Tuesday, March 03, 2026

Close-up: Cat’s Eye Nebula—NGC 6543 in Draco | Hubble & Euclid Space Telescopes

Close-up: Cat’s Eye NebulaNGC 6543 in Draco | Hubble & Euclid Space Telescopes

This is a Hubble image of one of the most visually intricate remnants of a dying star—the Cat’s Eye Nebula, also known as NGC 6543. This extraordinary planetary nebula has captivated astronomers for decades with its elaborate and multilayered structure. Observations with the European Space Agency’s Gaia mission place the nebula at a distance of 4,400 light years away in the Draco constellation.

This time, Hubble is joined by ESA’s Euclid space telescope to create a new image of NGC 6543. The nebula is showcased through the combined eyes of Hubble and Euclid, revealing the remarkable complexity of stellar death in this object. Though primarily designed to map the distant Universe, Euclid captures the Cat’s Eye Nebula as part of its deep imaging surveys. In Euclid’s wide, near-infrared and visible light view, the arcs and filaments of the nebula’s bright central region are situated within a halo of colorful fragments of gas zooming away from the star. This ring was ejected from the star at an earlier stage before the main nebula at the center formed. 

Planetary nebulae, so-called because of their round shape when viewed through early telescopes, are in fact expanding gas thrown off by stars in their final stages of evolution. It was the Cat’s Eye Nebula itself where this fact was first discovered in 1864—examining the spectrum of its light reveals the emission from individual molecules that is characteristic of a gas, distinguishing planetary nebulae from stars and galaxies.

The NASA/ESA Hubble Space Telescope has expanded our understanding of planetary nebulae; its detailed images showed that the simple, circular appearance of a planetary nebula seen from the ground belies a very complex morphology. This was particularly true of the Cat’s Eye Nebula, where Hubble’s images in 1995 revealed never-before-seen structures that broadened our understanding of how planetary nebulae come to be.

This new Hubble image shows the nebula's core filled with billowing gas via the High Resolution Channel sub-instrument on its Advanced Camera for Surveys (ACS). This instrument is optimized for capturing very sharp images of fine details in a small area, such as the complex features here. The data presents a mixture of concentric shells, jets of high-speed gas and dense knots formed by shock interactions. These structures are believed to record episodic mass loss from the dying star at the nebula’s center, creating a  record of its final stages.

Image Description: Two images of a planetary nebula in space. The image to the left, labeled “Euclid & Hubble”, shows the whole nebula and its surroundings. A star in the very center is surrounded by white bubbles and loops of gas, all shining with a powerful blue light. Farther away a broken ring of red and blue gas clouds surrounds the nebula. The background shows many stars and distant galaxies. A white box indicates the center of the nebula and this region is the image to the right, labeled “Hubble”. It shows the multi-layered bubbles, pointed jets and circular shells of gas that make up the nebula, as well as the central star, in greater detail.


Credit: ESA/Hubble & NASA, ESA Euclid/Euclid Consortium/NASA/Q1-2025, J.-C. Cuillandre & E. Bertin (CEA Paris-Saclay), Z. Tsvetanov
Duration: 30 seconds
Release Date: March 3, 2026

#NASA #ESA #Astronomy #Space #Science #Nebulae #PlanetaryNebulae #CatsEyeNebula #NGC6543 #Caldwell6 #DracoConstellation #MilkyWayGalaxy #Cosmos #Universe #HubbleSpaceTelescope #HST #EuclidSpaceTelescope #EST #SpaceTelescopes #Europe #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Cat’s Eye Nebula: NGC 6543 in Draco | Hubble & Euclid Space Telescopes

Cat’s Eye NebulaNGC 6543 in Draco | Hubble & Euclid Space Telescopes

This is a Hubble image of one of the most visually intricate remnants of a dying star—the Cat’s Eye Nebula, also known as NGC 6543. This extraordinary planetary nebula has captivated astronomers for decades with its elaborate and multilayered structure. Observations with the European Space Agency’s Gaia mission place the nebula at a distance of 4,400 light years away in the Draco constellation.

