Wednesday, September 09, 2026

Journey to Galaxy Proto-supercluster COSMOS-z3.1-A | Victor Blanco Telescope

Journey to Galaxy Proto-supercluster COSMOS-z3.1-A | Victor Blanco Telescope


This video zooms into the newly discovered galaxy proto-supercluster named COSMOS-z3.1-A. 
A proto-supercluster is a loose collection of galaxies that will one day coalesce into a stable ‘cluster-of-clusters’ of galaxies. Having been observed when the Universe was only 2.1 billion years old, COSMOS-z3.1-A is the earliest, most distant proto-supercluster ever found, and it boasts an impressive mass 5,000 times that of the Milky Way galaxy.

COSMOS-z3.1-A was discovered using data from the One-hundred-deg2 DECam Imaging in Narrowbands (ODIN) survey. This survey is conducted with the Department of Energy (DOE) fabricated Dark Energy Camera (DECam), mounted on the National Science Foundation (NSF) Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory (CTIO) in Chile, a program of NSF NOIRLab.

The members of the proto-supercluster are difficult to see in this image due to their expansive distribution against a crowded background.

Learn about the Víctor M. Blanco Telescope:
https://noirlab.edu/science/programs/ctio/telescopes/victor-blanco-4m-telescope


Credit: CTIO/NOIRLab/DOE/NSF/AURA
Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani & D. de Martin (NSF NOIRLab)
Duration: 1 minute
Release Date: Sept. 8, 2026

#NASA #Astronomy #Space #Science #Galaxies #GalaxyClusters #ProtoSuperclusters #COSMOSz31A #Cosmos #Universe #VictorBlancoTelescope #CTIO #CerroTololo #Chile #NOIRLab #NSF #AURA #UnitedStates #STEM #Education #HD #Video

Close-up: Galaxy proto-supercluster—COSMOS-z3.1-A | Victor Blanco Telescope

Close-up: Galaxy proto-superclusterCOSMOS-z3.1-A | Victor Blanco Telescope

Captured within this image is the newly discovered galaxy proto-supercluster named COSMOS-z3.1-A. A proto-supercluster is a loose collection of galaxies that will one day coalesce into a stable ‘cluster-of-clusters’ of galaxies. Having been observed when the Universe was only 2.1 billion years old, COSMOS-z3.1-A is the earliest, most distant proto-supercluster ever found, and it boasts an impressive mass 5,000 times that of the Milky Way galaxy.

COSMOS-z3.1-A was discovered using data from the One-hundred-deg2 DECam Imaging in Narrowbands (ODIN) survey. This survey is conducted with the Department of Energy (DOE) fabricated Dark Energy Camera (DECam), mounted on the National Science Foundation (NSF) Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory (CTIO) in Chile, a program of NSF NOIRLab.

The members of the proto-supercluster are difficult to see in this image due to their expansive distribution against a crowded background.

Learn about the Víctor M. Blanco Telescope:
https://noirlab.edu/science/programs/ctio/telescopes/victor-blanco-4m-telescope


Credit: CTIO/NOIRLab/DOE/NSF/AURA
Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani & D. de Martin (NSF NOIRLab)
Duration: 30 seconds
Release Date: Sept. 8, 2026

#NASA #Astronomy #Space #Science #Galaxies #GalaxyClusters #ProtoSuperclusters #COSMOSz31A #Cosmos #Universe #VictorBlancoTelescope #CTIO #CerroTololo #Chile #NOIRLab #NSF #AURA #UnitedStates #STEM #Education #HD #Video

COSMOS-z3.1-A: Most distant galaxy proto-supercluster | Victor Blanco Telescope

COSMOS-z3.1-A: Most distant galaxy proto-supercluster | Victor Blanco Telescope


Captured within this image is the newly discovered galaxy proto-supercluster named COSMOS-z3.1-A. A proto-supercluster is a loose collection of galaxies that will one day coalesce into a stable ‘cluster-of-clusters’ of galaxies. Having been observed when the Universe was only 2.1 billion years old, COSMOS-z3.1-A is the earliest, most distant proto-supercluster ever found, and it boasts an impressive mass 5,000 times that of the Milky Way galaxy.

