Monday, June 15, 2026

Journey to Galaxy NGC 3256 in Vela | Hubble Space Telescope

Journey to Galaxy NGC 3256 in Vela | Hubble Space Telescope

This video zooms in on the spiral galaxy NGC 3256, about 100 million light-years away. It starts with a view of the night sky focused on the constellation of Vela (The Sails), as seen from the ground. It then zooms through observations from the Digitized Sky Survey 2, and ends with a view of the galaxy obtained with the NASA/European Space Agency Hubble Space Telescope.

NGC 3256 is an impressive example of a peculiar galaxy that is actually the relict of a collision of two separate galaxies that took place in a distant past. The telltale signs of the collision are two extended luminous tails swirling out from the galaxy. NGC 3256 belongs to the Hydra-Centaurus supercluster complex and provides a nearby template for studying the properties of young star clusters in tidal tails. The system hides a double nucleus and a tangle of dust lanes in the central region. The tails are studded with a particularly high density of star clusters.

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: ESA/Hubble, NASA, Digitized Sky Survey 2 
Acknowledgement: Davide De Martin
Duration: 50 seconds
Release Date: May 31, 2018

#NASA #Astronomy #Space #Science #Galaxies #NGC3256 #VV65 #InteractingGalaxies #StarburstGalaxies #HydraCentaurusSupercluster #VelaConstellation #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #DSS2 #UnitedStates #Europe #STEM #Education #HD #Video

Close-up: Galaxy NGC 3256 in Vela | Hubble Space Telescope

Close-up: Galaxy NGC 3256 in Vela | Hubble Space Telescope

This video pans over NASA/European Space Agency Hubble Space Telescope observations of the starburst galaxy NGC 3256, located about 100 million light-years from Earth. The galaxy is the result of a merger between galaxies with similar masses. Although the collision is estimated to have happened 500 million years ago, the galaxy still bears the marks of this event: luminous tails of gas and dust surround the galaxy and in its center, new stars are born at a rapid rate.

NGC 3256 is an impressive example of a peculiar galaxy that is actually the relict of a collision of two separate galaxies that took place in a distant past. The telltale signs of the collision are two extended luminous tails swirling out from the galaxy. NGC 3256 belongs to the Hydra-Centaurus supercluster complex and provides a nearby template for studying the properties of young star clusters in tidal tails. The system hides a double nucleus and a tangle of dust lanes in the central region. The tails are studded with a particularly high density of star clusters.


Credit: ESA/Hubble; Risinger/Digitized Sky Survey 2
Duration: 25 seconds
Release Date: May 31, 2018

#NASA #Astronomy #Space #Science #Galaxies #NGC3256 #VV65 #InteractingGalaxies #StarburstGalaxies #HydraCentaurusSupercluster #VelaConstellation #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #DSS2 #UnitedStates #Europe #STEM #Education #HD #Video

Galaxy NGC 3256 in Vela | Hubble Space Telescope

Galaxy NGC 3256 in Vela | Hubble Space Telescope

NGC 3256 is an impressive example of a peculiar galaxy that is actually the relict of a collision of two separate galaxies that took place in a distant past. The telltale signs of the collision are two extended luminous tails swirling out from the galaxy. NGC 3256 belongs to the Hydra-Centaurus supercluster complex and provides a nearby template for studying the properties of young star clusters in tidal tails. The system hides a double nucleus and a tangle of dust lanes in the central region. The tails are studded with a particularly high density of star clusters.

Distance from Earth: ~100 million light years


Credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)
Release Date: April 24, 2008

#NASA #Astronomy #Space #Science #Galaxies #NGC3256 #VV65 #InteractingGalaxies #StarburstGalaxies #HydraCentaurusSupercluster #VelaConstellation #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Sunday, June 14, 2026

Wide-field view: Star-forming Region Gum 19 in Vela | Digitized Sky Survey 2

Wide-field view: Star-forming Region Gum 19 in Vela Digitized Sky Survey 2

This image shows the area around the star-forming region Gum 19 (also known as RCW 34), in the direction of the constellation of Vela (The Sails), as seen by the Digitized Sky Survey 2. The image covers an area of 3 by 3 degrees on the sky. Gum 19 is approximately 22,000 light years from Earth. 

