.

“Sean Gallagher’s leadership has been instrumental in strengthening NASA’s IT foundation and ensuring our workforce has the secure, modern tools needed to enable groundbreaking missions every day,” said NASA Deputy Administrator Matt Anderson. “As CIO, Sean will continue advancing the agency’s technology capabilities to support discovery, innovation, and mission success across NASA.”

Most recently, Gallagher also has served as the deputy chief information officer for Operations in the Office of the Chief Information Officer at NASA Headquarters in Washington, as well as a senior advisor for Transformation. This team provides services to tens of thousands of end users located in the U.S. and abroad in support of NASA missions, enabling discoveries, faster data sharing, increased workforce productivity, and more. Gallagher has worked with all NASA centers to implement efficient and effective IT operating models.

Previously, Gallagher was the CIO of NASA’s Glenn Research Center in Cleveland, leading IT initiatives for aeronautics, space, research and engineering, and test missions. He joined NASA in 2012 as Glenn’s deputy CIO and previously worked at Booz Allen Hamilton as a senior associate supporting a variety of federal, defense, and commercial customers.

Gallagher developed his leadership and management experience as a Signal Corps officer in the United States Army. He also served as a platoon leader managing the combat service support readiness of a tactical communications unit, a human resource manager for the 40th Signal Battalion, and as a network engineer for the 11th Signal Brigade. He has a bachelor’s degree in physics from John Carroll University and a master’s degree in computer information systems from the University of Phoenix.

For more information about NASA’s missions, visit:

https://www.nasa.gov

-end-

Camille Gallo / Cheryl Warner
Headquarters, Washington
202-358-1600
camille.m.gallo@nasa.gov / cheryl.m.warner@nasa.gov

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Jun 23, 2026
Editor
Jennifer M. Dooren

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58th Girl Scouts Unite Event

58th Girl Scouts Unite Event, July 23-25, 2026

Join NASA in the Exhibit Hall (Booth #206) for Hyperwall Storytelling by NASA experts. Full Hyperwall Agenda below.

Thursday, July 23

11:00AM – 11:15 AM From Daisy to NASA Engineer Barbara Hilton
11:15AM – 11:30 AM Exploring Mars, The Planet Next Door Lindsay Hays
11:30AM – 11:45 AM Get Ready With Me: Going to the Moon Naoma McCall
11:45Am – 12:00 PM NASA Is for Everyone! (talk about careers at NASA beyond science and engineering) Amy Kaminski
12:00PM – 12:15 PM Finding Asteroids Before They Find Us: Planetary Defense at NASA Kelly Fast

2:15 PM – 2:30 PM How to Nerd Your Way Into Science Communications Karen Romano Young
2:30 PM – 2:45 PM Earth: Exploring our home planet is a team effort Lesley Ott
2:45 PM – 3:00 PM TBD Jenny Mottar
3:00 PM – 3:15 PM The Journey Starts HERE: One CREW, Your HOME, Our MISSION Kaitlin Harbeck
3:15 PM – 3:30PM TBD – Artemis Overview Dominique Brewer
3:45 PM – 4:00 PM Social Media… For Science! Sofie Bates

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Tuesday, 23 June 2026

NASA Sounding Rocket to Launch Student Experiments

3 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

NASA’s Wallops Flight Facility in Virginia is scheduled to launch a sounding rocket carrying student-developed experiments for the agency’s RockSatX and RockOn programs Wednesday, June 24, between 5:30 and 9:30 a.m. EDT, with a backup day on Thursday, June 25.

In the foreground, a line of people stand at a safe distance away from a sounding rocket launching in the background. The rocket is just off the pad with a plume of fire and smoke underneath.
Students watch as their experiments launch aboard a sounding rocket for the RockSat-X program from NASA’s Wallops Flight Facility Aug. 11, 2022, at 6:09 p.m. EDT. The Terrier-Improved Malemute rocket carried the experiments to an altitude of 99 miles before descending via a parachute and landing in the Atlantic Ocean.
NASA Wallops/Terry Zaperach

The RockSat and RockOn programs provide technical training and hands-on experiences that prepare and equip students to enter the United States aerospace industry. For the first time, NASA will combine both the RockSat and RockOn missions into one rocket, which will carry experiments developed by nearly 250 participants from 38 university and community college teams.

