Wednesday, February 25, 2026

A "Planetary Parade" of Sonifications | NASA's Chandra X-ray Observatory

A "Planetary Parade" of Sonifications | NASA's Chandra X-ray Observatory

In late February 2026, people in the northern hemisphere can look up for a special sight—six planets will all be visible from clear and dark night skies. Since the planets in our Solar System travel around the Sun in same plane, known as the ecliptic, they will sometimes appear bunched together on the sky if their orbits find them on the same side of the Sun at the same time. When this happens, it looks like the planets have roughly formed a line from our vantage point on Earth.

New sonifications from NASA’s Chandra X-ray Observatory help commemorate this latest so-called planetary parade. In the latest sonifications, three of the planets that will be on display—Jupiter, Saturn, and Uranus—can be seen and heard in ways that they cannot from the ground on Earth.

While Chandra is best known for its X-ray insight into black holes and other extreme objects, the telescope has also played an important role in the exploration of our Solar System. The Sun gives off X-rays that travel out into the Solar System and can be reflected by planets, moons, and other bodies. This gives astronomers a unique window into certain physics that cannot be discovered through other kinds of telescopes.

The sonification of Jupiter combines X-ray data from Chandra with an infrared image from NASA’s Hubble Space Telescope. Woodwind sounds reveal Chandra’s X-ray data including emission from the planet’s auroras. More instruments join in to represent the planet’s complex cloud layers. Next, by combining an optical image from NASA’s Cassini mission with X-rays from Chandra, we can experience Saturn like never before. A siren-like sound follows the arc of the rings and tones of synthesizers play as the scan passes the planet itself. Finally, we can hear the ice giant of Uranus through the data collected by Chandra and the W.M. Keck Observatory. The data in this sonification reflect the amount of the different light detected from the planet and the orientation of its ring.

Sonifications are translations of astronomical data into sounds. This process of translation preserves the integrity of the data that arrives on Earth as a series of ones and zeroes (binary code), and shifts it into a form that our brains can process through hearing. Sonifications expand options for people to explore what telescopes discover in space, an example of NASA’s ongoing commitment to share its data as widely as possible.


Video Credit: NASA's Chandra X-ray Observatory
Duration: 3 minutes, 18 seconds
Release Date: Feb. 25, 2026

#NASA #ESA #Astronomy #Space #Science #SolarSystem #Planets #Jupiter #Saturn #Uranus  #Cosmos #Universe #NASAChandra #Xray #SpaceTelescopes #HST #Hubble #JWST #NASAWebb #CSA #JPL #GSFC #STScI #UnitedStates #Canada #Europe #STEM #Education #Sonifications #Audio #HD #Video

PMR 1: The Exposed Cranium Nebula in Vela (MIRI image) | Webb Telescope

PMR 1: The Exposed Cranium Nebula in Vela (MIRI image) | Webb Telescope

Exposed Cranium Nebula (MIRI image)
The differences in what Webb’s infrared instruments reveal and conceal within the PMR 1 “Exposed Cranium” nebula is apparent in this side-by-side view. More stars and background galaxies shine through the view of Webb’s Near-Infrared Camera (
NIRCam), while cosmic dust glows more prominently in the light captured by the Mid-Infrared Instrument (MIRI).

In this image captured by the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope’s Mid-Infrared Instrument (MIRI), more of the dusty material in the nebula PMR located in the Vela constellation shows up. Fewer stars and background galaxies appear in this image than in the near-infrared light captured by Webb’s  Near-Infrared Camera NIRCam instrument. Seeing the nebula in distinct wavelengths of infrared light gives astronomers a better idea of how much material the dying star at the heart of the nebula is shedding, and what phase of its decline Webb has captured.

Distance from Earth: ~5,000 light years

Like NIRCam, MIRI also shows two distinct phases of the nebula’s formation—an outer shell primarily of hydrogen that was blown off first, then a more complex and structured mix of material closer to the centre of the nebula. Together, these give the nebula the unusual appearance of a brain inside a semi-transparent skull.

The MIRI instrument shows the ejection of material at the top of the nebula more prominently than NIRCam, interrupting the overall oval, brain-like shape. Less prominent is a potential twin ejection on the opposite, bottom side, hinting at a potential bipolar outflow that, with further analysis, can shed light on the dynamics at play inside this “exposed cranium.”

Image Description: A nebula appears like a transparent bubble with a blue edge, inside which are two hemispheres of off-white material being blown out from the center, interspersed vertically by a dark lane that gives the overall appearance of a brain seen from above. At the top of the nebula the dark lane ends in an oval with the inner off-white material arcing overtop, giving the impression of an eruption. The bottom of the nebula mirrors this effect, but less dramatically. A few scattered background galaxies can be seen around the outer bubble.


Credit: NASA, ESA, CSA, STScI, 
Image Processing: Joseph DePasquale (STScI) 
Release Date: Feb. 25, 2026

#NASA #Astronomy #Space #Science #Nebulae #PlanetaryNebulae #PMR1 #ExposedCraniumNebula #VelaConstellation #Cosmos #Universe #JWST #NIRCam #InfraredAstronomy #SpaceTelescopes #GSFC #STScI #UnitedStates #ESA #Europe #CSA #Canada #STEM #Education

PMR 1—The Exposed Cranium Nebula: MIRI & NIRCam images | Webb Telescope

PMR 1—The Exposed Cranium Nebula: MIRI & NIRCam images | Webb Telescope


Nebula PMR 1 is a cloud of gas and dust located in the Vela constellation that bears an uncanny resemblance to a brain in a transparent skull, inspiring its nickname, the “Exposed Cranium” nebula. The NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope Webb captured its unusual features in both near- and mid-infrared light using two instruments that reveal enhancing details of the nebula’s brain-like appearance.
Distance from Earth: ~5,000 light years

The first image shown that reveals the light captured by Mid-Infrared Instrument (MIRI), while stars and background galaxies shine through in the second image from Webb’s Near-Infrared Camera (NIRCam).

The dark center lane that contributes to this nebula’s distinctive brain-like appearance is more noticeable in NIRCam, but its apparent role in the ejection of material at the top and bottom of the nebula is seen more clearly in MIRI’s view. Observing the cosmos in multiple wavelengths of light provides a more complete picture of how the universe works.


Credit: NASA, ESA, CSA, STScI, N. Bartmann (ESA/Webb)
Image Processing: Joseph DePasquale (STScI)
Duration: 30 seconds
Release Date: Feb. 25, 2026

#NASA #Astronomy #Space #Science #Nebulae #PlanetaryNebulae #PMR1 #ExposedCraniumNebula #VelaConstellation #Cosmos #Universe #JWST #NIRCam #MIRI #InfraredAstronomy #SpaceTelescopes #GSFC #STScI #UnitedStates #ESA #Europe #CSA #Canada #STEM #Education #HD #Video

Close-up: PMR 1—The Exposed Cranium Nebula in Vela | Webb Telescope

Close-up: PMR 1The Exposed Cranium Nebula in Vela | Webb Telescope

A distinct dark lane between two cosmic clouds adds to the brainy appearance of the planetary nebula PMR 1 located in the Vela constellation. The Near-Infrared Camera (NIRCam) instrument on the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope shows multiple phases of a dying star’s outbursts in one image—the skull-like, whitish outer bubble is from an initial ejection, mostly of hydrogen, followed by other heavier material, shown in orange in the nebula’s interior. As with many NIRCam images, many stars and even distant galaxies can be seen behind the nebula.

Distance from Earth: ~5,000 light years

Beyond its unusual appearance there is still much to be uncovered about PMR 1. It is unclear if the star creating the nebula is massive enough to undergo a supernova, or if it will evolve into a dense white dwarf once it has shed all its outer layers.

Image Description: A nebula appears like a transparent bubble with a white edge. Inside are two hemispheres of orange clouds being blown out from the center, split by a dark lane, giving the overall appearance of a see-through skull with a brain inside, as seen from above. A few stars appear with six points, and small background galaxies can be seen around and through the outer bubble.


