Wednesday, March 18, 2026

Fragmenting Comet C/2025 K1 (ATLAS): Animation | Hubble

Fragmenting Comet C/2025 K1 (ATLAS): Animation | Hubble

This animation steps through the three Hubble Space Telescope images of the fragmenting comet C/2025 K1 (ATLAS)], or K1 for short, taken consecutively on November 8, 9, and 10, 2025. Captured by Hubble’s Space Telescope Imaging Spectrograph (STIS) instrument, the sequence shows the progressive disintegration of the comet over the three-day period. This is the first time Hubble has witnessed a comet so early in the process of breaking up.

Hubble caught K1 fragmenting into at least four pieces, each with a distinct coma, the fuzzy envelope of gas and dust that surrounds a comet’s icy nucleus. Hubble cleanly resolved the fragments, but from the ground they only appeared at that time as barely distinguishable blobs. Hubble chronicled the sequence of events and showed exactly how the breakup happened.


Credit: NASA, ESA, D. Bodewits (Auburn), J. DePasquale (STScI)
Duration: 20 seconds
Release Date: March 18, 2026


#NASA #Astronomy #Hubble #Space #Science #Comets #Comet #CometaryComa #CometaryNuclei #C2025K1 #K1 #OortCloud #SolarSystem #Cosmos #Universe #HubbleSpaceTelescope #HST #STIS #GSFC #STScI #UnitedStates #ESA #Europe #Animation #STEM #Education #HD #Video 

An Archetypal Dwarf Galaxy: NGC 5477 in Ursa Major | Hubble

An Archetypal Dwarf Galaxy: NGC 5477 in Ursa Major | Hubble

The constellation of Ursa Major (The Great Bear) is home to Messier 101, the Pinwheel Galaxy. One of the biggest and brightest spiral galaxies in the night sky. Like the Milky Way, Messier 101 is not alone, with smaller dwarf galaxies in its neighborhood.

NGC 5477, one of these dwarf galaxies in the Messier 101 group, is the subject of this image from the NASA/European Space Agency Hubble Space Telescope. Without obvious structure, but with visible signs of ongoing starbirth, NGC 5477 looks much like an archetypal dwarf irregular galaxy. The bright nebulae that extend across much of the galaxy are clouds of glowing hydrogen gas in which new stars are forming. These glow pinkish red in real life, although the selection of green and infrared filters through which this image was taken makes them appear almost white.

Distance from Earth: 20 million light years

The observations were taken as part of a project to measure accurate distances to a range of galaxies within about 30 million light-years from Earth by studying the brightness of red giant stars.

In addition to NGC 5477, the image has numerous galaxies in the background, including a number that are visible right through NGC 5477. This serves as a reminder that galaxies, far from being solid, opaque objects, are actually largely made up of the empty space between their stars.

This image is a combination of exposures taken through green and infrared filters using Hubble's Advanced Camera for Surveys. The field of view is approximately 3.3 by 3.3 arcminutes. 


Credit: ESA/Hubble & NASA
Release Date: Jan. 7, 2013


#NASA #ESA #Astronomy #Space #Science #Galaxies #DwarfGalaxies #NGC5477 #IrregularGalaxies #UrsaMajorConstellation #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education

Tuesday, March 17, 2026

NASA Artemis II Mission Crew: Into the Path of Solar Eruptions

NASA Artemis II Mission Crew: Into the Path of Solar Eruptions

For the first time in half a century, four astronauts are leaving Earth’s protective magnetic field. They will enter a realm where massive solar eruptions can unleash more energy than a billion hydrogen bombs.

The Artemis II crew will fly through a dangerous environment, but they are not going it alone. On the voyage, the astronauts and their Orion capsule are outfitted with radiation trackers as ground teams monitor solar eruptions 24/7. This is how NASA and the National Oceanic and Atmospheric Administration (NOAA) are protecting explorers from the most powerful eruptions in the solar system. 🛡️

The Artemis II test flight will take Commander Reid Wiseman, Pilot Victor Glover, and Mission Specialist Christina Koch from NASA and Mission Specialist Jeremy Hansen from the Canadian Space Agency (CSA), around the Moon and back to Earth 

Artemis II will pave the way for new U.S. crewed missions on the lunar surface in preparation to send the first astronauts to Mars.

