Tuesday, March 10, 2026

Mars Telecommunications Orbiter | Rocket Lab

Mars Telecommunications Orbiter | Rocket Lab

"Human exploration and science at Mars relies on a robust telecommunications network. Rocket Lab’s Mars Telecommunications Orbiter (MTO) will make that possible."

"Proven hardware. Proven team. Proven Mars experience."

Video Credit: Rocket Lab
Duration: 2 minutes
Release Date: March 10, 2026

#NASA #Space #Astronomy #Science #Planets #Mars #MarsTelecommunicationsOrbiter #MTO #CommunicationsSatellites #CommunicationRelays #RocketLab #SolarSystem #SpaceExploration #PlanetaryExploration #HumanSpaceflight #UnitedStates #STEM #Education #HD #Video

Bright Globular Star Cluster Messier 92 in Hercules: All that Glitters | Hubble

Bright Globular Star Cluster Messier 92 in Hercules: All that Glitters | Hubble

This NASA/European Space Agency Hubble Space Telescope image shows a glittering bauble named Messier 92. Located in the northern constellation of Hercules, this globular cluster—a ball of stars that orbits a galactic core like a satellite—was first discovered by astronomer Johann Elert Bode in 1777.

Messier 92 is one of the brightest globular clusters in the Milky Way, and is visible to the naked eye under good observing conditions. It is very tightly packed with stars, containing around 330,000 stars in total. As is characteristic of globular clusters, the predominant elements within Messier 92 are hydrogen and helium, with only traces of others. It is actually what is known as an Oosterhoff type II (OoII) globular cluster, meaning that it belongs to a group of metal-poor clusters—to astronomers, metals are all elements heavier than hydrogen and helium.

By exploring the composition of globulars like Messier 92, astronomers can figure out how old these clusters are. As well as being bright, Messier 92 is also old, being one of the oldest star clusters in the Milky Way with an age almost the same as the age of the Universe.


Image Credit: ESA/Hubble & NASA 
Acknowledgement: Gilles Chapdelaine
Release Date: Dec. 8, 2014

#NASA #ESA #Astronomy #Space #Science #Stars #StarClusters #GlobularClusters #Messier92 #OoII #HerculesConstellation #MilkyWayGalaxy #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education

The Sun: View from Canary Islands

The Sun: View from Canary Islands


Astrophotographer Marina Prol Franco: "The Sun & INTA Maspalomas in early March and late September, from my home. I can watch the Sun set right behind the antennas of the Canary Islands Space Center. This time, it lined up with the Earth Observation antenna. I tried to capture the moment with my solar telescope, but with the Sun so low, the atmospheric turbulence, and those clouds 😌it didn’t turn out quite the way I hoped. I’ll keep trying though, because sometimes the journey is more interesting than the destination."

The National Institute for Aerospace Technology "Esteban Terradas" 
Spanish: Instituto Nacional de Técnica Aeroespacial or INTA

Maspalomas Station is an INTA-operated, ESTRACK radio antenna ground station for communication with spacecraft located at the southern area of Gran Canaria island, on the INTA campus. It is situated on the Montaña Blanca hill and is visible from the coastal resort of Meloneras, close to Maspalomas. It was originally established in the 1960s to support NASA's human spaceflight program.

The European Space Agency's tracking station network—Estrack—is a global system of ground stations providing links between satellites in orbit and the European Space Operations Center (ESOC), Darmstadt, Germany. The core Estrack network has six stations in six countries. 

The Canary Islands, also known informally as the Canaries, are a Spanish region, autonomous community and archipelago in the Atlantic Ocean. At their closest point to the African mainland, they are 100 kilometers (62 miles) west of Morocco and the Western Sahara. La Palma, also known as La isla bonita and historically San Miguel de La Palma, is the most northwesterly island of the Canary Islands, Spain.

Image Credit: Marina Prol Franco
Marina's website: https://www.marinaprol.com
Gran Canaria, Canary Islands (Spain)
Release Date: March 8, 2026

#NASA #ESA #Astronomy #Space #Science #Satellites #Spacecraft #Estrack #Stars #SolarSystem #Sun #Earth #RadioAntennae #MaspalomasStation #GranCanaria #CanaryIslands #IslasCanarias #AtlanticOcean #Africa #Spain #España #MilkyWayGalaxy #Universe #Astrophotography #MarinaProlFranco #Astrophotographers #STEM #Education

Winter Milky Way Galaxy Farewell

Winter Milky Way Galaxy Farewell

Astrophotographer James Perez-Rogers: "As we say goodbye to the winter end of the Milky Way, I wanted to capture not just Orion, but the surrounding stars and planets. In this image, Jupiter is centered in the top portion of the image. Beneath are an array of constellations including Orion. What can be seen here is approximately an hour of tracked data to reveal the larger dust structures of the Milky Way."

New York, also called New York State, is a state located in the northeastern United States. Bordering New England to its east, Canada to the north, and Pennsylvania and New Jersey to the south, its territory extends into both the Atlantic Ocean and the Great Lakes.

The Ashokan Reservoir is a major New York City water supply reservoir in Ulster County, New York, holding 122.9 billion gallons and supplying about 40% of the city’s daily water needs. The Ashokan Reservoir, located approximately 13 miles west of Kingston, New York, and 73 miles north of New York City, was created by damming the Esopus Creek. It was placed into service in 1915. The Ashokan Reservoir is part of the Catskill Water Supply System.


