Friday, August 22, 2025

Dramatic Lighting for Crew-10 Departure | International Space Station

Dramatic Lighting for Crew-10 Departure | International Space Station

Expedition 73 flight engineer and NASA astronaut Jonny Kim: "Crew-10 undocked earlier this month as the sun was just rising over the horizon. I did my best to capture this dynamic light range with marginal success. We’ll have another opportunity when the SpX-33 Cargo Dragon arrives later this month."

At 6:15 p.m. EDT on Friday, August 8, 2025, NASA astronauts Anne McClain and Nichole Ayers, along with Japan Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi and Roscosmos cosmonaut Kirill Peskov of Russia undocked from the forward-facing port of International Space Station’s Harmony module aboard the SpaceX Dragon spacecraft.

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: NASA's Johnson Space Center/J. Kim
Duration: 46 seconds
Release Date: Aug. 21, 2025


#NASA #Space #ISS #Science #Sun #Planets #Earth #SpaceX #CrewDragonSpacecraft #Crew10 #Astronauts #JonnyKim #AstronautPhotography #Japan #JAXA #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #UnitedStates #STEM #Education #HD #Video

Sprites Detected | International Space Station

Sprites Detected | International Space Station



Expedition 73 flight engineer and Japan Aerospace Exploration Agency (JAXA) astronaut Kimiya Yui: "I was able to capture footage of a sprite phenomenon, so I’d like to share it with you . . . It was purely by chance that I managed to capture it amidst a lot of lightning, so it was just a matter of luck. While lightning is terrifying from the ground, it looks beautiful when seen from space, which is a bit unsettling. Please take extra care during the lightning season, everyone! This post is wishing everyone good fortune as well! "
—Kimiya Yui 油井 亀美也

Red Sprites: These mysterious bursts of light in the upper atmosphere momentarily resemble gigantic jellyfish. One unusual feature of sprites is that they are relatively cold. They operate more like long fluorescent light tubes than hot compact light bulbs. In general, red sprites take only a fraction of a second to occur and are best seen when powerful thunderstorms are visible from the side.

Learn more here: https://uhu.epss.hu/en/tle-phenomena/

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.

Learn more about the important research being operated on Station:
https://www.nasa.gov/iss-science

For more information about STEM on Station:
https://www.nasa.gov/stemonstation
Science, Technology, Engineering, Math (STEM)

Image Credit: Kimiya Yui/JAXA
Release Dates: Aug. 19-20, 2025


#NASA #Space #ISS #Science #Planet #Earth #Atmosphere #Thunderstorms #Sprites #TLE #Sprite #Astronauts #KimiyaYui #AstronautPhotography #Japan #日本 #JAXA #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #UnitedStates  #STEM #Education

A Tale of Two 'Nebulae' in Lyra (AI Narration)

A Tale of Two 'Nebulae' in Lyra (AI Narration)

This colorful telescopic view towards the musical northern constellation Lyra reveals the faint outer halos and brighter central ring-shaped region of M57, popularly known as the Ring Nebula. To modern astronomers M57 is a well-known planetary nebula. With a central ring about one light-year across, M57 is definitely not a planet though, but the gaseous shroud of one of the Milky Way's dying sun-like stars. Roughly the same apparent size as M57, the fainter and more often overlooked barred spiral galaxy at the left is IC 1296. In fact, over 100 years ago IC 1296 would have been known as a spiral nebula. 

By chance the pair are in the same field of view, and while they appear to have similar sizes they are actually very far apart. At a distance of a mere 2,000 light-years M57 is well within our own Milky Way galaxy. Extragalactic IC 1296 (aka PGC62532) is more like 200,000,000 light-years distant. This is about 100,000 times farther away than M57 but since they appear roughly similar in size, former spiral nebula IC 1296 must also be about 100,000 times larger than planetary nebula M57. Look closely at the sharp 21st century astroimage to spot even more distant background galaxies scattered through the frame.


Image Credit & Copyright: Kent Biggs
Kent's website: 
Duration: 2 minutes, 30 seconds
Release Date: Aug. 22, 2025


#NASA #Space #Astronomy #Science #Nebulae #PlanetaryNebula #M57 #RingNebula #IC1296 #Lyra #Constellations #Cosmos #Universe #GSFC #UnitedStates #STEM #Education #HD #Video #APoD 

A Tale of Two 'Nebulae' in Lyra

A Tale of Two 'Nebulae' in Lyra

This colorful telescopic view towards the musical northern constellation Lyra reveals the faint outer halos and brighter central ring-shaped region of M57, popularly known as the Ring Nebula. To modern astronomers M57 is a well-known planetary nebula. With a central ring about one light-year across, M57 is definitely not a planet though, but the gaseous shroud of one of the Milky Way's dying sun-like stars. Roughly the same apparent size as M57, the fainter and more often overlooked barred spiral galaxy at the left is IC 1296. In fact, over 100 years ago IC 1296 would have been known as a spiral nebula. 

By chance the pair are in the same field of view, and while they appear to have similar sizes they are actually very far apart. At a distance of a mere 2,000 light-years M57 is well within our own Milky Way galaxy. Extragalactic IC 1296 (aka PGC62532) is more like 200,000,000 light-years distant. This is about 100,000 times farther away than M57 but since they appear roughly similar in size, former spiral nebula IC 1296 must also be about 100,000 times larger than planetary nebula M57. Look closely at the sharp 21st century astroimage to spot even more distant background galaxies scattered through the frame.


Image Credit & Copyright: Kent Biggs
Kent's website: https://www.kentbiggs.com/index.htm
Release Date: Aug. 22, 2025


#NASA #Space #Astronomy #Science #Nebulae #PlanetaryNebula #M57 #RingNebula #IC1296 #Lyra #Constellations #Cosmos #Universe #GSFC #UnitedStates #STEM #Education #APoD 

Category 5 Erin is the First Atlantic Hurricane of 2025 | NOAA [Budget Cut Alert]

Category 5 Erin is the First Atlantic Hurricane of 2025 | NOAA [Budget Cut Alert]

After a relatively quiet start to the Atlantic hurricane season, Erin became the first hurricane of the year in the Atlantic basin on Aug.15 and rapidly intensified into a major Category 5 storm the following day. This intensification is one of the fastest on record.

Learn how NOAA satellites monitored the storm: https://www.nesdis.noaa.gov/news/category-5-erin-the-first-atlantic-hurricane-of-2025

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:
Credits: NOAA, NASA, The Cooperative Institute for Research in the Atmosphere (CIRA)
Duration: 2 minutes, 13 seconds 
Release Date: Aug. 22, 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 #STEM #Education #HD #Video

Artemis Science: Exploring the Moon’s South Pole | NASA Goddard

Artemis Science: Exploring the Moon’s South Pole | NASA Goddard

The Moon is our nearest celestial neighbor, orbiting Earth at less than a quarter of a million miles on average. Now, for the first time since 1972, NASA is preparing to send astronauts to the Moon with the Artemis missions. Artemis III will target landing sites near the lunar South Pole. There, ancient rocks, minerals, and trapped water ice will not only provide resources for human explorers, they may also contain clues to the formation and evolution of our planet and the solar system.

Artemis campaign: 
https://www.nasa.gov/humans-in-space/artemis/

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

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


Credit: NASA’s Goddard Space Flight Center
Dan Gallagher: Producer/Editor
Kelsey Young: Scientist
Ernie Wright: Visualizer
Rob Andreoli: Videographer
John D. Philyaw: Videographer
Chris Smith: Animator
Brian Monroe: Animator
Derrol Nail: Launch Commentator
Lonnie Shekhtman: Public Affairs
Molly Wasser: Public Affairs
Caela Barry: Support
Aaron E. Lepsch: Technical Support
Duration: 2 minutes, 22 seconds
Release Date: Aug. 22, 2025

#NASA #Space #Astronomy #Science #Earth #Moon #LunarSouthPole #Geology #ArtemisProgram #ArtemisIII #SLSRocket #OrionSpacecraft #CrewedMissions #DeepSpace #MoonToMars #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NASAGoddard #GSFC #UnitedStates #STEM #Education #HD #Video

A Pair of Merging Galaxies: IC 1623 | Webb & Chandra Space Telescopes

A Pair of Merging Galaxies: IC 1623 | 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 1623 is a system where two galaxies are in the process of merging. As the galaxies collide, they trigger new bursts of star formation that glow dramatically in certain kinds of light. The merging galaxies may also be in the process of forming a supermassive black hole.

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:

X-rays from Chandra (magenta) with Webb infrared data (red, gold and gray)

Image Description: Backed by hot pink tendrils, swirls of speckled orange, and gauzy steel blue ribbons, two white clusters meet, gleaming with golden shafts of light.


Credit: X-ray: NASA/CXC/SAO; IR: NASA/ESA/CSA/STScI; Image Processing: NASA/CXC/SAO/L. Frattare and J. Major
Release Date: Aug. 22, 2025


#NASA #Astronomy #Space #Science #Galaxies #IC1623 #Cetus #Constellation #JamesWebb #JWST #UnfoldTheUniverse #NASAChandra #CXC #SpaceTelescopes #Cosmos #Universe #ESA #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education

Thursday, August 21, 2025

NASA Psyche Spacecraft View of Earth & Moon: Distance 180 Million Miles

NASA Psyche Spacecraft View of Earth & Moon: Distance 180 Million Miles

This is a black and white photograph of deep space where Earth appears as a bright point of light among other labeled stars. An inset in the corner shows a magnified view of the bright Earth with the much smaller Moon as a dot beside it.
An infographic of the Psyche mission's trajectory, showing its spiral path from a 2023 Earth launch. The spacecraft is depicted using a Mars gravity assist in 2026 to reach and orbit the asteroid Psyche in 2029.

