Friday, December 06, 2024

NASA's Space to Ground: "It's Very Suni in Space" | Week of Dec. 6, 2024

NASA's Space to Ground: "It's Very Suni in Space" Week of Dec. 6, 2024


NASA's Space to Ground is your weekly update on what's happening aboard the International Space Station. The science-packed SpaceX Dragon cargo spacecraft will wait another week before departing the International Space Station as mission managers monitor weather conditions at the splashdown sites. Meanwhile, the seven-member Expedition 72 crew geared up for a spacewalk planned later in December and serviced an array of science hardware and exercise equipment.

Expedition 72 Crew
Station Commander: Suni Williams
Roscosmos (Russia): Alexey Ovchinin, Ivan Vagner, Aleksandr Gorbunov
NASA: Butch Wilmore, Don Pettit, Nick Hague

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.

Learn more about the important research being operated on Station:
https://www.nasa.gov/iss-science 
For more information about STEM on Station:
https://www.nasa.gov/stemonstation
Science, Technology, Engineering, Math (STEM)


Video Credit: NASA's Johnson Space Center (JSC)
Duration: 4 minutes
Release Date: 
Dec. 6, 2024


#NASA #Space #Science #ISS #Earth #Astronaut #SuniWilliams #Astronauts #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #SpaceLaboratory #HumanSpaceflight #UnitedStates #Expedition72 #STEM #Education #HD #Video

Thursday, December 05, 2024

Vega-C Lifts off with Sentinel-1C Earth Satellite | European Space Agency

Vega-C Lifts off with Sentinel-1C Earth Satellite | European Space Agency





On December 5, 2024, the mobile building surrounding the Vega-C rocket with Earth-observer Sentinel-1C was rolled back at Europe's Spaceport in French Guiana, setting the rocket up for launch to a sun-synchronous orbit.
Vega-C on the launch pad with Earth-observer Sentinel-1C at Europe's Spaceport in French Guiana, 5 December 2024.
View of Vega-C rocket, flight VV25, looking up on the launch pad at Europe's Spaceport in French Guiana, December 4, 2024.
Following Sentinel-1C encapsulation inside the Vega-C rocket fairing, the team at Europe’s Spaceport in Kourou has signed the sticker on the rocket as per tradition.

The third Copernicus Sentinel-1 satellite, Sentinel-1C, has launched aboard a Vega-C rocket, flight VV25, from Europe’s Spaceport in French Guiana. The rocket lifted off on December 5, 2024, at 22:20 CET (18:20 local time).

Sentinel-1C extends the legacy of its predecessors, delivering high-resolution radar imagery to monitor Earth’s changing environment, supporting a diverse range of applications and advance scientific research. Additionally, Sentinel-1C introduces new capabilities for detecting and monitoring maritime traffic.

The launch also marks Vega-C’s ‘return to flight’, a key step in restoring Europe’s independent access to space. Vega-C is the evolution of the Vega family of rockets and delivers increased performance, greater payload volume and improved competitiveness.

Learn more about the European Space Agency's Copernicus Earth Observation Programme:
https://sentinel.esa.int/web/sentinel/copernicus/

Credits: ESA–M. Pédoussaut/S. Corvaj/CNES-ARIANESPACE/Optique vidéo du CSG-P.Piperot
Image Dates: Dec. 4-5, 2024

#NASA #ESA #Space #Science #Satellites #Sentinel1C #CopernicusProgramme #VegaCRocket #FlightVV25 #RadarSatellites #SAR #SyntheticApertureRadar #ElectromagneticSpectrum #Planet #Earth #Atmosphere #Climate #ClimateChange #Environment #Weather #Meteorology #ExtremeWeather #Europe #EarthObservation #RemoteSensing #STEM #Education

Mars Images: December 4-5, 2024 | NASA's Curiosity & Perseverance Rovers

Mars Images: December 4-5, 2024 | NASA's Curiosity & Perseverance Rovers

MSL - sol 4375
MSL - sol 4375
MSL - sol 4375
MSL - sol 4371
MSL - sol 4371
Mars 2020 - sol 1348
MSL - sol 4382
Celebrating 12+ Years on Mars (2012-2024)
Mission Name: Mars Science Laboratory (MSL)
Rover Name: Curiosity
Main Job: To determine if Mars was ever habitable to microbial life. 
Launch: Nov. 6, 2011
Landing Date: Aug. 5, 2012, Gale Crater, Mars

