Friday, May 22, 2026

SpaceX Starship's Role in NASA's Artemis Moon Exploration Program

SpaceX Starship's Role in NASA's Artemis Moon Exploration Program


NASA plans to use a lunar lander version of Starship to deliver astronauts and cargo to the Moon's surface during the Artemis IV mission and beyond, starting with the Human Landing System (HLS) Program.

Learn more about Starship:

Download the Free Starship User Guide (PDF):

Credit: Space Exploration Technologies Corporation (SpaceX)
Duration: 3 minutes
Release Date: May 20, 2026

#NASA #SpaceX #Space #Earth #Mars #Moon #MoonToMars #ArtemisProgram #ArtemisIII #ArtemisIV #Starship #StarshipV3 #StarshipFlight12 #ReusableSpacecraft #SuperHeavy #SuperHeavyV3 #ElonMusk #Engineering #SpaceTechnology #HumanSpaceflight #CommercialSpace #SpaceExploration #StarbaseTexas #Texas #UnitedStates #STEM #Education #HD #Video

A Tour of The Crystal Ball Nebula | NOIRLab

A Tour of The Crystal Ball Nebula | NOIRLab

The 8.1-meter Gemini North telescope, located on the summit of Maunakea in Hawai‘i, has captured NGC 1514, nicknamed the Crystal Ball Nebula, in awe-inspiring detail. This nebula, with its mesmerizing glow of gas, harbors hints of a past stellar death, and its asymmetrical shell is now being shaped by the binary pair that lies at its center.

NGC 1514 lies in the Taurus constellation approximately 1,500 light-years from Earth.

Gemini North is one half of the International Gemini Observatory, partly funded by the U.S. National Science Foundation (NSF) and operated by NSF NOIRLab.


Credit:
Images and Videos: 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), D. de Martin & M. Zamani (NSF NOIRLab)
Motion Graphics: Mik Garrison
Duration: 1 minute, 19 seconds
Release Date: May 22, 2026


#NASA #Astronomy #Space #Science #Stars #Nebulae #PlanetaryNebulae #NGC1514 #CrystalBallNebula #TaurusConstellation #Cosmos #Universe #InternationalGeminiObservatory #GeminiNorthTelescope #GMOS #Maunakea #Hawaii #NOIRLab #NSF #AURA #UnitedStates #STEM #Education #HD #Video

Journey to The Crystal Ball Nebula—NGC 1514 in Taurus | Gemini North Telescope

Journey to The Crystal Ball NebulaNGC 1514 in Taurus | Gemini North Telescope

The 8.1-meter Gemini North telescope, located on the summit of Maunakea in Hawai‘i, has captured NGC 1514, nicknamed the Crystal Ball Nebula, in awe-inspiring detail. This nebula, with its mesmerizing glow of gas, harbors hints of a past stellar death, and its asymmetrical shell is now being shaped by the binary pair that lies at its center. It was discovered by William Herschel on November 13, 1790. This planetary nebula has been studied by astronomers since the late 1700s. Astronomer William Herschel noted that NGC 1514 was the first deep sky object to appear genuinely cloudy—he could not resolve what he saw into individual stars within a cluster, like other objects he cataloged.

NGC 1514 lies in the Taurus constellation approximately 1,500 light-years from Earth.

Gemini North is one half of the International Gemini Observatory, 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), D. de Martin & M. Zamani (NSF NOIRLab)
Duration: 1 minute
Release Date: May 21, 2026


#NASA #Astronomy #Space #Science #Stars #Nebulae #PlanetaryNebulae #NGC1514 #CrystalBallNebula #TaurusConstellation #Cosmos #Universe #InternationalGeminiObservatory #GeminiNorthTelescope #GMOS #Maunakea #Hawaii #NOIRLab #NSF #AURA #UnitedStates #STEM #Education #HD #Video

Close-up: The Crystal Ball Nebula—NGC 1514 in Taurus | Gemini North Telescope

Close-up: The Crystal Ball NebulaNGC 1514 in Taurus | Gemini North Telescope

The 8.1-meter Gemini North telescope, located on the summit of Maunakea in Hawai‘i, has captured NGC 1514, nicknamed the Crystal Ball Nebula, in awe-inspiring detail. This nebula, with its mesmerizing glow of gas, harbors hints of a past stellar death, and its asymmetrical shell is now being shaped by the binary pair that lies at its center. It was discovered by William Herschel on November 13, 1790. This planetary nebula has been studied by astronomers since the late 1700s. Astronomer William Herschel noted that NGC 1514 was the first deep sky object to appear genuinely cloudy—he could not resolve what he saw into individual stars within a cluster, like other objects he cataloged.

