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NASA - Breaking News

NASA to Stream SpaceX Crew-12 Return, Splashdown Live

2026-10-05 21:44

NASA’s SpaceX Crew-12 members gather for a portrait in the pressure suits they will wear when they depart the International Space Station inside the SpaceX Dragon spacecraft. From left, Roscosmos cosmonaut and mission specialist Andrey Fedyaev, NASA astronauts Jack Hathaway and Jessica Meir, Crew-12 pilot and commander respectively, and ESA (European Space Agency) astronaut and mission specialist Sophie Adenot.
Credit: NASA/Anil Menon

NASA and SpaceX are targeting no earlier than 8:05 a.m. EDT, Wednesday, Oct. 7, for the undocking of the agency’s SpaceX Crew-12 mission from the International Space Station, pending weather conditions.

An Oct. 7 undock puts NASA astronauts Jessica Meir and Jack Hathaway, ESA (European Space Agency) astronaut Sophie Adenot, and Roscosmos cosmonaut Andrey Fedyaev on schedule to splash down off the coast of California at approximately 11:34 a.m. on Thursday, Oct. 8.

NASA’s live Crew-12 return coverage will stream through a variety of platforms. Learn where to watch online:

https://www.nasa.gov/live

Mission managers continue monitoring conditions in the recovery area, as undocking of the SpaceX Dragon depends on spacecraft readiness, recovery team readiness, weather conditions in the Pacific off the coast of California, and other factors.

NASA’s coverage is as follows (all times Eastern and subject to change based on real-time operations):

Wednesday, Oct. 7

6 a.m.: Hatch closure coverage begins

6:20 a.m.: Hatch closing

7:45 a.m.: Undocking coverage begins

8:05 a.m.: Undocking

Following the conclusion of undocking coverage, NASA will provide audio-only communications between Crew-12, the space station, and flight controllers during Dragon’s transit away from the orbital complex.

Thursday, Oct. 8

10:20 a.m.: Return coverage begins

10:46 a.m.: Deorbit burn

11:34 a.m.: Splashdown

1:15 p.m.: International Space Station briefing for Crew-12 return and SpaceX Commercial Resupply Services-35 launch with the following participants:

  • Bill Spetch, deputy manager of Commercial, NASA’s Low Earth Orbit Program
  • Dr. Liz Warren, deputy chief scientist, NASA’s Low Earth Orbit Program
  • Lee Echerd, senior mission manager, Customer Operations and Integration, SpaceX
  • Andreas Mogensen, leader, Human Exploration Group, ESA

To participate virtually in the teleconference, media must contact the NASA Johnson newsroom for call details by 12 p.m., Oct. 8, at: jsccommu@mail.nasa.gov or 281-483-5111. To ask questions, media must dial in no later than 10 minutes before the start of the call. The agency’s media credentialing policy is available online.

For more information about the Crew-12 mission, visit:

https://www.nasa.gov/mission/nasas-spacex-crew-12

-end-

Joshua Finch / Jimi Russell
Headquarters, Washington
202-358-1100
joshua.a.finch@nasa.gov / james.j.russell@nasa.gov

Sandra Jones / Joseph Zakrzewski
Johnson Space Center, Houston
281-483-5111
sandra.p.jones@nasa.gov / joseph.a.zakrzewski@nasa.gov

Steve Siceloff
Kennedy Space Center, Fla.
321-867-2468
steven.p.siceloff@nasa.gov

NASA Astronaut Christina Koch at Eagles vs. Rams

2026-10-05 17:42

NASA astronaut Christina Koch (left, facing the camera) claps on a football field. An NFL cameraperson films her. The Philadelphia Eagles mascot is on the field as well (right), along with a line of cheerleaders in the background. Fans can be seen in the stands.
NASA/Thalia Patrinos

NASA astronaut and mission specialist of the agency’s Artemis II mission, Christina Koch, leads the fans in singing the Eagles Fight Song from the field at an NFL game between the Philadelphia Eagles and the Los Angeles Rams at Lincoln Financial Field on Sunday, Oct. 4, 2026, in Philadelphia.

