Tuesday, September 15, 2026

Launch of Europe's FLEX and Sentinel-3C Earth Satellites on Vega-C Rocket

Launch of Europe's FLEX and Sentinel-3C Earth Satellites on Vega-C Rocket

The European Space Agency's FLEX Earth Explorer satellite and the Copernicus Sentinel-3C satellite have been launched together aboard a Vega-C rocket from Europe’s Spaceport in French Guiana on the northern coast of South America, as part of Europe’s Earth Observation Programs. Flight VV30 lifted off on September 15, 2026 at 03:21 (14 September at 22:21 local time).

FLEX is designed to reveal a phenomenon invisible to the human eye—the faint fluorescence emitted by plants as they photosynthesize. Equipped with a Fluorescence Imaging Spectrometer, FLEX will detect and measure this incredibly weak signal from orbit. Because the fluorescence varies with plant health and environmental conditions, the measurements will provide scientists with new information about photosynthetic activity and vegetation stress on a global scale.

Sentinel-3C is the third in the Sentinel-3 series. Copernicus Sentinel-3C will continue the mission’s task of measuring systematically Earth’s oceans, land, ice and atmosphere to monitor and understand large-scale global dynamics. The mission also provides essential information in near-real time for ocean and weather forecasting.

Europe’s Vega-C rocket can launch 2,300 kg into space, such as small scientific and Earth observation spacecraft. At 35 meters tall, Vega-C weighs 210 tons on the launch pad and reaches orbit with three solid-propellant-powered stages before the fourth liquid-propellant stage takes over for precise placement of satellites into their desired orbit around Earth.

This flight is a first dual launch for Vega-C, using a secondary payload adapter called Vespa. Sentinel-3C is placed on top of Vespa inside the main fairing and once deployed the Vespa adapter opens to reveal FLEX for its injection into orbit.

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


Credits: ESA/CNES/Avio
Duration: 2 minutes, 18 seconds
Release Date: Sept. 14, 2026

#NASA #Space #Astronomy #Science #CopernicusProgramme #Sentinel3 #Planets #Earth #Atmospheres #Oceans #Ice #Vegetation #Agriculture #EarthObservation #RemoteSensing #Environment #ClimateChange #GlobalHeating #VegaCRocket #GuianaSpaceCentre #KourouSpaceport #FrenchGuiana #Avio #ArianeGroup #STEM #Education #HD #Video

Monday, September 14, 2026

Planet Venus emerges from behind The Moon: A Lunar Occultation

Planet Venus emerges from behind The Moon: A Lunar Occultation

Astrophotographer Maximilian-Vlad Teodorescu: ". . .  the emergence of Venus from behind the Moon. A daytime event, requiring a lot of luck with the massive clouds rolling in."

The Moon just occulted Venus. The event was visible from India to Europe.

Occultation refers to the process where a celestial body, such as a star or planet, temporarily obscures another body, allowing astronomers to study its properties.


Image Credit: Maximilian-Vlad Teodorescu
Location: Magurele, Romania 
Image Details: 115 mm APO refractor, ASI 183MM, IR-pass 685 nm filter
Date: Sept. 14, 2026


#NASA #Astronomy #Space #Science #SolarSystem #Planets #Venus #Earth #Moon #LunarOccultations #Astrophotography #MaximilianVladTeodorescu #Astrophotographers #Magurele #Romania #România #STEM #Education

Full Dome View: Irregular Dwarf Galaxy IC 1613 in Cetus | VLT Survey Telescope

Full Dome View: Irregular Dwarf Galaxy IC 1613 in Cetus | VLT Survey Telescope

This image, captured with the OmegaCAM camera on the European Southern Observatory’s VLT Survey Telescope in Chile, shows an unusually clean small galaxy. IC 1613 contains very little cosmic dust, allowing astronomers to explore its contents with great clarity.

Note: The full dome video display format is designed for projection systems in planetariums.

The irregular dwarf galaxy IC 1613 contains around 100 million stars and is a member of our Local Group of galaxies. This also includes our Milky Way, the Andromeda spiral galaxy, and the Magellanic Clouds. It is at a distance of 2.4 million light-years and contains several examples of Cepheid variable stars—key calibrators of the cosmic distance ladder. The bulk of its stars were formed about 7 billion years ago and it does not appear to be undergoing star formation at the present day, unlike other very active dwarf irregulars, such as the Large and Small Magellanic clouds.