Celebrating 3+ Years on Mars
Mission Name: Mars 2020
Rover Name: Perseverance
Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.
Launch: July 30, 2020    
Landing: Feb. 18, 2021, Jezero Crater, Mars

For more information on NASA's Mars missions, visit: mars.nasa.gov

Image Credits: NASA/JPL-Caltech/ASU/MSSS
Processing: Kevin M. Gill
Image Release Date: Dec. 4-5, 2024

#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #CuriosityRover #MSL #MountSharp #GaleCrater #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #JPL #Caltech #UnitedStates #CitizenScience #KevinGill #STEM #Education

New Expedition 72 NASA Crew Images | International Space Station

New Expedition 72 NASA Crew Images | International Space Station

NASA astronauts Don Pettit and Suni Williams, Expedition 72 flight engineer and commander respectively, pose for a fun holiday season portrait while speaking on a ham radio inside the International Space Station's Columbus laboratory module.
NASA astronaut and Expedition 72 Commander Suni Williams poses for a fun holiday season portrait while speaking on a ham radio inside the International Space Station's Columbus laboratory module.
NASA astronaut and Expedition 72 Flight Engineer Nick Hague processes radiation-resistant samples of Arthrospira C micro-algae and stows them in an incubator for analysis inside the International Space Station's Columbus laboratory module. The samples will be exposed to different light intensities to observe how they affect the micro-algae’s cell growth and oxygen production. Results may advance the development of spacecraft life support systems and fresh food production in space.
NASA astronaut and Expedition 72 Commander Suni Williams smiles for a portrait inside the International Space Station's Zvezda service module during dinner time.
NASA astronauts (from left) Don Pettit and Butch Wilmore, both Expedition 72 flight engineers, pack external research hardware removed from the Kibo laboratory module's airlock. The hardware housed a variety of samples exposed to the vacuum of space such as polymers, photovoltaic devices, and more. The samples will be returned to Earth and examined to understand how space radiation, the extreme thermal environment, micrometeoroids, and more affect materials possibly benefitting the space industry.
Expedition 72 Commander Suni Williams and Flight Engineer Don Pettit, both NASA astronauts, pose for a portrait in front of the Advanced Plant Habitat located inside the International Space Station's Kibo laboratory module. The Plant Habitat provides a large, enclosed, environmentally controlled chamber designed to support commercial and fundamental plant research in microgravity.
NASA astronaut and Expedition 72 Flight Engineer Don Pettit takes a break and poses for a portrait aboard the International Space Station's Destiny laboratory module.
NASA astronaut and Expedition 72 Flight Engineer Butch Wilmore swaps sample cassettes inside the Advanced Space Experiment Processor-4 (ADSEP-4) located aboard the International Space Station's Kibo laboratory module. The ADSEP-4 is a portable research facility that supports multiple types of science experiments on the orbital outpost and also interfaces with the SpaceX Dragon and Northrop Grumman Cygnus cargo spacecraft.

The science-packed SpaceX Dragon cargo spacecraft will wait another week before departing the International Space Station as mission managers monitor weather conditions at the splashdown sites. Meanwhile, the seven-member Expedition 72 crew geared up for a spacewalk planned later in December and serviced an array of science hardware and exercise equipment.


Expedition 72 Crew
Station Commander: Suni Williams
Roscosmos (Russia): Alexey Ovchinin, Ivan Vagner, Aleksandr Gorbunov
NASA: Butch Wilmore, Don Pettit, Nick Hague

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.

Learn more about the important research being operated on Station:
https://www.nasa.gov/iss-science 
For more information about STEM on Station:
https://www.nasa.gov/stemonstation
Science, Technology, Engineering, Math (STEM)


Image Credit: NASA's Johnson Space Center (JSC)
Image Dates: Nov. 15-29, 2024

#NASA #Space #Science #ISS #Earth #Astronauts #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #SpaceLaboratory #HumanSpaceflight #UnitedStates #Expedition72 #STEM #Education