COSMOS-z3.1-A was discovered using data from the One-hundred-deg2 DECam Imaging in Narrowbands (ODIN) survey. This survey is conducted with the Department of Energy (DOE) fabricated Dark Energy Camera (DECam), mounted on the National Science Foundation (NSF) Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory (CTIO) in Chile, a program of NSF NOIRLab.

The members of the proto-supercluster are difficult to see in this image due to their expansive distribution against a crowded background.

Learn about the Víctor M. Blanco Telescope:
https://noirlab.edu/science/programs/ctio/telescopes/victor-blanco-4m-telescope


Credit: CTIO/NOIRLab/DOE/NSF/AURA
Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani & D. de Martin (NSF NOIRLab)
Release Date: Sept. 8, 2026

#NASA #Astronomy #Space #Science #Galaxies #GalaxyClusters #ProtoSuperclusters #COSMOSz31A #Cosmos #Universe #VictorBlancoTelescope #CTIO #CerroTololo #Chile #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

Tuesday, September 08, 2026

The Eclipse and The Stork

The Eclipse and The Stork

How do animals react to a total solar eclipse? 

The featured image shows a stork roosting on her nest in Poland at a partial phase of the recent total solar eclipse. If you are lucky enough to experience a total eclipse somewhere quiet and close to nature, you may be able to notice unusual daytime animal behaviors. During totality, you may hear nighttime sounds like crickets and frogs and see fireflies. In the dark, most birds are quiet. Thinking that it is time to go to bed, ducks and other waterfowl prepare to sleep on one leg with their heads turned around and their beaks tucked into their back feathers (they do not really sleep with their heads tucked under one wing). When sunlight returns at the end of totality, songbirds greet the new "morning" with their dawn songs. The crickets and frogs go quiet again. Animals and people resume their lives, only briefly disturbed by the chance alignment of our Sun and Moon.

A total solar eclipse occurs when the Moon passes directly between Earth and the Sun, completely blocking the face of the Sun.


Image Credit & Copyright: Włodzimierz Bubak
Włodzimierz's website: 
https://www.instagram.com/trzeci_plan
Text: Cecilia Chirenti (NASA GSFC, UMCP, CRESST II)
Release Date: Sept. 3, 2026

#NASA #Space #Astronomy #Science #Sun #SolarSystem #Moon #Earth #SolarEclipses #Astrophotography #WłodzimierzBubak #Astrophotographers #Poland #Polska #NASAGoddard #UMCP #UMD #Maryland #UnitedStates #STEM #Education

The Moon's Montes Carpatus Region | NASA's Lunar Reconnaissance Orbiter

The Moon's Montes Carpatus Region | NASA's Lunar Reconnaissance Orbiter

The Montes Carpatus region (16.67°N, 332.93°E) contains numerous examples of volcanic materials. The low albedo (dark) patterns may indicate pyroclastic (explosive) material that erupted over 3 billion years ago. Tobias Mayer G crater (7 kilometers in diameter) is seen in the upper left in this west-to-east view; incidence angle 44°, slew angle 68°, phase angle 36°. 

Montes Carpatus is a mountain range that forms the southern edge of the Mare Imbrium on the Moon. The selenographic coordinates of this range are 14.5° N, 24.4° W, and the formation has an overall diameter of 361 km (224 mi). They were named by astronomer Johann Heinrich von Mädler after the Carpathian Mountains in Central Europe.

Volcanic rocks are our best window to the deep interior of the Moon, and the Montes Carpatus has no shortage of volcanic landforms, including lava flows, pyroclatic deposits, and rilles. Lavas are formed as the mantle begins to melt, so by sampling volcanic rocks of various ages from regions across the Moon scientists can reconstruct the range of compositions and processes over time. The Montes Carpatus formed as a result of the giant impact that formed the mighty Imbrium basin, the mountains are actually the raised rim of the basin.