This time, Hubble is joined by ESA’s Euclid space telescope to create a new image of NGC 6543. The nebula is showcased through the combined eyes of Hubble and Euclid, revealing the remarkable complexity of stellar death in this object. Though primarily designed to map the distant Universe, Euclid captures the Cat’s Eye Nebula as part of its deep imaging surveys. In Euclid’s wide, near-infrared and visible light view, the arcs and filaments of the nebula’s bright central region are situated within a halo of colorful fragments of gas zooming away from the star. This ring was ejected from the star at an earlier stage before the main nebula at the center formed. 

Planetary nebulae, so-called because of their round shape when viewed through early telescopes, are in fact expanding gas thrown off by stars in their final stages of evolution. It was the Cat’s Eye Nebula itself where this fact was first discovered in 1864—examining the spectrum of its light reveals the emission from individual molecules that is characteristic of a gas, distinguishing planetary nebulae from stars and galaxies.

The NASA/ESA Hubble Space Telescope has expanded our understanding of planetary nebulae; its detailed images showed that the simple, circular appearance of a planetary nebula seen from the ground belies a very complex morphology. This was particularly true of the Cat’s Eye Nebula, where Hubble’s images in 1995 revealed never-before-seen structures that broadened our understanding of how planetary nebulae come to be.

This new Hubble image shows the nebula's core filled with billowing gas via the High Resolution Channel sub-instrument on its Advanced Camera for Surveys (ACS). This instrument is optimized for capturing very sharp images of fine details in a small area, such as the complex features here. The data presents a mixture of concentric shells, jets of high-speed gas and dense knots formed by shock interactions. These structures are believed to record episodic mass loss from the dying star at the nebula’s center, creating a  record of its final stages.

Image Description: Two images of a planetary nebula in space. The image to the left, labeled “Euclid & Hubble”, shows the whole nebula and its surroundings. A star in the very center is surrounded by white bubbles and loops of gas, all shining with a powerful blue light. Farther away a broken ring of red and blue gas clouds surrounds the nebula. The background shows many stars and distant galaxies. A white box indicates the center of the nebula and this region is the image to the right, labeled “Hubble”. It shows the multi-layered bubbles, pointed jets and circular shells of gas that make up the nebula, as well as the central star, in greater detail.


Credit: ESA/Hubble & NASA, ESA Euclid/Euclid Consortium/NASA/Q1-2025, J.-C. Cuillandre & E. Bertin (CEA Paris-Saclay), Z. Tsvetanov
Release Date: March 3, 2026

#NASA #ESA #Astronomy #Space #Science #Nebulae #PlanetaryNebulae #CatsEyeNebula #NGC6543 #Caldwell6 #DracoConstellation #MilkyWayGalaxy #Cosmos #Universe #HubbleSpaceTelescope #HST #EuclidSpaceTelescope #EST #SpaceTelescopes #Europe #GSFC #STScI #UnitedStates #Infographics #STEM #Education

Close-up: The Cat’s Eye Nebula in Draco—A New View | Hubble Space Telescope

Close-up: The Cat’s Eye Nebula in DracoA New View | Hubble Space Telescope


This is a new Hubble image of one of the most visually intricate remnants of a dying star—the Cat’s Eye Nebula, also known as NGC 6543. This extraordinary planetary nebula has captivated astronomers for decades with its elaborate and multilayered structure. Observations with the European Space Agency’s Gaia mission place the nebula at a distance of 4,400 light years away.

Planetary nebulae, so-called because of their round shape when viewed through early telescopes, are in fact expanding gas thrown off by stars in their final stages of evolution. It was the Cat’s Eye Nebula itself where this fact was first discovered in 1864—examining the spectrum of its light reveals the emission from individual molecules that is characteristic of a gas, distinguishing planetary nebulae from stars and galaxies.

The NASA/ESA Hubble Space Telescope also expanded our understanding of planetary nebulae; its detailed images showed that the simple, circular appearance of a planetary nebula seen from the ground belies a very complex morphology. This was particularly true of the Cat’s Eye Nebula, where Hubble’s images in 1995 revealed never-before-seen structures that broadened our understanding of how planetary nebulae come to be.