Learn about the European Southern Observatory's VLT Survey Telescope:

Credit: European Southern Observatory (ESO)
Acknowledgement: VST/OmegaCAM Local Group Survey
Duration: 20 seconds
Release Date: Jan. 27, 2016


#NASA #Astronomy #Space #Science #Stars #CepheidVariableStars #CepheidVariables #Galaxies #IrregularGalaxies #DwarfGalaxies #IC1613 #CetusConstellation #Cosmos #Universe #VLTSurveyTelescope #VSTOmegaCAM #ParanalObservatory #Chile #Europe #STEM #Education #FullDomeView #HD #Video

Wide-field view: Irregular Dwarf Galaxy IC 1613 in Cetus | Digitized Sky Survey 2

Wide-field view: Irregular Dwarf Galaxy IC 1613 in Cetus | Digitized Sky Survey 2


This wide-field view shows the sky around the dwarf galaxy IC 1613 in the constellation of Cetus (The Sea Monster). This picture was created from images forming part of the Digitized Sky Survey 2. The galaxy appears at the center of the picture as an irregularly shaped clump of faint stars.

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 (STScI) through its Guide Star Survey group.


Credit: European Southern Observatory (ESO)/Digitized Sky Survey 2
Acknowledgement: Davide De Martin
Release Date: Jan. 27, 2016


#NASA #Astronomy #Space #Science #Stars #CepheidVariableStars #CepheidVariables #Galaxies #IrregularGalaxies #DwarfGalaxies #IC1613 #CetusConstellation #Cosmos #Universe #VLTSurveyTelescope #VSTOmegaCAM #ParanalObservatory #Chile #Europe #STScI #UnitedStates #STEM #Education

Journey to Irregular Dwarf Galaxy IC 1613 in Cetus | VLT Survey Telescope

Journey to Irregular Dwarf Galaxy IC 1613 in Cetus | VLT Survey Telescope


This sequence starts with a broad view of the rather faint constellation of Cetus (The Sea Monster). As we zoom, we close in on a faint, but nearby galaxy, IC 1613. The final detailed image, captured with the OmegaCAM camera on the European Southern Observatory’s VLT Survey Telescope in Chile, shows an unusually clean small galaxy. IC 1613 contains very little cosmic dust, allowing astronomers to explore its contents with great clarity.

The irregular dwarf galaxy IC 1613 contains around 100 million stars and is a member of our Local Group of galaxies. This also includes our Milky Way, the Andromeda spiral galaxy, and the Magellanic Clouds. It is at a distance of 2.4 million light-years and contains several examples of Cepheid variable stars—key calibrators of the cosmic distance ladder. The bulk of its stars were formed about 7 billion years ago and it does not appear to be undergoing star formation at the present day, unlike other very active dwarf irregulars, such as the Large and Small Magellanic clouds.

Learn about the European Southern Observatory's VLT Survey Telescope:

Credit: European Southern Observatory (ESO)
Acknowledgement: VST/OmegaCAM Local Group Survey
Duration: 50 seconds
Release Date: Jan. 27, 2016


#NASA #Astronomy #Space #Science #Stars #CepheidVariableStars #CepheidVariables #Galaxies #IrregularGalaxies #DwarfGalaxies #IC1613 #CetusConstellation #Cosmos #Universe #VLTSurveyTelescope #VSTOmegaCAM #ParanalObservatory #Chile #Europe #STEM #Education #HD #Video

Close-up: The Irregular Dwarf Galaxy IC 1613 | VLT Survey Telescope

Close-up: The Irregular Dwarf Galaxy IC 1613 in Cetus | VLT Survey Telescope

This image, captured with the OmegaCAM camera on the European Southern Observatory’s VLT Survey Telescope in Chile, shows an unusually clean small galaxy. IC 1613 contains very little cosmic dust, allowing astronomers to explore its contents with great clarity.

The irregular dwarf galaxy IC 1613 contains around 100 million stars and is a member of our Local Group of galaxies. This also includes our Milky Way, the Andromeda spiral galaxy, and the Magellanic Clouds. It is at a distance of 2.4 million light-years and contains several examples of Cepheid variable stars—key calibrators of the cosmic distance ladder. The bulk of its stars were formed about 7 billion years ago and it does not appear to be undergoing star formation at the present day, unlike other very active dwarf irregulars, such as the Large and Small Magellanic clouds.