“The challenge was finding ways to fit as many experiments onto one sounding rocket as we could,” said Victoria Stoffel, workforce development lead at NASA Wallops. “The Sounding Rocket Program Office team found creative ways to fit nearly 50 experiments into one rocket. We are grateful to the Wallops teams for making this happen for the students to get the most from this experience.”

The RockOn teams work together to build their experiment onsite, getting hands-on experience putting together a circuit board from scratch and launching it into space. The more advanced RockSat program teams design and build their experiments, going through design reviews modeled on larger NASA missions. Each team can experience what it’s like working on a real NASA mission, from development to launch.

The RockSat student experiments range from taking measurements of weather and radiation in Earth’s upper atmosphere to testing technologies, such as heat shields, space-debris tracking, and robotic servicing, that could help future NASA missions.

The Terrier-Improved Malemute suborbital sounding rocket, which will carry the experiments, is expected to reach an altitude of about 100 miles before descending by parachute into the Atlantic Ocean to be recovered. The launch may be visible in the Chesapeake Bay region.

A visibility map showing the mid-Atlantic region. The map shows how many seconds after that people in the area may be able to see the Terrier-Improved Malemute sounding rocket in the sky.
A launch visibility map for a Terrier-Improved Malemute sounding rocket launching from NASA’s Wallops Flight Facility in Virginia.
NASA

The Wallops Visitor Center’s launch viewing area will open June 24 at 4:30 a.m. for viewing. A livestream will begin approximately 10 minutes before launch on the Wallops YouTube channel. Launch updates also are available via the center’s Facebook page.

For more information about NASA’s Sounding Rocket Program, visit:

https://www.nasa.gov/soundingrockets

By Jamie Adkins

NASA’s Wallops Flight Facility, Virginia

List of RockSat Teams

  • Capital Tech University, Maryland
  • Clemson University, South Carolina
  • College of the Canyons, California
  • Colorado Space Grant Consortium
    • University of Colorado Boulder
  • Escuela de Troquelería y Herramentaje, Puerto Rico
  • New Jersey Institute of Technology
  • Northwest Nazarene University, Idaho
  • Rockets of the Rockies, Colorado
    • Red Rocks Community College
    • Arapahoe Community College
  • Temple University, Pennsylvania
  • Tidewater Community College, Virginia
  • University of Alabama Huntsville
  • University of Delaware
  • University of Hartford, Connecticut
  • University of Hawaii Community Colleges
  • University of Kentucky
  • University of Nebraska Lincoln
  • University of Puerto Rico
  • University of Virginia
  • Virginia Tech
  • West Virginia Space Flight Design Challenge
    • Blue Ridge Community College
    • West Virginia Wesleyan College
    • West Virginia University
    • West Virginia State University
    • Marshall University

List of RockOn Teams

  • University of Delaware
  • Wilmington University, Delaware
  • Chief Dull Knife College, Montana
  • Grambling State University, Louisiana
  • College of the Canyons, California
  • Eastern Shore Community College, Virginia
  • Salisbury University, Maryland
  • Capitol Technology University, Maryland
  • College of the Desert, California
  • Flathead Valley Community College, Montana
  • Delgado Community College, Louisiana
  • Des Moines Area Community College, Iowa
  • Langston University, Oklahoma
  • University of Kentucky
  • Saginaw Valley State University, Michigan
  • Morgan State University, Maryland
  • Pennsylvania State Harrisburg
  • Middlesex College, New Jersey
  • University of Colorado
  • Wor-Wic Community College, Maryland
  • Tidewater Community College, Virginia
  • Montana Technological University
  • University of Hartford, Connecticut
  • University of Maryland Eastern Shore

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Last Updated
Jun 22, 2026
Editor
Jamie Adkins
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NASA Invites Media to Botswana Artemis Accords Signing Ceremony

Credit: NASA

The Republic of Botswana will sign the Artemis Accords during a ceremony at 9:30 a.m. EDT Thursday, June 25, at NASA Headquarters in Washington.

NASA Deputy Administrator Matt Anderson will host Botswana’s Minister of Communications and Innovation David Tshere and U.S. Department of State Senior Advisor for Space Gregory Autry for the event.