The furnace that fuels Gum 19’s luminosity is a gigantic, superhot star called V391 Velorum. Shining brightest in the scorching blue range of visible light—V391 Velorum boasts a surface temperature in the vicinity of 30,000 degrees Celsius. Within the neighborhood of this fitful supergiant, new stars nonetheless continue to grow. In several million years—a blink of an eye in cosmic time—they will eventually reach the high density at their centers necessary to ignite nuclear fusion. The fresh outpouring of energy and stellar winds from these newborn stars will also modify the gaseous landscape of Gum 19.

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: European Southern Observatory (ESO)/Digitized Sky Survey 2
Release Date: March 31, 2010


#NASA #ESO #Astronomy #Space #Science #Stars #V391Velorum #Nebulae #Gum19 #RCW34 #StellarNurseries #HIIRegion #EmissionNebulae #VelaConstellation #MilkyWayGalaxy #Cosmos #Universe #NTT #InfraredAstronomy #LaSillaObservatory #Chile #Europe #DSS2 #STScI #UnitedStates #STEM #Education

Journey to Star-forming Region Gum 19 in Vela | New Technology Telescope

Journey to Star-forming Region Gum 19 in Vela | New Technology Telescope

This video zooms in onto the star-forming region Gum 19, located towards the constellation of Vela (the Sail). The final image of the Gum 19 star-forming region was obtained with SOFI, an infrared instrument mounted on the European Southern Observatory's New Technology Telescope (NTT) that operates at the La Silla Observatory in Chile. Gum 19 is located in the direction of the constellation Vela (the Sail) at a distance of approximately 22,000 light years. 

The furnace that fuels Gum 19’s luminosity is a gigantic, superhot star called V391 Velorum. Shining brightest in the scorching blue range of visible light—V391 Velorum boasts a surface temperature in the vicinity of 30,000 degrees Celsius. Within the neighborhood of this fitful supergiant, new stars nonetheless continue to grow. In several million years—a blink of an eye in cosmic time—they will eventually reach the high density at their centers necessary to ignite nuclear fusion. The fresh outpouring of energy and stellar winds from these newborn stars will also modify the gaseous landscape of Gum 19.

The image is based on data obtained in three near-infrared bands (J, H, K; associated respectively to blue, green, and red). The image is 4.7 arcminutes across.


Credit: European Southern Observatory (ESO)/Digitized Sky Survey 2/A. Fujii
Duration: 1 minute
Release Date: March 31, 2010


#NASA #ESO #Astronomy #Space #Science #Stars #V391Velorum #Nebulae #Gum19 #RCW34 #StellarNurseries #HIIRegion #EmissionNebulae #VelaConstellation #MilkyWayGalaxy #Cosmos #Universe #NTT #InfraredAstronomy #LaSillaObservatory #Chile #Europe #STEM #Education #HD #Video

Star-forming Region Gum 19 in Vela (infrared) | New Technology Telescope

Star-forming Region Gum 19 in Vela (infrared) New Technology Telescope

This image of the Gum 19 star-forming region was obtained with SOFI, an infrared instrument mounted on the European Southern Observatory's New Technology Telescope (NTT) that operates at the La Silla Observatory in Chile. Gum 19 is located in the direction of the constellation Vela (the Sail) at a distance of approximately 22,000 light years. 

The furnace that fuels Gum 19’s luminosity is a gigantic, superhot star called V391 Velorum. Shining brightest in the scorching blue range of visible light—V391 Velorum boasts a surface temperature in the vicinity of 30,000 degrees Celsius. Within the neighborhood of this fitful supergiant, new stars nonetheless continue to grow. In several million years—a blink of an eye in cosmic time—they will eventually reach the high density at their centers necessary to ignite nuclear fusion. The fresh outpouring of energy and stellar winds from these newborn stars will also modify the gaseous landscape of Gum 19.

The image is based on data obtained in three near-infrared bands (J, H, K; associated respectively to blue, green, and red). The image is 4.7 arcminutes across.


