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NASA's Space Crew-11 Dragon Spacecraft Incoming | International Space Station
The SpaceX Dragon spacecraft carrying four members of NASA's SpaceX Crew-11 mission is pictured approaching the International Space Station 259 miles above central Pakistan.
The SpaceX Dragon spacecraft carrying four members of NASA's SpaceX Crew-11 mission is pictured approaching the International Space Station 260 miles above southern Pakistan.
The SpaceX Dragon spacecraft carrying NASA's Crew-11 mission approaches the International Space Station while orbiting 260 miles above the Indian Ocean coast of Tanzania on the African continent.
The SpaceX Dragon spacecraft carrying NASA's Crew-11 mission approaches the International Space Station while orbiting 260 miles above the Indian Ocean coast of Tanzania on the African continent.
On Aug. 2, 2025, the Crew-11 quartet joined the seven-member Expedition 73 crew. NASA astronauts Zena Cardman and Mike Fincke, Japan Aerospace Exploration Agency (JAXA) astronaut Kimiya Yui, and Roscosmos cosmonaut Oleg Platonov of Russia are now on their seven-month research mission in low Earth orbit.
Crew-11 is conducting scientific research to prepare for human exploration beyond low Earth orbit and benefit humanity on Earth. Participating crew members will simulate lunar landings, test strategies to safeguard vision, and advance other human spaceflight studies led by NASA’s Human Research Program. The crew also will study plant cell division and microgravity’s effects on bacteria-killing viruses, as well as perform experiments to produce a higher volume of human stem cells and generate on-demand nutrients.
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke
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.
Science on NASA's SpaceX 33rd Cargo Mission | International Space Station
Later this August, SpaceX's Dragon spacecraft is scheduled to launch to the International Space Station, carrying science experiments and other cargo to the orbiting laboratory.
Research traveling to the station aboard NASA's SpaceX 33rd commercial resupply mission includes testing 3D bioprinting of an implantable medical device, observing the behavior of engineered liver tissues, examining microgravity’s effects on bone-forming cells, and additional 3D printing of metal in space.
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke
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: National Aeronautics and Space Administration (NASA) Duration: 46 seconds Release Date: Aug. 13, 2025
A White Dwarf Star’s Unusual Atmosphere Uncovered | Hubble Space Telescope
Astronomers using NASA’s Hubble Space Telescope have found a rare ultra massive white dwarf formed from a stellar merger. The discovery was made possible by Hubble’s sensitive ultraviolet observations and suggests these unusual white dwarfs may be more common than once thought.
The white dwarf is 128 light-years away and 20 percent more massive than the Sun. In visible light it looked like a typical white dwarf, but Hubble’s ultraviolet data revealed something unusual . . .
SpaceX Crew-10 in Dragon Pressure Suits: Pre-departure | International Space Station
The four members of NASA's SpaceX Crew-10 mission pose for a portrait in their Dragon pressure suits aboard the International Space Station's Harmony module. The Commercial Crew members were testing their suits' components and ensuring a proper fit before their departure on Aug. 8, 2025, aboard Dragon ending their five-month space research mission inside the orbital outpost. From left are, Roscosmos cosmonaut Kirill Peskov of Russia, NASA astronauts Nichole Ayers and Anne McClain, and Japan Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi.
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke
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.
Image Credit: NASA's Johnson Space Center Image Date: July 29, 2025
European Weather Satellite Launch: EUMETSAT METOP-SGA1 | Ariane 6 Rocket
On August 12, 2025 at 9:37 p.m. local time in Kourou, French Guiana (00:37 a.m. UTC, 2:37 a.m. CEST, on August 13, 2025), Ariane 6 lifted off from Europe's Spaceport carrying EUMETSAT's Metop-SGA1 satellite.
With this second commercial flight, Ariane 6, the new European heavy-lift launcher operated by Arianespace, successfully placed Metop-SGA1 into Sun-synchronous orbit (SSO) at an altitude of 800 km. Spacecraft separation occurred 1 hour and 4 minutes after lift-off.
A few minutes after separation, EUMETSAT successfully acquired signals from the satellite.