This event is in person only. Media interested in attending must RSVP no later than 5 p.m. on Wednesday, June 24, to: hq-media@mail.nasa.gov. NASA’s media accreditation policy is online.

In 2020, during the first Trump Administration, the United States, led by NASA and the State Department, joined with seven other founding nations to establish the Artemis Accords, responding to the growing interest in lunar activities by both governments and private companies.

The accords introduced the first set of practical principles aimed at enhancing the safety, transparency, and coordination of civil space exploration on the Moon, Mars, and beyond. Botswana will be the 68th country to sign the Artemis Accords.

Learn more about the Artemis Accords at:

https://www.nasa.gov/artemis-accords

-end-

Camille Gallo / Jennifer Dooren 
Headquarters, Washington 
202-358-1600 
camille.m.gallo@nasa.gov / jennifer.m.dooren@nasa.gov



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Monday, 22 June 2026

NASA’s Chandra Finds Possible Supernova Remnant

Set against a backdrop packed with distant stars and other specks of light are two distinct, overlapping clouds. The larger, visually dominant cloud, is red and multifaceted. It has an irregular shape, and features patches of different textures, including pockets that resemble wispy smoke, tangles of faint red veins, and clear streaking lines. This large cloud of expanding gas represents radio data from the MeerKAT telescope in South Africa. Overlapping with that red cloud is a cloudy blue blob representing X-ray data from NASA's Chandra X-ray Observatory and ESA's XMM-Newton.
Using data from NASA’s Chandra X-ray Observatory, astronomers may have found a supernova remnant in an intriguing neighborhood in the middle of our galaxy.
X-ray: NASA/CXC/UCLA/Z. Zhu et al.; ESA/XMM-Newton; Optical: PanSTARRS; Radio: MeerKAT; Infrared (JWST): NASA/ESA/CSA/STScI; Image Processing: NASA/CXC/SAO/L. Frattare and P. Edmonds

Using data from NASA’s Chandra X-ray Observatory, astronomers may have found a supernova remnant – seen in this June 11, 2026, image – in an intriguing neighborhood in the middle of the Milky Way galaxy. Supernova remnants are the expanding remains of exploded stars and provide elements like iron, oxygen, and silicon that are critical for the formation of planets and for life as we know it to form and flourish.

This new supernova remnant, if confirmed, would be one of the closest ever discovered to the supermassive black hole at the central region of our home galaxy, an exotic region crammed with massive stars, long threads of magnetic fields and dense clouds of gas orbiting rapidly around the Galactic Center.

Read more about this discovery.

Image credit: -ray: NASA/CXC/UCLA/Z. Zhu et al.; ESA/XMM-Newton; Optical: PanSTARRS; Radio: MeerKAT; Infrared (JWST): NASA/ESA/CSA/STScI; Image Processing: NASA/CXC/SAO/L. Frattare and P. Edmonds



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NASA to Cover US Spacewalk 95, Host Preview News Conference

NASA astronaut Jessica Meir waves at the camera during a seven-hour, two-minute spacewalk outside the International Space Station on March 18, 2026.
Credit: NASA

NASA astronauts will venture outside the International Space Station on Tuesday, June 30, to replace a wrist joint on the orbital complex’s Canadarm2 robotic arm. The spacewalk is scheduled to begin at approximately 8 a.m. EDT.

Experts from NASA and CSA (Canadian Space Agency) will preview the upcoming spacewalk during a news conference at 2 p.m. on Thursday, June 25, on the agency’s YouTube channel. The briefing will take place at NASA’s Johnson Space Center in Houston. Learn how to watch NASA content through a variety of platforms, including social media.

Participants include:

  • Bill Spetch, operations and integration manager, International Space Station Program, NASA Johnson
  • Fiona Antkowiak, spacewalk flight director, NASA Johnson
  • Jason Dyer, deputy liaison manager, CSA

United States-based media interested in attending in person must contact the Johnson newsroom no later than 5 p.m. Wednesday, June 24, at: jsccommu@mail.nasa.gov. Media joining by phone should request dial‑in details by the same deadline. To ask a question, media must dial in no later than 15 minutes before the start of the news conference.

Tuesday, June 30

NASA astronauts Chris Williams and Jessica Meir will exit the station’s Quest airlock to replace a wrist joint that malfunctioned during normal Canadarm2 operations on May 27 after the arm drew elevated motor current and did not move as expected.

