Tuesday, November 11, 2025

Work on Shenzhou-20 Astronauts' Return "Progresses Orderly" | China Space Station

Work on Shenzhou-20 Astronauts' Return "Progresses Orderly" | China Space Station

All preparatory work for ensuring the safe return of the Shenzhou-20 crewed spacecraft has been progressing orderly, the China Manned Space Engineering Office (CMSEO) said on November 11, 2025.

The return of the Shenzhou-20 astronauts, originally scheduled to take place last Wednesday, has be postponed due to a suspected impact from tiny space debris.

Related contingency plans and measures have since been put in place to comprehensively conduct simulation analysis, tests and safety analysis for the Shenzhou-20 spacecraft and study the plan for implementing the crew's return to Earth, said the CMSEO.

All systems are conducting various tests and coordinated adjustments and tests in strict accordance with the procedures as well as assessing the status of key products and checking their quality, while the landing site is organizing comprehensive rehearsals for the return mission, it said.

Currently, the space station complex is in good condition and is capable of supporting two astronaut crews living aboard simultaneously.

The Shenzhou-20 crew is in good health and working normally and has been conducting scientific experiments and tests together with the Shenzhou-21 crew.

Shenzhou-20 Crew
Chen Dong (陈冬) - Commander - Third spaceflight
Chen Zhong Rui (陈中瑞) - Operator - First spaceflight
Wang Jie (王杰) - Flight Engineer - First spaceflight

Video Credit: CCTV
Duration: 1 minute
Release Date: Nov. 11, 2025

#NASA #Space #Science #China #中国 #Earth #Shenzhou20Mission #神舟二十号 #Shenzhou20Crew #Taikonauts #ChenDong #ChenZhongrui #WangJie #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

Galaxies Across Space and Time | Hubble Space Telescope | STScI

Galaxies Across Space and Time | Hubble Space Telescope | STScI

"This award-winning short film transforms images and data from NASA's Hubble Space Telescope into a voyage that sweeps viewers across the universe and back into cosmic history."

"The film opens with looming images of two mature galaxies that are relatively nearby Earth, and then pans through the vibrant and diverse panorama of thousands of galaxies in an image from the Great Observatories Origins Deep Survey. The ensuing 3-D journey through these galaxies provides more than just a new perspective in space; it also takes the audience back in time. Because light takes time to journey across space, the galaxies farther away from Earth are seen further back in cosmic history. The virtual voyage reveals galaxies as they appeared billions of years ago, when they were still in the process of forming."

Originally released as an IMAX film, "Hubble: Galaxies Across Space and Time" was named "Best Short Film" of 2004 by the Large Format Cinema Association.

Credits:
A production of the Office of Public Outreach at the Space Telescope Science Institute (STScI)
Producer: John Stoke
Director: Frank Summers
Writers: John Stoke and Frank Summers
Visualization Leads: Greg Bacon and Frank Summers
Narrator: Barbara Feldon
Duration: 2 minutes, 52 seconds
Release Date: Nov. 10, 2025

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

Monday, November 10, 2025

The Red Bubble: Supernova Remnant SNR 0509-67.5 in Dorado | STScI

The Red Bubble: Supernova Remnant SNR 0509-67.5 in Dorado | STScI

This video presents a visualization of the supernova remnant known as SNR 0509-67.5. The delicate sphere of gas, photographed by NASA's Hubble Space Telescope, is the result of gas that is being shocked by the expanding blast wave from a supernova. The bubble is the visible remnant of a powerful stellar explosion in the Large Magellanic Cloud (LMC), a small galaxy about 160,000 light-years from Earth. Ripples in the shell's surface may be caused by either subtle variations in the density of the ambient interstellar gas, or possibly driven from the interior by pieces of the ejecta. The bubble-shaped shroud of gas is 23 light-years across and is expanding at more than 11 million miles per hour (5,000 kilometers per second).

The unique three-dimensional view of the visualization reminds us that the objects in Hubble images are not all at the same distance, but rather spread across light-years of space. The stars and the shell of glowing gas from the Hubble two-dimensional image have been separated using both scientific knowledge and artistic license to create the depth in the video. Of note, the relative distances between stars and the nebula have been greatly compressed.