Closest-ever Look at a Quasar: 3C 273 in Virgo | Hubble Space Telescope

Closest-ever Look at a Quasar: 3C 273 in Virgo | Hubble Space Telescope

Image Description: A two-panel annotated image of quasar 3C 273, taken by different Hubble science instruments. The top panel is a Hubble Wide Field Planetary Camera 2 (WFPC2) image of quasar 3C 273. It looks like a bright white car headlight. There is a linear orange-white smoke-like feature stretching to the 4 o'clock position, an extragalactic jet launched from the quasar in the center of the black hole of an unseen galaxy. The bottom panel is a Hubble Space Telescope Imaging Spectrograph (STIS) coronagraph image of quasar 3C 273. It looks the same as the WFPC2 image, but in shades of blue. A black circle (labeled "core light blocked") blocks the glare of the quasar. Blue-colored filamentary material can be seen near the black hole. The extragalactic jet is still visible.

Astronomers have used the unique capabilities of NASA's Hubble Space Telescope to peer closer than ever into a huge and energetic black hole powering a quasar. A quasar is a galactic center that glows brightly as the black hole consumes material in its immediate surroundings.

The new Hubble views of the environment around the quasar show a lot of "weird things," according to Bin Ren of the Côte d'Azur Observatory and Université Côte d'Azur in Nice, France. "We've got a few blobs of different sizes, and a mysterious L-shaped filamentary structure. This is all within 16,000 light-years of the black hole."

Several of the objects could be small satellite galaxies around the black hole, and so they could offer the materials that will accrete onto the central super massive black hole, powering the bright lighthouse. "Thanks to Hubble's observing power, we're opening a new gateway into understanding quasars," said Ren. "My colleagues are excited because they've never seen this much detail before."

Quasars look starlike as point sources of light in the sky (hence the name quasi-stellar object). The quasar in the new study, 3C 273, was identified in 1963 by astronomer Maarten Schmidt as the first quasar. At a distance of 2.5 billion light-years it was too far away for a star. It must have been more energetic than ever imagined, with a luminosity over 10 times brighter than the brightest giant elliptical galaxies. This opened the door to an unexpected new puzzle in cosmology: What is powering this massive energy production? The likely culprit was material accreting onto a black hole.

In 1994 Hubble's new sharp view revealed that the environment surrounding quasars is far more complex than first suspected. The images suggested galactic collisions and mergers between quasars and companion galaxies, where debris cascades down onto supermassive black holes. This reignites the giant black holes that drive quasars.

For Hubble, staring into the quasar 3C 273 is like looking directly into a blinding car headlight and trying to see an ant crawling on the rim around it. The quasar pours out thousands of times the entire energy of stars in a galaxy. One of closest quasars to Earth, 3C 273 is 2.5 billion light-years away. (If it was very nearby, a few tens of light-years from Earth, it would appear as bright as the Sun in the sky!) Hubble's STIS instrument can serve as a coronagraph to block light from central sources, not unlike how the Moon block the Sun's glare during a total solar eclipse. Astronomers have used STIS to unveil dusty disks around stars to understand the formation of planetary systems, and now they can use STIS to better understand quasars’ host galaxies. The Hubble coronograph allowed astronomers to look eight times closer to the black hole than ever before.

Scientists got rare insight into the quasar's 300,000-light-year-long extragalactic jet of material blazing across space at nearly the speed of light. By comparing the STIS coronagraphic data with archival STIS images with a 22-year separation, the team led by Ren concluded that the jet is moving faster when it is farther away from the monster black hole.

"With the fine spatial structures and jet motion, Hubble bridged a gap between the small-scale radio interferometry and large-scale optical imaging observations, and thus we can take an observational step towards a more complete understanding of quasar host morphology. Our previous view was very limited, but Hubble is allowing us to understand the complicated quasar morphology and galactic interactions in detail.  In the future, looking further at 3C 273 in infrared light with the James Webb Space Telescope might give us more clues," said Ren.

At least 1 million quasars are scattered across the sky. They are useful background "spotlights" for a variety of astronomical observations. Quasars were most abundant about 3 billion years after the Big Bang, when galaxy collisions were more common.

The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and European Space Agency (ESA). NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute (STScI) in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.