NASA Artemis II Mission updates:
https://www.nasa.gov/mission/artemis-ii/

Artemis Program blog: 

Video Credit: NASA/Joy Ng
Duration: 1 minute, 32 seconds
Release Date: March 16, 2026

#NASA #Space #Science #Earth #Moon #ArtemisIIMission #SolarRadiation #AstronautHealth #OrionSpacecraft #SLS #SLSRocket #CrewedMissions #DeepSpace #MoonToMars #Engineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NASAGoddard #UnitedStates #CSA #Canada #STEM #Education #HD #Video

China's Commercial Satellites Drive Major Changes in Daily Life

China's Commercial Satellites Drive Major Changes in Daily Life

China's commercial satellites have become invisible, essential infrastructure in daily life, driving major changes by helping tracking crops in farmland, inspecting infrastructure, and support a growing range of services on the ground. 

The outline of the 15th Five-Year Plan (2026-2030), China's latest five-year blueprint that was adopted on Thursday, March 12, 2026, designated aerospace as one of the strategic emerging industries for priority development.

Among the companies driving the growth China's space sector is Changguang Satellite Technology Co., Ltd. in northeast China's Jilin Province. It has evolved from a research institute into a market-driven commercial space leader.

The company's Jilin-1 constellation had its first group of satellites launched back in October 2015. It now consists of 144 satellites and is capable of observing any point on the globe about forty times a day.

Despite these achievements, the company has continued to push for technological innovation, reducing satellite weight while maintaining imaging performance.

"Our Gaofen-06 satellites, along with the Magic Cube and Platform series, weigh about 20 kilograms at the lowest, while their imaging performance remains largely comparable to earlier satellites that weighed more than 400 kilograms," said Zhao Xiangyu, deputy director of the company's Microwave Satellite Research Laboratory.

The Jilin-1 constellation has increasingly integrated into daily life and industrial development. Its high-resolution data supports multiple sectors, from protecting farmland to monitoring urban expansion, bringing tangible changes to people's lives.

"Some projects, such as wind turbines and photovoltaic facilities, are built in remote mountainous areas. Supervising them manually would require significant manpower and efforts. What makes supervision possible today is Jilin-1's ability to frequently obtain large-scale data over vast areas," said Yang Hongwei, director of the Survey and Mapping Division at the Department of Natural Resources of Jilin.

As the 15th Five-Year Plan highlights the development of the space sector, Changguang is accelerating its expansion.

Inside a high-level clean workshop, satellites are being mass-produced. Beyond remote sensing, the company has also expanded into the communications satellite field, achieving technological breakthroughs in low-Earth-orbit satellite internet.

"(In the future research and development,) we aim to combine the technical challenges of traditional remote-sensing satellites with those of high-orbit communications satellites, while also meeting the requirements of modern communications services. These are the key challenges we are working to overcome," said Zhu Ruifei, the company's deputy chief engineer.


Video Credit: CCTV
Duration: 1 minute, 43 seconds
Release Date: March 17, 2026

#NASA #Space #Planets #Earth #Satellites #SatelliteConstellations #CommunicationSatellites #SatelliteCommunications #RemoteSensing #EarthObservation #Agriculture #DisasterPrevention #InfrastructureInspections #China #中国 #Aerospace #Gaofen06Satellites #MicrowaveSatelliteResearchLaboratory #ChangguangSatelliteTechnology #Jilin1 #Jilin #CommercialSpace #STEM #Education #HD #Video

U.S. Spacewalk 95 Animation Preview for March 18, 2026 | International Space Station

U.S. Spacewalk 95 Animation Preview for March 18, 2026 | International Space Station

An animation of U.S. spacewalk 95 when two NASA astronauts will prepare the 3B power channel for future installation of International Space Station Roll-Out Solar Arrays (IROSA) that will provide additional power ahead of a safe and controlled space station deorbit. This animation was narrated by flight director Ronak Dave.