Credit: NASA, ESA, CSA, STScI, N. Bartmann (ESA/Webb)
Image Processing: Joseph DePasquale (STScI)
Duration: 30 seconds
Release Date: Feb. 25, 2026

#NASA #Astronomy #Space #Science #Nebulae #PlanetaryNebulae #PMR1 #ExposedCraniumNebula #VelaConstellation #Cosmos #Universe #JWST #NIRCam #InfraredAstronomy #SpaceTelescopes #GSFC #STScI #UnitedStates #ESA #Europe #CSA #Canada #STEM #Education #HD #Video

PMR 1: The Exposed Cranium Nebula in Vela (NIRCam image) | Webb Telescope

PMR 1: The Exposed Cranium Nebula in Vela (NIRCam image) | Webb Telescope

A distinct dark lane between two cosmic clouds adds to the brainy appearance of the planetary nebula PMR 1 located in the Vela constellation. The Near-Infrared Camera (NIRCam) instrument on the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope shows multiple phases of a dying star’s outbursts in one image—the skull-like, whitish outer bubble is from an initial ejection, mostly of hydrogen, followed by other heavier material, shown in orange in the nebula’s interior. As with many NIRCam images, many stars and even distant galaxies can be seen behind the nebula.

Distance from Earth: ~5,000 light years

Beyond its unusual appearance there is still much to be uncovered about PMR 1. It is unclear if the star creating the nebula is massive enough to undergo a supernova, or if it will evolve into a dense white dwarf once it has shed all its outer layers.

Image Description: A nebula appears like a transparent bubble with a white edge. Inside are two hemispheres of orange clouds being blown out from the center, split by a dark lane, giving the overall appearance of a see-through skull with a brain inside, as seen from above. A few stars appear with six points, and small background galaxies can be seen around and through the outer bubble.


Credit: NASA, ESA, CSA, STScI, 
Image Processing: Joseph DePasquale (STScI) 
Release Date: Feb. 25, 2026

#NASA #Astronomy #Space #Science #Nebulae #PlanetaryNebulae #PMR1 #ExposedCraniumNebula #VelaConstellation #Cosmos #Universe #JWST #NIRCam #InfraredAstronomy #SpaceTelescopes #GSFC #STScI #UnitedStates #ESA #Europe #CSA #Canada #STEM #Education

Saturn Quadruple Moon Transit | Hubble Space Telescope

Saturn Quadruple Moon Transit | Hubble Space Telescope

This Hubble video shows four of Saturn's moons moving across the face of their parent planet on February 24, 2009. Icy moons Enceladus and Dione are on the far left, while the large orange moon Titan and icy Mimas are on the right. The closer the moon is to Saturn, the faster it orbits, according to the laws of gravity.

In astronomy, a transit (or astronomical transit) is the passage of a celestial body directly between a larger body and the observer. As viewed from a particular vantage point, the transiting body appears to move across the face of the larger body, covering a small portion of it.


Credit: NASA, ESA, and G. Bacon (STScI)
Duration: 33 seconds
Release Date: Feb. 24, 2026


#NASA #Hubble #Astronomy #Space #Science #Planets #Saturn #Moons #Titan #Enceladus #Dione #Mimas #SolarSystem #HubbleSpaceTelescope #HST #ESA #GSFC #STScI #STEM #Education #Timelapse #HD #Video

Open Star Cluster NGC 2477 in Puppis | European Southern Observatory

Open Star Cluster NGC 2477 in Puppis | European Southern Observatory


NGC 2477 (also known as Caldwell 71) is an open star cluster in the constellation Puppis. It contains about 300 stars, and was discovered by Abbe Lacaille in 1751. The cluster's age has been estimated at about 700 million years.
Distance from Earth: ~3600 light years

NGC 2477 is a stunning cluster, almost as extensive in the sky as the full moon. It has been called "one of the top open clusters in the sky", like a highly-resolved globular cluster without the dense center characteristic of globular clusters.


Credit: ESO/J.Pérez
Release Date: April 16, 2013


#NASA #ESO #Astronomy #Space #Science #Stars #StarClusters #NGC2477 #Caldwell71 #PuppisConstellation #Cosmos #Universe #Chile #Europe #STEM #Education

Tuesday, February 24, 2026

March 3, 2026 Total Lunar Eclipse over The Americas: Shadow Preview

March 3, 2026 Total Lunar Eclipse over The Americas: Shadow Preview

Map showing where the March 3, 2026 lunar eclipse is visible. Contours mark the edge of the visibility region at eclipse contact times, labeled in UTC.
Alignment of the Moon, Earth, and Sun during a lunar eclipse (not to scale).