NGC 1514 lies in the Taurus constellation approximately 1,500 light-years from Earth.

Gemini North is one half of the International Gemini Observatory, 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), D. de Martin & M. Zamani (NSF NOIRLab)
Duration: 30 seconds
Release Date: May 21, 2026


#NASA #Astronomy #Space #Science #Stars #Nebulae #PlanetaryNebulae #NGC1514 #CrystalBallNebula #TaurusConstellation #Cosmos #Universe #InternationalGeminiObservatory #GeminiNorthTelescope #GMOS #Maunakea #Hawaii #NOIRLab #NSF #AURA #UnitedStates #STEM #Education #HD #Video

Shenzhou-23 Crewed Spacecraft Ready for Launch | China Space Station

Shenzhou-23 Crewed Spacecraft Ready for Launch | China Space Station

The Shenzhou-23 crewed space mission conducted its last comprehensive practice before launch on Friday, May 22, 2026, completing function checks of all systems and other preparation work.

The combination of the spaceship and a Long March-2F carrier rocket was transported to the launch site last Saturday and is scheduled for launch in the coming days, with all facilities and equipment at the launch site in good condition, according to the China Manned Space Agency (CMSA).

Carried out by the Jiuquan Satellite Launch Center, the Xi'an Satellite Control Center, and various control stations under the coordination of the Beijing Aerospace Flight Control Center, the drill simulated all stages of the launch mission, including pre-launch preparations, liftoff, climb, and the in-orbit phase.

"The joint practice is to test the system's communication links, command capability, equipment, and personnel. Based on the current progress, everything is normal. What's going on in parallel is a full-system gas leak detection," He said.

The rehearsal validated the reliability of key systems, including the rocket, the spacecraft, the launch site, the control and communication equipment, and the coordination between different systems. It also verified the functionality and technical status of the Shenzhou-23 spacecraft-rocket combination.

"The Shenzhou-23 spacecraft is in the third batch of spacecraft after the completion of the construction of the space station. It incorporates many new quality control measures, and its payload transport capacity, reliability, and safety have all been significantly improved," said Li Zhe, an employee of the China Aerospace Science and Technology Corporation.

With all facilities in good condition, the Jiuquan launch site will later conduct rocket propellant filling and launch operations.

Search and recovery drills are also underway at the landing site, in preparation for the return of the Shenzhou-21 crew.


Video Credit: CCTV
Duration: 1 minute
Release Date: May 22, 2026

#NASA #Space #Science #China #中国 #CASC #JSLC #LongMarch2FRocket #Shenzhou23Mission #神舟二十三号 #Shenzhou23 #Taikonauts #Astronauts #LongDurationMissions #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #MicrogravityExperiments #SpaceLaboratory #CNSA #国家航天局 #HumanSpaceflight #STEM #Education #HD #Video

The Crystal Ball Nebula: NGC 1514 in Taurus | Gemini North Telescope

The Crystal Ball Nebula: NGC 1514 in Taurus | Gemini North Telescope

The 8.1-meter Gemini North telescope, located on the summit of Maunakea in Hawai‘i, has captured NGC 1514, nicknamed the Crystal Ball Nebula, in awe-inspiring detail. This nebula, with its mesmerizing glow of gas, harbors hints of a past stellar death, and its asymmetrical shell is now being shaped by the binary pair that lies at its center. It was discovered by William Herschel on November 13, 1790. This planetary nebula has been studied by astronomers since the late 1700s. Astronomer William Herschel noted that NGC 1514 was the first deep sky object to appear genuinely cloudy—he could not resolve what he saw into individual stars within a cluster, like other objects he cataloged.

NGC 1514 lies in the Taurus constellation approximately 1,500 light-years from Earth.