Learn about the European Southern Observatory's VLT Survey Telescope:

Credit: European Southern Observatory (ESO)
Acknowledgement: VST/OmegaCAM Local Group Survey
Duration: 50 seconds
Release Date: Jan. 27, 2016


#NASA #Astronomy #Space #Science #Stars #CepheidVariableStars #CepheidVariables #Galaxies #IrregularGalaxies #DwarfGalaxies #IC1613 #CetusConstellation #Cosmos #Universe #VLTSurveyTelescope #VSTOmegaCAM #ParanalObservatory #Chile #Europe #STEM #Education #HD #Video

The Irregular Dwarf Galaxy IC 1613 in Cetus | VLT Survey Telescope

The Irregular Dwarf Galaxy IC 1613 in Cetus | VLT Survey Telescope

This image, captured with the OmegaCAM camera on the European Southern Observatory’s VLT Survey Telescope in Chile, shows an unusually clean small galaxy. IC 1613 contains very little cosmic dust, allowing astronomers to explore its contents with great clarity.

The irregular dwarf galaxy IC 1613 contains around 100 million stars and is a member of our Local Group of galaxies. This also includes our Milky Way, the Andromeda spiral galaxy, and the Magellanic Clouds. It is at a distance of 2.4 million light-years and contains several examples of Cepheid variable stars—key calibrators of the cosmic distance ladder. The bulk of its stars were formed about 7 billion years ago and it does not appear to be undergoing star formation at the present day, unlike other very active dwarf irregulars, such as the Large and Small Magellanic clouds.

Learn about the European Southern Observatory's VLT Survey Telescope:

Credit: European Southern Observatory (ESO)
Acknowledgement: VST/OmegaCAM Local Group Survey
Release Date: Jan. 27, 2016


#NASA #Astronomy #Space #Science #Stars #CepheidVariableStars #CepheidVariables #Galaxies #IrregularGalaxies #DwarfGalaxies #IC1613 #CetusConstellation #Cosmos #Universe #VLTSurveyTelescope #VSTOmegaCAM #ParanalObservatory #Chile #Europe #STEM #Education

Flying over the Magellanic Clouds | ESO's VISTA Survey Telescope

Flying over the Magellanic Clouds (infrared views) | ESO's VISTA Survey Telescope

The Magellanic Clouds are two dwarf galaxies that orbit our home galaxy, the Milky Way. Using ESO’s Visible and Infrared Survey Telescope for Astronomy (VISTA) astronomers have taken very deep infrared images of the cores of these galaxies that will allow us to better understand their 3D shapes and motion. By repeating these observations over several years they could measure the subtle motion of stars in the cores. Moreover, they also monitored periodic changes in the brightness of certain stars, which can be used to measure distances and therefore reconstruct the 3D structure of the cores of these galaxies.


Credit: European Southern Observatory (ESO)
Animations & footage: ESO/M. R. Cioni et al., VMC Survey, P. Horálek, Zdeněk Bardon, N. Risinger
Script: J. C. Muñoz
Editing: M. Martins
Duration: 1 minute
Release Date: Sept. 14, 2026

#NASA #Astronomy #Space #Science #Galaxies #DwarfGalaxies #MagellanicClouds #LMC #SMC #Cosmos #Universe #VISTASurveyTelescope #InfraredAstronomy #ParanalObservatory #Chile #Europe #STEM #Education #HD #Video

Sunday, September 13, 2026

The Whale Galaxy: NGC 4631 in Canes Venatici (x-ray view) | NASA Chandra

The Whale Galaxy: NGC 4631 in Canes Venatici (x-ray view) | NASA Chandra


A spiral galaxy viewed from its side, featuring a giant halo of hot gas blowing out of its stellar disk. X-rays from Chandra and the European Space Agency’s XMM-Newton (purple and royal blue) trace hot gas driven out by supernovas and black holes and neutron stars pulling gas from their companions, while optical light (light blue, gold and white) from ground-based observer R. Jay GaBany showcases dense dust lanes. Edge-on views of galaxies allow astronomers to study how flat their stellar disks are and provide the clearest views of material located above or below the disk.