On March 3, 2025, the Moon enters the Earth's shadow, creating a total lunar eclipse, the first visible in the Americas since March 2025. This animation shows the changing appearance of the Moon as it travels into and out of the Earth's shadow, along with times at various stages. Celestial north is up in this imagery, corresponding to the view from mid-northern latitudes. Rotating the images by 180 degrees would create the south-up view for southern hemisphere observers.

The penumbra is the part of the Earth’s shadow where the Sun is only partially covered by the Earth. The umbra is where the Sun is completely hidden. The Moon's appearance is not affected much by the penumbra. The real action begins when the Moon starts to disappear as it enters the umbra at about 1:50 a.m. Pacific Sstandard Time. An hour and a half later, entirely within the umbra, the Moon is a ghostly copper color. The totally eclipsed Moon is 10 or more f-stops dimmer than a normal full Moon. This is captured in the animation by simulating an abrupt change of exposure near the start and end of totality. Totality lasts for about an hour before the Moon begins to emerge from the central shadow. During the eclipse, the Moon is moving through the constellation Leo.


Credit: NASA's Goddard Space Flight Center/Scientific Visualization Studio
Ernie Wright (USRA): Lead Visualizer
Release Date: Jan. 28, 2026

#NASA #Space #Astronomy #Science #Sun #SolarSystem #Moon #Earth #LunarEclipse #Umbra #Penumbra #NASAGoddard #GSFC #UnitedStates #Infographics #STEM #Education

March 3, 2026 Total Lunar Eclipse over The Americas: Shadow Preview

March 3, 2026 Total Lunar Eclipse over The Americas: Shadow Preview

On March 3, 2025, the Moon enters the Earth's shadow, creating a total lunar eclipse, the first visible in the Americas since March 2025. This animation shows the changing appearance of the Moon as it travels into and out of the Earth's shadow, along with times at various stages. Celestial north is up in this imagery, corresponding to the view from mid-northern latitudes. Rotating the images by 180 degrees would create the south-up view for southern hemisphere observers.

The penumbra is the part of the Earth’s shadow where the Sun is only partially covered by the Earth. The umbra is where the Sun is completely hidden. The Moon's appearance is not affected much by the penumbra. The real action begins when the Moon starts to disappear as it enters the umbra at about 1:50 a.m. Pacific Sstandard Time. An hour and a half later, entirely within the umbra, the Moon is a ghostly copper color. The totally eclipsed Moon is 10 or more f-stops dimmer than a normal full Moon. This is captured in the animation by simulating an abrupt change of exposure near the start and end of totality. Totality lasts for about an hour before the Moon begins to emerge from the central shadow. During the eclipse, the Moon is moving through the constellation Leo.


Credit: NASA's Goddard Space Flight Center/Scientific Visualization Studio
Ernie Wright (USRA): Lead Visualizer
Duration: 1 minute, 30 seconds
Release Date: Jan. 28, 2026

#NASA #Space #Astronomy #Science #Sun #SolarSystem #Moon #Earth #LunarEclipse #Umbra #Penumbra #NASAGoddard #GSFC #UnitedStates #STEM #Education #Animation #HD #Video

NASA Career Spotlight: Aerospace Welder

NASA Career Spotlight: Aerospace Welder

When you think of NASA, you might picture astronauts floating in space or scientists in control rooms. However, behind every rocket launch, orbiting satellite, and space station mission, there are welders making it possible. 

Learn more about the important role welders play at NASA: 
https://www.nasa.gov/learning-resources/career-spotlight-welder-ages-14-18/

We are inviting students to participate in NASA’s exciting missions, broad range of careers, and unique opportunities. Join us and our contractors as we apply science, technology, engineering, and mathematics to explore space, improve aeronautics, examine Earth, and strive to land the next humans on the Moon with the Artemis program.


