Friday, October 24, 2025

China Prepares to Launch Shenzhou-21 Crewed Spacecraft | China Space Station

China Prepares to Launch Shenzhou-21 Crewed Spacecraft | China Space Station

The combination of the Shenzhou-21 crew spacecraft and its Long March-2F carrier rocket was transferred to the launch area of the Jiuquan Satellite Launch Center in northwest China on the morning of October 24, 2025, as the country prepares to send another crew to its orbiting space station.

Carried by a mobile launch platform, the combination moved along 1.5 km of seamless rail toward the launch tower from the testing facility.

"This rocket incorporates 16 design changes, with the most important one being the fully upgraded optical navigation system, which greatly improves the redundant inertial measurement units and boost flight reliability," said Sun Yanqiu, an engineer of the China Aerospace Science and Technology Corp.

The Shenzhou-21 will be the 10th crewed mission since China began the initial construction of its space station and the sixth one since the space station entered the stage of application and development.

"After today's transfer, we will conduct checks on the combination's functions as well as a full-system launch rehearsal and an integrated rehearsal to verify compatibility between system interfaces, coordination and procedures. Once everything is confirmed normal, we will carry out rocket propellant filling and proceed to ignition and launch," said Zhao Lei, an engineer at the Jiuquan Satellite Launch Center.

According to schedule, the Shenzhou-21 crewed spacecraft is set to be launched at an appropriate time in the coming days.

The Shenzhou-21 crew will replace the astronauts of the Shenzhou-20 mission that have worked in orbit for six months.


Video Credit: CCTV
Duration: 1 minute, 38 seconds
Release Date: Oct. 24, 2025

#NASA #Space #Science #China #中国 #Earth #LongMarch2FRocket #Shenzhou21Mission #神舟二十一号 #Shenzhou21Crew #Taikonauts #Astronauts #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #SpaceLaboratory #MicrogravityResearch #CMSA #中国载人航天工程办公室 #HumanSpaceflight #JSLC #STEM #Education #HD #Video

Flight Through The Orion Nebula in Visible Light | Space Telescope Science Institute

Flight Through The Orion Nebula in Visible Light | Space Telescope Science Institute

This visualization explores the Orion Nebula as seen in visible-light observations from the Hubble Space Telescope.

As the camera flies into the star-forming region, it reveals a glowing gaseous landscape that has been illuminated and carved by the high-energy radiation and strong stellar winds from the massive hot stars in the central cluster. The high-resolution visible observations show fine details including the wispy bow shocks and tadpole-shaped proplyds.

The Orion Nebula (also known as Messier 42, M42, or NGC 1976) is a diffuse nebula in the Milky Way situated south of Orion's Belt in the constellation of Orion. It is known as the middle "star" in the "sword" of Orion. It is one of the brightest nebulae and is visible to the naked eye in the night sky with an apparent magnitude of 4.0. The Orion Nebula is the closest region of massive star formation to Earth. M42 is estimated to be 25 light-years across (so its apparent size from Earth is approximately 1 degree). It has a mass of about 2,000 times that of the Sun. 

Distance from Earth: 1,500 light-years


Video Credit: Space Telescope Science Institute (STScI)
Visualization: F. Summers, G. Bacon, Z. Levay, L. Frattare, M. Robberto and L. Hustak (STScI)
Acknowledgement: R. Gendler
Duration: 2 minutes, 17 seconds
Release Date: Oct. 23, 2025

#NASA #ESA #Astronomy #Space #Science #Hubble #Nebulae #OrionNebula #Messier42 #M42 #NGC1976 #Orion #Constellations #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI  #UnitedStates #Europe #STEM #Education #Visualization #HD #Video

Journey to Wolf-Rayet Star VFTS 682 in Nearby Large Magellanic Cloud Galaxy

Journey to Wolf-Rayet Star VFTS 682 in Nearby Large Magellanic Cloud Galaxy


This sequence starts with a view of the Milky Way galaxy and its two small neighboring galaxies, the Magellanic Clouds. We zoom in towards the Large Magellanic Cloud and focus on the huge star formation region around the Tarantula Nebula. The final sequence shows a very detailed view, captured in visible and infrared light, of the dense star cluster R 136 and the very brilliant, but strangely isolated, star VFTS 682. All Wolf–Rayet stars are highly luminous objects due to their high temperatures—thousands of times the luminosity of our Sun.