NASA's Lunar Reconnaissance Orbiter has made a 3-D map of the Moon's surface at 100-meter resolution and 98.2% coverage (excluding polar areas in deep shadow), including 0.5-meter resolution images of Apollo landing sites.

LRO has been studying the Moon from up close since 2009, making it the longest-lived lunar orbiting mission ever. The orbiter has mapped the Moon’s surface and measured its temperature, composition, and radiation environment in unprecedented detail. Data from LRO enables NASA, and our international and commercial partners, to select locations on the lunar surface where spacecraft and astronauts can safely land. The orbiter is also helping NASA identify areas near the Moon’s South Pole with crucial resources like water and extended sunlight that provides power for equipment and supports exploration activities.


Image Credit: NASA/GSFC/Arizona State University
Text Credit: Mark Robinson
Release Date: 
March 8, 2018

#NASA #Space #Astronomy #Science #Earth #Moon #Geology #Geoscience #MontesCarpatus #MariusHills #VolcanicRocks #LRO #LunarOrbiter #LROC #NAC #SpaceRobotics #SpaceTechnology #NASAGoddard #GSFC #ASU #UnitedStates #SolarSystem #SpaceExploration #STEM #Education

Aurora Borealis over Canada and The United States | International Space Station

Aurora Borealis over Canada and The United States | International Space Station

Expedition 75 flight engineer and NASA astronaut Anil Menon: "Insane auroras these days on every orbit over North America."

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/


Expedition 75 Crew
Station Commander: Jessica Meir
Roscosmos (Russia) Flight Engineers:
Andrey Fedyaev,
Anna Kikina, Pyotr Dubrov
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jack Hathaway, Anil Menon

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.


Video Credit: NASA's Johnson Space Center/A. Menon
Duration: 33 seconds
Release Date: Sept 8, 2026


#NASA #Space #Science #ISS #Planets #Earth #Atmospheres #Aurora #AuroraBorealis #Canada #Astronauts #AnilMenon #AstronautVideography #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #Europe #ESA #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education #HD #Video

Anak Krakatau Volcanic Eruption in Indonesia | Europe's Sentinel-3 Earth Satellite

Anak Krakatau Volcanic Eruption in Indonesia | Europe's Sentinel-3 Earth Satellite

This image, captured by the Copernicus Sentinel-3 mission on Saturday, September 3, 2026, shows a plume from the eruption of Anak Krakatau. The small volcanic island, in the Indonesian archipelago situated between Sumatra and Java, began spewing ash and lava on September 4. This caused disruption and flight cancellations at Jakarta's Soekarno-Hatta International Airport over the weekend, although the airport has now reopened.

In this image, the white plume is a mix of volcanic gases that have reached a high altitude—gases emitted during eruptions usually consist mainly of water vapor, carbon dioxide, and sulphur dioxide. The brown clouds also seen in the image are made up of ash and debris drifting at a lower altitude.

The image was captured by Sentinel-3’s Ocean and Land Color Instrument (OLCI), an imaging spectrometer. This optical instrument has 21 distinct spectral bands that measure data on ocean color and vegetation with a spatial resolution of 300 meters. This provides data for monitoring ocean ecosystems, supporting crop management and agriculture and providing estimates of atmospheric aerosol and clouds.

The Copernicus Sentinel-3 mission consists of two satellites with a third satellite due to launch on board a Vega-C launcher from Europe’s Spaceport in French Guiana no earlier than September 14, 2026.

EUMETSAT operates the Sentinel-3 satellites, in cooperation with the European Space Agency (ESA), and delivers the marine and atmospheric data on behalf of the European Union. 

The European Organization for the Exploitation of Meteorological Satellites (EUMETSAT) is an intergovernmental organization created through an international convention agreed by a current total of 30 European Member States. EUMETSAT's primary objective is to establish, maintain and exploit European systems of operational meteorological satellites. EUMETSAT is responsible for the launch and operation of the satellites and for delivering satellite data to end-users as well as contributing to the operational monitoring of climate and the detection of global climate changes.

