Friday, November 21, 2025

Planting an Artemis I Moon Tree | NASA Goddard

Planting an Artemis I Moon Tree | NASA Goddard

On Nov. 16, 2022, NASA launched the Artemis I test flight, sending an uncrewed Orion capsule beyond the Moon and back. On board were seeds from five species of trees, to be planted after returning to Earth. On Nov. 7, 2024, a seedling from the Artemis I flight was planted at the NASA Goddard Visitor Center by Artemis I Mission Manager Mike Sarafin, Artemis II Camera Lead Marie Henderson, Artemis III Project Scientist Noah Petro, Artemis IV Project Scientist Barbara Cohen, and others. In commemorating the event, Dr. Petro noted that planting a seedling is, like space exploration, an act of hope intended to bring fruit to future generations.

Learn more: https://www.nasa.gov/learning-resources/nasa-stem-artemis-moon-trees/


Credit: NASA’s Goddard Space Flight Center
Dan Gallagher: Producer/Editor
Noah Petro: Scientist
John D. Philyaw: Videographer
Lonnie Shekhtman: Public Affairs
Caela Barry: Support
Staci Horvath: Support
Kathryn Mersmann: Support
Derrol Nail: Launch Commentator
Aaron E. Lepsch: Technical Support
Duration: 1 minute, 33 seconds
Release Date: Nov. 20, 2025

#NASA #Space #Science #Moon #ArtemisProgram #ArtemisI #OrionSpacecraft #TreeSeeds #NASASLS #SpaceLaunchSystem #DeepSpace #MoonToMars #SpaceEngineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NASAGoddard #GSFC #Greenbelt #Maryland #UnitedStates #STEM #Education #HD #Video

Celestial Lightsabers: Stellar Jets in Herbig-Haro Object 24 | Hubble Visualization

Celestial Lightsabers: Stellar Jets in Herbig-Haro Object 24 Hubble Visualization

This sequence combines a two-dimensional zoom and a three-dimensional flight to explore Hubble’s striking image of the Herbig-Haro object known as HH24. This video starts with a night sky view of the Orion constellation and zooms in. Located above the left side of Orion’s Belt is the vast dark nebula called the Orion B molecular cloud complex. Within this molecular cloud are many bright regions where stars are forming. This video closes in toward one particularly energetic example.

The video then switches to an envisioned three-dimensional perspective. As the virtual camera flies into the dark nebula, the stars pass off-screen and the details of the forming stars and their jets of emission are revealed. The central star is hidden by gas and dust, but its prominent twin jets of emission resemble a cosmic, double-bladed lightsaber. These jets have carved an hourglass-shaped cavity in the near side of the nebula. The jet from another stellar newborn in this region has created a cylindrical tunnel through the gas extending to the left. Careful study of the Hubble data reveals a few other jets heating and displacing the gas and dust around them. The nebula provides a vivid example of a gas cloud shaped by stellar emission.


Credit: NASA, ESA, G. Bacon, L. Frattare, Z. Levay, and F. Summers (Viz3D Team, STScI)
Acknowledgment: NASA, ESA, A. Fujii, Digitized Sky Survey (DSS), STScI/AURA, Palomar/Caltech, UKSTU/AAO, T. Rector/University of Alaska Anchorage, H. Schweiker/WIYN and NOAO/AURA/NSF, Gemini Observatory/AURA/B. Reipurth, C. Aspin, and T. Rector, the Hubble Heritage (STScI/AURA)/Hubble-Europe (ESA) Collaboration, D. Padgett (GSFC), T. Megeath (University of Toledo), and B. Reipurth (University of Hawaii)
Duration: 1 minute
Release Date: Nov. 20, 2025

#NASA #ESA #Hubble #Astronomy #Space #Science #Star #Gas #Jets #HerbigHaroObjects #HH24 #Orion #Constellations #MilkyWayGalaxy #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education #3D #Visualization #HD #Video

Thursday, November 20, 2025

Blue Origin New Glenn-2 Rocket & Reusable Booster: New Pictures

Blue Origin New Glenn-2 Rocket & Reusable Booster: New Pictures









On November 18, 2025, Blue Origin welcomed Jacklyn and its fully reusable New Glenn first stage back to the Space Coast.