Distance from Earth: 170,000 light years


Credit: ESO/Digitized Sky Survey 2/R. Gendler/S. Brunier
Duration: 56 seconds
Release Date: May 25, 2011

#NASA #ESA #Astronomy #Space #Science #Stars #StarClusters #R136 #WolfRayetStars #VFTS682 #Nebulae #TarantulaNebula #LargeMagellanicCloud #LMC #Dorado #Constellations #Cosmos #Universe #VLT #VISTA #ParanalObservatory #MPGESOTelescope #LaSillaObservatory #Chile #Europe #STEM #Education #HD #Video

Wolf-Rayet Star VFTS 682 in Nearby Large Magellanic Cloud Galaxy | ESO

Wolf-Rayet Star VFTS 682 in Nearby Large Magellanic Cloud Galaxy | ESO

This view shows part of the very active star-forming region around the Tarantula Nebula in the Large Magellanic Cloud, a small neighbor of the Milky Way galaxy. At the exact center lies the brilliant, but isolated star, VFTS 682, and to its lower right the very rich star cluster R 136. The origins of VFTS 682 are unclear—was it ejected from R 136 or did it form on its own? The star appears yellow-red in this view that includes visible-light and infrared images from the Wide Field Imager at the 2.2-meter MPG/ESO Telescope at the La Silla Observatory and the 4.1-meter infrared VISTA telescope at the Paranal Observatory, because of the effects of dust.

Distance from Earth: 170,000 light years


Credit: ESO/M.-R. Cioni/VISTA Magellanic Cloud survey
Acknowledgment: Cambridge Astronomical Survey Unit
Release Date: May 25, 2011


#NASA #ESA #Astronomy #Space #Science #Stars #StarClusters #R136 #WolfRayetStars #VFTS682 #Nebulae #TarantulaNebula #LargeMagellanicCloud #LMC #Dorado #Constellations #Cosmos #Universe #VLT #VISTA #ParanalObservatory #MPGESOTelescope #LaSillaObservatory #Chile #Europe #STEM #Education

Thursday, October 23, 2025

China Landspace Reusable Zhuque-3 Commercial Rocket: Aerial View Preflight

China Landspace Reusable Zhuque-3 Commercial Rocket: Aerial View Preflight

Preparation for the maiden flight of China's reusable rocket Zhuque-3 has entered a critical phase after the completion of joint fueling drills and static ignition tests from October 18 to 20, 2025. The successful tests also laid the groundwork for the rocket's official launch and first-stage recovery later this year.

With a diameter of 4.5 meters and a total length of around 66 meters, the Zhuque-3 rocket can carry up to 18 satellites per launch, making it an ideal choice for launching satellites for large-scale constellation networks.

Equipped with landing legs and grid fins for controlled descent, the rocket is designed to vertically recover its most expensive component—the first stage, accounting for 70 percent of the rocket's total cost.

As its first stage is designed to be reused at least 20 times, the rocket has the potential to reduce launch costs by 80 to 90 percent compared with single-use rockets.

Powered by a parallel cluster of nine liquid oxygen-methane engines, the first-stage can achieve meter-level landing precision, as five of the engines are capable of gimballing.

In addition, these engines produce a combined thrust of more than 7,500 kilonewtons, setting a new record for Chinese commercial liquid-fueled rockets.