Credit: NASA, European Space Agency (ESA), and G. Bacon, T. Borders, L. Frattare, Z. Levay, and F. Summers (STScI)
Duration: 48 seconds
Release Date: Nov. 9, 2025

#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #Nebulae #SupernovaRemnant #SNR0509675 #Dorado #Constellations #LargeMagellanicCloud #LMC #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education #3D #Visualization #HD #Video

Japan's HTV-X1 Cargo Ship Captured by Canadarm2 | International Space Station

Japan's HTV-X1 Cargo Ship Captured by Canadarm2 | International Space Station



On October 29, 2025, the Canadian Space Agency's Canadarm2 captured the Japan Aerospace Exploration Agency's HTV-X1 cargo spacecraft. 

The Japan Aerospace Exploration Agency (JAXA) launched its HTV-X1 cargo spacecraft on a H3-24L rocket to the International Space Station (ISS) from the Yoshinobu Launch Complex at Tanegashima Space Center in southeastern Japan on October 26, 2025. This was Japan's first cargo shipment to the ISS in five years.

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
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke

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: Japan Aerospace Exploration Agency (JAXA)/Kimiya Yui
Duration: 1 minute
Release Date: Oct. 29, 2025

#NASA #Space #Astronomy #Science #Earth #ISS #Canadarm2 #CSA #Canada #HTVX #新型宇宙ステーション補給機 #CargoSpacecraft #Astronauts #KimiyaYui #油井亀美也 #Japan #日本 #JAXA #宇宙航空研究開発機構 #UnitedStates #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education #HD #Video

Fresh Food Delivery by Japan's HTV-X Cargo Spacecraft | International Space Station

Fresh Food Delivery by Japan's HTV-X Cargo Spacecraft | International Space Station

Apples, tomatoes, two varieties of Japanese pears, and Satsuma mandarins have been delivered to Expedition 73 astronaut Kimiya Yui of the Japan Aerospace Exploration Agency (JAXA).

With HTV-X, cargo can be loaded even closer to launch time than with the previous "Kounotori" cargo spaecraft making it possible to carry even fresher foods. Japan's seasonal flavors are also helping to reduce stress for the crew, including Astronaut Yui, and improve their work performance.

The Japan Aerospace Exploration Agency (JAXA) launched its HTV-X1 cargo spacecraft on a H3-24L rocket to the International Space Station (ISS) from the Yoshinobu Launch Complex at Tanegashima Space Center in southeastern Japan on October 26, 2025. This was Japan's first cargo shipment to the ISS in five years.

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
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke

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: Japan Aerospace Exploration Agency (JAXA)/Kimiya Yui
Release Date: Nov. 10, 2025

#NASA #Space #Astronomy #Science #Earth #ISS #FreshProduce #Fruit #HTVXCargoSpacecraft #Astronauts #KimiyaYui #油井亀美也 #Japan #日本 #JAXA #宇宙航空研究開発機構 #UnitedStates #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education

New Lasers for a Gigantic Virtual Telescope—A New Era for Interferometry | ESO

New Lasers for a Gigantic Virtual Telescope—A New Era for Interferometry | ESO

"We have been working towards this for decades, and now the time has finally come. Last week, the European Southern Observatory’s Paranal Observatory was host to a show unlike any other as four lasers, one from each of the 8-meter telescopes of the Very Large Telescope (VLT), were projected into the skies. All in the name of science, of course."

"In this Chasing Starlight episode, we will explore GRAVITY+, a massive upgrade to the European Southern Observatory’s VLT Interferometer and how new lasers are opening up the southern sky to this facility."

GRAVITY+ was carried out by a consortium led by the Max Planck Institute for Extraterrestrial Physics. Principal Investigator (PI): Frank Eisenhauer


Video Credit: European Southern Observatory (ESO)
Duration: 6 minutes
Release Date: Nov. 10, 2025

#NASA #ESO #Astronomy #Space #Science #Stars #Galaxies #Nebulae #Cosmos #Universe #LaserGuides #Interferometry #GravityPlus #VLT #VLTInterferometer #ParanalObservatory #Chile #Europe #STEM #Education #Starlight #HD #Video

Close-up: NGC 4102 in Ursa Major—An Unusual Spiral Galaxy | Hubble

Close-up: NGC 4102 in Ursa MajorAn Unusual Spiral Galaxy | Hubble


What lies at the heart of this unusual-looking spiral galaxy? The NGC 4102, featured in this Hubble picture is home to what astronomers call an active galactic nucleus. Active galactic nuclei are luminous galactic centers powered by supermassive black holes that contain millions to billion times the mass of our Sun. As these black holes ensnare gas from their surroundings and draw it close with their intense gravitational pull, the gas becomes so hot that it begins to glow and emits light from X-ray to radio wavelengths.

At a distance of just 56 million light-years away in the constellation Ursa Major (The Great Bear), NGC 4102 provides an ideal opportunity to study the ways in which active galactic nuclei interact with their home galaxies. Active galactic nuclei come in many different flavors, from extremely powerful types that consume massive amounts of matter and shoot out jets of charged particles, to calmer types that sip gas from their surroundings and glow more faintly.

NGC 4102 likely falls into the latter category. It is classified as Compton-thick—a way of saying that its nucleus is obscured by a thick layer of gas—and a LINER, or low-ionization nuclear emission-line region. LINER galaxies are identified by emission lines from certain weakly ionized elements, and they can be powered by a supermassive black hole that is lazily collecting gas from around it. 

A previous image of this galaxy, made from data taken with Hubble’s Wide Field Planetary Camera 2 (WFPC2), was released in 2014. This new version presents an upgraded view of the galaxy, using data from the Wide Field Camera 3 that replaced WFPC2 in 2009 and improved upon its resolution and field of view. The new observations come from a program that will combine visible-light images from Hubble with X-ray information from the Chandra X-ray Observatory to study the relationship between NGC 4102 and its active galactic nucleus.

Image Description: A spiral galaxy. The inner region immediately around the bright center is golden in color. A gap separates this region from a bright ring, itself surrounded by a glowing halo. Strands of dark brown dust swirl around the center and the outer ring, joined in one spot by a curved arm. Bright, blue and pink specks of light dot the ring, showing where stars are concentrated or have recently formed.


Credit: European Space Agency (ESA)/Hubble & NASA, G. Fabbiano, N. Bartmann (ESA/Hubble)
Duration: 30 seconds
Release Date: Nov. 3, 2025


#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #Galaxies #NGC4102 #StarburstGalaxies #UrsaMajor #Constellations #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Galaxy NGC 1511 in Hydrus: A Disruptive Neighbor | Hubble

Galaxy NGC 1511 in Hydrus: A Disruptive Neighbor | Hubble

Though interesting to look at, NGC 1511 is one galaxy you might not want for a neighbor. As this Hubble picture shows, NGC 1511 is a peculiar spiral galaxy located roughly 50 million light-years away in the constellation Hydrus. Like many galaxies, NGC 1511 does not travel through space alone. Instead, it has a pair of small galactic companions called NGC 1511A and NGC 1511B, that lie outside the frame of this Hubble image. NGC 1511B is situated closest to NGC 1511, and the two galaxies have apparently clashed in the past; a narrow strand of hydrogen gas connects them, and NGC 1511B has been stretched and distorted by the encounter. Researchers have even found evidence that NGC 1511 once had another small companion galaxy that it has disrupted entirely!

These disruptions have an impact on NGC 1511, too. The galaxy is experiencing a burst of star formation, and its disc features strange loops and plumes that could point to past interactions with its neighboring galaxies. Researchers will use Hubble’s keen observations of NGC 1511 to study star clusters embedded within its dusty gas, seeking to understand how matter is cycled from interstellar clouds to stars and back to clouds once again.

Image Description: A spiral galaxy, tilted away so that it is seen mostly from the edge. The disc of the galaxy glows blue from its center, due to younger stars in the spiral arms. There are large and small patches of gas, glowing in red and pink colors, where new stars are forming. Webs of dark dust are spread over the disc.


Credit: ESA/Hubble & NASA, D. Thilker
Release Date: Nov. 10, 2025

#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #Galaxies #NGC1511 #PeculiarGalaxies #NGC1511A #NGC1511B #Hydrus #Constellations #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education

China CAS Space Kinetica-1 Rocket Liftoff of Earth Observation Satellites

China CAS Space Kinetica-1 Rocket Liftoff of Earth Observation Satellites

This CAS Space Kinetica-1 rocket launched a pair of China Aerospace Science and Industry Corporation (CASIC) built very low Earth orbit (VLEO) Earth observation satellites, named Chutian-2-01 & 02, in crystal clear weather at the Jiuquan Satellite Launch Center in northwestern China at 03:32 UTC on November 9, 2025.

The Kinetica-1 Y9 vehicle is painted with decals celebrating the 15th National Games of China, currently being held in the Hong Kong-Macau-Guangzhou region. The painting reads "I love Guangzhou".

China's has accomplished a new national launch record. The country made its 69th & 70th orbital launch attempts of 2025 with a China Aerospace Science and Technology Corporation (CASC) CZ-11 rocket launch from the Yellow Sea the day before, carrying Shiyan-32 (01-03) satellites, and with this CAS Space Kinetica-1 launch today from Jiuquan, carrying the Chutian-2 (01+02) satellites. This surpasses 2024's total of 68 launches.

The Jiuquan Satellite Launch Center (JSLC) is a Chinese spaceport located between Ejin, Alxa, Inner Mongolia and Hangtian Town, Jinta County, Jiuquan, Gansu Province. It is part of the Dongfeng Aerospace City.


Image Credit: CAS Space
Duration: 20 seconds
Date: Nov. 9, 2025

#NASA #Space #Satellites #Earth #CASSpace #Kinetica1 #Kinetica1Y9Rocket #RocketLaunches #Chutian201 #Chutian202 #VLEO #EarthObservation #China #中国 #CASSpace #中科宇航 #CAS #中国科学院 #LaunchVehicles #SolidFuelRockets #CommercialSpace #JSLC #InnerMongolia #STEM #Education #HD #Video

Sunday, November 09, 2025

China's CAS Space Kinetica-1 Rocket Launches Earth Observation Satellites

China's CAS Space Kinetica-1 Rocket Launches Earth Observation Satellites








This CAS Space Kinetica-1 rocket launched a pair of China Aerospace Science and Industry Corporation (CASIC) built very low Earth orbit (VLEO) Earth observation satellites, named Chutian-2-01 & 02, in crystal clear weather at the Jiuquan Satellite Launch Center in northwestern China at 03:32 UTC on November 9, 2025.

The Kinetica-1 Y9 vehicle is painted with decals celebrating the 15th National Games of China, currently being held in the Hong Kong-Macau-Guangzhou region. The painting reads "I love Guangzhou".

China's has accomplished a new national launch record. The country made its 69th & 70th orbital launch attempts of 2025 with a China Aerospace Science and Technology Corporation (CASC) CZ-11 rocket launch from the Yellow Sea the day before, carrying Shiyan-32 (01-03) satellites, and with this CAS Space Kinetica-1 launch today from Jiuquan, carrying the Chutian-2 (01+02) satellites. This surpasses 2024's total of 68 launches.

The Jiuquan Satellite Launch Center (JSLC) is a Chinese spaceport located between Ejin, Alxa, Inner Mongolia and Hangtian Town, Jinta County, Jiuquan, Gansu Province. It is part of the Dongfeng Aerospace City.


Image Credit: CAS Space
Date: Nov. 9, 2025

#NASA #Space #Satellites #Earth #CASSpace #Kinetica1 #Kinetica1Y9Rocket #RocketLaunches #Chutian201 #Chutian202 #VLEO #EarthObservation #China #中国 #CASSpace #中科宇航 #CAS #中国科学院 #LaunchVehicles #SolidFuelRockets #CommercialSpace #JSLC #InnerMongolia #STEM #Education

The "Golden" Comet and Leo Triplet of Galaxies

"Golden" Comet C/2025 K1 (ATLAS) and The Leo Triplet of Galaxies

C/2025 K1 (ATLAS) is an Oort cloud comet first seen in May 2025. It is one of many comets discovered by the Asteroid Terrestrial-impact Last Alert System (ATLAS) that was developed by the University of Hawaii and funded by NASA.

The Leo Triplet (also known as the M66 Group) is a small group of galaxies about 35 million light-years away in the constellation Leo. This galaxy group consists of the spiral galaxies M65, M66, and NGC 3628.


Image Credit: Dan Bartlett
Dan's website: https://app.astrobin.com/u/h2ologg#gallery
Location: June Lake, California, USA
Image Date: Nov. 7, 2025 


#NASA #Astronomy #Space #Science #Comets #CometC2025A6Lemmon #Coma #CometaryTails #OortCloud #SolarSystem #MilkyWayGalaxy #Galaxies #LeoTriplet #M66Galaxies #Universe #Astrophotography #DanBartlett #Astrophotographers #JuneLake #California #USA #STEM #Education

NASA's Mars ESCAPADE Mission: Blue Origin New Glenn Rocket Ready for Launch

NASA's Mars ESCAPADE Mission: Blue Origin New Glenn Rocket Ready for Launch




The Blue Origin New Glenn rocket is fueled for its second mission. The launch window for NASA's ESCAPADE Mars Mission, opens at 2:45 p.m. Eastern Time (ET) / 19:45 UTC, today, November 9, 2025. Join us for the webcast, hosted by Ariane Cornell and Tabitha Lipkin, beginning 45 minutes before launch here: 

The twin spacecraft for NASA's ESCAPADE Mars Mission were manufactured by Rocket Lab.

🚀Blue Origin's New Glenn Rocket:

ESCAPADE Spacecraft Contractor: Rocket Lab

The NASA Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) Mars Mission will study the planet's unique hybrid magnetosphere. ESCAPADE will investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. It will take ESCAPADE about 11 months to arrive at Mars after leaving Earth orbit.

ESCAPADE is led by the UC Berkeley Space Sciences Laboratory, which is responsible for mission management, systems engineering, science leadership, navigation, operations, the electron & ion electrostatic analyzers, and science data processing and archiving.

Key partners are Rocket Lab USA (spacecraft), NASA Goddard Space Flight Center (magnetometers), Embry Riddle Aeronautical University (Langmuir probes), Advanced Space LLC (mission design), and Blue Origin (launch).

Learn more about the two identical spacecraft designed, built, integrated, and tested by Rocket Lab for the University of California Berkeley’s Space Science Laboratory and NASA's Mars Mission:


Image Credits: Blue Origin/UC Berkeley Space Sciences Laboratory (SSL)
Release Date: Nov. 9, 2025


#NASA #Space #Astronomy #Science #Stars #Sun #SpaceWeather #Planets #Mars #Magnetosphere #MartianAtmosphere #ESCAPADEMission #ESCAPADESpacecraft #RocketLab #SolarSystem #SpaceExploration #GSFC #SSL #UCBerkeley #ERAU #AdvancedSpace #BlueOrigin #NewGlenn #CapeCanaveral #Florida #UnitedStates #STEM #Education

Comet C/2025 A6 (Lemmon): View of Dynamic Gas & Dust Tails from Arizona

Comet C/2025 A6 (Lemmon): View of Dynamic Gas & Dust Tails from Arizona

Astrophotographer Andrew McCarthy: "Captured last night—probably the coolest comet shot I've ever gotten. I've never seen such a dynamic tail on a come. Incredible active, and moving quickly, which makes photographing it a challenge." 

Comet Lemmon was discovered early this year as it headed into the inner Solar System. The comet reached its closest point to the Sun on November 8, 2025. It passed nearest to the Earth—about half of the Earth-Sun distance—on October 21.

A comet tail is a projection of material from a comet that often becomes visible when illuminated by the Sun, while the comet passes through the inner Solar System. As a comet approaches the Sun, solar radiation causes the volatile materials within the comet to vaporize and stream out of the comet nucleus, carrying dust away with them.

Blown by the solar wind, these materials typically form two separate tails that extend outwards from the comet's orbit: the dust tail, composed of comet dust, and the gas or ion tail, composed of ionized gases. They become visible through different mechanisms: the dust tail reflects sunlight directly, while the gas tail glows because of the ionization.

Larger dust particles are less affected by solar wind and tend to persist along the comet's trajectory, forming a dust trail which, when seen from Earth in certain conditions, appears as an anti-tail (or antitail) extending in the opposite directions to the main tail.

Initially, a comet's tail may be difficult to observe, but as the comet heats up, it vaporizes its icy nucleus, releasing gas and dust particles that form the tail. This process is known as sublimation, where the heat causes the comet's volatile materials to vaporize and stream out, creating a cloud of gas and dust around the nucleus.

The tail typically points away from the Sun due to the solar wind's influence, but as the comet approaches perihelion, the tail becomes more prominent and extends further away from the Sun.  As the comet recedes from the Sun, the tail's length may decrease, and its direction may change based on the comet's trajectory and the effects of solar wind.

Arizona is a landlocked state in the Southwestern region of the United States, sharing the Four Corners region of the western United States with Colorado, New Mexico, and Utah. It also borders Nevada to the northwest and California to the west, and shares an international border with the Mexican states of Sonora and Baja California to the south and southwest. 


Image Credit: Andrew McCarthy
Andrew's website: https://cosmicbackground.io
Image Date: Oct. 26, 2025

#NASA #Astronomy #Space #Science #Sun #SolarWind #Comets #CometC2025A6Lemmon #Coma #CometaryTails #SolarSystem #MilkyWayGalaxy #Cosmos #Universe #Astrophotography #AndrewMcCarthy #Astrophotographers #CitizenScience #Arizona #UnitedStates #STEM #Education

NASA Mars ESCAPADE Mission: New Glenn Rocket Propellant Loading | Blue Origin

NASA Mars ESCAPADE Mission: New Glenn Rocket Propellant Loading | Blue Origin


The New Glenn launch window for NASA ESCAPADE Mars Mission, opens at 2:45 p.m. Eastern Time (ET) / 19:45 UTC, today, November 9, 2025. Join us for the webcast, hosted by Ariane Cornell and Tabitha Lipkin, beginning 45 minutes before launch here: 

The twin spacecraft for NASA's ESCAPADE Mars Mission were manufactured by Rocket Lab.

🚀Blue Origin's New Glenn Rocket:

ESCAPADE Spacecraft Contractor: Rocket Lab

The NASA Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) Mars Mission will study the planet's unique hybrid magnetosphere. ESCAPADE will investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. It will take ESCAPADE about 11 months to arrive at Mars after leaving Earth orbit.

ESCAPADE is led by the UC Berkeley Space Sciences Laboratory, which is responsible for mission management, systems engineering, science leadership, navigation, operations, the electron & ion electrostatic analyzers, and science data processing and archiving.

Key partners are Rocket Lab USA (spacecraft), NASA Goddard Space Flight Center (magnetometers), Embry Riddle Aeronautical University (Langmuir probes), Advanced Space LLC (mission design), and Blue Origin (launch).

Learn more about the two identical spacecraft designed, built, integrated, and tested by Rocket Lab for the University of California Berkeley’s Space Science Laboratory and NASA's Mars Mission:


Image Credit: Blue Origin
Image Date: Nov. 9, 2025


#NASA #Space #Astronomy #Science #Stars #Sun #SpaceWeather #Planets #Mars #Magnetosphere #MartianAtmosphere #ESCAPADEMission #ESCAPADESpacecraft #RocketLab #SolarSystem #SpaceExploration #GSFC #SSL #UCBerkeley #ERAU #AdvancedSpace #BlueOrigin #NewGlenn #JacklynLandingPlatform #LPV1 #CapeCanaveral #Florida #UnitedStates #STEM #Education

Saturday, November 08, 2025

Comet C/2025 A6 (Lemmon) Before Close Sun Approach | International Space Station

Comet C/2025 A6 (Lemmon) Before Close Sun Approach | International Space Station



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. Will it survive this encounter? It passed nearest to the Earth—about half of the Earth-Sun distance—on October 21.

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
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke

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: Japan Aerospace Exploration Agency (JAXA)/Kimiya Yui
Release Date: Nov. 8, 2025

#NASA #Space #Astronomy #Science #Earth #ISS #CometC2025A6Lemmon #AstronautVideography #Astronauts #KimiyaYui #油井亀美也 #Japan #日本 #JAXA #宇宙航空研究開発機構 #UnitedStates #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education

Comet C/2025 A6 (Lemmon), The Milky Way & Satellites | International Space Station

Comet C/2025 A6 (Lemmon), The Milky Way & Satellites | International Space Station

Expedition 73 astronaut Kimiya Yui of the Japan Aerospace Exploration Agency (JAXA): ". . . I'd like to introduce a freshly shot timelapse video for you to enjoy."

"It's a short clip right after sunset, featuring the Milky Way, Comet Lemmon, countless artificial satellites, and Japan all together."

"It looks like they're all competing in beauty, doesn't it?"

"May everyone have beautiful and pleasant dreams!"

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
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke

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: Japan Aerospace Exploration Agency (JAXA)/Kimiya Yui
Duration: 15 seconds
Release Date: Nov. 8, 2025

#NASA #Space #Astronomy #Science #Earth #ISS #CometC2025A6Lemmon #MilkyWayGalaxy #Satellites #AstronautVideography #Astronauts #KimiyaYui #油井亀美也 #Japan #日本 #JAXA #宇宙航空研究開発機構 #UnitedStates #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education #HD #Video