The activities of EUMETSAT contribute to a global meteorological satellite observing system coordinated with other space-faring states.

The European Space Agency's Copernicus Earth Observation Program: 
https://sentinel.esa.int/web/sentinel/copernicus/


Credits: contains modified Copernicus Sentinel data (2026), processed by ESA; CC BY-SA 3.0 IGO
Release Date: Sept. 8, 2026


#NASA #Space #Science #Satellites #CopernicusProgramme #Sentinel3 #Earth #Atmospheres #AnakKrakatau #Indonesia #Volcanoes #AshClouds #EUMETSAT #Europe #InternationalCooperation #Environment #EarthObservation #RemoteSensing #STEM #Education

Tiny Worlds Discovered by Hubble and Webb Space Telescopes

Tiny Worlds Discovered by Hubble and Webb Space Telescopes

Beyond Neptune, countless frozen worlds have orbited the Sun for billions of years, preserving clues from the earliest days of our solar system.

By combining observations from NASA’s Hubble and James Webb space telescopes, astronomers discovered previously unknown Trans-Neptunian Objects, or TNOs, in the deepest search for these distant objects ever conducted. 

Together, Hubble and Webb are giving scientists a new look at some of the solar system’s oldest survivors and revealing new clues about how the building blocks of planets, including Earth, first formed.

For more information, visit:
science.nasa.gov/mission/hubble


Credit: NASA's Goddard Space Flight Center 
Paul Morris: Lead Producer
Duration: 2 minutes, 39 seconds
Release Date: Sept. 8, 2026

#NASA #ESA #Astronomy #Space #Science #TransNeptunianObjects #TNOs #Cosmos #Universe #JWST #InfraredAstronomy #HubbleSpaceTelescope #HST #SpaceTelescopes #Europe #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Monday, September 07, 2026

Isar Aerospace Achieves First Launch to Orbit from Continental Europe | ESA

Isar Aerospace Achieves First Launch to Orbit from Continental Europe | ESA


German company ‪Isar Aerospace ‬successfully reached orbit with their Spectrum launcher, lifting off from Andøya Spaceport in Norway at 21:12 BST/22:12 Central European Summer Time (CEST) on September 5, 2026. It became the first commercial space company from Europe to successfully deliver satellites into orbit, on what was only its second flight.

Spectrum is a two-stage, 28 meter tall launch vehicle and, with its ten engines, is targeting to launch payloads of up to 1000 kg to low Earth orbit. 

The mission ‘Onward and Upward’ is supported by the European Space Agency’s Boost! program. Isar Aerospace also won the first Microlauncher Competition awarded by the German Space Agency (DLR). This resulted in the selection of the payloads on this flight. 

Initially supported by ESA’s Business Incubation Centrer, Isar Aerospace has received several rounds of co-funding as part of the European Space Agency’s Boost! program that helps commercial initiatives offering space transportation services. Under Boost! contract, ESA supported the development of the Spectrum launch service, including this second Spectrum flight . 

In 2025, Isar Aerospace was one of the launch service operators selected for the European Launcher Challenge. As a first important milestone, the European Launcher Challenge requires launch service providers to achieve an orbital launch no later than 2027. This flight has demonstrated the Spectrum launch system successfully, making Isar Aerospace the first provider to reach this milestone for the European Launcher Challenge. 

Learn more about Isar Aerospace:
https://isaraerospace.com


Credits: Isar Aerospace
Duration: 1 minute, 37 seconds
Release Date: Sept. 7, 2026

#NASA #ESA #Space #Satellites #‪IsarAerospace #Germany #Deutschland #SpectrumLaunchVehicle #RocketLaunch #AndøyaSpaceport #Norway #Norge #CommercialSpace #STEM #Education #HD #Video

The Milky Way's Core: View from Outer Banks, North Carolina

The Milky Way's Core: View from The Outer Banks, North Carolina

Astrophotographer Jonathan Harmon: A "shot of Bodie Island light with Milky Way core."

