Tuesday, September 15, 2026

China Landspace ZhuQue-2E Commercial Rocket Qianfan Constellation Launch

China Landspace ZhuQue-2E Commercial Rocket Qianfan Constellation Launch








China on Tuesday, Sept. 15, 2026, completed its first large-scale launch of networking satellites for the Qianfan (Spacesail) mega constellation using a commercial rocket as the launch vehicle.

The Zhuque-2E Y7 carrier rocket, developed by Chinese commercial launch company LandSpace, blasted off from the Dongfeng commercial space innovation pilot zone in northwest China at 14:26 Beijing Time, sending ten networking satellites for a mega-constellation into their preset polar orbits. The satellites were produced by the Innovation Academy for Microsatellites at the Chinese Academy of Sciences, bring Qianfan's total count deployed to 248.

The Qianfan mega-constellation is operated by Shanghai Spacesail Technologies Co. Ltd. that aims to provide space-based Internet connectivity services in China and abroad in places including Brazil, Malaysia, Kazakhstan, Türkiye, and via airlines, around the fourth quarter of this year.

Compared to typical single-satellite launches, the difficulty of large-scale satellite constellation deployment lies not only in the increased number of satellites.

The simultaneous launch of multiple satellites requires addressing a series of challenges, including multi-satellite coordination, satellite-launcher coordination, batch deployment, orbital control, and the passivation and deorbiting of the rocket's end stage, placing higher demands on coordination throughout the entire mission.

"For this mission, we have conducted system-level preparations in areas such as satellite interfaces, flight procedures, multi-satellite deployment sequencing, ground testing and launch procedures, and have carried out extensive work of collaboration with the client. We aim to standardize, formalize and visualize such constellation deployment missions," said Ma Haijing, general manager of LandSpace's marketing department.

China's low-Earth orbit satellite Internet sector is entering a phase of large-scale network deployment, and the continued construction of large satellite constellations is placing higher demands on the reliability, launch frequency, and the sustained supply of launch capacity of carrier rockets.

"The Zhuque-2 series has completed nine flights. Today's mission successfully deployed 10 networking satellites at an altitude of 900 kilometers with high precision, demonstrating that the Zhuque-2E's payload capacity, propulsion system, stage separation technology and orbital insertion precision control have all reached industry-leading levels," said Ma after Tuesday's launch.

While advancing routine commercial launches with the Zhuque-2E, LandSpace is also continuing its efforts to advance reuse of the Zhuque-3 reusable rocket. The two rocket models are being developed in tandem to meet distinct payload capacities and mission requirements, further enhancing the company's capability for sustained and stable access to space.

Costing under 10 million Yuan (1.47 million United States dollars) apiece, each Qianfan satellite weighs 300 kilograms and has a ‘flat pack’ design with a single solar array to fit as many satellites as possible inside the rocket fairing in two parallel stacks. For maneuvering in orbit, each satellite has an electric hall-effect thruster burning krypton to generate 20 millinewtons of thrust with a specific impulse of 1,385 seconds.

By deploying ten Qianfan satellites, LandSpace has become the first of three enterprises contracted in August 2025 to fulfill its demonstration launch, beating CAS Space by about a month and far ahead of Space Pioneer. In the future, the company plans to deploy further satellite groups to assist with the constellation's growth towards having thousands in orbit.

Today’s mission was the 6th flight of Zhuque-2E, the 8th flight of LandSpace’s Zhuque-2 series, and LandSpace’s 11th orbital launch attempt. This was also the 63rd launch from China in 2026.


Image Credit: Landspace
Text Credit: CCTV, Jack C.
Date: Sept. 15, 2026

#NASA #Space #Science #Earth #Satellites #CommunicationsSatellites #SpaceSailConstellation #ShanghaiSpacesailTechnologies #CAS #Earth #LEO #China #中国 #LandSpace #蓝箭 #Zhuque2Rocket #Zhuque2EY7 #RocketLaunches #InnerMongolia #CommercialSpace #STEM #Education

China Landspace ZhuQue-2E Commercial Rocket Qianfan Constellation Launch

China Landspace ZhuQue-2E Commercial Rocket Qianfan Constellation Launch

China on Tuesday, Sept. 15, 2026, completed its first large-scale launch of networking satellites for the Qianfan (Spacesail) mega constellation using a commercial rocket as the launch vehicle.

The Zhuque-2E Y7 carrier rocket, developed by Chinese commercial launch company LandSpace, blasted off from the Dongfeng commercial space innovation pilot zone in northwest China at 14:26 Beijing Time, sending ten networking satellites for a mega-constellation into their preset polar orbits. The satellites were produced by the Innovation Academy for Microsatellites at the Chinese Academy of Sciences, bring Qianfan's total count deployed to 248.

