Russian Soyuz MS-28 Crew Spacecraft Arrival | International Space Station
Image Date: Nov. 27, 2025
Release Date: Dec. 2, 2025
Friends of NASA (FoN) is an independent non-governmental organization (NGO) dedicated to building international support for peaceful space exploration, commerce, scientific discovery, and STEM education.
Russian Soyuz MS-28 Crew Spacecraft Arrival | International Space Station
Shenzhou-20 Spacecraft to Make Uncrewed Return to Earth | China Space Station
After a potential space debris impact, the Shenzhou-20 spacecraft, currently docked with China's space station, will make an uncrewed return to Earth, according to Ji Qiming, a project spokesperson with the country's crewed space program.
Following a suspected debris strike on Shenzhou-20's viewport, the three astronauts originally scheduled to return to Earth aboard the spacecraft were redirected to Shenzhou-21, which brought them home safely on Nov. 14, 2025.
China launched the Shenzhou-22 on Nov. 25 to provide a new return vehicle for the orbiting crew— completing the first emergency launch in the history of its crewed space program.
During a subsequent spacewalk, the Shenzhou-21 crew, who are now undertaking a six-month orbital stay, may be tasked with inspecting the cracked viewport. They may also perform protective work on it using specialized devices delivered by the Shenzhou-22 launch—a procedure still being validated in ground tests, said Ji in a interview with China Media Group (CMG).
A day prior to their planned return on Nov. 5, the Shenzhou-20 crew spotted an anomaly on the viewport's edge—a triangular, paint-like mark. They photographed it from multiple angles and under different lights, while the station's robotic arm cameras were employed to take supplemental external pictures.
"We eventually reached a consensus: there must have been a crack, a penetrating one that had gone through the glass, from the inner surface to the outer surface," said Jia Shijin, chief designer of the crewed spacecraft system from the China Academy of Space Technology.
After this initial investigation, ground teams conducted extensive simulations and tests, and commissioned two research institutions to perform wind tunnel tests for independent verification, Jia revealed.
In a worst-case scenario, the cracks could spread, causing the outer pane to detach, with this leading to the failure of the inner pressure-sealing glass, resulting in cabin depressurization and the ingress of high-speed gases, Jia explained.
He said that further and more detailed investigation will be conducted after the return of the Shenzhou-20 spacecraft.
"Through our initial assessment of the crack, we believe the space debris is less than one millimeter in size, but moving at a very high speed. The entire crack is over 10 millimeters in size. From one corner, it looks like it has been pierced through. But as the spacecraft is still in orbit, we can't see it with our own eyes. We may be able to observe it more closely after the Shenzhou-20 spacecraft returns," Jia said.
Following the principle of astronaut safety first, China opted for the historic alternative return and emergency launch procedures.
Ji said that Shenzhou-20's uncrewed return mission will generate meaningful real-world experimental data for subsequent missions.
Four mice traveled to space aboard Shenzhou-21 spacecraft. They were initially scheduled for a 5-to-7-day experiment on orbit, but instead stayed for about two weeks before returning with the Shenzhou-20 crew, according to Wu Dawei from the China Astronaut Research and Training Center. All mice returned in healthy condition, Wu said.
With the emergency launch of Shenzhou-22, the development of subsequent spacecraft has been accelerated across the board. Shenzhou-23, originally scheduled for delivery in March next year, is expected to be completed two months ahead of schedule; Shenzhou-24 is also being pushed forward with full force, aiming for delivery next summer.
As the astronaut crew number usually matches with that of the spacecraft mission, the next crew will be named "Shenzhou-23 astronaut crew", meaning that the "Shenzhou-22 astronaut crew" will remain permanently vacant in the sequence.
"This serves as a reminder to the entire project: we should never assume our work is perfect. For crewed spaceflight, the work is never ending; perfection is our eternal goal, and we must continuously strive towards it. Even if we have done our utmost, there are still uncertainties from the space environment. I think this serves as a warning to everyone," he said.
NASA Artemis III Moon Rocket Liquid Oxygen Tank for Core Stage | NASA Michoud
Move crews at NASA’s Michoud Assembly Facility in New Orleans, Louisiana, move the liquid oxygen tank for the core stage of the agency’s Artemis III mission into the facility’s vertical assembly building on Nov. 3, 2025. Teams with Space Launch System (SLS) prime contractor, Boeing, later lifted the tank into the production cell currently housing the intertank to mate the flight hardware together before capping them off with the forward skirt to complete the core stage forward join.