Image Credit: NASA, European Space Agency (ESA), Bin Ren (Université Côte d’Azur/CNRS)
Acknowledgment: John Bahcall (IAS)
Image Processing: Joseph DePasquale/Space Telescope Science Institute (STScI)
Release Date: Dec. 5, 2024

#NASA #ESA #Astronomy #Space #Science #Hubble #BlackHoles #Galaxies #Galaxy #Quasar #3C273 #GalacticCenter #Virgo #Constellation #Astrophysics #Cosmos #Universe #HubbleSpaceTelescope #HST #STIS #GSFC #STScI #UnitedStates #Europe #Infographic #STEM #Education

NASA Espacio a Tierra | Seis minutos de serenidad: 27 de noviembre de 2024

NASA Espacio a Tierra | Seis minutos de serenidad: 27 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


Video Credit: National Aeronautics and Space Administration (NASA)
Duration: 6 minutes, 46 seconds
Release Date: Dec. 4, 2024

#NASA #Space #Science #ISS #Earth #NASAenespañol #español #EarthObservation #Astronauts #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #SpaceLaboratory #HumanSpaceflight #UnitedStates #Expedition72 #STEM #Education #HD #Video

Europe's Proba 3 Mission: Creating 'artificial eclipses' to study The Sun | ESA

Europe's Proba 3 Mission: Creating 'artificial eclipses' to study The Sun | ESA

The European Space Agency's Proba-3 is an ambitious mission that needs more than a single spacecraft to succeed. In order for Proba-3’s Coronagraph spacecraft to observe the Sun’s faint surrounding atmosphere, its disk-bearing Occulter spacecraft must block out the fiery solar disk. This means Proba-3’s Occulter ends up facing the Sun continuously, making it a valuable platform for science in its own right.

Europe's Proba-3 Mission lifted off on an Indian Space Research Organisation (ISRO) PSLV-XL rocket from the Satish Dhawan Space Center in Sriharikota, India, on Thursday, December 5, 2024, at 11:34 CET (10:34 GMT, 16:04 local time). ISRO placed both satellites (currently attached) into their designated orbit.

Proba-3 will maintain a fixed configuration as a ‘large rigid structure’ in a highly elliptical orbit to form an approximately 150-meter long solar coronagraph to study the Sun’s faint corona closer than ever before. Europe’s Proba-3 (Project for Onboard Anatomy) consists of two satellites—Coronagraph (310kg) and Occulter (240 kg). The pair must maintain a precise formation down to "a single millimeter" to study the corona, the sun’s outer atmosphere.


Video Credit: European Space Agency (ESA)
Duration: 9 minutes
Release Date: Dec. 3, 2024


#NASA #ESA #Space #Astronomy #Science #Star #Sun #Atmosphere #Corona #Satellites #Proba #Proba3 #Coronagraph #Occulter #Heliophysics #RocketLaunch #ISRO #NSIL #SDSC #Sriharikota #India #Europe #STEM #Education #HD #Video

European Proba-3 Solar Science Mission: Liftoff on ISRO PSLV-XL Rocket

European Proba-3 Solar Science Mission: Liftoff on ISRO PSLV-XL Rocket

The European Space Agency’s Proba-3 Mission lifted off on an ISRO PSLV-XL rocket from the Satish Dhawan Space Center in Sriharikota, India, on Thursday, December 5, 202, at 11:34 CET (10:34 GMT, 16:04 local time). The Indian Space Research Organisation (ISRO) placed both satellites (currently attached) into their designated orbit.

The European Space Agency (ESA) has successfully launched a pair of satellites, called Proba-3, that will maintain a fixed configuration as a ‘large rigid structure’ in a highly elliptical orbit to form an approximately 150-m long solar coronagraph to study the Sun’s faint corona closer than ever before. Europe’s Proba-3 (Project for Onboard Anatomy) consists of two satellites—Coronagraph (310kg) and Occulter (240 kg). The pair must maintain a precise formation down to "a single millimeter" to study the corona, the sun’s outer atmosphere.

“We are honoured that ESA entrusted NewSpace India Limited, NSIL, with its Proba-3 mission, and we are extremely satisfied to have delivered the satellites precisely into their designated orbit,” remarked Radhakrishnan Durairaj, Chairman and Managing Director of NSIL. “This is an extremely ambitious mission, with an ambitious orbit to go with it: the satellites have been placed into a highly elliptical orbit which extends more than 60,500 km from the surface of Earth. Reaching this orbit required the most powerful PSLV-XL variant of our launcher, equipped with additional propellant in its six solid rocket boosters.” 


Proba-3 Facts & Figures
Mass: Coronagraph spacecraft 340 kg; Occulter spacecraft 200 kg
Orbit: High Earth orbit, 19.7 hours orbital period, 60 530 km apogee, 600 km perigee
Instrument: External coronagraph
Ground station: Mission antenna will be at Santa Maria des Azores, and ground station at Redu, Belgium


Video Credit: ISRO - NSIL/European Space Agency (ESA)
Duration: 2 minutes, 35 seconds
Release Date: Dec. 5, 2024

#NASA #ESA #Space #Astronomy #Science #Star #Sun #Atmosphere #Corona #Satellites #Proba #Proba3 #Coronagraph #Occulter #Heliophysics #RocketLaunch #ISRO #ISROPSLVXLRocket #NSIL #RocketLiftoff #SDSC #Sriharikota #India #Europe #STEM #Education #HD #Video

Wednesday, December 04, 2024

Our Alien Earth: The Lava Fields of Holuhraun, Iceland | NASA Astrobiology

Our Alien Earth: The Lava Fields of Holuhraun, Iceland | NASA Astrobiology

Go off-road with Dr. Amanda Stockton of Georgia Tech and her team as they venture into the lava fields of a recently-erupted volcano, studying how quickly microbial life on Earth recovers from such a catastrophic event. Follow the expedition team as they use drones to map the field site, take samples of volcanic rock, and perform laboratory analyses; all mimicking the same exploration and science performed by the Mars Curiosity and Perseverance rovers.

Our Alien Earth

Follow NASA scientists into the field as they explore the most extreme environments on Earth, testing technologies that directly inform NASA missions to detect and discover extraterrestrial life in the universe.

Learn more about the NASA Astrobiology Program:

Video Credit: NASA Astrobiology
Duration: 20 minutes
Release Date: Dec. 4, 2024

#NASA #Astronomy #Space #Science #Astrobiology #SolarSystem #Planets #Planet #Earth #Geology #LavaFields #Holuhraun #Iceland #Ísland #ExtremeEnvironments #MarsAnalogs #Mars #CuriosityRover #MSL #PerseveranceRover #Mars2020 #MicrobialLife #Biosignatures #UnitedStates #STEM #Education #HD #Video

Planet Mars Images: December 2024 | NASA's Curiosity & Perseverance Rovers

Planet Mars Images: December 2024 | NASA's Curiosity & Perseverance Rovers

Mars 2020 - sol 1347
MSL - sol 4382
MSL - sol 4382
Mars 2020 - sol 1347
Mars 2020 - sol 1347

Celebrating 12+ Years on Mars (2012-2024)
Mission Name: Mars Science Laboratory (MSL)
Rover Name: Curiosity
Main Job: To determine if Mars was ever habitable to microbial life. 
Launch: Nov. 6, 2011
Landing Date: Aug. 5, 2012, Gale Crater, Mars

Celebrating 3+ Years on Mars
Mission Name: Mars 2020
Rover Name: Perseverance
Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.
Launch: July 30, 2020    
Landing: Feb. 18, 2021, Jezero Crater, Mars

For more information on NASA's Mars missions, visit: mars.nasa.gov

Image Credits: NASA/JPL-Caltech/ASU/MSSS
Processing: Kevin M. Gill
Image Release Date: Dec. 3-4, 2024

#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #CuriosityRover #MSL #MountSharp #GaleCrater #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #JPL #Caltech #UnitedStates #CitizenScience #KevinGill #STEM #Education

Star Trails: "Techno-cool" Space Art | International Space Station

Star Trails: "Techno-cool" Space Art | International Space Station

NASA Astronaut & Expedition 72 Flight Engineer Don Pettit: "Star trail from ISS; I think these are a blend of both science and art. There is so much techno-geek stuff to see, or you can simply sit back and think “How cool” . . . This one shows atmospheric airglow, yellow-green at 120km and the fainter upper red at 400km, star trails moving in arcs on the left and straight lines on the right, Starlink satellites flashing sunlight off their solar panel, the Cygnus cargo vehicle (left), my Soyuz vehicle (center), and the Russian laboratory module MLM (right)."

"So full of techno-cool and art-cool."


