Wednesday, December 03, 2025

Electric Sparks Detected in Martian Dust Devils | NASA's Perseverance Mars Rover

Electric Sparks Detected in Martian Dust Devils | NASA's Perseverance Mars Rover

Three Martian dust devils can be seen near the rim of Jezero Crater in this short video made of images taken by a navigation camera aboard NASA’s Perseverance rover on Sept. 6, 2025.

NASA’s Perseverance Mars rover has recorded the sounds of electrical discharges—sparks —and mini-sonic booms in dust devils on planet Mars. Long theorized, the phenomenon has now been confirmed through audio and electromagnetic recordings captured by the rover’s SuperCam microphone. The discovery, published Nov. 26, 2025, in the journal Nature, has implications for Martian atmospheric chemistry, climate, and habitability, and could help guide the design of future robotic and human missions to Mars.

A frequent occurrence on the Red Planet, dust devils form from rising and rotating columns of warm air. Air near the planet’s surface becomes heated by contact with the warmer ground and rises through the denser, cooler air above. As other air moves along the surface to take the place of the rising warmer air, it begins to rotate. When the incoming air rises into the column, it picks up speed like spinning ice skaters bringing their arms closer to their body. The air rushing in also picks up dust, and a dust devil is born.

SuperCam has recorded 55 distinct electrical events over the course of the mission, beginning on the mission’s 215th Martian day, or sol, in 2021. Sixteen have been recorded when dust devils passed directly over the rover.

Decades before Perseverance landed, scientists theorized that the friction generated by tiny dust grains swirling and rubbing against each other in Martian dust devils could generate enough of an electrical charge to eventually produce electrical arcs. Called the triboelectric effect, the same phenomenon at play when someone walks over a carpet in socks and then touches a metal doorknob, generating a spark. In fact, that is about the same level of discharge as what a Martian dust devil might produce.

“Triboelectric charging of sand and snow particles is well documented on Earth, particularly in desert regions, but it rarely results in actual electrical discharges,” said Baptiste Chide, a member of the Perseverance science team and a planetary scientist at L’Institut de Recherche en Astrophysique et Planétologie in France. “On Mars, the thin atmosphere makes the phenomenon far more likely, as the amount of charge required to generate sparks is much lower than what is required in Earth’s near-surface atmosphere.”

Perseverance’s SuperCam instrument carries a microphone to analyze the sounds of the instrument’s laser when it zaps rocks, but the team has also captured the sounds of wind and even the first audio recording of a Martian dust devil. Scientists knew it could pick up electromagnetic disturbance (static) and sounds of electrical discharges in the atmosphere. What they did not know was if such events happened frequently enough, or if the rover would ever be close enough, to record one. Then they began to assess data amassed over the mission, and it did not take long to find the telltale sounds of electrical activity.

Crackle, pop

“We got some good ones where you can clearly hear the ‘snap’ sound of the spark,” said coauthor Ralph Lorenz, a Perseverance scientist at the Johns Hopkins Applied Physics Lab in Laurel, Maryland. “In the Sol 215 dust devil recording, you can hear not only the electrical sound, but also the wall of the dust devil moving over the rover. And in the Sol 1,296 dust devil, you hear all that plus some of the particles impacting the microphone.”

Thirty-five other discharges were associated with the passage of convective fronts during regional dust storms. These fronts feature intense turbulence that favor triboelectric charging and charge separation. This occurs when two objects touch, transfer electrons, and separate—the part of the triboelectric effect that results in a spark of static electricity.

Researchers found electrical discharges did not seem to increase during the seasons when dust storms that globally increase the presence of atmospheric dust, are more common on Mars. This result suggests that electrical buildup is more closely tied to the localized, turbulent lifting of sand and dust rather than high dust density alone.

Profound effects

The proof of these electrical discharges is a discovery that dramatically changes our understanding of Mars. Their presence means that the Martian atmosphere can become sufficiently charged to activate chemical reactions, leading to the creation of highly oxidizing compounds, such as chlorates and perchlorates. These strong substances can effectively destroy organic molecules (components of life) on the surface and break down many atmospheric compounds, completely altering the overall chemical balance of the Martian atmosphere.