A spacewalk by NASA astronauts Jessica Meir and Chris Williams is scheduled for Wednesday, March 18, 2026, at the International Space Station. The team has reviewed the spacewalking tools and tasks necessary to install a modification kit and route cables on the port side of the orbital outpost.

On her first spaceflight, Jessica Meir completed the first three all-woman spacewalks with fellow NASA astronaut Christina Koch, totaling 21 hours and 44 minutes outside of the station.

NASA Astronaut/Dr. Jessica Meir's Biography:
https://www.nasa.gov/people/jessica-u-meir/


Expedition 74 Crew
Station Commander: Sergey-Kud Sverchkov (Russia)
Roscosmos (Russia) Flight Engineers: 
Andrey Fedyaev, Sergei Mikaev
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jessica Meir, Jack Hathaway, Chris Williams

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
Duration: 4 minutes
Release Date: March 17, 2026

#NASA #Space #ISS #Planets #Earth #Spacewalks #EVAs #Spacewalk95 #Astronauts #JessicaMeir #ChrisWilliams #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #JSC #UnitedStates #STEM #Education #Animation #HD #Video

NASA Artemis II Mission: How to Train for The Moon | Johnson Space Center

NASA Artemis II Mission: How to Train for The Moon | Johnson Space Center

Before the Artemis II crew journeys to the Moon inside the Orion spacecraft, they will spend countless hours practicing every aspect of their mission. At NASA’s Johnson Space Center, the Artemis II crew trains inside Orion simulators to practice procedures, troubleshoot malfunctions, and work through realistic mission scenarios. This training ensures the astronauts and flight control team are ready to operate Orion’s systems and respond to any challenge during the 10-day flight.

From learning the fundamentals of Orion’s life support systems to conducting integrated simulations with flight controllers, every training session helps ensure mission success. Using Johnson’s full-scale Orion mockup in the Space Vehicle Mockup Facility and simulators like the Orion Mission Simulator and the Beta Dome, the crew is prepared for any scenario they may encounter aboard Orion during Artemis II. 

This is how to train for the Moon.

The Artemis II test flight will take Commander Reid Wiseman, Pilot Victor Glover, and Mission Specialist Christina Koch from NASA and Mission Specialist Jeremy Hansen from the Canadian Space Agency (CSA), around the Moon and back to Earth 

Artemis II will pave the way for new U.S. crewed missions on the lunar surface in preparation to send the first astronauts to Mars.

NASA Artemis II Mission updates:
https://www.nasa.gov/mission/artemis-ii/

Artemis Program blog: 

Credit: NASA's Johnson Space Center
Writer: Erika Peters
Editor: Phil Sexton
Producers: Rad Sinyak, Erika Peters
Duration: 4 minutes, 36 seconds
Release Date: March 17, 2026

#NASA #Space #Science #Earth #Moon #ArtemisProgram #ArtemisII #OrionSpacecraft #SLS #SLSRocket #CrewedMissions #Astronauts #DeepSpace #MoonToMars #Engineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #JSC #Houston #Texas #UnitedStates #CSA #Canada #STEM #Education #HD #Video

The 'Tadpoles' of Star Forming Region IC 410 in Auriga

The 'Tadpoles' of Star Forming Region IC 410 in Auriga

Emission nebula IC 410 lies around 10,000 light-years away, toward the nebula-rich constellation Auriga. It is nicknamed the Tadpole Nebula because of the tadpole-shaped clouds of dark dust that appear to be swimming towards the center. The Tadpole Nebula is a region of ionized hydrogen gas spanning over 100 light years across.