NASA’s engagement at NFL games is part of the agency’s Inspiration Tour, aimed at strengthening connections between NASA and its partners and showcasing innovation in air and space in the lead up to the MAX POWER aerospace technology expo and airshow at the agency’s Kennedy Space Center in early November.

Image credit: NASA/Thalia Patrinos

NASA Testing Aims at Supercooled Large Droplet Aviation Safety

2026-10-05 15:27

3 Min Read

NASA Testing Aims at Supercooled Large Droplet Aviation Safety

Ice collection seen on un-heated sections of the 1D2D-X ice drop detection probe in the test section of the IRT (Icing Research Tunnel). Drop Size Probe testing – SFD (Subsonic Flight Demonstrator) of SLD (Supercooled Large Drop) Instrumentation Test in IRT (Icing Research Tunnel) – Particle Size Distribution Entry, June 8-11, 2026 Large Drop Testing in IRT
Credits: NASA/Quentin Schwinn

NASA is leveraging its expertise and enhancing its test facilities to help address a rare but persistent aviation hazard: icing that occurs when aircraft encounter unusually large, very cold water droplets in clouds.  

The problem, known as “supercooled large droplet icing,” occurs when aircraft fly through clouds containing unusually large drops of water that are very cold but remain liquid. When a plane passes through those drops, they can rapidly freeze to surfaces that are not protected from ice buildup.  

With a series of tests in the Icing Research Tunnel at Glenn Research Center in Cleveland, NASA researchers are helping U.S. industry better understand the phenomenon. 

SFD (Subsonic Flight Demonstrator) of SLD (Supercooled Large Drop) Instrumentation Test – Particle Size Measurement in the IRT (Icing Research Tunnel), June 8-11, 2026. Drop size shown on computer from Drop Sizing Probe seen in the IRT test section.
NASA/Quentin Schwinn

Supercooled water is common in clouds – droplets can go below 32 degrees Farenheit but not freeze unless they encounter dust or other tiny particles around which they can crystalize. Aircraft are designed to encounter typical icing conditions where droplets range from 2 to 100 microns in diameter (for comparison, a human hair is about 70 microns wide). But in rarer cases, clouds can contain supercooled large drops up to 2,000 microns in diameter (if you’ve ever been caught in freezing rain, you’ve encountered these droplets at ground level). These much larger droplets can hit or splash to the aft of an aircraft, including areas behind conventional ice protection systems.  

The aviation industry relies on engineering tools to help design their aircraft. Current tools work well for typical clouds, but engineers have questions about how well they account for the physics of supercooled large drops. To help answer those questions, NASA is working to enhance the equipment it uses to generate and measure experimental clouds for testing in the Icing Research Tunnel.  

Ice collection seen on un-heated sections of the ice drop detection probe in the test section of the IRT (Icing Research Tunnel). Drop Size Probe testing – SFD (Subsonic Flight Demonstrator) of SLD (Supercooled Large Drop) Instrumentation Test in IRT (Icing Research Tunnel) – Particle Size Distribution Entry, June 8-11, 2026
NASA/Quentin Schwinn

NASA researchers have experimented with brand new probes that help calibrate the sizes of the drops in the clouds the tunnel produces. The probes can “see” drops larger than 45 microns and perform a real-time analysis of their sizes. NASA will compare these results, a laborious technique of post-processing droplet size image data from the tunnel. The results will be mated to results from a different probe that measures droplets smaller than 45 microns. With this, the complete droplet size spectrum is known. 

The test campaign marks an important milestone for the Subsonic Flight Demonstrator project, part of NASA’s Research and Technology Mission Directorate. Detailed analysis of the collected data continues, and NASA’s project team will share results with the broader aerospace community once complete.

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Suspected Second-generation Planet Solves NASA Hubble Cold Case

2026-10-05 15:00

5 Min Read

Suspected Second-generation Planet Solves NASA Hubble Cold Case

A gaseous planet in the right foreground, seen mostly in silhouette, orbits a small, white star in the background at left. The star is surrounded by a thin, bright white disk tilted from lower left to upper right. A semi-transparent tail of material comes off the planet toward upper right. Distant stars dot the black background of space.

This artist’s concept depicts a possible explanation for the unusual chemical abundances NASA’s Hubble Space Telescope detected in the HS 0209+0832 system: a second-generation planet orbiting a white dwarf star. 

Credits:
Artwork: NASA, ESA, Leah Hustak (STScI)

Diligent sleuthing by astronomers has broken open a cold case in the data archive of NASA’s Hubble Space Telescope. In a study published Monday in Nature Astronomy, researchers report uncovering a surprising chemical clue that indicates the white dwarf star HS 0209+0832 may host a second-generation planet. 

A white dwarf is the remnant core of a low-mass star that has burned through all its nuclear fuel and lost its outer envelope of gas and dust to space. A second-generation planet is a world that forms around the stellar remnant from its cast-off material. 

“Rather than the white dwarf stage being a kind of epilogue to the story of a star and its planets, this research points to the systems we are familiar with only being the first chapter of a potentially much longer tale, with some new characters showing up. That’s a really exciting prospect to pursue,” said Jamie Williams, astronomer and lead author, a doctoral candidate at the University of Warwick in the United Kingdom.

Earth and the other planets in our solar system are first-generation planets, which form from material left over from a star’s birth. 

Illustration divided into quadrants, showing the evolution of a star system over time. The upper left is labeled 1. Sun-like star. It shows a small, glowing yellow star centered with other faint stars in the background of space. The upper right quadrant is labeled 2. Red giant. It shows a much larger, puffy orange-red star with a yellow glow within. The bottom left quadrant is labeled 3. White dwarf with second-generation protoplanetary disk, showing a bright white star, smaller than the original Sun-like star, surrounded by a glowing dusty blueish-white disk that is brighter closer to the star. The lower right quadrant is labeled 4. Accretion of a second-generation planet. It shows a similar star to quadrant 3, but the disk is reduced in size and is more purple in color. A planet orbits to the lower left of the star. The planet is larger than the star and has a faint tail leading back to the disk around the star.
This artist’s concept, not to scale, imagines the evolution of a Sun-like star (1) into an aging red giant (2) and then a small, bright white dwarf surrounded by a disk of its expelled outer layers (3), from which a second-generation planet forms (4). 
Illustration: NASA, ESA, Leah Hustak (STScI)

“What Hubble is showing us in this white dwarf system is something we haven’t seen before: a high abundance of the element niobium, the signature of which I was unfamiliar with when I first found it in the archival data,” Williams said.

When Hubble first observed the star in 1999, the data contained roughly 100 chemical features that could not be identified. Williams went back to those records armed with an updated chemical database and found that niobium matched many of the mystery features.

Williams explained that, while niobium is found in our solar system and has multiple uses on Earth, including in jewelry and medical imaging devices, the amount Hubble found in the HS 0209+0832 system points to a planet forming not from a star’s birth, but from the material ejected as it dies. 

“Niobium and other elements heavier than iron are astronomically special because, unlike many common elements, they are not formed in the cores of stars by thermonuclear fusion,” said Nicholas Stone, a theoretical astrophysicist at the University of Wisconsin – Madison and member of the research team. “Instead, these heavy elements can only be synthesized in the exotic conditions that briefly emerge inside dying stars. The presence of niobium is a signpost of these ‘death’ throes, and the expulsion of the dying star’s innards into space.” 

Once the star ejected this chemically enriched material, the team theorizes that some of it coalesced into a gas giant planet. The remainder of the ejecta dispersed long ago, but the planet remains.

“When Jamie asked me about niobium in relation to this study I was truly gobsmacked, as that element had not been reported in any other white dwarf analyzed to date. Once we realized it was there, everything fell into place,” said astronomer and study co-author Boris Gaensicke, also at the University of Warwick.

Line graph titled HS 0209+0832, White Dwarf Atmosphere Features. Hubble Space Telescope spectral data is shown in white, compared with a best fit model in red. The vertical y axis is labeled Brightness, with brighter at the top and dimmer at the bottom. The horizontal x axis is labeled Wavelength of light, angstroms. One-third of the way across the x axis is labeled 1452. To the right of the graph’s center is angstrom label 1453, and the right edge of the graph is labeled angstrom 1454.