Gemini North is one half of the International Gemini Observatory, 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), D. de Martin & M. Zamani (NSF NOIRLab)
Release Date: May 21, 2026


#NASA #Astronomy #Space #Science #Stars #Nebulae #PlanetaryNebulae #NGC1514 #CrystalBallNebula #TaurusConstellation #Cosmos #Universe #InternationalGeminiObservatory #GeminiNorthTelescope #GMOS #Maunakea #Hawaii #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

Thursday, May 21, 2026

'Underground Tunnels' Observe the Universe | European Southern Observatory

'Underground Tunnels' Observe the Universe | European Southern Observatory


Larger telescopes allow us to see smaller details, and thanks to interferometry we can link multiple telescopes into a single “virtual” one that can make very sharp observations. How does this actually work? 

Follow us on an exclusive tour of the underground tunnels beneath the European Southern Observatory’s Very Large Telescope Interferometer (VLTI) in Chile, and learn about the technology that has allowed us to see details on the surface of distant stars, and track the orbits of stars around the supermassive black hole at the center of our galaxy.

0:00 - Introduction

0:59 - Arranging the telescopes

3:50 - Radio vs infrared interferometry

5:09 - Synchronizing the light beams

7:09 - From fringes to images

9:43 - What has the VLTI found?


Video Credit: European Southern Observatory (ESO)
Duration: 11 minutes
Release Date: May 21, 2026

#NASA #ESO #Space #Astronomy #Science #Cosmos #Universe #Chile #Telescopes #Europe #ParanalObservatory #VLTI #Chile #Europe #STEM #Education #HD #Video

Did you know the Moon has “tan lines”? | NASA's Lunar Reconnaissance Orbiter

Did you know the Moon has “tan lines”? | NASA's Lunar Reconnaissance Orbiter

😎 These tan lines feature bright tendrils and swirls amid darkened areas. They are caused by the Sun. However, this is only half of the story. These space weathered patches also give us clues as to what is going on below the lunar surface. 

Reiner Gamma is a geographical feature of the Moon known as a lunar swirl. It is one of the most visible lunar swirls from Earth, visible from most telescopes.

 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
Duration: 1 minute, 25 seconds
Release Date: May 21
, 2026

#NASA #Space #Astronomy #Science #SolarSystem #Sun #Moon #SpaceWeather #Geology #Geoscience #LunarSwirls #ReinerGamma #LROC #NAC #WAC #SpaceRobotics #SpaceTechnology #NASAGoddard #GSFC #ASU #UnitedStates #SolarSystem #SpaceExploration #STEM #Education #HD #Video

SpaceX Starship (Version 3) 12th Flight Test: Pre-launch | Starbase Texas

SpaceX Starship (Version 3) 12th Flight Test: Pre-launch | Starbase Texas





Go Starship! Go SpaceX! The 12th flight test of SpaceX's Starship is preparing to launch as soon as today, Thursday, May 21, 2026, from Pad 2 at Starbase, Texas. The 90-minute launch window opens at 5:30 p.m. Central Time (CT).

Learn about today's flight test objectives here: 
https://www.spacex.com/launches/starship-flight-12
A live webcast of the flight test will begin about 45 minutes before liftoff. Watch here:
https://www.spacex.com/launches/starship-flight-12

As is the case with all developmental testing, the schedule is dynamic and likely to change, so stay tuned for updates.

Today's flight will debut the next generation Starship and Super Heavy vehicles, powered by the next evolution of the Raptor engine. Read more about the key upgrades designed to enhance performance and unlock Starship's full capabilities here: https://www.spacex.com/updates/starship-v3

As of October 13, 2025, the SpaceX Starship has been "launched 11 times with 6 successes and 5 failures." SpaceX has developed Starship with the intention of lowering launch costs using economies of scale. It aims to achieve this by reusing both rocket stages, increasing payload mass to orbit, increasing launch frequency, creating a mass-manufacturing pipeline and adapting it to a wide range of space missions.

NASA plans to use a lunar lander version of Starship for landing astronauts on the Moon during the Artemis IV mission through the Human Landing System (HLS) program.

Learn more about Starship:

Download the Free Starship User Guide (PDF):

Credit: Space Exploration Technologies Corporation (SpaceX)
Release Date: May 20, 2026

#NASA #SpaceX #Space #Earth #Mars #Moon #MoonToMars #ArtemisProgram #ArtemisIII #ArtemisIV #Starship #StarshipV3 #StarshipFlight12 #ReusableSpacecraft #SuperHeavy #SuperHeavyV3 #ElonMusk #Engineering #SpaceTechnology #HumanSpaceflight #CommercialSpace #SpaceExploration #StarbaseTexas #Texas #UnitedStates #STEM #Education

Astronaut Rescue Team Protects Shenzhou-23 Crew | China Space Station

Astronaut Rescue Team Protects Shenzhou-23 Crew | China Space Station

China conducted a complete system rehearsal for the launch of its Shenzhou-23 crewed spacecraft at the Jiuquan Satellite Launch Center on May 20, 2026, with the astronaut emergency evacuation team working as the last safety barrier during the pre-launching stage.