Expedition 72 Crew
Station Commander: Suni Williams
Roscosmos (Russia): Alexey Ovchinin, Ivan Vagner, Aleksandr Gorbunov
NASA: Butch Wilmore, Don Pettit, Nick Hague

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 (JSC)
Release Date: Dec. 3, 2024


#NASA #Space #Science #ISS #Stars #Earth #Airglow #Satellites #Astronauts #DonPettit #SpaceArt #AstronautPhotography #StarTrails #Timelapse #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #HumanSpaceflight #SpaceLaboratory #UnitedStates #Expedition72 #STEM #Education

Falling Material Kicks Up Dust Cloud on Dunes | NASA MRO

Falling Material Kicks Up Dust Cloud on Dunes | NASA MRO

There is a vast region of sand dunes at high northern latitudes on Mars. In the winter, a layer of carbon dioxide ice covers the dunes, and in the spring as the sun warms the ice it evaporates. This is a very active process, and sand dislodged from the crests of the dunes cascades down, forming dark streaks.

In this image, falling material has kicked up a small cloud of dust. The color of the ice surrounding adjacent streaks of material suggests that dust has settled on the ice at the bottom after similar events.

Also discernible in this subimage are polygonal cracks in the ice on the dunes (the cracks disappear when the ice is gone).

Image cutout is less than 1 km (under a mile) across and the spacecraft altitude was 320 km (199 mi). 

Image Location:
Latitude (centered)
83.506°
Longitude (East)
118.588°

The High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter captured this image.

Mars Reconnaissance Orbiter (MRO) is a spacecraft designed to study the geology and climate of Mars, to provide reconnaissance of future landing sites, and to relay data from surface missions back to Earth. It was launched on August 12, 2005, and reached Mars on March 10, 2006. 

The Jet Propulsion Laboratory (JPL) manages MRO for NASA’s Science Mission Directorate in Washington. Caltech, in Pasadena, manages JPL for NASA. The University of Arizona, in Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., in Boulder, Colorado. The Context Camera was built by, and is operated by, Malin Space Science Systems in San Diego.

For more information on MRO, visit:

Image Credit: NASA/JPL-Caltech/University of Arizona
Caption Credit: Candy Hansen
Image Date: April 7, 2008
Release Date: Dec. 4, 2024


#NASA #Space #Astronomy #Science #Mars #Planet #RedPlanet #Geology #Landscape #Terrain #NorthernLatitudes #SandDunes #CarbonDioxideIce #DarkStreaks #Sand #Geoscience #MRO #MarsOrbiter #MarsSpacecraft #HiRISECamera #JPL #Caltech #BallAerospace #MSSS #UnitedStates #STEM #Education

The Spiderweb Galaxy Protocluster in Hydra | James Webb Space Telescope

The Spiderweb Galaxy Protocluster in Hydra | James Webb Space Telescope

This image shows the Spiderweb protocluster as seen by Webb’s Near-InfraRed Camera (NIRCam).
This annotated image shows the galaxy distribution in the Spiderweb protocluster as seen by Webb’s Near-InfraRed Camera (NIRCam). The galaxies are annotated by white circles, and the collection of gravitationally-bound galaxies is identified in the centre of the image. A selection of these galaxies are featured as individual close-ups at the bottom of the image.
This annotated image shows the galaxy distribution in the Spiderweb protocluster as seen by Webb’s NIRCam (Near-InfraRed Camera). The galaxies are annotated by white circles, and the collection of gravitationally-bound galaxies is identified in the centre of the image.

Using the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope, an international team of astronomers have found new galaxies in the Spiderweb protocluster. Their characteristics shed light on the growth of galaxies in these large cosmic 'cities' with the finding that gravitational interactions in these dense regions are not as important as previously thought.

With the use of Webb’s capabilities, astronomers have now sought to better understand this protocluster and to reveal new galaxies within it. Infrared radiation passes more freely through cosmic dust than visible light, which is scattered by the dust. Because Webb can see infrared light very well, scientists used it to observe regions of the Spiderweb that were previously hidden to us by cosmic dust, and to find out to what degree this dust obscures them.

This image shows the Spiderweb protocluster as seen by Webb’s NIRCam (Near-InfraRed Camera).

Image Description: Hundreds of galaxies appear in this view. It is set against the black background of space. There are many overlapping objects at various distances. They include large, blue foreground stars, a number with eight diffraction spikes, plus white and pink spiral and elliptical galaxies are visible. Numerous tiny orange dots appear throughout the scene.