Beijing-based LandSpace is a leading Chinese private space company. With its Zhuque-2 rocket, LandSpace became the world's first company to launch a methane-liquid oxygen rocket to Earth orbit in July 2023, ahead of U.S. rivals, including Elon Musk's SpaceX and Jeff Bezos' Blue Origin.

The successful Zhuque-3 development marks a significant stride in the pursuit of low-cost, high-frequency, and large-capacity space launches for China's private space industry.

The Jiuquan Satellite Launch Center (JSLC) was founded in 1958. It was the first of China's four spaceports. The launch center has been the focus of many of China's historic space ventures, including the country's first satellite Dong Fang Hong I in 1970 and their first crewed space mission, Shenzhou V, on October 15, 2003. JSLC is now a home for many new Chinese commercial space launch firms, like Landspace.


Credit: Landspace
Duration: 43 seconds
Release Date: Oct. 23, 2025


#NASA #Space #Satellites #Earth #LEO #China #中国 #LandSpace #蓝箭 #Zhuque3Rocket #Zhuque3 #ReusableRockets #LaunchVehicles #MethaneLiquidOxygen #Methalox #JSLC  #JiuquanSatelliteLaunchCenter #酒泉卫星发射中心 #InnerMongolia #CommercialSpace #CommercialSpaceflight #STEM #Education #HD #Video

Wolf-Rayet Star WR 31a & Nebula in Carina | Hubble Space Telescope

Wolf-Rayet Star WR 31a & Nebula in Carina | Hubble Space Telescope


WR 31a, commonly referred to as Hen 3-519, is a Wolf–Rayet (WR) star in the southern constellation of Carina. It is surrounded by an expanding Wolf–Rayet nebula—a shell of ionized gas nearly eight light-years wide. It is not a classical old stripped-envelope WR star, but a young massive star that still has significant hydrogen left in its atmosphere. All Wolf–Rayet stars are highly luminous objects due to their high temperatures—thousands of times the luminosity of our Sun.

Distance from Earth: about 31,000 light years

WR 31a is surrounded by a blue bubble nebula created by a powerful stellar wind impacting material expelled during earlier stages of the star's life. This nebula was found by Yale University astronomer, Ellen Dorrit Hoffleit (1907-2007), in 1953.


Credit: NASA & European Space Agency
Image Processing: Judy Schmidt
Release Date: J
une 14, 2014


#NASA #ESA #Astronomy #Space #Hubble #Stars #WolfRayetStars #WR31 #Hen3519 #Carina #Constellations #MilkyWayGalaxy #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #JudySchmidt #CitizenScience #UnitedStates #Europe #STEM #Education

Stars & Dust in The Carina Nebula | ESO

Stars & Dust in The Carina Nebula | ESO

The European Southern Observatory's Visible and Infrared Survey Telescope for Astronomy (VISTA) has allowed us to peer through the hot gas and dark dust shrouding the spectacular Carina Nebula to show us myriad stars, both newborn and in their death throes.

Distance from Earth: approximately 8,500 light-years


Credit: European Southern Observatory (ESO)
Directed & Edited by: Nico Bartmann
Written by: Ivana Kurecic and Calum Turner   
Footage and photos: ESO, G. Hüdepohl, DSS, N. Risinger, M. Kornmesser
Executive Producer: Lars Lindberg Christensen
Duration: 1 minute, 15 seconds
Release Date: Aug. 29, 2018

#NASA #ESA #Astronomy #Space #Hubble #Stars #Trumpler14 #Tr14 #StarClusters #BokGlobules #CarinaNebula #NGC3372 #Carina #Constellations #MilkyWayGalaxy #Cosmos #Universe #VLT #VISTA #ParanalObservatory #Chile #Europe #STEM #Education #HD #Video

Highlights of The Carina Nebula (infrared view) | ESO

Highlights of The Carina Nebula (infrared view) | ESO


These highlights are part of a broader view of the Carina Nebula, a region of massive star formation in the southern skies. It was taken in infrared light using the HAWK-I camera on the European Southern Observatory’s Very Large Telescope. This stellar nursery contains dark nebulae where new stars are forming, clusters of young stars and many curious features sculpted from huge clouds of gas and dust.
Distance from Earth: approximately 8,500 light-years

The image section at the center shows the star cluster Trumpler 14 and also reveals a strange golden crescent-shaped cloud. The cutout at the center of the bottom row features a dark cloud known as the caterpillar at the bottom and obscured young stars at the top. The small cluster of stars, appearing yellow in the cutout at the lower right, was discovered in this image.


Credit: ESO/T. Preibisch
Release Date: Feb. 8, 2012


#NASA #ESA #Astronomy #Space #Hubble #Stars #Trumpler14 #Tr14 #StarClusters #BokGlobules #Nebulae #CarinaNebula #NGC3372 #Carina #Constellations #MilkyWayGalaxy #Cosmos #Universe #VLT #ParanalObservatory #Chile #Europe #STEM #Education

Journey to Open Star Cluster Trumpler 14 in The Carina Nebula | ESO

Journey to Open Star Cluster Trumpler 14 in The Carina Nebula | ESO

This short sequence zooms in on the open young cluster of stars, Trumpler 14. It was imaged in great detail thanks to the Multi-Conjugate Adaptive Optics Demonstrator (MAD) mounted on the European Southern Observatory’s Very Large Telescope (VLT). Trumpler 14, inside the Carina Nebula, towards the constellation of Carina (the Keel), is located 8,000 light-years away. It is the adaptive optics image that covers the largest area of sky.


Credit: European Southern Observatory (ESO), H. Sana, Digitized Sky Survey 2 and A. Fujii
Duration: 58 seconds
Release Date: Dec. 3, 2009


#NASA #ESA #Astronomy #Space #Hubble #Stars #Trumpler14 #Tr14 #StarClusters #BokGlobules #CarinaNebula #NGC3372 #Carina #Constellations #MilkyWayGalaxy #Cosmos #Universe #VLT #ParanalObservatory #Chile #Europe #STEM #Education #HD #Video

The Crab Nebula: Multiwavelength Structure of a Pulsar Wind Nebula | STScI

The Crab Nebula: Multiwavelength Structure of a Pulsar Wind Nebula | STScI

This visualization features a three-dimensional multiwavelength representation of the Crab Nebula, a pulsar wind nebula that is the remains of an exploded star. The video is based on images from NASA’s three Great Observatories: the Chandra X-ray Observatory and the Hubble and Spitzer Space Telescopes.

The video begins by showing the Crab Nebula in context, pinpointing the location of the observed supernova in the constellation Taurus. This view zooms in to present the Hubble, Spitzer, and Chandra images of the Crab Nebula, each highlighting one of the nested structures in the system.

The video then begins a slow buildup of the three-dimensional X-ray structure, showing the pulsar and disk of energized material, and adding jets of particles firing off from opposite sides of the energetic dynamo.

Appearing next is a rotating infrared view of a glowing cloud of emission, called synchrotron radiation, enveloping the pulsar system. This distinctive form of radiation occurs when streams of charged particles spiral around the pulsar’s magnetic field lines.

The visible-light outer shell of the Crab Nebula appears next. Looking like a cage around the entire system, this shell of glowing gas consists of tentacle-shaped filaments of ionized oxygen. The tsunami of particles unleashed by the pulsar is pushing on this expanding debris cloud like an animal rattling its cage.

The x-ray, infrared, and visible-light models are combined at the end of the video to reveal both a rotating three-dimensional multiwavelength view and the corresponding two-dimensional multiwavelength image of the Crab Nebula.


Credit: Space Telescope Science Institute, NASA, ESA, F. Summers, J. Olmsted, L. Hustak, J. DePasquale, G. Bacon (STScI), N. Wolk (CfA|H&S/CXC), R. Hurt (Caltech/IPAC)
Duration: 3 minutes, 43 seconds
Release Date: Oct. 22, 2025


#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #NeutronStars #Nebulae #SupernovaRemnanta #CrabNebula #NGC1952 #Taurus #Constellations #Cosmos #Universe #SpaceTelescopes #HST #NASAChandra #NASASpitzer #GSFC #STScI #UnitedStates #Europe #STEM #Education #Visualization #HD #Video

Comet C/2025 A6 Lemmon & Aurora Borealis: View from Alaska

Comet C/2025 A6 Lemmon & Aurora Borealis: View from Alaska

Astrophotographer Todd Salat: "Comet Lemmon rises through the aurora glow in the northeast from Trapper Creek, Alaska, a little after 6 am on October 21, 2025. During today’s closest approach to Earth, the comet is star trekking through the constellation Boötes 'The Herdsman,' which includes Arcturus, the bright star near the bottom of this image."

Comet Lemmon is brightening and moving into morning northern skies as it enters the inner solar system where the Sun increasingly makes its ion tail highly active. Besides Comet SWAN25B and Comet ATLAS, Comet C/2025 A6 (Lemmon) is now the third comet currently visible with binoculars and on long camera exposures. Comet Lemmon was discovered early this year. Comet Lemmon will round the Sun on November 8, 2025. It passed nearest to the Earth—about half of the Earth-Sun distance—on October 21.

Earth auroras have different names depending on the pole they occur at. Aurora Borealis, or the northern lights, is the name given to auroras around the north pole and Aurora Australis, or the southern lights, is the name given for auroras around the south pole.

Image Credit: Todd Salat 
Location: Trapper Creek, Alaska
Image Date: Oct. 21, 2025

#NASA #Astronomy #Space #Science #Earth #Aurora #AuroraBorealis #Comets #CometC2025A6Lemmon #Coma #CometaryTails #SolarSystem #MilkyWayGalaxy #Cosmos #Universe #Astrophotography #ToddSalat #Astrophotographers #TrapperCreek #Alaska #UnitedStates #STEM #Education

Comet C/2025 A6 Lemmon at Closest Distance to Earth: View from Austria

Comet C/2025 A6 Lemmon at Closest Distance to Earth: View from Austria


Astrophotographer Michael Jaeger: "The comet is now entering the inner region of the sun where its ion tail is highly active."

Comet Lemmon is brightening and moving into morning northern skies. Besides Comet SWAN25B and Comet ATLAS, Comet C/2025 A6 (Lemmon) is now the third comet currently visible with binoculars and on long camera exposures. Comet Lemmon was discovered early this year and is still headed into the inner Solar System. The comet will round the Sun on November 8, 2025. It passed nearest to the Earth—about half of the Earth-Sun distance—on October 21.

Image Credit: Michael Jaeger, Gerald Rhemann
Image Details:  C/2025 A6 Lemmon 2025-10-22 17.44 UT RGB 5x2 min 11" RASA QHY 600
Capture Location: Astronomical Centre Martinsberg (AZM), Austria
Image Date: Oct. 22, 2025

#NASA #Astronomy #Space #Science #Comets #CometC2025A6Lemmon #Coma #CometaryTails #SolarSystem #MilkyWayGalaxy #Cosmos #Universe #Astrophotography #MichaelJaeger #GeraldRhemann #Astrophotographers #Martinsberg #Austria #Europe #STEM #Education

Wide-field View: Trumpler 14 Open Star Cluster in The Carina Nebula | ESO

Wide-field View: Trumpler 14 Open Star Cluster in The Carina Nebula | ESO

This image of the Carina Nebula shows the position of the Trumpler 14 open cluster of stars. About 2,000 stars have been identified in Trumpler 14. It is one of the youngest known star clusters, estimates range from 300 to 500 thousand years old. Due to its location within the inner parts of the Carina Nebula, Trumpler 14 is currently undergoing massive star formation.