Video Credit: National Aeronautics and Space Administration (NASA)
Duration: 3 minutes
Release Date: Feb. 17, 2026

#NASA #Space #Science #Astronomy #Engineering #Earth #Moon #SpaceExploration #Spaceflight #SolarSystem #ArtemisProgram #HumanSpaceflight #Aerospace #Welders #AerospaceWelders #Spacecraft #Satellites #Careers #JobOpportunities #CareerOpportunities #JobTraining #Students #HighSchool #College #STEM #Education #HD #Video

Bright Supernova in Nearby Galaxy NGC 2403 | Hubble Space Telescope

Bright Supernova in Nearby Galaxy NGC 2403 | Hubble Space Telescope



This detailed view of spiral galaxy NGC 2403 shows the location of Supernova 2004dj, numerous star clusters, and several other stars that exploded in previous years. The region was observed with the Hubble Space Telescope's Advanced Camera for Surveys on Aug. 17, 2004
The image at left represents a small region of NGC 2403, a galaxy located 11 million light-years from Earth. The photo was taken two months before a massive star exploded. The image pinpoints the location of the stellar blast, known as supernova 2004dj, within a cluster of massive, generally blue (but some red) stars called Sandage 96. The cluster's total mass is estimated at about 24,000 times the mass of the Sun. The stars in this cluster are so far away that their light blends together, appearing as the light of a single star. The yellow object below and to the left of the cluster is a foreground star in our Milky Way Galaxy. The pink blob at bottom, center is a star-birth region. This image was taken May 8, 2004, with the WIYN 0.9-meter mosaic camera at Kitt Peak National Observatory in Arizona.

The image at right pinpoints the supernova blast. The photo was taken on Aug. 17, 2004, with the Hubble Space Telescope's Advanced Camera for Surveys. The light from this outburst outshines every star in the massive cluster. Similar blue clusters of stars can be seen throughout the image. The bluish-pink blob towards the bottom of the image is a large star-birth region.

The explosion of a massive star blazes with the light of 200 million Suns in this NASA/European Space Agency Hubble Space Telescope image. The arrow at top right in the second image points to the stellar blast, called a supernova. The supernova is so bright in this image that it easily could be mistaken for a foreground star in our Milky Way Galaxy. And yet, this supernova, called SN 2004dj, resides far beyond our galaxy. Its home is in the outskirts of NGC 2403, a galaxy located 11 million light-years from Earth.

A supernova is the biggest explosion that humans have ever seen. Each blast is the extremely bright, super-powerful explosion of a star.


Credit: NASA, ESA, A.V. Filippenko (University of California, Berkeley), P. Challis (Harvard-Smithsonian Center for Astrophysics), et al.
Release Date: Sept. 2, 2004


#NASA #ESA #Astronomy #Space #Science #Galaxies #NGC2403 #Caldwell7 #Supernovae #SN2004dj #StellarLifecycles #CamelopardalisConstellation #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education

A Galaxy of "Birth and Death": NGC 2403 in Camelopardalis | Mayall Telescope

A Galaxy of "Birth and Death": NGC 2403 in Camelopardalis | Mayall Telescope

Captured by the Mosaic camera on the Nicholas U. Mayall 4-meter Telescope at the Kitt Peak National Observatory (KPNO), a Program of the United States National Science Foundation (NSF) NOIRLab, the spiral galaxy NGC 2403, also known as Caldwell 7, highlights the dynamic birth and death of stars. The glowing red spots dotting the galaxy are clouds of ionized hydrogen gas known as HII regions. These areas indicate the birth of young, hot stars that often ionize nearby hydrogen gas during their dynamic formation. Conversely, NGC 2403 has also been the home of the supernova SN 2004dj. The region in NGC 2403 containing the star that became a supernova in 2004 had been observed before, during, and after the explosion, providing a fascinating timeline of the impact of the event. 

Since star formation occurs on a timescale much longer than a human lifetime, the process has to be pieced together like a puzzle through observations of stars at distinct stages of the stellar life cycle. It is very satisfying for astronomers to be able to observe supernovae that occur incredibly quickly even by human standards, to confirm and develop theories of the life cycle of stars.

Learn more about the Mayall Telescope: 
https://noirlab.edu/science/programs/kpno/telescopes/nicholas-mayall-4m-telescope


Credit: KPNO/NOIRLab/NSF/AURA/M. T. Patterson (New Mexico State University)
Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani & D. de Martin (NSF NOIRLab)
Release Date: May 25, 2022


#NASA #Astronomy #Space #Science #Galaxies #NGC2403 #Caldwell7 #Supernovae #SN2004dj #StarBirth #StellarNurseries #StellarLifecycles #CamelopardalisConstellation #Cosmos #Universe #MayallTelescope #KPNO #Arizona #NSF #AURA #UnitedStates #STEM #Education

Aurora Borealis with Moonlight: View from Norway | Earth Science

Aurora Borealis with Moonlight: View from Norway | Earth Science



Photographer Eva Kristiansen: "A beautiful evening drifting into night, bathed in moonlight and crowned by glorious Northern Lights pure magic, simply breathtaking."