Image Credit: James Perez-Rogers
Image Details: EXIF: Sony A7Rii Tokina Firin 20mm F2 F2.8 16x 3min tracked exposures for the stars 1x 3min untracked exposure for the foreground Stacked and blended in Photoshop Edits performed in Lightroom
James' website: https://www.jamesperezrogers.com
Location: Ashokan Reservoir, New York, United States
Release Date: March 9, 2026

#NASA #Astronomy #Space #Science #Galaxies #MilkyWayGalaxy #Stars #Planets #Earth #NorthernHemisphere #AshokanReservoir #NewYork #UnitedStates #Astrophotography #AlynWallace #Astrophotographer #CitizenScience #STEM #Education

China's Plans to Detect Lunar Water, Return Mars Samples | Solar System Exploration

China's Plans to Detect Lunar Water, Return Mars Samples | Solar System Exploration

China is advancing a series of ambitious plans to explore deep space, ranging from hunting for water on the Moon to bringing back samples from Mars with an ultimate goal to probe outer reaches of the solar system, said Chinese experts.

In the field of lunar exploration, China's Chang'e-7 lunar probe, scheduled for launch later this year, will target the Moon's south pole to search for water ice. The mission could make China the first country to detect water ice on the Moon.

"Scientists around the world believe there's water on the Moon, but no one has found any yet. Now China is going to look for it. And we're using many methods, from searching the surface to exploring inside craters," said Ye Peijian, an academician with the Chinese Academy of Sciences (CAS).

The Chang'e-7 probe is composed of an orbiter, a lander, a rover, a hopper and a relay satellite.

At the Moon's south pole, there are craters that never see sunlight. Scientists think they hold huge reserves of water ice. However, no spacecraft has ever entered to investigate until the Chang'e-7. With its specially designed hopper, it will be the first to approach and explore a lunar shadow crater.

Researchers at the Harbin Institute of Technology's space laboratory in northeast China's Heilongjiang Province are conducting experiments to support the Chang'e-7 mission of locating water ice.

"We've just created a lunar soil simulant for the Moon's polar region. Next, we will use this set of equipment to convert that soil into water ice. The equipment can create a vacuum environment on the Moon. Secondly, it can cool the lunar mineral material down to minus 240 degrees Celsius. Then, this water molecule excitation device will produce a steady stream of water molecules. When the water molecules come into contact with the cold lunar soil, they will adsorb and deposit to form ice. By using special tools and molds, we can create samples of lunar water ice," said Zhang Weiwei, associate professor at the School of Mechatronics Engineering at the Harbin Institute of Technology.

Apart from lunar missions, China's Tianwen series, the country's planetary exploration program, is also advancing rapidly.

"The Tianwen-2 mission is embarking on a 'star-chasing' journey to collect samples from a near-Earth small body and return them to the Earth. The Tianwen-3 aims to bring back Mars samples to the ground. The Tianwen-4 is our mission to explore Jupiter. I believe this demonstrates our capability and means to expand our horizons from the Earth and cislunar space to interplanetary space and even to the entire solar system and beyond in the future," said Sun Zezhou, a deputy to the National People's Congress (NPC) and a researcher at the Fifth Academy of China Aerospace Science and Technology Corporation (CASC).

China's deep-space ambitions extend beyond the Chang'e and Tianwen missions. With plans to explore the Sun, the solar system's frontiers, and Venus, the country is building a deep-space exploration system that covers everything from cislunar space and the moon to Mars, small bodies, and other planets.


Video Credit: CCTV
Duration: 1 minute, 53 seconds
Release Date: March 10, 2026


#NASA #CNSA #Space #Astronomy #Science #China #中国 #CAS #Moon #Geology #WaterIce #SouthPole #CLEP #Change7 #嫦娥七号 #Tianwen2 #天问二号 #Tianwen3 #天问三号 #MarsSampleReturn #Tianwen4 #天问四号 #Jupiter #SpaceTechnology #SpaceExploration #DeepSpace #SolarSystem #STEM #Education #HD #Video

Crash of Extreme Stars Found in Unexpected Site | NASA's Chandra X-ray Observatory

Extreme Collision of Neutron Stars Found in Unexpected Site | NASA Chandra

Astronomers have spotted the merger between two neutron stars in a very odd place. This extreme collision was found in a tiny galaxy embedded in a stream of gas. Scientists needed NASA’s Chandra, Fermi, Swift, and Hubble observatories to make this discovery. This result may help answer two mysteries about stars and intergalactic space.

A neutron star is the gravitationally collapsed core of a massive supergiant star. It results from the supernova explosion of a massive star—combined with gravitational collapse—that compresses the core past white dwarf star density to that of atomic nuclei. Surpassed only by black holes, neutron stars are the second smallest and densest known class of stellar objects.


Credits: NASA's Chandra X-ray Observatory
X-ray: NASA/CXC/Penn State Univ./S. Dichiara; Infrared: NASA/ESA/STScI
Duration: 46 seconds
Release Date: March 10, 2026

#NASA #ESA #Astronomy #Space #Science #Stars #NeutronStars #StellarCollisions #Cosmos #Universe #NASAChandra #XrayAstronomy #CXC #HubbleSpaceTelescope #HST #InfraredAstronomy #ESA #Europe #STScI #UnitedStates #STEM #Education #Art #Illustration #HD #Video

Milky Way Galaxy View | International Space Station

Milky Way Galaxy View | International Space Station


NASA astronaut and former International Space Station flight engineer Don Pettit shared this photo: "The Milky Way as seen from the International Space Station with stars as points, rising sun, and cities as golden streaks below."