Here, a profusion of starbirth lights up the galactic center, revealing bands of dark material between us and the starburst—a region of intense star formation. The galaxy’s activity tapers off  in its outer regions where there are fewer stars and less dust, but these are still punctuated by pockets of star formation.

The Whale Galaxy is about 30 million light-years away from us in the constellation of Canes Venatici (The Hunting Dogs) and is a spiral galaxy much like the Milky Way. From our vantage point, however, we see the Whale Galaxy edge-on, seeing its glowing center through dusty spiral arms. The galaxy's central bulge and asymmetric tapering disc have suggested the shape of a whale or a herring to past observers.

Many supernovae—the explosions of hot, blue, short-lived stars at least eight times the mass of the Sun—have gone off in the core of the Whale Galaxy. The stellar pyrotechnics have bathed the galaxy in hot gas visible to x-ray telescopes. 

From such work, the triggers of the starburst in the Whale Galaxy and others can be elucidated. The gravitational "feeding" on intergalactic material, as well as clumping caused by the gravitational interactions with its galactic neighbors, creates the areas of greater density where stars start to coalesce. Just as blue whales, the biggest creatures on Earth, can gorge themselves on comparatively tiny bits of plankton, so the Whale Galaxy has become filled with the gas and dust that powers a high rate of star formation.


Credit: X-ray: NASA/CXC/SAO; Optical: ©2011-2015 by R Jay GaBany
Image Processing: NASA/CXC/SAO/L. Frattare
Release Date: Aug. 25, 2026


#NASA #Astronomy #Space #Science #Stars #Supernovae #Galaxies #NGC4631 #SpiralGalaxies #StarburstGalaxies #CanesVenaticiConstellation #Cosmos #Universe #CXC #SpaceTelescopes #ESA #XMMNewton #XrayAstronomy #UnitedStates #ESA #Europe #Astrophotographers #RJayGaBany #Astrophotography #STEM #Education

Irregular Dwarf Galaxy IC 1613 in Cetus | Victor Blanco Telescope

Irregular Dwarf Galaxy IC 1613 in Cetus | Victor Blanco Telescope


The irregular dwarf galaxy IC 1613 contains around 100 million stars and is a member of our Local Group of galaxies. This also includes our Milky Way, the Andromeda spiral galaxy, and the Magellanic Clouds. It is at a distance of 2.4 million light-years and contains several examples of Cepheid variable stars—key calibrators of the cosmic distance ladder. The bulk of its stars were formed about 7 billion years ago and it does not appear to be undergoing star formation at the present day, unlike other very active dwarf irregulars, such as the Large and Small Magellanic clouds.

To the lower right of IC 1613, one may view a background galaxy cluster (several hundred times more distant than IC 1613) consisting of dozens of orange-yellow blobs, centered on a pair of giant cluster elliptical galaxies. To the left of the irregular galaxy is a bright, sixth magnitude, foreground, Milky Way star in the constellation of Cetus the Whale, identified here as a star by its sharp diffraction spikes radiating at 45-degree angles. 

This image is an excerpt from the Dark Energy Survey. It has released a massive, public collection of astronomical data and calibrated images from six years of work. The Dark Energy Survey is a global collaboration that includes the Department of Energy's (DOE) Fermi National Accelerator Laboratory (Fermilab), the National Center for Supercomputing Applications (NCSA), and the National Science Foundation (NSF) NOIRLab. The image was taken with the Dark Energy Camera, fabricated by DOE, on the Víctor M. Blanco 4-meter Telescope.

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


Credit: DES/DOE/Fermilab/NCSA & CTIO/NOIRLab/NSF/AURA
Acknowledgments: Image processing: DES, Jen Miller (Gemini Observatory/NSF NOIRLab), Travis Rector (University of Alaska Anchorage), Mahdi Zamani & Davide de Martin
Release Date: Jan. 14, 2021


#NASA #Astronomy #Space #Science #Stars #CepheidVariableStars #CepheidVariables #Galaxies #IrregularGalaxies #DwarfGalaxies #IC1613 #Cosmos #Universe #VictorBlancoTelescope #CTIO #CerroTololo #Chile #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

Planetary Nebula Sh2-42 in Sagittarius: "A Star's Funeral Pyre" | SMARTS Telescope

Planetary Nebula Sh2-42 in Sagittarius: "A Star's Funeral Pyre" SMARTS Telescope

This image shows the planetary nebula Sh2-42 in the constellation Sagittarius. It was captured using the SMARTS 0.9-meter Telescope at Cerro Tololo Inter-American Observatory in Chile, a Program of the U.S. National Science Foundation's NOIRLab. 

Despite the name, planetary nebulae have nothing to do with planets. They are spectacular 'funeral pyres' formed by red giant stars at the end of their lives. As these giant stars expand and throw their outer gaseous layers into space, the hot exposed core of the star ionizes the surrounding material, causing it to glow in a range of vivid colors. As it reaches the end of its life, our own Sun is expected to form a planetary nebula—but not for another 5 billion years.

Learn more about the SMARTS–GSU 0.9-meter Telescope:
https://noirlab.edu/public/programs/ctio/smarts-gsu-09m-telescope/


Credit: CTIO/NOIRLab/NSF/AURA
Acknowledgments: Image Processing: T. A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani & D. de Martin (NSF NOIRLab)
Release Date: May 26, 2021

#NASA #Astronomy #Space #Science #Stars #Nebulae #PlanetaryNebulae #Sh242 #SagittariusConstellation #Cosmos #Universe #SMARTSTelescope #CTIO #CerroTololo #Chile #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

'Cosmic Questions?' Aurora: View from Norway

'Cosmic Questions?' Aurora: View from Norway

Astrophotographer Karsten Berger: "A cosmic question mark appeared in the sky last night . . ."

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/

Norway, officially the Kingdom of Norway, is a Nordic country located on the Scandinavian Peninsula in Northern Europe. The country shares a long eastern border with Sweden, and is bordered by Finland and Russia to the northeast.

Image Credit: Karsten Berger
Location: Alta, Norway
Date: Sept. 9, 2026

#NASA #Space #Astronomy #Science #Planets #Earth #Aurora #AuroraBorealis #NorthernLights #SolarSystem #Sun #Astrophotography #KarstenBerger #Astrophotographer #Alta #Norway #Norge #STEM #Education

Aurora on 'Top of the World': View from Norway

Aurora on 'Top of the World': View from Norway


Astrophotographer Karsten Berger: "The North Cape is known for its notoriously bad weather. Last night, we were fortunate to experience clear skies and an active aurora display."

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/

Norway, officially the Kingdom of Norway, is a Nordic country located on the Scandinavian Peninsula in Northern Europe. The country shares a long eastern border with Sweden, and is bordered by Finland and Russia to the northeast.

Image Credit: Karsten Berger
Location: North Cape, Norway
Date: Sept. 12, 2026

#NASA #Space #Astronomy #Science #Planets #Earth #Aurora #AuroraBorealis #NorthernLights #SolarSystem #Sun #Astrophotography #KarstenBerger #Astrophotographer #NorthCape #Norway #Norge #STEM #Education

Saturday, September 12, 2026

Hong Kong Astronaut Lai Ka-ying: Sleeping Quarters Tour | China Space Station

Hong Kong Astronaut Lai Ka-ying: Sleeping Quarters Tour | China Space Station

On Wednesday, September 9, 2026, the Shenzhou 23 crew gave students in China's Hong Kong (香港) and Macao (香港) Special Administrative Regions (SARs) a unique science lesson from the Tiangong Space Station, a classroom 400 kilometers above planet Earth.

The three astronauts—Zhu Yangzhu, Zhang Zhiyuan, and Lai Ka-ying—served as space teachers. More than 200 primary and secondary school students from Hong Kong and Macao attended the class at Tsuen Wan Public Ho Chuen Yiu Memorial College in Hong Kong. It is the alma mater of Lai Ka-ying, Hong Kong's first payload specialist. Many more students across the two regions watched the class via livestream.

During the lecture, Lai gave a tour of her sleeping quarters on board the station.

The event featured scientific explanations, demonstrations conducted on the space station and questions from students, followed by a live dialogue between the astronauts and students in Hong Kong and Macao.

