Planet Mars Images: Aug. 19-20, 2025 | NASA's Curiosity & Perseverance Rovers
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Wednesday, August 20, 2025
Planet Mars Images: Aug. 19-20, 2025 | NASA's Curiosity & Perseverance Rovers
Orbital Earth Night Views | International Space Station
Orbital Earth Night Views | International Space Station
https://blogs.nasa.gov/spacestation/
Image Dates: July 22-28, 2025
#NASA #Space #ISS #Science #Stars #Planets #Earth #Aurora #IndianOcean #SoutheastAsia #Astronauts #AstronautPhotography #Japan #JAXA #Cosmonauts #Russia #Россия #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education
Tuesday, August 19, 2025
China's CAS Space: Kinetica-1 Y10 Commercial Rocket Launch of Mexican Satellites
China's CAS Space: Kinetica-1 Y10 Commercial Rocket Launch of Mexican Satellites
🚀A CAS Space Kinetica-1 Y10 carrier rocket blasted off at 3:33 p.m. Beijing Time on August 19, 2025, successfully sending seven satellites into orbit from the Dongfeng Commercial Aerospace Innovation Pilot Zone at the Jiuquan Satellite Launch Center (JSLC) in northwest China.
The satellites on this rideshare included Zhongke Satellite-05, Multi-functional Test Satellites No. 2-01, 02, and 03, Tianyan-26, plus ThumbSat-1, and ThumbSat-2 for Mexico.
This marks the eighth successful flight mission of the Kinetica-1 launch vehicle and the forty-eighth launch for China in 2025.
Notably, the Kinetica-1 Y10 rocket was painted with calligraphy representing the “Women of China”. The marking is part of CAS Space's collaboration with the All-China Women’s Federation to celebrate progress in equality as well as the contributions of the country's 689 million women. Through the mission's success, CAS Space wishes to convey this message and to recognize the achievements of all women worldwide.
Mission Y10 has been declared a complete success. A total of 70 satellites, or 7 tons of payload, have now been delivered by Kinetica-1 rockets since its debut with more to come this year.
CAS Space is a Chinese commercial space launch provider based in Guangzhou, the 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 commercial space launch firms, like CAS Space.
China's CAS Space: Kinetica-1 Y10 Commercial Rocket Launch of Mexican Satellites
China's CAS Space: Kinetica-1 Y10 Commercial Rocket Launch of Mexican Satellites
🚀A CAS Space Kinetica-1 Y10 carrier rocket blasted off at 3:33 p.m. Beijing Time on August 19, 2025, successfully sending seven satellites into orbit from the Dongfeng Commercial Aerospace Innovation Pilot Zone at the Jiuquan Satellite Launch Center (JSLC) in northwest China.
The satellites on this rideshare included Zhongke Satellite-05, Multi-functional Test Satellites No. 2-01, 02, and 03, Tianyan-26, plus ThumbSat-1, and ThumbSat-2 for Mexico.
This marks the eighth successful flight mission of the Kinetica-1 launch vehicle and the forty-eighth launch for China in 2025.
Notably, the Kinetica-1 Y10 rocket was painted with calligraphy representing the “Women of China”. The marking is part of CAS Space's collaboration with the All-China Women’s Federation to celebrate progress in equality as well as the contributions of the country's 689 million women. Through the mission's success, CAS Space wishes to convey this message and to recognize the achievements of all women worldwide.
Mission Y10 has been declared a complete success. A total of 70 satellites, or 7 tons of payload, have now been delivered by Kinetica-1 rockets since its debut with more to come this year.
CAS Space is a Chinese commercial space launch provider based in Guangzhou, the 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 commercial space launch firms, like CAS Space.
Release Date: Aug. 19, 2025
Giant Galaxies in Pavo (AI Narration)
Giant Galaxies in Pavo (AI Narration)
Other members of the southern Pavo galaxy group are scattered through this magnificent galaxy group portrait, with the dominant giant elliptical galaxy, NGC 6876, above and right of the soaring Condor galaxy.
