Thirty Seconds on Planet Mars | NASA Curiosity Rover Panorama
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Wednesday, May 21, 2025
Thirty Seconds on Planet Mars | NASA Curiosity Rover Panorama
CAS Space Lijian-1 Y7 Commercial Rocket Launches Six Satellites
CAS Space Lijian-1 Y7 Commercial Rocket Launches Six Satellites
CAS Space is a Chinese commercial space launch provider based in Guangzhou, capital and largest city of Guangdong province in southern China. CAS Space was founded in 2018 and is majority owned by the Chinese Academy of Sciences (CAS).
The Jiuquan Satellite Launch Center (JSLC) was founded in 1958. It was the first of China's four spaceports. The launch center has been the focus of many of China's historic space ventures, including the country's first satellite Dong Fang Hong I in 1970 and their first crewed space mission, Shenzhou V, on October 15, 2003. JSLC is now a home for many new Chinese launch firms, like CAS Space.
Release Date: May 21, 2025
CAS Space Lijian-1 Y7 Commercial Rocket Launch: Six Satellites Delivered to Orbit
CAS Space Lijian-1 Y7 Commercial Rocket Launch: Six Satellites Delivered to Orbit
CAS Space is a Chinese commercial space launch provider based in Guangzhou, capital and largest city of Guangdong province in southern China. It was founded in 2018 and is majority owned by the Chinese Academy of Sciences (CAS).
The Jiuquan Satellite Launch Center (JSLC) was founded in 1958. It was the first of China's four spaceports. The launch center has been the focus of many of China's historic space ventures, including the country's first satellite Dong Fang Hong I in 1970 and their first crewed space mission, Shenzhou V, on October 15, 2003. JSLC is now a home for many new Chinese launch firms, like CAS Space.
Release Date: May 21, 2025
Wide-field View of Interacting Galaxies: A 'Cosmic Joust' | DESI Legacy Survey
Wide-field View of Interacting Galaxies: A 'Cosmic Joust' | DESI Legacy Survey
Release Date: May 21, 2025
#NASA #ESO #Space #Astronomy #Science #Galaxies #GalacticMerger #InteractingGalaxies #Quasars #Blackholes #Cosmos #Universe #DESILegacySurvey #UniteStates #STEM #Education
Zooming to a Pair of Merging Galaxies | ESO
Zooming to a Pair of Merging Galaxies | ESO
This video zooms into a galactic merging event in deep space, like a ‘cosmic joust’. One of these galaxies is piercing the other with intense radiation, emitted by a quasar at its core. This radiation is disrupting the gas and dust inside the other galaxy, dampening its ability to form stars.
Using the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers resolved these two galaxies despite how close they are to each other in the sky. Using the X-shooter instrument on the European Southern Observatory’s Very Large Telescope (VLT), they examined how radiation affected the material inside the galaxy being bombarded by a quasar.
The various images shown here were blended together to create this zoom. They come from a range of telescopes, observing at distinct times, ending with a close-up of the galaxies as seen by ALMA. At the very end, we see an artist’s illustration depicting how the beam of radiation affects the companion galaxy.
Duration: 1 minute
Release Date: May 21, 2025
#NASA #ESO #Space #Astronomy #Science #Galaxies #GalacticMerger #InteractingGalaxies #Quasars #Blackholes #Universe #VLT #ParanalObservatory #Chile #Europe #RadioAstronomy #ALMA #NSF #NRAO #UnitedStates #NAOJ #Japan #日本 #Art #Illustration #STEM #Education #HD #Video
Galactic Merger: Intense Black Hole-powered Quasar Radiation Observed | ESO
Galactic Merger: Intense Black Hole-powered Quasar Radiation Observed | ESO
Astronomers have witnessed a violent galactic merger in deep space. Like a ‘cosmic joust’, one galaxy is affecting another with a cone of intense radiation. The results of their analysis, using the European Southern Observatory’s Very Large Telescope (VLT) and the Atacama Large Millimeter/submillimeter Array (ALMA), show that this radiation is disrupting the gas and dust within the other galaxy reducing its star formation.
The source of the radiation is a quasar in one of the galaxies. Quasars are the bright cores of distant galaxies that are powered by supermassive black holes, releasing huge amounts of radiation. Quasars and galaxy mergers used to be far more common, appearing more frequently in the Universe’s first few billion years, so to observe them astronomers peer into the distant past with powerful telescopes. The light from this ‘cosmic joust’ has taken over 11 billion years to reach us, so we see it as it was when the Universe was only 18% of its current age.