Credit: European Southern Observatory (ESO)
Release Date: March 31, 2010


#NASA #ESO #Astronomy #Space #Science #Stars #V391Velorum #Nebulae #Gum19 #RCW34 #StellarNurseries #HIIRegion #EmissionNebulae #VelaConstellation #MilkyWayGalaxy #Cosmos #Universe #NTT #InfraredAstronomy #LaSillaObservatory #Chile #Europe #STEM #Education

Europe-China SMILE Science Mission Tracks Solar Storms around Planet Earth

Europe-China SMILE Science Mission Tracks Solar Storms around Planet Earth

🛰️📡For the first time, we are able to capture a global view of how the solar wind interacts with the Earth’s magnetosphere. How do we track a solar storm for 40 hours? From a highly elliptical orbit above the polar region, SMILE studies where the solar wind meets Earth's magnetic field. This provides a fuller picture of the effects of space weather.

Scientific questions being examined include:
How does the solar wind reshape our magnetic shield?
What triggers auroral substorms?
How do solar eruptions spark geomagnetic storms?

The Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) is an international space science mission designed to investigate how the solar wind interacts with Earth's magnetosphere. By observing these dynamic processes from space, SMILE will help scientists better understand space weather and its effects on our planet's magnetic environment.

The European Space Agency (ESA) was responsible for providing SMILE’s payload module (carrying three of the four science instruments), one of the spacecraft’s four science instruments (the soft X-ray imager, SXI), the launcher, and the Assembly Integration and Testing facilities and services. ESA contributed to a second science instrument (the ultraviolet imager, UVI) and the mission operations once SMILE is in orbit.

The Chinese Academy of Sciences provided the other three science instruments and the spacecraft platform, and is responsible for operating the spacecraft in orbit.


Video Credit: Chinese Academy of Sciences (CAS)
Duration: 1 minute, 35 seconds
Date: June 12, 2026

#NASA #Space #Astronomy #Science #Stars #Sun #Earth #SpaceWeather #SolarWind #MagneticField #Magnetosphere #Aurorae #Europe #ESA #China #中国 #CAS #中国科学院 #SMILEMission #Heliophysics #Physics #InternationalCooperation #STEM #Education #HD #Video

Mammatus Clouds over Sicily | Earth Science

Mammatus Clouds over Sicily | Earth Science

Photographer Giuseppe Pappa: "A spectacular display of mammatus clouds (Cumulonimbus mammatus) captured this afternoon over Pedara, a village located on the southern slopes of Mount Etna in Sicily, Italy. These bulbous, pouch-like structures formed at the base of a severe thunderstorm cell, creating an ominous yet mesmerizing sky. Mammatus clouds typically occur when cold, saturated downdrafts sink rapidly into warmer, drier air beneath the storm's anvil, causing ice crystals to sublimate and produce these smooth, pocketed shapes."

Mammatus clouds are actually altocumulus, cirrus, cumulonimbus, or other types of clouds that have these pouch-like shapes hanging out of the bottom. The pouches are created when cold air within the cloud sinks down toward the Earth. They can indicate a risk of severe weather.


Image Credit: Giuseppe Pappa
Location: Pedara, Sicily, Italy
Image Details: Camera—Canon EOS 760D; Lens: 17-50mm
Location: Pedara, Catania (Sicily, Italy)
Release Date: June 11, 2026

#NASA #Science #Planets #Earth #Atmospheres #Weather #Meteorology #Clouds #MammatusClouds #Pedara #Sicily #Italy #Italia #Photography #CitizenScience #Photographers #STEM #Education

Elliptical Galaxy Messier 49 in Virgo: 200 Billion Stars Plus | Hubble

Elliptical Galaxy Messier 49 in Virgo: 200 Billion Stars Plus | Hubble


This fuzzy orb of light is a giant elliptical galaxy filled with an incredible 200 billion stars. Unlike spiral galaxies that have a well-defined structure and boast picturesque spiral arms, elliptical galaxies appear fairly smooth and featureless. This is likely why this galaxy, named Messier 49, was discovered by French astronomer Charles Messier in 1771. At a distance of 56 million light-years, and measuring 157,000 light-years across, M49 was the first member of the Virgo Cluster of galaxies to be discovered, and it is more luminous than any other galaxy at its distance or nearer.

Elliptical galaxies tend to contain a larger portion of older stars than spiral galaxies and also lack young blue stars. Messier 49 itself is very yellow. This indicates that the stars within it are mostly older and redder than the Sun. In fact, the last major episode of star formation was about six billion years ago—before the Sun was even born!

Messier 49 is also rich in globular clusters; it hosts about 6,000, a number that dwarfs the 150 found in and around the Milky Way. On average, these clusters are 10 billion years old. Messier 49 is also known to host a supermassive black hole at its center with the mass of more than 500 million Suns, identifiable by the x-rays pouring out from the heart of the galaxy (as this Hubble image comprises infrared observations, these x-rays are not visible here).


Credit: ESA/Hubble & NASA, J. Blakenslee, P Cote et al.
Release Date: March 18, 2019

#NASA #Astronomy #Space #Science #Galaxies #Messier49 #M49 #EllipticalGalaxies #VirgoConstellation #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Saturday, June 13, 2026

Meet the Earth “Space Eye” Detecting Climate Heating Gases | China Space Station

Meet the Earth “Space Eye” Detecting Climate Heating Gases | China Space Station

🌍🚀 The Multi-Spectral Imaging Carbon Observatory (MUSICO), also known as the Tianyun Camera, was launched aboard the Tianzhou-10 cargo spacecraft last month. Designed to detect carbon dioxide (CO₂) and methane (CH₄) emissions from orbit, MUSICO provides high-resolution monitoring of greenhouse gases across low- and mid-latitude regions worldwide, helping to pinpoint major emission sources. It was jointly developed by the Hong Kong University of Science and Technology, in collaboration with the Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences.

It represents a new step forward for space-based climate science.


Video Credit: Chinese Academy of Sciences (CAS)
Duration: 25 seconds
Date: June 12, 2026

#NASA #Space #Science #Planets #Earth #Atmospheres #Climate #ClimateChange #MUSICO #GreenhouseGases #China #中国 #Taikonauts #Astronauts #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #SpaceLaboratory #SpaceResearch #CAS #HKUST #CMSA #HumanSpaceflight #EarthObservation #RemoteSensing #STEM #Education #HD #Video

Send Your Name to Space with NASA's Nancy Grace Roman Space Telescope

Send Your Name to Space with NASA's Nancy Grace Roman Space Telescope






You can send your name along with NASA's Nancy Grace Roman Space Telescope that will be placed a million miles away for planet Earth. It is currently scheduled to launch on August 30, 2026. 

Sign up here: https://go.nasa.gov/4ejkRcR 

Submissions close July 12.

Submitted names will be uploaded to a Secure Digital (SD) card attached to the observatory. Stay tuned for the latest mission updates, including information about launch, at nasa.gov/roman.

Plus, download a free Nancy Grace Roman Space Telescope poster here: 



Named after NASA’s first chief astronomer, the ‘mother of the Hubble Space Telescope,’ the Nancy Grace Roman Space Telescope will have a field of view at least 100 times larger than Hubble's, potentially measuring light from a billion galaxies in its lifetime. This observatory will also be able to block starlight to directly see exoplanets and planet-forming disks, complete a statistical census of planetary systems in our galaxy, and address key questions in the areas of dark energy, exoplanets, and infrared astrophysics. The Nancy Grace Roman Space Telescope is scheduled to launch no earlier than September 2026.

The Roman telescope and the discoveries it will enable: 
https://www.stsci.edu/roman

Learn more about Dr. Nancy Grace Roman: 
https://science.nasa.gov/people/nancy-roman/

Image Credits: NASA's Goddard Space Flight Center
Release Date: June 12, 2026

#NASA #Space #Astronomy #Science #NASARoman #RomanSpaceTelescope #NancyGraceRomanSpaceTelescope #Posters #FreeDownload #NancyGraceRoman #Exoplanets #Planets #SolarSystem #Stars #MilkyWayGalaxy #Galaxies #Cosmos #Universe #SpaceTelescopes #NASAGoddard #GSFC #STScI #UnitedStates #Infographics #STEM #Education

Distant & Ancient Galaxy Cluster SPT0615 in Pictor | Hubble Space Telescope

Distant & Ancient Galaxy Cluster SPT0615 in Pictor | Hubble Space Telescope


Dotted across the sky in the constellation of Pictor (The Painter’s Easel) is the galaxy cluster highlighted here by the NASA/European Space Agency Hubble Space Telescope: SPT-CL J0615-5746, or SPT0615 for short. First discovered by the South Pole Telescope less than a decade ago, SPT0615 is exceptional among the myriad clusters so far cataloged in our map of the Universe—it is among the highest-redshift clusters that has a full, strong lens model published.

