Wednesday, August 20, 2025

Russia Launches Biomedical Research Satellite Bion-M No.2 | Roscosmos

Russia Launches Biomedical Research Satellite Bion-M No.2 | Roscosmos

Russia launched the Bion-M No.2 satellite at 17:13 UTC on Wednesday, Aug. 20, 2025, aboard a Soyuz-2-1b rocket from Site 31/6 at the Baikonur Cosmodrome. This biomedical satellite is a continuation of a Soviet and later Russian scientific program. This started with the launch of Bion 1 back in 1973.

The Bion program aims to study the effects of microgravity and space environment on living organisms, a goal that Bion-M No.2 will advance by carrying out a comprehensive study of the combined biological effects of microgravity and high levels of cosmic radiation at the systemic, organ, cellular, and molecular levels on living animals and plants aboard the spacecraft. It carries several special instruments that will register the radiation load at distinct points inside the spacecraft.

The Bion program uses spacecraft that are based on the Zenit series of reconnaissance satellites, sharing the same basic design, in particular the reentry capsule and service module. The Zenit series was itself derived from the Vostok spacecraft, which carried the first humans into space in the 1960s.

Bion-M No.2 will spend 30 days in space, in an orbit averaging between 370 and 380 km above the Earth at an inclination of 96.62°. The mission had originally been planned to use a higher orbit, with an altitude of 800 km, but in the first half of 2025 this was changed so it would be closer to the planned orbit of the proposed Russian Orbital Station (ROS). The final orbital parameters for ROS, particularly its inclination, are still under discussion.

The main passengers aboard Bion-M No.2 are 75 four-month-old male laboratory mice of the most common C57BL/6 line, delivered to Moscow from the Novosibirsk breeding station. The mice will be used for experiment MLZh-02, which sees them divided into different groups. One is a control group of ordinary mice; the others consist of “knockout mice” with genes that determine the functioning of the body’s immune system, primarily in relation to radiation, have been altered.

The NRF2 gene, which regulates the detoxification and antioxidant protection system—directly related to resistance to radiation—is the focus of this research. In one group of mice, this has been altered to be more sensitive to radiation, while in another group it has been made less sensitive.

The mice were bred specifically for this spaceflight. From birth, they have lived in groups of three to ensure they will be comfortable and avoid aggression during the flight, where they will spend enclosed in cylindrical boxes, each containing three mice.

Most of the mice will be fed a food paste that combines both dry food (based on compound feed with a full set of essential vitamins and minerals) and water. The dosing device will dispense the paste six times a day. One group will receive solid food and water separately, delivered in the form of a gel.

Most rodents have sensors implanted under their skin to register their physiological parameters: body temperature and heart rate. There will be no real-time observation or live stream from the spacecraft: scientists from the Institute of Biomedical Problems (IMBP)—part of the Russian Academy of Sciences (RAS)—will receive only short videos during the flight that will allow them to assess whether everything is safe with the mice.

The full recordings from video cameras and data from the sensors will be available only after the spacecraft returns to Earth. The planned landing of Bion-M № 2 is on September 19, 2025, on the steppe in the Orenburg region.

In addition to the data collected by their sensors, scientists plan to study the behavior of the mice. These animals were trained to perform certain actions before the flight, and will be evaluated to see if they retain these skills after the mission, in order to study how the flight has affected their memory. Alexander Andreev-Andrievsky, the head of IMBP’s Laboratory of Animal Phenotyping, expanded on this in an interview ahead of the mission. “For example, to get something pleasant, we teach mice to poke their noses into a button. Whether they will remember this after the flight is a question. In addition, we plan to develop a new skill based on the existing one. This is necessary in order to understand how animals learn after flight”.

After the flight, the experiments on mice returned from space will begin immediately. The first tests will be carried out on them on the landing site; some of the rodents will be dissected on the first day, then on the 5th, 15th, and 30th days to check their level of recovery from the spaceflight. The rest of them will stay alive to check other parameters of their health.

The 25 cylindrical containers that will house the mice are larger than those on the previous mission, Bion-M No.1, launched in 2013. Each container has a diameter of 16 cm and a height of 12 cm. An automatically changing backlight has been added, creating the illusion of day and night for the mice.

Bion-M No.2 is also carrying over 1,000 Drosophila flies to study their reproduction. This follows on from an experiment flown on the Foton-M No.4 satellite in 2014. During that mission, the flies gave birth to offspring that were then sent back into space, to the Russian segment of the ISS. This experiment showed that the descendants surpassed their parents in reproductive activity. Bion-M No.2 aims to determine whether the higher levels of radiation it will be exposed to will affect how well the flies reproduce.