David Cavaillolès, CEO of Arianespace, declared: “Tonight, Arianespace has successfully launched EUMETSAT's Metop-SGA1 satellite, on board Ariane 6. The first of the next generation of European polar-orbiting weather satellites, Metop-SGA1 notably hosts the Copernicus programme Sentinel-5 atmospheric monitoring mission. This success pinpoints our dedication to ensuring Europe's autonomous and reliable access to space while also supporting an ambitious environmental mission that will provide cutting-edge data for weather and climate monitoring . . ."
Phil Evans, Director-General of EUMETSAT, commented: “Extreme weather has cost Europe hundreds of billions of euros and tens of thousands of lives over the past 40 years—storms like Boris, Daniel and Hans, record heatwaves and fierce wildfires are just the latest reminders. The launch of Metop-SGA1 is a major step forward in giving national weather services in our member states sharper tools to save lives, protect property, and build resilience against the climate crisis. These positive impacts will be felt even beyond that and over the Atlantic, as Metop-SGA1 is Europe's first contribution to the Joint Polar System with the National Oceanic and Atmospheric Administration (NOAA) . . . ”
Ariane 6 is a program developed within the framework of the European Space Agency (ESA).
The Metop-SGA1 (Second Generation A1) satellite will be the first of the next generation of European polar-orbiting weather satellites. Metop-SGA1 will host a total of six atmospheric sounding and imaging instrument missions that will provide optical, infrared, and microwave observations essential data for weather forecasting, climate monitoring, and a wide range of other services and applications. Amongst its hosts, Metop-SGA1 will carry the new Sentinel-5 atmospheric monitoring mission, part of the European Commission's Copernicus programme. The spacecraft was built by Airbus Defence and Space, under a contract with the European Space Agency, and will be operated throughout its lifetime by EUMETSAT, that will also distribute its data to users.
China Distributes 125.42 Grams of Lunar Samples for Global Scientific Research
China has distributed 125.42 grams of lunar samples for scientific research, including 2.18 grams of Chang'e-5 specimens shared with seven institutions from six countries, the China National Space Administration (CNSA) announced.
To date, domestic and international scientists have produced over 150 published research findings utilizing samples from the Chang'e-5 (near side) and Chang'e-6 (far side/south pole) lunar missions.
The lunar sample allocation follows a rigorous two-stage approval process combining online applications with expert peer review. Qualified research institutions may access the dedicated online platform to review sample catalogs and submit formal research proposals.
"This page displays all the available samples for application as well as those currently on loan. Look here—it shows 'lent' status, which means this sample has been borrowed," said Hou Jun, deputy director of Science and Technology Engineering Department of the China Lunar Exploration and Space Engineering Center of the CNSA.
Currently, lunar sample applications are accepted twice yearly, with each submission window open for approximately one month. Following submission, an expert committee conducts a thorough review before final approval and issuance by the CNSA. The entire process—from application to sample distribution—typically takes about five months.
"Applications for one or two grams are exceptionally rare; most allocated samples are measured in milligrams. We centrally manage these samples and perform customized processing in our laboratory based on researchers' specific requirements," said Yang Wei, a researcher at the Chinese Academy of Sciences' Institute of Geology and Geophysics.
China's Chang'e-6 mission collected 1,935.3 grams of samples from the far side of the Moon—the first in human history. Meanwhile, the Chang'e-5 mission retrieved about 1,731 grams of lunar samples.
In July 2021, China delivered the first batch of lunar samples to research institutions. So far, the country has lent nine batches of lunar samples to institutions for research purposes.
The Chang'e-5 mission made China the third country to return samples from the Moon after the United States and the Soviet Union.
The Chang'e-5 lander/ascender arrived on the Moon December 1, 2020. The Chang'e 5 landing site is at 43.1°N (in latitude), 51.8°W (in longitude) in the Northern Oceanus Procellarum near a huge volcanic complex, Mons Rümker, located in the northwest lunar near side. The area is mapped as 'Eratosthenian Mare' by the United States Geological Survey (USGS). The Chang'e 5 landing site, named Statio Tianchuan, is within the Procellarum KREEP Terrain, with elevated heat-producing elements, thin crust, and prolonged volcanism. This area is characterized by examples of the youngest mare basalts on the Moon (~1.21 billion years old) with elevated titanium, thorium, and olivine abundances. These were never sampled by the U.S. Apollo or Soviet Luna programs.