A Blue Origin New Glenn-2 rocket successfully launched NASA's ESCAPADE Mars Mission on November 13, 2025. This was the second mission to date for the New Glenn rocket series. Blue Origin also landed its fully reusable New Glenn first stage booster on the drone ship Jacklyn in the Atlantic Ocean. 

The NASA Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) Mars Mission will study the planet's unique hybrid magnetosphere. ESCAPADE will investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. It will take ESCAPADE about 11 months to arrive at Mars after leaving Earth orbit.

ESCAPADE is led by the UC Berkeley Space Sciences Laboratory. It is responsible for mission management, systems engineering, science leadership, navigation, operations, the electron and ion electrostatic analyzers, plus science data processing and archiving.

Key partners are Rocket Lab USA (spacecraft), NASA Goddard Space Flight Center (magnetometers), Embry Riddle Aeronautical University (Langmuir probes), Advanced Space LLC (mission design), and Blue Origin (launch).

Learn more about the two identical spacecraft designed, built, integrated, and tested by Rocket Lab for the University of California Berkeley’s Space Science Laboratory and NASA's Mars Mission:
https://escapade.ssl.berkeley.edu

🚀Blue Origin's New Glenn Rocket:

The twin spacecraft for NASA's ESCAPADE Mars Mission were manufactured by Rocket Lab:

Image Credit: Blue Origin
Release Dates: Nov. 15-20, 2025


#NASA #Space #Astronomy #Science #Stars #Sun #SpaceWeather #Planets #Mars #Magnetosphere #MartianAtmosphere #ESCAPADEMission #ESCAPADESpacecraft #SolarSystem #SpaceExploration #GSFC #SSL #UCBerkeley #ERAU #AdvancedSpace #BlueOrigin #NewGlennRocket #NewGlenn2 #Florida #UnitedStates #Infographics #STEM #Education

"Movie Night" | International Space Station

"Movie Night" | International Space Station



Expedition 73 Flight Engineer and NASA Astronaut Jonny Kim: "We work hard on the International Space Station, but we also like to relax together. Sometimes we do movie nights in space."


Expedition 73 Crew
Station Commander: Sergey Ryzhikov (Roscosmos)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Alexey Zubritskiy, Oleg Platonov
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.


Image Credit: NASA/JSC/Jonny Kim
Release Date: Nov. 18, 2025


#NASA #Space #Astronomy #Science #Earth #ISS #MovieNights #Films #Entertainment #Astronauts #JonnyKim #AstronautPhotography #UnitedStates #Japan #日本 #JAXA #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education

NASA's Artemis II Moon Rocket Fully Integrated | Kennedy Space Center

NASA's Artemis II Moon Rocket Fully Integrated | Kennedy Space Center

NASA’s Artemis II Orion crew spacecraft with its launch abort system was recently stacked atop the agency’s Space Launch System (SLS) rocket in High Bay 3 of the Vehicle Assembly Building (VAB) at NASA's Kennedy Space Center (KSC) in Florida. This milestone marks a huge step in the mission that will carry four astronauts on a 10-day mission around the Moon and back in early 2026. 

Ahead of rolling out the integrated SLS rocket to the launch pad, teams will be conducting a series of verification tests. 

Artemis II will officially launch "no earlier than April 2026."