Shenzhou-23 Crew
Zhang Zhiyuan 张志远, Pilot (first spaceflight)
Zhu Yangzhu 朱杨柱, Commander & Flight Engineer (second spaceflight)
Lai Ka-ying/Li Jiaying 黎家盈, Payload Specialist (first spaceflight) [Hong Kong SAR]

Video Credit: China Manned Space Agency (CMSA), CCTV
Duration: 1 minute, 15 seconds
Release Date: Sept. 9, 2026


#NASA #Space #Science #Earth #China #中国 #Students #Macao #HongKong #Shenzhou23Mission #神舟二十三号 #Shenzhou23 #Taikonauts #Astronauts #ZhuYangzhu #ZhangZhiyuan #LiJiaying #LaiKaying #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #MicrogravityExperiments #SpaceLaboratory #CMSA #中国载人航天工程办公室 #HumanSpaceflight #STEM #Education #HD #Video

Peculiar Galaxy NGC 3256 in Vela | NASA's Chandra X-ray Observatory

Peculiar Galaxy NGC 3256 in Vela | NASA's Chandra X-ray Observatory

A pair of colliding, gas-rich spiral galaxies merging into a single massive system. Chandra’s X-ray data (pink) isolates point sources and shock-heated gas, Hubble’s optical light (blue and white) captures tidal tails of stars, and Webb’s infrared vision (red and orange) cuts through the dust to show hidden star formation. Galaxy collisions like this offer a preview of our far future, showing what might happen if our own Milky Way collides and merges with the nearby Andromeda Galaxy.

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: X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI; Infrared: NASA/ESA/CSA/STScI
Image Processing: NASA/CXC/SAO/L. Frattare
Release Date: Aug. 25, 2026


#NASA #Astronomy #Space #Science #Galaxies #NGC3256 #InteractingGalaxies #StarburstGalaxies #HydraCentaurusSupercluster #VelaConstellation#Cosmos #Universe #SpaceTelescopes #NASAChandra #XrayAstronomy #CXC #NASAWebb #JWST #NASAHubble #HST #NASAGoddard #STScI #UnitedStates #STEM #Education 

Dwarf Galaxy NGC 1569 in Camelopardalis | NASA's Chandra X-ray Observatory

Dwarf Galaxy NGC 1569 in Camelopardalis | NASA's Chandra X-ray Observatory

The nearby dwarf galaxy NGC 1569 is a hotbed of vigorous star birth activity. It blows huge bubbles and super-bubbles that riddle the main body of the galaxy. The galaxy's vigorous "star factories" are also manufacturing brilliant blue star clusters. This galaxy had a sudden and relatively recent onset of star birth 25 million years ago. It subsided about the time the very earliest human ancestors appeared on Earth.

Distance from Earth: about 11 million light years

In this image, the bubble structure is sculpted by the galactic super-winds and outflows caused by a colossal input of energy from collective supernova explosions that are linked with a massive episode of star birth.

The bubble-like structures seen in this image are made of hydrogen gas that glows when hit by the fierce winds and radiation from hot young stars and is racked by supernovae shocks. The first supernovae blew up when the most massive stars reached the end of their lifetimes roughly 20-25 million years ago. The environment in NGC 1569 is still turbulent and the supernovae may not only deliver the gaseous raw material needed for the formation of further stars and star clusters, but also actually trigger their birth in the tortured swirls of gas.

Chandra and XMM-Newton observations (blue and purple) reveal massive bubbles of million-degree gas inflated by stellar winds, set against a backdrop of optical light (magenta, orange and white) imaged by astrophotographer, Adam Block. Dwarf starburst galaxies can serve as local laboratories for studying the conditions of the early universe, where small, primitive galaxies formed stars at frantic rates.


Credit: X-ray: (XMM): ESA/XMM-Newton, (Chandra): NASA/CXC/SAO; Optical: Univ. of Arizona/Mt. Lemmon SkyCenter/Adam Block/Josep Drudis
Image Processing: NASA, CXC/SAO/L. Frattare
Release Date: Aug. 25, 2026


#NASA #Astronomy #Space #Science #Galaxies #DwarfGalaxies #NGC1569 #Stars #Supernovae  #CamelopardalisConstellation #Cosmos #Universe #NASAChandra #CXC #SpaceTelescopes #ESA #XMMNewton #XrayAstronomy #UA #AdamBlock #UnitedStates #Europe #STEM #Education