Three dramatic dips in the spectrum are labeled with element names and abbreviations: Niobium, Nb, Nickel, Ni, and Calcium, Ca. The niobium Hubble data and model match well and appear to the right of the 1452 angstrom label. To the right, Hubble’s nickel data is much dimmer than the model, appearing just left of the graph’s center. Hubble’s data for calcium is a little dimmer than the model, and appears to the right, about one-sixth of the way from the right-hand edge of the graph.
NASA’s Hubble Space Telescope spectrum shows the unusual abundances of certain elements it found in the HS 0209+0832 system. Dips indicate where niobium, nickel, and calcium are absorbing light, so less light in that part of the spectrum reached Hubble. 
Illustration: NASA, ESA, Leah Hustak (STScI)

The research team confirmed the Hubble observations with data from NASA’s retired FUSE (Far Ultraviolet Spectroscopic Explorer) mission, which also showed strong signatures of niobium in the HS 0209+0832 system. 

NASA’s TESS (Transiting Exoplanet Survey Satellite) also observed the white dwarf for four months, allowing it to detect periodic brightness variations that indicate that a planet orbits at a distance of about 3.7 million miles (6 million kilometers), much closer than Mercury orbits the Sun. 

The research team estimates the candidate planet is a gas giant about the size of Jupiter that is rapidly losing atmosphere. Because the white dwarf star is relatively new, it is still very hot and likely blasting this planet with energy that is stripping its outer material. This could result in the planet having a comet-like tail of material that would form a disk around the white dwarf star and fall back on to its surface, leading to Hubble detecting the niobium when studying the star. Despite this mass loss, Williams said that the planet is likely not a temporary blip on the cosmic radar. 

“If the second-generation planet is there, I think it is likely to survive. Eventually the white dwarf will cool and then maintain a consistent temperature, with the planet in its stable habitable zone for millions of years,” Williams said.

Williams added that there is still a lot of work to do to understand these types of systems — how second-generation planets form, how common or rare they are, and how they evolve in orbit around a “dead” star. He’ll use Hubble to explore these questions for the next several years, hoping to build up substantial data and statistics about these new types of celestial bodies.

“I think this research is an important example of the fact that scientific discovery is not a straight path,” Gaensicke said. “It often needs that magical moment when people discuss big questions on their minds and realize that together they can find unexpected answers.”

The Hubble Space Telescope has been operating for more than three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.


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Details

Last Updated

Oct 05, 2026

Editor
Andrea Gianopoulos
Contact

Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov

Leah Ramsay, Christine Pulliam
Space Telescope Science Institute
Baltimore, Maryland

APOD: 2026 October 5 – M104: The Sombrero Galaxy’s Tidal Streams

2026-10-05 04:05

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 starfield has an bright blobby mess in middle. Running vertically through the very middle is a dark streak. A diagonal ring of brightness surrounds the central blob.

M104: The Sombrero Galaxy’s Tidal Streams

Explanation: A deep image of the Sombrero galaxy reveals surprises. M104 is named the Sombrero galaxy because, on shorter exposures, it looks like a hat. A key defining feature of this huge galaxy is a dark brim of dust that circles the disk galaxy’s center. A much longer exposure, however, brings up a hairy past where a bright, hazy halo is revealed that extends well past the central disk and contains many unresolved stars. Surprisingly, in this stellar haze, structures can be seen that include a diagonal ring. These structures and tidal streams provide fresh evidence that M104 had a violent past and is surely the result of collisions and mergers of smaller galaxies. Light takes about 30 million years to reach us from the Sombrero galaxy, which fully spans about 150 thousand light years across. The featured image was taken over seven days in mid-2026 from Namibia.

Your Sky Surprise: What picture did APOD feature on your birthday? (post 1995)
Tomorrow’s picture: a smile

Date October 5, 2026
Credit & Copyright Engelbert Vollmer
Authors & editors: Robert Nemiroff, Jerry Bonnell, Cecilia Chirenti, Keighley Rockcliffe
A service of: ASD at NASA / GSFC,
NASA Science Activation & Michigan Tech. U.

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