This new Hubble image shows the nebula's core filled with billowing gas via the High Resolution Channel sub-instrument on its Advanced Camera for Surveys (ACS). This instrument is optimized for capturing very sharp images of fine details in a small area, such as the complex features here. The data presents a mixture of concentric shells, jets of high-speed gas and dense knots sculpted by shock interactions. These structures are believed to record episodic mass loss from the dying star at the nebula’s center, creating a  record of its final stages.

A portion of this data was used in a previous image of the Cat’s Eye Nebula, released in 2004. Previously unused data from ACS is combined with the latest processing techniques to create this new image, the sharpest so far.

Image Description: An image of the center of a planetary nebula. A blue star sits at the center within a series of overlapping, translucent bubbles of gas. The bubbles have a complex, filamentary structure. The two largest bubbles overlap halfway, creating an eye-like shape with the star at the center. Jets of high-speed gas point out of the top and bottom of the nebula. Faint, concentric circles of gas also surround the star, out beyond the bubbles.


Credit: ESA/Hubble & NASA, Z. Tsvetanov
Duration: 30 seconds
Release Date: March 3, 2026

#NASA #ESA #Astronomy #Space #Science #Nebulae #PlanetaryNebulae #CatsEyeNebula #NGC6543 #Caldwell6 #DracoConstellation #MilkyWayGalaxy #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

The Cat’s Eye Nebula in Draco: A New View | Hubble Space Telescope

The Cat’s Eye Nebula in Draco: A New View | Hubble Space Telescope


This is a new Hubble image of one of the most visually intricate remnants of a dying star: the Cat’s Eye Nebula, also known as NGC 6543. This extraordinary planetary nebula has captivated astronomers for decades with its elaborate and multilayered structure. Observations with the European Space Agency’s Gaia mission place the nebula at a distance of 4,400 light years away.

Planetary nebulae, so-called because of their round shape when viewed through early telescopes, are in fact expanding gas thrown off by stars in their final stages of evolution. It was the Cat’s Eye Nebula itself where this fact was first discovered in 1864—examining the spectrum of its light reveals the emission from individual molecules that is characteristic of a gas, distinguishing planetary nebulae from stars and galaxies.

The NASA/ESA Hubble Space Telescope also expanded our understanding of planetary nebulae; its detailed images showed that the simple, circular appearance of a planetary nebula seen from the ground belies a very complex morphology. This was particularly true of the Cat’s Eye Nebula, where Hubble’s images in 1995 revealed never-before-seen structures that broadened our understanding of how planetary nebulae come to be.

This new Hubble image shows the nebula's core filled with billowing gas via the High Resolution Channel sub-instrument on its Advanced Camera for Surveys (ACS). This instrument is optimized for capturing very sharp images of fine details in a small area, such as the complex features here. The data presents a mixture of concentric shells, jets of high-speed gas and dense knots sculpted by shock interactions. These structures are believed to record episodic mass loss from the dying star at the nebula’s center, creating a  record of its final stages.

A portion of this data was used in a previous image of the Cat’s Eye Nebula, released in 2004. Previously unused data from ACS is combined with the latest processing techniques to create this new image, the sharpest so far.

Image Description: An image of the center of a planetary nebula. A blue star sits at the center within a series of overlapping, translucent bubbles of gas. The bubbles have a complex, filamentary structure. The two largest bubbles overlap halfway, creating an eye-like shape with the star at the center. Jets of high-speed gas point out of the top and bottom of the nebula. Faint, concentric circles of gas also surround the star, out beyond the bubbles.


Credit: ESA/Hubble & NASA, Z. Tsvetanov
Release Date: March 3, 2026

#NASA #ESA #Astronomy #Space #Science #Nebulae #PlanetaryNebulae #CatsEyeNebula #NGC6543 #Caldwell6 #DracoConstellation #MilkyWayGalaxy #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education

Lunar Eclipse March 3, 2026: View from Florida

Lunar Eclipse March 3, 2026: View from Florida

Photographer: "Total lunar eclipse of 3/3/2026 at Moonset over the Gulf, just before sunrise from Tarpon Springs, Florida." 