The Qianfan mega-constellation is operated by Shanghai Spacesail Technologies Co. Ltd. that aims to provide space-based Internet connectivity services in China and abroad in places including Brazil, Malaysia, Kazakhstan, Türkiye, and via airlines, around the fourth quarter of this year.

Compared to typical single-satellite launches, the difficulty of large-scale satellite constellation deployment lies not only in the increased number of satellites.

The simultaneous launch of multiple satellites requires addressing a series of challenges, including multi-satellite coordination, satellite-launcher coordination, batch deployment, orbital control, and the passivation and deorbiting of the rocket's end stage, placing higher demands on coordination throughout the entire mission.

"For this mission, we have conducted system-level preparations in areas such as satellite interfaces, flight procedures, multi-satellite deployment sequencing, ground testing and launch procedures, and have carried out extensive work of collaboration with the client. We aim to standardize, formalize and visualize such constellation deployment missions," said Ma Haijing, general manager of LandSpace's marketing department.

China's low-Earth orbit satellite Internet sector is entering a phase of large-scale network deployment, and the continued construction of large satellite constellations is placing higher demands on the reliability, launch frequency, and the sustained supply of launch capacity of carrier rockets.

"The Zhuque-2 series has completed nine flights. Today's mission successfully deployed 10 networking satellites at an altitude of 900 kilometers with high precision, demonstrating that the Zhuque-2E's payload capacity, propulsion system, stage separation technology and orbital insertion precision control have all reached industry-leading levels," said Ma after Tuesday's launch.

While advancing routine commercial launches with the Zhuque-2E, LandSpace is also continuing its efforts to advance reuse of the Zhuque-3 reusable rocket. The two rocket models are being developed in tandem to meet distinct payload capacities and mission requirements, further enhancing the company's capability for sustained and stable access to space.

Costing under 10 million Yuan (1.47 million United States Dollars) apiece, each Qianfan satellite weighs 300 kilograms and has a ‘flat pack’ design with a single solar array to fit as many satellites as possible inside the rocket fairing in two parallel stacks. For maneuvering in orbit, each satellite has an electric hall-effect thruster burning krypton to generate 20 millinewtons of thrust with a specific impulse of 1,385 seconds.

By deploying ten Qianfan satellites, LandSpace has become the first of three enterprises contracted in August 2025 to fulfill its demonstration launch, beating CAS Space by about a month and far ahead of Space Pioneer. In the future, the company plans to deploy further satellite groups to assist with the constellation's growth towards having thousands in orbit.

Today’s mission was the 6th flight of Zhuque-2E, the 8th flight of LandSpace’s Zhuque-2 series, and LandSpace’s 11th orbital launch attempt. This was also the 63rd launch from China in 2026.


Video Credit: CCTV
Text Credit: CCTV, Jack C.
Duration: 1 minute
Release Date: Sept. 15, 2026

#NASA #Space #Science #Earth #Satellites #CommunicationsSatellites #SpaceSailConstellation #ShanghaiSpacesailTechnologies #CAS #Earth #LEO #China #中国 #LandSpace #蓝箭 #Zhuque2Rocket #Zhuque2EY7 #RocketLaunches #InnerMongolia #CommercialSpace #STEM #Education #HD #Video

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 lift off aboard a Vega-C rocket from Europe’s Spaceport in French Guiana.
The European Space Agency's FLEX Earth Explorer satellite and the Copernicus Sentinel-3C satellite lift off aboard a Vega-C rocket from Europe’s Spaceport in French Guiana.
The European Space Agency's FLEX Earth Explorer satellite and the Copernicus Sentinel-3C satellite lift off aboard a Vega-C rocket from Europe’s Spaceport in French Guiana.
The Vega-C gantry is rolled back for the launch of the European Space Agency's FLEX satellite and the Copernicus Sentinel-3C satellite at Europe’s Spaceport in French Guiana.
European Space Agency's FLEX satellite and the Copernicus Sentinel-3C satellite within the rocket fairing after being rolled out to the launch pad at Europe’s Spaceport in French Guiana.
European Space Agency's FLEX satellite and the Copernicus Sentinel-3C satellite rolled out within the rocket fairing to the launch tower at Europe’s Spaceport in French Guiana
European Space Agency's FLEX satellite and the Copernicus Sentinel-3C satellite rolled out within the rocket fairing to the launch tower at Europe’s Spaceport in French Guiana
European Space Agency's FLEX satellite and the Copernicus Sentinel-3C satellite rolled out within the rocket fairing to the launch tower at Europe’s Spaceport in French Guiana

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 (September 14 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
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

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 (September 14 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