#NASA #Astronomy #Space #Science #Galaxies #Galaxy #NGC6872 #CondorGalaxy #SpiralGalaxies #IC4970 #InteractingGalaxies #NGC6876 #EllipticalGalaxies #Pavo #Constellation #Cosmos #Universe #Astrophotography #AdamBlock #Astrophotographer #GSFC #UnitedStates #STEM #Education #HD #Video
Giant Galaxies in Pavo
Giant Galaxies in Pavo
Over 500,000 light years across, NGC 6872 (bottom left) is a truly enormous barred spiral galaxy. At least five times the size of our own large Milky Way, NGC 6872 is the largest known spiral galaxy. About 200 million light-years distant toward the southern constellation Pavo, the Peacock, the appearance of this giant galaxy's stretched out spiral arms suggest the wings of a giant bird. So its popular moniker is the Condor Galaxy. Lined with massive young, bluish star clusters and star-forming regions, the extended and distorted spiral arms are due to NGC 6872's past gravitational interactions with the nearby smaller galaxy IC 4970, visible here below the giant spiral galaxy's core.
Other members of the southern Pavo galaxy group are scattered through this magnificent galaxy group portrait, with the dominant giant elliptical galaxy, NGC 6876, above and right of the soaring Condor galaxy.
Release Date: Aug. 19, 2025
#NASA #Astronomy #Space #Science #Galaxies #Galaxy #NGC6872 #CondorGalaxy #SpiralGalaxies #IC4970 #InteractingGalaxies #NGC6876 #EllipticalGalaxies #Pavo #Constellation #Cosmos #Universe #Astrophotography #AdamBlock #Astrophotographer #GSFC #UnitedStates #STEM #Education
Views of Hurricane Erin | International Space Station
Views of Hurricane Erin | International Space Station
The International Space Station flew 260 miles over Hurricane Erin at 11:41 a.m. EDT Tuesday, Aug. 19, 2025. External cameras on the orbiting laboratory captured views of the hurricane as it traveled northwest through the Caribbean with maximum sustained wind speeds of 105 mph. Hurricane Erin is not expected to make landfall and is projected to move between the U.S. East coast and Bermuda before heading out into the Atlantic Ocean.
https://blogs.nasa.gov/spacestation/
Release Date: Aug. 19, 2025
#NASA #Space #ISS #Science #Planets #Earth #AtlanticOcean #Weather #Meteorology #HurricaneErin #Astronauts #AstronautPhotography #UnitedStates #Japan #日本 #JAXA #宇宙航空研究開発機構 #Cosmonauts #Russia #Россия #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education #HD #Video
Circular Arcs of Star Trails | International Space Station
Circular Arcs of Star Trails | International Space Station
https://blogs.nasa.gov/spacestation/
Image Date: July 26, 2025
#NASA #Space #ISS #Science #Stars #StarTrails #Planets #Earth #Astronauts #AstronautPhotography #TimelapsePhotography #Kibo #きぼう#Japan #日本 #JAXA #宇宙航空研究開発機構 #Cosmonauts #Russia #Россия #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition73 #STEM #Education
New Moon Discovered Orbiting Planet Uranus | James Webb Space Telescope
New Moon Discovered Orbiting Planet Uranus | James Webb Space Telescope
This timelapse animation shows the newly discovered moon of the planet Uranus, designated S/2025 U1, as well as 13 of the 28 other known moons orbiting the planet. The observations by NASA’s James Webb Space Telescope’s Near-Infrared Camera (NIRCam) were taken over the course of about 6 hours on Feb. 2, 2025, under program ID 6379 (principal investigator: M. El Moutamid).
The animation is comprised of data taken with NIRCam’s wide band F150W2 filter that transmits infrared wavelengths from about 1.0 to 2.4 microns. Due to the drastic differences in brightness levels, the animation is a composite of three separate treatments of the data, allowing the viewer to see details in the planetary atmosphere, the surrounding rings, and the orbiting moons. The small moon Cordelia orbits just inside the outermost ring, but is not visible in these views due to glare from the rings.