Directed by: Angelos Tsaousis and Martin Wallner
Editing: Angelos Tsaousis
Written by: Amy Briggs and Sean Bromilow
Footage and photos: ESO/Luis Calçada, Cristoph Malin, Martin Kornmesser, Angelos Tsaousis, Babak Tafreshi, Jose Porte, ALMA (ESO/NAOJ/NRAO)/S. Balashev and P. Noterdaeme et al.
Scientific consultant: Paola Amico, Mariya Lyubenova
Duration: 2 minutes
Release Date: May 21, 2025
#NASA #ESO #Space #Astronomy #Science #Galaxies #GalacticMerger #InteractingGalaxies #Quasars #Blackholes #Universe #VLT #ParanalObservatory #Chile #Europe #RadioAstronomy #ALMA #NSF #NRAO #UnitedStates #NAOJ #Japan #日本 #STEM #Education #HD #Video
China Launches Lijian-1 Y7 Rocket, Sending Six Satellites into Orbit
China Launches Lijian-1 Y7 Rocket, Sending Six Satellites into Orbit
China launched its Lijian-1 Y7 carrier rocket from the Jiuquan Satellite Launch Center in northwest China on May 21, 2025, placing six satellites into orbit. This marks the seventh launch of the Lijian-1 carrier rocket series.
CAS Space is a Chinese commercial space launch provider based in Guangzhou. It was founded in 2018 and majority owned by the Chinese Academy of Sciences (CAS).
The Jiuquan Satellite Launch Center (JSLC) was founded in 1958. It was the first of China's four spaceports. The launch center has been the focus of many of China's historic space ventures, including the country's first satellite Dong Fang Hong I in 1970 and their first crewed space mission, Shenzhou V, on October 15, 2003. JSLC is now a home for many new Chinese launch firms, like CAS Space.
Release Date: May 21, 2025
Starlink Constellations: Orbital View | International Space Station
Starlink Constellations: Orbital View | International Space Station
https://blogs.nasa.gov/spacestation/
Roscosmos (Russia) Flight Engineers: Kirill Peskov, Sergey Ryzhikov, Alexey Zubritskiy
https://www.nasa.gov/iss-science
Science, Technology, Engineering, Math (STEM)
Image Credit: NASA's Johnson Space Center
Release Date: May 20, 2025
#NASA #Space #ISS #Science #Stars #Earth #Satellites #Starlink #Astronauts #DonPettit #AstronautPhotography #UnitedStates #Japan #日本 #JAXA #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition72 #Expedition73 #STEM #Education
How Big is Space? We Asked a NASA Expert
How Big is Space? We Asked a NASA Expert
How big is space? It is one of the most mind-bending questions we can ask because the deeper we look, the more the universe keeps going. We have measured billions of light-years in every direction and still have not reached the edge.
A NASA scientists explains what we know—and do not know—about the size of the cosmos.
https://science.nasa.gov/exoplanets/what-is-the-universe/
Producers: Scott Bednar, Pedro Cota, Jessie Wilde
Editor: Daniel Salazar
Duration: 1 minute, 36 seconds
Release Date: May 21, 2025
Tuesday, May 20, 2025
China Long March-7A Rocket Launch of Communication Satellite in Hainan
China Long March-7A Rocket Launch of Communication Satellite in Hainan
🚀A China Long March-7A carrier rocket successfully launched the ChinaSat3B satellite at 7:50 p.m. (Beijing Time) on May 20, 2025, from the Wenchang Space Launch Site in the southern island province of Hainan. The satellite will provide voice, data, radio, and television transmission services.
This marks the second Long March-7A rocket launch mission of 2025, utilizing its basic configuration with a 4.2-meter-diameter fairing. Known as Bingjian or "Ice Arrow," this 60.1-meter-long medium-lift liquid-fueled rocket is powered by kerosene and liquid oxygen. It can carry up to 7 metric tons of payload to geosynchronous transfer orbit (GTO) with an optional third stage. The Long March 7 aims to handle 70% of China's annual launches, solidifying its role in the nation's space endeavors. Long March 7 also plays a critical role in the China Space Station program. It is used to launch the Tianzhou robotic cargo and resupply spacecraft to the station.