The propellant tank is one of five major elements that make up the 212-foot-tall rocket stage. The core stage, along with its four RS-25 engines, produce more than two million pounds of thrust to help launch NASA’s Orion spacecraft, astronauts, and supplies beyond Earth’s orbit and to the lunar surface for Artemis.
Moon Shadows on Planet Saturn | Hubble Space Telescope
Saturn's wide, but very thin, rings are tilted with respect to its plane of orbit around the Sun. Once every 15 years, the rings are edge-on (perpendicular) to the Sun. During those times, Saturn's moons can cast shadows across the rings.
This time-lapse video shows the icy moons Enceladus, Mimas, Dione, and Tethys orbiting Saturn. Enceladus, seemingly chased by Mimas, is first to speed past the rings and in front of the planet. Both moons cast small shadows on the planet, but only Enceladus casts a shadow on the rings. The orbit of Mimas is inclined so that its shadow misses the rings. Dione is next, and its long shadow also tracks across the ring system. As the three moons move across Saturn's disk, the viewer catches a fleeting view of Tethys as it moves behind the planet on the right.
The 30-second movie is created from Hubble images taken over a 9½-hour span. The images were taken Nov. 17, 1995, with Hubble's Wide Field and Planetary Camera 2. The video has a standard aspect ratio, but is presented within a widescreen frame—the black bars along the sides are normal.
Mediterranean & Africa Flyover: History in Lights | International Space Station
NASA Astronaut Don Pettit: "Orbiting the Mediterranean, from Europe into Africa. So much human history to see in the lights!"
This video from low-Earth orbit was captured by experienced NASA astronaut and former Expedition 71/72 flight engineer, Don Pettit. NASA astronaut Don Pettit returned to Earth on April 19, 2025, concluding a seven-month science mission aboard the International Space Station. Pettit spent 220 days in space, earning him a total of 590 days in space over the course of his four spaceflights. He orbited the Earth 3,520 times, traveling 93.3 million miles in low-Earth orbit.
Stellar Pre-Winter Seasonal Offerings | NASA's Chandra X-ray Observatory
Four images that one can imagine connections to fall have been released by NASA’s Chandra X-ray Observatory. The images are the star-forming region NGC 6334, supernova remnant G272.2-0.3, interacting spiral galaxies NGC 2207 and IC 2163, as well as R Aquarii. Each image contains X-rays from Chandra that have been combined with data from other telescopes that detect different types of light. Pareidolia is the phenomenon that allows people to see familiar patterns or shapes in data. Before fall gives way to winter in the northern hemisphere, NASA’s Chandra X-ray Observatory has several images that celebrate autumn and its many delights to share. In spirit of the season, this collection gathers Chandra data with those from its telescopic family including NASA’s James Webb, Hubble, and Spitzer Space Telescopes, plus others in space and on the ground.
A First: All Docking Ports Used for Eight Spacecraft | International Space Station
For the first time in International Space Station history, all eight docking ports aboard the orbital outpost are occupied following the reinstallation of Northrop Grumman’s Cygnus XL cargo spacecraft to the Earth-facing port of the station’s Unity module. The eight spacecraft attached to the complex are: two SpaceX Dragons, Cygnus XL, JAXA’s (Japan Aerospace Exploration Agency) HTV-X1, two Roscosmos Soyuz crew spacecraft, and two Progress cargo ships.
This milestone follows the reattachment of the Cygnus XL spacecraft, supporting the Northrop Grumman-23 commercial resupply services mission for NASA. It was removed last week by the robotics officer at the agency’s Mission Control Center in Houston using the space station’s Canadarm2 robotic arm. The Cygnus XL movement was coordinated between NASA, Northrop Grumman, and Roscosmos to provide appropriate clearance for the arriving crewed Soyuz MS-28 spacecraft on Nov. 27, 2025.
Cygnus will remain attached to the orbiting laboratory until no earlier than March 2026, when it is scheduled to safely depart and dispose of up to 11,000 pounds of trash and unneeded cargo when it harmlessly burns up in Earth’s atmosphere.