"If you have been wanting to see the Milky Way at a civilized hour, now is the time to look. Right after sunset, the backbone of our galaxy materializes in the south and reaches straight up into the sky."

"In early September, the core of the Milky Way is visible after dusk and peaks between 9 p.m. and 10 p.m., letting you view it without staying up past midnight. The early evening sky will remain essentially moonless for the next week, setting the stage for long exposures of the galaxy's dust lanes and star clouds."

Learn about Bodie Island Light Station:
https://www.nps.gov/caha/planyourvisit/bils.htm

North Carolina is a state in the Southeastern region of the United States. It is bordered by Virginia to the north, the Atlantic Ocean to the east, South Carolina to the south, Georgia to the southwest, and Tennessee to the west.


Image Credit: Jonathan Harmon
Text Credit: Spaceweather[dot]com
Location: The Outer Banks, Nags Head, North Carolina, United States
Date: Sept. 1, 2026

#NASA #Astronomy #Space #Science #SolarSystem #Stars #SagittariusConstellation  #MilkyWayGalaxy #Cosmos #Universe #Astrophotography #JonathanHarmon #Astrophotographers #TheOuterBanks #NagsHead #NorthCarolina  #UnitedStates #STEM #Education

Journey to Galaxy Cluster Abell 370 in Cetus | Hubble Space Telescope

Journey to Galaxy Cluster Abell 370 in Cetus | Hubble Space Telescope


The final image shows the massive galaxy cluster Abell 370 embedded in the middle of a field of nearly 8,000 galaxies scattered across space and time. Located approximately 4 billion light-years away in the constellation Cetus, the Sea Monster, this immense cluster is a rich mix of a variety of galaxy shapes. This "galaxies galore" snapshot is from a Hubble Space Telescope survey to enlarge the area around huge galaxy clusters previously photographed by Hubble.

Galaxy clusters like Abell 370 are mainly composed of dark matter. Their large masses distort space, turning them into gravitational lenses that magnify and distort the light coming from distant background galaxies. This allows the discovery of background galaxies and supernovas that are so distant and faint that they could not have been photographed by Hubble without the aid of this additional gravitational amplification.

This image is part of the Beyond Ultra-deep Frontier Fields And Legacy Observations (BUFFALO) survey.


Credit: NASA, ESA, A. Koekemoer (STScI), M. Jauzac (Durham University), C. Steinhardt (Niels Bohr Institute), and the BUFFALO team, Digitized Sky Survey 2, Nick Risinger
Duration: 50 seconds
Released Date: Sept. 13, 2018


#NASA #ESA #Hubble #Astronomy #Space #Science #Galaxies #GalaxyClusters #Abell370 #CetusConstellation #Cosmos #Universe #HubbleSpaceTelescope #HST #NASAGoddard #GSFC #DSS2 #STScI #STEM #Education #HD #Video

Close-up: Galaxy Cluster Abell 370 in Cetus | Hubble Space Telescope

Close-up: Galaxy Cluster Abell 370 in Cetus | Hubble Space Telescope

This beautiful image shows the massive galaxy cluster Abell 370 embedded in the middle of a field of nearly 8,000 galaxies scattered across space and time. Located approximately 4 billion light-years away in the constellation Cetus, the Sea Monster, this immense cluster is a rich mix of a variety of galaxy shapes. This "galaxies galore" snapshot is from a Hubble Space Telescope survey to enlarge the area around huge galaxy clusters previously photographed by Hubble.

Galaxy clusters like Abell 370 are mainly composed of dark matter. Their large masses distort space, turning them into gravitational lenses that magnify and distort the light coming from distant background galaxies. This allows the discovery of background galaxies and supernovas that are so distant and faint that they could not have been photographed by Hubble without the aid of this additional gravitational amplification.

This image is part of the Beyond Ultra-deep Frontier Fields And Legacy Observations (BUFFALO) survey.


