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Webb Sees Turbulent Star Nursery

A nebula made of clouds of gas and dust with stars forming within. In the center and out to the left it is filled with thin, wispy blue gas that forms delicate layers. Around this are thicker orange clouds with dark ridges. Thin red filaments of gas cross the center of the nebula. Glowing bubbles in the gas contain dense, very bright clusters of stars. In the edges, distant stars are visible as bright points on a dark background.
ESA/Webb, NASA & CSA, E. Sabbi, M. Zamani (ESA/Webb); Acknowledgement: M. H. Özsaraç

In this Webb image released on Oct. 22, 2026, we see a turbulent cauldron of star formation filled with dense clumps of gas. This region is named N159 and is located 161,000 light-years away in the Large Magellanic Cloud, one of the satellite galaxies orbiting the Milky Way galaxy.

This region has a lower metallicity (proportion of elements that are heavier than helium and hydrogen) than the Milky Way, giving astronomers an opportunity to learn more about conditions found in the early universe and how stars formed under those conditions.

Read more about N159.

Image credit: ESA/Webb, NASA & CSA, E. Sabbi, M. Zamani (ESA/Webb); Acknowledgement: M. H. Özsaraç

NASA’s Neo Surveyor Sunshade

A technician in a white clean room gown and face mask shines a flashlight to inspect the dark, patterned cells of a large spacecraft solar array inside a clean room.
BAE Systems Space & Mission Systems

A technician inspects the large sunshade of NASA’s Near-Earth Object (NEO) Surveyor mission in this image released on Oct. 26, 2026. The sunshade structure, which stands 20 feet (6 meters) tall and measures 8 feet (2.4 meters) wide at its base, will keep the infrared space telescope cool as it searches for near-Earth asteroids and comets while also providing the spacecraft with power.

When in space, NEO Surveyor will detect some of the hardest-to-find asteroids and comets, some of which may be located in the direction of the Sun — a region of sky where ground-based optical telescopes have a harder time searching.

Read more about the sunshade and NEO Surveyor.

Image credit: BAE Systems Space & Mission Systems

NASA’s X-59 Aircraft and Test Pilot

NASA test pilot Mike Lippert stands on a gray metal ladder before getting into the X-59 plane. He is holding his helmet under his right arm. The cockpit of the plane is open.
NASA/Carla Escamilla

NASA test pilot Mike Lippert poses for a photo ahead of his first time flying the agency’s X-59 quiet supersonic research aircraft on Oct. 21, 2026. The X-59 has flown numerous times since its inaugural flight in November 2025; its first supersonic flight was on June 5, 2026.

Lippert took off from NASA’s Armstrong Flight Research Center in Edwards, California, and landed one hour later. The flight came after scheduled maintenance and a review of the X-59’s systems following the aircraft’s busiest week of testing to date.

Read more about Lippert and the Oct. 21 flight.

Image credit: NASA/Carla Escamilla

RS-25 Engine Tests at NASA Stennis

A massive cloud of white vapor billows out from a structure where an RS-25 engine is firing. The flames are just barely visible through the structure. In the foreground is a body of water.
NASA/Danny Nowlin

Teams at NASA’s Stennis Space Center near Bay St. Louis, Mississippi tested RS-25 engine No. 10001 on Oct. 21, 2026. The hot fire test lasted for almost eight-and-a-half minutes (500 seconds), the same amount of time RS-25 engines fire during launch of NASA’s SLS (Space Launch System) rocket, with a 111% power level. For each Artemis mission, four RS-25 engines produce up to 2 million pounds of combined thrust to help launch the SLS rocket.

Prior to use, all RS-25 engines are proven flightworthy at NASA Stennis. While this developmental engine will not be used in flight, the hot fire test provides NASA and NASA’s prime engine contractor L3Harris Technologies with the capability to capture critical data to improve engine performance and reliability.

Image credit: NASA/Danny Nowlin

Spiral’s Edge

An edge-on spiral galaxy. Its rusty-brown dust lanes bisect the galaxy lengthwise. Bright-blue points dot the galaxy and seem to be more dense on its left side. A bright foreground star shines just to the left of the galaxy's center. The background is black and dotted with distant galaxies and a smattering of foreground stars, which are easily identified by their diffraction spikes.
NASA, ESA, Michael Jones (California Institute of Technology); Image Processing: Gladys Kober (NASA/Catholic University of America)

This NASA Hubble Space Telescope image released on Oct. 16, 2026, features the edge-on, intermediate spiral galaxy NGC 1827, located roughly 37 million light-years away in the constellation Columba, the Dove. Hubble captured the image as part of a survey looking at 260 satellite galaxies around 22 Milky Way-like host galaxies within a radius of about 32 million light-years from Earth. Low-mass galaxies like the ones in this Hubble observing program provide a way to test the predictions of cosmological models on small scales, which struggle to match observations.