Lunar eclipses occur at the full Moon phase. When Earth is positioned precisely between the Moon and Sun, Earth’s shadow falls upon the surface of the Moon, dimming it and sometimes turning the lunar surface a striking red over the course of a few hours. Each lunar eclipse is visible from half of Earth.

Learn more: https://science.nasa.gov/moon/eclipses/


Image Credit: Barry Ollikkala
Image Details: Canon R7, RF 200-800mm f6.3-9 lens on iOptron Skyguider Pro star tracker, on Meade heavy-duty field tripod
Location: Tarpon Springs, Florida
Release Date: March 3, 2026


#NASA #Space #Astronomy #Science #Sun #SolarSystem #Moon #Earth #LunarEclipse #Umbra #Penumbra #NASAGoddard #GSFC #UnitedStates #TaerponSprings #Florida #Astrophotography #BarryOllikkala #Astrophotographers #Americas #STEM #Education

March 3, 2026 Lunar Eclipse Schedule by Time Zone: The Americas

March 3, 2026 Lunar Eclipse Schedule by Time Zone: The Americas

Pacific Standard Time (PST)
Mountain Standard Time (MST)
Central Standard Time (CST)
Eastern Standard Time (EST)
Coordinated Universal Time (UTC)

Viewing a total lunar eclipse is as easy as looking up! Lunar eclipses are completely eye-safe, unlike solar eclipses. Feel free to enjoy this lunar eclipse with your naked eye!

The eclipse reaches totality at 6:04 a.m. Eastern Time/3:04 a.m. Pacific Time on the morning of Tuesday, March 3, 2026. ⬇️

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 Standard 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. During the eclipse, the Moon is moving through the constellation Leo.


Credits: NASA Goddard/Spaceweather[dot]com
Release Date: March 2, 2026

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

Monday, March 02, 2026

NASA's Crew-12: Home Planet Awe | International Space Station

NASA's Crew-12: Home Planet Awe | International Space Station

Expedition 74 Flight Engineer and European Space Agency Astronaut Sophie Adenot: "Throwback to one of the first pictures of Crew‑12 in space . . . and we were of course looking back at Earth from this orbital vantage point. First‑ and second‑time fliers united in their love for our home planet and their awe at its beauty. We were at a loss for words to describe how stunning Earth is—and how this view made us feel."

"This picture was taken on Saturday, February 14, during the 34 hours SpaceX Dragon Freedom spent chasing the Station before docking."


Expedition 74 Crew
Station Commander: Sergey-Kud Sverchkov (Russia)
Roscosmos (Russia) Flight Engineers: 
Andrey Fedyaev, Sergei Mikaev
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jessica Meir, Jack Hathaway, Chris Williams

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.

Credit: European Space Agency (ESA)/S. Adenot
Image Date: Feb. 14, 2026
Release Date: March 2, 2026

#NASA #Space #ISS #Earth #OverviewEffect #SpaceX #SpaceXCrew12 #CrewDragonSpacecraft #Astronauts #JessicaMeir #JackHathaway #SophieAdenot #France #Europe #ESA #Cosmonauts #AndreyFedyaev #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #JSC #UnitedStates #STEM #Education

How to Watch Lunar Eclipses | NASA

How to Watch Lunar Eclipses | NASA

Viewing a total lunar eclipse is as easy as looking up! Lunar eclipses are completely eye-safe, unlike solar eclipses. Feel free to enjoy this lunar eclipse with your naked eye!

We know space fans want to get the most out of seeing the Moon turn red, so we asked a lunar scientist for tips. This is our breakdown of how to enjoy the eclipse, reaching totality 6:04 a.m. Eastern Time/3:04 a.m. Pacific Time tomorrow morning. ⬇️

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
Duration: 28 seconds
Release Date: March 2, 2026

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

The Dusty Surroundings of Orion and The Pleiades Star Cluster

The Dusty Surroundings of Orion and The Pleiades Star Cluster

This image contains a wide variety of astronomical objects, including the Pleiades star cluster, Barnard's Loop, the Orion Nebula, Aldebaran, Betelgeuse, Witch Head Nebula, Eridanus Loop, and the California Nebula. The 'tapestry' of our night sky has an extremely deep hidden complexity. This image shows a dusty starfield with intricate dust filaments all over. Red, blue, and brown nebulas fill the field.

View labeled version here: 
https://apod.nasa.gov/apod/ap260302.html

This composite image required 16 hours of  exposure in dark skies over Granada, Spain.


Image Credit & Copyright: Ignacio Fernández
Release Date: March 2, 2026

#NASA #Astronomy #Space #Science #Stars #Aldebaran #Betelgeuse #PleiadesStarCluster #Nebulae #WitchHeadNebula #CaliforniaNebula #OrionNebula #BarnardsLoop #EridanusLoop #OrionConstellation #MilkyWayGalaxy #Universe #Astrophotography #IgnacioFernández
 #Astrophotographer #CitizenScience #Granada #Spain #España #GSFC #STEM #Education #APoD

Cosmonaut Photos: Volcanoes of Russia's Kamchatka | International Space Station

Cosmonaut Photos: Volcanoes of Russia's Kamchatka | International Space Station

These images were shared by Expedition 74 Station Commander and Cosmonaut Sergey Kud-Sverchkov of Russia aboard the International Space Station: "There's a place in Russia where people experience volcanoes as a common and integral part of the landscape. This is the Kamchatka Krai! Unlike most of the peninsula's volcanoes, located in hard-to-reach areas, the home volcanoes are located just 25–35 kilometers from the city, and in clear weather, their cones dominate the view."

"So, meet the 🏔 'Home Group' of volcanoes in Petropavlovsk-Kamchatsky (in order of decreasing distance from the coast):

🏔 Koryaksky Volcano (3,456 m)

The absolute dominant feature of the city's panorama. Thanks to its classic conical shape and impressive height, this beauty is visible from virtually anywhere in Petropavlovsk. One of the most picturesque volcanoes on the peninsula, its last eruption occurred in 2008–2009. 

🏔 Avachinsky Volcano (2,741 m)

A truly "working" volcano in Kamchatka is one of the most active and accessible for climbing. You can climb Avacha from Petropavlovsk and return in one day. This is perhaps the easiest way to experience true volcanic activity. (This is what I did.) Its crater regularly makes its presence known with steam and gas emissions. 

🏔 Kozelsky Volcano (~2,180 m)

The least noticeable member of this group, almost merging with Avachinsky, but no less significant. Its slopes are covered with glaciers and snowfields that do not melt even in summer. Of particular interest to climbers and lovers of glacial landscapes."

"Despite their beauty and the kind epithet bestowed upon them by locals, the 'home' volcanoes are active and remain formidable natural features. Keep this in mind when planning a climb."

The Kamchatka Peninsula is a 1,250-kilometer-long (777 mi) peninsula in the Russian Far East with an area of about 270,000 km2 (100,000 sq mi). The Sea of Okhotsk bounds the peninsula's western coastline on the Pacific Ocean.

The Kamchatka Peninsula, the Commander Islands, and Karaginsky Island constitute Kamchatka Krai of the Russian Federation. The Kamchatka Peninsula contains the volcanoes of Kamchatka, a UNESCO World Heritage Site, that form part of the Ring of Fire.


Expedition 74 Crew
Station Commander: Sergey-Kud Sverchkov (Russia)
Roscosmos (Russia) Flight Engineers: 
Andrey Fedyaev, Sergei Mikaev
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jessica Meir, Jack Hathaway, Chris Williams

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.