Distance from Earth:  9,000 light-years

A color-composite image of the Carina Nebula, revealing exquisite details in the stars and dust of the region made with the 2.2-meter MPG/ESO telescope at the La Silla Observatory in Chile. Several well known astronomical objects can be seen in this wide field image—to the bottom left of the image is one of the most impressive binary stars in the Universe, Eta Carinae, with the famous Keyhole Nebula just adjacent to the star. The collection of very bright, young stars above and to the right of Eta Carinae is the open star cluster Trumpler 14. A second open star cluster, Collinder 228 is also seen in the image, just below Eta Carinae. The Carina Nebula also bears the NGC 3372 designation. 

On this image, North is up and East is to the left. The field of view is 0.55 x 0.55 degrees, covering a 72 x 72 light-year region at the distance of the nebula.


Credit: European Southern Observatory (ESO)
Release Date: Dec. 3, 2009


#NASA #ESA #Astronomy #Space #Hubble #Stars #Trumpler14 #Tr14 #StarClusters #BokGlobules #CarinaNebula #NGC3372 #Carina #Constellations #MilkyWayGalaxy #Cosmos #Universe #MPGESOTelescope #LaSillaObservatory #Chile #Europe #STEM #Education

Young Stars of Open Cluster Trumpler 14 in Carina | Hubble

Young Stars of Open Cluster Trumpler 14 in Carina | Hubble


Image Processor Judy Schmidt: "This is a very young star cluster located within the Carina Nebula. These are newly formed stars and we are peering at them through a reddening nebula of dust and gas. The longpass near-infrared filter cuts through much of the nebula and reveals many apparently dimmer stars as reddish pinpricks of light. I have adjusted the colors so that the brighter, whiter stars and their surroundings appear bluer because this is a young cluster. In reality, they are at least a little reddened. There is an interesting arc of cloud at the bottom edge of the frame. "

Distance from Earth:  9,000 light-years

Trumpler 14 (Tr 14) is an open cluster with a diameter of six light-years located within the inner regions of the Carina Nebula. About 2,000 stars have been identified in Trumpler 14. It is one of the youngest known star clusters, estimates range from 300 to 500 thousand years old. For comparison, the massive super star cluster R136 is about 1 to 2 million years old, and the famous Pleiades is about 115 million years old.

Due to its location within the inner parts of the Carina Nebula, Trumpler 14 is currently undergoing massive star formation.


Credit: NASA & European Space Agency
Image Processing: Judy Schmidt
Release Date: September 1, 2014


#NASA #ESA #Astronomy #Space #Hubble #Stars #Trumpler14 #Tr14 #StarClusters #BokGlobules #CarinaNebula #NGC3372 #Carina #Constellations #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #JudySchmidt #CitizenScience #UnitedStates #Europe #STEM #Education

Wednesday, October 22, 2025

China Landspace Reusable Zhuque-3 Commercial Rocket: A Closer Look Pre-flight

China Landspace Reusable Zhuque-3 Commercial Rocket: A Closer Look Pre-flight


Preparation for the maiden flight of China's reusable rocket Zhuque-3 has entered a critical phase after the completion of joint fueling drills and static ignition tests from October 18 to 20, 2025. The successful tests also laid the groundwork for the rocket's official launch and first-stage recovery later this year.

With a diameter of 4.5 meters and a total length of around 66 meters, the Zhuque-3 rocket can carry up to 18 satellites per launch, making it an ideal choice for launching satellites for large-scale constellation networks.

Equipped with landing legs and grid fins for controlled descent, the rocket is designed to vertically recover its most expensive component—the first stage, accounting for 70 percent of the rocket's total cost.

As its first stage is designed to be reused at least 20 times, the rocket has the potential to reduce launch costs by 80 to 90 percent compared with single-use rockets.

Powered by a parallel cluster of nine liquid oxygen-methane engines, the first-stage can achieve meter-level landing precision, as five of the engines are capable of gimballing.