Also known as the southern lights (aurora australis) or northern lights (aurora borealis), auroras are colorful, dynamic, and often visually delicate displays of an intricate dance of particles and magnetism between the Sun and Earth called space weather. When energetic particles from space collide with atoms and molecules in the atmosphere, they can cause the colorful glow that we call auroras.

Learn more about auroras: 
https://science.nasa.gov/sun/auroras/

Norway, officially the Kingdom of Norway, is a Nordic country located on the Scandinavian Peninsula in Northern Europe. The country shares a long eastern border with Sweden, and is bordered by Finland and Russia to the northeast.

Image Credit: Eva Kristiansen
Image Details: Nikon D850
Location: Tromsø, Norway
Eva's website: https://www.instagram.com/xevitak/
Date: Feb. 23, 2026

#NASA #Space #Astronomy #Science #Planets #Earth #Moon #Moonlight #Aurora #AuroraBorealis #NorthernLights #SolarSystem #Sun #Astrophotography #Astrophotographer #EvaKristiansen #Tromsø #Norway #Norge #UnitedStates #STEM #Education

Cyclone Horacio: East of Madagascar, Indian Ocean | Meteosat-12 Weather Satellite

Cyclone Horacio: East of Madagascar, Indian Ocean | Meteosat-12 Weather Satellite


Cyclone Horacio, captured on February 23, 2026, by the Flexible Combined Imager (FCI) instrument onboard Europe's Meteosat-12 geostationary weather satellite at an altitude of around 36,000 kilometers. Currently positioned far to the east of Madagascar, the cyclone is forecast to move south and gradually weaken. The Meteosat weather satellites provide imagery for the early detection of fast-developing severe weather, weather forecasting and climate monitoring.

The progression of the storm can be followed every ten minutes on EUMETView: https://view.eumetsat.int/productviewer?v=180312

In meteorology, a cyclone is a large air mass that rotates around a strong center of low atmospheric pressure, counterclockwise in the Northern Hemisphere and clockwise in the Southern Hemisphere as viewed from above (opposite to an anticyclone). Cyclones are characterized by inward-spiraling winds that rotate about a zone of low pressure. Cyclones have also been seen on planets other than the Earth, such as Mars, Jupiter, and Neptune.

Madagascar, officially the Republic of Madagascar, is an island country in the Indian Ocean that includes the island of Madagascar and numerous smaller peripheral islands. Lying off the southeastern coast of Africa, it is the world's fourth-largest island, the second-largest island country, and the 46th-largest country overall. 

Launched on December 13, 2022, Meteosat-12 scans the full Earth disc every 10 minutes, delivering data more frequently and in sharper detail than its predecessor. It carries two main instruments: the Flexible Combined Imager (FCI) and Lightning Imager (LI). The FCI delivers imaging data in twice as many spectral channels than its predecessor and with an improved spatial resolution, providing more detailed views of fast-changing weather such as storms, fog, and rapidly forming clouds. The satellite also carries the LI, Europe’s first space-based instrument to detect lightning across Europe and Africa, day and night, helping forecasters assess storm development, intensity, and risk.

EUMETSAT has established cooperation with Earth observation satellite operators in Europe, China, India, Japan, South Korea and the United States.


United Nations: What is Climate Change?
https://www.un.org/en/climatechange/what-is-climate-change

Image Credit: European Organization for the Exploitation of Meteorological Satellites (EUMETSAT)
Release Date: Jan. 8, 2026

#NASA #ESA #EUMETSAT #Space #Science #Satellites #Planets #Earth #IndianOcean #Cyclones #CycloneHoracio #Madagascar #Weather #Meteorology #Environment #Climate #ClimateChange #GlobalHeating #Meteosat12 #MeteosatSatellites #EarthObservation #Europe #EuropeanUnion #InternationalCooperation #CivilianSpace #STEM #Education

Martian ‘Spiderwebs’ Up Close: Mineral Nodules Revealed | NASA Curiosity Rover

Martian ‘Spiderwebs’ Up Close: Mineral Nodules Revealed | NASA Curiosity Rover

These bumpy nodules were formed by minerals left behind as groundwater was drying out on Mars billions of years ago. NASA’s Curiosity rover captured images of these pea-size features while exploring geologic formations called boxwork on Aug. 21, 2025. 
NASA’s Curiosity Mars rover captured this panorama of boxwork formations—the low ridges seen here with hollows in between the—using its Mastcam on Sept. 26, 2025.

