Martian Landscapes: November 2024 | NASA's Curiosity & Perseverance Rovers
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Celebrating 12+ Years on Mars (2012-2024)
Celebrating 3+ Years on Mars
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Martian Landscapes: November 2024 | NASA's Curiosity & Perseverance Rovers
Support FriendsofNASA.org
Celebrating 12+ Years on Mars (2012-2024)
Celebrating 3+ Years on Mars
Blue Ghost's Journey to The Moon | Firefly Aerospace | NASA CLPS Program
Firefly’s first Blue Ghost mission, named Ghost Riders in the Sky, will deliver 10 scientific instruments and technology demonstrations to the lunar surface as part of NASA’s Commercial Lunar Payload Services (CLPS) initiative. Upon launching in mid-January 2025, Blue Ghost will spend approximately 45 days in transit to the Moon, allowing ample time to conduct health checks on each subsystem and begin payload science. Blue Ghost will then land in Mare Crisium and operate payloads for a complete lunar day (about 14 Earth days). Following payload operations, Blue Ghost will capture imagery of the lunar sunset and provide critical data on how lunar regolith reacts to solar influences during lunar dusk conditions. The lander will then operate for several hours into the lunar night.
For more information on Blue Ghost mission visit: https://fireflyspace.com/missions/blue-ghost-mission-1/
Firefly's Blue Ghost mission will land near a volcanic feature called Mons Latreille within Mare Crisium, a more than 300-mile-wide basin located in the northeast quadrant of the lunar near side. The mission will carry NASA investigations and first-of-their-kind technology demonstrations to further our understanding of the Moon’s environment and help prepare for future human missions to the lunar surface, as part of the agency’s Moon to Mars exploration approach.
It includes payloads testing lunar subsurface drilling, regolith sample collection, global navigation satellite system abilities, radiation tolerant computing, and lunar dust mitigation. The data captured also benefits humanity by providing insights into how space weather and other cosmic forces impact Earth.
Under the CLPS model, NASA is investing in commercial delivery services to the Moon to enable industry growth and support long-term lunar exploration. As a primary customer for CLPS deliveries, NASA aims to be one of many customers on future flights.
As part of its Artemis campaign, NASA is working with multiple U.S. companies to deliver science and technology to the lunar surface. These companies are eligible to bid on task orders to deliver NASA payloads to the Moon. The task order includes payload integration and operations and launching from Earth and landing on the surface of the Moon. Existing CLPS contracts are indefinite-delivery/indefinite-quantity contracts with a cumulative maximum contract value of $2.6 billion through 2028.
Galaxy NGC 2090 in Visible/UV vs. Infrared Light | Hubble & Webb Telescope Views
This was one of the group of galaxies studied early on by the NASA/European Space Agency Hubble Space Telescope, observing Cepheid variable stars in it as part of refining the measurement of the Hubble constant. The Cepheid-based measurement from that study in 1998 put NGC 2090 as 37 million light-years away; the newest measurements have NGC 2090 slightly farther away, at 40 million light-years. Hubble is to this day surveying galaxies in visible and ultraviolet (UV) light.
Before and since that project, NGC 2090 has been well studied as a very prominent nearby example of star formation. It has been described as a flocculent spiral, meaning a spiral galaxy with a patchy, dusty disc and arms that are flaky or not visible at all. Visible-light images show this well, but the near-infrared data from NIRCam used in this image reveal the spiral arms with remarkable clarity. NIRCam also picks up bright light from stars, displayed by the blue colors most visible in the center. Meanwhile, mid-infrared light emitted mainly by the important carbon-based compounds known as polycyclic aromatic hydrocarbons along the many strands of gas and dust is captured by MIRI and shown here in red.
These data on NGC 2090 were collected as part of an observing program (#3707) taking a census of nearby massive, star-forming galaxies much like it. These galaxies are at just the right distance, with the right size and level of activity, that Webb’s instruments can capture a comprehensive picture of the star-forming activity, including the tightly-bound clusters that stars often form in, and the clouds of gas in the galaxy where stars can be born. The rich collection of detailed images like this one will be of value to astronomers studying this area for years to come.
Close-up View: Spiral Galaxy NGC 2090 in Infrared | Webb Telescope
This was one of the group of galaxies studied early on by the NASA/European Space Agency Hubble Space Telescope, observing Cepheid variable stars in it as part of refining the measurement of the Hubble constant. The Cepheid-based measurement from that study in 1998 put NGC 2090 as 37 million light-years away; the newest measurements have NGC 2090 slightly farther away, at 40 million light-years. Hubble is to this day surveying galaxies in visible and ultraviolet light.