Video Credit: CCTV Duration: 1 minute, 17 seconds Release Date: Aug. 10, 2025
X "Marks the Spot" above Cerro Tololo, Chile | NOIRLab
Celestial beams of light formed from the Milky Way galaxy and zodiacal light crisscrossing above the telescopes of the U.S. National Science Foundation Cerro Tololo Inter-American Observatory (CTIO), a Program of National Science Foundation (NSF) NOIRLab. The US Naval Observatory Deep South Telescope sits on the far left of this image. Moving towards the right, there is also the DIMM1 Seeing Monitor, the CHilean Automatic Supernova sEarch dome (CHASE), the UBC Southern Observatory, and the Planetary Defense 1.0-meter Telescope. These represent only a subset of the nearly 40 telescopes at CTIO, so this celestial X truly marks the spot of a treasure trove of discovery!
The zodiacal light is a faint, diffuse band of light in the night sky, reaching up from the horizon. It follows the direction of the ecliptic—the plane of Earth's orbit around the Sun. This plane is rich in tiny particles of dust. It scatters sunlight and creates this phenomenon. The glow is so faint that light pollution or even moonlight can outshine it.
Many of the telescopes pictured here have specialized purposes on behalf of their sponsors. For example, the UBC Southern Observatory 0.35-meter (1.15-foot) telescope was made specifically for the site-testing campaign of the Thirty Meter Telescope. Today, it is used by the University of British Columbia in Canada for research on transiting exoplanets and space debris. Another specialized telescope at CTIO is the Planetary Defense 1.0-meter Telescope, operated by the University of North Carolina and the Astronomical Research Institute. This telescope conducts southern-sky astrometric follow-up observations of Near-Earth Asteroids (NEAs).
Close-up: Galaxy NGC 45 in Cetus | Hubble Space Telescope
This NASA/European Space Agency Hubble Space Telescope picture zooms in on the feathery spiral arms of the galaxy NGC 45. It lies just 22 million light-years away in the constellation Cetus (The Whale).
The data used to create this portrait were drawn from two complementary observing programs. The first took a broad view of 50 nearby galaxies, leveraging Hubble’s ability to observe light from the ultraviolet to the near-infrared in order to study star formation in these galaxies. The second program examined many of the same nearby galaxies as the first, narrowing in on a particular wavelength of red light called H-alpha. Star-forming nebulae are powerful producers of H-alpha light, and several of these regions can be identified across NGC 45 by their bright pink-red color.
These observing programs aimed to study star formation in galaxies of various sizes, structures, and degrees of isolation. NGC 45 is a particularly interesting target. Alhough it may appear to be a regular spiral galaxy, NGC 45 is actually a remarkable type called a low surface brightness galaxy.
Low surface brightness galaxies are fainter than the night sky itself, making them incredibly difficult to detect. They appear unexpectedly faint because they have relatively few stars for the amount of gas and dark matter they carry. In the decades since the first low surface brightness galaxy was serendipitously discovered in 1986, researchers have learned that 30–60% of all galaxies may fall into this category. Studying these hard-to-detect galaxies is key to understanding how galaxies form and evolve, and Hubble’s sensitive instruments are equal to the task.
Image Description: This Hubble image features a close-up view of the outer arms of the spiral galaxy NGC 45. These spiral arms are filled with tiny blue dots—stars—and glowing pink clouds—star-forming nebulae. This is shown against a dark background.
Credit: ESA/Hubble & NASA, D. Calzetti, R. Chandar, N. Bartmann (ESA/Hubble) Acknowledgement: M. H. Özsaraç
NASA Artemis II Orion Spacecraft Move: Preparing for Moon Rocket Integration
Crews transport NASA’s Artemis II Orion spacecraft from the Multi-Payload Processing Facility (MPPF) to the Launch Abort System Facility (LASF) at the agency’s Kennedy Space Center in Florida on Sunday, Aug. 10, 2025. Technicians will integrate Orion with its 44-foot-tall launch abort system designed to carry the crew to safety in the event of an emergency during launch or ascent atop the Space Launch System (SLS) rocket. The Artemis II test flight will send NASA astronauts Reid Wiseman, Victor Glover, and Christina Koch, and Canadian Space Agency (CSA) astronaut Jeremy Hansen around the Moon and return them safely back home.