This telescopic close-up shows off the central regions of otherwise faint IC 410, captured under backyard skies. Presented in a Hubble color palette, the image combines visible broadband and narrowband data with data from the near-infrared. Below and right of center are two remarkable inhabitants of the interstellar pond of gas and dust. the Tadpoles of IC 410. Partly obscured by foreground dust, the nebula itself surrounds NGC 1893, a young galactic cluster of stars. Formed in the interstellar cloud a mere 4 million years ago, the intensely hot, bright cluster stars energize the glowing gas. However, the cosmic tadpoles themselves are composed of denser cooler gas and dust. Around 10 light-years long they are likely sites of ongoing star formation. Sculpted by stellar winds and radiation their heads are outlined by bright ridges of ionized gas while their tails trail away from the cluster's central young stars. 


Image Credit & Copyright: Nico Carver
Nico's website:

#NASA #Astronomy #Space #Science #Nebulae #IC410 #EmissionNebulae #StarCluster #NGC1893 #AurigaConstellation #MilkyWayGalaxy #Universe #Astrophotography #NicoCarver #Astrophotographer #GSFC #STEM #Education #APoD

Colorful Glows: Aurora & Milky Way Galaxy over Australia

Colorful Glows: Aurora & Milky Way Galaxy over Australia

This is a view of the Aurora Australis and our Milky Way Galaxy in southern Australia near the town of Tarlee.

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/

Image Credit: Ian Inverarity
Location: Tarlee, South Australia, Australia
Date: May 11, 2024


#NASA #Astronomy #Space #Science #Planets #Earth #Aurora #AuroraAustralis #SouthernLights #Stars #MilkyWayGalaxy #Cosmos #Universe #CitizenScience #IanInverarity #Astrophotographer #Astrophotography #SolarSystem #Tarlee #SouthAustralia #Australia #STEM #Education

The Pinwheel Galaxy in Ursa Major: Wide-field view | Digitized Sky Survey 2

The Pinwheel Galaxy in Ursa Major: Wide-field view | Digitized Sky Survey 2

This two-color image shows 3.7 x 2.7 degrees of the surroundings around the Pinwheel Galaxy, also known as Messier 101 (M101). It was composed from Digitized Sky Survey 2 images.

Distance from Earth: 25 million light-years 

The giant spiral disk of stars, dust, and gas is 170,000 light-years across—nearly twice the diameter of our galaxy, the Milky Way. Astronomers estimate that M101 contains at least one trillion stars. The galaxy’s spiral arms are sprinkled with large regions of star-forming nebulas. These nebulas are areas of intense star formation within giant molecular hydrogen clouds. Brilliant, young clusters of hot, blue, newborn stars trace out the spiral arms.

Pierre Méchain, one of Charles Messier’s colleagues, discovered the Pinwheel galaxy in 1781. Located in the constellation Ursa Major, M101 has an apparent magnitude of 7.9. It can be spotted through a small telescope and is most easily observed during June.

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 through its Guide Star Survey group.


Credit: ESA/Hubble and Digitized Sky Survey 2
Acknowledgements: Davide De Martin (ESA/Hubble)
Release Date: Feb. 28, 2006


#NASA #ESA #Astronomy #Space #Science #Galaxies #SpiralGalaxies #Messier101 #M101 #PinwheelGalaxy #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #DSS2 #STScI #UnitedStates #STEM #Education

Monday, March 16, 2026

Shenzhou-21 Astronauts Complete Second Series of Spacewalks | China Space Station

Shenzhou-21 Astronauts Complete Second Series of Spacewalks | China Space Station

The Shenzhou-21 crew aboard China's orbiting space station completed their mission's second series of extravehicular activities (EVAs) on March 16, 2026, according to the China Manned Space Agency (CMSA).

The astronaut trio—Zhang Lu, Wu Fei and Zhang Hongzhang—worked for roughly seven hours and completed their tasks at 19:35 (Beijing Time), assisted by the space station's robotic arm and a team on Earth.

Zhang Lu has so far carried out six EVAs, making him one of the Chinese astronauts with the most spacewalks to date.

The trio completed the installation of a space debris protection device for the space station along with other tasks. Zhang Lu and Wu Fei, who have conducted spacewalk operations, returned to the Wentian lab module safely, according to the CMSA.