Before and since that project, NGC 2090 has been well studied as a very prominent nearby example of star formation. It has been described as a flocculent spiral, meaning a spiral galaxy with a patchy, dusty disc and arms that are flaky or not visible at all. Visible-light images show this well, but the near-infrared data from NIRCam used in this image reveal the spiral arms with remarkable clarity. NIRCam also picks up bright light from stars, displayed by the blue colors most visible in the center. Meanwhile, mid-infrared light emitted mainly by the important carbon-based compounds known as polycyclic aromatic hydrocarbons along the many strands of gas and dust is captured by MIRI and shown here in red.
These data on NGC 2090 were collected as part of an observing program (#3707) taking a census of nearby massive, star-forming galaxies much like it. These galaxies are at just the right distance, with the right size and level of activity, that Webb’s instruments can capture a comprehensive picture of the star-forming activity, including the tightly-bound clusters that stars often form in, and the clouds of gas in the galaxy in which stars can be born. The rich collection of detailed images like this one will be of value to astronomers studying this area for years to come.
Image Description: A spiral galaxy with a wide, oval-shaped disc. It has a shining spot at the center where two curving, pale red spiral arms emerge, wrapping once each around the galaxy. They are surrounded by a whirl of bright threads and patches of dust with spots of star formation scattered throughout. The glow of the disc fades smoothly into the background where patches of dust can be seen, as well as foreground stars.
Spiral Galaxy NGC 2090: Tracing Spiral Arms in Infrared | Webb Telescope
This NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope picture shows the spiral galaxy NGC 2090, located in the constellation Columba. This combination of data from Webb’s Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI) shows the galaxy’s two winding spiral arms and the swirling gas and dust of its disc in magnificent and unique detail.
This was one of the group of galaxies studied early on by the NASA/European Space Agency Hubble Space Telescope, observing Cepheid variable stars in it as part of refining the measurement of the Hubble constant. The Cepheid-based measurement from that study in 1998 put NGC 2090 as 37 million light-years away; the newest measurements have NGC 2090 slightly farther away, at 40 million light-years. Hubble is to this day surveying galaxies in visible and ultraviolet light.
Before and since that project, NGC 2090 has been well studied as a very prominent nearby example of star formation. It has been described as a flocculent spiral, meaning a spiral galaxy with a patchy, dusty disc and arms that are flaky or not visible at all. Visible-light images show this well, but the near-infrared data from NIRCam used in this image reveal the spiral arms with remarkable clarity. NIRCam also picks up bright light from stars, displayed by the blue colors most visible in the center. Meanwhile, mid-infrared light emitted mainly by the important carbon-based compounds known as polycyclic aromatic hydrocarbons along the many strands of gas and dust is captured by MIRI and shown here in red.
These data on NGC 2090 were collected as part of an observing program (#3707) taking a census of nearby massive, star-forming galaxies much like it. These galaxies are at just the right distance, with the right size and level of activity, that Webb’s instruments can capture a comprehensive picture of the star-forming activity, including the tightly-bound clusters that stars often form in, and the clouds of gas in the galaxy in which stars can be born. The rich collection of detailed images like this one will be of value to astronomers studying this area for years to come.
Image Description: A spiral galaxy with a wide, oval-shaped disc. It has a shining spot at the center where two curving, pale red spiral arms emerge, wrapping once each around the galaxy. They are surrounded by a whirl of bright threads and patches of dust with spots of star formation scattered throughout. The glow of the disc fades smoothly into the background where patches of dust can be seen, as well as foreground stars.
#NASA #ESA #Astronomy #Space #Galaxies #Galaxy #NGC2090 #Columba #SpiralGalaxy #FlocculentSpiral #HubbleConstant #CepheidVariableStars #TFDistanceMethod #Constellation #Cosmos #Universe #UnfoldTheUniverse #JWST #InfraredAstronomy #Europe #CSA #Canada #GSFC #STScI #UnitedStates #Europe #STEM #Education
NASA's Space to Ground—Six Minutes of Serenity | Week of Nov. 27, 2024
Take some time during this holiday season and enjoy a few minutes of serenity as we offer a glimpse of the beauty of our home planet from the vantage point of the International Space Station.
Happy Thanksgiving!
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 #Space #Science #ISS #Earth #ThanksgivingHoliday #Astronauts #Astronaut #DonPettit #SpaceArt #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #SpaceLaboratory #HumanSpaceflight #UnitedStates #Expedition72 #STEM #Education #HD #Video
Liftoff of China's Landspace Zhuque-2E Methalox Commercial Rocket
Chinese private aerospace company Landspace is a commercial world leader in methane/liquid oxygen powered rocket engines that have proved capable of delivering payloads to low-Earth orbit.
The new Zhuque-2E rocket has upgraded first stage engines and a new second stage with an engine nozzle that swivels. The Zhuque-2E will finally reach the 6 metric ton low-Earth orbit (LEO)/4 metric ton Sun-synchronous orbit (SSO) capability Landspace planned. China's pioneering commercial space launch company, LandSpace, now has the opportunity to send heavy satellite payloads to Earth orbit before SpaceX's Starship does using methane/liquid oxygen engines.
LandSpace Technology Corporation is a Chinese commercial space launch provider based in Beijing. It was founded in 2015 by Zhang Changwu. In July 2023, the company's Zhuque-2 rocket became the first methane-fueled orbital launch vehicle in the world after reaching orbit on its second flight. LandSpace planned three Zhuque-2 launches in 2024 and another six in 2025.
Zhuque-2E Y1 Methalox Rocket Data Sheet:
47.3m*3.35m, 220t liftoff mass
4 TQ-12 methalox engines provide 282t liftoff thrust
1 TQ-15A vacuum engine in 2nd stage
Mission profile:
T+140s 1st stage off
T+143s stagging
T+145s 2nd stage ignition
T+214s fairings jettison
T+243s throttling to 60%
T+395s 2nd stage off
T+505s satellites separation
2 satellites to 300km*500km*50° LEO
Launch of China's Landspace Zhuque-2E Methalox Commercial Rocket
Chinese private aerospace company Landspace is a commercial world leader in methane/liquid oxygen powered rocket engines that have proved capable of delivering payloads to low-Earth orbit.
The new Zhuque-2E rocket has upgraded first stage engines and a new second stage with an engine nozzle that swivels. The Zhuque-2E will finally reach the 6 metric ton low-Earth orbit (LEO)/4 metric ton Sun-synchronous orbit (SSO) capability Landspace planned. China's pioneering commercial space launch company, LandSpace, now has the opportunity to send heavy satellite payloads to Earth orbit before SpaceX's Starship does using methane/liquid oxygen engines.
LandSpace Technology Corporation is a Chinese commercial space launch provider based in Beijing. It was founded in 2015 by Zhang Changwu. In July 2023, the company's Zhuque-2 rocket became the first methane-fueled orbital launch vehicle in the world after reaching orbit on its second flight. LandSpace planned three Zhuque-2 launches in 2024 and another six in 2025.
Zhuque-2E Y1 Methalox Rocket Data Sheet:
47.3m*3.35m, 220t liftoff mass
4 TQ-12 methalox engines provide 282t liftoff thrust
1 TQ-15A vacuum engine in 2nd stage
Mission profile:
T+140s 1st stage off
T+143s stagging
T+145s 2nd stage ignition
T+214s fairings jettison
T+243s throttling to 60%
T+395s 2nd stage off
T+505s satellites separation
2 satellites to 300km*500km*50° LEO
NASA’s Europa Clipper: Millions of Miles Down, Instruments Deploying | JPL
This animation demonstrates how the boom of Europa Clipper’s magnetometer deployed—while the spacecraft was in flight—to its full length of 28 feet (8.5 meters). Headed to Jupiter’s moon Europa, the Europa Clipper spacecraft is operating without a hitch and will reach Mars in just three months for a gravity assist.
NASA’s Europa Clipper, launched Oct. 14, 2024, on a journey to Jupiter’s ocean moon Europa, is already 13 million miles (20 million kilometers) from Earth. Two science instruments have deployed hardware that will remain at attention, extending out from the spacecraft, for the next decade—through the cruise to Jupiter and the entire prime mission.
A SpaceX Falcon Heavy rocket launched the Europa Clipper spacecraft away from Earth’s gravity, and now the spacecraft is zooming along at 22 miles per second (35 kilometers per second) relative to the Sun. Europa Clipper is the largest spacecraft NASA has ever developed for a planetary mission. It will travel 1.8 billion miles (2.9 billion kilometers) to arrive at Jupiter in 2030 and in 2031 will begin a series of 49 flybys, using a suite of instruments to gather data that will tell scientists if the icy moon and its internal ocean have the conditions needed to harbor life.