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

Image Credit: NASA/JSC/Don Pettit
Image Details: Taken with Nikon Z9, Sigma 14mm f1.4 lens, 15 seconds, f1.4, ISO 6400 with homemade orbital sidereal drive to compensate for orbital pitch rate (4 degrees/min)
Release Date: March 9, 2026

#NASA #Space #Astronomy #Science #ISS #Planets #Earth #Galaxies #MilkyWayGalaxy #DonPettit #AstronautPhotography #UnitedStates #ESA #France #Europe #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition71 #Expedition72 #STEM #Education

Monday, March 09, 2026

Planet Earth: Northern Lights of Alaska & Canada | International Space Station

Planet Earth: Northern Lights of Alaska & Canada | International Space Station

Expedition 74 Flight Engineer and NASA Astronaut Jessica Meir: "On my first mission I completely fell in love with space photography—tough not to when you’re graced with this kind of unique perspective of viewing all that Earth has to behold from above. I’ve been so happy to bust out the array of impressive lenses that we have up here once again, and this time with even better cameras (Nikon Z9, vs the D5 from my previous mission)."

"I was lucky enough to capture some pretty good aurora (northern lights, here over Alaska and Canada) on my first timelapse attempt of the mission, stay tuned for more!"

"Hoping for some impressive solar events to put on a fascinating show like the ones a few months ago."

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/
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.

Video Credit: NASA/Jessica Meir
Duration: 47 seconds
Release Date: March 9, 2026

#NASA #Space #Astronomy #Science #ISS #Planets #Earth #Aurora #NorthernLights #Alaska #Canada #Astronauts #JessicaMeir #AstronautPhotography #UnitedStates #ESA #France #Europe #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition74 #STEM #Education #HD #Video

Japan's HTV‑X1 Cargo Spacecraft Departs | International Space Station

Japan's HTV‑X1 Cargo Spacecraft Departs | International Space Station


The HTV‑X1 cargo spacecraft from the Japan Aerospace Exploration Agency (JAXA) is in the grasp of the Canadarm2 robotic arm after being detached from the Earth‑facing port of the International Space Station’s Harmony module. The orbital outpost was soaring 274 miles above the Pacific Ocean off the coast of South America’s Patagonia region at the time of this photograph. 

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.

Credit: NASA/Jessica Meir
Image Date: March 5, 2026

#NASA #Space #Astronomy #Science #ISS #Planets #Earth #HTVX1CargoSpacecraft #JAXA #宇宙航空研究開発機構 #Japan #日本 #Astronauts #JessicaMeir #AstronautPhotography #UnitedStates #ESA #France #Europe #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition74 #STEM #Education

Star Cluster NGC 6604 in Serpens Cauda: Wide-field view | Digitized Sky Survey 2

Star Cluster NGC 6604 in Serpens Cauda: Wide-field view | Digitized Sky Survey 2

This visible-light wide-field image of the region around the star cluster NGC 6604 was created from photographs taken through blue, red and infrared filters and forming part of the Digitized Sky Survey 2. The star cluster appears close to the center, as a knot of bright stars. This view shows the rich landscape of gas and dust clouds surrounding the cluster. The field of view is approximately 2.9 degrees across.

Distance from Earth: ~5500 light years

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: ESO and Digitized Sky Survey 2
Release Date: April 25, 2012

#NASA #ESO #Astronomy #Space #Science #Stars #StarClusters #NGC6604 #Sh254 #EagleNebula #SerpensCaudaConstellation #MilkyWayGalaxy #Cosmos #Universe #DSS2 #STScI #UnitedStates #STEM #Education

Journey to Star Cluster NGC 6604 in Serpens Cauda | ESO

Journey to Star Cluster NGC 6604  in Serpens Cauda | ESO

This zoom starts with a broad panorama of the brightest and most spectacular parts of the Milky Way. We slowly zoom in on a region featuring the famous Eagle Nebula, but the final object of attention is the star cluster NGC 6604 and its surrounding gas and dust clouds. The final view is a detailed image of the cluster’s environment from the Wide Field Imager attached to the MPG/ESO 2.2-meter telescope at the La Silla Observatory in Chile.

Distance from Earth: ~5500 light years

Learn more about the MPG/ESO 2.2-meter telescope:
https://www.eso.org/public/teles-instr/lasilla/mpg22/

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: European Southern Observatory (ESO)/Digitized Sky Survey 2/Nick Risinger
Duration: 56 seconds
Release Date: April 25, 2012

#NASA #ESO #Astronomy #Space #Science #Stars #StarClusters #NGC6604 #Sh254 #EagleNebula #SerpensCaudaConstellation #MilkyWayGalaxy #Cosmos #Universe #MPGESOTelescope #LaSillaObservatory #Chile #Europe #DSS2 #STScI #UnitedStates #STEM #Education #HD #Video

Close-up: Star Cluster NGC 6604 and its surroundings in Serpens Cauda | ESO

Close-up: Star Cluster NGC 6604 and its surroundings in Serpens Cauda | ESO

The star cluster NGC 6604 is shown in this image taken by the Wide Field Imager attached to the 2.2-meter MPG/European Southern Observatory telescope at the La Silla Observatory in Chile. NGC 6604 is the bright grouping towards to the upper left of the image. It is a young star cluster that is the densest part of a more widely scattered association containing about one hundred brilliant blue-white stars. The picture also shows the cluster’s associated nebula—a cloud of glowing hydrogen gas that is called Sh2-54—as well as dust clouds.