Watch NASA’s live U.S. spacewalk 95 coverage beginning at 6:30 a.m. EDT on NASA+, Amazon Prime, Netflix, and the agency’s YouTube channel. The spacewalk is expected to last roughly six-and-a-half hours.

NASA worked alongside CSA to understand the issue and determined a spacewalk was required to replace the joint using a spare already aboard the space station. Repairs to robotics, like Canadarm2, are normal and expected after more than 25 years of continuous operations, as the system was designed with replaceable components and planned maintenance in mind.

This spacewalk will be the second for Williams and the fifth for Meir. Williams will serve as spacewalk crew member 1 and will wear a suit with red stripes. Meir will serve as crew member 2 and will wear an unmarked suit. It will be the 280th spacewalk in support of space station assembly, maintenance, and upgrades.

To learn more about International Space Station research, operations, and its crews, visit:

https://www.nasa.gov/station

-end-

Jimi Russell
Headquarters, Washington
202-358-1100
james.j.russell@nasa.gov

Sandra Jones
Johnson Space Center, Houston
281-483-5111
sandra.p.jones@nasa.gov



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NASA’s Webb Finds Clues to Ancient, Distant Origin of Comet 3I/ATLAS

4 Min Read

NASA’s Webb Finds Clues to Ancient, Distant Origin of Comet 3I/ATLAS

Comparison of three telescope images side by side. They are roughly spherical but pixelated, with more intense color saturation in the center. From left to right: smallest sphere is blue and labeled H2O, orange is larger and labeled CO2, and red is largest and labeled CO. A scale bar at the lower left is labeled 1300 km/1 arcsecond and is about one fourth of each of the three images. A compass at the lower right shows north pointing up to 12 o’clock, east pointing left to 9 o’clock, and a fainter arrow labeled to Sun pointing down to 8 o’clock.
Researchers used the NIRSpec (Near-Infrared Spectrograph) instrument on NASA’s James Webb Space Telescope to map specific chemical contents of comet 3I/ATLAS as it moved away from the Sun. Full image shown below.
Credits:
Image: NASA, ESA, CSA, STScI, Martin Cordiner (CUA, NASA-GSFC); Image Processing: Alyssa Pagan (STScI)

As interstellar comet 3I/ATLAS began moving away from the Sun in December 2025, astronomers took the opportunity to turn NASA’s powerful James Webb Space Telescope in its direction and capture detailed measurements of its chemical components. The comet was freshly warmed from its closest pass by the Sun, and its ancient ice had been converted to a bright coma of gas ideal for observation. 

Webb captured detailed data, including chemical ratios of carbon and deuterium, also known as heavy hydrogen, that are not found in solar system comets. The results surprised researchers. Working backward, astronomers used the components that make up comet 3I/ATLAS to understand the environment in which it formed. 

A paper detailing the findings published June 22 in the journal Nature

Image: Interstellar Comet 3I/ATLAS (NIRSpec IFU)

Comparison of three telescope images side by side. They are roughly spherical but pixelated, with more intense color saturation in the center. From left to right: smallest sphere is blue and labeled H2O, orange is larger and labeled CO2, and red is largest and labeled CO. A scale bar at the lower left is labeled 1300 km/1 arcsecond and is about one fourth of each of the three images. A compass at the lower right shows north pointing up to 12 ou2019clock, east pointing left to 9 ou2019clock, and a fainter arrow labeled to Sun pointing down to 8 ou2019clock.
Researchers used the NIRSpec (Near-Infrared Spectrograph) instrument on NASA’s James Webb Space Telescope to map specific chemical contents of comet 3I/ATLAS as it moved away from the Sun. 
Image: NASA, ESA, CSA, STScI, Martin Cordiner (CUA, NASA-GSFC); Image Processing: Alyssa Pagan (STScI)

The comet’s name comes from its status as the third confirmed interstellar comet, meaning it originated outside the solar system, and the telescope that first spotted it, the NASA-funded ATLAS (Asteroid Terrestrial-impact Last Alert System).

“This was a unique opportunity to study an ancient object from the distant galaxy, probably pre-dating our Sun and solar system,” said astro-chemist Martin Cordiner of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and lead author of the study. “On the one hand, we get direct insight into that distant time and place, and on the other, we learn something about how unusual our own solar system may be.”

Cordiner and the research team joined astronomers from many sub-disciplines in taking the opportunity to get a look at 3I/ATLAS on its journey through the solar system. They received approval to interrupt Webb’s planned schedule of observations to make use of its NIRSpec (Near-Infrared Spectrograph) instrument to study the comet. 

NIRSpec revealed exceptionally high levels of deuterium, about 30 times more than seen in solar system comets. This implies that 3I/ATLAS may have originated in a very cold system much earlier in the history of our galaxy. During its formation, the material that became incorporated into 3I/ATLAS was likely exposed to plenty of radiation, but not any long-term warmth that would have reprocessed its “heavy water” ice, with deuterium, into the type of H2O ice we are familiar with on Earth.

Image: 3I/ATLAS Compared to Solar System Comets

Infographic showing differences in measured ratios of heavy carbon and heavy hydrogen between solar system comets and interstellar comet 3I/ATLAS. Title text reads Comet 3I/ATLAS, Composition Compared With Solar System Comets. Top portion of the infographic has headline Heavy Carbon, plus a horizontal scale in increments of 50 ranging from zero to 250 measuring the ratio of Carbon-12 to Carbon-13. Three solar system comets appear just below 100 on the scale, while 3I/ATLAS appears above 150 for carbon monoxide and about 170 for carbon dioxide.  
Bottom portion of infographic has headline Heavy Hydrogen and a horizontal scale ranging from 10 to the negative fifth power on the left to approximately 10 to the negative first power on the right, though 10 to the first is not labeled. This scale is labeled Ratio of Heavy Hydrogen Measured in Water. Eleven solar system comets appear on the graph, all falling to the right of 10 to the negative fourth power. Comet 3I/ATLAS appears at 10 to the negative second power.
These graphs lay out the significant difference in composition between the interstellar comet 3I/ATLAS and comets originating in our solar system. This very specific data helps researchers build a picture of the comet’s original planetary system. 
Illustration: NASA, ESA, CSA, Martin Cordiner (CUA, NASA-GSFC), Leah Hustak (STScI)

Additionally, NIRSpec showed only traces of carbon-13 compared to lighter-weight carbon-12. This also points to a very old origin for 3I/ATLAS, as stellar systems become enriched with carbon-13 over time as generations of stars are born and die in the galaxy. That is why there are higher levels of carbon-13 in our system, around our Sun, which formed relatively recently, 4.5 billion years ago.

The research team estimates that 3I/ATLAS could have formed as long as 10 to 12 billion years ago, during the universe’s “cosmic noon,” when star formation was at its height. Its young origin system was likely ensconced in a relatively cold, dense cloud. The abundance of heavy water shows that 3I/ATLAS spent its formative years in a deeply frozen state. 

A separate study using the European Southern Observatory’s Very Large Telescope, led by astronomer Cyrielle Opitom of the University of Edinburgh, complements Webb’s findings with an analysis of 3I/ATLAS’s carbon and nitrogen varieties in the form of the chemical cyanide.

“For us as scientists, finding these rare isotopes is fascinating, but the bigger picture here is looking at the possibilities of prebiotic chemistry elsewhere in the galaxy,” said Stefanie Milam of NASA Goddard and co-author of the study with Cordiner. “So far, we know of only one place in the vast cosmos where chemical ingredients led to life – our solar system, our Earth. Analysis of these interstellar objects is a major step towards learning how common, or uncommon, the conditions for the evolution of life are in the universe.”

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).

To learn more about Webb, visit:

https://science.nasa.gov/webb

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The following sections contain links to download this article’s images and videos in all available resolutions followed by related information links, media contacts, and if available, research paper and Spanish translation links.

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Read more: NASA’s Webb Detects Methane on Interstellar Comet 3I/ATLAS

Explore more: NASA’s 3I/ATLAS Observation Timeline

Watch: Interstellar Visitor is Fastest Comet Ever Recorded

Watch: ViewSpace | Interstellar Comet Measured

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Playing the Moon Game 

Science Earth Observatory Playing the Moon Game  Earth Earth Observatory Image of the Day EO Explorer All Topics Atmo...