For now, the information mission teams are receiving from the spacecraft is strictly engineering data (the science will come later), telling them how the hardware is operating. Things are looking good. The team has a checklist of actions the spacecraft needs to take as it travels deeper into space.
Here is a peek:
Boom Times
Shortly after launch, the spacecraft deployed its massive solar arrays that extend the length of a basketball court. Next on the list was the magnetometer’s boom. It uncoiled from a canister mounted on the spacecraft body, extending a full 28 feet (8.5 meters).
To confirm that all went well with the boom deployment, the team relied on data from the magnetometer’s three sensors. Once the spacecraft is at Jupiter, these sensors will measure the magnetic field around Europa, both confirming the presence of the ocean thought to be under the moon’s icy crust and telling scientists about its depth and salinity.
On the Radar
After the magnetometer, the spacecraft deployed several antennas for the radar instrument. Now extending crosswise from the solar arrays, the four high-frequency antennas form what look like two long poles, each measuring 57.7 feet (17.6 meters) long. Eight rectangular very-high-frequency antennas, each 9 feet (2.76 meters) long, were also deployed—two on the two solar arrays.
“It’s an exciting time on the spacecraft, getting these key deployments done,” said Europa Clipper project manager Jordan Evans of NASA’s Jet Propulsion Laboratory in Southern California. “Most of what the team is focusing on now is understanding the small, interesting things in the data that help them understand the behavior of the spacecraft on a deeper level. That’s really good to see.”
Instrument Checkout
The remaining seven instruments will be powered on and off through December 2024 and January 2025 so that engineers can check their health. Several instruments, including the visible imager and the gas and dust mass spectrometers, will keep their protective covers closed for the next three or so years to guard against potential damage from the Sun during Europa Clipper’s time in the inner solar system.
Mars-Bound
Once all the instruments and engineering subsystems have been checked out, mission teams will shift their focus to Mars. On March 1, 2025, Europa Clipper will reach Mars’ orbit and begin to loop around the Red Planet, using the planet’s gravity to gain speed. (This effect is similar to how a ball thrown at a moving train will bounce off the train in another direction at a higher speed.) Mission navigators already have completed one trajectory correction maneuver, as planned, to get the spacecraft on the precise course.
At Mars, scientists plan to turn on the spacecraft’s thermal imager to capture multicolored images of Mars as a test operation. They also plan to collect data with the radar instrument so engineers can be sure it is operating as expected.
The spacecraft will perform another gravity assist in December 2026, swooping by Earth before making the remainder of the long journey to the Jupiter system. At that time, the magnetometer will measure Earth’s magnetic field, calibrating the instrument.
More About Europa Clipper
Europa Clipper’s three main science objectives are to determine the thickness of the moon’s icy shell and its interactions with the ocean below, to investigate its composition, and to characterize its geology. The mission’s detailed exploration of Europa will help scientists better understand the astrobiological potential for habitable worlds beyond our planet.
Managed by Caltech in Pasadena, California, JPL leads the development of the Europa Clipper mission in partnership with the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, for NASA’s Science Mission Directorate in Washington. APL designed the main spacecraft body in collaboration with JPL and NASA’s Goddard Space Flight Center in Greenbelt, Maryland, NASA’s Marshall Space Flight Center in Huntsville, Alabama, and Langley Research Center in Hampton, Virginia. The Planetary Missions Program Office at Marshall executes program management of the Europa Clipper mission. NASA’s Launch Services Program, based at Kennedy, managed the launch service for the Europa Clipper spacecraft.
NASA "Espacio a Tierra" | El arte de la ciencia espacial: 08 de noviembre de 2024
Espacio a Tierra, la versión en español de las cápsulas Space to Ground de la NASA, te informa semanalmente de lo que está sucediendo en la Estación Espacial Internacional.
Aprende más sobre la ciencia a bordo de la estación espacial: https://www.nasa.gov/international-space-station/space-station-research-and-technology/ciencia-en-la-estacion/
Ciencia de la NASA: https://ciencia.nasa.gov
Para obtener más información sobre la ciencia de la NASA, suscríbete al boletín semanal: https://www.nasa.gov/suscribete
#NASA #Space #Science #ISS #Earth #NASAenespañol #español #SpaceX #SpaceXDragonSpacecraft #Reboost #SpaceArt #DonPettit #Astronauts #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #HumanSpaceflight #SpaceLaboratory #UnitedStates #Expedition72 #STEM #Education #HD #Video
NASA's Launch Services Program: 2024 Highlights | Kennedy Space Center
NASA’s Launch Services Program (LSP) started in 2024 with plans to keep up a steady "PACE"! How did that "GOES"? It was twice over successful with PREFIRE and a Demo 2 lift off from distant launch pads before we set sail for Europa. We recap a stellar year of science missions!