Since completing the first series of EVAs on Dec. 9, 2025, the Shenzhou-21 crew has carried out equipment inspection and maintenance, environmental monitoring, and health management aboard the space station. The crew members have also conducted in-orbit training exercises, including rendezvous and docking, medical rescue, and emergency lifesaving.

The scientific experiment and test projects they undertook, covering space life science and human research, microgravity physics, and new space technologies, have been progressing steadily. They also celebrated the Spring Festival in Year of the Horse while in orbit.

The CMSA said the three astronauts have been working in orbit for more than four months. According to the mission plan, additional EVAs will be carried out by the crew during the Shenzhou-21 mission with relevant scientific experiments and technical tests continuing as scheduled.

Shenzhou-21 Crew
Zhang Lu (张陆) - Commander & Pilot - 2nd spaceflight
Wu Fei (武飞)  Flight Engineer - 1st spaceflight
Zhang Hong Zhang (张洪章) - Payload Specialist - 1st spaceflight


Video Credit: CCTV
Duration: 30 seconds
Release Date: March 17, 2026


#NASA #Space #Science #China #中国 #Shenzhou21Mission #神舟二十一号 #Shenzhou21 #Taikonauts #Astronauts #EVA #Spacewalks #ZhangLu #WuFei #ZhangHongzhang #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #MicrogravityExperiments #SpaceLaboratory #CNSA #国家航天局 #HumanSpaceflight #STEM #Education #HD #Video

The Pinwheel Galaxy: M101 in Ursa Major | Hubble, Spitzer & Chandra Telescopes

The Pinwheel Galaxy: M101 in Ursa Major | Hubble, Spitzer & Chandra Telescopes

This image of the spiral galaxy Messier 101 is a composite of views from the Spitzer Space Telescope, Hubble Space Telescope, and Chandra X-ray Observatory. Each wavelength region shows aspects of celestial objects and often reveals new objects that could not otherwise be studied. The red color shows Spitzer's view in infrared light. It highlights the heat emitted by dust lanes in the galaxy where stars can form. The yellow color is Hubble's view in visible light. Most of this light comes from stars, and they trace the same spiral structure as the dust lanes. The blue color shows Chandra's view in X-ray light. Sources of X-rays include million-degree gas, exploded stars, and material colliding around black holes. Such composite images allow astronomers to see how features seen in one wavelength match up with those seen in another wavelength. It is like seeing with a camera, night vision goggles, and X-ray vision all at once.

The giant spiral disk of stars, dust, and gas is 170,000 light-years across—nearly twice the diameter of our galaxy, the Milky Way. Astronomers estimate that M101 contains at least one trillion stars. The galaxy’s spiral arms are sprinkled with large regions of star-forming nebulas. These nebulas are areas of intense star formation within giant molecular hydrogen clouds. Brilliant, young clusters of hot, blue, newborn stars trace out the spiral arms.

Pierre Méchain, one of Charles Messier’s colleagues, discovered the Pinwheel galaxy in 1781. Located 25 million light-years away from Earth in the constellation Ursa Major, M101 has an apparent magnitude of 7.9. It can be spotted through a small telescope and is most easily observed during June.


Credit: NASA, ESA, CXC, SSC and STScI
Release Date: Feb. 10, 2009

#NASA #ESA #Astronomy #Space #Science #Galaxies #SpiralGalaxies #Messier101 #M101 #PinwheelGalaxy #Cosmos #Universe #NASASpitzer #InfraredAstronomy #NASAChandra #XrayAstronomy #HubbleSpaceTelescope #HST #SpaceTelescopes #Europe #GSFC #STScI #CXC #UnitedStates #STEM #Education

NASA Spacewalker Jessica Meir: Suit-up Practice | International Space Station

NASA Spacewalker Jessica Meir: Suit-up Practice | International Space Station

Experienced NASA astronaut Jessica Meir can be seen practicing tool-use in her spacesuit ahead of a scheduled spacewalk.

NASA astronaut Jack Hathaway, on his first spaceflight, assists experienced NASA spacewalker Jessica Meir with her spacesuit on her second.