Image Credit: NASA/Kim Shiflett Image Date: Aug. 10, 2025
The light from an orbital sunrise refracts through a window inside the International Space Station's "window to the world," the Cupola. At bottom, a portion of the orbital outpost's U.S. segment is illuminated including the SpaceX Dragon crew spacecraft docked to the Harmony module's forward port. The station was soaring 259 miles above the Republic of Kiribati in the Pacific Ocean at approximately 3:40 a.m. local time when this photograph was taken.
The Cupola is a panoramic control tower for the International Space Station—a dome-shaped module with windows that allows operations on the outside of the station to be observed and guided. It is a pressurized observation and work area that accommodates command and control workstations and other hardware. The Cupola offers a 360 degree view.
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke
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.
Image Credit: NASA's Johnson Space Center Image Date: June 13, 2025
Galaxy NGC 2146 | Hubble & Chandra [Budget Alert: Chandra to be Canceled)
NGC 2146 is a spiral galaxy with one of its dusty arms blocking the view of the galaxy’s center from Earth’s perspective. X-rays from NASA's Chandra X-ray Observatory show double star systems and hot gas that is being driven away from the galaxy by supernova explosions and winds from giant stars.
X-rays from Chandra show as pink and purple, while optical data from the Hubble Space Telescope and the Las Cumbres Observatory in Chile and infrared data from the National Science Foundation’s Kitt Peak Observatory are in red, green, and blue.
NASA's Chandra X-ray Observatory is being canceled in NASA's Fiscal Year 2026 Budget Request, along with 18 other active science missions. NASA's science budget is being reduced by nearly 50%. NASA's total budget will become the lowest since 1961, after accounting for inflation.
Contact your representatives in the United States Congress, House and Senate, to express your concerns about severe budget cuts at NASA:
NGC 2146 is classified as a barred spiral due to its shape, but the most distinctive feature is the dusty spiral arm that has looped in front of the galaxy's core as seen from our perspective. The forces required to pull this structure out of its natural shape and twist it up to 45 degrees are colossal. The most likely explanation is that a neighboring galaxy is gravitationally perturbing it and distorting the orbits of many of NGC 2146’s stars. It is probable that we are currently witnessing the end stages of a process which has been occurring for tens of millions of years.
NCG 2146 is undergoing intense bouts of star formation, to such an extent that it is referred to as a starburst galaxy. This is a common state for barred spirals, but the extra gravitational disruption that NGC 2146 is enduring no doubt exacerbates the situation, compressing hydrogen-rich nebulae and triggering stellar birth.
Measuring about 80,000 light-years from end to end, NGC 2146 is slightly smaller than the Milky Way. It lies approximately 70 million light-years distant in the faint northern constellation of Camelopardalis (The Giraffe). Although it is fairly easy to see with a moderate-sized telescope as a faint elongated blur of light it was not spotted until 1876 when the German astronomer Friedrich Winnecke found it visually using just a 16 cm telescope.
Credits: X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI and NOIRLab/NSF/AURA Infrared: NSF/NOAO/KPNO
Image Processing: NASA/CXC/SAO/L. Frattare Release Date: Aug. 11, 2025
NASA's SpaceX Crew-10: Helicopter Flight Post-splashdown Off California Coast
NASA astronaut Anne McClain is seen inside an elevator onboard the SpaceX recovery ship Shannon that will take her up to a waiting helicopter to fly to Long Beach, California
NASA astronaut Nichole Ayers is helped aboard a helicopter on the SpaceX recovery ship Shannon to fly to Long Beach, California
NASA astronaut Anne McClain is helped aboard a helicopter on the SpaceX recovery ship Shannon to fly to Long Beach, California
Japan Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi is helped aboard a helicopter on the SpaceX recovery ship Shannon to fly to Long Beach, California
Roscosmos cosmonaut Kirill Peskov of Russia is seen inside an elevator onboard the SpaceX recovery ship Shannon that will take him up to a waiting helicopter to fly to Long Beach, California
The helicopter carrying NASA astronauts Anne McClain and Nichole Ayers, Japan Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi, and Roscosmos cosmonaut Kirill Peskov of Russia takes off from the SpaceX recovery ship Shannon shortly after they landed in the Pacific Ocean off the coast of San Diego, Calif., Saturday, Aug. 9, 2025.