SPT0615 is a massive cluster of galaxies, one of the farthest observed to cause gravitational lensing. Gravitational lensing occurs when light from a background object is deflected around mass between the object and the observer. Among the identified background objects, there is SPT0615-JD (highlighted in the second image's inset), a galaxy that is thought to have emerged just 500 million years after the Big Bang. This puts it among the very earliest structures to form in the Universe. It is also the farthest galaxy ever imaged by means of gravitational lensing. Though a few other primitive galaxies have been seen at this early epoch, they have essentially all looked like red dots, given their small size and tremendous distances.

Image analysis shows that the galaxy weighs in at no more than 3 billion solar masses (roughly 1/100th the mass of our Milky Way galaxy). It is less than 2500 light-years across, half the size of the Small Magellanic Cloud (SMC), a satellite galaxy of the Milky Way. The object is considered prototypical of young galaxies that emerged during the epoch shortly after the Big Bang.

Just as ancient paintings can tell us about the period of history when they were painted, so too can ancient galaxies tell us about the era of the Universe when they existed. To learn about cosmological history, astronomers explore the most distant reaches of the Universe, probing ever further out into the cosmos. The light from distant objects travels to us from so far away that it takes an immensely long time to reach us, meaning that it carries information from the past—information about the time when it was emitted.

By studying such distant objects, astronomers are continuing to fill the gaps in our picture of what the very early Universe looked like, and uncover more about how it evolved into its current state.


Image Credits: ESA/Hubble & NASA, I. Karachentsev et al., F. High et al., and B. Salmon (STScI)
Release Dates: May 6, 2019 (image 1), January 12, 2018 (image 2)


#NASA #ESA #Astronomy #Space #Science #Galaxies #SPT0615JD #GalaxyClusters #SPTCLJ06155746 #PictorConstellation #GravitationalLensing #Astrophysics #Cosmology #Cosmos #EarlyUniverse #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education

The Cat's Eye Galaxy: Messier 94 in Canes Venatici | Kitt Peak National Observatory

The Cat's Eye Galaxy: Messier 94 in Canes Venatici | Kitt Peak National Observatory


Messier 94 (also known as NGC 4736, Cat's Eye Galaxy, Crocodile Eye Galaxy, or Croc's Eye Galaxy) is a spiral galaxy in the mid-northern constellation Canes Venatici. It was discovered by Pierre Méchain in 1781, and cataloged by Charles Messier two days later. 

Spiral galaxy M94 in the constellation Canes Venatici has been considered to be in a group including M64 and other fainter galaxies. It has an extremely bright innner region surrounded by a blue ring of young star clusters, then a fainter yellowish region of older stars also surrounded by traces of young stars, and even further out a very much fainter outer ring. All of these features are visible in this picture, due to the use of a drastically compressed intensity mapping. This stretch also reveals quite a few small faint background galaxies. This picture was taken in May 1998 at the KPNO 0.9-meter telescope. Image size 17.0 arc minutes.


Credit: Hillary Mathis, N.A.Sharp/NOIRLab/NSF/AURA/
Release Date: Dec. 16, 2002


#NASA #Astronomy #Space #Science #Galaxies #Messier94 #M94 #NGC4736 #SpiralGalaxies #StarburstGalaxies #StarburstRings #DoubleRingGalaxies #CanesVenaticiConstellation #Cosmos #Universe #KPNO #KittPeakNationalObservatory #Arizona #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

Planets, Stars and Clouds: View from Italy

Planets, Stars and Clouds: View from Italy

Astrophotographer Paolo Bardelli: "Fantastic evening. A cluster of lenticular altocumulus clouds in front of this evening's parade of planets with the colors of the sunset."

Castor is the second-brightest object in the zodiac constellation of Gemini. With an apparent visual magnitude of 1.58, it is one of the brightest stars in the night sky. Castor appears singular to the naked eye, but it is actually a sextuple star system organized into three binary pairs.