Distance from Earth: ~5500 light years

Learn more about the MPG/ESO 2.2-meter telescope:
https://www.eso.org/public/teles-instr/lasilla/mpg22/


Credit: European Southern Observatory (ESO)
Duration: 38 seconds
Release Date: April 25, 2012

#NASA #ESO #Astronomy #Space #Science #Stars #StarClusters #NGC6604 #Sh254 #SerpensCaudaConstellation #MilkyWayGalaxy #Cosmos #Universe #MPGESOTelescope #LaSillaObservatory #Chile #Europe #STEM #Education #HD #Video

Star Cluster NGC 6604 and its surroundings in Serpens Cauda | ESO

Star Cluster NGC 6604 and its surroundings in Serpens Cauda | ESO


The star cluster NGC 6604 is shown in this image taken by the Wide Field Imager attached to the 2.2-meter MPG/European Southern Observatory telescope at the La Silla Observatory in Chile. NGC 6604 is the bright grouping towards to the upper left of the image. It is a young star cluster that is the densest part of a more widely scattered association containing about one hundred brilliant blue-white stars. The picture also shows the cluster’s associated nebula—a cloud of glowing hydrogen gas that is called Sh2-54—as well as dust clouds.

Distance from Earth: ~5500 light years

Learn more about the MPG/ESO 2.2-meter telescope:
https://www.eso.org/public/teles-instr/lasilla/mpg22/


Credit: European Southern Observatory (ESO)
Release Date: April 25, 2012

#NASA #ESO #Astronomy #Space #Science #Stars #StarClusters #NGC6604 #Sh254 #SerpensCaudaConstellation #MilkyWayGalaxy #Cosmos #Universe #MPGESOTelescope #LaSillaObservatory #Chile #Europe #STEM #Education

Iridescence around The Sun: View from Colorado | Earth Science

Iridescence around The Sun: View from Colorado | Earth Science

Photographer Paul Robinson: "Strongly colored irridescent rings around the sun formed by cirrus clouds. 2pm MST"

Iridescence is a colorful optical phenomenon that can occur in the general proximity of the Sun. The colors resemble those seen in soap bubbles and oil on a water surface. The colors are usually pastel, but can be very vivid or mingled together, sometimes similar to mother-of-pearl. When appearing near the Sun, the effect can be difficult to spot as it is drowned in the Sun's glare. This may be overcome by shielding the sunlight with one's hand or hiding it behind a tree or building. Other aids are dark glasses, or observing the sky reflected in a convex mirror or in a pool of water.

Iridescence occurs when sunlight interacts with tiny water droplets or ice crystals suspended in the atmosphere. These microscopic particles act as tiny prisms, refracting and scattering light in such a way that it separates into its component colors, creating a stunning display of hues.

Iridescent clouds are an optical effect that can appear in various thin cloud layers, such as altocumulus, cirrocumulus, lenticular, and cirrus clouds. The phenomenon occurs when sunlight or moonlight interacts with small, uniform water droplets or ice crystals, scattering and diffracting the light to produce a spectrum of colors.

Colorado is a state in the Western United States. It is one of the Mountain states, and Southwestern region of the United States, sharing the Four Corners region with Arizona, New Mexico, and Utah. It is also bordered by Wyoming to the north, Nebraska to the northeast, Kansas to the east, and Oklahoma to the Southeast.


Image Credit: Paul Robinson
Location: Longmont, Colorado, USA
Date: Feb. 15, 2026

#NASA #Science #Planet #Earth #Atmosphere #CirrusClouds #IceCrystals #Sunlight #Iridescence #Photography #PaulRobinson #Photographer #CitizenScience #Longmont #Colorado #UnitedStates #STEM #Education

Stars & Gas Clouds around Milky Way's Supermassive Central Black Hole | ESO

Stars & Gas Clouds around Milky Way's Supermassive Central Black Hole | ESO

A new view on the heart of our Milky Way galaxy is presented in this picture taken with the European Southern Observatory’s Very Large Telescope (VLT). It reveals the stars and gas surrounding an invisible giant—a supermassive black hole, located about 27,000 light-years away. This is a hugely dynamic environment with stars and gas clouds passing by the black hole at high speeds.

A team of astronomers at the Max Planck Institute for Extraterrestrial Physics in Germany has detected a new gas cloud, named G2t, orbiting the supermassive black hole. Two gas clouds, G1 and G2, were already known, but their nature and origin were still being debated. In particular, it was unclear whether these clouds were hiding a star inside or consisted purely of gas. However, the discovery of a third gas cloud now helps answer these questions.

The observations were done with the Enhanced Resolution Imager and Spectrograph (ERIS) instrument on ESO’s VLT. Thanks to this, astronomers were able to measure the 3D orbits of the clouds around the black hole. The clouds move within a very small region at the center of this wide-field image. It was revealed that G1, G2 and G2t are on almost identical orbits, only rotated a bit with respect to each other. This rules out the possibility that each cloud hides a star in their core, as the odds of stars having almost identical orbits are slim. The similarity of the orbits suggests that the three clouds probably share the same origin, most likely IRS16SW, a pair of massive stars expelling an enormous amount of gas. As IRS16SW moves around the black hole, each cloud of gas is ejected in similar orbits, explaining the close trajectories of the ‘G-triplet’.

This discovery shows that despite decades of monitoring our Milky Way center new unanswered curiosities arise. 

Image Description: This image has a black background with thousands of light sources visible. There are stars closer and farther away present, appearing as simple white dots on the night sky. At image center, closer stars are gathered. These centered stars are embedded in a pinkish haze of gas.