Seeds from 20 species of wild and cultivated plants are being carried on Bion-M No.2, including bupleurum aureum, Schrenck’s tulip, fern leaf peony, laser, Persian poppy, pepper, tomatoes, wheat, leafy crops, thale cress, apple three seeds, and others. The mission will evaluate the germination of seeds, study the effects of space conditions on the plants, and the post–flight development of seedlings.

Various microorganisms are also flying on board the satellite: anaerobic, spore-forming microorganisms and extremophiles that scientists collected in the thermal springs of Kamchatka and in Oymyakon, the coldest permanently inhabited place on Earth. They are a part of the Meteorite experiment, studying the theory that life may have been brought to Earth from space. It consists of granite disks with various microorganisms, embedded in the shell of the lander. After the flight, they will be removed and tested to determine which microorganisms have survived.

Other experiments aboard Bion-M No.2 include in vitro cell cultures placed in special containers with a controlled environment. As part of collaboration with the Laboratory of Geochemistry of the Moon and Planets, another institute of RAS, a container with 16 test tubes with a new lunar soil analog will be tested for use in future astrobiological experiments. These will be exposed to open space radiation for a month. Another experiment will test using microorganisms to generate electrical energy aboard the satellite. Another experiment will show if the microorganisms can be used for recycling of used clothes and other waste in spaceflight.

Furthermore, a place on board has been found for two experiments designed by school students. The first one, Ecosystem in Orbit, is a small transparent plexiglass container with ants embedded in it. The second is the Russo-Belarusian scholar experiment “Into Space with your Tomato”, consisting of tomato seeds.

The Bion-M No.2 mission comes over 12 years after the previous mission, Bion-M No.1, returned to Earth in May 2013. Although it was recovered successfully, it had been subject to failures of onboard equipment and the death of some of the animals, preventing its research program from being fully completed. Scientists are hoping for a better result when the Vostok-shaped Bion-M No.2 capsule returns to Earth at the end of September 2025.


Video Credit: Roscosmos
Article Credit: P. Katin/NASASpaceflight
Time: 1 minute
Date: Aug. 20, 2025

#NASA #Roscosmos #Роскосмос #Space #Satellite #BionMNo2Satellite #BionProgram #Science #Russia #Россия #Biomedicine #RadiationStudies #MicrogravityLaboratory #SoyuzRocket #Soyuz21bRocket #BaikonurCosmodrome #Kazakhstan #Қазақстан #STEM #Education #HD #Video

"Cosmic Hand": Pulsar B1509-58 in Circinus | NASA Chandra [Budget Cancellation]

"Cosmic Hand": Pulsar B1509-58 in Circinus | NASA Chandra [Budget Cancellation]

In 2009, NASA’s Chandra X-ray Observatory released a captivating image: a pulsar and its surrounding nebula that is shaped like a hand. Since then, astronomers have used Chandra and other telescopes to continue to observe this object. Now, new radio data from the Australia Telescope Compact Array has been combined with Chandra’s X-ray data to provide a fresh view of this exploded star and its environment and to help understand its unique properties.

At the center of this new image lies the pulsar B1509-58, a rapidly spinning neutron star that is only about 12 miles in diameter. This tiny object is responsible for producing an intricate nebula—called MSH 15-52—that spans over 150 light-years, or about 900 trillion miles. The nebula, produced by energetic particles, resembles a human hand with a palm and extended fingers pointing to the upper right in X-rays.

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:
NASA's Fiscal Year 2026 Budget Request (PDF) Document Download: https://www.nasa.gov/fy-2026-budget-request/ (See Fiscal Year 2026 Budget Request Summary)

The collapse of a massive star created the pulsar when much of the star crashed inward once it burned through its sustainable nuclear fuel. An ensuing explosion sent the star’s outer layers outward into space as a supernova.

The pulsar spins around almost seven times every second and has a strong magnetic field, about 15 trillion times stronger than the Earth’s. The rapid rotation and strong magnetic field make B1509-58 one of the most powerful electromagnetic generators in the Galaxy, enabling it to drive an energetic wind of electrons and other particles away from the pulsar, creating the nebula.

This new composite image from Chandra and radio data, plus an optical image, reveals complex filaments that are aligned with the directions of the nebula’s magnetic field, shown by the short straight lines when you mouse over the image. These filaments could result from the collision of the pulsar’s particle wind with the supernova’s debris.

By comparing the radio and X-ray data, researchers identified key variations between these two types of sources. This helps to reveal many unique features. There are, however, still many open questions regarding the formation and evolution of these structures. Further simulations are needed to provide a better understanding of the complex interplay between the pulsar wind and the supernova ejecta.


