Blue Ghost Moon Lander Mission End: Final Images | Firefly Aerospace
Learn more about NASA's CLPS Program:
https://www.nasa.gov/content/commercial-lunar-payload-services
Release Date: March 17, 2025
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Blue Ghost Moon Lander Mission End: Final Images | Firefly Aerospace
Learn more about NASA's CLPS Program:
https://www.nasa.gov/content/commercial-lunar-payload-services
Meet Astronaut Takuya Onishi of Japan (JAXA): Crew-10 Mission Specialist
Japan Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi will serve as mission specialist for NASA’s SpaceX Crew-10 mission. With 113 days in space, Crew-10 will mark Onishi’s second trip to the International Space Station. After being selected as an astronaut by JAXA in 2009, he flew as a flight engineer for Expeditions 48 and 49, becoming the first Japanese astronaut to robotically capture the Cygnus spacecraft. He also constructed a new experimental environment aboard Kibo, the station’s Japanese experiment module. After his first spaceflight, Onishi became certified as a JAXA flight director, leading the team responsible for operating Kibo from JAXA Mission Control in Tsukuba, Japan. He holds a bachelor’s degree in Aeronautics and Astronautics from the University of Tokyo.
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.
Meet Roscosmos Cosmonaut Kirill Peskov of Russia: Crew-10 Mission Specialist
Kirill Peskov will serve as a mission specialist for NASA’s SpaceX Crew-10 mission to the International Space Station, marking his first spaceflight. Before his selection as a Russian cosmonaut in 2018, he earned a degree in Engineering from the Ulyanovsk Civil Aviation School and was a co-pilot on the Boeing 757 and 767 aircraft for airlines Nordwind and Ikar. Assigned as a test cosmonaut in 2020, he has additional experience in skydiving, zero-gravity training, scuba diving, and wilderness survival.
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.
Meet NASA Astronaut Nichole Ayers: Crew-10 Pilot
NASA astronaut Nichole Ayers is the pilot of NASA’s SpaceX Crew-10 mission. This will be the first spaceflight for Ayers, who became a NASA astronaut in 2021. She is originally from Colorado Springs and Divide, Colorado. Ayers earned a bachelor’s degree in Mathematics from the U.S. Air Force Academy in Colorado and went on to earn a master’s degree in Computational and Applied Mathematics from Rice University in Houston, Texas. She is an active duty major in the U.S. Air Force and has flown over 1,400 flight hours.
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.
Meet Veteran NASA Astronaut Anne McClain: Crew-10 Commander
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 Mission Overview (Pre-launch) | International Space Station
NASA’s SpaceX Crew-10 mission to the International Space Station features NASA astronauts commander Anne McClain and pilot Nichole Ayers, Japanese Aerospace Exploration Agency (JAXA) astronaut and mission specialist Takuya Onishi, and Roscosmos cosmonaut and mission specialist Kirill Peskov of Russia.
The flight was the 10th crew rotation with SpaceX to the International Space Station as part of NASA’s Commercial Crew Program (CCP). While aboard, the international crew will conduct scientific investigations and technology demonstrations to help prepare humans for future missions and benefit people on Earth.
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's Johnson Space Center (JSC)
Duration: 3 minutes, 37 seconds
Release Date: March 17, 2025
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NASA’s Crew-10 SpaceX Dragon Spacecraft Docking | International Space Station
Following docking, the quartet opened the hatch and floated onboard the orbital outpost before providing welcoming remarks as their mission aboard the space station began. The crew members will conduct a long-duration science mission living and working aboard the microgravity laboratory to advance scientific knowledge and demonstrate new technologies for future human and robotic exploration missions. Such research benefits people on Earth and lays the groundwork for future human exploration through the agency’s Artemis missions, which will send astronauts to the Moon to prepare for future expeditions to Mars.
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/JSC/D. Pettit
Duration: 27 seconds
Release Date: March 16, 2025
Images of Young, Giant Exoplanets: Carbon Dioxide Detected | Webb Telescope
The NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope has captured direct images of multiple gas giant planets within an iconic planetary system. HR 8799, a young system 130 light-years away, has long been a key target for planet formation studies.
The observations indicate that the well-studied planets of HR 8799 are rich in carbon dioxide gas. This provides strong evidence that the system’s four giant planets formed much like Jupiter and Saturn, by slowly building solid cores that attract gas from within a protoplanetary disk.
The results also confirm that Webb can infer the chemistry of exoplanet atmospheres through imaging. This technique complements Webb’s powerful spectroscopic instruments, which resolve the atmospheric composition.