This discovery could also explain the puzzling ability of Martian methane to vanish rapidly, offering a crucial piece of the puzzle for understanding the constraints life may have faced and, therefore, the planet's potential to be habitable.

Given the widespread availability of dust on Mars, the presence of electrical charges generated by particles rubbing together would seem likely to influence dust transport on Mars as well. How dust travels on Mars plays a central role in the planet’s climate but remains poorly understood.

Confirming the presence of electrostatic discharges will also help NASA understand potential risks to the electronic equipment of current robotic missions. That no adverse electrostatic discharge effects have been reported in several decades of Mars surface operations may attest to careful spacecraft grounding practices. The findings could also influence safety measures developed for future astronauts exploring the Red Planet.

Managed for NASA by Caltech, the Jet Propulsion Laboratory in Southern California built and manages operations of the Perseverance rover on behalf of the agency’s Science Mission Directorate as part of NASA’s Mars Exploration Program portfolio.

Learn more about NASA's Perseverance Mars Rover:


Credit: NASA/JPL-Caltech/Space Science Institute (SSI)
Duration: 7 seconds
Release Date: Dec. 3, 2025

#NASA #Space #Astronomy #Science #Planets #Mars #Meteorology #Weather #DustDevils #ElectricalDischarges #TriboelectricEffect #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #JPL #Caltech #SSI #UnitedStates #STEM #Education #HD #Video

The Bright Bluish Supergiant Stars: Alnitak, Alnilam & Mintaka in Orion

The Bright Bluish Supergiant Stars: Alnitak, Alnilam & Mintaka in Orion

Alnitak, Alnilam, and Mintaka are the bright bluish stars from east to west (upper right to lower left) along the diagonal in this cosmic vista. Otherwise known as the Belt of Orion, these three blue supergiant stars are hotter and much more massive than the Sun. They lie from 700 to 2,000 light-years away, born of Orion's well-studied interstellar clouds. In fact, clouds of gas and dust adrift in this region have surprisingly familiar shapes, including the dark Horsehead Nebula and Flame Nebula near Alnitak at the upper right. The famous Orion Nebula itself is off the right edge of this colorful starfield. The telescopic frame spans almost 4 degrees on the sky.


Image Credit & Copyright: Aygen Erkaslan
Aygen's website: 

#NASA #Space #Astronomy #Science #Nebulae #HorseheadNebula #Barnard33 #FlameNebula #NGC2024 #Sh2277 #Stars #Supergiants #Alnitak #Alnilam #Mintaka #Orion #Constellations #MilkyWayGalaxy #Cosmos #Universe #Astrophotography #AygenErkaslan #Astrophotographers #GSFC #UnitedStates #STEM #Education #APoD

North Africa: Rings of Rock in The Sahara | International Space Station

North Africa: Rings of Rock in The Sahara | International Space Station

A top-down view shows circular rocky formations rising from a flat, sandy-brown landscape. Darker brown sand encircles the rocky rings, with lighter patches of outwash spreading across the terrain.
In southeastern Libya, Jabal Arkanū’s concentric rock rings stand as relics of past geologic forces that churned beneath the desert.

In northeastern Africa, within the driest part of The Sahara, dark rocky outcrops rise above pale desert sands. Several of these formations, including Jabal Arkanū, display striking ring-shaped structures.

Jabal Arkanū (also spelled Arkenu) lies in southeastern Libya, near the border with Egypt. Several other massifs are clustered nearby, including Jabal Al Anaynat (or Uweinat), located about 20 kilometers (12 miles) to the southeast. Roughly 90 kilometers to the west are the similarly named Arkenu structures. These circular features were once thought to have formed by meteorite impacts, but later fieldwork suggested they resulted from terrestrial geological processes.