From right to left, Japan Aerospace Exploration Agency (JAXA) astronaut Aki Hoshide, NASA astronaut Frank Rubio, and Roscosmos cosmonaut Sergey Prokopyev of Russia are seen aboard a helicopter en route to stage for the landing of the SpaceX Dragon Endurance spacecraft
At 11:33 a.m. EDT, on Saturday, August 9, 2025, the SpaceX Dragon spacecraft, carrying NASA astronauts Anne McClain and Nichole Ayers, Japan Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi, and Roscosmos cosmonaut Kirill Peskov of Russia splashed down off the coast of San Diego, California. This completes a stay in space of 148 days for the four-person crew. After egressing the spacecraft, the crew received medical checks before being flown via helicopter to meet up with a NASA aircraft in Long Beach, California, bound for Houston.
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke
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.
NASA’s SpaceX Crew-10 Returns to Ellington Field | Johnson Space Center
Video coverage of NASA’s SpaceX Crew-10 returning at Ellington Field in Houston, Texas, on August 9, 2025. Footage includes aircraft approach, landing, and taxi, as well as NASA leadership and fellow NASA astronauts greeting NASA astronauts Anne McClain and Nichole Ayers, Japan Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi, and Roscosmos cosmonaut Kirill Peskov of Russia as the crew exits the aircraft.
Crew-10 completed a long-duration science mission aboard the International Space Station and spent a total of 148 days in space. After undocking from the orbiting laboratory, Crew-10 splashed down at 11:33 a.m. EDT on Saturday, August 9, 2025, in the in the Pacific Ocean off the coast of California.
NASA Flight Engineers: Jonny Kim, Zena Cardman, Mike Fincke
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: National Aeronautics and Space Administration (NASA) Time: 3 minutes
Capture Date: Aug. 9, 2025 Release Date: Aug. 11, 2025
Gemini South Observatory's Laser Guide Star | NOIRLab
The Gemini South Telescope, half of the International Gemini Observatory, shines a low power laser into the sky to create a laser guide star. This laser guide star serves as a reference for the telescope's adaptive optics system so that it can 'cancel out' the effect of atmospheric turbulence on the images of its actual targets. The Gemini South telescope is located on a mountain in the Chilean Andes called Cerro Pachón, where very dry air and negligible cloud cover make this another prime telescope location.
Inside the Vera Rubin Auxiliary Telescope in Chile | NOIRLab
Bask in the red lights and enjoy a night inside the Rubin Auxiliary Telescope. As the telescope slews to its various targets, the Large Magellanic Cloud (0:03) and the Milky Way (0:08) peek through the dome slit.
The jointly funded National Science Foundation (NSF) and United States Department of Energy Vera C. Rubin Observatory is a brand new astronomy and astrophysics facility that is nearing completion on Cerro Pachón in Chile. It is named after the astronomer Vera Rubin. She provided the first convincing evidence for the existence of dark matter.
Learn more about Vera Rubin and the Rubin Auxiliary Telescope:
NASA Artemis II Orion Spacecraft: Moon Rocket Integration Prep | NASA Kennedy
NASA engineers and technicians pose for a photograph in front of the agency’s Artemis II Orion spacecraft on Thursday, Aug. 7, 2025, inside the Multi-Payload Processing Facility (MPPF) at NASA’s Kennedy Space Center in Florida. Orion arrived at the MPPF in early May for fueling and processing and will next head to the spaceport’s Launch Abort System Facility (LASF) to be integrated with its 44-foot-tall launch abort system. Once integration is complete, the stack will be transported to High Bay 3 inside NASA Kennedy’s Vehicle Assembly Building and integrated with the Space Launch System (SLS) rocket that will launch NASA’s Artemis II astronauts Reid Wiseman, Victor Glover, and Christina Koch, and Canadian Space Agency (CSA) astronaut Jeremy Hansen around the Moon and back.
The Artemis II crew will be sent on a ten-day Moon journey no earlier than April 2026.
Check the NASA Artemis II Mission page for updates: