Planet Mars Images: March 5-11, 2026 | NASA's Perseverance Rover
Friends of NASA (FoN) is an independent non-governmental organization (NGO) dedicated to building international support for peaceful space exploration, commerce, scientific discovery, and STEM education.
Thursday, March 12, 2026
Planet Mars Images: March 5-11, 2026 | NASA's Perseverance Rover
Wednesday, March 11, 2026
China's Space Program Reaching New Heights
China's Space Program Reaching New Heights
China's space program has undergone a significant transformation over the last five years. It will reach even greater heights in the next five. From the China Space Station to deep-space exploration, China is charting an extraordinary course through the cosmos. This episode of CGTN's special series Charting the Future zooms in on the country's space program.
Duration: 4 minutes, 38 seconds
Release Date: March 10, 2026
What is Dark Matter and Dark Energy? | NASA Science
What is Dark Matter and Dark Energy? | NASA Science
Dida Markovic - Astrophysicist at NASA JPL
Jason Rhodes - Astrophysicist at NASA JPL
Eric Huff - Astrophysicist at NASA JPL
Host and Co-Producer: Chelsea Gohd
Editor/Director/Co-Producer: Keith Miller (Caltech-IPAC)
Science Visualizations/Co-Producer: Robert Hurt (Caltech-IPAC)
Duration: 6 minutes
Release Date: March 11, 2026
Planet Mars: Dune Field of Matara Crater | NASA's Mars Reconnaissance Orbiter
Planet Mars: Dune Field of Matara Crater | NASA's Mars Reconnaissance Orbiter
NASA's Mars Reconnaissance Orbiter (MRO) has spent over twenty years (2006-2026) orbiting the Red Planet, collecting valuable scientific data. Matara Crater is a favorite image owing to the massive and gorgeous sand sheet that dominates the floor. We often image these dunes for the gullies that form on them due to carbon dioxide ice. Matara is located in Noachis Terra and is 48 kilometers (30 mi) in diameter. This crater is notable for its large sand deposit and dune features that are sculpted by the wind.
Noachis Terra is an extensive southern landmass (terra). It lies west of the giant Hellas impact basin, roughly between the latitudes −20° and −80° and longitudes 30° west and 30° east, centered on 45°S 350°E. It is in the Noachis quadrangle.
This is a non-narrated clip with ambient sound. Image is less than 5 km (3 mi) across and the spacecraft altitude was 251 km (156 mi).
The University of Arizona, in Tucson, operates the High Resolution Imaging Science Experiment (HiRISE). It was built by BAE Systems in Boulder, Colorado. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate (SMD), Washington.
Duration: 3 minutes, 30 seconds
Release Date: July 4, 2023
#NASA #Space #Astronomy #Science #Mars #Planet #RedPlanet #Geology #Geoscience #Landscape #Terrain #SandDunes #Gullies #CarbonDioxideIce #MataraCrater #NoachisTerra #SouthernHemisphere #MRO #MarsOrbiter #MarsSpacecraft #HiRISECamera #JPL #Caltech #UA #UnitedStates #STEM #Education #HD #Video
How America's New Vera C. Rubin Observatory Maps the Universe Each Night
How America's New Vera C. Rubin Observatory Maps the Universe Each Night
Each night, Rubin produces 10 terabytes of data to map and survey the universe and generates millions of alerts about changing objects to help scientists zoom in with other telescopes, including the James Webb and Hubble space telescopes or ground-based instruments.
The United States Department of Energy-National Science Foundation Vera C. Rubin Observatory is about to change how we explore the universe. In this video, we break down how Rubin runs the Legacy Survey of Space and Time (LSST), what its images contain, how the data gets processed, and why this observatory is designed as a discovery engine for the entire science community. You will also see Rubin first-light imagery presented with scientifically accurate scaling and positioning against a real 360° all-sky backdrop.
https://rubinobservatory.org
Rubin’s survey is not about single, ultra-detailed snapshots like space telescopes. Instead, Rubin revisits the same regions again and again, building a 10-year time-lapse of the entire southern sky. This allows scientists to detect changes—moving asteroids, exploding stars, variable objects, and subtle shifts that only appear when you compare new images to a reference set of images of the entire southern sky.
Rubin and space telescopes serve complementary roles. Rubin finds what is new and changing, then issues alerts and targets of interest so that deeper, narrower-field observatories like the James Webb Space Telescope and the Hubble Space Telescope can zoom in and study those objects in close detail. Rubin will also create yearly highly detailed catalogs of 20 billion galaxies in our universe, 17 billion stars in the Milky Way, and millions of objects in the solar system.
