Tuesday, February 24, 2026

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

Spiral Galaxy NGC 1637: Wide-field view of surrounding area | ESO

Spiral Galaxy NGC 1637: Wide-field view of surrounding area | ESO

This image shows the sky around spiral galaxy NGC 1637 located about 38 million light-years away in the constellation of Eridanus (The River). It was created from images from the Digitized Sky Survey 2 (DSS2).

In 1999 and 2025, scientists discovered supernovae in this galaxy and followed its slow fading over the following years.

The Digitized Sky Survey (DSS) is a ground-based imaging survey of the entire sky in several colors of light produced by the Space Telescope Science Institute through its Guide Star Survey group.

Credit: ESO/Digitized Sky Survey 2. Acknowledgement: Davide De Martin
Release Date: March 20, 2013

#NASA #Astronomy #Space #Science #Galaxies #NGC1637 #Supernovae #1999em #2025pht #TypeIISupernovae #EridanusConstellation #Cosmos #Universe #DSS2 #GSFC #STScI #UnitedStates #Europe #STEM #Education

Journey to Galaxy NGC 1637 in Eridanus | European Southern Observatory

Journey to Galaxy NGC 1637 in Eridanus | European Southern Observatory


This video sequence starts with a view of the bright constellation of Orion (The Hunter). As we zoom in, we focus on an adjacent region of the constellation of Eridanus (The River) and a faint glow appears. This is the spiral galaxy NGC 1637, appearing in all its glory in the final view from the European Southern Observatory’s Very Large Telescope at the Paranal Observatory in Chile. In 1999, scientists discovered a Type II supernova in this galaxy and followed its slow fading over the following years.

A Type II (Type 2) supernova is a violent explosion occurring at the end of a massive star's life (at least 8–50 solar masses) caused by the rapid core collapse of an iron core. These events are distinguished by the presence of hydrogen spectral lines and occur in spiral galaxies' star-forming regions, leaving behind a neutron star or black hole.


Credit: European Southern Observatory (ESO)
Duration: 46 seconds
Release Date: March 20, 2013

#NASA #Astronomy #Space #Science #Galaxies #NGC1637 #1999em #Supernovae #TypeIISupernovae #EridanusConstellation #Cosmos #Universe #VLT #ParanalObservatory #Chile #SouthAmerica #Europe #STEM #Education #HD #Video

Close-up: Galaxy NGC 1637 in Eridanus | European Southern Observatory

Close-up: Galaxy NGC 1637 in Eridanus | European Southern Observatory

This pan sequence from the European Southern Observatory’s Very Large Telescope (VLT) takes a close look at the Paranal Observatory in Chile shows NGC 1637, a spiral galaxy located about 38 million light-years away in the constellation of Eridanus (The River). In 1999, scientists discovered a Type II supernova in this galaxy and followed its slow fading over the following years. The position of the supernova is marked.

A Type II (Type 2) supernova is a violent explosion occurring at the end of a massive star's life (at least 8–50 solar masses) caused by the rapid core collapse of an iron core. These events are distinguished by the presence of hydrogen spectral lines and occur in spiral galaxies' star-forming regions, leaving behind a neutron star or black hole.


Credit: European Southern Observatory (ESO)
Duration: 46 seconds
Release Date: March 20, 2013

#NASA #Astronomy #Space #Science #Galaxies #NGC1637 #1999em #Supernovae #TypeIISupernovae #EridanusConstellation #Cosmos #Universe #VLT #ParanalObservatory #Chile #SouthAmerica #Europe #STEM #Education #HD #Video

Supernova 1999em in Galaxy NGC 1637 | European Southern Observatory

Supernova 1999em in Galaxy NGC 1637 | European Southern Observatory

This image from the European Southern Observatory’s Very Large Telescope (VLT) at the Paranal Observatory in Chile shows NGC 1637, a spiral galaxy located about 38 million light-years away in the constellation of Eridanus (The River). In 1999, scientists discovered a Type II supernova in this galaxy and followed its slow fading over the following years. The position of the supernova is marked.

A Type II (Type 2) supernova is a violent explosion occurring at the end of a massive star's life (at least 8–50 solar masses) caused by the rapid core collapse of an iron core. These events are distinguished by the presence of hydrogen spectral lines and occur in spiral galaxies' star-forming regions, leaving behind a neutron star or black hole.