A spacewalk by NASA astronauts Jessica Meir and Chris Williams is scheduled for Wednesday, March 18, 2026, at the International Space Station. The team has reviewed the spacewalking tools and tasks necessary to install a modification kit and route cables on the port side of the orbital outpost. This external maintenance work will enable the next roll-out solar array to be installed on a future spacewalk after it is delivered on a SpaceX Dragon spacecraft.

This is Jessica Meir's second spaceflight. After her arrival to the International Space Station, she joined Expedition 74/75, kicking off a long-duration science expedition aboard the orbiting laboratory. She was selected as a NASA astronaut in 2013. The Caribou, Maine, native earned a bachelor’s degree in biology Brown University, a master’s degree in space studies from the International Space University, and a doctorate in marine biology from Scripps Institution of Oceanography in San Diego. 

On her first spaceflight, Meir spent 205 days as a flight engineer during Expedition 61/62, and she completed the first three all-woman spacewalks with fellow NASA astronaut Christina Koch, totaling 21 hours and 44 minutes outside of the station. Since then, she has served in various roles, including assistant to the chief astronaut for commercial crew (SpaceX), deputy for the Flight Integration Division, and assistant to the chief astronaut for the human landing system.

NASA Astronaut/Dr. Jessica Meir's Biography:
https://www.nasa.gov/people/jessica-u-meir/


Expedition 74 Crew
Station Commander: Sergey-Kud Sverchkov (Russia)
Roscosmos (Russia) Flight Engineers: 
Andrey Fedyaev, Sergei Mikaev
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jessica Meir, Jack Hathaway, Chris Williams

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.

Credit: NASA's Johnson Space Center
Release Date: March 16, 2026

#NASA #Space #ISS #Planets #Earth #Spacesuits #EVAs #Astronauts #JessicaMeir #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #JSC #UnitedStates #STEM #Education

The Pinwheel Galaxy: Messier 101 in Ursa Major | Webb & Hubble Telescopes

The Pinwheel Galaxy: Messier 101 in Ursa Major | Webb & Hubble Telescopes

The heart of Messier 101, or the Pinwheel Galaxy, shines in this image that combines data from NASA’s Hubble Space Telescope and James Webb Space Telescope.
A close-up view shows a galaxy’s bright, yellow center, surrounded by patches of glowing orange-brown dust and pink stars.
This image shows the location of Messier 101's galactic core.
 At lower left, an image shows a spiral galaxy with a yellow core and winding arms full of brown dust and blue star formation. A rectangle graphic outlines the core, and lines extend to a larger image at upper right, showing a closer view of the galaxy’s center, surrounded by patches of glowing orange-brown dust and pink stars.
Hubble Space Telescope (HST) image of spiral galaxy Messier 101
This star chart for M101 represents the view from mid-northern latitudes for the given month and time.

In the first image, the heart of Messier 101, or the Pinwheel Galaxy, in the constellation Ursa Major, shines. It combines data from NASA’s Hubble Space Telescope and James Webb Space Telescope. At 25 million light-years away, M101 is one of the closest “face-on” spiral galaxies to us. With that in mind, Hubble’s ultraviolet, visible, and near-infrared data were taken as part of studies to find out more about its stellar population and galactic structure. Webb’s near- and mid-infrared observations helped astronomers study the formation and evolution of polycyclic aromatic hydrocarbons. These are complex, carbon-based molecules, and the smallest dust grains that glow in infrared light.

The second image shows Messier 101—one of the largest images Hubble has captured of a spiral galaxy. Assembled from 51 exposures taken during various studies over nearly ten years, this infrared and visible-light image measures 16,000 by 12,000 pixels. Ground-based images were used to fill in the portions of the galaxy that Hubble did not observe.

The giant spiral disk of stars, dust, and gas is 170,000 light-years across—nearly twice the diameter of our galaxy, the Milky Way. Astronomers estimate that M101 contains at least one trillion stars. The galaxy’s spiral arms are sprinkled with large regions of star-forming nebulas. These nebulas are areas of intense star formation within giant molecular hydrogen clouds. Brilliant, young clusters of hot, blue, newborn stars trace out the spiral arms.