Credit: Roscosmos/Sergey-Kud Sverchkov
Release Date: Feb. 26, 2026

#NASA #Space #ISS #Planets #Earth #Geology #Stratovolcanoes #Volcanoes #KamchatkaPeninsula #KamchatkaKrai #Камчатка #PacificOcean #SeaOfOkhotsk #EastAsia #Cosmonauts #SergeyKudSverchkov #CosmonautPhotography #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #UnitedStates #STEM #Education

What's Up for March 2026: Skywatching Tips from NASA | JPL

What's Up for March 2026: Skywatching Tips from NASA JPL

Here are examples of skywatching highlights for the northern hemisphere in March 2026:

A total lunar eclipse blood moon takes center stage, Venus and Saturn cozy up for a conjunction, and we celebrate the vernal equinox. 

0:00 Intro

0:12 Total lunar eclipse

1:22 Venus + Saturn conjunction

1:57 Vernal equinox

2:39 March Moon phases

Blood Moons can occur only when the Sun, Earth, and Moon are exactly or very closely aligned with Earth between the other two. During these rare events, the full Moon rapidly darkens and then glows red as it enters the Earth's shadow. A small amount of indirect sunlight is still reaching the Moon, passing through Earth's atmosphere, resulting in a reddish hue. This light appears reddish due to the Rayleigh scattering of blue light—the same reason sunrises and sunsets are more orange than during the day.


Video Credit: NASA's Jet Propulsion Laboratory
Duration: 3 minutes
Release Date: March 2, 2026

#NASA #Astronomy #Space #Science #SolarSystem #Planets #Venus #Saturn #Earth #Moon #BloodMoon #LunarEclipse #Stars #VernalEquinox #Nebulae #Galaxies #MilkyWayGalaxy #Skywatching #JPL #Caltech #UnitedStates #Canada #Mexico #NorthernHemisphere #STEM #Education #HD #Video

Blue Ghost Mission 1 Moon Landing: 1-Year Anniversary | Firefly Aerospace

Blue Ghost Mission 1 Moon Landing: 1-Year Anniversary | Firefly Aerospace

Firefly’s Blue Ghost Mission 1, named Ghost Riders in the Sky, launched on January 15, 2025, and performed the first fully successful commercial Moon landing on March 2. Blue Ghost then completed more than 14 days of surface operations (346 hours of daylight) and just over 5 hours of operations into the lunar night. This achievement marks the longest commercial operations on the Moon to date.

Blue Ghost lander's work was part of NASA’s Commercial Lunar Payload Services (CLPS) initiative and Artemis campaign to establish a long-term lunar presence. Blue Ghost Mission 1 performed science and technology demonstrations, including lunar subsurface drilling, sample collection, and X-ray imaging of Earth’s magnetic field to advance research for future human missions on the Moon, as well as to provide insights into space weather effects.

Learn more about Blue Ghost Mission 1: 

Learn more about CLPS: https://www.nasa.gov/clps


Video Credit: Firefly Aerospace
Duration: 2 minutes
Release Date: June 2, 2025

#NASA #Space #Astronomy #Science #ArtemisProgram #Moon #LunarLanders #FireflyAerospace #BlueGhostLunarLander #BlueGhostMission1 #BGM1 #CommercialSpace #UnitedStates #Robotics #Engineering #SpaceTechnology #SolarSystem #SpaceExploration #MSFC #STEM #Education #HD #Video

Spiral Galaxy NGC 941 in Cetus | Subaru Telescope

Spiral Galaxy NGC 941 in Cetus | Subaru Telescope

NGC 941 is a spiral galaxy about 55 million light-years away in the constellation Cetus. This faint galaxy is classified as an intermediate spiral, exhibiting characteristics between a barred spiral with a central bar and an unbarred spiral. Barred spiral galaxies are a type of spiral galaxy characterized by a central bar-shaped structure composed of stars that extends from the core and leads into spiral arms. They account for about half of all known spiral galaxies, including the Milky Way.

NGC 941 has a diameter of approximately 55,000 light years. The galaxies NGC 926, NGC 934, NGC 936, NGC 955 are located in the same sky area. NGC 941 was discovered by German-British astronomer William Herschel on January 6, 1785.