Three new residents are living aboard the space station following the arrival of the Soyuz MS-28 spacecraft on Thursday, Nov. 27, 2025. NASA astronaut Chris Williams and Roscosmos cosmonauts Sergey Kud-Sverchkov and Sergei Mikaev will stay in space until July 2026, conducting advanced space research benefiting humans living on and off Earth.
On Dec. 8, the orbital outpost will return to seven members and become the Expedition 74 crew when NASA astronaut Jonny Kim and Roscosmos cosmonauts Sergey Ryzhikov and Alexey Zubritsky enter the Soyuz MS-27 spacecraft, undock from the Prichal module, and parachute to a landing in Kazakhstan. Kim, Ryzhikov, and Zubritsky are nearing the end of an eight-month space science mission that began on April 8, 2025.
China Unveils Next-gen Space Situational Awareness Constellation for Space Debris
High above Earth, an estimated 140 million tiny debris fragments, a portion as small as 1 to 10 millimeters, race through orbit at several kilometers per second. And larger pieces, those over 10 centimeters, now number more than 50,000.
With tens of thousands of satellites going up, space is becoming crowded.
Unlike ground-based radars or telescopes, this space-based constellation or EYESAT is not limited by geography or weather. Once they reach 156 satellites, they will be capable of monitoring the entire orbital environment, including orbits above remote regions like the South Pole. When fully deployed, EYESAT is expected to become one of the world's largest space-based debris-tracking systems. EYESAT will detect, track, identify and catalog on-orbit satellites, while also monitoring space debris. The data services for space traffic management from EYESAT will help safeguard near-Earth space and improve long-term sustainability.
EYESAT satellites are scheduled for launch beginning in the first half of 2026.
Stellar Pre-Winter Seasonal Offerings | NASA's Chandra X-ray Observatory
Before fall gives way to winter in the northern hemisphere, NASA’s Chandra X-ray Observatory has several images that celebrate autumn and its many delights to share. In spirit of the season, this collection gathers Chandra data with those from its telescopic family including NASA’s James Webb, Hubble, and Spitzer Space Telescopes, plus others in space and on the ground.
Here is a sample of the seasonal offerings that space has in store:
For many, nothing evokes fall more than fallen leaves. In this view of NGC 6334, glowing pockets of dust and gas in the nebula resemble leaves that have been picked up by a wind gust. This region is indeed home to strong winds blowing from the young stars that have formed there. This image contains X-ray data from Chandra (blue, green, and yellow) that shows the effects of these winds, which have been combined with infrared data from the now-retired Spitzer Space Telescope (red, brown), which shows the dust and gas that fuels the growing stars.
Born after a violent explosion of a star, this cosmic gourd is the supernova remnant G272.2-03.2. X-ray observations from Chandra provide evidence that G272 is the result of a Type Ia supernova explosion, where a white dwarf star pulls material from a companion star until it triggers a thermonuclear explosion and obliterates the star. The inside of the “pumpkin” is superheated gas that is filling the space cleared out by the explosion as it moves outward.
A cornucopia is a horn-shaped basket that traditionally carries fruits and vegetables. There is nothing edible in this pair of galactic cornucopias but there are a bounty of stars, dust, and other ingredients that make up these two spiral galaxies, known as NGC 2207 and IC 2163, that we see face-on. This view of NGC 2207 and IC 2163 takes a James Webb infrared image and adds the X-ray view from Chandra. Together, it is quite an eye-catching result.
Multiple telescopes teamed up to capture an image that looks like a cozy sweater with fuzzy arms. X-rays from Chandra and ESA’s XMM-Newton, optical light data from Hubble and the Very Large Telescope in Chile, and an optical [PE1] image from an astrophotographer combine to reveal R Aquarii. Nestled within the cozy ‘body’ of R Aquarii is a pair of stars where a white dwarf is pulling material from a much larger red giant companion. When enough material accumulates on the surface of the white dwarf, it triggers an outburst that sends a jet out into space. Over time, these jets twist and loop around each other weaving the structure seen today.
What's Up for December 2025: Skywatching Tips from NASA | JPL
Here are examples of skywatching highlights for the northern hemisphere in December 2025:
The 3I/ATLAS comet makes its closest approach to Earth, the Geminid meteor shower sparkles across the sky, and the Moon and Jupiter get close for a conjunction.
