Thursday, August 21, 2025

'Squid Galaxy': NGC 1068 in Cetus | Webb+VLA+Hubble+Chandra [Budget Alert]

'Squid Galaxy': NGC 1068 in Cetus Webb+VLA+Hubble+Chandra [Budget Alert]


A new eye-catching compilation of images is being released that features data from NASA’s Chandra X-ray Observatory along with a host of other telescopes, including NASA’s James Webb Space Telescope.

NGC 1068 is a relatively nearby spiral galaxy containing a black hole at its center that is twice as massive as the Milky Way’s. Chandra shows a million-mile-per-hour wind is being driven from NGC 1068’s black hole and lighting up the center of the galaxy in X-rays.

X-rays from Chandra (blue), radio data from NSF’s VLA radio data (pink), and optical data from Hubble and Webb (yellow, grey and gold)

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:

Image Description: This nearby spiral galaxy is viewed face-on with its tightly packed golden arms and faint purple clouds spiraling around a hazy core. There, million-mile-per-hour winds swirl around a glowing black hole.


Image Credit: X-ray: NASA/CXC/SAO; Optical/IR: NASA/ESA/CSA/STScI (HST and JWST); Radio: NSF/NRAO/VLA; Image Processing: NASA/CXC/SAO/J. Schmidt and N. Wolk
Release Date: Aug. 21, 2025


#NASA #ESA #Astronomy #Space #Science #Galaxies #Galaxy #SquidGalaxy #Messier77 #SeyfertGalaxies #Cetus #Constellations #Universe #JWST #HST #NASAChandra #SpaceTelescopes #GSFC #STScI #CSA #Canada #VLA #UnitedStates #Europe #STEM #Education

Star-forming Region IC 348 in Perseus | Webb & Chandra Space Telescopes

Star-forming Region IC 348 in Perseus | Webb & Chandra Space Telescopes

A new eye-catching compilation of images is being released that features data from NASA’s Chandra X-ray Observatory along with a host of other telescopes, including NASA’s James Webb Space Telescope.

IC 348 is a star-forming region in our Milky Way galaxy. The wispy structures that dominate the image are interstellar material that reflect the light from the cluster’s stars. The point-like sources in Chandra’s X-ray data are young stars in the cluster developing there.

This is the central portion of the star cluster IC 348. Astronomers combed the cluster in search of tiny, free-floating brown dwarfs: objects too small to be stars but larger than most planets. They found three brown dwarfs that are less than eight times the mass of Jupiter. The smallest weighs just three to four times as much as Jupiter, challenging theories for star formation.

The wispy curtains filling the image are interstellar material reflecting the light from the cluster’s stars—what is known as a reflection nebula. The material also includes carbon-containing molecules known as polycyclic aromatic hydrocarbons, or PAHs. The bright star closest to the center of the frame is actually a pair of type B stars in a binary system, the most massive stars in the cluster. Winds from these stars may help sculpt the large loop seen on the right side of the field of view.

X-rays from Chandra (red, green and blue) and Webb infrared data (pink, orange and purple)


Credit: X-ray: NASA/CXC/SAO; Infrared: NASA/ESA/CSA/STScI; Image Processing: NASA/CXC/SAO/J. Major
Release Date: Aug. 21, 2025

#NASA #Space #Astronomy #Science #Stars #Starclusters #Starcluster #IC348 #BrownDwarfStars #ReflectionNebula #Perseus #Constellation #MilkyWayGalaxy #Universe #UnfoldTheUniverse #JWST #NASAChandra #SpaceTelescopes #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education

Star Cluster Westerlund 1 | Webb, Hubble & Chandra Space Telescopes [Budget Alert]

Star Cluster Westerlund 1 | Webb, Hubble & Chandra Space Telescopes [Budget Alert]


A new eye-catching compilation of images is being released that features data from NASA’s Chandra X-ray Observatory along with a host of other telescopes including NASA’s James Webb Space Telescope. Westerlund 1 is the biggest and closest “super” star cluster to Earth. Data from Chandra and other telescopes is helping astronomers delve deeper into this galactic factory where stars are vigorously being produced. Observations from Chandra have uncovered thousands of individual stars pumping out X-ray emission into the cluster.