Animation: NASA, ESA, CSA, STScI, Maryame El Moutamid (SwRI), Matthew Hedman (University of Idaho), Joseph DePasquale (STScI)
Duration: 17 seconds
Release Date: Aug. 19, 2025
NASA Artemis III Moon Rocket Processing Begins | Kennedy Space Center
NASA Artemis III Moon Rocket Processing Begins | Kennedy Space Center
Buildup of NASA’s Space Launch System (SLS) rocket for the Artemis III lunar mission has started at the agency’s Kennedy Space Center in Florida, even as NASA prepares for the launch of the Artemis II mission, the second Artemis mission in NASA’s efforts to return humans to the Moon and eventually land on Mars.
The Artemis III SLS engine section and boat-tail that protects the engines during launch moved from the Space Systems Processing Facility (SSPF) at NASA Kennedy to the mammoth Vehicle Assembly Building (VAB) in late July, just a few feet from where the Artemis II SLS is mostly stacked and undergoing integrated testing and checkouts.
This engine section is one the most complex and intricate parts of the rocket stage that will help power the Artemis missions to the Moon.
Over the course of about 30 days, the Artemis III astronauts will travel to lunar orbit, where two crew members will descend to the surface and spend approximately a week near the South Pole of the Moon conducting new science before returning to lunar orbit to join their crew for the journey back to Earth. Launch is currently scheduled for mid-2027.
https://www.nasa.gov/humans-in-space/artemis/
Follow updates on the Artemis blog:
https://blogs.nasa.gov/artemis/
NASA's Space Launch System (SLS)
https://www.nasa.gov/sls
NASA's Artemis III Mission:
https://www.nasa.gov/mission/artemis-iii/
Read the Artemis Plan (74-page PDF Free Download):
https://www.nasa.gov/sites/default/files/atoms/files/artemis_plan-20200921.pdf
Image Dates: July 29-Aug. 13, 2025
#NASA #Space #Earth #Moon #Artemis #ArtemisIII #SLS #SLSRocket #CoreStage #Boeing #CrewedMissions #DeepSpace #MoonToMars #Science #Engineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NASAKennedy #KSC #MerrittIsland #Florida #UnitedStates #STEM #Education
Monday, August 18, 2025
NASA’s Quesst Mission: X-59 Quiet Supersonic Aircraft Testing | NASA Armstrong
NASA’s Quesst Mission: X-59 Quiet Supersonic Aircraft Testing | NASA Armstrong
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.
https://www.nasa.gov/sites/default/files/atoms/files/x-59-maker-bundle-v8.pdf
Image Dates: July 10-17, 2025
#NASA #Aerospace #SupersonicFlight #SupersonicAircraft #X59 #Sonicboom #QuietAviation #Aviation #QuesstMission #CommercialAviation #Science #Physics #Engineering #AerospaceResearch #AeronauticalResearch #FlightTests #LockheedMartin #SkunkWorks #NASAArmstrong #AFRC #Palmdale #California #UnitedStates #JAXA #Japan #STEM #Education
Close-up: Galaxy NGC 4900—A Spiral and a Star in Virgo | Hubble
Close-up: Galaxy NGC 4900—A Spiral and a Star in Virgo | Hubble
This NASA/European Space Agency Hubble Space Telescope picture features a sparkling spiral galaxy paired with a prominent star, both in the constellation Virgo. While the galaxy and the star appear to be close to one another, even overlapping, they are actually a great distance apart. The star, marked with four long diffraction spikes, is in our own galaxy. It is just 7,109 light-years away from Earth. The galaxy, named NGC 4900, lies about 45 million light-years from Earth.
This image combines data from two of Hubble’s instruments: the Advanced Camera for Surveys, installed in 2002 and is still in operation today, and the older Wide Field and Planetary Camera 2—in use from 1993 to 2009. The data used here were taken more than 20 years apart for two different observing programs—a real testament to Hubble’s long scientific lifetime.