Rubin is a ground-based observatory located on Cerro Pachón in northern Chile at 2,680 meters elevation. That site combines altitude, dry air, and stable conditions that are ideal for wide-field survey astronomy. Being ground-based is key to Rubin’s speed. The telescope is engineered to take 15-30 seconds exposures every 30-40 seconds. It slews and settles quickly to the next field while tracking precisely to compensate for Earth’s rotation during each exposure. Rubin’s data processing system also detects and removes artifacts such as satellite streaks (by combining multiple images of the same area) so they do not contaminate the final data products.
NSF–DOE Vera C. Rubin Observatory is a joint initiative of the U.S. National Science Foundation (NSF) and the U.S. Department of Energy’s Office of Science. Rubin is operated jointly by NSF NOIRLab and SLAC National Accelerator Laboratory.
Presenter: Phil Marshall, Deputy Director of Operations, Rubin Observatory/SLAC
Duration: 5 minutes, 33 seconds
Release Date: March 11, 2026
Galaxy UGC 4879 in Ursa Major: "A Mysterious Hermit" | Hubble
Galaxy UGC 4879 in Ursa Major: "A Mysterious Hermit" | Hubble
This galaxy is also very isolated. There are about 2.3 million light years between UGC 4879 and its closest neighbor, Leo A. This is about the same distance as that between the Andromeda Galaxy and the Milky Way.
Distance from Earth: ~4 million light years
This galaxy’s isolation means that it has not interacted with any surrounding galaxies, making it an ideal laboratory for studying star formation uncomplicated by interactions with other galaxies. Studies of UGC 4879 have revealed a significant amount of star formation in the first 4-billion-years after the Big Bang, followed by a strange nine-billion-year lull in star formation, ended 1-billion-years ago by a more recent reignition. The reason for this behavior, however, remains mysterious, and the solitary galaxy continues to provide ample study material for astronomers looking to understand the complex mysteries of starbirth throughout the Universe.
The Hubble Space Telescope is a joint ESA/NASA project and was launched in 1990 by the Space Shuttle mission STS-31 into a low-Earth orbit 600 km above the ground. During its lifetime Hubble has become one of the most important science projects ever.
Release Date: June 6, 2016
#NASA #ESA #Astronomy #Space #Science #Galaxies #UGC4879 #IrregularGalaxies #DwarfGalaxies #UrsaMajorConstellation #MilkyWayGalaxy #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education
Reflection Nebula GGD 27 in Sagittarius (near-infrared) | Gemini South Telescope
Reflection Nebula GGD 27 in Sagittarius (near-infrared) | Gemini South Telescope
Gemini South Telescope:
https://noirlab.edu/public/programs/gemini-observatory/gemini-south/
Release Date: Dec. 29, 2016
#NASA #Astronomy #Space #Science #Nebulae #GD27 #ReflectionNebula #Stars #Protostars #GGD27ILL #StellarNurseries #SagittariusConstellation #Cosmos #Universe #InternationalGeminiObservatory #GeminiSouthTelescope #FLAMINGOS2 #InfraredAstronomy #GeminiObservatory #CerroPachón #Chile #NOIRLab #AURA #NSF #UnitedStates #STEM #Education
Planet Mars Images: March 6-10, 2026 | NASA's Curiosity & Perseverance Rovers
Planet Mars Images: March 6-10, 2026 | NASA's Curiosity & Perseverance Rovers
Delhi and Indian subcontinent at night | International Space Station
Delhi and Indian subcontinent at night | International Space Station
The well‑lit nighttime cityscape of the Indian subcontinent is highlighted by Delhi (center top), the capital territory of India with a metropolitan population of about 33.8 million. The International Space Station was orbiting 264 miles above southwestern China at approximately 11:21 p.m. local time when this photograph was taken.
Delhi, officially the National Capital Territory (NCT) of Delhi, is a megacity and a union territory of India containing New Delhi, the capital of India. Straddling the Yamuna river, but spread chiefly to the west, or beyond its right bank, Delhi shares borders with the state of Uttar Pradesh in the east and with the state of Haryana in the remaining directions.
Station Commander: Sergey-Kud Sverchkov (Russia)
Roscosmos (Russia) Flight Engineers: Andrey Fedyaev, Sergei Mikaev
Image Date: Feb. 28, 2026
Tuesday, March 10, 2026
Mars Telecommunications Orbiter | Rocket Lab
Mars Telecommunications Orbiter | Rocket Lab
"Proven hardware. Proven team. Proven Mars experience."
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.
Release Date: Dec. 8, 2014
The Sun: View from Canary Islands
The Sun: View from Canary Islands
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.
Location: Ashokan Reservoir, New York, United States
Release Date: March 9, 2026
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.
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.
X-ray: NASA/CXC/Penn State Univ./S. Dichiara; Infrared: NASA/ESA/STScI
Duration: 46 seconds
Release Date: March 10, 2026
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."
Release Date: March 9, 2026
















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