A hilly landscape that looks like spiderwebs when viewed from orbit holds clues to the history of water on ancient Mars.

For about six months, NASA’s Curiosity Mars rover has been exploring a region full of geologic formations called boxwork, low ridges standing roughly 3 to 6 feet (1 to 2 meters) tall with sandy hollows in between. Crisscrossing the surface for miles, the formations suggest ancient groundwater flowed on this part of the Red Planet later than scientists expected. This possibility raises new questions about how long microbial life could have survived on Mars billions of years ago, before rivers and lakes dried up and left a freezing desert world behind.

The boxwork formations look like giant spiderwebs when viewed from space. To explain the shapes, scientists have proposed that groundwater once flowed through large fractures in the bedrock, leaving behind minerals. Those minerals then strengthened the areas that became ridges while other portions without mineral reinforcement were eventually hollowed out by wind.

Until Curiosity arrived at this region, however, no one could be sure what these formations looked like up close, and there were even more questions about how they were made.

Unpacking boxwork
Although Earth also has boxwork ridges, they are rarely taller than a few centimeters and are usually found in caves or in dry, sandy environments. The Curiosity team wanted to get a close look at the Martian formations and gather more data. This posed a real challenge for rover drivers. They needed to send instructions to Curiosity, the size of a sport utility vehicle-size weighing nearly a ton (899 kilograms), so that it could roll across the tops of ridges not much wider than the rover itself.

“It almost feels like a highway we can drive on. But then we have to go down into the hollows, where you need to be mindful of Curiosity’s wheels slipping or having trouble turning in the sand,” said operations systems engineer Ashley Stroupe of NASA’s Jet Propulsion Laboratory in Southern California that built Curiosity and leads the mission. “There’s always a solution. It just takes trying different paths.”

For scientists, the challenge is piecing together how such a vast network of boxwork could exist on Mount Sharp, the 3-mile-tall (5-kilometer-tall) mountain the rover has been ascending. Each layer of the mountain formed in a different era of Mars’ ancient, changing climate. The higher Curiosity goes, the more the landscape bears signs that water was drying out over time with occasional wet periods that saw the return of rivers and lakes.

“Seeing boxwork this far up the mountain suggests the groundwater table had to be pretty high,” said Tina Seeger of Rice University in Houston, one of the mission scientists leading the boxwork investigation. “And that means the water needed for sustaining life could have lasted much longer than we thought looking from orbit.”

Previous orbital imagery included one crucial piece of evidence—dark lines running across the “spiderwebs.” In 2014, it was proposed that these lines might be what are known as central fractures, where groundwater seeped through rock cracks and allowed minerals to concentrate. Investigating the ridges up close, Curiosity found that these lines are in fact fractures, lending weight to that hypothesis.

The rover also discovered bumpy textures called nodules, an obvious sign of past groundwater that has been spotted many times by Curiosity and other Mars missions. Unexpectedly, these nodules were not found near the central fractures, but along a ridge’s walls and the hollows between them.

“We can’t quite explain yet why the nodules appear where they do,” Seeger said. “Maybe the ridges were cemented by minerals first, and later episodes of groundwater left nodules around them.”

Roving laboratory
A major part of Curiosity’s science centers on rock samples collected by the rock-pulverizing drill on the end of the rover’s robotic arm. The resulting powder can be trickled into complex science instruments in the vehicle’s body for analysis.

Last year, three samples from the boxwork region—one from a ridgetop, one from bedrock within a hollow, and one from a transitional area before Curiosity reached the ridges—were collected by the drill and analyzed with X-rays and a high-temperature oven. The X-ray analyses found clay minerals in the ridge and carbonate minerals in the hollow, providing additional clues to help understand how these features formed.