Credit: NASA, ESA, A. Koekemoer (STScI), M. Jauzac (Durham University), C. Steinhardt (Niels Bohr Institute), and the BUFFALO team
Duration: 50 seconds
Released Date: Sept. 13, 2018


#NASA #ESA #Hubble #Astronomy #Space #Science #Galaxies #GalaxyClusters #Abell370 #CetusConstellation #Cosmos #Universe #HubbleSpaceTelescope #HST #NASAGoddard #GSFC #STScI #STEM #Education #HD #Video

China's Commercial Space Firms Set Sights on The Moon

China's Commercial Space Firms Set Sights on The Moon

In China, private space companies are getting ready to go lunar. At the International Deep Space Exploration Conference this week in Hefei, capital of Anhui province, companies showcased plans for lunar exploration—from robots to rovers to new rockets built for deeper space missions.


Video Credit: CGTN
Duration: 2 minutes, 30 seconds
Release Date: Sept. 7, 2026

#NASA #Space #Astronomy #Science #China #中国 #Moon #SouthPole #CLEP #SpaceRobotics #LunarRovers #SpaceTechnology #LunarExploration #SpaceExploration #SolarSystem #CASSpace #中科宇航 #CommercialSpace #Anhui #安徽 #InternationalCooperation #STEM #Education #HD #Video

Galaxy Cluster Abell 370 in Cetus | Hubble Space Telescope

Galaxy Cluster Abell 370 in Cetus | Hubble Space Telescope

This beautiful image shows the massive galaxy cluster Abell 370 embedded in the middle of a field of nearly 8,000 galaxies scattered across space and time. Located approximately 4 billion light-years away in the constellation Cetus, the Sea Monster, this immense cluster is a rich mix of a variety of galaxy shapes. This "galaxies galore" snapshot is from a Hubble Space Telescope survey to enlarge the area around huge galaxy clusters previously photographed by Hubble.

Galaxy clusters like Abell 370 are mainly composed of dark matter. Their large masses distort space, turning them into gravitational lenses that magnify and distort the light coming from distant background galaxies. This allows the discovery of background galaxies and supernovas that are so distant and faint that they could not have been photographed by Hubble without the aid of this additional gravitational amplification.

This image is part of the Beyond Ultra-deep Frontier Fields And Legacy Observations (BUFFALO) survey.


Credit: NASA, ESA, A. Koekemoer (STScI), M. Jauzac (Durham University), C. Steinhardt (Niels Bohr Institute), and the BUFFALO team
Released Date: Jan. 10, 2019


#NASA #ESA #Hubble #Astronomy #Space #Science #Galaxies #GalaxyCluster#Abell370 #CetusConstellation #Cosmos #Universe #HubbleSpaceTelescope #HST #NASAGoddard #GSFC #STScI #STEM #Education

Sunday, September 06, 2026

NASA Artemis III RS-25 SLS Rocket Engine Install | Kennedy Space Center

NASA Artemis III RS-25 SLS Rocket Engine Install | Kennedy Space Center

Technicians prepare to transfer the #2 RS-25 Space Launch System (SLS) rocket engine (front) to the work stand with the #3 engine (back) for integration with the Artemis III core stage rocket on Tuesday, Aug. 25, 2026, inside the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida.
The first of four RS-25 Space Launch System (SLS) rocket engines, is installed on the work stand and integrated with the Artemis III core stage rocket on Tuesday, Aug. 25, 2026, inside the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida.



Technicians lift and transfer the #2 RS-25 Space Launch System (SLS) rocket engine (back) to the work stand. Visible in the foreground is the #3 engine already integrated with the Artemis III core stage rocket on Tuesday, Aug. 25, 2026.
Technicians prepare the #2 RS-25 Space Launch System (SLS) rocket engine for transfer onto a work stand ahead of integration with the Artemis III core stage rocket on Tuesday, Aug. 25, 2026.
Technicians lift and transfer the #2 RS-25 Space Launch System (SLS) rocket engine (back) to the work stand. Visible in the foreground is the #3 engine already integrated with the Artemis III core stage rocket on Tuesday, Aug. 25, 2026.