Check the NASA Artemis II Mission page for updates:

Learn more about NASA's Space Launch System (SLS) rocket: nasa.gov/sls

Follow updates on the Artemis blog: 

Image Credit: NASA
Duration: 1 minute, 15 seconds
Release Date: Nov. 20, 2025


#NASA #Space #Science #Earth #Moon #Artemis #ArtemisII #OrionSpacecraft #SLS #SLSRocket #CrewedMissions #DeepSpace #MoonToMars #Engineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NASAKennedy #KSC #LockheedMartin #Florida #UnitedStates #STEM #Education #HD #Video

The Apep Wolf-Rayet Binary Star System | Webb Visualization | STScI

The Apep Wolf-Rayet Binary Star System | Webb Visualization | STScI

This scientific visualization models what three of the four dust shells sent out by two Wolf-Rayet stars in the Apep system look like in 3D based on mid-infrared observations from NASA’s James Webb Space Telescope. Apep is made up of two Wolf-Rayet binary stars that are orbiting together with a third supergiant star. For 25 years during every 190-year orbit, the Wolf-Rayet stars’ winds collide, producing and sending out new waves of amorphous carbon dust. The width of the widest bubble is at least 4.6 light-years across. 

Wolf-Rayet stars can be around 20 times as massive as our sun, but seem to be on a mission to shed surplus mass as quickly as possible—they blast substantial winds of particles out into space, causing them to dwindle at a rapid rate. A typical star of this type can lose a mass equal to that of our sun in just 100,000 years!

These massive stars are also incredibly hot, with surface temperatures some 10 to 40 times that of the sun, and very luminous, glowing at tens of thousands to several million times the brightness of the sun. Many of the brightest and most massive stars in the Milky Way are Wolf-Rayet stars.

Because these stars are so intense they do not last very long, burning up their fuel and blasting their bulk out into the cosmos on very short timescale—only a few hundred thousand years. 


Credits: Space Telescope Science Institute (STScI), NASA, European Space Agency, Canadian Space Agency 
Simulation: Yinuo Han (CALTECH), Ryan White (Macquarie University)
Image Processing: Alyssa Pagan (STScI)
Visualization: Christian Nieves (STScI)
Duration: 41 seconds
Release Date: Nov. 19, 2025

#NASA #Astronomy #Space #Science #NASAWebb #Nebula #ApepNebula #BinaryStarSystems #Norma #Constellations #Astrophysics #Cosmos #Universe #UnfoldTheUniverse #JWST #NIRCam #InfraredAstronomy #ESA #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education #Visualization  #HD #Video

New View: A Pair of Wolf-Rayet Stars Named Apep | James Webb Space Telescope

New View: A Pair of Wolf-Rayet Stars Named Apep | James Webb Space Telescope

This new NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope’s mid-infrared image shows four coiled shells of dust around a pair of Wolf-Rayet stars known as Apep for the first time. Previous observations by other telescopes showed only one.

Webb’s data, combined with observations from the European Southern Observatory’s Very Large Telescope (VLT) in Chile, confirmed that the two Wolf-Rayet stars sail past one another approximately every 190 years. Over each orbit, they make a close pass for 25 years, producing and spewing amorphous carbon dust.

Wolf-Rayet stars can be around 20 times as massive as our sun, but seem to be on a mission to shed surplus mass as quickly as possible—they blast substantial winds of particles out into space, causing them to dwindle at a rapid rate. A typical star of this type can lose a mass equal to that of our sun in just 100,000 years!

These massive stars are also incredibly hot, with surface temperatures some 10 to 40 times that of the sun, and very luminous, glowing at tens of thousands to several million times the brightness of the sun. Many of the brightest and most massive stars in the Milky Way are Wolf-Rayet stars.

Because these stars are so intense they do not last very long, burning up their fuel and blasting their bulk out into the cosmos on very short timescale—only a few hundred thousand years. 

Webb’s new data also confirmed that there are three stars gravitationally bound to one another in this system. Holes are “sliced” into these shells by the third star, a massive supergiant.

Image description: Four dust shells in Wolf-Rayet Apep expand away from three central stars that appear as a single pinpoint of light. The shells are curved, and the interior shell looks like a backward lowercase e shape.