Credit: European Southern Observatory (ESO)
Release Date: March 20, 2013

#NASA #Astronomy #Space #Science #Galaxies #NGC1637 #1999em #Supernovae #EridanusConstellation #Cosmos #Universe #VLT #ParanalObservatory #Chile #SouthAmerica #Europe #STEM #Education

Spiral Galaxy NGC 1637 in Eridanus: Supernova Found | Webb & Hubble Telescopes

Spiral Galaxy NGC 1637 in Eridanus: Supernova Found | Webb & Hubble Telescopes


Forty million years ago, a star in a nearby galaxy exploded, spewing material across space and generating a brilliant beacon of light. That light traveled across the cosmos, reaching Earth on June 29, 2025, where it was detected by the All-Sky Automated Survey for Supernovae. Astronomers immediately turned their resources to this new supernova, designated 2025pht, to learn more about it. However, one team of scientists instead turned to archives, seeking to use pre-supernova images to identify exactly which star among many had exploded. And they succeeded.

Images of galaxy NGC 1637 taken by the James Webb Space Telescope showed a single red supergiant star located exactly where the supernova now shines. This represents the first published detection of a supernova progenitor by Webb. The results were published in the Astrophysical Journal Letters.

“We’ve been waiting for this to happen—for a supernova to explode in a galaxy that Webb had already observed. We combined Hubble and Webb data sets to completely characterize this star for the first time,” said lead author Charlie Kilpatrick of Northwestern University in the United States.

The main image at left shows a combined Webb and Hubble view of spiral galaxy NGC 1637 with the region of interest in the top right. The remaining three panels show a detailed view of a red supergiant star before and after it exploded. The star is not visible in the Hubble image before the explosion, but appears in the Webb image. The July 2025 view from Hubble shows the glowing aftermath of the explosion.

By carefully aligning Hubble and Webb images taken of NGC 1637, the team was able to identify the progenitor star in images taken by Webb’s MIRI (Mid-Infrared Instrument) and NIRCam (Near-Infrared Camera) in 2024. They found that the star appeared surprisingly red—an indication that it was surrounded by dust that blocked shorter, bluer wavelengths of light.

“It’s the reddest, most dusty red supergiant that we’ve seen explode as a supernova,” said graduate student and co-author Aswin Suresh of Northwestern University.


Credit: NASA, ESA, CSA, STScI, C. Kilpatrick (Northwestern), A. Suresh (Northwestern); Image Processing: J. DePasquale (STScI)
Release Date: Feb. 23, 2026

#NASA #Astronomy #Space #Science #Galaxies #NGC1637 #2025pht #Supernovae #EridanusConstellation #Cosmos #Universe #SpaceTelescopes #HubbleSpaceTelescope #HST #WebbTelescope #JWST #ESA #CSA #GSFC #STScI #Europe #UnitedStates #STEM #Education

Two's Company: Binary Star System AFGL 4106 in Carina | ESO

Two's Company: Binary Star System AFGL 4106 in Carina | ESO

The pair of points at the center of the image, taken with the European Southern Observatory ’s Very Large Telescope (VLT), are an old stellar couple—a binary system officially called AFGL 4106. As most stars are born in pairs, a big question for astronomers is how does being in a couple impact a star's death?

Before dying, stars expel huge amounts of gas and dust, ingredients for a growing nebula. The massive stars shown here are at close yet distinct late stages of their lifecycles with one having blown off enough mass to produce a dusty surrounding envelope. In a new paper led by Gabriel Tomassini, a PhD student at the Université Côte d’Azur (France), researchers have mapped this debris, shown here in orange, and precisely characterized the central stars (marked in black).

Imaging astronomical objects close to stars poses a challenge due to the overpowering effect of a star's brightness and, in fact, the stars themselves appear in black as their brightness saturated the detector of the instrument used to make this image. Fortunately, the SPHERE instrument on the VLT is well equipped to deal with large contrasts in light levels, enabling a detailed study of both the high luminosity stars and the faint surrounding nebula for the first time. Moreover, it can correct the blur caused by atmospheric turbulence, delivering very sharp images.

The shape of the nebula reveals the significant impact the companion is having on the gas ejection of the dying star, introducing asymmetries and shifting the clouds of gas and dust away from a perfectly spherical shape. Further observations of star systems like this one allow scientists to better understand how the presence of companions affects the death of stars.

Image Description: This image consists of an orange slightly egg-shaped nebula with a cloud-like texture against a black background. The nebula is more yellow-orange and opaque at the center and darker-orange and more diffuse at its perimeter. At the center of the image inside the nebula there are two small black dots. Diagonal lines the same colour as the nebula form a cross centered on the black dots.