Capture Date: May 20, 2025
Exploring Planet Jupiter: New Perijove 72 Images | NASA Juno Mission
Exploring Planet Jupiter: New Perijove 72 Images | NASA Juno Mission
China Long March-7A Rocket Launches Communication Satellite in Hainan
China Long March-7A Rocket Launches Communication Satellite in Hainan
🚀A China Long March-7A carrier rocket successfully launched the ChinaSat3B satellite at 7:50 p.m. (Beijing Time) on May 20, 2025, from the Wenchang Space Launch Site in the southern island province of Hainan. The satellite will provide voice, data, radio, and television transmission services.
This marks the second Long March-7A rocket launch mission of 2025, utilizing its basic configuration with a 4.2-meter-diameter fairing. Known as Bingjian or "Ice Arrow," this 60.1-meter-long medium-lift liquid-fueled rocket is powered by kerosene and liquid oxygen. It can carry up to 7 metric tons of payload to geosynchronous transfer orbit (GTO) with an optional third stage. The Long March 7 aims to handle 70% of China's annual launches, solidifying its role in the nation's space endeavors. Long March 7 also plays a critical role in the China Space Station program. It is used to launch the Tianzhou robotic cargo and resupply spacecraft to the station.
Capture Date: May 20, 2025
Why is Neptune Glowing Like This? | NASA
Why is Neptune Glowing Like This? | NASA
Neptune is glowing—and it is not what we expected. NASA’s James Webb Space Telescope just spotted auroras stretching across Neptune’s mid-latitudes—not the poles. Why? The planet’s bizarre magnetic field and a shockingly cold upper atmosphere may hold the answer.
These new findings are rewriting what we know about the solar system’s most distant planet.
Watch to see how Webb is revealing Neptune in a whole new light.
For more information, visit: https://nasa.gov/webb
Producer: Paul Morris
Writer: Thaddeus Cesari
Narrator: Dr. Quyen Hart
Images: NASA, ESA, CSA, STSci
Duration: 3 minutes
Release Date: May 20, 2025
Planet Mars: Cloudy Giant Shield Volcano Ascraeus Mons | Europe's Mars Express
Planet Mars: Cloudy Giant Shield Volcano Ascraeus Mons | Europe's Mars Express
ESA Mars Express Instrument: High Resolution Stereo Camera (HRSC)
Orbit: 24799
The orbiter will continue its study of Mars until at least the end of 2026, with a special extension from January 1, 2027 to December 31, 2028 to support the JAXA-led Mars Moons eXploration (MMX) mission (Japan), followed by two years of post-operations.
Mars Express has conducted data relay for seven rovers and landing platforms, and enabled scientific collaboration with a further five orbiters.
The past 20 years of observations from Mars Express have solidified our picture of Mars as a once-habitable planet, with warmer and wetter epochs that may have been oases for ancient life.
Image Processing: Andrea Luck
Image Date: Aug. 22, 2023
#NASA #ESA #Space #Astronomy #Science #Planet #Mars #Geology #Volcanoes #AscraeusMons #TharsisProvince #MarsExpress #MarsExpressSpacecraft #HRSC #Europe #DLR #FUBerlin #Berlin #Germany #Deutschland #STEM #Education
NASA’s Perseverance Mars Rover Explores“Krokodillen” in Jezero Crater | JPL
NASA’s Perseverance Mars Rover Explores“Krokodillen” in Jezero Crater | JPL
Scientists expect a new area of interest on the lower slope of Jezero Crater’s rim to offer examples of the oldest rocks on the Red Planet.
NASA’s Perseverance Mars rover is now exploring an area called “Krokodillen” that may contain rocks representing the oldest on Mars. It has been on the Perseverance science team’s wish list because it marks an important boundary between the oldest rocks of Jezero Crater’s rim and those of the plains beyond the crater.
“The last five months have been a geologic whirlwind,” said Ken Farley, deputy project scientist for Perseverance from Caltech in Pasadena. “As successful as our exploration of “Witch Hazel Hill” has been, our investigation of Krokodillen promises to be just as compelling.”
Named by Perseverance mission scientists after a mountain ridge on the island of Prins Karls Forland, Norway, Krokodillen (meaning “the crocodile” in Norwegian) is a 73-acre (about 30-hectare) plateau of rocky outcrops located downslope to the west and south of Witch Hazel Hill.