Image credit: NASA, ESA, Michael Jones (California Institute of Technology); Image Processing: Gladys Kober (NASA/Catholic University of America)

Science on the Space Station with NASA Astronaut Jessica Watkins

NASA astronaut Jessica Watkins looks up at the camera while doing a science experiment. Her arms and hands are inside a rectangular glovebox that we can see inside. Her arms are covered with the white gloves that are attached to the glovebox and she is wearing blue gloves.
NASA/Anil Menon

NASA astronaut and Expedition 75 flight engineer Jessica Watkins works inside the Kibo laboratory module’s Life Science Glovebox on Oct. 9, 2026, safely mixing living cell samples with a bioink and then filling a special cartridge with the cell‑ink mixture.

The advanced research operations were part of the InSPA‑Auxilium Bioprinter‑Cell Printing investigation, which explores 3D bioprinting cartilage tissue in microgravity of higher quality than that produced on Earth. Results may advance the ability to biomanufacture cartilage, benefiting patients on Earth and crew members on long‑duration space missions.

Image credit: NASA/Anil Menon

Webb Captures Stellar Jets

A young star cluster filled with many stars that display Webb’s unique eight-pronged diffraction pattern. At its center is a yellow star which sports the largest diffraction pattern. To the left of the star, there is a region filled with yellow dust and gas that extends from the star to the left border of the image. This yellow region extends from the bottom, covering about two-thirds of the image. The yellow region has several blue stars of different sizes embedded within. The top third, which lies outside of the yellow region, holds a few bright protostars, within dense gray gas. Those stars illuminate the gas, making it appear blue. A few red outflows from other protostars are visible above this grayish-blue region. To the right of the central star, there is a clumpy, flame-like plume of red dust and gas with protostars that emit a soft white light within. The plume is surrounded by more dense gray gas and dust. There are several background galaxies strewn throughout the image.
NASA’s James Webb Space Telescope has revealed many protostars and stars within the glowing gases of NGC 7129. Hot, atomic hydrogen gas is shown here in the golden region, while cooler, molecular hydrogen gas, shocked by embedded protostars, is represented in red.
NASA, ESA, CSA, STScI; Image Processing: Alyssa Pagan (STScI)

An image from NASA’s James Webb Space Telescope released on Oct. 6, 2026, reveals a cauldron of cosmic creation. Webb has unveiled numerous stars formerly hidden by clouds of dust in a stellar nursery known as NGC 7129, which resides about 3,300 light-years from Earth.

Learn more about this region – and tour it in an interactive experience.

Image credit:  NASA, ESA, CSA, STScI; Image Processing: Alyssa Pagan (STScI)

Martian Dawn

A stark, grayish-tan Martian landscape features jagged rock formations and rolling mountain ridges beneath a pale, hazy sky.
NASA/JPL-Caltech/MSSS

NASA’s Curiosity captures the dawn on Mars – as well as elongated ridges formed by wind erosion, or yardangs – in this close-up from a panorama released on Oct. 6, 2026. This is the most detailed view yet of distant, wind-carved Martian cliffs, highlighting features the mission’s scientists have long been waiting to see up close.

The panorama was captured by Curiosity’s Mastcam on Aug. 11, the 4,982nd Martian day, or sol, of the mission, and comprises six individual images that were stitched together after being sent to Earth.

Image credit: NASA/JPL-Caltech/MSSS

Artemis II Heat Shield After Splashdown

The Orion spacecraft's heat shield dominates this underwater photo. Due to the water, the heat shield appears to be teal-colored.
US Navy

Shortly after NASA’s Artemis II mission splashed down on April 10, 2026, U.S. Navy divers captured underwater imagery of the Orion spacecraft’s heat shield. In the months after, the agency measured whether the thermal protection system effectively safeguarded the crew and Orion systems as the spacecraft reentered Earth’s atmosphere. This rigorous analysis confirmed that the heat shield performed as expected.

Learn how Orion’s heat shield was examined.

Image credit: US Navy

Chandra Finds Possible Origin of ‘Treble Clef’ Waves

A composite image of a remarkable radio wave formation that strongly resembles a treble clef musical symbol, hovering in the midst of two colliding galaxy clusters. Here, galaxies in the galaxy clusters, plus foreground and background stars and galaxies, blanket the image with specks of light set against the blackness of space. At the center of the frame is a large, oval, blue-purple cloud with ragged edges. In the middle of the purple field, tilting slightly to our left, is what appears to be a giant treble clef, loosely drawn with a neon pink marker. Like the musical notation for which it's named, the formation has a strong vertical stroke with a continuous, fluid line swooping back and forth as it moves from top to bottom.
X-ray: NASA/CXC/INAF-IRA/A. Botteon et al.; Infrared: UKIDSS-GPS ; Radio: ASTRON/LOFAR; Image processing: NASA/CXC/SAO/N. Wolk

A formation of radio waves looks remarkably like a treble clef in this Oct. 14, 2026, image from NASA’s Chandra X-Ray Observatory. Researchers used Chandra to find that the Treble Clef is likely caused by an outburst from a supermassive black hole, followed by a collision of two galaxy clusters.

Read more about this discovery.

Image credit: X-ray: NASA/CXC/INAF-IRA/A. Botteon et al.; Infrared: UKIDSS-GPS ; Radio: ASTRON/LOFAR; Image processing: NASA/CXC/SAO/N. Wolk

NASA’s Space X CRS-35 Launch Jellyfish

The exhaust plumes of a SpaceX Falcon 9 rocket carrying the company’s Dragon spacecraft are seen illuminated by sunlight against the predawn sky.
NASA/John Kraus

Sunlight illuminates the exhaust plumes of a SpaceX Falcon 9 rocket carrying the company’s Dragon spacecraft on Oct. 13, 2026. This visual phenomenon is known as a “jellyfish”; it happens near sunrise or sunset when the exhaust plume from the rocket becomes brightly illuminated, creating a glowing shape resembling a jellyfish.

The mission lifted off at 6:33 a.m. EDT from Space Launch Complex 40 at Cape Canaveral Space Force Station, carrying scientific investigations, supplies, and equipment to the International Space Station on SpaceX’s 35th commercial resupply services mission for NASA. The rocket’s exhaust plumes were visible across the eastern United States.

Watch the uncrewed Dragon spacecraft rendezvous with and dock to the International Space Station on Oct. 15. Coverage begins at 9:15 a.m. EDT.

Image credit: NASA/John Kraus

Transporter-18 SmallSats Encapsulation

View of a SpaceX payload fairing interior showing mounted satellites and hardware arranged along the center structure, surrounded by the curved black fairing walls.
SpaceX

Three NASA-supported small spacecraft, along with many commercial payloads, are shown before being encapsulated in a SpaceX Falcon 9 ahead of launch on Oct. 1, 2026. The ASCENT Propulsion Dual Mode CubeSat, the Supernova Remnants and Proxies for ReIonization Testbed Experiment (SPRITE) CubeSat, and the Small Spacecraft Propulsion and Inspection Capability (SSPICY) mission will demonstrate new propulsion technologies, study how galactic dust and high-energy radiation move through galaxies, and advance capabilities for inspecting inactive satellites.

Image credit: SpaceX

Cosmic House of Mirrors

A massive galaxy cluster, made of many golden elliptical galaxies with the largest, brightest one in the center. Heavily distorted orange galaxies appear all around the cluster, the largest concentrated in a large arc around the cluster's center; these are images of very distant galaxies, created by gravitational lensing. A few galaxies are large and bluish-white in color; bright, nearby stars are the same color.
ESA/Webb, NASA & CSA, L. Furtak, S. Fujimoto

Galaxies warp and multiply as if in a house of mirrors in this image from NASA’s James Webb Space Telescope released on Sept. 29, 2026.

The brilliant golden galaxies seen here are part of a galaxy cluster called MACS J0454.1-0300. The orange galaxies bunched together on one side of the image, however, are not actually part of the cluster, but rather galaxies much farther away whose light has been bent and magnified by gravitational lensing. This phenomenon occurs when the enormous mass of a foreground object such as a galaxy cluster bends and magnifies the light from a more distant object in the background.

Learn more about this galaxy cluster.

Image credit: ESA/Webb, NASA & CSA, L. Furtak, S. Fujimoto

Crew-12 Returns to Earth

A cone-shaped spacecraft and the four large parachutes attached to it against a backdrop of fluffy white clouds in the sky.
NASA/Keegan Barber

The SpaceX Crew Dragon Freedom spacecraft is seen moments before splashing down in the Pacific Ocean off the coast of California in this Oct. 8, 2026, photograph. Aboard were NASA’s SpaceX Crew-12 members NASA astronauts Jessica Meir and Jack Hathaway, ESA (European Space Agency) astronaut Sophie Adenot, and Roscosmos cosmonaut Andrey Fedyaev. The four spent nearly eight months aboard the International Space Station.

See more photos from splashdown.

Image credit: NASA/Keegan Barber

Artemis II Crew Moon Photo Annotations

A simulated image of the crew’s view of the dark, eclipsed Moon on April 6, 2026. Three crew members annotated impact flashes on this image in OneNote. Reid Wiseman wrote in blue. Victor “Ike” Glover wrote in green. Jeremy Hansen wrote in red. General annotations are in purple ink. A note on the left side in purple is “circled likely same impacts.” Five impact flashes are numbered across the Moon. #1 with a blue dot (observed by Wiseman) is located at the 4 o’clock position, but more central. #2 is circled with a red dot (observed by Hansen) and a blue dot (observed by Wiseman) is located at the 8’clock position, but near the Moon’s center. #3 with a red dot (observed by Hansen) is located at 3 o’clock. #4 is circled with a red dot (observed by Hansen), a blue dot (observed by Wiseman), and a green dot (observed by Glover). It is at the 6 o’clock position. A note of “(later)” is under #4. #5 with a blue dot (observed by Wiseman) is located at the 12 o’clock position. A note of “towards end” is to the right of #5. Wiseman wrote an additional note in blue: “these three roughly 10 min into eclipse.” The three indicated are the blue dots at #1, #2, and #4.
NASA

A visualization of a dark Moon eclipsing the Sun is marked with handwritten notes in this April 6, 2026, screenshot from an Artemis II crew member’s tablet.

NASA astronauts Reid Wiseman (in blue) and Victor “Ike” Glover (in green) and CSA (Canadian Space Agency) Jeremy Hansen (in red) observed impact flashes and their locations, which are noted on the image. Overall, the astronauts reported seeing five extremely faint “pinprick” bursts of light from their view aboard Orion, which was 46,000 miles away from the Moon at the time. These flashes are sparked by rocky fragments hitting the Moon.

From April 1 through April 10, 2026, NASA’s Artemis II crew traveled to the Moon and back and along the way, captured stunning imagery and scientific observations of our nearest neighbor. Now, the full lunar science dataset from their journey is available to the global science community, and to the public, for further study. Read about the report, listen to crew audio observations, and explore more.

Image credit: NASA

Astronomers Solve Cosmic Cold Case with NASA Hubble Data

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.
NASA, ESA, Leah Hustak (STScI)

Diligent sleuthing by astronomers uncovered a surprising chemical clue that indicates the white dwarf star HS 0209+0832 may host a second-generation planet. This artist’s concept released on Oct. 5, 2026, depicts that possible explanation.

The white dwarf is the “dead” core of a star that burned through all of its nuclear fuel and lost its outer envelope of gas and dust to space. The second-generation planet formed from that cast-off gas and dust, which is why its chemical content is very different from a planet that formed as its host star was forming.

Learn more about this scientific discovery.

Image credit: NASA, ESA, Leah Hustak (STScI)

NASA Astronaut Christina Koch at Eagles vs. Rams

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’s DAVINCI Probe Can Stand the Heat

An engineering model of the DAVINCI descent probe.
An engineering model of NASA’s DAVINCI (Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging) descent probe passed a key test that ran from Aug. 28 to Sept. 10, showing it can survive the extreme temperatures of Venus.
NASA/Mike Guinto

The engineering development unit for NASA’s DAVINCI (Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging) probe is photographed prior to a major thermal evaluation.

The DAVINCI team put the yoga ball-sized vessel into a ceramic-lined chamber with heat-scorched walls and ratcheted up the temperature to 869 F, or 465 C, over the course of about an hour — the same pace the probe will heat up during its descent to the surface of Venus.

DAVINCI will study the origin, evolution, and present state of Venus in unprecedented detail to help determine whether it was once wet and habitable, like Earth.

Read more about the test.

Image credit: NASA/Mike Guinto

NASA’s SpaceX Crew-13 Launches

A SpaceX Falcon 9 rocket carrying the company's Dragon spacecraft launches. There is a bright column of fire under the rocket as it moves upward. Clouds of vapor spread out below the rocket, almost blending into the similarly shaped clouds in the sky.
NASA/Joel Kowsky

In this Oct. 1, 2026, photo, a SpaceX Falcon 9 rocket and Dragon spacecraft launch from Space Launch Complex 40 at Cape Canaveral Space Force Station in Florida. The spacecraft is carrying NASA astronauts Jessica Watkins and Luke Delaney, CSA (Canadian Space Agency) astronaut Joshua Kutryk, and Roscosmos cosmonaut Sergey Teteryatnikov to the International Space Station for a long-duration science mission. They are expected to dock at the space station at 7 p.m. EDT.

NASA will stream Crew‑13’s arrival across multiple platforms. The agency’s live broadcast begins at 5:20 p.m. EDT. Learn where to watch at: https://www.nasa.gov/live

Learn more about the Crew-13 launch and mission.

Image credit: NASA/Joel Kowsky

Star Trails

Streaks of blue and yellow lights cover Earth. Above, faint streaks of light made by stars can be seen.
NASA/Anil Menon

This long-duration image shows star trails above Earth and the blue lights of fishing boats and the yellow lights of Indonesian cities stretching below the International Space Station as it orbited 258 miles above the Banda Sea on Sept. 20, 2026.

Image credit: NASA/Anil Menon

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