The open cluster Westerlund 1 is located roughly 12,000 light-years away in the southern constellation Ara (the Altar) where it resides behind a huge interstellar cloud of gas and dust. It was discovered in 1961 from Australia by Swedish astronomer Bengt Westerlund. Westerlund 1 is an incomparable natural laboratory for the study of extreme stellar physics, helping astronomers to find out how the most massive stars in our Galaxy live and die.

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:

The unique draw of Westerlund 1 is its large, dense, and diverse population of massive stars, which has no counterpart in other known Milky Way galaxy clusters in terms of the number of stars and the richness of spectral types and evolutionary phases. All stars identified in this cluster are evolved and very massive, spanning the full range of stellar classifications including Wolf-Rayet stars, OB supergiants, yellow hypergiants (nearly as bright as a million Suns) and luminous blue variables. Because such stars have a rather short life, Westerlund 1 is very young, astronomically speaking. Astronomers estimate the cluster’s age to be somewhere between 3.5 and 5 million years (its exact age is still a matter of debate), making it a newborn cluster in our galaxy. In the future, it is believed that it will likely evolve from an open cluster into a globular cluster. These are roughly spherical, tightly packed collections of old stars bound together by gravity.

Currently, only a handful of stars form in our galaxy each year, but in the past the situation was different. The Milky Way galaxy used to produce many more stars, likely hitting its peak of churning out dozens or hundreds of stars per year about 10 billion years ago and then gradually declining ever since. Astronomers think that most of this star formation took place in massive clusters of stars, known as “super star clusters”. These are young clusters of stars that contain more than 10,000 times the mass of the Sun, packed into an unbelievably small volume. They represent the most extreme environments in which stars and planets can form. Only a few super star clusters still exist in our galaxy—Westerlund 1 is one—but they offer important clues about this earlier era when most of our galaxy’s stars formed.

Westerlund 1 is an impressive example of a super star cluster: it contains hundreds of very massive stars, a number shining with a brilliance of almost one million Suns and others two thousand times larger than the Sun (as large as the orbit of Saturn). Indeed, if the Solar System was located at the heart of this remarkable cluster, our sky would be full of hundreds of stars as bright as the full Moon. It appears to be the most massive compact young cluster yet identified in the Milky Way galaxy: astronomers believe that this extreme cluster contains between 50,000 and 100,000 times the mass of the Sun, yet all of its stars are located within a region less than six light-years across. Even so, it is the biggest of these remaining super star clusters in the Milky Way galaxy, and the closest super star cluster to Earth. These qualities make Westerlund 1 an excellent target for studying the impact of a super star cluster’s environment on the formation process of stars and planets, as well as the evolution of stars over a broad range of masses.

The huge population of massive stars in Westerlund 1 suggests that it will have a very significant impact on its surroundings. The cluster contains so many massive stars that in a time span of less than 40 million years, it will be the site of more than 1,500 supernovae. This super star cluster now provides astronomers with a unique perspective towards one of the most extreme environments in the Universe. Westerlund 1 will certainly provide new opportunities in the long-standing quest for more and finer details about how stars, and especially massive stars, form.

X-rays from Chandra (pink, blue, purple and orange) with Webb infrared data (yellow, gold and blue) and Hubble optical data (cyan, grey and light yellow)


Image Credit: X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI; IR: NASA/ESA/CSA/STScI; Image Processing: NASA/CXC/SAO/L. Frattare
Release Date: Aug. 21, 2025


#NASA #ESA #Astronomy #Space #Science #StarClusters #Westerlund1 #StarCluster #Stars #HypergiantStars #RedSupergiants #Ara #Constellation Universe #JWST #HST #NASAChandra #SpaceTelescopes #STScI #GSFC #UnitedStates #Europe #CSA #Canada #STEM #Education

Close-up: Ghostly Galaxy LEDA 22057 in Gemini | Hubble

Close-up: Ghostly Galaxy LEDA 22057 in Gemini | Hubble

This NASA/European Space Agency Hubble Space Telescope picture features the galaxy LEDA 22057. It is located about 650 million light-years away in the constellation Gemini. LEDA 22057 is the site of a supernova explosion, named SN 2024PI, that was discovered by an automated survey in January 2024. The survey covers the entire northern half of the night sky every two days and has cataloged over 10,000 supernovae.