Both programs aimed to understand the demise of massive stars. In one, researchers studied the sites of past supernovae, aiming to estimate the masses of the stars that exploded and investigate how supernovae interact with their surroundings. NGC 4900 was selected for study because it hosted a supernova named SN 1999br.
In the other program, researchers laid the groundwork for studying future supernovae by collecting images of more than 150 nearby galaxies. After a supernova is detected in one of these galaxies, researchers can examine these images, searching for a star at the location of the supernova. Identifying a supernova progenitor star in pre-explosion images gives valuable information about how, when and why supernovae occur.
Image Description: A spiral galaxy seen face-on. Broken spiral arms made of blue patches of stars and thin strands of dark dust swirl around the galaxy’s center, forming a broad, circular disc. An extended circular halo surrounds the disc. The center is a brightly-glowing, stubby bar-shaped area in a pale yellow color. A bright star in our own galaxy, with long cross-shaped diffraction spikes, is visible atop the distant galaxy.
Release Date: March 10, 2025
#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #Galaxies #Galaxy #NGC900 #SpiralGalaxy #Virgo #Constellation #Star #MilkyWayGalaxy #Cosmos #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video
Close-up: Spiral Galaxy UGC 11397 in Lyra | Hubble
Close-up: Spiral Galaxy UGC 11397 in Lyra | Hubble
The light that the NASA/European Space Agency Hubble Space Telescope collected to create this picture reached the telescope after a journey of 250 million years. Its source was the spiral galaxy UGC 11397. It resides in the constellation Lyra (The Lyre). At first glance, UGC 11397 appears to be an average spiral galaxy. It sports two graceful spiral arms that are illuminated by stars and defined by dark, clumpy clouds of dust.
What sets UGC 11397 apart from a typical spiral lies at its center, where a supermassive black hole containing 174 million times the mass of the Sun is growing. As a black hole ensnares gas, dust, and even entire stars from its vicinity, this doomed matter heats up and puts on a fantastic cosmic light show. Material trapped by the black hole emits light from gamma rays to radio waves and can brighten and fade without warning. However, in galaxies like UGC 11397, thick clouds of dust hide much of this energetic activity from view in optical light. Despite this, UGC 11397's actively growing black hole was revealed through its bright X-ray emission—high-energy light that can pierce the surrounding dust. This led astronomers to classify it as a Type 2 Seyfert galaxy, a category used for active galaxies whose central regions are hidden from view in visible light by a doughnut-shaped cloud of dust and gas.
Using Hubble, researchers will study hundreds of galaxies that, like UGC 11397, harbor a supermassive black hole that is gaining mass. The Hubble observations will help researchers weigh nearby supermassive black holes, understand how black holes grew early in the Universe’s history, and even study how stars form in the extreme environment found at the very center of a galaxy.
Image Description: A spiral galaxy seen at an angle that gives it an oval shape. It has two spiral arms that curl out from the center. They start narrow but broaden out as they wrap around the galaxy before merging into a faint halo. The galaxy’s disc is golden in the center with a bright core, and pale blue outside that. A swirl of dark dust strands and speckled blue star-forming regions follow the arms through the disc.
Release Date: June 23, 2025
#NASA #ESA #Astronomy #Space #Science #Hubble #Hubble35 #Galaxies #Galaxy #UGC11397 #SpiralGalaxy #SuperMassiveBlackHole #BlackHoles #Type2SeyfertGalaxy #Lyra #Constellation #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video
Close-up: Galaxy Cluster Abell 209 in Cetus | Hubble Space Telescope
Close-up: Galaxy Cluster Abell 209 in Cetus | Hubble Space Telescope
This Hubble image of Abell 209 shows more than a hundred galaxies, but there is more to this cluster than even Hubble’s discerning eye can see. Abell 209’s galaxies are separated by millions of light-years, and the seemingly empty space between the galaxies is actually filled with hot, diffuse gas that can be spotted only at X-ray wavelengths. An even more elusive occupant of this galaxy cluster is dark matter: a form of matter that does not interact with light. The Universe is understood to be comprised of 5% normal matter, 25% dark matter, and 70% dark energy
Hubble observations like the ones used to create this image can help astronomers answer fundamental questions about our Universe, including mysteries surrounding dark matter and dark energy. These investigations leverage the immense mass of a galaxy cluster. This can bend the fabric of spacetime itself and create warped and magnified images of background galaxies and stars in a process called gravitational lensing.