Credit: NASA, ESA, CSA, STScI, Y. Han (Caltech), R. White (Macquarie University), A. Pagan (STScI)
Release Date: Nov. 19, 2025


#NASA #Astronomy #Space #Science #NASAWebb #Nebula #ApepNebula #BinaryStarSystems #Norma #Constellations #Astrophysics #Cosmos #Universe #UnfoldTheUniverse #JWST #NIRCam #InfraredAstronomy #ESA #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education

Wednesday, November 19, 2025

Blue Origin New Glenn-2 Reusable Rocket Booster Arrival Post-launch

Blue Origin New Glenn-2 Reusable Rocket Booster Arrival Post-launch

On November 18, 2025, Blue Origin welcomed Jacklyn and its fully reusable New Glenn first stage back to the Space Coast.

A Blue Origin New Glenn rocket successfully launched NASA's ESCAPADE Mars Mission on November 13, 2025. This was the second mission to date for the New Glenn rocket series. Blue Origin also landed the fully reusable New Glenn first stage booster on the drone ship Jacklyn in the Atlantic Ocean. 

The NASA Escape and Plasma Acceleration and Dynamics Explorers (ESCAPADE) Mars Mission will study the planet's unique hybrid magnetosphere. ESCAPADE will investigate how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape. It will take ESCAPADE about 11 months to arrive at Mars after leaving Earth orbit.

ESCAPADE is led by the UC Berkeley Space Sciences Laboratory. It is responsible for mission management, systems engineering, science leadership, navigation, operations, the electron and ion electrostatic analyzers, plus science data processing and archiving.

Key partners are Rocket Lab USA (spacecraft), NASA Goddard Space Flight Center (magnetometers), Embry Riddle Aeronautical University (Langmuir probes), Advanced Space LLC (mission design), and Blue Origin (launch).

Learn more about the two identical spacecraft designed, built, integrated, and tested by Rocket Lab for the University of California Berkeley’s Space Science Laboratory and NASA's Mars Mission:
https://escapade.ssl.berkeley.edu

🚀Blue Origin's New Glenn Rocket:

The twin spacecraft for NASA's ESCAPADE Mars Mission were manufactured by Rocket Lab:

Video Credit: Blue Origin
Duration: 50 seconds
Release Date: Nov. 19, 2025


#NASA #Space #Astronomy #Science #Stars #Sun #SpaceWeather #Planets #Mars #Magnetosphere #MartianAtmosphere #ESCAPADEMission #ESCAPADESpacecraft #SolarSystem #SpaceExploration #GSFC #SSL #UCBerkeley #ERAU #AdvancedSpace #BlueOrigin #NewGlennRocket #NewGlenn2 #Florida #UnitedStates #STEM #Education #HD #Video

NASA’s X-59 Completes Historic First Flight | Armstrong Flight Research Center

NASA’s X-59 Completes Historic First Flight | Armstrong Flight Research Center

NASA’s X-59 quiet supersonic research aircraft took to the skies for the first time Tuesday, Oct. 28, 2025, departing from Lockheed Martin’s Skunk Works facility in Palmdale, California, and arriving at NASA’s Armstrong Flight Research Center in Edwards, California. The milestone marks a major step for NASA’s Quesst mission and its goal of enabling quiet supersonic flight over land.

The X-59 aircraft builds on decades of supersonic flight research and is the centerpiece of NASA’s Quesst mission. The vast amount of data collected over the years has given designers the tools they needed to craft the shape of the X-59. The goal is to enable the aircraft to fly at supersonic speeds and reduce a loud sonic boom to a quieter “sonic thump.” Follow the X-59 team as they take on the exciting journey of building the X-59 and working toward quiet supersonic flight.

Data gathered during X-59 research flights will be shared with the U.S. and international regulators to inform the establishment of new, data-driven acceptable noise thresholds related to supersonic commercial flight over land.

The X-59’s engine, a modified F414-GE-100, packs 22,000 pounds of thrust. This will enable the X-59 to achieve the desired cruising speed of Mach 1.4 (925 miles per hour) at an altitude of approximately 55,000 feet. It sits in a nontraditional spot–atop the aircraft—to aid in making the X-59 quieter.

The X-59's goal is to help change existing national and international aviation rules that ban commercial supersonic flight over land.

For more information about the X-59 and NASA's Quesst mission, visit www.nasa.gov/quesst


Video Credit: NASA's Armstrong Flight Research Center (AFRC)
Duration: 1 minute, 43 seconds
Release Date: Nov. 19, 2025


#NASA #Aerospace #SupersonicFlight #SupersonicAircraft #X59 #Sonicboom #QuietAviation #Aviation #QuesstMission #CommercialAviation #Science #Physics #Engineering #AerospaceResearch #AeronauticalResearch #FlightTests #LockheedMartin #SkunkWorks #NASAArmstrong #AFRC #Palmdale #Edwards #California #UnitedStates #STEM #Education #HD #Video

Views of Interstellar Comet 3I/ATLAS | NASA Mars Spacecraft: MRO & MAVEN

Views of Interstellar Comet 3I/ATLAS | NASA Mars Spacecraft: MRO & MAVEN

The High Resolution Imaging Science Experiment (HiRISE) camera aboard NASA's Mars Reconnaissance Orbiter (MRO) captured this image of interstellar comet 3I/ATLAS on October 5, 2025. At the time it was imaged, the comet was about 0.2 astronomical units (19 million miles or 30 million kilometers) from the spacecraft. 
An ultraviolet image composite of the hydrogen atoms surrounding comet 3I/ATLAS, the third interstellar object ever detected by astronomers as it passes through our solar system. This image was taken on September 28, 2025—just days before the comet's closest approach to Mars—by an instrument on NASA's MAVEN spacecraft that has been studying Mars since 2014. The instrument, the Imaging Ultraviolet Spectrograph, takes pictures in the ultraviolet part of the spectrum to reveal the chemical composition of objects. The image shows hydrogen emitted from multiple sources: the comet (dim spot on the far left), hydrogen from Mars (bright emission on the right) and hydrogen flowing through our solar system between the planets (dim emission in the middle). Hydrogen emission from the comet is confined to the location of the comet in the sky. This is why it is small and round instead of extended.

NASA is in the middle of an unprecedented solar system-wide observation campaign, turning its spacecraft and space telescopes to follow comet 3I/ATLAS, the third known interstellar object to pass through our solar system. Twelve NASA assets have captured and processed imagery of the comet since it was first discovered on July 1, 2025, and several others will have opportunities to capture more images as the comet continues to pass through our solar system. 

By observing the comet from so many locations, NASA has an opportunity to learn about the ways that 3I/ATLAS differs from our solar system’s home-grown comets and give scientists a new window into how the compositions of other systems may differ from our own.

Observations from Mars
The closest imagery of the comet was taken by NASA’s spacecraft at Mars. Earlier this fall, 3I/ATLAS passed by Mars from a distance of 19 million miles, where it was observed by three NASA spacecraft. The Mars Reconnaissance Orbiter (MRO) captured one of the closest images of the comet, while the Mars Atmosphere and Volatile EvolutioN (MAVEN) orbiter obtained ultraviolet images that will help scientists understand the comet’s make-up. Meanwhile, the Perseverance rover grabbed a faint glimpse from the surface of Mars.

Sun watchers’ view
NASA has heliophysics missions with the unique ability to observe areas of the sky near the Sun. This allowed them to track comet 3I/ATLAS as it passed behind our Sun as seen from Earth, making observations with ground-based telescopes impossible. NASA’s Solar Terrestrial Relations Observatory (STEREO) captured images from Sept. 11 to Oct. 2, 2025, and the European Space Agency (ESA) and NASA mission Solar and Heliospheric Observatory (SOHO) observed the comet from Oct. 15 to 26. Images from NASA’s Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission, launched earlier this year, reveal the comet’s tail during observations from Sept. 20 to Oct. 3.
Despite previously observing and discovering thousands of comets, this is the first time NASA’s heliophysics missions have purposefully observed an object originating in another solar system.

The NASA-funded Asteroid Terrestrial-impact Last Alert System (ATLAS) telescope in Chile discovered 3I/ATLAS on July 1, 2025. Later that month it was viewed by NASA’s Hubble Space Telescope. In August, both NASA’s James Webb Telescope and Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer (SPHEREx) captured imagery. 

Comet 3I/ATLAS will fly closest to Earth about Friday, Dec. 19, 2025, at 170 million miles. This is almost twice the distance between the Earth and Sun. NASA spacecraft will continue to observe the comet as it makes its journey through the solar system, passing the orbit of Jupiter in spring 2026. 

For more information on NASA’s comet 3I/ATLAS observations, visit:
https://go.nasa.gov/3I-ATLAS


Credit: NASA/JPL-Caltech/University of Zrizona
Release Date: Nov. 19, 2025

#NASA #Astronomy #Space #Science #InterstellarComet3IATLAS #InterstellarObjects #Astrobiology #Astrochemistry #Astrogeology #Astrophysics #Planets #Mars #MRO #MAVEN #NASASpacecraft #PlanetarySpacecraft #SolarSystem #Infographics #STEM #Education

Journey to Ua ʻŌhiʻa Lani Nebula (NGC 6823) in Vulpecula | Gemini North Telescope

Journey to Ua ʻŌhiʻa Lani Nebula (NGC 6823) in Vulpecula | Gemini North Telescope

To celebrate 25 years since the completion of the International Gemini Observatory, students in Hawai‘i voted for the Gemini North telescope to image NGC 6820—an emission nebula and open star cluster in the constellation Vulpecula. The image was named Ua ʻŌhiʻa Lani, the Heavenly ʻŌhiʻa Rains, after the traditional Hawaiian story of the ʻŌhiʻa forests. The International Gemini Observatory is partly funded by the U.S. National Science Foundation (NSF) and operated by NSF NOIRLab.

Distance from Earth: ~ 6,000 light years



Credit: International Gemini Observatory/NOIRLab/NSF/AURA
Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF NOIRLab)
Duration: 1 minute
Release Date: Nov. 19, 2025

#NASA #Astronomy #Space #Science #StarClusters #Nebulae #NGC6823 #EmissionNebulae #Vulpecula #Constellations #Cosmos #Universe #GeminiInternationalObservatory #GeminiNorthTelescope #OpticalAstronomy #NOIRLab #AURA #NSF #Maunakea #Hawaii #UnitedStates #STEM #Education #HD #Video

Close-up: Ua ʻŌhiʻa Lani Nebula (NGC 6823) in Vulpecula | Gemini North Telescope

Close-up: Ua ʻŌhiʻa Lani Nebula (NGC 6823) in Vulpecula | Gemini North Telescope

To celebrate 25 years since the completion of the International Gemini Observatory, students in Hawai‘i voted for the Gemini North Telescope to image NGC 6820—a striking emission nebula and open star cluster in the constellation Vulpecula.

Distance from Earth: ~ 6,000 light years

The image was named Ua ʻŌhiʻa Lani, the Heavenly ʻŌhiʻa Rains, after the traditional Hawaiian story of the ʻŌhiʻa forests. The International Gemini Observatory is partly funded by the U.S. National Science Foundation (NSF) and operated by NSF NOIRLab.


Credit: International Gemini Observatory/NOIRLab/NSF/AURA
Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF NOIRLab)
Duration: 30 seconds
Release Date: Nov. 19, 2025

#NASA #Astronomy #Space #Science #StarClusters #Nebulae #NGC6823 #EmissionNebulae #Vulpecula #Constellations #Cosmos #Universe #GeminiInternationalObservatory #GeminiNorthTelescope #OpticalAstronomy #NOIRLab #AURA #NSF #Maunakea #Hawaii #UnitedStates #STEM #Education #HD #Video

Ua ʻŌhiʻa Lani Emission Nebula (NGC 6823) in Vulpecula | Gemini North Telescope

Ua ʻŌhiʻa Lani Emission Nebula (NGC 6823) in Vulpecula | Gemini North Telescope

To celebrate 25 years since the completion of the International Gemini Observatory, students in Hawai‘i voted for the Gemini North Telescope to image NGC 6820—a striking emission nebula and open star cluster in the constellation Vulpecula.

Distance from Earth: ~ 6,000 light years

The image was named Ua ʻŌhiʻa Lani, the Heavenly ʻŌhiʻa Rains, after the traditional Hawaiian story of the ʻŌhiʻa forests. The International Gemini Observatory is partly funded by the U.S. National Science Foundation (NSF) and operated by NSF NOIRLab.


Credit: International Gemini Observatory/NOIRLab/NSF/AURA
Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF NOIRLab)
Release Date: Nov. 19, 2025

#NASA #Astronomy #Space #Science #StarClusters #Nebulae #NGC6823 #EmissionNebulae #Vulpecula #Constellations #Cosmos #Universe #GeminiInternationalObservatory #GeminiNorthTelescope #OpticalAstronomy #NOIRLab #AURA #NSF #Maunakea #Hawaii #UnitedStates #STEM #Education

Close-up: Early Universe View of Galaxy CANUCS-LRD-z8.6 | Webb

Close-up: Early Universe View of Galaxy CANUCS-LRD-z8.6 | Webb


This image shows the location of galaxy CANUCS-LRD-z8.6 in galaxy cluster MACS J1149.5+2223, as seen by the James Webb Space Telescope’s Near-Infrared Camera (NIRCam). CANUCS-LRD-z8.6 is located in the constellation Leo (the Lion), and is seen by Webb just 570 million years after the Big Bang. It is part of a class of small, very distant and strikingly red galaxies called Little Red Dots (LRDs) that have been spotted in increasing numbers by Webb’s surveys of the early Universe. 

With the help of Webb’s Near-Infrared Spectrograph (NIRSpec), researchers have confirmed an actively growing supermassive black hole in CANUCS-LRD-z8.6. Analyzing the galaxy’s spectrum yielded an estimate of the black hole’s mass, revealing it to be unusually large for such an early stage in the Universe, and showed that CANUCS-LRD-z8.6 is compact and has not yet produced many heavy elements (a galaxy at an early stage of its evolution). This combination challenges existing theories about the formation of galaxies and black holes in the early Universe.

Science paper "Extreme properties of a compact and massive accreting black hole host in the first 500 Myr":
https://www.nature.com/articles/s41467-025-65070-x


Credit: ESA/Webb, NASA & CSA, G. Rihtaršič (University of Ljubljana, FMF), R. Tripodi (University of Ljubljana, FMF)
Duration: 30 seconds
Release Date: Nov. 19, 2025

#NASA #Astronomy #Space #Science ##EarlyUniverse #Galaxies #CANUCSLRDz86 #LittleRedDots #LRDs #BlackHoles #Leo #Constellations #Universe #SpaceTelescopes #JWST #NIRCam #InfraredAstronomy #GSFC #STScI #UnitedStates #ESA #Europe #CSA #Canada #STEM #Education #HD #Video

Early Universe Supermassive Black Hole in Galaxy CANUCS-LRD-z8.6 | Webb

Early Universe Supermassive Black Hole in Galaxy CANUCS-LRD-z8.6 | Webb

The left side of this visual shows an image of many glowing galaxies in various shapes and colors, including spiral and elliptical galaxies, on a black background. A small box near the top of this image highlights a small collection of galaxies. This box is pulled out to the right side, showing the same area zoomed in to reveal its details up close. This region shows a small circular red galaxy in the center, which is labelled “CANUCS-LRD-z8.6”.
This image shows a portion of the galaxy cluster MACS J1149.5+2223, as seen by Webb’s Near-Infrared Camera (NIRCam). With Webb’s excellent sensitivity to infrared light and the hours of exposure time combined in this image, distant galaxies (red colours) are brought out of the darkness. Other galaxies glow strongly from the abundance of light they radiate.