NASA’s Launch Services Program (LSP) is responsible for launching rockets delivering spacecraft that observe the Earth, visit other planets and explore the universe—from weather satellites to telescopes to Mars rovers and more.
LSP functions as a broker, matching spacecraft with the best-suited rockets, managing the launch process, providing support from pre-mission planning to post-launch. LSP helps implement NASA’s policy of a mixed-fleet launch strategy that uses both existing and emerging domestic launch capabilities to assure access to space.
NASA’s Launch Services Program is based at the agency’s Kennedy Space Center in Florida.
New Mars Images: Nov. 24-25, 2024 | NASA's Mars Curiosity & Perseverance Rovers
Celebrating 12+ Years on Mars (2012-2024)
Celebrating 3+ Years on Mars
NASA's Firefly Blue Ghost Robotic Moon Lander Mission 1: Early 2025 Launch
The company named the mission Ghost Riders in the Sky. It will land near a volcanic feature called Mons Latreille within Mare Crisium, a more than 300-mile-wide basin located in the northeast quadrant of the lunar near side. The mission will carry NASA investigations and first-of-their-kind technology demonstrations to further our understanding of the Moon’s environment and help prepare for future human missions to the lunar surface, as part of the agency’s Moon to Mars exploration approach. This includes payloads testing lunar subsurface drilling, regolith sample collection, global navigation satellite system abilities, radiation tolerant computing, and lunar dust mitigation. The data captured also benefits humanity by providing insights into how space weather and other cosmic forces impact Earth.
Under the CLPS model, NASA is investing in commercial delivery services to the Moon to enable industry growth and support long-term lunar exploration. As a primary customer for CLPS deliveries, NASA aims to be one of many customers on future flights.
As part of its Artemis campaign, NASA is working with multiple U.S. companies to deliver science and technology to the lunar surface. These companies are eligible to bid on task orders to deliver NASA payloads to the Moon. The task order includes payload integration and operations and launching from Earth and landing on the surface of the Moon. Existing CLPS contracts are indefinite-delivery/indefinite-quantity contracts with a cumulative maximum contract value of $2.6 billion through 2028.
Long March 12: Rollout of China's New Medium Lift Rocket | Wenchang Launch Site
Experts said due to its enhanced overall capacity, the new rocket, the country's first single-core liquid carrier rocket with a diameter of 3.8 meters, will gradually replace China's older 3.35-meter diameter series. With better reliability in attitude control, the Long March-12 is expected to become the basic model for future reusable rockets in China.
The rocket, developed by the Shanghai Academy of Spaceflight Technology, features a two-stage configuration. The first stage is powered by four liquid oxygen/kerosene engines, each with a thrust of 1,250 kilonewtons, while the second stage uses two liquid oxygen/kerosene engines with a thrust of 180 kilonewtons each, China Central Television reported.
Its payload capacity to low Earth orbit is no less than 10 tons, and its capacity to reach a 700-kilometer sun-synchronous orbit is no less than 6 tons. The rocket's fairing is standardly available in diameters of 5.2 meters and 4.2 meters, allowing for multi-size adaptation based on different missions, the report said.
Apart from the 5-meter diameter Long March-5 rocket, the "fatty" in the family, the Long March series typically features a diameter of 3.35 meters, while solid rockets are generally slimmer, with diameters usually below 3 meters.
The Long March-12 rocket represents a significant advancement in the country's space launch capabilities, as the increased diameter addresses the limitations of the previous 3.35-meter rockets, allowing for more powerful engines, enhanced payload capacity, and better expandability of rocket thrust. Therefore, the Long March-12 is expected to significantly improve overall launch capability compared to previous generations, gradually replacing the older 3.35-meter models, Chinese space analyst Song Zhongping told the Global Times on Tuesday.
According to CCTV, the pioneering shape of the Long March-12 is based on the improved development of China's new generation of main liquid oxygen/kerosene engines, the YF-100 series, and is the result of repeated verification, research, and testing.
This notable feature allows for both railway transportation to various launch sites and the optimization of compatibility between the rocket's diameter and the number of engines, facilitating capability expansion and thus laying the groundwork for future reusable rockets, experts said.