The mission recently collected a fourth sample that was analyzed with a special technique reserved for the most intriguing science targets. After the pulverized rock went into the rover’s high-temperature oven, chemical reagents reacted with the sample to conduct what is called wet chemistry. The resulting reactions make it easier to detect certain organic compounds, carbon-based molecules important to the formation of life.

Sometime in March, Curiosity will leave the boxwork formations behind. The whole region is part of a layer on Mount Sharp enriched in salty minerals called sulfates that formed as water was drying out on Mars. Curiosity’s team plans to continue exploring this sulfate layer for many miles in the coming year, learning more about how the ancient Red Planet’s climate changed billions of years ago.

More about Curiosity
Curiosity was built by NASA’s Jet Propulsion Laboratory, managed by Caltech in Pasadena, California. JPL leads the mission on behalf of NASA’s Science Mission Directorate in Washington as part of NASA’s Mars Exploration Program portfolio.

Celebrating 13+ Years on Mars (2012-2025)
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

To learn more about Curiosity, visit: science.nasa.gov/mission/msl-curiosity

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


Credit: NASA/JPL-Caltech/MSSS
Release Date: Feb. 23, 2026

#NASA #Space #Astronomy #Science #Planets #Mars #Astrobiology #Geology #BoxworkFormations #Groundwater #Minerals #Nodules #CuriosityRover #MSL #MountSharp #GaleCrater #Robotics #SpaceTechnology #SpaceEngineering #MSSS #JPL #Caltech #UnitedStates #STEM #Education

Monday, February 23, 2026

A Young "Sun" Caught Blowing Bubbles | NASA's Chandra X-ray Observatory

A Young "Sun" Caught Blowing Bubbles | NASA's Chandra X-ray Observatory 


For the first time, astronomers have seen a bubble around a star that is similar in size and mass to our Sun, but much younger. This discovery, made using NASA’s Chandra X-ray Observatory, teaches astronomers about what may have been happening on our own Sun billions of years ago.

The discovery of this bubble, called an “astrosphere” by astronomers, was made around the star named HD 61005. This star is located about 120 light-years from Earth in the constellation Puppis.

Where does this astrosphere come from? 
Winds from the star’s surface are blowing up the bubble and filling it with hot gas as it expands into much cooler gas and dust surrounding the star. Our Sun has a similar bubble called the heliosphere. Scientists are interested not only how the heliosphere works today, but also how it behaved in the past.

The discovery of the astrosphere around HD 61005 gives them a window into our younger Sun. HD 61005 is only about 100 million years old, compared to the Sun’s age of about 5 billion years. Because it is so young, HD 61005 has winds of particles blowing from its surface that are about hundreds of times stronger than the wind from the Sun.

This is the first full view of an astrosphere that astronomers have obtained around a star like the Sun. For a few decades, astronomers have been trying to get an image of an astrosphere. Up until now, they were only able to capture images that were just a single point of light and did not give any information on the structure of the astrosphere itself.

Chandra was finally able to detect the astrosphere around HD 61005 because it is producing X-rays as the stellar wind runs into cooler dust and gas that surrounds the star. It required an X-ray telescope with the sharp vision of Chandra, plus a long enough observation time to collect the data to make this discovery.

Previously, astronomers had nicknamed HC 61005 the “Moth” because the large amounts of dust in a disk around the star that you can see in infrared data. This gives it the appearance of the insect. This disk formed when rocks and icy bodies left behind after the star collided together. This is where the Kuiper Belt in our own solar system came from.

Because the strong wind should be blowing dust in the disk away from the star, the dust that makes up the moth-like structure around HD 61005 either does not last very long or is continually replenished by an unseen massive disk that keeps stirring itself to create more dust grains. This is something that astronomers will continue to investigate.

While you will not be able to see all the things that Chandra and the other telescopes in space can, you can spot it with binoculars if you know where to look!


Video Credit: NASA's Chandra X-ray Observatory
Duration: 3 minutes, 27 seconds
Release Date: Feb. 23, 2026

#NASA #Space #Astronomy #Science #Stars #HD61005 #Astrosphere #PuppisConstellation #Heliophysics #Astrophysics #Cosmos #Universe #NASAChandra #ChandraObservatory #SpaceTelescopes #XrayAstronomy #MSFC #UnitedStates #STEM #Education #HD #Video