The first image shows the location of galaxy CANUCS-LRD-z8.6 in galaxy cluster MACS J1149.5+2223, as seen by the James Webb Space Telescope’s Near-Infrared Camera (NIRCam). CANUCS-LRD-z8.6 is part of a class of small, very distant and strikingly red galaxies called Little Red Dots (LRDs), which have been spotted in increasing numbers by Webb’s surveys of the early Universe. It is located in the constellation Leo (the Lion), and is seen by Webb just 570 million years after the Big Bang.

With the help of Webb’s Near-Infrared Spectrograph (NIRSpec), researchers have confirmed an actively growing supermassive black hole in CANUCS-LRD-z8.6. Analyzing the galaxy’s spectrum yielded an estimate of the black hole’s mass, revealing it to be unusually large for such an early stage in the Universe, and showed that CANUCS-LRD-z8.6 is compact and has not yet produced many heavy elements (a galaxy at an early stage of its evolution). This combination challenges existing theories about the formation of galaxies and black holes in the early Universe.

Science paper "Extreme properties of a compact and massive accreting black hole host in the first 500 Myr":
https://www.nature.com/articles/s41467-025-65070-x


Credit: ESA/Webb, NASA & CSA, G. Rihtaršič (University of Ljubljana, FMF), R. Tripodi (University of Ljubljana, FMF)
Release Date: Nov. 19, 2025


#NASA #Astronomy #Space #Science ##EarlyUniverse #Galaxies #CANUCSLRDz86 #LittleRedDots #LRDs #BlackHoles #Leo #Constellations #Universe #SpaceTelescopes #JWST #NIRCam #InfraredAstronomy #GSFC #STScI #UnitedStates #ESA #Europe #CSA #Canada #STEM #Education

Tuesday, November 18, 2025

New Expedition 73 Crew Photos | International Space Station

New Expedition 73 Crew Photos | International Space Station

Four Expedition 73 flight engineers pose for a playful portrait through a circular opening in a hatch thermal cover aboard the International Space Station. The cover provides micrometeoroid and orbital debris protection while maintaining cleanliness and pressure integrity in the vestibule between Northrop Grumman's Cygnus XL cargo spacecraft and the orbital outpost.

Expedition 73 flight engineer and NASA astronaut Zena Cardman is seen here working on the microgravity associated bone loss (MABL) study. It is examining intracellular signaling pathways to determine what therapeutic countermeasures can protect astronaut bone health on future long duration missions to places like the Moon or Mars.

NASA astronaut and Expedition 73 flight engineer Jonny Kim shows off a variety of food items from South Korea and the U.S. during lunchtime aboard the International Space Station's Unity module.
NASA astronaut and Expedition 73 flight engineer Mike Fincke shows off a portion of a hatch seal during maintenance work on the hatch between the Destiny laboratory module and the Harmony module aboard the International Space Station.
Japan Aerospace Exploration Agency (JAXA) astronaut and Expedition 73 flight engineer Kimiya Yui smiles for a portrait during weekend housecleaning activities inside the International Space Station's Harmony module.

NASA astronaut and Expedition 73 flight engineer Jonny Kim is pictured inside the vestibule between the International Space Station's Unity module and the Cygnus XL cargo spacecraft from Northrop Grumman. Kim was preparing to open Cygnus' hatch to begin unloading about 11,000 pounds of new science and supplies for the Expedition 73 crew.

Four Expedition 73 flight engineers gather together inside the International Space Station's Harmony module and watch NASA's announcement of its 2025 Astronaut Candidate Class from the Johnson Space Center in Houston, Texas. From left, are NASA astronauts Jonny Kim, Zena Cardman, and Mike Fincke, and Japan Aerospace Exploration Agency (JAXA) astronaut Kimiya Yui.
Expedition 73 crew emblem


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Expedition 73 Crew
Station Commander: Sergey Ryzhikov (Roscosmos)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Alexey Zubritskiy, Oleg Platonov
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.

Image Credit: NASA/JSC
Release Date: Nov. 18, 2025

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