Video Credit: NASA's Chandra X-ray Observatory
Duration: 3 minutes
Release Date: Aug. 20, 2025

#NASA #Space #Astronomy #Science #Pulsars #Stars #NeutronStars #PSRB150958 #B1509 #Nebulae #MSH1552 #RCW89 #GasClouds #Circinus #Constellation #Cosmos #Universe #NASAChandra #ChandraObservatory #SpaceTelescopes #XrayAstronomy #ATCA #RadioAstronomy #Australia #MSFC #UnitedStates #STEM #Education #HD #Video

Planet Mars Images: Aug. 19-20, 2025 | NASA's Curiosity & Perseverance Rovers

Planet Mars Images: Aug. 19-20, 2025 | NASA's Curiosity & Perseverance Rovers

Mars 2020 - sol 1599
Mars 2020 - sol 1596
Mars 2020 - sol 1596
Mars 2020 - sol 1596
MSL - sol 4634
MSL - sol 4631
MSL - sol 4632
MSL - sol 4634

Celebrating 13+ Years on Mars (2012-2024)
Mission Name: Mars Science Laboratory (MSL)
Rover Name: Curiosity
Main Job: To determine if Mars was ever habitable to microbial life. 
Launch: Nov. 6, 2011
Landing Date: Aug. 5, 2012, Gale Crater, Mars

Celebrating 4+ Years on Mars
Mission Name: Mars 2020
Rover Name: Perseverance
Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.
Launch: July 30, 2020    
Landing: Feb. 18, 2021, Jezero Crater, Mars

For more information on NASA's Mars missions, visit: mars.nasa.gov

Image Credits: NASA/JPL-Caltech/ASU/MSSS
Processing: Kevin M. Gill
Image Release Dates: Aug. 19-20, 2025

#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #CuriosityRover #MSL #MountSharp #GaleCrater #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #MSSS #JPL #Caltech #UnitedStates #CitizenScience #KevinGill #STEM #Education

Orbital Earth Night Views | International Space Station

Orbital Earth Night Views | International Space Station

A vivid red and green aurora crowns Earth’s horizon over the southern Indian Ocean in this photo from the International Space Station as it orbited 270 miles above. At top left, a lit window reveals the docked SpaceX Dragon crew spacecraft docked to the orbital outpost's forward port on the Harmony module, set against a starry sky captured with long-exposure, low-light settings.
A wispy aurora spikes across the Indian Ocean with a set of the International Space Station's main solar arrays (augmented by its rollout solar arrays) draping the foreground. At right, is the unoccupied Rassvet module that hosts visiting spacecraft from Roscosmos. The orbital outpost was soaring 270 miles above Earth southwest of Australia at the time of this photograph.
The aurora australis appears to lap over the Earth like a tide washing ashore in this photograph taken at approximately 3:45 a.m. local time from the International Space Station as it orbited 269 miles above the Indian Ocean southwest of Australia.
The warm city lights of Southeast Asia streak below the silvery U.S. segment of the International Space Station in this 30-second exposure from the orbital outpost as it soared 259 miles above China at approximately 10:39 a.m. local time. Near the top center, is the partially obscured SpaceX Dragon spacecraft that docked to the Harmony module's forward port carrying NASA's Crew-11 mission.
The International Space Station soars 259 miles above Cambodia in this long-duration photograph revealing star trails, lightning storms, and the city lights of Southeast Asia streaking below.

Auroras happen when charged particles from the Sun interact with Earth's magnetic field, creating dazzling light shows in the sky. Auroras occurs in an upper layer of Earth’s atmosphere called the ionosphere.


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: NASA's Johnson Space Center
Image Dates: July 22-28, 2025


#NASA #Space #ISS #Science #Stars #Planets #Earth #Aurora #IndianOcean #SoutheastAsia #Astronauts #AstronautPhotography #Japan #JAXA #Cosmonauts #Russia #Россия #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education

Tuesday, August 19, 2025

China's CAS Space: Kinetica-1 Y10 Commercial Rocket Launch of Mexican Satellites

China's CAS Space: Kinetica-1 Y10 Commercial Rocket Launch of Mexican Satellites








🚀A CAS Space Kinetica-1 Y10 carrier rocket blasted off at 3:33 p.m. Beijing Time on August 19, 2025, successfully sending seven satellites into orbit from the Dongfeng Commercial Aerospace Innovation Pilot Zone at the Jiuquan Satellite Launch Center (JSLC) in northwest China.

The satellites on this rideshare included Zhongke Satellite-05, Multi-functional Test Satellites No. 2-01, 02, and 03, Tianyan-26, plus ThumbSat-1, and ThumbSat-2 for Mexico. 

This marks the eighth successful flight mission of the Kinetica-1 launch vehicle and the forty-eighth launch for China in 2025. 