The rehearsal included exercises in launch preparations, ignition, and rocket-spacecraft separation.

The combination of the spacecraft and a Long March-2F carrier rocket was transferred to the launching area on Saturday and is scheduled for launch in the coming days with all facilities and equipment at the launch site in good condition, according to the China Manned Space Agency (CMSA).

The astronaut emergency evacuation team at the launch center is primarily responsible for emergency sheltering, evacuation, and safe transfer of astronauts during the pre-launching stage, serving as the final safeguard for astronauts' lives.

As the Shenzhou-23 mission enters its launching stage, the launch center conducted a realistic emergency evacuation support rehearsal for astronauts.

"Simulated astronaut NO.1 ready, prepare, jump," said an astronaut emergency evacuation team member.

The rehearsal closely simulated real mission scenarios. The team members, dressed neatly, responded swiftly with clear division of labor, taking positions quickly according to the established plan.

From rapidly donning protective gear and accurately assessing evacuation conditions, to operating the escape slide and explosion-proof elevator, and then simulating emergency shelter on the tower and orderly evacuation, the entire sequence was smooth, standardized, precise and efficient.

As the final safety barrier during the rocket pre-launching stage, the team remained on duty until the mission successfully commenced.

"For the Shenzhou-23 mission, we routinely conduct full-process, full-element multi-level backup evacuation rehearsals, refining every support detail. We have mastered various evacuation support methods based on the tower structure and mission preparation plans. All training and plans are thoroughly prepared and ready for use, aiming to build a safety assurance system that guarantees 100 percent astronaut safety," said Zhang Zhixu, astronaut emergency evacuation team member.

To achieve full safety coverage, the team has established a complete safety chain: "primary shelter on the tower and secondary evacuation from shelter rooms."

The two backup evacuation modes each have their advantages and complement each other.

The escape slide backup mode is suited for rapid response scenarios, offering high efficiency and independence from power equipment, the explosion-proof elevator backup mode is suited for routine, stable scenarios, enabling orderly and secure evacuation.

Based on routine tower shelter standby, the team has also preset secondary evacuation procedures from shelter rooms, solidifying the mission's safety foundation from all aspects.

"Based on daily rehearsals, we simulate various emergency scenarios in real environments, iteratively improve our plans, and conduct precise evacuation training. We ensure all team members memorize procedures, standardize actions, and always align rehearsals with the conditions. We thoroughly understand the routes and processes. It's better to be prepared and not need it than to need it and not be prepared," Zhang said.

To perfect the ultimate backup support of the safety shelter rooms, the team has formulated two standardized long-distance backup evacuation plans: exiting the shaft to the technical area, and evacuating along the cable corridor to the technical area. The two routes are set up simultaneously and serve as backups for each other.

"All our team members have completed multiple rounds of specialized joint rehearsals and full-process rehearsals. All personnel, equipment, and emergency response plans are in optimal readiness. We will always stand guard at the final safety checkpoint, successfully complete the emergency evacuation support tasks during the pre-launching stage, and do our utmost to ensure the safety of the astronauts," Zhang said.


Video Credit: CCTV
Duration: 2 minutes, 31 seconds
Release Date: May 21, 2026

#NASA #Space #Science #China #中国 #CASC #JSLC #LongMarch2FRocket #Shenzhou23Mission #神舟二十三号 #Shenzhou23 #Taikonauts #Astronauts #LongDurationMissions #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #MicrogravityExperiments #SpaceLaboratory #CNSA #国家航天局 #HumanSpaceflight #STEM #Education #HD #Video

The Flame Nebula in Orion (visible light)

The Flame Nebula in Orion: Wide-field view in visible light

This is the Flame Nebula in visible light. The bright star above it is Alnitak. The nebulae to the upper left of it are IC 431 and IC 432.

The Flame Nebula lies in the Orion Molecular Cloud Complex and is home to cosmic objects, called brown dwarfs, that are not quite planets, but are also so small their cores cannot sustain fusing hydrogen like full-fledged stars do.