In addition, these engines produce a combined thrust of more than 7,500 kilonewtons, setting a new record for Chinese commercial liquid-fueled rockets.

Beijing-based LandSpace is a leading Chinese private space company. With its Zhuque-2 rocket, LandSpace became the world's first company to launch a methane-liquid oxygen rocket to Earth orbit in July 2023, ahead of U.S. rivals, including Elon Musk's SpaceX and Jeff Bezos' Blue Origin.

The successful Zhuque-3 development marks a significant stride in the pursuit of low-cost, high-frequency, and large-capacity space launches for China's private space industry.

The Jiuquan Satellite Launch Center (JSLC) was founded in 1958. It was the first of China's four spaceports. The launch center has been the focus of many of China's historic space ventures, including the country's first satellite Dong Fang Hong I in 1970 and their first crewed space mission, Shenzhou V, on October 15, 2003. JSLC is now a home for many new Chinese commercial space launch firms, like Landspace.


Credit: Landspace
Duration: 1 minute, 42 seconds
Release Date: Oct. 22, 2025


#NASA #Space #Satellites #Earth #LEO #China #中国 #LandSpace #蓝箭 #Zhuque3Rocket #Zhuque3 #ReusableRockets #LaunchVehicles #MethaneLiquidOxygen #Methalox #JSLC  #JiuquanSatelliteLaunchCenter #酒泉卫星发射中心 #InnerMongolia #CommercialSpace #CommercialSpaceflight #STEM #Education #HD #Video

Mars: A Light-Toned Deposit in Arsinoes Chaos | NASA Mars Reconnaissance Orbiter

Mars: A Light-Toned Deposit in Arsinoes Chaos | NASA Mars Reconnaissance Orbiter

The objective of this observation is to examine a light-toned deposit in a region of chaos terrain. The deposit displays a rough surface, in contrast to the smoothness of the surounding area. Parts of the surface appear as if they were eroded by a fluid flowing north and south. This deposit may have formed in an ancient lake.

Arsinoes Chaos is a chaos terrain in the Margaritifer Sinus quadrangle on Mars. This region of Mars is famous because NASA's Opportunity Rover landed there on January 25, 2004. Arsinoes Chaos is 200 kilometers in diameter. Its location is 7.66 °S and 27.9 °W. Arsinoes Chaos was named after Arsinoe, a queen of ancient Egypt, daughter of Ptolemy and Berenice.

Buttes and mesas in Arsinoes display layering. Many places on Mars show rocks arranged in layers that can form in a variety of ways. Volcanoes, wind, or water can produce them. Of course, layers can be hardened by the action of groundwater. Martian ground water probably moved hundreds of kilometers, and in the process it dissolved many minerals from the rock it passed through. When ground water surfaces in low areas containing sediments, water evaporates in the thin atmosphere and leaves behind minerals as deposits and/or cementing agents. Consequently, layers of dust could not later easily erode away since they were cemented together. On Earth, mineral-rich waters often evaporate forming large deposits of various types of salts and other minerals.

This HiRISE enhanced color camera image (less than 1 km in size) was captured by NASA's Mars Reconnaissance Orbiter (MRO) at an altitude of 269 kilometers (167 miles).

The University of Arizona, in Tucson, operates the High Resolution Imaging Science Experiment (HiRISE). It was built by BAE Systems in Boulder, Colorado. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate (SMD), Washington.

For more information on MRO, visit:

Image Credit: NASA/JPL-Caltech/University of Arizona
Text Credits: UA, Wikipedia
Image Date: Aug. 12, 2025


#NASA #Space #Astronomy #Science #Mars #Planet #RedPlanet #Geology #Geoscience #Landscape #Terrain #ArsinoesChaos # #MRO #MarsOrbiter #MarsSpacecraft #HiRISECamera #JPL #Caltech #UA #UnitedStates #STEM #Education