During late August 2026, technicians at NASA’s Kennedy Space Center in Florida began the installation of the four RS-25 engines in the core stage of the agency’s Space Launch System (SLS) rocket that will launch the Artemis III crew next year. These engines will generate more than two million pounds of thrust at liftoff.

The milestone on Aug. 24 marked the next phase of core stage integration following the mating of the engine section to the top four-fifths of the stage earlier this summer. Inside High Bay 2 at the spaceport’s Vehicle Assembly Building (VAB), teams will continue installing the remaining engines, as well as the propulsion and electrical systems throughout the stage.

Weighing in at approximately 7,700 pounds, each engine produces nearly 500,000 pounds of thrust. All four engines are located at the base of the SLS and are integrated inside the engine section. Built to withstand the extreme conditions during launch, this section protects the engines from severe temperatures. During ascent, the engines fire continuously for more than eight minutes, consuming propellant from the core stage’s two massive propellant tanks at a rate of approximately 1,500 gallons per second.

Each RS-25 engine carries a unique serial number that traces its detailed flight history. The four engines assigned to Artemis III, including E2054, E2057, E2048, and E2052, previously powered multiple shuttle missions. Engine 2048 helped power NASA astronaut Randy Bresnik’s previous mission on space shuttle Atlantis during the STS-129 mission. The engine also powered Space Shuttle Discovery on STS-95 in 1998, which was the mission that returned 77-year-old space pioneer U.S. Sen. John Glenn to orbit, making him the oldest person to fly in space at the time.

Technicians also continue to integrate the twin solid rocket booster motor segments atop the mobile launcher inside the VAB. Teams began stacking the segments in early July and are now more than halfway complete after streamlining processes and procedures learned from previous Artemis launches.

Progress on the Orion spacecraft continues after the recent integration of the crew and service modules. Technicians recently installed the umbilical connector, which bridges the electrical, data, and fluid systems between the two modules, and installed its electrical connectors and fluid lines. Teams powered on the spacecraft for the first time since joining the two components to ensure electrical connectivity through the umbilical mechanism and that the communications of the subsystems between the crew and service module work as planned.

Planned to launch in 2027, the Artemis III Mission will practice docking the Orion spacecraft with two lunar landers in low Earth orbit. 

On future missions, including Artemis IV in 2028, landers will bring astronauts to the lunar surface. While Artemis III will not land on the Moon, it will test the complex capabilities NASA needs to return—this time to stay.

Learn more about NASA’s Artemis program:

Image Credit: NASA/Clayton Rougelot
Release Date: Aug. 27, 2026

#NASA #Space #Science #Earth #Moon #ArtemisProgram #ArtemisIII #ArtemisIIIMission #LunarLanders #HLS #NASASLS #OrionSpacecraft #Astronauts #RandyBresnik #FrankRubio #AndreDouglas #LucaParmitano #Italy #Italia #Europe #HumanSpaceflight #SolarSystem #SpaceExploration #NASAKennedy #MerrittIsland #Florida #UnitedStates #STEM #Education

Waning gibbous Moon above Earth’s atmosphere | International Space Station

Waning gibbous Moon above Earth’s atmosphere | International Space Station

The waning gibbous Moon appears above Earth’s blue atmosphere in this image taken from the International Space Station while orbiting 258 miles above the coast of Hong Kong, China.

The waning gibbous intermediate Moon phase starts after the Full Moon and lasts until half of the Moon’s face remains lit up at the Third Quarter.


Expedition 75 Crew
Station Commander: Jessica Meir
Roscosmos (Russia) Flight Engineers:
Andrey Fedyaev,
Anna Kikina, Pyotr Dubrov
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jack Hathaway, Anil Menon

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's Johnson Space Center
Image Date: Aug. 30, 2026


#NASA #Space #Science #ISS #Planets #Earth #China #中国 #HongKong #香港 #Moon #WaningGibbous #AstronautPhotography #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #Expedition75 #InternationalCooperation #UnitedStates #STEM #Education