Pierre Méchain, one of Charles Messier’s colleagues, discovered the Pinwheel galaxy in 1781. Located 25 million light-years away from Earth in the constellation Ursa Major, M101 has an apparent magnitude of 7.9. It can be spotted through a small telescope and is most easily observed during June.


Image 1 Credit: NASA, CSA, ESA, D. Calzetti (University of Massachusetts - Amherst), C. Clark (Space Telescope Science Institute - ESA - JWST), K. Kuntz (The John Hopkins University), and B. Shappee (University of Hawaii) ; Processing: Gladys Kober (NASA/Catholic University of America)
Image 2 Credit: HST Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana) and STScI; CFHT Image: Canada-France-Hawaii Telescope/J.-C. Cuillandre/Coelum; NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/NOAO/AURA/NSF; HST + JWST Image: NASA, CSA, ESA, D. Calzetti (University of Massachusetts - Amherst), C. Clark (Space Telescope Science Institute - ESA - JWST), K. Kuntz (The John Hopkins University), and B. Shappee (University of Hawaii); Processing: Gladys Kober (NASA/Catholic University of America)
Image 3 Credit: Stellarium
Release Date: March 16, 2026


#NASA #ESA #Astronomy #Space #Science #Galaxies #SpiralGalaxies #Messier101 #M101 #PinwheelGalaxy #Cosmos #Universe #JWST #InfraredAstronomy #HubbleSpaceTelescope #HST  #SpaceTelescopes #Europe #GSFC #STScI #UnitedStates #STEM #Education

How to Make Planet Jupiter | International Space Station

How to Make Planet Jupiter | International Space Station

Expedition 71/72 flight engineer and NASA astronaut Don Pettit: "How to make planet Jupiter:

1) Be on the International Space Station

2) Make a thin film sphere of water

3) Add food coloring

4) Blow on the edge to create swirls

This is way cool!"

NASA astronaut Don Pettit returned to Earth on April 19, 2025, concluding a seven-month science mission aboard the International Space Station. Pettit spent 220 days in space, earning him a total of 590 days in space over the course of his four spaceflights. He orbited the Earth 3,520 times, traveling 93.3 million miles in low-Earth orbit.

Follow Expedition 74:

Expedition 74 Crew
Station Commander: Sergey-Kud Sverchkov (Russia)
Roscosmos (Russia) Flight Engineers: 
Andrey Fedyaev, Sergei Mikaev
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jessica Meir, Jack Hathaway, Chris Williams

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/D. Pettit
Duration: 37 seconds
Release Date: March 12, 2026

#NASA #Space #Astronomy #Science #SolarSystem #Planets #Earth #Jupiter #MicrogravityExperiments #FluidPhysics #Astronauts #DonPettit #AstronautVideography #UnitedStates #ESA #France #Europe #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition74 #STEM #Education #HD #Video

Pictor Constellation: 2nd-Gen Star Found in Ancient Dwarf Galaxy | NOIRLab

Pictor Constellation: 2nd-Gen Star Found in Ancient Dwarf Galaxy NOIRLab

Photo of the constellation Pictor produced by NOIRLab in collaboration with Eckhard Slawik, a German astrophotographer.
Photo of the constellation Pictor with annotations from International Astronomical Union (IAU) and Sky & Telescope

This is a photo of the constellation Pictor produced by NOIRLab in collaboration with Eckhard Slawik, a German astrophotographer. 

Astronomers have discovered one of the most chemically primitive stars ever identified—an ancient stellar relic that preserves the chemical imprint of the very first stars in the Universe. This star, named PicII-503, resides in the tiny, ultra-faint dwarf galaxy Pictor II located in the constellation Pictor. The discovery was enabled by the U.S. Department of Energy-fabricated Dark Energy Camera (DECam), mounted on the U.S. National Science Foundation Víctor M. Blanco 4-meter Telescope, at the National Science Foundation Cerro Tololo Inter-American Observatory (CTIO) in Chile, a Program of NSF NOIRLab.

Pictor II contains several thousand stars and is more than ten billion years old. PicII-503 lies on the outskirts of the galaxy, and it contains less iron than any other star ever measured outside of the Milky Way, while also having an extreme overabundance of carbon. These signatures unmistakably match those of carbon-enhanced stars found in the outer reaches of the Milky Way, whose origins have, until now, been a mystery.

Credit: E. Slawik/NOIRLab/NSF/AURA/M. Zamani
Release Date: March 16, 2026

#NASA #Astronomy #Space #Science #Star #PicII503 #Galaxies #PictorII #DwarfGalaxies #PictorIIConstellation #Cosmos #Universe #NOIRLab #NSF #DOE #AURA #UnitedStates #IAU # #Astrophotography #EckhardSlawik #Astrophotographer #STEM #Education

Rare 2nd-Gen Star Discovered inside Ancient Relic Dwarf Galaxy | NOIRLab

Rare 2nd-Gen Star Discovered inside Ancient Relic Dwarf Galaxy | NOIRLab

This image shows the star PicII-503 with the lowest iron content ever measured outside of the Milky Way.
This image shows stars in the ultra-faint dwarf galaxy, Pictor II. Pictor II is a satellite galaxy of the Large Magellanic Cloud (LMC). LMC is a satellite galaxy of the Milky Way.
This image shows stars in the ultra-faint dwarf galaxy, Pictor II. Pictor II is a satellite galaxy of the Large Magellanic Cloud. This is a satellite galaxy of the Milky Way, and is located in the constellation Pictor. The system is made up of several thousand stars and is more than ten billion years old.

Astronomers have discovered one of the most chemically primitive stars ever identified—an ancient stellar relic that preserves the chemical imprint of the very first stars in the Universe. This star, named PicII-503, resides in the tiny, ultra-faint dwarf galaxy Pictor II. The discovery was enabled by the U.S. Department of Energy-fabricated Dark Energy Camera (DECam), mounted on the U.S. National Science Foundation Víctor M. Blanco 4-meter Telescope, at the National Science Foundation Cerro Tololo Inter-American Observatory (CTIO) in Chile, a Program of NSF NOIRLab.

Pictor II is located in the constellation Pictor. It contains several thousand stars and is more than ten billion years old. PicII-503 lies on the outskirts of the galaxy, and it contains less iron than any other star ever measured outside of the Milky Way, while also having an extreme overabundance of carbon. These signatures unmistakably match those of carbon-enhanced stars found in the outer reaches of the Milky Way, whose origins have, until now, been a mystery.

The study was led by Anirudh Chiti, Brinson Prize Fellow at Stanford University, and the results are presented in a paper appearing in Nature Astronomy.

The first stars in the Universe formed from gas that contained only the simple elements, hydrogen and helium. Within their fiery cores, this first generation of stars created the first elements heavier than helium, such as carbon and iron, that astronomers refer to as “metals.” When these stars exploded, they released their heavy elements into the interstellar medium to be recycled into the next generation of stars.

Second-generation stars are like time capsules, preserving the low amounts of heavy elements released during the explosive deaths of first-generation stars. By searching for these rare, low-metallicity stars and deriving their chemistry, scientists can better understand the mechanisms of initial element production in the Universe.

PicII-503 is the first unambiguous example of a second-generation star in an ultra-faint dwarf galaxy. It was uncovered in data from the DECam Mapping the Ancient Galaxy in CaHK (MAGIC) survey, a 54-night observing program designed to identify the oldest and most chemically primitive stars in the Milky Way and its dwarf galaxy companions. Using a specialized narrow-band filter sensitive to calcium absorption features, astronomers were able to estimate the metal content of thousands of stars from imaging data alone.

Credit: CTIO/NOIRLab/DOE/NSF/AURA
Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani & D. de Martin (NSF NOIRLab)
Acknowledgments: PI: Anirudh Chiti, Alex Drlica-Wagner
Date: March 16, 2026

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