Credit: European Southern Observatory (ESO)/D. Ribeiro for the MPE GC team
Release Date: March 9, 2026


#NASA #Astronomy #Space #Science #Galaxies #MilkyWayGalaxy #Stars #GasClouds #G1 #G2 #G2t #GCIRS #16SW #IRS16SW #SagittariusConstellation #Cosmos #Universe #VLT #ERIS #ParanalObservatory #Chile #SouthAmerica #MPE #Germany #Europe #STEM #Education

SpaceX Starship V3 Testing: Cryoproofing Complete for Flight 12 | Starbase Texas

SpaceX Starship V3 Testing: Cryoproofing Complete for Flight 12 | Starbase Texas

SpaceX Update: "Ship 39 cryoproof operations complete, the first campaign with a next generation Starship V3. Across several days, engineers tested the vehicle’s redesigned propellant system and its structural strength, including squeeze tests to mimic the forces of future ship catches."

SpaceX CEO Elon Musk Updates: "Starship V3 first flight in about 4 weeks. I am highly confident that the V3 design will achieve full reusability."

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.

"Starship is essential to both SpaceX’s plans to deploy its next-generation Starship system as well as for NASA, which will use a lunar lander version of Starship for landing astronauts on the Moon during the Artemis III 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)
Duration: 52 seconds
Date: March 7, 2026

#NASA #SpaceX #Space #Earth #Mars #Moon #MoonToMars #ArtemisProgram #ArtemisIII #Starship #StarshipSpacecraft #StarshipV3 #StarshipV3SN1 #StarshipFlight12 #ReusableSpacecraft #ElonMusk #Engineering #SpaceTechnology #HumanSpaceflight #CommercialSpace #SpaceExploration #StarbaseTexas #Texas #UnitedStates #STEM #Education #HD #Video

Sunday, March 08, 2026

Shenzhou-21 Crew Advances Experiments, Health Monitoring | China Space Station

Shenzhou-21 Crew Advances Experiments, Health Monitoring | China Space Station

China's Shenzhou-21 astronauts have steadily carried out in-orbit experiments, health monitoring, and maintenance tasks aboard the Tiangong Space Station over the past week, according to the China Manned Space Agency (CMSA).

The crew consists of mission commander Zhang Lu and astronauts Wu Fei and Zhang Hongzhang. They have spent over four months in orbit, and are all in good condition.

In the field of space medicine, the astronauts completed several studies including research on trust and cooperation mechanisms, human-machine trust in spaceflight, and intuitive physical behavior in microgravity.

The crew also used a space Raman spectrometer to analyze metabolic components in urine samples. The data collected will help researchers further refine indicator systems and evaluation criteria for related metabolic markers.

In addition, the astronauts used electroencephalography (EEG) equipment to gather data for experiments on metacognitive monitoring and group brain cognition-emotion analysis and regulation, supporting ongoing research by scientists on the ground.

In the area of microgravity physical science, the crew followed scheduled procedures to carry out maintenance and experiment operations. These included replacing a sampling cover in the combustion science experiment rack, performing vacuum pumping and exhaust removal, and changing experimental samples in the fluid physics experiment rack.

For station management, the crew conducted routine inspections of the space station platform and completed environmental monitoring tasks, such as dew point testing, temperature measurement, and wind speed monitoring to ensure a safe and habitable environment in orbit.

The astronauts also carried out several medical examinations, including intraocular pressure and fundus checks, body mass measurements, and cardiopulmonary fitness tests during exercise. They additionally used a traditional Chinese medicine diagnostic device to collect health data, allowing ground teams to closely monitor the crew's physical condition while in orbit.

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: 1 minute, 31 seconds
Release Date: March 9, 2026


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

Galaxy NGC 1275 in Perseus | WIYN Telescope

Galaxy NGC 1275 in Perseus | WIYN Telescope


This image shows a deep Hydrogen-alpha image of the brightest X-ray source in the sky, NGC 1275, taken by the WIYN 3.5-meter telescope at Kitt Peak National Observatory near Tucson, Arizona.

NGC 1275 is a type 1.5 Seyfert galaxy. Seyfert galaxies account for about 10% of all galaxies and are among the most intensely studied objects in astronomy, as they are thought to be powered by the same phenomena that occur in quasars, although they are closer and less luminous than quasars. These galaxies have supermassive black holes at their centers surrounded by accretion discs of in-falling material.

The filaments emanating from this galaxy are produced through largely unknown mechanisms, but they likely are the result of an interaction between the black hole in the center of the galaxy and the intracluster medium surrounding it. (The glowing background objects in this image are galaxies in that same galaxy cluster.)

At a distance of about 230 million light-years, this is the nearest example to Earth of such vast structures that are seen surrounding the most massive galaxies throughout the Universe.

NGC 1275 is a member of the large Perseus Cluster of galaxies. It was discovered by German-British astronomer William Herschel on October 17, 1786.

Learn more about the WIYN Observatory:
https://www.wiyn.org/0.9m/index.html

Credit: C. Conselice/Caltech and WIYN/NOIRLab/NSF/AURA
Release Date: July 18, 2005


#NASA #Astronomy #Space #Science #Galaxies #NGC1275 #PerseusA #Caldwell24 #SeyfertGalaxy #PerseusCluster #PerseusConstellation #MilkyWayGalaxy #Universe #WIYNTelescope #KPNO #KittPeakNationalObservatory #Arizona #NOIRLab #NOAO #NSF #AURA #UnitedStates #STEM #Education

Celebrating International Women’s Day | China Space Station

Celebrating International Women’s Day | China Space Station

💐Happy International Women’s Day❤️! 

Liu Yang: China's first female astronaut in space on June 16, 2012
Wang Yaping: First Chinese woman to work at Tiangong Space Station on a long duration mission, the first Chinese woman to perform a spacewalk, and record holder for longest stay in space by a female Chinese astronaut with a cumulative 197 days in space
Wang Haoze: China’s first female space engineer to work aboard China's Tiangong Space Station on a long duration mission

International Women's Day (IWD) is celebrated on March 8 each year, commemorating women's fight for equality along with the women's rights movement. China's national space program is celebrating International Women’s Day by recognizing three female taikonauts (astronauts):

Image 1: Liu Yang—China's first female astronaut in space on June 16, 2012

Image 2: Wang Yaping—First Chinese woman to work at Tiangong Space Station on a long duration mission, the first Chinese woman to perform a spacewalk, and record holder for longest stay in space by a female Chinese astronaut with a cumulative 197 days in space

Image 3: Wang HaozeChina’s first female space engineer to work aboard China's Tiangong Space Station

Follow the current Shenzhou-21 Mission at the China Space Station: 

Launched into space on October 31 last year, the Shenzhou-21 crew is now over 128 days into its six-month space mission. All tasks including scientific experiments, equipment maintenance and health management are progressing smoothly, according to China's space agency—the China National Space Administration (CNSA).

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


Image Credit: China National Space Administration (CNSA)
Release Date: March 8, 2026


#NASA #Space #Science #China #中国 #ChineseWomen #InternationalWomensDay #IWD2026  #GenderEquality #Taikonauts #Astronauts #LiuYang #WangYaping #WangHaoze #Shenzhou21Mission #神舟二十一号 #Shenzhou21 #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #SpaceLaboratory #CNSA #国家航天局 #HumanSpaceflight #STEM #Education

Mysterious Object CK Vulpeculae: Wide-field view | Digitized Sky Survey 2

Mysterious Object CK Vulpeculae: Wide-field view | Digitized Sky Survey 2


This wide-field view shows the sky around the location of the historical exploding star CK Vulpeculae (in the constellation Vulpecula) that European astronomers saw in 1670. The remains of the nova are only very faintly visible at the center of this picture.

The star was not a typical nova, but may have been a much rarer, violent breed of stellar collision. A nova is a sudden and dramatic increase in the brightness of a star. CK Vulpeculae was spectacular enough to be easily seen with the naked eye during its first outburst, but the traces it left were so faint that very careful analysis using submillimeter telescopes is required.

Distance to Earth: ~10,000 light years

Models suggest CK Vulpeculae may not be a classic nova; rather it may be classified as a luminous red nova that is the result of two main sequence stars colliding and merging. A 2018 study found it was most likely the result of an unusual collision of a white dwarf star and a brown dwarf star. However, a 2020 article ruled out this proposed mechanism and proposes that CK Vulpeculae is an intermediate luminosity optical transient (ILOT), another type of object in the luminosity gap between supernovae and novae.

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: ESO/Digitized Sky Survey 2. Acknowledgement: Davide De Martin
Release Date: July 30, 2018


#NASA #Astronomy #Space #Science #Stars #Nebulae #CKVulpeculae #NovaVulpeculae1670 #StellarObjects #AstronomicalObjects #ILOT #VulpeculaConstellation #Cosmos #Universe #ESO #Chile #Europe #DSS2 #STScI #UnitedStates #STEM #Education

Journey to Mysterious Object CK Vulpeculae: Appeared in Year 1670

Journey to Mysterious Object CK Vulpeculae: Appeared in Year 1670

This video sequence takes the viewer deep into a rich part of the northern Milky Way in the constellation of Vulpecula (The Fox), close to the more famous constellation of Cygnus (The Swan) to the enigmatic CK Vulpeculae nebula. Using radio telescope data from the Atacama Pathfinder Experiment (APEX) in Chile, the Hawaiian Submillimeter Array (SMA) and visible light data from the Gemini North Observatory in Hawaii, the final picture shows the remains of the new star that was seen in the year 1670. This view was created from a combination of visible-light images from the Gemini telescope (blue), a submillimeter map showing the dust from the SMA (yellow) and finally a map of the molecular emission from APEX and the SMA (red).

Distance to Earth: ~10,000 light years

The star that European astronomers saw in 1670 was not a typical nova, but may have been a much rarer, violent breed of stellar collision. A nova is a sudden and dramatic increase in the brightness of a star. CK Vulpeculae was spectacular enough to be easily seen with the naked eye during its first outburst, but the traces it left were so faint that very careful analysis using submillimeter telescopes is required.

Models suggest CK Vulpeculae may not be a classic nova; rather it may be classified as a luminous red nova that is the result of two main sequence stars colliding and merging. A 2018 study found it was most likely the result of an unusual collision of a white dwarf star and a brown dwarf star. However, a 2020 article ruled out this proposed mechanism and proposes that CK Vulpeculae is an intermediate luminosity optical transient (ILOT), another type of object in the luminosity gap between supernovae and novae.

Learn about APEX & SMA:

Credit: ESO/T. Kamiński
Release Date: March 23, 2015

#NASA #Astronomy #Space #Science #Stars #Nebulae #CKVulpeculae #NovaVulpeculae1670 #StellarObjects #AstronomicalObjects #ILOT #VulpeculaConstellation #Universe #InternationalGeminiObservatory #GeminiNorthTelescope #SMA #Maunakea #Hawaii #NOIRLab #NSF #AURA #UnitedStates #ESO #APEX #Chile #STEM #Education #HD #Video

Mysterious Object CK Vulpeculae from Year 1670 | Radio & Visible Light Views

Mysterious Object CK Vulpeculae from Year 1670 | Radio & Visible Light Views

The enigmatic CK Vulpeculae nebula. Using radio telescope data from the Atacama Pathfinder Experiment (APEX) in Chile, the Hawaiian Submillimeter Array (SMA) and visible light data from the Gemini North Observatory in Hawaii, this picture shows the remains of the new star that was seen in the year 1670. This view was created from a combination of visible-light images from the Gemini telescope (blue), a submillimeter map showing the dust from the SMA (yellow) and finally a map of the molecular emission from APEX and the SMA (red).

Distance to Earth: ~10,000 light years

The star that European astronomers saw in 1670 was not a typical nova, but may have been a much rarer, violent breed of stellar collision. A nova is a sudden and dramatic increase in the brightness of a star. CK Vulpeculae was spectacular enough to be easily seen with the naked eye during its first outburst, but the traces it left were so faint that very careful analysis using submillimeter telescopes is required.

Distance to Earth: ~10,000 light years

Models suggest CK Vulpeculae may not be a classic nova; rather it may be classified as a luminous red nova that is the result of two main sequence stars colliding and merging. A 2018 study found it was most likely the result of an unusual collision of a white dwarf star and a brown dwarf star. However, a 2020 article ruled out this proposed mechanism and proposes that CK Vulpeculae is an intermediate luminosity optical transient (ILOT), another type of object in the luminosity gap between supernovae and novae.

Learn about APEX & SMA:

Credit: ESO/T. Kamiński
Release Date: March 23, 2015

#NASA #Astronomy #Space #Science #Stars #Nebulae #CKVulpeculae #NovaVulpeculae1670 #StellarObjects #AstronomicalObjects #ILOT #VulpeculaConstellation #Universe #InternationalGeminiObservatory #GeminiNorthTelescope #SMA #Maunakea #Hawaii #NOIRLab #NSF #AURA #UnitedStates #ESO #APEX #Chile #STEM #Education

Mysterious Object CK Vulpeculae: Appeared in Year 1670 | Gemini North Telescope

Mysterious Object CK Vulpeculae: Appeared in Year 1670 | Gemini North Telescope

The enigmatic CK Vulpeculae nebula. This picture shows the remains of the new star that was seen in the year 1670. The star that European astronomers saw in 1670 was not a typical nova, but may have been a much rarer, violent breed of stellar collision. A nova is a sudden and dramatic increase in the brightness of a star. CK Vulpeculae was spectacular enough to be easily seen with the naked eye during its first outburst, but the traces it left were so faint that very careful analysis using submillimeter telescopes is required.

Distance to Earth: ~10,000 light years

Models suggest CK Vulpeculae may not be a classic nova; rather it may be classified as a luminous red nova that is the result of two main sequence stars colliding and merging. A 2018 study found it was most likely the result of an unusual collision of a white dwarf star and a brown dwarf star. However, a 2020 article ruled out this proposed mechanism and proposes that CK Vulpeculae is an intermediate luminosity optical transient (ILOT), another type of object in the luminosity gap between supernovae and novae.


Credit: International Gemini Observatory/NOIRLab/NSF/AURA
Image Processing: Travis Rector (University of Alaska Anchorage), Jen Miller (Gemini Observatory/NSF NOIRLab), Mahdi Zamani & Davide de Martin
Release Date: March 23, 2015

#NASA #Astronomy #Space #Science #Stars #Nebulae #CKVulpeculae #NovaVulpeculae1670 #StellarObjects #AstronomicalObjects #ILOT #VulpeculaConstellation #Cosmos #Universe #InternationalGeminiObservatory #GeminiNorthTelescope #Maunakea #Hawaii #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

Planet Earth Lightning Flashes | International Space Station

Planet Earth Lightning Flashes | International Space Station


NASA astronaut Don Pettit shared this photo: "Lightning appears as bright blue flashes across the time history of our orbit seen in these exposures from the International Space Station. And visualize the intensity of the storm!"

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

Image Credit: NASA's Johnson Space Center
Duration: 6 seconds
Release Date: March 5, 2026

#NASA #Space #Astronomy #Science #ISS #Planets #Earth #Atmosphere #Meteorology #LightningStorms #Astronauts #DonPettit #AstronautPhotography #UnitedStates #ESA #France #Europe #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition71 #Expedition72 #STEM #Education #HD #Video

Soaring above The Pacific Ocean with Airglow | International Space Station

Soaring above The Pacific Ocean with Airglow | International Space Station

The International Space Station was soaring 263 miles above the Pacific Ocean near the island of Hawaii when this 30‑second long‑duration photograph was taken, revealing Earth’s atmospheric glow and star trails at approximately midnight local time.

You will notice layers of red, orange and yellow airglow in this image. Airglow occurs when atoms and molecules in the Earth's upper atmosphere, excited by sunlight, emit light to shed their excess energy. Or, it can happen when atoms and molecules that have been ionized by sunlight collide with and capture a free electron. In both cases, they eject a particle of light—called a photon—in order to relax again. The phenomenon is similar to auroras, but where auroras are driven by high-energy particles originating from the solar wind, airglow is energized by ordinary, day-to-day solar radiation. 

Unlike episodic and fleeting auroras, airglow shines constantly throughout Earth’s atmosphere, and the result is a tenuous bubble of light that closely encases our entire planet. (Auroras, on the other hand, are usually constrained to Earth’s poles.) Just a tenth as bright as all the stars in the night sky, airglow is far more subdued than auroras, too dim to observe easily except in orbit or on the ground with clear, dark skies and a sensitive camera.

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.