Credit: ESA/Webb, NASA & CSA, H. Dannerbauer
Release Date: Dec. 4, 2024

#NASA #ESA #Astronomy #Space #Science #Galaxies #GalaxyClusters #SpiderwebProtocluster #Hydra #Constellation #Cosmos #Universe #JWST #NIRCam #InfraredAstronomy #WebbSpaceTelescope #GSFC #STScI #CSA #Canada #ESA #Europe #UnitedStates #STEM #Education

Cosmic Wonders of The Hubble Space Telescope

Cosmic Wonders Hubble Space Telescope

Cosmic Wonders presents a series of 18 astronomy visualizations. Each sequence combines Hubble Space Telescope images or research computer simulations with scientific knowledge and insight to create three dimensional visions of celestial sights.

These visualizations were produced by astronomers and artists at the Space Telescope Science Institute.


Credits: Video: NASA, ESA, Space Telescope Science Institute (STScI), Editor: Danielle Kirshenblat (STScI); Visualization: Greg Bacon (STScI), Frank Summers (STScI), Joseph DePasquale (STScI), Leah Hustak (STScI), Joseph Olmsted (STScI), Alyssa Pagan (STScI), Tiffany Borders-Davis (STScI), Lisa Frattare (STScI), Zolt G. Levay (STScI), Dani Player (STScI)
Duration: 2 minutes, 37 seconds
Release Date: Dec. 3, 2024


Video Credit: Space Telescope Science Institute (STScI)
Duration: 2 minutes, 37 seconds
Release Date: Dec. 3, 2024  


#NASA #Hubble #Astronomy #Space #Science #Stars #Supernovae #StarClusters #Nebulae #Galaxies #InteractingGalaxies #Cosmos #Universe #HubbleSpaceTelescope #HST #ESA #Europe #GSFC #STScI #UnitedStates #SpaceExploration #STEM #Education #Art #Visualizations #HD #Video

Fly over Ares Vallis on Mars: Animation | European Space Agency's Mars Express

Fly over Ares Vallis on Mars: Animation | European Space Agency's Mars Express

Explore the immense power of water as the European Space Agency’s Mars Express takes us on a flight over curving channels, streamlined islands and muddled ‘chaotic terrain’ on Mars, soaking up rover landing sites along the way.

This flight around the Oxia Palus region of Mars covers a total area of approximately 890 000 km², more than twice the size of Germany. Central to the tour is one of Mars’ largest outflow channels, Ares Vallis. It stretches for more than 1,700 km and cascades down from the planet’s southern highlands to enter the lower-lying plains of Chryse Planitia.

Billions of years ago, water surged through Ares Vallis, neighboring Tiu Vallis, and numerous other smaller channels, creating many of the features observed in this region today.

After a global view of Mars, we focus in on the area marked by the white rectangle. Our flight starts over the landing site of NASA’s Pathfinder mission, whose Sojourner rover explored the floodplains of Ares Vallis for 12 weeks in 1997.

Continuing to the south, we pass over two large craters named Masursky and Sagan. The partially eroded crater rim of Masursky in particular suggests that water once flowed through it, from nearby Tiu Vallis.

The Masurky Crater is filled with jumbled blocks, and you can see many more as we turn north to Hydaspis Chaos. This ‘chaotic terrain’ is typical of regions influenced by massive outflow channels. Its distinctive muddled appearance is thought to arise when subsurface water is suddenly released from underground to the surface. The resulting loss of support from below causes the surface to slump and break into blocks of various sizes and shapes.

Just beyond this chaotic array of blocks is Galilaei crater, which has a highly eroded rim and a gorge carved between the crater and neighbouring channel. It is likely that the crater once contained a lake. This flooded out into the surroundings. Continuing on, we see streamlined islands and terraced river banks, the teardrop-shaped island ‘tails’ pointing in the downstream direction of the water flow at the time.

Crossing over Ares Vallis again, the flight brings us to the smoother terrain of Oxia Planum and the planned landing site for the European Space Agency's ExoMars Rosalind Franklin rover. The primary goal of the mission is to search for signs of past or present life on Mars. This once water-flooded region is an ideal location.