A quick earlier investigation into the region revealed the presence of clays in this ancient bedrock. Because clays require liquid water to form, they provide important clues about the environment and habitability of early Mars. The detection of clays elsewhere within the Krokodillen region would reinforce the idea that abundant liquid water was present sometime in the distant past, likely before Jezero Crater was formed by the impact of an asteroid. Clay minerals are also known on Earth for preserving organic compounds, the building blocks of life.
“If we find a potential biosignature here, it would most likely be from an entirely different and much earlier epoch of Mars evolution than the one we found last year in the crater with 'Cheyava Falls,'” said Farley, referring to a rock sampled in July 2024 with chemical signatures and structures that could have been formed by life long ago. “The Krokodillen rocks formed before Jezero Crater was created, during Mars’ earliest geologic period, the Noachian, and are among the oldest rocks on Mars
Data collected from NASA’s Mars orbiters suggest that the outer edges of Krokodillen may also have areas rich in olivine and carbonate. While olivine forms from magma, carbonate minerals on Earth typically form during a reaction in liquid water between rock and dissolved carbon dioxide. Carbonate minerals on Earth are known to be excellent preservers of fossilized ancient microbial life and recorders of ancient climate.
The Perseverance rover celebrated its 1,500th day of surface operations on May 9, 2025. It is currently analyzing a rocky outcrop in Krokodillen called “Copper Cove” that may contain Noachian rocks.
Ranking Mars Rocks
The rover’s arrival at Krokodillen comes with a new sampling strategy for the nuclear-powered rover that allows for leaving cored samples unsealed in case the mission finds a more scientifically compelling geologic feature down the road.
To date, Perseverance has collected and sealed two regolith (crushed rock and dust) samples, three witness tubes, and one atmospheric sample. It has also collected 26 rock cores and sealed 25 of them. The rover’s one unsealed sample is its most recent, a rock core taken on April 28 that the team named “Bell Island,” which contains small round stones called spherules. If at some point the science team decides a new sample should take its place, the rover could be commanded to remove the tube from its bin in storage and dump the previous sample.
“We have been exploring Mars for over four years, and every single filled sample tube we have on board has its own unique and compelling story to tell,” said Perseverance acting project scientist Katie Stack Morgan of NASA’s Jet Propulsion Laboratory in Southern California. “There are seven empty sample tubes remaining and a lot of open road in front of us, so we’re going to keep a few tubes—including the one containing the Bell Island core—unsealed for now. This strategy allows us maximum flexibility as we continue our collection of diverse and compelling rock samples.”
Before the mission adopted its new strategy, the engineering sample team assessed whether leaving a tube unsealed could diminish the quality of a sample. The answer was no.
“The environment inside the rover met very strict standards for cleanliness when the rover was built. The tube is also oriented in such a way within its individual storage bin that the likelihood of extraneous material entering the tube during future activities, including sampling and drives, is very low,” said Stack Morgan.
In addition, the team assessed whether remnants of a sample that was dumped could “contaminate” a later sample. “Although there is a chance that any material remaining in the tube from the previous sample could come in contact with the outside of a new sample,” said Stack Morgan, “it is a very minor concern—and a worthwhile exchange for the opportunity to collect the best and most compelling samples when we find them.”
Release Date: May 19, 2025
Milky Way & Nebulae over Maunakea, Hawaii
Milky Way & Nebulae over Maunakea, Hawaii
"Have you ever seen the band of our Milky Way Galaxy? In a clear sky from a dark location at the right time, a faint band of light becomes visible across the sky. Soon after your eyes become dark adapted, you might spot the band for the first time. It may then become obvious. Then spectacular. One reason for your growing astonishment might be the realization that this fuzzy swath, the Milky Way, contains billions of stars. Visible in the featured image, high above in the night sky, the band of the Milky Way Galaxy arcs. Also visible are the colorful clouds of Rho Ophiuchi on the right, and the red and circular Zeta Ophiuchi nebula near the top center. Taken in late February from Maunakea, Hawaii, USA, the foreground telescope is the University of Hawaii's 2.2-Meter Telescope. Fortunately, you do not need to be near the top of a Hawaiian volcano to see the Milky Way."
Image Description: A wide starfield is shown with the dark and light band arching horizontally across the middle. On the right is a colorful and complex nebula, and near the top center is a red circular nebula.
Release Date: May 20, 2025









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