Saturday, March 21, 2026

The Cat's Eye Galaxy: Messier 94 with Starburst Ring in Canes Venatici

The Cat's Eye Galaxy: Messier 94 with Starburst Ring in Canes Venatici

This image shows the galaxy Messier 94. It lies in the small northern constellation of the Hunting Dogs (Canes Venatici), about 16 million light-years away.

Within the bright ring around Messier 94 new stars are forming at a high rate and many young, bright stars are present within it—thanks to this feature called a starburst ring.

The cause of this peculiarly shaped star-forming region is likely a pressure wave going outwards from the galactic center, compressing the gas and dust in the outer region. The compression of material means the gas starts to collapse into denser clouds. Inside these dense clouds, gravity pulls the gas and dust together until temperature and pressure are high enough for stars to be born.

Messier 94 (also known as the Crocodile Eye Galaxy, or Croc's Eye Galaxy) was discovered by Pierre Méchain in 1781, and cataloged by Charles Messier.


Image Credit: Alessandro Cipolat Bares
Image Details: ARTEC 200E and ZWO AI2600MC, 80x300"
Capture Location: Aosta Valley, Western Alps, Italy
Image Date: March 13, 2026
Release Date: March 14, 2026


#NASA #Astronomy #Space #Science #Galaxies #Messier94 #M94 #SpiralGalaxies #StarburstGalaxies #StarburstRings #DoubleRingGalaxies #CanesVenaticiConstellation #Cosmos #Universe #Hubble #HST #SpaceTelescopes #ESA #Europe #STScI #GSFC #UnitedStates #STEM #Education

The Black Eye Galaxy: Messier 64 in Coma Berenices | Webb & Hubble

The Black Eye Galaxy: Messier 64 in Coma Berenices | Webb & Hubble


Easily identified by the spectacular band of dark dust that partially obscures its bright core, Messier 64, or the Black Eye Galaxy, is characterized by its bizarre internal motion. The gas in the outer regions of this spiral galaxy is rotating in the opposite direction from the gas and stars in its inner regions. This strange behavior may be the result of a merger between M64 and a satellite galaxy over a billion years ago.

Distance from Earth: 17 million light-years

New stars are forming in the region where the oppositely rotating gases collide, are compressed, and then contract. Particularly noticeable in this stunning Hubble image of the galaxy’s core are recently formed hot, blue stars and pink clouds of glowing hydrogen gas that fluoresce when exposed to ultraviolet light from the newly-formed stars.

English astronomer Edward Pigott first spotted M64 in March 1719, just 12 days before German astronomer Johann Elert Bode, and roughly a year before Charles Messier independently rediscovered it in March of 1780. The galaxy is located 17 million light-years from Earth in the constellation Coma Berenices. The best time of year to look for the Black Eye Galaxy is May. Its apparent magnitude of 9.8 requires a moderately sized telescope and dark sky site.

This image is a composite view from NASA’s Hubble Space Telescope and James Webb Space Telescope. It shows Messier 64 captured at near- and mid-infrared wavelengths by Webb, while Hubble’s image shows the galaxy in ultraviolet, visible, and near-infrared light. These observations were taken to learn more about star formation in nearby galaxies. 

Image Description: A massive spiral galaxy glows with a yellow core, surrounded by arms full of orange-brown dust and pink and blue patches of star formation. Framed by a haze of dark dust, the galaxy shines against black space dotted with a few stars.


Image Credit: NASA, CSA, ESA, F. Belfiore (European Southern Observatory – Germany), J. Lee (Space Telescope Science Institute), A. Leroy (The Ohio State University), and D. Thilker (The Johns Hopkins University)
Processing: Gladys Kober (NASA/Catholic University of America)
Release Date: March 20, 2026


#NASA #ESA #Astronomy #Space #Science #Galaxies #Messier64 #M64 #SpiralGalaxies  #InteractingGalaxies #ComaBerenicesConstellation #Cosmos #Universe #JWST #InfraredAstronomy #HubbleSpaceTelescope #HST #UltravioletAstronomy #SpaceTelescopes #CSA #Canada #Europe #GSFC #STScI #UnitedStates #STEM #Education

The Cat's Paw Nebula: NGC 6334 | Webb & Chandra Space Telescopes

The Cat's Paw Nebula: NGC 6334 | Webb & Chandra Space Telescopes


Part of a collection of images from NASA's Chandra X-ray Observatory and other telescopes features regions where stars are forming, areas often nicknamed “stellar nurseries.” X-rays are energetic enough that they can penetrate the gas and dust of these regions, giving insight to the young stars and other high-energy phenomena that are happening within, including the effects of X-rays on any planets or planet-forming disks orbiting the stars.