Distance from Earth: 1350 light years


Image Details:
Imaging Telescope: Celestron RASA (400 focal length)
Focuser: Celestron Electronic Focuser
Mount: Sky-Watcher EQ6-R Pro
Imaging Camera: ZWO ASI533MC Color
Total Exposure Time: 9.39 hours

Image Credit: Chuck Ayoub
Release Date: March 4, 2025

#NASA #Astronomy #Space #Science #Nebulae #Nebula #EmissionNebulae #FlameNebula #NGC2024 #Sh2277 #IC431 #IC432 #Stars #Alnitak #BrownDwarfs #OrionConstellation #Cosmos #Universe #Astrophotographers #ChuckAyoub #Astrophotography #STEM #Education

The Flame Nebula in Orion | Webb Telescope & Chandra X-ray Observatory

The Flame Nebula in Orion | Webb Telescope & Chandra X-ray Observatory


The Flame Nebula image features Chandra’s X-rays (purple) embedded within a dusty-grey landscape seen in infrared by James Webb. Several dozen young stars illuminate the gas cloud, appearing as white cores surrounded by thick, neon purple-pink X-ray halos. This image captures the "stellar soil" of a region where stars are currently forming and beginning their life cycles.

The Flame Nebula lies in the Orion Molecular Cloud Complex and is home to cosmic objects, called brown dwarfs, that are not quite planets, but are also so small their cores cannot sustain fusing hydrogen like full-fledged stars do.

Distance from Earth: 1350 light years


Credit: X-ray: NASA/CXC/PSU/K. Getman, E. Feigelson, M. Kuhn & the MYStIX team; JWST Image: NASA, ESA, CSA, STScI, M. Meyer (University of Michigan), M. De Furio (UT Austin), M. Robberto (STScI), A. Pagan (STScI)
Image Processing: NASA/CXC/SAO/L. Frattare
Release Date: May 15, 2026


#NASA #ESA #Astronomy #Space #Science #JWST #JamesWebb #WebbTelescope #Nebulae #Nebula #FlameNebula #NGC2024 #Stars #BrownDwarfs #OrionConstellation #Cosmos #Universe #JWST #InfraredAstronomy #NASAChandra #XrayAstronomy #SpaceTelescopes #ESA #CSA #GSFC #STScI #CXC #UnitedStates #STEM #Education

Wednesday, May 20, 2026

NASA's Artemis II Moon Crew Visits the U.S. Capitol

NASA's Artemis II Moon Crew Visits the U.S. Capitol

On May 12, 2026, NASA astronauts Christina Koch, Reid Wiseman, and Victor Glover, and Canadian Space Agency (CSA) astronaut Jeremy Hansen visited Capitol Hill in Washington, D.C., where they met U.S. senators and representatives and spoke about their historic mission around the Moon.

NASA's Artemis II Mission took Wiseman, Glover, Koch, and Hansen on a nearly 10-day journey around the Moon and back to Earth.

The Orion spacecraft successfully splashed down on Friday, April 10, 2026, in the Pacific Ocean following its journey around the Moon.

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

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

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

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


Credit: NASA
Duration: 1 minute
Release Date: May 20, 2026


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

Wide-field view: The Pleiades Star Cluster | Australian Astronomical Observatory

Wide-field view: The Pleiades Star Cluster | Australian Astronomical Observatory

The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years away in the direction of the northern constellation of Taurus. A handful of the brightest stars cluster together in space and have been recognized as a group since ancient times. However, even the brightest of the Pleiades stars (Alcyone, apparent visual mag +2.9) is relatively faint and would be inconspicuous (and nameless) if it were not a member of the cluster The faintest named star is Asterope, (V = +5.8), close to the threshold of naked eye visibility. All the visible stars of the Pleiades are in reality much more luminous than the Sun.

The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust this cluster has drifted into. It appears blue because these tiny motes of interstellar dust scatter blue light more efficiently than the longer wavelengths of red light, and it is streaky because of the distribution of dust particles in space. Care has been taken to ensure that the colors visible here are realistic.