Arkanū’s ring-shaped structures also have an earthly origin. They are thought to have formed as magma rose toward the surface and intruded into the surrounding rock. Repeated intrusion events produced a series of overlapping rings, their centers roughly aligned toward the southwest. The resulting ring complex—composed of igneous basalt and granite—is bordered to the north by a hat-shaped formation made of sandstone, limestone, and quartz layers.

This photograph, taken by an astronaut aboard the International Space Station on September 13, 2025, shows the massif casting long shadows across the desert. The ridges stand nearly 1,400 meters above sea level, or about 800 meters above the surrounding sandy plains. Notice several outwash fans of boulders, gravel, and sand spreading from the mountain’s base toward the bordering longitudinal dunes.

Two wadis, or typically dry riverbeds, wind through the structure. However, water is scarce in this part of The Sahara. Past research using data from NASA and the Japan Aerospace Exploration Agency's now-completed Tropical Rainfall Measuring Mission (TRMM) indicated that southeastern Libya, along with adjacent regions of Egypt and northern Sudan, receives only about 1 to 5 millimeters of rain per year. Slightly higher accumulations, around 5 to 10 millimeters per year, occur near Jabal Arkanū and neighboring massifs, suggesting a modest orographic effect from the mountains.

This is an astronaut photograph, taken by a member of the Expedition 73 crew. It was taken with a Nikon Z9 digital camera using a focal length of 800 millimeters. 

The Sahara is a desert spanning across North Africa. With an area of 9,200,000 square kilometres (3,600,000 sq mi), it is the largest hot desert in the world and the third-largest desert overall, smaller only than the deserts of Antarctica and the northern Arctic.

The name "Sahara" is derived from Arabic: صَحَارَى, romanized: ṣaḥārā /sˤaħaːraː/, a broken plural form of ṣaḥrā' (صَحْرَاء /sˤaħraːʔ/), meaning "desert".

The desert covers much of North Africa, excluding the fertile region on the Mediterranean Sea coast, the Atlas Mountains of the Maghreb, and the Nile Valley in Egypt and the Sudan.

It stretches from the Red Sea in the east and the Mediterranean in the north to the Atlantic Ocean in the west, where the landscape gradually changes from desert to coastal plains. To the south it is bounded by the Sahel, a belt of semi-arid tropical savanna around the Niger River valley and the Sudan region of sub-Saharan Africa. The Sahara can be divided into several regions, including the western Sahara, the central Ahaggar Mountains, the Tibesti Mountains, the Aïr Mountains, the Ténéré desert, and the Libyan Desert.

Follow Expedition 73:

Expedition 73 Crew
Station Commander: Sergey Ryzhikov (Roscosmos)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Alexey Zubritskiy, Oleg Platonov, Sergey-Kud Sverchkov, Sergei Mikaev
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke, Chris Williams

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.

Image Credit: NASA's Johnson Space Center
Article Credit: Kathryn Hansen
Image Date: Sept. 13, 2025
Release Date: Nov. 28, 2025

#NASA #Space #ISS #Earth #Sahara #Libya #Africa #JabalArkanū #Geology #Astronauts #Cosmonauts #HumanSpaceflight #SpaceLaboratory #JSC #UnitedStates #Russia #Россия #Roscosmos #Роскосмос #Japan #JAXA #Expedition73 #Expedition74 #STEM #Education

U.S. & Canadian Cities: Great Lakes, Aurora+Moonrise | International Space Station

U.S. & Canadian Cities: Great Lakes, Aurora+Moonrise | International Space Station

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.

The Great Lakes, also called the Great Lakes of North America, are a series of large interconnected freshwater lakes spanning the Canada–United States border. The five lakes are Superior, Michigan, Huron, Erie, and Ontario (though hydrologically, Michigan and Huron are a single body of water, joined at the Straits of Mackinac). 

Follow Expedition 73:

Expedition 73 Crew
Station Commander: Sergey Ryzhikov (Roscosmos)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Alexey Zubritskiy, Oleg Platonov, Sergey-Kud Sverchkov, Sergei Mikaev
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke, Chris Williams

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.

Video Credit: NASA's Johnson Space Center/J. Kim
Video Details: Nikon Z9 | 15mm | ISO 25600 f1.8 1/4s
Duration: 35 seconds
Capture Date: Sept. 2, 2025
Release Date: Dec. 2, 2025

#NASA #Space #ISS #Earth #Moon #Aurora #AuroraBorealis #Canada #GreatLakes #NorthAmerica #Astronauts #Cosmonauts #HumanSpaceflight #SpaceLaboratory #JSC #UnitedStates #Russia #Roscosmos #Japan #JAXA #Expedition73 #Expedition74 #STEM #Education #HD #Video

Tuesday, December 02, 2025

Close-up: Spiral Galaxy NGC 4535 in Virgo | Hubble

Close-up: Spiral Galaxy NGC 4535 in Virgo | Hubble

This Hubble picture features the spiral galaxy NGC 4535. It is located about 50 million light-years away in the constellation Virgo (The Maiden). This galaxy has been nicknamed the ‘Lost Galaxy’ because it is extremely faint when viewed through a small telescope. With a mirror spanning 2.4 meters across, Hubble is well equipped to observe dim galaxies like NGC 4535 and pick out features like its massive spiral arms and central bar of stars.

On full display in this Hubble image are NGC 4535’s young star clusters that dot the galaxy’s spiral arms. Many of the groupings of bright blue stars are enclosed by glowing pink clouds. These clouds, called H II (‘H-two’) regions, are a sign that the galaxy is home to especially young, hot, and massive stars that are blazing with high-energy radiation. By heating the clouds in which they were born, shooting out powerful stellar winds, and eventually exploding as supernovae, massive stars certainly shake up their surroundings. 

This Hubble image incorporates data from an observing program that will catalogue roughly 50,000 H II regions in nearby star-forming galaxies like NGC 4535. A previous image of NGC 4535 was released in 2021. Both the 2021 image and today’s image incorporate observations from the PHANGS program that seek to understand the connections between young stars and cold gas. This  current image adds a new dimension to our understanding of NGC 4535 by capturing the brilliant red glow of the nebulae that encircle massive stars in their first few million years of life.

Image Description: A close-in view of a spiral galaxy that faces the viewer. Brightly lit spiral arms swing outwards through the galaxy’s disc, starting from an elliptical region in the center. Thick strands of dark reddish dust are spread across the disc, mostly following the spiral arms. The arms also contain many glowing pink-red spots where stars form. The galaxy is a bit fainter beyond the arms, but speckled with blue stars.


Credit: ESA/Hubble & NASA, F. Belfiore, J. Lee and the PHANGS-HST Team, N. Bartmann (ESA/Hubble)
Duration: 30 seconds
Release Date: Nov. 17, 2025


#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #Galaxies #NGC4535 #SpiralGalaxies #Virgo #Constellations #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Close-up: NGC 4490 & NGC 4485 Dwarf Galaxies in Canes Venatici | Webb Telescope

Close-up: NGC 4490 & NGC 4485 Dwarf Galaxies in Canes Venatici | Webb Telescope

The NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope has spied a pair of dwarf galaxies engaged in a gravitational 'dance.' These two galaxies are named NGC 4490 (left) and NGC 4485 (top right). They are located about 24 million light-years away in the constellation Canes Venatici (The Hunting Dogs). Aside from the Milky Way’s own dwarf companions (the Large and Small Magellanic Clouds), this is the closest known interacting dwarf-dwarf system where astronomers have directly observed a gas bridge and resolved stellar populations. Together NGC 4490 and NGC 4485 form the system Arp 269, featured in the Atlas of Peculiar Galaxies. At such a close distance (and with Webb’s impressive ability to peer through dusty cosmic clouds) these galaxies allow astronomers to witness up close the kinds of galaxy interactions that were common billions of years ago.

Dwarf galaxies likely share many similarities with young galaxies in the early Universe: they are much less massive than galaxies like the Milky Way, they typically have small amounts of metals (what astronomers call elements heavier than helium), and they contain a lot of gas and relatively few stars. When nearby dwarf galaxies collide, merge, or steal gas from one another, it can tell us how galaxies billions of years ago might have grown and evolved. 