Credit: NASA/Chris Williams
Image Date: Feb. 24, 2026

#NASA #Space #Astronomy #Science #ISS #Planets #Earth #Atmosphere #Airglow #PacificOcean #Astronauts #ChrisWilliams #AstronautPhotography #UnitedStates #ESA #France #Europe #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition74 #STEM #Education

"The Aurora Tree"

"The Aurora Tree"

Pictured is a visual coincidence between the dark branches of a nearby tree and bright glow of a distant aurora. The beauty of the aurora—combined with how it seemed to mimic a tree right nearby—mesmerized the photographer to such a degree that he momentarily forgot to take pictures. When viewed at the right angle, it seemed that this tree had aurora for leaves. Fortunately, before the aurora morphed into a different overall shape, he came to his senses and captured the awe-inspiring momentary coincidence. 

Typically triggered by solar explosions, aurora are caused by high energy electrons impacting the Earth's atmosphere around 150 kilometers up. The unusual Earth-sky collaboration was witnessed during March 2017 in Iceland.

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 Description: A leafless tree is pictured below a starry sky. In the sky behind the tree is an aurora glowing mostly green, along with purple. The shape of the aurora seems to follow the branches of the tree.


Image Credit & Copyright: Alyn Wallace
Alyn's Website: 
https://www.instagram.com/alynwallace/
Image Date: March 2017
Release Date: March 8, 2026

#NASA #Astronomy #Space #Science #Planets #Earth #Aurora #AuroraBorealis #NorthernLights #MagneticField #Magnetosphere #SolarWind #Sun #Stars #Photography #AlynWallace #Photographer #CitizenScience #Iceland #NASAGoddard #GSFC #UnitedStates #STEM #Education #APoD

Saturday, March 07, 2026

SpaceX Starship V3: Preparing for Flight 11—A Retrospective | Starbase Texas

SpaceX Starship V3: Preparing for Flight 11—A Retrospective | Starbase Texas

SpaceX CEO Elon Musk Updates: "Starship V3 first flight in about 4 weeks. I am highly confident that the V3 design will achieve full reusability."

"Starship is essential to both SpaceX’s plans to deploy its next-generation Starship system as well as for NASA, which will use a lunar lander version of Starship for landing astronauts on the Moon during the Artemis III 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)
Date: March 7, 2026

#NASA #SpaceX #Space #Earth #Mars #Moon #MoonToMars #ArtemisProgram #ArtemisIII #Starship #StarshipSpacecraft #StarshipV3 #StarshipV3SN1 #StarshipFlight11 #ReusableSpacecraft #ElonMusk #Engineering #SpaceTechnology #HumanSpaceflight #CommercialSpace #SpaceExploration #StarbaseTexas #Texas #UnitedStates #STEM #Education #HD #Video

China Long March-8A Rocket Moved to Launch Area in Hainan

China Long March-8A Rocket Moved to Launchpad in Hainan


A Long March 8A carrier rocket was transferred to the launch pad at Hainan commercial spacecraft launch site in southern China on Saturday, March 7, 2026, for an upcoming mission. The Long March-8A carrier rocket, designed by the China Academy of Launch Vehicle Technology (CALT), represents a significant upgrade to the Long March-8 series. It successfully conducted its maiden flight on Feb. 11, 2025.

The rocket, 50.5 meters long with a takeoff weight of 371 tonnes, is capable of carrying up to seven tonnes to a sun-synchronous orbit at an altitude of 700 km. It is designed specifically for high-density, rapid constellation deployment, serving as a core vehicle for China's satellite internet constellation construction.

So far, it has successfully completed seven missions. About 15 launch missions are scheduled for the Long March 8 series rockets this year, involving the Long March 8A and Long March 8 rockets.

As a new-generation medium-lift liquid-fueled carrier rocket, the Long March 8 series rockets have become the mainstay for China's low-to-medium orbit satellite launches since its maiden flight, thanks to its modular design, high cost-effectiveness, and rapid response capabilities.

Hainan International Commercial Aerospace Launch Co., Ltd., or HICAL, is a Chinese state-owned company that operates the Wenchang Commercial Space Launch Site, China's first commercial spaceport. Established in 2022, HICAL is the first commercially incorporated company in China to independently own and manage a spaceport.


Video Credit: CCTV
Duration: 48 seconds
Release Date: March 7, 2026

#NASA #Space #China #中国 #Satellites #RocketLaunch #LongMarch8A #长征八号运载火箭 #LongMarch8ARocket #CALT #CommercialSpace #SpaceTechnology #Engineering #HICAL #WCSLS #文昌商业航天发射场 #Spaceports #Hainan #STEM #Education #HD #Video

Journey to Newborn Star HH 46/47 in Vela | New Technology Telescope

Journey to Newborn Star HH 46/47 in Vela | New Technology Telescope

This zoom sequence starts with a wide view of the southern Milky Way and then closes in on a rich region of dark clouds and young stars in the constellation of Vela (The Sails). One of these dark star-forming clouds features the Herbig-Haro object HH 46/47 where jets from a young star are colliding with the surrounding material. 


The final image of Herbig-Haro object HH 46/47 was captured by the European Southern Observatory’s New Technology Telescope at the La Silla Observatory in Chile.

Distance: 1,400 light years

Learn more about ESO's New Technology Telescope:
https://www.eso.org/public/teles-instr/lasilla/ntt/

Credit: ESO/Digitized Sky Survey 2/Nick Risinger 
Duration: 56 seconds
Release Date: Aug. 20, 2013

#NASA #ESO #Astronomy #Space #Science #Stars #StarFormation #HH4647 #HerbigHaroObject #StellarJets #CircumstellarMaterial #VelaConstellation #MilkyWayGalaxy #Cosmos #Universe #NTTTelescope #LaSillaObservatory #Chile #Europe #STEM #Education #HD #Video