Learn more about Japan's Subaru Telescope: 
https://subarutelescope.org/en/

Credit: National Astronomical Observatory of Japan (NAOJ)
Release Date: Feb. 25, 2026

#NASA #Astronomy #Space #Science #SubaruTelescope #すばる望遠鏡 #NAOJ #国立天文台 #HyperSuprimeCam #HSC #Galaxies #Galaxy #NGC941 #Galaxy #Supernovae #SN2005ab #CetusConstellation #Cosmos #Universe #Japan #日本 #MaunaKea #Hawaii #UnitedStates #STEM #Education

Aurora Australis over Western Australia

Aurora Australis over Western Australia

"Another one from [the] spectacular worldwide aurora event on May 11, 2024. This was taken at Stirling Dam, 1.5 hours south of Perth in Western Australia."

Also known as the northern lights (aurora borealis) or southern lights (aurora australis), 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: Trevor Dobson
Location: Stirling Dam, Harvey Region, Western Australia
Image Details: Nikon d810a, 35mm, ISO 5000, f/2.0, 5 x 3 seconds
Image Date: May 11, 2024
Release Date: Aug. 15, 2025

#NASA #Space #Astronomy #Science #SolarSystem #Earth #Aurora #AuroraAustralis #Science #CitizenScience #Astrophotographer #TrevorDobson #Astrophotography #StirlingDam #WesternAustralia #Australia #STEM #Education

Spiral Galaxy UGC 3912: A Suspected Galactic Encounter | Hubble

Spiral Galaxy UGC 3912: A Suspected Galactic Encounter | Hubble

This Hubble Space Telescope image is of the spiral galaxy UGC 3912, located approximately 60–63 million light-years away in the constellation Canis Minor. It is classified as a spiral galaxy. However, UGC 3912’s distorted shape typically indicates a gravitational encounter with another galaxy. When galaxies interact—brushing up against each other’s gravitational fields or even collide— their stars, dust, and gas can be pulled into new paths. UGC 3912 may have been an organized-looking spiral once, but it looks like it has been smudged out of shape.

Fortunately, when galaxies interact, the individual stars and objects that orbit them remain whole even though their orbits can change so dramatically that the entire galaxy’s shape is altered. This is because the distances between stars in galaxies are so vast that they do not crash into one another, just continue serenely along their new orbits.

Astronomers have been studying UGC 3912 as part of an investigation into supernovae activity—when stars at least eight times larger than our Sun explode at the end of their lives. Hubble is examining one of the several types of supernovae, a hydrogen-rich phenomenon known as Type II. Though ample Type II supernovae have been observed, they exhibit enormous diversity in their brightness and spectroscopy and are not well understood.

Image Description: "A scattered grouping of blue and violet stars shines near the lower half of the image. Distant galaxies fill the black background of space, and bright stars with diffraction spikes are visible throughout."

The Hubble Space Telescope is a partnership between the European Space Agency (ESA) and NASA.


Image Credit: NASA, ESA, and C. Kilpatrick (Northwestern University); Processing: Gladys Kober (NASA/Catholic University of America)
Release Date: Feb. 1, 2024

#NASA #ESA #Astronomy #Space #Science #Galaxies #UGC3912 #IRAS073150439 #CanisMinorConstellation #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education

Sunday, March 01, 2026

Aurora at Dawn | International Space Station

Aurora at Dawn | International Space Station

NASA astronaut and former International Space Station flight engineer Don Pettit shared this photo. Don Pettit returned to Earth on April 19, 2025, concluding a seven-month science mission aboard the International Space Station. Pettit spent 220 days in space, earning him a total of 590 days in space over the course of his four spaceflights. He orbited the Earth 3,520 times, traveling 93.3 million miles in low-Earth orbit.

Also known as the northern lights (aurora borealis) or southern lights (aurora australis), 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: 

Follow Expedition 74:

Expedition 74 Crew
Station Commander: Mike Fincke (NASA)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Oleg Platonov, Sergey-Kud Sverchkov, Sergei Mikaev
NASA Flight Engineers: Zena Cardman, Chris Williams

Image Credit: NASA's Johnson Space Center/D. Pettit
Release Date: March 1, 2026

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