“By spotting these strong carbon dioxide features, we have shown there is a sizable fraction of heavier elements, like carbon, oxygen, and iron, in these planets’ atmospheres,” said William Balmer, of Johns Hopkins University in Baltimore. “Given what we know about the star they orbit, that likely indicates they formed via core accretion, which is an exciting conclusion for planets that we can directly see.”
Balmer is the lead author of the study announcing the results published today in The Astrophysical Journal. Balmer and his team’s analysis also includes Webb’s observation of a system 97 light-years away called 51 Eridani.
HR 8799 is a young system about 30 million years old, a fraction of our solar system’s 4.6 billion years. Still hot from their tumultuous formation, the planets within HR 8799 emit large amounts of infrared light that give scientists valuable data on how they formed.
Giant planets can take shape in two ways: by slowly building solid cores with heavier elements that attract gas, just like the giants in our solar system, or when particles of gas rapidly coalesce into massive objects from a young star’s cooling disk, which is made mostly of the same kind of material as the star. Knowing which formation model is more common can give scientists clues to distinguish between the types of planets they find in other systems.
“Our hope with this kind of research is to understand our own solar system, life, and ourselves in comparison to other exoplanetary systems, so we can contextualize our existence,” Balmer said. “We want to take pictures of other solar systems and see how they’re similar or different when compared to ours. From there, we can try to get a sense of how weird our solar system really is—or how normal.”
Of the nearly 6,000 exoplanets discovered, few have been directly imaged, as even giant planets are many thousands of times fainter than their stars. The images of HR 8799 and 51 Eridani were made possible by Webb’s NIRCam (Near-Infrared Camera) coronagraph, which blocks light from bright stars to reveal otherwise hidden worlds.
This technology allowed the team to look for infrared light emitted by the planets in wavelengths that are absorbed by specific gases. The team found that the four HR 8799 planets contain more heavy elements than previously thought.
“Webb's unique capabilities are allowing us to explore the wide diversity of these directly-imaged planets for the first time. This gives us important clues as to how such planetary systems have formed.” said Emily Rickman of the European Space Agency, a co-author of the study. “These new observations reiterate how valuable the HR 8799 multi-planet system is as a stepping stone to understand the formation of exoplanetary systems and of our own Solar System.”
The team is paving the way for more detailed observations to determine whether objects they see orbiting other stars are truly giant planets or objects such as brown dwarfs, which form like stars but don’t accumulate enough mass to ignite nuclear fusion.
“We have other lines of evidence that hint at these four HR 8799 planets forming using this bottom-up approach,” said Laurent Pueyo, an astronomer at the Space Telescope Science Institute in Baltimore, who co-led the work. “How common is this for planets we can directly image? We don’t know yet, but we’re proposing more Webb observations to answer that question.”
“We knew Webb could measure colors of the outer planets in directly imaged systems,” added Rémi Soummer, director of STScI’s Russell B. Makidon Optics Lab and former lead for Webb coronagraph operations. “We have been waiting for 10 years to confirm that our finely tuned operations of the telescope would also allow us to access the inner planets. Now the results are in and we can do interesting science with it.”
The NIRCam observations of HR 8799 and 51 Eridani were conducted as part of Guaranteed Time Observations programs 1194 and 1412 respectively.
Webb is the largest, most powerful telescope ever launched into space. Under an international collaboration agreement, ESA provided the telescope’s launch service, using the Ariane 5 launch vehicle. Working with partners, ESA was responsible for the development and qualification of Ariane 5 adaptations for the Webb mission and for the procurement of the launch service by Arianespace. ESA also provided the workhorse spectrograph NIRSpec and 50% of the mid-infrared instrument MIRI, which was designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) in partnership with JPL and the University of Arizona.
Webb is an international partnership between NASA, ESA and the Canadian Space Agency (CSA).
#NASA #ESA #Astronomy #Space #Science #JWST #JamesWebb #WebbTelescope #Stars #Planets #Exoplanets #PlanetarySystems #Star #HR8799 #51Eridani #Eridanus #Constellation #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education
The Small Magellanic Cloud: Colorful Clouds of a Nearby Galactic Neighbor | Hubble
Thanks to its proximity, the SMC is one of only a few galaxies that can be seen from Earth without the help of a telescope or binoculars. For viewers in the southern hemisphere and certain latitudes within the northern hemisphere, the SMC resembles a piece of the Milky Way that has broken off, though in reality it is much farther away than any part of our own galaxy.