In western literature and legend, the stars bear the names of the Seven Sisters, the daughters of Atlas and Pleone. They were also half-sisters to the goddesses of the nearby Hyades stars. The delicate beauty of the stars identified them as a group of women in many cultures, from Australian Aborigine to Native American. To the Japanese they are 'Subaru', a conglomerate or collection (i.e. cluster), while Chinese legends refer to a swarm of bees. Maori and Pacific Islands people often called the Pleiades 'Matariki', the star cluster that heralds the start of the Maori New Year.

Photograph made from plates taken in 1983 October (G) and December (B, R). Image width is about 3.5 degrees.


Image Credit: David Malin
Copyright: Australian Astronomical Observatory
Release Date: April 15,
2000

#NASA #Space #Astronomy #Science #Nebulae #ReflectionaNebulae #Stars #StarClusters #ThePleiades #SevenSisters #Messier45 #M45 #OpenStarCluster #BrownDwarfStars #TaurusConstellation #Cosmos #Universe #Astronomers #DavidMalin #AustralianAstronomicalObservatory #Australia #STEM #Education

The Pleiades Star Cluster in Taurus | Australian Astronomical Observatory

The Pleiades Star Cluster in Taurus | Australian Astronomical Observatory

The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years away in the direction of the northern constellation of Taurus. A handful of the brightest stars cluster together in space and have been recognized as a group since ancient times. However, even the brightest of the Pleiades stars (Alcyone, apparent visual mag +2.9) is relatively faint and would be inconspicuous (and nameless) if it were not a member of the cluster The faintest named star is Asterope, (V = +5.8), close to the threshold of naked eye visibility. All the visible stars of the Pleiades are in reality much more luminous than the Sun.

The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust this cluster has drifted into. It appears blue because these tiny motes of interstellar dust scatter blue light more efficiently than the longer wavelengths of red light, and it is streaky because of the distribution of dust particles in space. Care has been taken to ensure that the colors visible here are realistic.

In western literature and legend, the stars bear the names of the Seven Sisters, the daughters of Atlas and Pleone. They were also half-sisters to the goddesses of the nearby Hyades stars. The delicate beauty of the stars identified them as a group of women in many cultures, from Australian Aborigine to Native American. To the Japanese they are 'Subaru', a conglomerate or collection (i.e. cluster), while Chinese legends refer to a swarm of bees. Maori and Pacific Islands people often called the Pleiades 'Matariki', the star cluster that heralds the start of the Maori New Year.

Photograph made from plates taken in October 1983 (G) and December (B, R). Image width is about 100 arc min.


Image Credit: David Malin
Copyright: Australian Astronomical Observatory
Date: Aug. 17, 1984

#NASA #Space #Astronomy #Science #Nebulae #ReflectionaNebulae #Stars #StarClusters #ThePleiades #SevenSisters #Messier45 #M45 #OpenStarCluster #BrownDwarfStars #TaurusConstellation #Cosmos #Universe #Astronomers #DavidMalin #AustralianAstronomicalObservatory #Australia #STEM #Education

Distant Irregular Galaxy NGC 2719 & Companion in Lynx | Hubble Space Telescope

Distant Irregular Galaxy NGC 2719 & Companion in Lynx | Hubble Space Telescope

NGC 2719 is a Magellanic irregular galaxy in the constellation of Lynx. A Magellanic spiral galaxy has only one spiral arm. The long galaxy is NGC 2719 and the smaller one is NGC 2719A. NGC 2719 was discovered by German-British astronomer William Herschel on March 28, 1786. Together with the galaxy NGC 2719A (also known as PGC 2528A), NGC 2719 is listed in Halton Arp's Atlas of Peculiar Galaxies as Arp 202. The galaxy pair is also listed as Holm 105 in Erik Holmberg's A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems, published in 1937.

Distance from Earth: ~159 million light-years

Image Processor Judy Schmidt: "They're an interacting pair, and the smaller one seems to have a rather long string of stars trailing it, visible at the lower right edge of the image. The stream itself is difficult to see, but does connect. Luckily, the stream just made it onto the detector. You can see a tiny sliver of a blank spot at the lower right corner."


Image Credit: NASA, ESA, Space Telescope Science Institute (STScI)
Processing: Judy Schmidt
Release Date: Sept. 15, 2025

#NASA #ESA #Hubble #Astronomy #Space #Science #Galaxies #InteractingGalaxies #NGC2719 #Arp202 #NGC2719A #PGC2528A #Holm105 #LynxConstellation #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #JudySchmidt #UnitedStates #Europe #STEM #Education