This image reveals a chaotic scene still in development—massive young stars are carving away at nearby gas and dust, while their bright starlight is producing a bright nebulous glow represented in blue. The disruptive young stars, with their relatively short lifespans and luminosity, will eventually quench the local star formation process.

The Cat’s Paw Nebula is located approximately 4,000 light-years away in the constellation Scorpius.

Image Description: The Cat’s Paw Nebula including X-rays from Chandra (pink) and infrared data from James Webb. A mottled patch of purple at the center reveals young, million-year-old stars tucked behind thick, overlapping rings of dark orange cosmic dust. The pockets of blue sky appearing through the clouds highlight the complex structure of this stellar nursery.


Credits: X-ray: NASA/SAO/CXC; Infrared: NASA/ESA/CSA/STScI
Image Processing: NASA/CXC/SAO/J. Major
Release Date: March 19, 2026

#NASA #Astronomy #Space #Science #NASAWebb #Nebulae #CatsPawNebula #NGC6334 #ScorpiusConstellation #Universe #NASAChandra #XrayAstronomy #JWST #InfraredAstronomy #NIRCam #UnfoldTheUniverse #ESA #Europe #CSA #Canada #GSFC #STScI #CXC #UnitedStates #STEM #Education

Friday, March 20, 2026

NASA Artemis II Moon Rocket Launchpad Arrival: Part II | Kennedy Space Center

NASA Artemis II Moon Rocket Launchpad Arrival: Part II | Kennedy Space Center









NASA’s Artemis II Space Launch System (SLS) rocket and Orion spacecraft, secured to the mobile launcher, are seen as they arrive at Launch Pad 39B, Friday, March 20, 2026, at NASA’s Kennedy Space Center in Florida. NASA’s Artemis II flight test 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 with launch opportunities beginning in April 2026. 

Check the NASA Artemis II Mission page for updates:

This was a multi-hour trek from the Vehicle Assembly Building (VAB) to Launch Pad 39B. The four-mile journey on the crawler-transporter-2, at a careful speed of roughly 1 mile per hour, can take up to 12 hours. The massive crawler keeps the mobile launcher and rocket perfectly level throughout the trip, even on the gentle slopes of the crawlerway. At the pad, the stack will be secured and ground support systems will be connected in preparation for flight.

The crawler-transporters, formally known as the Missile Crawler Transporter Facilities, are a pair of tracked vehicles used to transport launch vehicles from NASA's Vehicle Assembly Building (VAB) along the Crawlerway to Launch Complex 39. They were originally used to transport the Saturn IB and Saturn V rockets during the Apollo, Skylab and Apollo–Soyuz programs. They were then used to transport Space Shuttles from 1981 to 2011. The crawler-transporters carry vehicles on the mobile launcher platforms (MLPs) used by NASA, and after each launch return to the pad to take the platform back to the VAB.

The two crawler-transporters were designed and built by Marion Power Shovel Company using some components designed and built by Rockwell International at a cost of US$14 million (US$128.5 million in 2022) each. Upon its construction, the crawler-transporter became the largest self-powered land vehicle in the world. 


Image Credit: NASA/Joel Kowsky
Date: March 20, 2026

#NASA #Space #Science #Earth #Moon #ArtemisProgram #ArtemisII #OrionSpacecraft #SLS #SLSRocket #CrawlerTransporter2 #CrewedMissions #Astronauts #DeepSpace #MoonToMars #Engineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NASAKennedy #KSC #VAB #MerrittIsland #Florida #UnitedStates #STEM #Education

NASA Artemis II Moon Rocket Launchpad Journey: Part II | Kennedy Space Center

NASA Artemis II Moon Rocket Launchpad Journey: Part II | Kennedy Space Center








NASA’s Artemis II Space Launch System (SLS) rocket and Orion spacecraft, secured to the mobile launcher, are seen as they make the 4.2 mile journey toward Launch Pad 39B, Friday, March 20, 2026, at NASA’s Kennedy Space Center in Florida. NASA’s Artemis II flight test 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 with launch opportunities beginning in April 2026. 