With its 2.4-meter ‘eye’ and sensitive instruments, Hubble’s view of the SMC is far more detailed and vivid than what humans can see. Researchers used Hubble’s Wide Field Camera 3 instrument to observe this scene through four different filters. Each filter admits different wavelengths of light, creating a multicolored view of dust clouds drifting across a field of stars. Hubble’s view, however, is much more zoomed-in than our eyes, the better for it to observe very distant objects. This image captures a small region of the SMC near the center of NGC 346, a star cluster that is home to dozens of massive young stars.
Image Description: An area of space that is filled with stars. Most of the stars are small, distant dots in orange colors; closer stars shine with a bright glow and four thin spikes around them. These closer stars appear in bluish and reddish colors. Clouds from a nebula cover the left half of the scene, giving it a blue-greenish cast. More pieces of cloud drift over the black background of space on the right.
Planet Mars Images: March 14-16, 2025 | NASA's Curiosity & Perseverance Rovers
NASA’s SpaceX Crew-10 Mission: Extra Images & Outtakes | Kennedy Space Center
The flight was the 10th crew rotation with SpaceX to the International Space Station as part of NASA’s Commercial Crew Program (CCP). While aboard, the international crew will conduct scientific investigations and technology demonstrations to help prepare humans for future missions and benefit people on Earth.
The number of crew aboard the space station will increase to 11 for a short time as Crew-10 joins NASA astronauts Nick Hague, Suni Williams, Butch Wilmore, and Don Pettit, as well as Roscosmos cosmonauts Aleksandr Gorbunov, Alexey Ovchinin, and Ivan Vagner. Following a brief handover period, Hague, Williams, Wilmore, and Gorbunov will return to Earth no earlier than Wednesday, March 19, 2025. Ahead of Crew-9’s departure from station, mission teams will review weather conditions at the splashdown sites off the coast of Florida.
#NASA #Space #ISS #Science #SpaceXCrew10 #SpaceX #Falcon9Rocket #Astronauts #AnneMcClain #NicholeAyers #TakuyaOnishi #Japan #日本 #Cosmonaut #KirillPeskov #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition73 #KSC #Florida #UnitedStates #STEM #Education
Open Star Cluster NGC 460 in Tucana: Cocooned in Gas | Hubble
An open cluster of stars shines through misty, cocoon-like gas clouds in this Hubble Space Telescope image of NGC 460. NGC 460 is part of a greater collection of nebulae and star clusters known as the N83-84-85 complex. NGC 460 is located in a region of the Small Magellanic Cloud, a dwarf galaxy that orbits the Milky Way. This particular region contains a number of young star clusters and nebulae of different sizes—all likely related to each other. The clouds of gas and dust can give rise to stars as portions of them collapse, and radiation and stellar winds from those hot, young bright stars in turn shape and compress the clouds, triggering new waves of star formation. The hydrogen clouds are ionized by the radiation of nearby stars, causing them to glow.
The NGC 460 star cluster resides in one of the youngest parts of this interconnected complex of stellar clusters and nebulae. It is also home to a number of O-type stars: the brightest, hottest and most massive of the normal, hydrogen-burning stars (called main-sequence stars) like our Sun. O-type stars are rare—out of more than 4 billion stars in the Milky Way, only about 20,000 are estimated to be O-type stars. The area that holds NGC 460, known as N83, may have been created when two hydrogen clouds in the region collided with one another, creating several O-type stars and nebulae.
Open clusters like NGC 460 are made of anywhere from a few dozen to a few thousand stars loosely knitted together by gravity. Open clusters generally contain young stars that may migrate outward into their galaxies as time progresses. NGC 460’s stars may someday disperse into the Small Magellanic Cloud, one of the Milky Way’s closest galactic neighbors at about 200,000 light-years away. Because it is close and bright, it offers an opportunity to study phenomena that are difficult to examine in more distant galaxies.
Six overlapping observations from a study of the gas and dust between stars, called the interstellar medium, were combined to create this Hubble image. The study aims to understand how gravitational forces between interacting galaxies can foster bursts of star formation. This highly detailed 65 megapixel mosaic includes both visible and infrared wavelengths.
Image Description: Two bulbous, bluish clouds of gas against a field of multi-colored stars. Stars shine within the clouds as well as outside.
Shenzhou-19 Crew: 130+ Days in Orbit Advancing Science | China Space Station
The Shenzhou-19 crew has spent more than 130 days aboard China's Tiangong Space Station, advancing key scientific experiments, maintaining equipment, and conducting medical evaluations.