Credit: ESO/G. Tomassini et al.
Release Date: Feb. 23, 2026

#NASA #ESO #Astronomy #Space #Science #Nebulae #Stars #BinaryStarSystems #AFGL4106 #HD302821 #CarinaConstellation #Cosmos #Universe #VLT #SPHERE #ParanalObservatory #Chile #SouthAmerica #Europe #STEM #Education

Spiral Galaxy NGC 7331 in Pegasus: Wide-view | Kitt Peak National Observatory

Spiral Galaxy NGC 7331 in Pegasus: Wide-view | Kitt Peak National Observatory

NGC 7331 is the brightest and closest galaxy in the visual galaxy group that bears its name, the NGC 7331 Group. It is one of 18 galaxies chosen by the HST Extragalactic Distance Scale Key Project to calibrate secondary distance estimators. The project is using the Hubble Space Telescope (HST) to obtain an accurate distance to galaxies via Cepheid variables, with the ultimate goal of using these to measure H0 (a cosmological parameter) to an external accuracy of 10%. It was determined this galaxy is about 40 million light years away (and perhaps 30,000 light years across). In this image, you can see examples of its nearby neighbors—both spiral and elliptical galaxies. Nearby this field (not shown) is another famous group of galaxies known as Stephan's Quintet.

Also known as Caldwell 30, this galaxy is often thought of as a twin to the Milky Way owing to its similar size and spiral structure. However, there are a couple of features of its core that set it apart from our home galaxy. For instance, astronomers have found evidence that the Milky Way has a central bar of stars and dust cutting through its center, a feature common to many spiral galaxies. However, NGC 7331 lacks this feature. Additionally, NGC 7331’s central bulge rotates in the opposite direction to its galactic disk—unusual behavior compared to other galaxies and unlike what we observe in the Milky Way.

This image was taken as part of Advanced Observing Program (AOP) at Kitt Peak Visitor Center during 2014.


Credit: KPNO/NOIRLab/NSF/AURA/Paul Mortfield and Dietmar Kupke/Flynn Haase
Release Date: May 7, 2014


#NASA #Astronomy #Space #Science #Galaxies #NGC7331 #Caldwell30 #NGC7331Group #PegasusConstellation #Cosmos #Universe #KPNO #KittPeakNationalObservatory #Arizona #NOIRLab #NSF #AURA #STEM #Education

Spiral Galaxy NGC 7331 in Pegasus: A Milky Way Twin | Gemini North Telescope

Spiral Galaxy NGC 7331 in Pegasus: A Milky Way Twin | Gemini North Telescope

The magnificent spiral galaxy NGC 7331, located approximately 40 million light-years away in the constellation Pegasus, is the brightest and closest galaxy in the visual galaxy group that bears its name, the NGC 7331 Group. Revealed in the details of this image are populations of hot stars and dark dust lanes winding throughout the spiral arms. 

Also known as Caldwell 30, this galaxy is often thought of as a twin to the Milky Way owing to its similar size and spiral structure. However, there are a couple of features of its core that set it apart from our home galaxy. For instance, astronomers have found evidence that the Milky Way has a central bar of stars and dust cutting through its center, a feature common to many spiral galaxies. However, NGC 7331 lacks this feature. Additionally, NGC 7331’s central bulge rotates in the opposite direction to its galactic disk—unusual behavior compared to other galaxies and unlike what we observe in the Milky Way.

This image was taken by Gemini North, one half of the International Gemini Observatory, supported in part by the U.S. National Science Foundation and operated by NSF NOIRLab.

Learn about the Gemini North Telescope:
https://noirlab.edu/public/programs/gemini-observatory/gemini-north/


Credit: International Gemini Observatory/NOIRLab/NSF/AURA
Image Processing: J. Miller (International Gemini Observatory/NSF NOIRLab), M. Rodriguez (International Gemini Observatory/NSF NOIRLab) & M. Zamani (NSF NOIRLab)
Release Date: Dec. 18, 2024


#NASA #Astronomy #Space #Science #Galaxies #NGC7331 #Caldwell30 #NGC7331Group #PegasusConstellation #Cosmos #Universe #InternationalGeminiObservatory #GeminiNorthTelescope #GeMS #AdaptiveOptics #Maunakea #Hawaii #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

Sunday, February 22, 2026

Aurora Australis: View from New Zealand

Aurora Australis: View from New Zealand


Astrophotographer Ian Griffin: "Cloud filled the sky over Dunedin, New Zealand, as geomagnetic activity began to rise—but experience (and stubborn optimism) sent me out anyway. For a while, it looked hopeless. Then the clouds thinned, the southern horizon cleared, and the sky exploded. A brilliant aurora australis surged over Hoopers Inlet tonight, green fire along the horizon with crimson towers reaching high into the stars. Reflected in the still water below, the display followed intensified solar wind conditions that pushed the auroral oval deep over New Zealand’s South Island. It was one of those unforgettable southern nights when patience is suddenly and spectacularly rewarded. Now, all I have to do is get up for work in the morning . . ."