Headed for a metal-rich asteroid of the same name, NASA's Psyche spacecraft successfully calibrated its cameras by looking homeward. On schedule for its 2029 arrival at the asteroid Psyche, NASA’s Psyche spacecraft recently looked back toward home and captured images of Earth and our Moon from about 180 million miles (290 million kilometers) away. For comparison, the average distance between Earth and Mars is approximately 140 million miles (225 million km).

The images were obtained during one of the mission team’s periodic checkouts of the spacecraft’s science instruments. When choosing targets for the imager testing, scientists look for bodies that shine with reflected sunlight, just as the asteroid Psyche does. 

On July 20 and July 23, the spacecraft’s twin cameras captured multiple long-exposure (up to 10-second) pictures of the two bodies. They appear as dots sparkling with reflected sunlight amid a starfield in the constellation Aries.

The Psyche multispectral imager instrument comprises a pair of identical cameras equipped with filters and telescopic lenses to photograph the asteroid Psyche’s surface in multiple wavelengths of light. The color and shape of a planetary body’s spectrum can reveal details about what it is made of. The Moon and the giant asteroid Vesta, for example, have similar kinds of “bumps and wiggles” in their spectra that scientists could potentially also detect at Psyche. Members of the mission’s science team are interested in Psyche because it will help them better understand the formation of rocky planets with metallic cores, including Earth.

When choosing targets for the imager testing and calibration, scientists look for bodies that shine with reflected sunlight, just as the asteroid Psyche does. They also look at objects that have a spectrum they are familiar with, so they can compare previous telescopic or spacecraft data from those objects with what Psyche’s instruments observe. Earlier this year, Psyche turned its lenses toward Jupiter and Mars for calibration—each has a spectrum more reddish than the bluer tones of Earth. That checkout also proved a success.

To determine whether the imager’s performance is changing, scientists also compare data from tests. Thus, when the spacecraft slips into orbit around Psyche, scientists can be sure that the instrument behaves as expected.

“After this, we may look at Saturn or Vesta to help us continue to test the imagers,” said Jim Bell, the Psyche imager instrument lead at Arizona State University in Tempe. “We’re sort of collecting solar system ‘trading cards’ from these different bodies and running them through our calibration pipeline to make sure we’re getting the right answers.”

Strong and Sturdy
The imager was not the only instrument that got a successful checkout in late July: The mission team also put the spacecraft’s magnetometer and the gamma-ray and neutron spectrometer through a gamut of tests—something they do every six months.

“We are up and running, and everything is working well,” said Bob Mase, the mission’s project manager at NASA’s Jet Propulsion Laboratory in Southern California. “We’re on target to fly by Mars in May 2026, and we are accomplishing all of our planned activities for cruise.”

This flyby is the spacecraft’s next major milestone, when it will use the Red Planet’s gravity as a slingshot to help the spacecraft get to the asteroid Psyche. It will mark Psyche’s first of two planned loops around the solar system and 1 billion miles (1.6 billion kilometers) since launching from NASA’s Kennedy Space Center in October 2023.

The Psyche mission is led by Arizona State University (ASU). Lindy Elkins-Tanton of the University of California, Berkeley is the principal investigator. A division of Caltech in Pasadena, JPL is responsible for the mission’s overall management, system engineering, integration and test, and mission operations. Maxar Technologies in Palo Alto, California, provided the high-power solar electric propulsion spacecraft chassis. ASU leads the operations of the imager instrument, working in collaboration with Malin Space Science Systems in San Diego on the design, fabrication, and testing of the cameras.

Psyche is the 14th mission selected as part of NASA’s Discovery Program, managed by the agency’s Marshall Space Flight Center in Huntsville, Alabama. NASA’s Launch Services Program, based at Kennedy, managed the launch service.

For more information about NASA’s Psyche mission visit:


Image Credit: NASA/JPL-Caltech/ASU
Release Date: Aug. 19, 2025

#NASA #Space #Astronomy #Planets #Earth #Moon #PsycheAsteroid #16Psyche #Asteroids #Science #PsycheMission #PsycheSpacecraft #Mars #Jupiter #AsteroidBelt #SolarSystem #SpaceExploration #JPL #Caltech #ASU #UnitedStates #Infographics #STEM #Education 

'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