The supernova is visible in this image: located just down and to the right of the galactic nucleus, the pale blue dot of SN 2024PI stands out against the galaxy’s ghostly spiral arms. This image was taken about a month and a half after the supernova was discovered, so the supernova is seen here many times fainter than its maximum brilliance.

SN 2024PI is classified as a Type Ia supernova. This type of supernova requires a remarkable object called a white dwarf, the crystallized core of a star with a mass less than about eight times the mass of the Sun. When a star of this size uses up the supply of hydrogen in its core, it balloons into a red giant, becoming cool, puffy and luminous. Over time, pulsations and stellar winds cause the star to shed its outer layers, leaving behind a white dwarf and a colorful planetary nebula. White dwarfs can have surface temperatures higher than 100,000 degrees and are extremely dense, packing roughly the mass of the Sun into a sphere the size of Earth. 

While nearly all of the stars in the Milky Way will one day evolve into white dwarfs—this is the fate that awaits the Sun some five billion years in the future—not all of them will explode as Type Ia supernovae. For that to happen, the white dwarf must be a member of a binary star system. When a white dwarf syphons material from a stellar partner, the white dwarf can become too massive to support itself. The resulting burst of runaway nuclear fusion destroys the white dwarf in a supernova explosion that can be seen many galaxies away.

Image Description: A spiral galaxy with two thin, slowly-curving arms, one fainter than the other, coming off the tips of a bright, oval-shaped core region. The disc of the galaxy is also oval-shaped and filled with fuzzy dust under the arms. It has bright spots where stars are concentrated, especially along the arms. The core has a white glow in the center and thick bands of gas around it. A supernova is visible as a pale blue dot near the core.


Credit: ESA/Hubble & NASA, R. J. Foley (UC Santa Cruz)
Duration: 30 seconds
Release Date: Dec. 30, 2024


#NASA #Hubble #Astronomy #Space #Science #Galaxies #Galaxy #LEDA22057 #Supernovae #SN2024PI #TypeIA #Gemini #Constellation #MilkyWayGalaxy #Cosmos #Universe #HST #HubbleSpaceTelescope #ESA #Europe #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Hurricane Erin in Atlantic Ocean | NOAA Weather Satellite [Budget Cut Alert]

Hurricane Erin in Atlantic Ocean | NOAA Weather Satellite [Budget Cut Alert]

At 11:00 AM EDT (1500 UTC), August, 21, 2025, the center of Hurricane Erin was located near latitude 35.4 North, longitude 70.9 West. Erin is moving toward the north-northeast near 18 mph (30 km/h). A faster northeastward to east-northeastward motion is expected during the next couple of days. On the forecast track, the center of Erin will move over the western Atlantic between the U.S. east coast and Bermuda through early Friday, and then pass south of Atlantic Canada Friday and Saturday.
 
Maximum sustained winds are near 100 mph (155 km/h) with higher gusts.  Gradual weakening is forecast during the next couple of days.  Erin is expected to become post-tropical on Saturday.
 
Erin is a very large hurricane. Hurricane-force winds extend outward up to 105 miles (165 km) from the center and tropical-storm-force winds extend outward up to 320 miles (520 km). A WeatherFlow station at Jennette's Pier in Nags Head, North Carolina, recently measured a sustained wind of 44 mph (70 km/h) and a gust to 52 mph (83 km/h).

Follow updates: 

The White House budget request on May 2, 2025, calls for a 24 percent cut to NOAA's budget. The Department of Government Efficiency (DOGE) has already terminated over 800 NOAA employees, raising concerns about the frequency of essential forecasting tasks like launching weather balloons. And the NOAA science budget is hit even harder. Trump proposes a 74 percent cut to NOAA's Office of Oceanic Research.

Contact your representatives in the United States Congress, House and Senate, to express your concerns about severe budget cuts at NOAA:
Credit: National Oceanic and Atmospheric Administration (NOAA)/GOES-East/GOES-19
Release Date: Aug. 21, 2025


#NASA #NOAA #Space #Satellites #GOES #GOES19 #GOESEast #Science #Planets #Earth #Atmosphere #Meteorology #Weather #Oceans #AtlanticOcean #Bermuda #HurricaneErin #SeaTemperatures #ClimateChange #GlobalHeating #Environment #Hurricanes #HurricaneSeason #UnitedStates #Animation #STEM #Education

Wednesday, August 20, 2025

Creating Oxygen on Planet Mars for Human Life Support | NASA Space Technology

Creating Oxygen on Planet Mars for Human Life Support | NASA Space Technology

Could magnets help astronauts breathe on Mars?

Mars may be our next destination, but surviving there depends on creating oxygen in space. And in microgravity, splitting water is not as easy as it is on Earth. This is why researchers are developing a powerful new technique: magnetohydrodynamic oxygen production.

This system:

🧲 Uses strong magnets to separate gases from liquid water

 🌬️ Produces oxygen without moving parts, ideal for zero-gravity

💧 Captures hydrogen for making fuel and water

NASA 360 presents this NASA Innovative Advanced Concept (NIAC) that could provide a dependable life support system for astronauts millions of miles from home. 

Learn more: https://go.nasa.gov/3BV4CTL


Video Credit: Space Technology
Duration: 2 minutes
Release Date: Aug. 20, 2025

#NASA #Space #Astronomy #Science #Planet #Mars #OxygenProduction #Magnets #H2O #Hydrogen #Magnetohydrodynamics #MartianGravity #NAIC #Astronauts #HumanSpaceflight #SpaceTechnology #SpaceEngineering #UnitedStates #STEM #Education #HD #Video

Close-up: Distant Galaxy LEDA 803211 in Hydra | Hubble

Close-up: Distant Galaxy LEDA 803211 in Hydra | Hubble


This NASA/European Space Agency Hubble Space Telescope picture shows a tiny patch of sky in the constellation Hydra. The stars and galaxies depicted here span a mind-bending range of distances. Nearest to us in this image are stars within our own Milky Way galaxy that are marked by diffraction spikes. The bright star that sits just at the edge of the prominent bluish galaxy is only 3,230 light-years away, as measured by the European Space Agency's Gaia space observatory.

Behind this star is a galaxy named LEDA 803211. At 622 million light-years distant, this galaxy is close enough that its bright galactic nucleus is clearly visible, as are numerous star clusters scattered around its patchy disc. Many of the more distant galaxies in this frame appear star-like, with no discernible structure, but without the diffraction spikes of a star in our galaxy.

Of all the galaxies in this frame, one pair stands out in particular: a smooth golden galaxy encircled by a nearly complete ring in the upper-right corner of the image. This curious configuration is the result of gravitational lensing, where the light from a distant object is warped and magnified by the gravity of a massive foreground object, like a galaxy or a cluster of galaxies. Einstein predicted the curving of spacetime by matter in his general theory of relativity, and galaxies seemingly stretched into rings like the one in this image are called Einstein rings.

The lensed galaxy, whose image we see as the ring, lies incredibly far away from Earth: we are seeing it as it was when the Universe was just 2.5 billion years old. The galaxy acting as the gravitational lens itself is likely much closer. A nearly perfect alignment of the two galaxies is necessary to give us this rare kind of glimpse into galactic life in the early days of the Universe.

Image Description: Many mostly small, bright objects scattered over a dark background in space. In the top half on the right is an elliptical galaxy, a round light larger than the others, with a slightly warped ring of light around it. In the bottom half there is a barred spiral galaxy, big enough that we can see its bluish arms and its core in detail. Other objects include distant galaxies and nearby stars.


Credit: European Space Agency (ESA)/Hubble & NASA, D. Erb
Duration: 30 seconds
Release Date: Jan. 6, 2025


#NASA #Astronomy #Hubble #Space #Science #Galaxies #Galaxy #LEDA803211 #Hydra #Constellation #Astrophysics #GravitationalLensing #EinsteinRings #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #ESA #Europe #STEM #Education #HD #Video

Dwarf Planet Ceres: Long-Standing Energy to Fuel Habitability | NASA/JPL

Dwarf Planet Ceres: Long-Standing Energy to Fuel Habitability | NASA/JPL

Dwarf planet Ceres is shown in these enhanced-color renderings that use images from NASA’s Dawn mission. New thermal and chemicals models that rely on the mission’s data indicate Ceres may have long ago had conditions suitable for life.
This illustration depicts the interior of dwarf planet Ceres, including the transfer of water and gases from the rocky core to a reservoir of salty water. Carbon dioxide and methane are among the molecules carrying chemical energy beneath Ceres’ surface. 

The dwarf planet is cold now, but new research paints a picture of Ceres hosting a deep, long-lived energy source that may have maintained habitable conditions in the past.

New NASA research has found that Ceres may have had a lasting source of chemical energy: the right types of molecules needed to fuel microbial metabolisms. Although there is no evidence that microorganisms ever existed on Ceres, the finding supports theories that this intriguing dwarf planet, the largest body in the main asteroid belt between Mars and Jupiter, may have once had conditions suitable to support single-celled lifeforms.

Science data from NASA’s Dawn mission that ended in 2018, previously showed that the bright, reflective regions on Ceres’ surface are mostly made of salts left over from liquid that percolated up from underground. Later analysis in 2020 found that the source of this liquid was an enormous reservoir of brine, or salty water, below the surface. In other research, the Dawn mission also revealed evidence that Ceres has organic material in the form of carbon molecules—essential, though not sufficient on its own, to support microbial cells.

The presence of water and carbon molecules are two critical pieces of the habitability puzzle on Ceres. The new findings offer the third: a long-lasting source of chemical energy in Ceres’ ancient past that could have made it possible for microorganisms to survive. This result does not mean that Ceres had life, but rather, that there likely was “food” available should life have ever arisen on Ceres.

In the study, published in Science Advances on Aug. 20, 2025, the authors built thermal and chemical models mimicking the temperature and composition of Ceres’ interior over time. They found that 2.5 billion years or so ago, Ceres’ subsurface ocean may have had a steady supply of hot water containing dissolved gases traveling up from metamorphosed rocks in the rocky core. The heat came from the decay of radioactive elements within the dwarf planet’s rocky interior that occurred when Ceres was young—an internal process thought to be common in our solar system.

“On Earth, when hot water from deep underground mixes with the ocean, the result is often a buffet for microbes—a feast of chemical energy. So it could have big implications if we could determine whether Ceres’ ocean had an influx of hydrothermal fluid in the past,” said Sam Courville, lead author of the study. Now based at Arizona State University in Tempe, he led the research while working as an intern at NASA’s Jet Propulsion Laboratory in Southern California that managed the Dawn mission.

Catching Chill
The Ceres we know today is unlikely to be habitable. It is cooler with more ice and less water than in the past. There is currently insufficient heat from radioactive decay within Ceres to keep the water from freezing, and what liquid remains has become a concentrated brine.

The period when Ceres would most likely have been habitable was between a half-billion and 2 billion years after it formed (or about 2.5 billion to 4 billion years ago), when its rocky core reached its peak temperature. This was when warm fluids would have been introduced into Ceres’ underground water.

The dwarf planet also does not have the benefit of present-day internal heating generated by the push and pull of orbiting a large planet, like Saturn’s moon Enceladus and Jupiter’s moon Europa do. So Ceres’ greatest potential for habitability-fueling energy was in the past.

This result has implications for water-rich objects throughout the outer solar system, too. Many of the other icy moons and dwarf planets that are of similar size to Ceres (about 585 miles, or 940 kilometers, in diameter) and do not have significant internal heating from the gravitational pull of planets could have also had a period of habitability in their past.

More About Dawn
A division of Caltech in Pasadena, JPL managed Dawn’s mission for NASA’s Science Mission Directorate in Washington. Dawn was a project of the directorate’s Discovery Program, managed by NASA’s Marshall Space Flight Center in Huntsville, Alabama. JPL was responsible for overall Dawn mission science. Northrop Grumman in Dulles, Virginia, designed and built the spacecraft. The German Aerospace Center, Max Planck Institute for Solar System Research, Italian Space Agency and Italian National Astrophysical Institute were international partners on the mission team.

Learn more about NASA's Dawn Mission, visit:


Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
Release Date: Aug. 20, 2025

#NASA #Astronomy #Space #Science #SolarSystem #DwarfPlanets #Ceres #DawnMission #AsteroidBelt #Mars #Jupiter #Astrobiology #JPL #Caltech #Illustrations #Infographics #STEM #Education

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