The mission's three astronauts—Cai Xuzhe, Song Lingdong, and Wang Haoze—have been living and working on the Tiangong Space Station throughout this period.
Over the past week, operations inside the national space laboratory have seen marked progress, with the crew conducting multiple scientific experiments, environmental monitoring, and equipment maintenance.
In the field of space medicine, they further examined the kinematic characteristics of astronauts during long-duration missions. This process utilized a structured-light 3D camera to capture motion data of astronauts in microgravity, enabling the analysis of movement patterns and offering valuable insights for future operations.
The crew has also conducted a study investigating changes in operational force under typical postures in orbit, as well as microgravity physics experiments. Additionally, they conducted self-checks on the space radiation biology exposure experiment module. It supports research on radiation damage, genetic mutations, protective drugs, and biological risk assessments on human beings and living organisms.
Other completed tasks include replacing samples for containerless experiment cabinets.
As part of their schedule, the astronauts underwent in-orbit medical emergency training to refine their skills, to become familiar with equipment placement, and to adapt rescue techniques to the microgravity environment.
They also filled out cognitive workload and fatigue assessment forms to contribute data on the impact of long-term spaceflight on operational performance.
Another key feature has been regular health monitoring, including dynamic electrocardiogram (ECG) and blood pressure checks, alongside exercise routines to counteract the effects of weightlessness. They also regularly cut their hair during their stay at the space station.
The Shenzhou-19 crew, including the country's first female space engineer, was sent into space on October 30, 2024, for a six-month mission. Their mission work includes 86 space science research and technology experiments.
Shenzhou-19 Crew:
Commander Cai Xuzhe (蔡旭哲)
Mission Specialist Wang Haoze (王浩泽)
Mission Specialist Song Lingdong (宋令东)
NASA’s SpaceX Crew-10 Dragon Spacecraft Docking | International Space Station
Following docking, the quartet opened the hatch and floated onboard the orbital outpost before providing welcoming remarks as their mission aboard the space station began. The crew members will conduct a long-duration science mission living and working aboard the microgravity laboratory to advance scientific knowledge and demonstrate new technologies for future human and robotic exploration missions. Such research benefits people on Earth and lays the groundwork for future human exploration through the agency’s Artemis missions, which will send astronauts to the Moon to prepare for future expeditions to Mars.
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/JSC/D. Pettit
Duration: 27 seconds
Release Date: March 16, 2025
NASA’s SpaceX Crew-10 Arrival: Highlights | International Space Station
NASA’s SpaceX Crew-10 mission with NASA astronauts Anne McClain, Nichole Ayers, Japan Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi, and Roscosmos cosmonaut Kirill Peskov of Russia autonomously docked to the forward-facing port of the Harmony module of the International Space Station at 12:04 a.m. EDT on March 16 , 2025, following a launch Friday, March 14, 2025, on the SpaceX Dragon Endurance spacecraft aboard a Falcon 9 rocket from Launch Complex 39A at the agency’s Kennedy Space Center in Florida.
Following docking, the quartet opened the hatch and floated onboard the orbital outpost before providing welcoming remarks as their mission aboard the space station began. The crew members will conduct a long-duration science mission living and working aboard the microgravity laboratory to advance scientific knowledge and demonstrate new technologies for future human and robotic exploration missions. Such research benefits people on Earth and lays the groundwork for future human exploration through the agency’s Artemis missions, which will send astronauts to the Moon to prepare for future expeditions to Mars.
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)
Duration: 28 minutes
Release Date: March 16, 2025
NASA's SpaceX Crew-10 Arrives at International Space Station
NASA's Crew-10 SpaceX Dragon spacecraft docked to the International Space Station on Sunday, March 16, 2025, at 12:04 a.m. Eastern Daylight Time (EDT), while the station was roughly 260 statute miles over the Atlantic Ocean. NASA astronauts Anne McClain and Nichole Ayers, Japan Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi, and Roscosmos cosmonaut Kirill Peskov of Russia entered the International Space Station shortly after opening the hatches between the space station and the SpaceX Dragon spacecraft at 1:35 a.m. EDT. McClain, Ayers, Onishi, and Peskov were welcomed by the Expedition 72 crew, including NASA astronauts Nick Hague, Don Petitt, Suni Williams, and Butch Wilmore, as well as Roscosmos cosmonauts Aleksandr Gorbunov, Alexey Ovchinin, and Ivan Vagner of Russia.
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.