0:00 Intro
0:13 3I/ATLAS
1:24 Geminid meteor shower
1:57 Moon + Jupiter conjunction
2:31 December Moon phases
#NASA #Astronomy #Space #Science #Comets #InterstellarComets #Comet3IATLAS #Planets #Jupiter #Earth #MeteorShowers #Geminids #Moon #Stars #SolarSystem #Nebulae #Galaxies #Constellations #MilkyWayGalaxy #Skywatching #JPL #Caltech #UnitedStates #Canada #Mexico #NorthernHemisphere #STEM #Education #HD #Video
United Launch Alliance (ULA) Rocket Factory Tour in Alabama
The Vulcan rocket's journey to space begins in Decatur, Alabama, USA, at the United Launch Alliance’s 2.2 million square foot rocket factory. Long before the path to orbit, the missions start on the factory floor.
The Tails of Interstellar Comet 3I/ATLAS: View from Texas
How typical is our Solar System?
Studying 3I/ATLAS, a comet just passing through, is providing clues. Confirmed previous interstellar visitors include an asteroid, a comet, a meteor, and a gas wind dominated by hydrogen and helium. Comet 3I/ATLAS appears relatively normal when compared to Solar System comets, therefore providing more evidence that our Solar System is a somewhat typical one. For example, Comet 3I/ATLAS has a broadly similar chemical composition and ejected dust. The featured image was captured last week from Texas and shows a green coma, a wandering blue-tinted ion tail likely deflected by our Sun's wind, and a slight anti-tail, all typical cometary attributes. The comet, visible with a telescope, passed its closest to the Sun in late October and will pass its closest to the Earth in mid-December. Afterwards, it will return to interstellar space and never return.
Image Description: A starfield is shown around a comet. The green coma of the comet is on the lower left. A meandering blue-tinted tail goes off to the upper right. A slight anti-tail is seen from the coma toward the lower left.
Starburst Spiral Galaxy NGC 1792 in Columba | European Southern Observatory
Color composite image of the starburst spiral galaxy NGC 1792 obtained with the FORS1 and FORS2 multi-mode instruments (at the Very Large Telescope MELIPAL and YEPUN, respectively). It is located over 50 million light-years from Earth in the constellation Columba (the Dove).
The optical appearance of NGC 1792 is quite chaotic, due to the patchy distribution of dust throughout the disc of this galaxy. It is very rich in neutral hydrogen gas—fuel for the formation of new stars—and is indeed rapidly forming such stars. The galaxy is characterized by unusually luminous far-infrared radiation; this is due to dust heated by young stars. Note the numerous background galaxies in this sky field. North is up and East is to the left.
#NASA #ESO #Astronomy #Space #Science #Stars #Galaxies #Galaxy #NGC1792 #SpiralGalaxies #StarburstGalaxies #Columba #Constellations #Cosmos #Universe #VLT #FORS2 #ParanalObservatory #Chile #SouthAmerica #Europe #STEM #Education
Spiral Galaxy NGC 1792 in Columba: A Storm of New Stars | Hubble
NGC 1792 is just as fascinating to astronomers as its chaotic look might imply. Classified as a starburst galaxy, it is a powerhouse of star formation with spiral arms rich in star-forming regions. In fact, it is surprisingly luminous for its mass. The galaxy is close to a larger neighbor, NGC 1808, and the strong gravitational interaction between the two is believed to be what has stirred up the reserves of gas in this galaxy. The result is a torrent of star formation, concentrated on the side where gravity has a stronger effect. It is a perfect target for astronomers seeking to understand the complex interactions between gas, star clusters and supernovae in galaxies.
Hubble provided an image of this galaxy in 2020. This image includes additional data collected throughout 2025, providing a deeper view of the tumultuous astrophysical activity taking place in the galaxy. Blossoming red lights in the arms mark out so-called H-alpha emission from dense clouds of hydrogen molecules. Stars form within these clouds and shine powerfully with ultraviolet radiation. They ionize the gas around them, causing the gas to emit a very particular red wavelength of light—a tell-tale sign of new stars.
Image Description: A spiral galaxy, seen partly from the side, with a messy, turbulent appearance. Its disc is made of multiple patchy arms that contain numerous sparkling blue and glowing red regions—star clusters and star-forming nebulae. Thick clumps of dark reddish dust swirl through the disc. The glow of the disc extends out into the dark background, where both distant and nearby stars can be seen.
#NASA #Astronomy #Hubble #Space #Science #Stars #Galaxies #Galaxy #NGC1792 #SpiralGalaxies #StarburstGalaxies #Columba #Constellations #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #ESA #Europe #STEM #Education
Shenzhou-21 Astronauts Conduct Science Experiments & Drills | China Space Station
The Shenzhou-21 crew members aboard China's Tiangong Space Station carried out multiple science experiments and their first full-system emergency response drills, among other tasks, in orbit over the past week.
The three astronauts—Zhang Lu, Wu Fei, and Zhang Hongzhang—have been in orbit for a month as of Sunday, November 30, 2025.
Using laptops aboard the space station, the astronauts conducted microgravity experiments on intuitive physical behavior, collecting relevant behavioral data to explore the impact of long-term spaceflight on human's intuitive physical representations and the mechanisms of their recovery.
They used space Raman spectrometer to analyze metabolic components in urine samples. The collected information will be used for further refinement and improvement of the relevant characteristic metabolite indicator system and evaluation criteria.
Additionally, the crew completed the installation of new software for space medical experiments. In microgravity physics science, the crew completed scheduled tasks including replacing the high-speed image storage unit in the two-phase system experiment cabinet and disassembling and assembling experimental modules.
Additionally, per experimental schedule, they cleaned and replaced samples within the containerless cabinet's experimental chamber, cleaned window cover lenses and conducted other relevant mission tasks.
The crew also conducted their first full-system emergency pressure response drills in orbit as planned. This simulated the full emergency response process for an internal depressurization scenario, reinforcing and enhancing the crew's emergency handling capabilities and ground-space coordination.
In equipment inspection and maintenance, the crew performed patrols of the cryogenic storage units and the minus 80-degree space refrigerator, checked pressures in the environmental control gas cylinder, and conducted maintenance on the regenerative life support system equipment.
In station management, the crew organized supplies and cleaned the cabin, keeping their orbiting home tidy. In addition, they underwent multiple medical examinations, including non-invasive cardiac function tests, providing data for ground teams to closely monitor their health in orbit.
Shenzhou-21 Crew
Zhang Lu (张陆) - Commander & Pilot - 2nd spaceflight
Wu Fei (武飞) Flight Engineer - 1st spaceflight
Zhang Hong Zhang (张洪章) - Payload Specialist - 1st spaceflight
Video Credit: CCTV
Duration: 1 minute, 29 seconds
Release Date: Nov. 30, 2025
A 'Double Helix' Lunar Eclipse with Zodical Light & The Milky Way over China
This image was timed to capture a total lunar eclipse—but it came with quite a twist. First, the eclipse: the fully Earth-shadowed Moon is visible as an orange orb near the top. The eclipsed Moon's orange color is caused by a slight amount of red light scattered first by Earth's atmosphere, adding a color like a setting Sun. Now, the twist: one of the apparent double helix bands is the Milky Way, the central disk of our home galaxy. The second band is zodiacal light, sunlight scattered by dust within our Solar System. The reason they cross is because the plane where dust orbits our Sun is tilted relative to the plane where stars orbit our Galaxy. This well-known tilt is shown dramatically in the featured wide-angle Mercator-projected picture, spanning from horizon to horizon, captured in early September from Mingantu Observing Station in China's Inner Mongolia Autonomous Region.
Zodiacal light is produced by starlight reflecting off of dust orbiting our Sun. At certain times of the year, a band of sun-reflecting dust from the inner Solar System appears prominently just after sunset—or just before sunrise—and is called zodiacal light. Although the origin of this dust is still being investgated, a leading hypothesis holds that zodiacal dust originates mostly from faint Jupiter-family comets and that it slowly spirals inwards toward the Sun.
Image Description: A wide angle image of the night sky is punctuated by a radio telescope on the lower left. Two bands of light run through the sky—the Milky Way and zodiacal light. The bands intertwine like a double helix. Near the top is an orange orb that is a totally eclipsed moon.