Notably, the Kinetica-1 Y10 rocket was painted with calligraphy representing the “Women of China”. The marking is part of CAS Space's collaboration with the All-China Women’s Federation to celebrate progress in equality as well as the contributions of the country's 689 million women. Through the mission's success, CAS Space wishes to convey this message and to recognize the achievements of all women worldwide.

Mission Y10 has been declared a complete success. A total of 70 satellites, or 7 tons of payload, have now been delivered by Kinetica-1 rockets since its debut with more to come this year.

CAS Space is a Chinese commercial space launch provider based in Guangzhou, the capital and largest city of Guangdong province in southern China. CAS Space was founded in 2018 and is majority owned by the Chinese Academy of Sciences (CAS).

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 CAS Space.


Image Credits: CAS Space/Wang Heng/Wang Jiangbo/Wang Haixia
Image Date: Aug. 19, 2025

#NASA #Space #Satellites #Earth #China #中国 #CASSpace #中科宇航 #CAS #中国科学院 #Kinetica1Y10 #LaunchVehicles #SolidFuelRockets #CommercialSatellites #ThumbSat1 #ThumbSat2 #Mexico #CommercialSpace #JSLC #STEM #Education

China's CAS Space: Kinetica-1 Y10 Commercial Rocket Launch of Mexican Satellites

China's CAS Space: Kinetica-1 Y10 Commercial Rocket Launch of Mexican Satellites

🚀A CAS Space Kinetica-1 Y10 carrier rocket blasted off at 3:33 p.m. Beijing Time on August 19, 2025, successfully sending seven satellites into orbit from the Dongfeng Commercial Aerospace Innovation Pilot Zone at the Jiuquan Satellite Launch Center (JSLC) in northwest China.

The satellites on this rideshare included Zhongke Satellite-05, Multi-functional Test Satellites No. 2-01, 02, and 03, Tianyan-26, plus ThumbSat-1, and ThumbSat-2 for Mexico. 

This marks the eighth successful flight mission of the Kinetica-1 launch vehicle and the forty-eighth launch for China in 2025. 

Notably, the Kinetica-1 Y10 rocket was painted with calligraphy representing the “Women of China”. The marking is part of CAS Space's collaboration with the All-China Women’s Federation to celebrate progress in equality as well as the contributions of the country's 689 million women. Through the mission's success, CAS Space wishes to convey this message and to recognize the achievements of all women worldwide.

Mission Y10 has been declared a complete success. A total of 70 satellites, or 7 tons of payload, have now been delivered by Kinetica-1 rockets since its debut with more to come this year.

CAS Space is a Chinese commercial space launch provider based in Guangzhou, the capital and largest city of Guangdong province in southern China. CAS Space was founded in 2018 and is majority owned by the Chinese Academy of Sciences (CAS).

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 CAS Space.


Video Credit: CAS Space
Duration: 34 seconds
Release Date: Aug. 19, 2025

#NASA #Space #Satellites #Earth #China #中国 #CASSpace #中科宇航 #CAS #中国科学院 #Kinetica1Y10 #LaunchVehicle #SolidFuelRockets #CommercialSatellites #ThumbSat1 #ThumbSat2 #Mexico #CommercialSpace #JSLC #STEM #Education #HD #Video

Giant Galaxies in Pavo (AI Narration)

Giant Galaxies in Pavo (AI Narration)

Over 500,000 light years across, NGC 6872 (bottom left) is a truly enormous barred spiral galaxy. At least five times the size of our own large Milky Way, NGC 6872 is the largest known spiral galaxy. About 200 million light-years distant toward the southern constellation Pavo, the Peacock, the appearance of this giant galaxy's stretched out spiral arms suggest the wings of a giant bird. So its popular moniker is the Condor Galaxy. Lined with massive young, bluish star clusters and star-forming regions, the extended and distorted spiral arms are due to NGC 6872's past gravitational interactions with the nearby smaller galaxy IC 4970, visible here below the giant spiral galaxy's core. 

Other members of the southern Pavo galaxy group are scattered through this magnificent galaxy group portrait, with the dominant giant elliptical galaxy, NGC 6876, above and right of the soaring Condor galaxy.


Credit & Copyright: Adam Block
Adam's website: 
Time: 1 minute, 51 seconds
Release Date: Aug. 19, 2025


#NASA #Astronomy #Space #Science #Galaxies #Galaxy #NGC6872 #CondorGalaxy #SpiralGalaxies #IC4970 #InteractingGalaxies #NGC6876 #EllipticalGalaxies #Pavo #Constellation #Cosmos #Universe #Astrophotography #AdamBlock #Astrophotographer #GSFC #UnitedStates #STEM #Education #HD #Video

Giant Galaxies in Pavo

Giant Galaxies in Pavo

Over 500,000 light years across, NGC 6872 (bottom left) is a truly enormous barred spiral galaxy. At least five times the size of our own large Milky Way, NGC 6872 is the largest known spiral galaxy. About 200 million light-years distant toward the southern constellation Pavo, the Peacock, the appearance of this giant galaxy's stretched out spiral arms suggest the wings of a giant bird. So its popular moniker is the Condor Galaxy. Lined with massive young, bluish star clusters and star-forming regions, the extended and distorted spiral arms are due to NGC 6872's past gravitational interactions with the nearby smaller galaxy IC 4970, visible here below the giant spiral galaxy's core. 

Other members of the southern Pavo galaxy group are scattered through this magnificent galaxy group portrait, with the dominant giant elliptical galaxy, NGC 6876, above and right of the soaring Condor galaxy.


Image Credit & Copyright: Adam Block
Adam's website: 
https://www.adamblockphotos.com
Release Date: Aug. 19, 2025


#NASA #Astronomy #Space #Science #Galaxies #Galaxy #NGC6872 #CondorGalaxy #SpiralGalaxies #IC4970 #InteractingGalaxies #NGC6876 #EllipticalGalaxies #Pavo #Constellation #Cosmos #Universe #Astrophotography #AdamBlock #Astrophotographer #GSFC #UnitedStates #STEM #Education

Views of Hurricane Erin | International Space Station

Views of Hurricane Erin | International Space Station

The International Space Station flew 260 miles over Hurricane Erin at 11:41 a.m. EDT Tuesday, Aug. 19, 2025. External cameras on the orbiting laboratory captured views of the hurricane as it traveled northwest through the Caribbean with maximum sustained wind speeds of 105 mph. Hurricane Erin is not expected to make landfall and is projected to move between the U.S. East coast and Bermuda before heading out into the Atlantic Ocean.


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: NASA Video
Duration: 3 minutes
Release Date: Aug. 19, 2025


#NASA #Space #ISS #Science #Planets #Earth #AtlanticOcean #Weather #Meteorology #HurricaneErin #Astronauts #AstronautPhotography #UnitedStates #Japan #日本 #JAXA #宇宙航空研究開発機構 #Cosmonauts #Russia #Россия #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education #HD #Video

Circular Arcs of Star Trails | International Space Station

Circular Arcs of Star Trails International Space Station


This long-exposure photograph, taken over 31 minutes from a window inside the International Space Station’s Kibo laboratory module, captures circular arcs of star trails. In the foreground is a portion of Kibo’s Exposed Facility, where a variety of payloads and experiments can be mounted for direct exposure to the vacuum of space. The Japanese Experiment Module—Kibo—is Japan’s contribution to the International Space Station (ISS). Kibō (meaning 'Hope' in Japanese) is a Japanese science module developed by the Japan Aerospace Exploration Agency (JAXA). It is the largest single ISS module, and is attached to the Harmony module.

Learn more about Kibō:
https://humans-in-space.jaxa.jp/en/kibo/


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: NASA's Johnson Space Center
Image Date: July 26, 2025


#NASA #Space #ISS #Science #Stars #StarTrails #Planets #Earth #Astronauts #AstronautPhotography #TimelapsePhotography #Kibo #きぼう#Japan #日本 #JAXA #宇宙航空研究開発機構 #Cosmonauts #Russia #Россия #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education

New Moon Discovered Orbiting Planet Uranus | James Webb Space Telescope

New Moon Discovered Orbiting Planet Uranus | James Webb Space Telescope

This timelapse animation shows the newly discovered moon of the planet Uranus, designated S/2025 U1, as well as 13 of the 28 other known moons orbiting the planet. The observations by NASA’s James Webb Space Telescope’s Near-Infrared Camera (NIRCam) were taken over the course of about 6 hours on Feb. 2, 2025, under program ID 6379 (principal investigator: M. El Moutamid). 

The animation is comprised of data taken with NIRCam’s wide band F150W2 filter that transmits infrared wavelengths from about 1.0 to 2.4 microns. Due to the drastic differences in brightness levels, the animation is a composite of three separate treatments of the data, allowing the viewer to see details in the planetary atmosphere, the surrounding rings, and the orbiting moons. The small moon Cordelia orbits just inside the outermost ring, but is not visible in these views due to glare from the rings.


Video Credit: National Aeronautics and Space Administration (NASA)
Animation: NASA, ESA, CSA, STScI, Maryame El Moutamid (SwRI), Matthew Hedman (University of Idaho), Joseph DePasquale (STScI)
Duration: 17 seconds
Release Date: Aug. 19, 2025


#NASA #Astronomy #Space #Science #NASAWebb #SolarSystem #Planets #Uranus #Moons #Moon #S2025U1 #Cosmos #Universe #UnfoldTheUniverse #JWST #NIRCam #InfraredAstronomy #ESA #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education #Animation #HD #Video

NASA Artemis III Moon Rocket Processing Begins | Kennedy Space Center

NASA Artemis III Moon Rocket Processing Begins | Kennedy Space Center

Teams from NASA’s Kennedy Space Center in Florida transport the engine section of the agency’s Artemis III Space Launch System (SLS) core stage from the spaceport’s Space Systems Processing Facility to the center’s Vehicle Assembly Building on Tuesday, July 29, 2025. The engine section is one the most complex and intricate parts of the rocket stage that will help power the Artemis missions to the Moon.
Teams from NASA’s Kennedy Space Center in Florida integrate NASA’s Artemis III Space Launch System (SLS) core stage engine section with its boat-tail inside the spaceport’s Vehicle Assembly Building on Wednesday, July 30, 2025. 
Teams from NASA’s Kennedy Space Center in Florida transport the engine section of the agency’s Artemis III Space Launch System (SLS) core stage from the spaceport’s Space Systems Processing Facility to the center’s Vehicle Assembly Building on Tuesday, July 29, 2025.
Teams from NASA’s Kennedy Space Center in Florida transport the engine section of the agency’s Artemis III Space Launch System (SLS) core stage from the spaceport’s Space Systems Processing Facility to the center’s Vehicle Assembly Building on Tuesday, July 29, 2025.
Teams from NASA’s Kennedy Space Center in Florida transport the engine section of the agency’s Artemis III Space Launch System (SLS) core stage from the spaceport’s Space Systems Processing Facility to the center’s Vehicle Assembly Building on Tuesday, July 29, 2025.
Teams from NASA’s Kennedy Space Center in Florida integrate NASA’s Artemis III Space Launch System (SLS) core stage engine section with its boat-tail inside the spaceport’s Vehicle Assembly Building on Wednesday, July 30, 2025.
Teams from Kennedy lift NASA’s integrated Artemis III Space Launch System (SLS) core stage engine section with its boat-tail inside the center’s Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida on Wednesday, Aug. 13, 2025.
Teams from Kennedy lift NASA’s integrated Artemis III Space Launch System (SLS) core stage engine section with its boat-tail inside the center’s Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida on Wednesday, Aug. 13, 2025. Shown inside the facility’s High Bay 2 for processing, the engine section is one the most complex and intricate parts of the rocket stage that will help power the Artemis missions to the Moon. 

Buildup of NASA’s Space Launch System (SLS) rocket for the Artemis III lunar mission has started at the agency’s Kennedy Space Center in Florida, even as NASA prepares for the launch of the Artemis II mission, the second Artemis mission in NASA’s efforts to return humans to the Moon and eventually land on Mars.

The Artemis III SLS engine section and boat-tail that protects the engines during launch moved from the Space Systems Processing Facility (SSPF) at NASA Kennedy to the mammoth Vehicle Assembly Building (VAB) in late July, just a few feet from where the Artemis II SLS is mostly stacked and undergoing integrated testing and checkouts.

This engine section is one the most complex and intricate parts of the rocket stage that will help power the Artemis missions to the Moon.

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.

Learn more about the Artemis campaign: 
https://www.nasa.gov/humans-in-space/artemis/
Follow updates on the Artemis blog: 
https://blogs.nasa.gov/artemis/
NASA's Space Launch System (SLS)
https://www.nasa.gov/sls
NASA's Artemis III Mission:
https://www.nasa.gov/mission/artemis-iii/
Read the Artemis Plan (74-page PDF Free Download): 
https://www.nasa.gov/sites/default/files/atoms/files/artemis_plan-20200921.pdf


Image Credit: NASA/Cory Huston
Image Dates: July 29-Aug. 13, 2025

 

#NASA #Space #Earth #Moon #Artemis #ArtemisIII #SLS #SLSRocket #CoreStage #Boeing #CrewedMissions #DeepSpace #MoonToMars #Science #Engineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NASAKennedy #KSC #MerrittIsland #Florida #UnitedStates #STEM #Education

Monday, August 18, 2025

NASA’s Quesst Mission: X-59 Quiet Supersonic Aircraft Testing | NASA Armstrong

NASA’s Quesst Mission: X-59 Quiet Supersonic Aircraft Testing | NASA Armstrong

NASA’s X-59 quiet supersonic research aircraft sits on the ramp at sunrise before ground tests at Lockheed Martin’s Skunk Works facility in Palmdale, California, on July 18, 2025.
NASA test pilot Nils Larson lowers the canopy of the X-59 quiet supersonic research aircraft during ground tests at Lockheed Martin’s Skunk Works facility in Palmdale, California, on July 18, 2025.
NASA’s X-59 quiet supersonic research aircraft taxis across the runway during a low-speed taxi test at U.S. Air Force Plant 42 in Palmdale, California, on July 10, 2025. The test marks the start of taxi tests and the last series of ground tests before first flight.
Here you see the X-59 scaled model inside the Japan Aerospace Exploration Agency (JAXA) supersonic wind tunnel during critical tests related to sound predictions.

The X-59 is the centerpiece of NASA’s Quesst Mission to demonstrate quiet supersonic flight. The aircraft is scheduled to make its first flight later in 2025. NASA’s X-59 quiet supersonic research aircraft has completed taxi tests, marking the first time this one-of-a-kind experimental aircraft has moved under its own power. The aircraft completed its first low-speed taxi test, allowing engineers and flight crews to monitor how it handled moving across the runway under its own power. Taxi tests mark the final major ground test before flight operations begin. 

NASA’s Quesst Mission aims to demonstrate quiet supersonic flight by reducing the loud sonic boom to a quieter “thump”. Data gathered during X-59 research flights will be shared with the U.S. and international regulators to inform the establishment of new, data-driven acceptable noise thresholds related to supersonic commercial flight over land.

The X-59’s engine, a modified F414-GE-100, packs 22,000 pounds of thrust. This will enable the X-59 to achieve the desired cruising speed of Mach 1.4 (925 miles per hour) at an altitude of approximately 55,000 feet. It sits in a nontraditional spot–atop the aircraft—to aid in making the X-59 quieter.

The X-59's goal is to help change existing national and international aviation rules that ban commercial supersonic flight over land.



Image Credits: NASA/Carla Thomas, Lockheed Martin Corporation/Garr, Japan Aerospace Exploration Agency (JAXA)
Image Dates: July 10-17, 2025

#NASA #Aerospace #SupersonicFlight #SupersonicAircraft #X59 #Sonicboom #QuietAviation #Aviation #QuesstMission #CommercialAviation #Science #Physics #Engineering #AerospaceResearch #AeronauticalResearch #FlightTests #LockheedMartin #SkunkWorks #NASAArmstrong #AFRC #Palmdale #California #UnitedStates #JAXA #Japan #STEM #Education

Close-up: Galaxy NGC 4900—A Spiral and a Star in Virgo | Hubble

Close-up: Galaxy NGC 4900A Spiral and a Star in Virgo | Hubble

This NASA/European Space Agency Hubble Space Telescope picture features a sparkling spiral galaxy paired with a prominent star, both in the constellation Virgo. While the galaxy and the star appear to be close to one another, even overlapping, they are actually a great distance apart. The star, marked with four long diffraction spikes, is in our own galaxy. It is just 7,109 light-years away from Earth. The galaxy, named NGC 4900, lies about 45 million light-years from Earth.

This image combines data from two of Hubble’s instruments: the Advanced Camera for Surveys, installed in 2002 and is still in operation today, and the older Wide Field and Planetary Camera 2—in use from 1993 to 2009. The data used here were taken more than 20 years apart for two different observing programs—a real testament to Hubble’s long scientific lifetime.

Both programs aimed to understand the demise of massive stars. In one, researchers studied the sites of past supernovae, aiming to estimate the masses of the stars that exploded and investigate how supernovae interact with their surroundings. NGC 4900 was selected for study because it hosted a supernova named SN 1999br.

In the other program, researchers laid the groundwork for studying future supernovae by collecting images of more than 150 nearby galaxies. After a supernova is detected in one of these galaxies, researchers can examine these images, searching for a star at the location of the supernova. Identifying a supernova progenitor star in pre-explosion images gives valuable information about how, when and why supernovae occur.

Image Description: A spiral galaxy seen face-on. Broken spiral arms made of blue patches of stars and thin strands of dark dust swirl around the galaxy’s center, forming a broad, circular disc. An extended circular halo surrounds the disc. The center is a brightly-glowing, stubby bar-shaped area in a pale yellow color. A bright star in our own galaxy, with long cross-shaped diffraction spikes, is visible atop the distant galaxy.