Check the NASA Artemis II Mission page for updates:

This is a multi-hour trek from the Vehicle Assembly Building (VAB) to Launch Pad 39B. The four-mile journey on the crawler-transporter-2, at a careful speed of roughly 1 mile per hour, will take up to 12 hours. The massive crawler keeps the mobile launcher and rocket perfectly level throughout the trip, even on the gentle slopes of the crawlerway. Once at the pad, the stack will be secured, ground support systems will be connected in preparation for flight.

The crawler-transporters, formally known as the Missile Crawler Transporter Facilities, are a pair of tracked vehicles used to transport launch vehicles from NASA's Vehicle Assembly Building (VAB) along the Crawlerway to Launch Complex 39. They were originally used to transport the Saturn IB and Saturn V rockets during the Apollo, Skylab and Apollo–Soyuz programs. They were then used to transport Space Shuttles from 1981 to 2011. The crawler-transporters carry vehicles on the mobile launcher platforms (MLPs) used by NASA, and after each launch return to the pad to take the platform back to the VAB.

The two crawler-transporters were designed and built by Marion Power Shovel Company using some components designed and built by Rockwell International at a cost of US$14 million (US$128.5 million in 2022) each. Upon its construction, the crawler-transporter became the largest self-powered land vehicle in the world. 


Image Credit: NASA/Joel Kowsky/Aubrey Gemignani
Image Date: March 20, 2026

#NASA #Space #Science #Earth #Moon #ArtemisProgram #ArtemisII #OrionSpacecraft #SLS #SLSRocket #CrawlerTransporter2 #CrewedMissions #Astronauts #DeepSpace #MoonToMars #Engineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NASAKennedy #KSC #VAB #MerrittIsland #Florida #UnitedStates #STEM #Education

NASA Artemis II Moon Rocket Rollout: Part II | Kennedy Space Center

NASA Artemis II Moon Rocket Rollout: Part II | Kennedy Space Center









NASA’s Artemis II Space Launch System (SLS) rocket and Orion spacecraft, secured to the mobile launcher, is seen inside and outside the Vehicle Assembly Building (VAB) as preparations continue for roll out to Launch Pad 39B, Thursday, March 19, 2026, at NASA’s Kennedy Space Center in Florida. NASA’s Artemis II flight test 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 with launch opportunities beginning in April 2026. 

Check the NASA Artemis II Mission page for updates:

This is a multi-hour trek from the Vehicle Assembly Building (VAB) to Launch Pad 39B. The four-mile journey on the crawler-transporter-2, at a careful speed of roughly 1 mile per hour, will take up to 12 hours. The massive crawler keeps the mobile launcher and rocket perfectly level throughout the trip, even on the gentle slopes of the crawlerway. Once at the pad, the stack will be secured, ground support systems will be connected in preparation for flight.

The crawler-transporters, formally known as the Missile Crawler Transporter Facilities, are a pair of tracked vehicles used to transport launch vehicles from NASA's Vehicle Assembly Building (VAB) along the Crawlerway to Launch Complex 39. They were originally used to transport the Saturn IB and Saturn V rockets during the Apollo, Skylab and Apollo–Soyuz programs. They were then used to transport Space Shuttles from 1981 to 2011. The crawler-transporters carry vehicles on the mobile launcher platforms (MLPs) used by NASA, and after each launch return to the pad to take the platform back to the VAB.

The two crawler-transporters were designed and built by Marion Power Shovel Company using some components designed and built by Rockwell International at a cost of US$14 million (US$128.5 million in 2022) each. Upon its construction, the crawler-transporter became the largest self-powered land vehicle in the world. 


Image Credit: NASA/Joel Kowsky/Aubrey Gemignani
Image Dates: March 19-20, 2026

#NASA #Space #Science #Earth #Moon #ArtemisProgram #ArtemisII #OrionSpacecraft #SLS #SLSRocket #CrawlerTransporter2 #CrewedMissions #Astronauts #DeepSpace #MoonToMars #Engineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NASAKennedy #KSC #VAB #MerrittIsland #Florida #UnitedStates #STEM #Education

NASA Artemis II Moon Rocket Rollout: Part II | Kennedy Space Center

NASA Artemis II Moon Rocket Rollout: Part II | Kennedy Space Center








NASA’s Artemis II Space Launch System (SLS) rocket and Orion spacecraft, secured to the mobile launcher, is seen inside and outside the Vehicle Assembly Building (VAB) as preparations continue for roll out to Launch Pad 39B, Thursday, March 19, 2026, at NASA’s Kennedy Space Center in Florida. NASA’s Artemis II flight test 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 with launch opportunities beginning in April 2026. 

Check the NASA Artemis II Mission page for updates:

This is a multi-hour trek from the Vehicle Assembly Building (VAB) to Launch Pad 39B. The four-mile journey on the crawler-transporter-2, at a careful speed of roughly 1 mile per hour, will take up to 12 hours. The massive crawler keeps the mobile launcher and rocket perfectly level throughout the trip, even on the gentle slopes of the crawlerway. Once at the pad, the stack will be secured, ground support systems will be connected in preparation for flight.

The crawler-transporters, formally known as the Missile Crawler Transporter Facilities, are a pair of tracked vehicles used to transport launch vehicles from NASA's Vehicle Assembly Building (VAB) along the Crawlerway to Launch Complex 39. They were originally used to transport the Saturn IB and Saturn V rockets during the Apollo, Skylab and Apollo–Soyuz programs. They were then used to transport Space Shuttles from 1981 to 2011. The crawler-transporters carry vehicles on the mobile launcher platforms (MLPs) used by NASA, and after each launch return to the pad to take the platform back to the VAB.

The two crawler-transporters were designed and built by Marion Power Shovel Company using some components designed and built by Rockwell International at a cost of US$14 million (US$128.5 million in 2022) each. Upon its construction, the crawler-transporter became the largest self-powered land vehicle in the world. 


Image Credit: NASA/Joel Kowsky
Image Dates: March 19-20, 2026

#NASA #Space #Science #Earth #Moon #ArtemisProgram #ArtemisII #OrionSpacecraft #SLS #SLSRocket #CrawlerTransporter2 #CrewedMissions #Astronauts #DeepSpace #MoonToMars #Engineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NASAKennedy #KSC #VAB #MerrittIsland #Florida #UnitedStates #STEM #Education

California Sunset: The Novaya Zemlya Effect | Earth Science

California Sunset: The Novaya Zemlya Effect | Earth Science

"I have seen quite a few Novaya Zemlya sunsets but the one I saw on March 17 was special. The sunset was delayed for 14 minutes! At times, it felt as the universe stands still.Thanks to the Novaya Zemlya effect, this pancaked sun stayed visible until it was geometrically 3.4° below the horizon."

The Novaya Zemlya effect is an atmospheric refraction phenomenon that is occasionally seen over large flat areas of the Earth's surface. The effect consists of the trapping of light rays within the lower layers of the atmosphere. The process can be transmitted over hundreds of kilometers around the curvature of the Earth. The effect appears when direct rays from the sun are trapped so that the image of the sun appears, although the sun is well below the horizon. This effect is named because it was first observed on the arctic island of Novaya Zemlya—an archipelago in northern Russia.

The first person to record the phenomenon was Gerrit de Veer, a member of Willem Barentsz's ill-fated third expedition into the north polar region in 1596–1597. Trapped by the ice, the party was forced to stay for the winter in a makeshift lodge on the archipelago of Novaya Zemlya and endure the polar night.

On January 24, 1597, De Veer and another crew member claimed to have seen the Sun appear above the horizon, approximately two weeks prior to its calculated return. They were met with disbelief by the rest of the crew—who accused De Veer of having used the old Julian calendar instead of the Gregorian calendar introduced several years earlier—but on January 27, the Sun was seen by all "in his full roundnesse". For centuries the account was the source of skepticism, until in the 20th century the phenomenon was finally proven to be genuine.

Apart from the image of the Sun, the effect can also elevate the image of other objects above the horizon, such as coastlines that are normally invisible due to their distance. After studying the Saga of Erik the Red, Waldemar Lehn concluded that the effect may have aided the Vikings in their discovery of Iceland and Greenland that are not visible from the mainland under normal atmospheric conditions.

San Francisco, California, is located on a peninsula between the Pacific Ocean and San Francisco Bay, making it a coastal city.

California is a state in the Western United States that lies on the Pacific Coast. It borders Oregon to the north, Nevada and Arizona to the east, and shares an international border with the Mexican state of Baja California to the south. 


Image Credit: Mila Zinkova 
Location: San Francisco, California, USA
Date: March 17, 2026

#NASA #Astronomy #Space #Science #Stars #SolarSystem #Sun #Planets #Earth #Atmosphere #AtmosphericRefraction #Sunlight #NovayaZemlyaEffect #SanFrancisco #California #PacificOcean #UnitedStates #History #STEM #Education

NASA's Nancy Grace Roman Space Telescope: Final Assembly Update

NASA's Nancy Grace Roman Space Telescope: Final Assembly Update

This video, covering the second half of 2025, shows the Goddard Space Flight Center’s largest clean room, the Spacecraft Systems Development and Integration Facility in Greenbelt, Maryland. The room is a class 10,000 clean room with over one million cubic feet of space.

The outside half of NASA's Nancy Grace Roman Space Telescope, called OSD, contains the solar panels & protective layers. The Deployable Aperture Cover protects the mirrors during launch and then unfolds to help shield them from sunlight does a test deployment. During this test, lines connect to it and pull upward to negate Earth’s gravitational forces. Of course, Roman will not experience this in space. Then, the Solar Array Sun Shield panels deploy. There are four panels that move. They fold against the spacecraft to fit in the rocket fairing and deploy in space to make a large flat plane that collects light to generate electricity and helps keep the rest of Roman cool.

In preparation for additional testing, technicians put a clean tent over OSD and transport it out of the clean room. They push it into the acoustic test chamber where a six-foot-tall horn projects up to 150-decibel sound at varying frequencies. The other tests are on two vibration tables that shake Roman along all three axes: up/down, left/right & forward/backward. Engineers attach hundreds of sensors and run tests of increasing intensity. During and after each test, they carefully study the data to make sure that Roman is reacting as expected.

While these tests occur, Roman’s inside half, containing the mirrors, instruments & support equipment, move into Goddard’s largest thermal vacuum chamber, the Space Environment Simulator (SES). This 40-foot-tall chamber can simulate the vacuum of space & the wide temperature range that Roman will experience there: from -310° F (-190° C) to 302° F (150° C). The move to the chamber happens without a clean tent, so the entire path was cleaned, and all the workers dress in full clean-room garb to ensure that no dirt contaminates the sensitive parts of the spacecraft. Once the two layers of doors are sealed, Roman spends 72 days inside running through tests at various temperatures and with equipment turned on to ensure that it works at low temperature in a vacuum. A special array installed above the mirror projects light that engineers use to test the optics and sensors.

After leaving the SES chamber and returning to the SSDIF, Roman’s primary and secondary mirrors are carefully cleaned and inspected. It is a balance to get the mirrors as clean as possible while not cleaning too aggressively and damaging the delicate surfaces. The mirrors are cleaned horizontally with a gentle vacuum cleaner and vertically with brushes. After this cleaning, every inch is visually inspected and photographed to record the exact optical characteristics. This was the last time the primary mirror would be accessible.

Finally, in late November, Roman’s two halves are joined together to form the complete observatory. The process takes the better part of a day. Two guide poles are installed on the inside half to help direct OSD down onto it. At various times, the clearances between the two halves are only a few inches. With the observatory complete, it begins preparing for another round of deployments and testing.

On track to launch in fall 2026, the Roman Space Telescope is NASA’s next flagship astrophysics mission. An infrared survey telescope with the same resolution as Hubble but at least 100 times the field of view, Roman is being built and tested at NASA Goddard. Partners worldwide are contributing to this effort.  

0:00 - Roman in the Clean Room

0:14 - Deployment Tests

0:33 - Acoustic and Vibration Tests

1:05 - Thermal Vacuum Testing

1:40 - Mirror Cleaning

1:56 - Joining the Halves


The Roman telescope and the discoveries it will enable: 
https://www.stsci.edu/roman


Credit: NASA’s Goddard Space Flight Center
Producer: Scott Wiessinger (eMITS)
Videographers (eMITS): Sophia Roberts, Scott Wiessinger, Rob Andreoli, John Philyaw
Editor: Scott Wiessinger (eMITS)
Science Writer: Ashley Balzer (eMITS)
Duration: 2 minutes, 29 seconds
Release Date: March 19, 2026

#NASA #Space #Astronomy #Science #NASARoman #RomanSpaceTelescope #NancyGraceRoman #Exoplanets #Planets #SolarSystem #Stars #MilkyWayGalaxy #Galaxies #Cosmos #Universe #SpaceTelescopes #NASAGoddard #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

The Owl Nebula: Planetary Nebula M97 in Ursa Major | Gemini North Telescope

The Owl Nebula: Planetary Nebula M97 in Ursa Major | Gemini North Telescope

Gemini North image of the planetary nebula Messier 97 (M97), also known as the Owl Nebula, imaged by the Gemini Multi-Object Spectrograph (GMOS). The approximately 6,000 year-old nebula is located about 2,600 light-years away, and has a diameter ofabout three light-years across. It is located in the constellation of Ursa Major (containing the Big Dipper).

Since their discovery in the late 1700s, astronomers have learned that planetary nebulae, or the expanding shell of glowing gas expelled by a low-intermediate mass star late in its life, can come in all shapes and sizes. Most planetary nebulae present as circular, elliptical, or bi-polar, but others can vary from this.

Learn about the Gemini North Telescope:
https://noirlab.edu/public/programs/gemini-observatory/gemini-north/


Credit: International Gemini Observatory/NOIRLab/NSF/AURA/Émilie Storer (Collège Charlemagne, QUE)/André-Nicolas Chené (HIA/NRCof Canada)/T. Rector (U.Alaska, Anchorage).
Release Date: March 25, 2010

#NASA #Astronomy #Space #Science #Stars #Nebulae #PlanetaryNebulae #Messier97 #M97 #UrsaMajorConstellation #Cosmos #Universe #InternationalGeminiObservatory #GeminiNorthTelescope #GMOS #Maunakea #Hawaii #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

A Dwarf Galaxy Ravaged by Grand Design: NGC 5474 in Ursa Major | Hubble

A Dwarf Galaxy Ravaged by Grand Design: NGC 5474 in Ursa Major | Hubble


The subject of this Hubble image is NGC 5474, a dwarf galaxy located 21 million light-years away in the constellation of Ursa Major (The Great Bear). This beautiful image was taken with Hubble's Advanced Camera for Surveys (ACS).

The term "dwarf galaxy" may sound diminutive, but do not let that fool you—NGC 5474 contains several billion stars! However, when compared to the Milky Way with its hundreds of billions of stars, NGC 5474 does seem relatively small.

NGC 5474 itself is part of the Messier 101 Group. The brightest galaxy within this group is the well-known spiral Pinwheel Galaxy (also known as Messier 101, heic0602). This galaxy's prominent, well-defined arms classify it as a "grand design galaxy", along with other spirals Messier 81 (heic0710) and Messier 74 (heic0719).

Also within this group are Messier 101's galactic neighbors. It is possible that gravitational interactions with these companion galaxies have influenced Messier 101's striking shape. Similar interactions with Messier 101 may have caused the distortions visible in NGC 5474.

The Messier 101 Group and our own Local Group reside within the Virgo Supercluster, making NGC 5474 a neighbor in galactic terms.


Credit: ESA/Hubble & NASA
Release Date: June 16, 2014

#NASA #ESA #Astronomy #Space #Science #Galaxies #DwarfGalaxies #NGC5474 #IrregularGalaxies #Messier101Group #UrsaMajorConstellation #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education

Thursday, March 19, 2026

NASA's Quesst Mission: A Future with Quiet Supersonic Flight

NASA's Quesst Mission: A Future with Quiet Supersonic Flight

NASA’s Quesst mission seeks to collect data that could make commercial supersonic flight over land possible, dramatically reducing travel time in the United States or anywhere in the world. The centerpiece of the Quesst mission is NASA’s X-59 quiet supersonic research aircraft, designed to fly supersonic, or faster than the speed of sound, while reducing typical loud sonic booms to quieter sonic “thumps”. 

Through the Quesst mission, NASA will fly the X-59 over several U.S. communities to gather data on human responses to the sound generated during supersonic flight and will deliver that data set to U.S. and international regulators. This will inform the establishment of new, data-driven noise thresholds, opening the door to a future with commercial supersonic flight over land.

The X-59 aircraft builds on decades of supersonic flight research and is the centerpiece of NASA’s Quesst mission. The vast amount of data collected over the years has given designers the tools they needed to craft the shape of the X-59. The goal is to enable the aircraft to fly at supersonic speeds and reduce a loud sonic boom to a quieter “sonic thump.”

The X-59’s engine, a modified F414-GE-100, packs 22,000 pounds of thrust. This will enable the X-59 to achieve the desired cruising speed of Mach 1.4 (925 miles per hour) at an altitude of approximately 55,000 feet. It sits in a nontraditional spot–atop the aircraft—to aid in making the X-59 quieter.

The X-59's goal is to help change existing national and international aviation rules that ban commercial supersonic flight over land.

For more information about the X-59 and NASA's Quesst mission, visit www.nasa.gov/quesst


Video Credit: National Aeronautics and Space Administration (NASA)
Duration: 2 minutes
Release Date: March 19, 2026


#NASA #Aerospace #SupersonicFlight #SupersonicAircraft #X59 #Sonicboom #QuietAviation #Aviation #QuesstMission #CommercialAviation #Science #Physics #Engineering #AerospaceResearch #AeronauticalResearch #FlightTests #LockheedMartin #NASAArmstrong #AFRC #Edwards #California #UnitedStates #STEM #Education #HD #Video

Green Airglow—A High Pressure, Heat Dome over Colorado | Earth Science

Green AirglowA High Pressure, Heat Dome over Colorado | Earth Science

A record-setting ridge of high pressure recently occured over the American west, creating a heat dome that meteorologists have called "otherworldly." It might be partly responsible for last night's display of green airglow over Colorado:

"I've heard that airglow loves high pressure," says Aaron Watson, who photographed the all-sky glow from the West Elk Mountains. "I was hoping to see the auroras, but was treated to this green glow instead."

Airglow is produced by photochemistry in Earth's upper atmosphere. For instance, there is a thin layer of air 95 km high where oxygen atoms (O) and oxygen molecules (O2) mix together. When O bumps into O2, the collision creates a spark of green light—airglow. Other reactions contribute, too.

High pressure can accelerate these reactions. Pressure gradients and powerful mountain winds associated with extreme ridging events drive intense atmospheric gravity waves into the mesosphere, boosting the intensity of airglow.

A heat dome occurs when a large area of high pressure in the atmosphere forms a ridge over a region and remains stationary for days or even weeks. This phenomenon acts like a lid, preventing heat from escaping and blocking cloud formation. This can result in persistently high temperatures and minimal relief from the heat.


Image Credit: Aaron Watson
Location: West Elk Mountains, Colorado, USA
Aaron's website: https://www.skies-alive.com/gallery
Date: March 19, 2026

#NASA #Astronomy #Space #Science #Planets #Earth #Atmosphere #Airglow #GreenAirglow #Photochemistry #Meteorology #Weather #HeatDome #HighAirPressure #Astrophotography #AaronWatson #Astrophotographers #WestElkMountains #Colorado #UnitedStates #STEM #Education #HD #Video

Multiple Views: Capturing Explosion Data for Next-gen Rockets | NASA Stennis

Multiple Views: Capturing Explosion Data for Next-gen Rockets | NASA Stennis

NASA Stennis Space Center Update: 
"During a controlled detonation last month at Eglin Air Force Base in Florida, synchronized cameras captured the blast in striking detail. This testing brings together expertise in test operations, execution, logistics, and cryogenics in ways rarely combined outside of actual launch operations."

"Wait for the visible shockwave!💥👀"

"Flash. Fireball. Shockwave.💥"

This is how NASA is collecting explosion data for next generation rockets at Eglin Air Force Base in Florida. NASA's Stennis Space Center has made many critical contributions to NASA's Moon exploration plans through the agency's Apollo and Artemis human spaceflight programs.

For example, the Saturn V S-IC-6 first stage that launched Apollo 11 was tested on NASA Stennis’ B-2 Test Stand on August 13, 1968. The S-II-6 second stage was tested on the A-2 Test Stand on October 3, 1968. 

NASA’s Stennis Space Center near Bay St. Louis, Mississippi, has also achieved key milestones in testing Space Launch System (SLS) rocket stages to fly on future Artemis missions to the Moon and beyond.

“NASA Stennis is at the front end of the critical path for future space exploration,” said Barry Robinson, project manager for exploration upper stage Green Run testing on the Thad Cochran Test Stand.

Learn more about NASA's Stennis Space Center in Mississippi: 
https://www.nasa.gov/stennis/

United States Eglin Air Force Base:
https://www.eglin.af.mil/

Video Credit: John C. Stennis Space Center
Duration: 22 seconds
Release Date: March 19, 2026

#NASA #Space #Astronomy #Science #Moon #ArtemisProgram #ApolloProgram #NextGenerationRockets #RocketTesting #EngineTesting #HumanSpaceflight #NASAStennis #Mississippi #EglinAirForceBase #USAF #Florida #UnitedStates #SolarSystem #SpaceExploration #STEM #Education #History #HD #Video

Capturing Explosion Data for Next-gen Rockets | NASA Stennis Space Center

Capturing Explosion Data for Next-gen Rockets | NASA Stennis Space Center

"Wait for the visible shockwave!💥👀"

This is how NASA is collecting explosion data for next generation rockets at Eglin Air Force Base in Florida. NASA's Stennis Space Center has made many critical contributions to NASA's Moon exploration plans through the agency's Apollo and Artemis human spaceflight programs.

For example, the Saturn V S-IC-6 first stage that launched Apollo 11 was tested on NASA Stennis’ B-2 Test Stand on August 13, 1968. The S-II-6 second stage was tested on the A-2 Test Stand on October 3, 1968. 

NASA’s Stennis Space Center near Bay St. Louis, Mississippi, has also achieved key milestones in testing Space Launch System (SLS) rocket stages to fly on future Artemis missions to the Moon and beyond.

“NASA Stennis is at the front end of the critical path for future space exploration,” said Barry Robinson, project manager for exploration upper stage Green Run testing on the Thad Cochran Test Stand.

Learn more about NASA's Stennis Space Center in Mississippi: 
https://www.nasa.gov/stennis/

United States Eglin Air Force Base:
https://www.eglin.af.mil/

Video Credit: John C. Stennis Space Center
Duration: 21 seconds
Release Date: March 19, 2026

#NASA #Space #Astronomy #Science #Moon #ArtemisProgram #ApolloProgram #NextGenerationRockets #RocketTesting #EngineTesting #HumanSpaceflight #NASAStennis #Mississippi #EglinAirForceBase #USAF #Florida #UnitedStates #SolarSystem #SpaceExploration #STEM #Education #History #HD #Video

Russian Cosmonaut views of The Andes, Chile & Bolivia | International Space Station

Russian Cosmonaut views of The Andes, Chile & Bolivia | International Space Station

This video was shared by Expedition 74 Station Commander and Cosmonaut Sergey Kud-Sverchkov of Russia aboard the International Space Station: "Flying over the Andes, Chile, and Bolivia. Working on the orbital station, you involuntarily become accustomed to the views of our planet. You see the same places dozens of times—continents, oceans, islands, mountain ranges. It becomes "just a view from the window." But sometimes you stop and, looking at Earth, think:

"Damn it, our planet is so amazing! And how extraordinary it is to soar above it, being able to travel between continents in a matter of minutes and see all this beauty!"

...and then you grab your documentation, your tools, and go back to work."

The Andes are the longest continental mountain range in the world, forming a continuous highland along the western edge of South America.

Chile, officially the Republic of Chile, is a country in western South America. It is the southernmost country in the world and the closest to Antarctica, extending along a narrow strip of land between the Andes Mountains and the Pacific Ocean.

Bolivia, officially the Plurinational State of Bolivia, is a landlocked country located in central South America. It is bordered by Brazil to the north and east, Paraguay to the southeast, Argentina to the south, Chile to the southwest, and Peru to the west.


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: Roscosmos/SK Sverchkov
Duration: 2 minute, 22 seconds
Release Date: March 19, 2025


#NASA #Space #ISS #Planets #Earth #Andes #Chile #Bolivia #SouthAmerica #Astronauts #Cosmonauts #CosmonautVideography #SergeyKudSverchkov #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #JSC #UnitedStates #STEM #Education #HD #Video