Zooming out, the flight ends with a bird’s-eye view of Ares Vallis and its water-enriched neighborhood. 

Disclaimer: This video is not representative of how Mars Express flies over the surface of Mars. 
See processing notes below.

How the animation was made

This video was created using the Mars Express High Resolution Stereo Camera Mars Chart (HMC30) data, an image mosaic made from single orbit observations of the High Resolution Stereo Camera (HRSC). The mosaic, centered at 12°N/330°E, is combined with topography information from the digital terrain model to generate a three-dimensional landscape. 

For every second of the animation, 50 separate frames are rendered following a predefined camera path in the scene. A three-fold vertical exaggeration has been applied. Atmospheric effects such as clouds and haze have been added to conceal the limits of the terrain model. The haze starts building up at a distance of 300 km. 

The HRSC camera on Mars Express is operated by the German Aerospace Center (DLR). The systematic processing of the camera data took place at the DLR Institute for Planetary Research in Berlin-Adlershof. The working group of Planetary Science and Remote Sensing at Freie Universität Berlin used the data to create the film.

Learn more about the European Space Agency's Mars Express:


Video Credits: 
Images: ESA/DLR/FU Berlin/NASA/MSSS, CC BY-SA 3.0 IGO
Data Processing/Animation: Björn Schreiner, Image Processing Group (FU Berlin)
Duration: 4 minutes, 37 seconds
Release Date: Nov. 20, 2024

#NASA #ESA #Space #Astronomy #Science #Planet #Mars #FlyOver #AresVallis #OxiaPalus #Geology #MarsExpress #MarsExpressSpacecraft #HRSC #Europe #DLR #FUBerlin #Berlin #Germany #Deutschland #STEM #Education #Animation #Visualization #HD #Video

Tuesday, December 03, 2024

Views of The Milky Way & Magellanic Cloud Galaxies | International Space Station

Views of The Milky Way & Magellanic Cloud Galaxies | International Space Station

This long-duration photograph looks out a window on the SpaceX Dragon crew spacecraft to the Milky Way as the International Space Station orbited 262 miles above the Pacific Ocean northeast of New Zealand.
The Milky Way appears in the vastness of space behind the SpaceX Dragon crew spacecraft docked to the Harmony module's space-facing port on the International Space Station. NASA astronaut and Expedition 71 Flight Engineer Matt Dominick can be seen peering out of the left window on Dragon while soaring 254 miles above the Pacific Ocean.
This long-duration photograph looks out a window on the SpaceX Dragon crew spacecraft to the Large and Small Magellanic Clouds, two irregular dwarf galaxies, as the International Space Station orbited 260 miles above the Pacific Ocean off the coast of Mexico.

This long-duration photograph looks out a window on the SpaceX Dragon crew spacecraft to the Large and Small Magellanic Clouds, two irregular dwarf galaxies, as the International Space Station orbited 260 miles above the Pacific Ocean northeast of Australia.

Nearly 200,000 light-years from Earth, the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way, floats in space, in a long and slow dance around our galaxy. The Small Magellanic Cloud (SMC) is one of the Milky Way’s closest galactic neighbors. Even though it is a small, or so-called dwarf galaxy, the SMC is so bright that it is visible to the unaided eye from the Southern Hemisphere and near the equator. Many navigators, including Ferdinand Magellan who lends his name to the SMC, used it to help find their way across the oceans. Modern astronomers are also interested in studying the SMC (and its cousin, the Large Magellanic Cloud), but for very different reasons. Because the SMC is so close and bright, it offers an opportunity to study phenomena that are difficult to examine in more distant galaxies.

Expedition 72 Updates:

Expedition 72 Crew
Station Commander: Suni Williams
Roscosmos (Russia): Alexey Ovchinin, Ivan Vagner, Aleksandr Gorbunov
NASA: Butch Wilmore, Don Pettit, Nick Hague

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 Credits: NASA's Johnson Space Center/Don Pettit
Image Dates: June 29-Nov. 28, 2024
Release Date: Dec. 2, 2024

#NASA #Space #Science #ISS #SpaceXCrewDragon #Earth #Galaxies #MilkyWayGalaxy #MagellanicCloudGalaxies #LMC #SMC #Astronauts #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #SpaceLaboratory #HumanSpaceflight #UnitedStates #Expedition71 #Expedition72 #STEM #Education