Credit: ESA/Hubble & NASA, S. J. Smartt, C. Kilpatrick
Time: 30 seconds
Release Date: March 10, 2025


#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #Galaxies #Galaxy #NGC900 #SpiralGalaxy #Virgo #Constellation #Star #MilkyWayGalaxy #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Close-up: Spiral Galaxy UGC 11397 in Lyra | Hubble

Close-up: Spiral Galaxy UGC 11397 in Lyra | Hubble

The light that the NASA/European Space Agency Hubble Space Telescope collected to create this picture reached the telescope after a journey of 250 million years. Its source was the spiral galaxy UGC 11397. It resides in the constellation Lyra (The Lyre). At first glance, UGC 11397 appears to be an average spiral galaxy. It sports two graceful spiral arms that are illuminated by stars and defined by dark, clumpy clouds of dust.

What sets UGC 11397 apart from a typical spiral lies at its center, where a supermassive black hole containing 174 million times the mass of the Sun is growing. As a black hole ensnares gas, dust, and even entire stars from its vicinity, this doomed matter heats up and puts on a fantastic cosmic light show. Material trapped by the black hole emits light from gamma rays to radio waves and can brighten and fade without warning. However, in galaxies like UGC 11397, thick clouds of dust hide much of this energetic activity from view in optical light.  Despite this, UGC 11397's actively growing black hole was revealed through its bright X-ray emission—high-energy light that can pierce the surrounding dust. This led astronomers to classify it as a Type 2 Seyfert galaxy, a category used for active galaxies whose central regions are hidden from view in visible light by a doughnut-shaped cloud of dust and gas.

Using Hubble, researchers will study hundreds of galaxies that, like UGC 11397, harbor a supermassive black hole that is gaining mass. The Hubble observations will help researchers weigh nearby supermassive black holes, understand how black holes grew early in the Universe’s history, and even study how stars form in the extreme environment found at the very center of a galaxy.

Image Description: A spiral galaxy seen at an angle that gives it an oval shape. It has two spiral arms that curl out from the center. They start narrow but broaden out as they wrap around the galaxy before merging into a faint halo. The galaxy’s disc is golden in the center with a bright core, and pale blue outside that. A swirl of dark dust strands and speckled blue star-forming regions follow the arms through the disc.


Credit: ESA/Hubble & NASA, M. J. Koss, A. J. Barth, N. Bartmann (ESA/Hubble)
Duration: 30 seconds
Release Date: June 23, 2025


#NASA #ESA #Astronomy #Space #Science #Hubble #Hubble35 #Galaxies #Galaxy #UGC11397 #SpiralGalaxy #SuperMassiveBlackHole #BlackHoles #Type2SeyfertGalaxy #Lyra #Constellation #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Close-up: Galaxy Cluster Abell 209 in Cetus | Hubble Space Telescope

Close-up: Galaxy Cluster Abell 209 in Cetus | Hubble Space Telescope

A massive, spacetime-warping cluster of galaxies is the setting of this NASA/European Space Agency Hubble Space Telescope picture. The galaxy cluster in question is Abell 209. It is located 2.8 billion light-years away in the constellation Cetus (The Whale).

This Hubble image of Abell 209 shows more than a hundred galaxies, but there is more to this cluster than even Hubble’s discerning eye can see. Abell 209’s galaxies are separated by millions of light-years, and the seemingly empty space between the galaxies is actually filled with hot, diffuse gas that can be spotted only at X-ray wavelengths. An even more elusive occupant of this galaxy cluster is dark matter: a form of matter that does not interact with light. The Universe is understood to be comprised of 5% normal matter, 25% dark matter, and 70% dark energy

Hubble observations like the ones used to create this image can help astronomers answer fundamental questions about our Universe, including mysteries surrounding dark matter and dark energy. These investigations leverage the immense mass of a galaxy cluster. This can bend the fabric of spacetime itself and create warped and magnified images of background galaxies and stars in a process called gravitational lensing.

While this image lacks the dramatic rings that gravitational lensing can sometimes create, Abell 209 still shows subtle signs of lensing at work, in the form of streaky, slightly curved galaxies within the cluster’s golden glow. By measuring the distortion of these galaxies, astronomers can map the distribution of mass within the cluster, illuminating the underlying cloud of dark matter. This information, which Hubble’s fine resolution and sensitive instruments help to provide, is critical for testing theories of how our Universe has evolved.

Image Description: A cluster of distant, mainly elliptical galaxies. They appear as brightly shining points radiating golden light that each take the shape of a smooth, featureless oval. They crowd around one that is extremely large and bright. A few spiral galaxies of comparable size appear too, bluer in color and with unique shapes. Of the other, more small and distant galaxies covering the scene, a few are warped into long lines.


Credit: ESA/Hubble & NASA, M. Postman, P. Kelly, N. Bartmann (ESA/Hubble)
Time: 30 seconds
Release Date: July 7, 2025

#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #Galaxies #GalaxyClusters #Abell209 #Cetus #Constellation #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video