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/

Image Credit: Ian Griffin 
Ian's website: https://www.instagram.com/portobellopictures/
Location: Hoopers Inlet, South Island, New Zealand 
Date: Feb. 22, 2026

#NASA #Space #Astronomy #Science #Sun #SolarSystem #Planets #Earth #Aurora #AuroraAustralis #SouthernLights #Astrophotography #IanGriffin #Astrophotographer #HoopersInlet #SouthIsland #NewZealand #STEM #Education 

Planet Mars Images: Feb. 17-22, 2026 | NASA's Curiosity & Perseverance Rovers

Planet Mars Images: Feb. 17-22, 2026 | NASA's Curiosity & Perseverance Rovers

Mars 2020 - sol 1779
MSL - sol 4810
Mars 2020 - sol 1777
Mars 2020 - sol 1779
Mars 2020 - sol 1779
Mars 2020 - sol 1779
Mars 2020 - sol 1779
Mars 2020 - sol 1780

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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

Celebrating 5+ 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: Feb. 17-22, 2026

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

Globular Star Cluster NGC 1851 in Columba: Near Infrared | Gemini North Telescope

Globular Star Cluster NGC 1851 in Columba: Near Infrared | Gemini North Telescope

This near-infrared image obtained with GeMS adaptive optics system resolves the stars inside NGC 1851, an ancient globular star cluster around 40,000 light-years away. NGC 1851, or Caldwell 73, was discovered by the Scottish astronomer James Dunlop in 1826. This dense globular cluster can be spotted through a pair of binoculars, appearing as a fuzzy patch of light. Small telescopes can resolve examples of the cluster’s individual stars, away from its compact center. Caldwell 73 is easiest to view from equatorial latitudes in the Northern Hemisphere during the winter and from the Southern Hemisphere during the summer.

The stars in many known globular clusters are about the same age, indicating that the stars formed at roughly the same time. However, observations of Caldwell 73 reveal that it hosts stellar populations with distinct ages. The cluster is also encircled by a diffuse halo of stars. Although the origins of the halo and multiple star populations are unknown, one idea is that Caldwell 73 is a remnant of two clusters that collided within a dwarf galaxy that once hosted them both. When the clusters merged, the outer regions of the host galaxy may have been stripped away via interactions with more massive galaxies, leaving only the stellar nucleus and halo behind.

Learn about the Gemini North Telescope:
https://noirlab.edu/public/programs/gemini-observatory/gemini-north/


Credit: International Gemini Observatory, Alan McConnachie (Herzberg Institute of Astrophysics) and T.A. Rector (University of Alaska Anchorage)
Release Date: June 30, 2020

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Globular Star Cluster NGC 1851 in Columba | Hubble

Globular Star Cluster NGC 1851 in Columba | Hubble

NGC 1851, or Caldwell 73, was discovered by the Scottish astronomer James Dunlop in 1826. It is located roughly 40,000 light-years from Earth in the constellation Columba and has an apparent magnitude of 7.3. This dense globular cluster can be spotted through a pair of binoculars, appearing as a fuzzy patch of light. Small telescopes can resolve examples of the cluster’s individual stars, away from its compact center. Caldwell 73 is easiest to view from equatorial latitudes in the Northern Hemisphere during the winter and from the Southern Hemisphere during the summer.

The stars in many known globular clusters are about the same age, indicating that the stars formed at roughly the same time. However, observations of Caldwell 73 reveal that it hosts stellar populations with distinct ages. The cluster is also encircled by a diffuse halo of stars. Although the origins of the halo and multiple star populations are unknown, one idea is that Caldwell 73 is a remnant of two clusters that collided within a dwarf galaxy that once hosted them both. When the clusters merged, the outer regions of the host galaxy may have been stripped away via interactions with more massive galaxies, leaving only the stellar nucleus and halo behind.

This image of Caldwell 73 was captured by Hubble’s Wide Field Camera 3. It is a composite of multiple observations taken at ultraviolet and visible wavelengths. The observations were taken to help astronomers better understand why some globular clusters appear to play host to multiple generations of stars. A bright, blue, giant star appears to the lower left of center.


Credit: NASA, ESA, and G. Piotto (Università degli Studi di Padova)
Image Processing: Gladys Kober (NASA/Catholic University of America)
Release Date: April 9, 2019

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