While this image lacks the dramatic rings that gravitational lensing can sometimes create, Abell 209 still shows subtle signs of lensing at work, in the form of streaky, slightly curved galaxies within the cluster’s golden glow. By measuring the distortion of these galaxies, astronomers can map the distribution of mass within the cluster, illuminating the underlying cloud of dark matter. This information, which Hubble’s fine resolution and sensitive instruments help to provide, is critical for testing theories of how our Universe has evolved.
Image Description: A cluster of distant, mainly elliptical galaxies. They appear as brightly shining points radiating golden light that each take the shape of a smooth, featureless oval. They crowd around one that is extremely large and bright. A few spiral galaxies of comparable size appear too, bluer in color and with unique shapes. Of the other, more small and distant galaxies covering the scene, a few are warped into long lines.
Release Date: July 7, 2025
Alaska 'Daylight' Aurora and The Andromeda Galaxy
Alaska 'Daylight' Aurora and The Andromeda Galaxy
Astrophotographer John Chumack: "Sometimes the northern lights occur overhead when it is still daylight, but because of the bright blue sky when the Sun is up, we do not see them. However, I was able to capture this charming daylight aurora outside of Fairbanks, Alaska, on March 22, 2025. The Sun had just set, and so the sky was just dark enough to detect it with the human eye."
"Note that the Andromeda Galaxy (our sister galaxy) is visible on the left center edge of the frame. At approximately 2.2 million light years away, it is considered the furthest object the human eye can see without optical aid."
Photo Details: Canon DSLR camera; 16-35mm lens set to 25mm; F2.8; ISO 3200; 8 seconds exposure.
Auroras happen when charged particles from the Sun interact with Earth's magnetic field, creating dazzling light shows in the sky. The aurora borealis, also known as the northern lights, occurs in an upper layer of Earth’s atmosphere called the ionosphere.
https://www.aurorasaurus.org
https://science.nasa.gov/feature/nasas-guide-to-finding-and-photographing-auroras/
Text Credit: John Chumack
John's website: https://www.galacticimages.com
Capture Location: Fairbanks, Alaska Coordinates: 64.8401, -147.7200
Release Date: Aug. 18, 2025
Building a New Milky Way Spectator: The Extremely Large Telescope (ELT) | ESO
Building a New Milky Way Spectator: The Extremely Large Telescope (ELT) | ESO
This picture shows the Milky Way galaxy flowing over the European Southern Observatory’s Extremely Large Telescope (ELT). As the light of the Milky Way band appears to pour into the ELT, the enormous cranes around it seem to do the same while they further advance the telescope. Once the assembly is complete, the soon-to-be largest telescope in the world will be breaking down the light above in unparalleled detail.
The very bright and orange patch in the Milky Way right above the open dome is the core of our galaxy, with its filamentary dark clouds of gas and dust. The stars in the Milky Way center look redder partly because they are older and partly because dust reddens them, similar to how particles in our atmosphere make the Sun look red at sunrise or sunset.
Focusing back down on Earth, the ELT will scrutinize the pristine night sky above the Chilean Atacama Desert with unprecedented precision. It will help us learn more about the close environment of Sagittarius A*, the supermassive black hole at the center of our galaxy. It will analyze the atmospheres of exoplanets, answer questions about the births and deaths of stars we yet cannot even begin to ask, and explore how galaxies form and evolve, among many other exciting questions. We eagerly await the mysteries of the cosmos the world’s biggest eye on the sky will unveil.
Altitude: 3,046 meters
Planned year of technical first light: 2027
Release Date: Aug. 18, 2025




















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