Song pointed to an important technical parameter for launch vehicles, the length-to-diameter ratio, which affects the rocket's stability during recovery.
"Theoretically, a more optimal length-to-diameter ratio enhances the stability of a reusable rocket. The previous 3.35-meter rocket was relatively slender and long, making it more challenging to control its attitude. By increasing the diameter, the length-to-diameter ratio can be reduced, making it easier to control the rocket's stability and facilitating recovery," he said.
The expert anticipates that the Long March-12 rocket will become the basic model for future reusable rockets in China, while allowing for the development of various configurations based on it. This standardization will be crucial for the future of rocket recovery and reuse, Song noted.
Previous media reports said the Hainan Commercial Space Launch Site will be equipped with two liquid rocket launch pads. The first launch pad will be dedicated to the Long March-8 carrier rocket, while the other launch pad will provide launch services for the Long March-12 vehicle.
Canadarm2's DEXTRE: Robotic 'Hands' at Work | International Space Station
NASA Astronaut Don Pettit: "Payload package deployment from the Japan Aerospace Exploration Agency (JAXA) airlock using the [Canadian Space Agency's] Canadarm2 with the Special Purpose Dexterious Manipulator (SPDM). This timelapse shows the two smaller arms on SPDM grappling a materials exposure payload (MISSE) and moving it away. I especially like the sun angles moving around the window frame like a 16-hour sundial. This time exposure represents about 10 hours."
The International Space Station's Dextre, also known as the Special Purpose Dexterous Manipulator (SPDM), is the fine-tuned robotic hand, attached to the Canadarm2 robotic arm.
The 17-meter-long (55+ feet) Canadarm2 robotic arm and the 3.7m (12 feet) high Dextre fine-tuned robotic hand are part of Canada's contribution to the International Space Station (ISS). Canadarm2 was extensively involved in the assembly of the orbiting laboratory.
Dextre tackles the tough or routine jobs that need to be done in the harsh environment of space. The Station's robotic assistant allows astronauts to spend more time doing scientific experiments instead of performing risky spacewalks.
Dextre's body was designed to move in many different ways. Each of its arms has seven joints that can move up and down, go from side to side, and rotate. This large range of motion means Dextre can actually carry out more complex movements than a human arm. Each hand has a retractable motorized wrench, a camera and lights for close-up viewing, and a retractable connector to provide power, data and video connection.
The robot can carefully grip delicate equipment without causing damage. For example, it can successfully manipulate small safety caps, cables and wires with minute precision—all while being controlled from Earth, hundreds of kilometers away. Dextre can can ride on the end of Canadarm2 to move from each worksite or be ferried on the Mobile Base System to work almost anywhere on the ISS.
The robot is operated by ground control teams at the Canadian Space Agency (CSA) headquarters outside Montreal, Quebec, and at NASA.
An international partnership of space agencies provides and operates the elements of the ISS. The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.
Video details: Nikon Z9, Nikon 8mm f2.8 fisheye, timelapse assembled by Chris Getteau of NASA/JSC
#NASA #Space #Astronomy #Science #ISS #SpaceTechnology #Canada #CSA #Canadarm2 #SPDM #Dextre #Robotics #Robots #JAXA #Japan #日本 #Astronaut #DonPettit #Expedition72 #HumanSpaceflight #InternationalCooperation #JSC #UnitedStates #STEM #Education #Timelapse #HD #Video
The Sombrero Galaxy: New Close-up View | James Webb Space Telescope
The NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope recently imaged the Sombrero galaxy with its Mid-InfraRed Instrument (MIRI), resolving the clumpy nature of the dust along the galaxy’s outer ring.
The mid-infrared light highlights the gas and dust that are a feature of the star formation taking place among the Sombrero galaxy’s outer disc. The rings of the Sombrero galaxy produce less than one solar mass of stars per year, in comparison to the Milky Way’s roughly two solar masses a year. It is not a particular hotbed of star formation.
The Sombrero galaxy is around 30 million light-years from Earth in the constellation Virgo.
#NASA #ESA Astronomy #Space #Science #Galaxies #Galaxy #SombreroGalaxy #Messier104 #M104 #NGC4594 #Virgo #Constellation #Universe #JWST #InfraredAstronomy #WebbSpaceTelescope #GSFC #STScI #CSA #Canada #ESA #Europe #UnitedStates #STEM #Education #HD #Video