The nearby dwarf galaxies NGC 4490 and NGC 4485 form an intriguing pair. Nearly three decades ago, astronomers discovered a wispy bridge of gas connecting the two galaxies, showing that they have interacted in the past. Despite many studies with powerful telescopes like the Hubble Space Telescope, the history between NGC4490 and NGC 4485 has remained mysterious.

Recently, Webb observed this curious galactic pair as part of the Feedback in Emerging extrAgalactic Star clusTers (FEAST) program (#1783; PI: A. Adamo). The FEAST program used Webb’s sensitive infrared eyes to reveal the formation of new stars in different types of nearby galaxies.

This image was developed using data from Webb’s Near-InfraRed Camera (NIRCam) and Mid-InfraRed Instrument (MIRI), as well as a single narrow-band filter from Hubble (657N). It reveals NGC 4490 and NGC 4485 in never-before-seen detail and illuminates the bridge of gas and stars that connects them. NGC 4490 dominates the image as the larger object occupying the left side of the image, while NGC 4485 is the smaller galaxy that hosts the top-right portion of the image. By dissecting these galaxies star by star, researchers were able to map out where young, middle-aged, and old stars reside, and trace the timeline of the galaxies’ interaction.

Roughly 200 million years ago, these galaxies whirled close to one another before waltzing away. The larger galaxy, NGC 4490, ensnared a stream of gas from its companion, and this gas now trails between the galaxies like dancers connected by outstretched arms. Along the newly formed bridge of gas and within the two galaxies, this interaction spurred a burst of new stars. The concentrated areas of bright blue that appear throughout the field indicate highly ionized regions of gas by the recently formed star clusters. Just 30 million years ago, these galaxies burst alight with stars once more, with new clusters coalescing where the gas of the two galaxies mixed together.

By capturing the history of the galactic dancers NGC 4490 and NGC 4485, Webb has revealed new details in how dwarf galaxies interact, giving us a glimpse of how small galaxies near and far grow and evolve.

Image Description: This Webb image shows two interacting galaxies. NGC 4490 occupies the left side of the image, while NGC 4485 appears as a white glowing hue in the top right of the field. Both galaxies are connected by a bright stream of red stretching from the top left of the image, through the bottom center, and ending at the right under galaxy NGC 4485. There are regions of bright blue ionized gas visible in concentrated areas of the red stream. The background is black with multiple galaxies in various shapes throughout.


Credit: ESA/Webb, NASA & CSA, A. Adamo (Stockholm University), G. Bortolini, and the FEAST JWST team
Duration: 30 seconds
Release Date: Dec. 2, 2025

#NASA #Space #Astronomy #Science #Galaxies #NGC4490 #NGC4485 #ARP269 #InteractingGalaxies #CanesVenatici #Constellations #Cosmos #Universe #JWST #InfraredAstronomy #NIRCam #MIRI #SpaceTelescopes #ESA #CSA #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

NGC 4490 & NGC 4485: Dwarf Galaxies in Canes Venatici | Webb Telescope

NGC 4490 & NGC 4485: Dwarf Galaxies in Canes Venatici | Webb Telescope

The NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope has spied a pair of dwarf galaxies engaged in a gravitational 'dance.' These two galaxies are named NGC 4490 (left) and NGC 4485 (top right). They are located about 24 million light-years away in the constellation Canes Venatici (The Hunting Dogs). Aside from the Milky Way’s own dwarf companions (the Large and Small Magellanic Clouds), this is the closest known interacting dwarf-dwarf system where astronomers have directly observed a gas bridge and resolved stellar populations. Together NGC 4490 and NGC 4485 form the system Arp 269, featured in the Atlas of Peculiar Galaxies. At such a close distance (and with Webb’s impressive ability to peer through dusty cosmic clouds) these galaxies allow astronomers to witness up close the kinds of galaxy interactions that were common billions of years ago.

Dwarf galaxies likely share many similarities with young galaxies in the early Universe: they are much less massive than galaxies like the Milky Way, they typically have small amounts of metals (what astronomers call elements heavier than helium), and they contain a lot of gas and relatively few stars. When nearby dwarf galaxies collide, merge, or steal gas from one another, it can tell us how galaxies billions of years ago might have grown and evolved. 

The nearby dwarf galaxies NGC 4490 and NGC 4485 form an intriguing pair. Nearly three decades ago, astronomers discovered a wispy bridge of gas connecting the two galaxies, showing that they have interacted in the past. Despite many studies with powerful telescopes like the Hubble Space Telescope, the history between NGC4490 and NGC 4485 has remained mysterious.

Recently, Webb observed this curious galactic pair as part of the Feedback in Emerging extrAgalactic Star clusTers (FEAST) program (#1783; PI: A. Adamo). The FEAST program used Webb’s sensitive infrared eyes to reveal the formation of new stars in different types of nearby galaxies.

This image was developed using data from Webb’s Near-InfraRed Camera (NIRCam) and Mid-InfraRed Instrument (MIRI), as well as a single narrow-band filter from Hubble (657N). It reveals NGC 4490 and NGC 4485 in never-before-seen detail and illuminates the bridge of gas and stars that connects them. NGC 4490 dominates the image as the larger object occupying the left side of the image, while NGC 4485 is the smaller galaxy that hosts the top-right portion of the image. By dissecting these galaxies star by star, researchers were able to map out where young, middle-aged, and old stars reside, and trace the timeline of the galaxies’ interaction.

Roughly 200 million years ago, these galaxies whirled close to one another before waltzing away. The larger galaxy, NGC 4490, ensnared a stream of gas from its companion, and this gas now trails between the galaxies like dancers connected by outstretched arms. Along the newly formed bridge of gas and within the two galaxies, this interaction spurred a burst of new stars. The concentrated areas of bright blue that appear throughout the field indicate highly ionized regions of gas by the recently formed star clusters. Just 30 million years ago, these galaxies burst alight with stars once more, with new clusters coalescing where the gas of the two galaxies mixed together.

By capturing the history of the galactic dancers NGC 4490 and NGC 4485, Webb has revealed new details in how dwarf galaxies interact, giving us a glimpse of how small galaxies near and far grow and evolve.

Image Description: This Webb image shows two interacting galaxies. NGC 4490 occupies the left side of the image, while NGC 4485 appears as a white glowing hue in the top right of the field. Both galaxies are connected by a bright stream of red stretching from the top left of the image, through the bottom center, and ending at the right under galaxy NGC 4485. There are regions of bright blue ionized gas visible in concentrated areas of the red stream. The background is black with multiple galaxies in various shapes throughout.


Credit: ESA/Webb, NASA & CSA, A. Adamo (Stockholm University), G. Bortolini, and the FEAST JWST team
Release Date: Dec. 2, 2025

#NASA #Space #Astronomy #Science #Galaxies #NGC4490 #NGC4485 #ARP269 #InteractingGalaxies #CanesVenatici #Constellations #Cosmos #Universe #JWST #InfraredAstronomy #NIRCam #MIRI #SpaceTelescopes #ESA #CSA #GSFC #STScI #UnitedStates #STEM #Education

Russian Soyuz MS-28 Crew Spacecraft Arrival | International Space Station

Russian Soyuz MS-28 Crew Spacecraft Arrival | International Space Station







Expedition 74 Crew Emblem

The Russian Soyuz MS-28 crew spacecraft carrying NASA astronaut Chris Williams and Roscosmos cosmonauts Sergey Kud-Sverchkov and Sergei Mikaev of Russia approaches the International Space Station. Both spacecraft were orbiting 262 miles above the hot desert landscape of Western Sahara and the mountainous region in southern Morocco at the time of these photographs.

Follow Expedition 73:

Expedition 73 Crew
Station Commander: Sergey Ryzhikov (Roscosmos)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Alexey Zubritskiy, Oleg Platonov, Sergey-Kud Sverchkov, Sergei Mikaev
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke, Chris Williams

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.

Image Credit: NASA's Johnson Space Center
Image Date: Nov. 27, 2025
Release Date: Dec. 2, 2025

#NASA #Space #ISS #Earth #Sahara #Africa #Spacecraft #SoyuzMS28 #SoyuzMS28Spacecraft #Astronauts #ChrisWilliams #Cosmonauts #SergeyKudSverchkov #SergeyMikaev #HumanSpaceflight #SpaceLaboratory #JSC #UnitedStates #Russia #Россия #Roscosmos #Роскосмос #Japan #JAXA #Expedition73 #Expedition74 #STEM #Education

Shenzhou-20 Spacecraft to Make Uncrewed Return to Earth | China 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 edgea 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.


Video Credit: CCTV
Duration: 2 minutes
Release Date: Dec. 2, 2025

#NASA #Space #Science #China #中国 #Earth #Shenzhou20Mission #神舟二十号 #Shenzhou20Spacecraft #Taikonauts #Astronauts #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #SpaceLaboratory #CMSA #中国载人航天工程办公室 #HumanSpaceflight #DongfengLandingSite #InnerMongoliaAutonomousRegion #STEM #Education #HD #Video

NASA Artemis III Moon Rocket Liquid Oxygen Tank for Core Stage | NASA Michoud

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.

Over the course of about 30 days, the Artemis III astronauts will travel to lunar orbit, where two crew members will descend to the surface and spend approximately a week near the South Pole of the Moon conducting new science before returning to lunar orbit to join their crew for the journey back to Earth. Launch is currently scheduled for mid-2027.

Follow updates on the Artemis blog: 
https://blogs.nasa.gov/artemis/

NASA's Space Launch System (SLS)
https://www.nasa.gov/sls


Read the Artemis Plan (74-page PDF Free Download): 
https://www.nasa.gov/sites/default/files/atoms/files/artemis_plan-20200921.pdf

NASA's Michoud Assembly Facility (MAF)
https://www.nasa.gov/michoud-assembly-facility/

Image Credit: NASA/Michael DeMocker
Date: Nov. 3, 2025

#NASA #Space #Earth #Moon #Artemis #ArtemisIII #SLS #SLSRocket #CoreStage #LiquidOxygenTank #O2Tank #Boeing #CrewedMissions #DeepSpace #MoonToMars #Science #Engineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #MSFC #MAF #NewOrleans #Louisiana #UnitedStates #STEM #Education 

Moon Shadows on Planet Saturn | Hubble Space Telescope

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.


Video Credit: Space Telescope Science Institute (STScI)
Duration: 48 seconds
Release Date: Dec. 1, 2025

#NASA #Hubble #Astronomy #Space #Science #Planets #Saturn #Moons #Enceladus #Mimas #Dione #Tethys #SolarSystem #HubbleSpaceTelescope #HST #ESA #GSFC #STScI #STEM #Education #HD #Video

Mediterranean & Africa Flyover: History in Lights | International Space Station

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.

Follow Expedition 73:

Expedition 73 Crew
Station Commander: Sergey Ryzhikov (Roscosmos)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Alexey Zubritskiy, Oleg Platonov, Sergey-Kud Sverchkov, Sergei Mikaev
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke, Chris Williams

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.

Video Credit: NASA's Johnson Space Center/D. Pettit
Duration: 38 seconds
Release Date: Nov. 25, 2025

#NASA #Space #ISS #Science #Earth #Mediterranean #NorthAfrica #Africa #Europe #DonPettit #AstronautVideography #UnitedStates #Japan #JAXA #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition71 #Expedition72 #STEM #Education #HD #Video

Stellar Pre-Winter Seasonal Offerings | NASA's Chandra X-ray Observatory

Stellar Pre-Winter Seasonal Offerings | NASA's Chandra X-ray Observatory


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 actually 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.
Credit:  X-ray: NASA/SAO/CXC; Infrared: NASA/JPL/CalTech/Spitzer; Image Processing: NASA/CXC/SAO/J. Schmidt
Born after a violent explosion of a star, this cosmic gourd is the supernova remnant G272.2-03.2. X-ray observations (orange and magenta) 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.
Credit:  X-ray: NASA/CXC/SA0; Optical: NOIRLab/DECaPS2; Image Processing: NASA/CXC/SAO/L. Frattare
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 (purple), optical light data from Hubble and the Very Large Telescope in Chile (orange, red, and violet), and an optical image from astrophotographers Bob Fera and Steve Mandel (deep blue) 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.
Credit:  X-ray: NASA/CXC/SAO; ESA/XMM-Newton; Optical HST: NASA/ESA/STScI; Optical Ground: Deep Space Remote observatories/B. Fera and S. Mandel; ESO/VLT; Image Processing: NASA/CXC/SAO/L. Frattare
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 than make up these two spiral galaxies, known as NGC 2207 (right) and IC 2163 (left), that we see face-on. This view of NGC 2207 and IC 2163 takes a James Webb infrared image (white, gray, and red) and adds the X-ray view from Chandra (blue). Together, it is quite an eye-catching result.
Credit:  X-ray: NASA/CXC/SAO; Infrared: NASA/ESA/CSA/STScI/Webb; Image Processing: NASA/CXC/SAO/L. Frattare

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.

NASA's Chandra X-ray Observatory is being canceled in NASA's Fiscal Year 2026 Budget Request, along with 18 other active science missions. NASA's science budget is being reduced by nearly 50%. NASA's total budget will become the lowest since 1961, after accounting for inflation.

Contact your representatives in the United States Congress, House and Senate, to express your concerns about severe budget cuts at NASA:


Credit: NASA's Chandra X-ray Observatory
Release Date: Nov. 24, 2025

#NASA #Space #Astronomy #Science #Nebulae #NGC6334 #Stars #RAquarii #SupernovaRemnants #G2722032 #Galaxies #NGC2207 #IC2163 #Cosmos #Universe #NASAChandra #ChandraObservatory #SpaceTelescopes #XrayAstronomy #MSFC #UnitedStates #STEM #Education

Monday, December 01, 2025

A First: All Docking Ports Used for Eight Spacecraft | International Space Station

A First: All Docking Ports Used for Eight Spacecraft | International Space Station

International Space Station Configuration on Dec. 1, 2025

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.

Follow Expedition 73:

Expedition 73 Crew
Station Commander: Sergey Ryzhikov (Roscosmos)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Alexey Zubritskiy, Oleg Platonov, Sergey-Kud Sverchkov, Sergei Mikaev
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke, Chris Williams

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.

Image Credit: NASA's Johnson Space Center
Release Date: Dec. 1, 2025

#NASA #Space #ISS #Earth #Spacecraft #Astronauts #Cosmonauts #HumanSpaceflight #SpaceLaboratory #JSC #UnitedStates #Russia #Россия #Roscosmos #Роскосмос #Japan #日本 #JAXA #宇宙航空研究開発機構 #Expedition73 #Expedition74 #Infographics #STEM #Education

China Unveils Next-gen Space Situational Awareness Constellation for Space Debris

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.


Credit: SMG
Duration: 1 minute, 47 seconds
Release Date: Nov. 30, 2025

#NASA #Space #Science #Satellites #SatelliteConstellations #SpaceDebris #Earth #China #中国 #EYESAT #SpaceTrafficManagement #Spaceflight #CommercialSpace #STEM #Education #HD #Video

Stellar Pre-Winter Seasonal Offerings | NASA's Chandra X-ray Observatory

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.


Video Credit: NASA's Chandra X-ray Observatory
Duration: 3 minutes, 23 seconds
Release Date: Nov. 24, 2025


#NASA #Space #Astronomy #Science #Nebulae #NGC6334 #Stars #RAquarii #SupernovaRemnants #G2722032 #Galaxies #NGC2207 #IC2163 #Cosmos #Universe #NASAChandra #ChandraObservatory #SpaceTelescopes #XrayAstronomy #MSFC #UnitedStates #STEM #Education #HD #Video