Pollux is the brightest star in the constellation of Gemini. This is an orange-hued, evolved red giant located at a distance of 34 light-years, making it the closest red giant (and giant star) to the Sun. In 2006, an exoplanet (designated Pollux b or β Geminorum b, later named Thestias) was announced to be orbiting it.


Image Credit: Paolo Bardelli
Location: Sumirago (Varese), Italy
Image Details: Canon 6D + 50mm lens
Date: June 12, 2026

#NASA #Space #Astronomy #Science #Stars #Sun #Pollux #Castor #SolarSystem #Planets #Earth #Atmosphere #Clouds #LenticularAltocumulusClouds #Mercury #Venus #Jupiter #PlanetaryConjunctions #Astrophotography #Astrophotographers #PaoloBardelli #CitizenScience #Sumirago #Varese #Italy #Italy #STEM #Education

Friday, June 12, 2026

Japan H3 Rocket No. 6 Satellite Launch | Tanegashima Space Center

Japan H3 Rocket No. 6 Satellite Launch | Tanegashima Space Center

🚀H3 Rocket No. 6 was successfully launched from Tanegashima Space Center in southwestern Japan at 9:53:59 a.m. on June 12, 2026. This was the debut of the H3-30 configuration: three LE-9 engines and no strap-on solid rocket boosters (SRBs). Onboard was a test satellite for flight data verification, plus six university/organization microsatellites. The Japan Aerospace Exploration Agency (JAXA) says the model is lighter and less expensive than other H3 types. It is the country's first rocket launch powered solely by liquid-fuel engines.

The H3 is a Japanese medium-lift launch vehicle developed by JAXA and Mitsubishi Heavy Industries (MHI). A hydrolox-fuelled rocket, it is the successor to the H-IIA and H-IIB launch vehicles. The H3 uses the LE-9 main engine, which was designed to be less expensive to produce as part of a broader effort to lower launch costs. The rocket has a modular design. Its first stage is powered by two or three LE-9 engines and can be fitted with zero, two, or four SRB-3 solid rocket boosters. The second stage uses the LE-5B-3 engine, an upgraded version of the engine family used since the H-I rocket.

In addition to launching satellites into Earth orbit, the H3 is used to launch Japan's HTV-X cargo spacecraft to the International Space Station.


Video Credit: JAXA
Duration: 53 seconds
Date: June 12, 2026


#NASA #Space #Satellites #H3RocketNo6 #MitsubishiHeavyIndustries #三菱重工業株式会社 #Japan #日本 #KagoshimaPrefecture #TanegashimaSpaceCenter #種子島宇宙センター #JAXA #宇宙航空研究開発機構 #STEM #Education #HD #Video

NASA Artemis II Crew View Solar Eclipse on Lunar Flyby

NASA Artemis II Crew View Solar Eclipse on Lunar Flyby

During their lunar flyby, the Artemis II crew enjoyed the rare opportunity to experience a solar eclipse from their Orion spacecraft. With the Sun hidden behind the Moon, the astronauts were able to capture views of the Sun’s outermost atmosphere, also known as the solar corona.

The first crewed test flight of NASA’s Artemis Program lifted off from Launch Pad 39B at the agency’s Kennedy Space Center in Florida on April 1, 2026, carrying the first astronauts to travel to the Moon in more than half a century. 

During their nearly 10-day mission, the crew completed a record-setting lunar flyby, taking them 252,756 miles at their farthest distance from Earth and 4,067 miles above the lunar surface at their closest approach. 

Artemis II splashed down on April 10 in the Pacific Ocean off the coast of San Diego. 

Under Artemis, NASA will send astronauts on increasingly difficult missions to explore more of the Moon for scientific discovery, economic benefits, and to build on our foundation for the first crewed missions to Mars.

Learn more about NASA's Artemis II Mission:
https://www.nasa.gov/mission/artemis-ii/


Video Credit: NASA
Duration: 2 minutes, 50 seconds
Capture Date: April 7, 2026

#NASA #Space #Science #Earth #Moon #SolarEclipse #ArtemisProgram #ArtemisII #OrionSpacecraft #Astronauts #ReidWiseman #VictorGlover #ChristinaKoch #JeremyHansen #CSA #Canada #HumanSpaceflight #SolarSystem #SpaceExploration #UnitedStates #STEM #Education #HD #Video