Mars is Mighty: First Observations | James Webb Space Telescope

Mars is Mighty: First Observations | James Webb Space Telescope

The James Webb Space Telescope captured its first images and spectra of Mars on September 5, 2022. The telescope, an international collaboration between NASA, the European Space Agency and the Canadian Space Agency, provides a unique perspective with its infrared sensitivity on our neighboring planet, complementing data being collected by orbiters, rovers, and other telescopes.

Webb’s unique observation post nearly 1.5 million kilometers away at the Sun-Earth Lagrange point 2 (L2) provides a view of Mars’ observable disk (the portion of the sunlit side that is facing the telescope). As a result, Webb can capture images and spectra with the spectral resolution needed to study short-term phenomena like dust storms, weather patterns, seasonal changes, and, in a single observation, processes that occur at different times (daytime, sunset, and nighttime) of a Martian day.

Because it is so close, the Red Planet is one of the brightest objects in the night sky in terms of both visible light (which human eyes can see) and the infrared light that Webb is designed to detect. This poses special challenges to the observatory, which was built to detect the extremely faint light of the most distant galaxies in the universe. Webb’s instruments are so sensitive that without special observing techniques, the bright infrared light from Mars is blinding, causing a phenomenon known as “detector saturation.” Astronomers adjusted for Mars’ extreme brightness by using very short exposures, measuring only some of the light that hit the detectors, and applying special data analysis techniques.

Webb’s first images of Mars, captured by the Near-Infrared Camera (NIRCam), show a region of the planet’s eastern hemisphere at two different wavelengths, or colors of infrared light. This image shows a surface reference map from NASA and the Mars Orbiter Laser Altimeter (MOLA) on the left, with the two Webb NIRCam instrument field of views overlaid. The near-infrared images from Webb are shown on the right.

The NIRCam shorter-wavelength (2.1 microns) image [top right] is dominated by reflected sunlight, and thus reveals surface details similar to those apparent in visible-light images [left]. The rings of the Huygens Crater, the dark volcanic rock of Syrtis Major, and brightening in the Hellas Basin are all apparent in this image.

The NIRCam longer-wavelength (4.3 microns) image [lower right] shows thermal emission—light given off by the planet as it loses heat. The brightness of 4.3-micron light is related to the temperature of the surface and the atmosphere. The brightest region on the planet is where the Sun is nearly overhead, because it is generally warmest. The brightness decreases toward the polar regions, which receive less sunlight, and less light is emitted from the cooler northern hemisphere, which is experiencing winter at this time of year.

However, temperature is not the only factor affecting the amount of 4.3-micron light reaching Webb with this filter. As light emitted by the planet passes through Mars’ atmosphere, some gets absorbed by carbon dioxide (CO2) molecules. The Hellas Basin—which is the largest well-preserved impact structure on Mars, spanning more than 2,000 kilometers—appears darker than the surroundings because of this effect.

In the future, Webb will be using this imaging and spectroscopic data to explore regional differences across the planet, and to search for trace species in the atmosphere, including methane and hydrogen chloride.

These observations of Mars were conducted as part of Webb’s Cycle 1 Guaranteed Time Observation (GTO) Solar System program led by Heidi Hammel of the Association of Universities for Research in Astronomy (AURA).

The  European Space Agency (ESA) operates two Mars orbiters, Mars Express and the ExoMars Trace Gas Orbiter, that have brought a treasury of insight into the Red Planet’s atmosphere and surface. Furthermore, ESA collaborates with the Japanese Aerospace Exploration Agency (JAXA) on the Martian Moons eXploration (MMX) mission, soon to launch for Mars’ moon Phobos.

Note: This post highlights images from Webb science in progress, which has not yet been through the peer-review process.

Credit: NASA, European Space Agency (ESA), Canadian Space Agency (CSA), Space Telescope Science Institute (STScI), Mars JWST/GTO team

Release Date: September 19, 2022

#NASA #ESA #Astronomy #Space #Science #Mars #Planet #RedPlanet #HuygensCrater #SyrtisMajor #HellasBasin #NIRCam #Infrared #JamesWebb #WebbTelescope #JWST #SpaceTelescope #SolarSystem #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #STEM #Education

Bright Night Lights of London | International Space Station

Bright Night Lights of London | International Space Station

European Space Agency Astronaut Samantha Cristoforetti of Italy:

"Lights shine bright in London at night . . . My thoughts are with the family and all those who bid farewell to Her Majesty Queen Elizabeth II today." 

Learn about Samantha's Minerva Mission: https://bit.ly/MissionMinerva

Expedition 67 Crew

Commander Oleg Artemyev (Russia)

Roscosmos Flight Engineers: Denis Matveev and Sergey Korsakov (Russia)

NASA Flight Engineers: Kjell Lindgren, Bob Hines, Jessica Watkins (USA)

European Space Agency (ESA) Flight Engineer: Samantha Cristoforetti (Italy)

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. The ISS has been the most politically complex space exploration program ever undertaken.

Learn more about the important research being operated on ISS: https://www.nasa.gov/iss-science

Credit: ESA/NASA-S.Cristoforetti

Release Date: September 19, 2022

#NASA #Space #ISS #ESA #UnitedKingdom #QueenElizabethII #Funeral #London #City #Night #Astronaut #FlightEngineer #SamanthaCristoforetti #Minerva #MissionMinerva #Italy #Italia #Science #Technology #HumanSpaceflight #Expedition67 #Europe #UnitedStates #Russia #Россия #Japan #日本 #International #STEM #Education

Scarp Dune Blues at North Pole of Mars | NASA's Mars Reconnaissance Orbiter

Scarp Dune Blues at North Pole of Mars | NASA's Mars Reconnaissance Orbiter

This enhanced color image (using the red-green-blue filter) shows a group of lovely barchan dunes along a scarp (cliff) in Chasma Boreale in the North Pole of Mars. A barchan or barkhan dune is a crescent-shaped dune. Our primary goal is to track for seasonal changes over time.

These dunes were captured by NASA's Mars Reconnaissance Orbiter (MRO) using the High Resolution Imaging Science Experiment (HiRISE) instrument. MRO has orbited the Red Planet since 2006.

Image cutout is less than 1 km (under a mile) across and the spacecraft altitude was 197 km.

Malin Space Science Systems built the Mars Color Imager (MARCI), Context Camera (CTX) systems for MRO.

The University of Arizona, Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., Boulder, Colorado. 

NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington.

Credit: NASA/JPL-Caltech/University of Arizona

Release Date: September 6, 2022

#NASA #Space #Astronomy #Mars #Planet #RedPlanet #Science #Geology #Landscape #Terrain #Geoscience #NorthPole #ChasmaBoreale #BarchanDunes #Dunes #MRO #Orbiter #Spacecraft #HiRISE #Camera #JPL #Caltech #UniversityOfArizona #BallAerospace #MSSS #STEM #Education

Soyuz MS-21 Crew Spacecraft over the Caribbean Sea | International Space Station

Soyuz MS-21 Crew Spacecraft over the Caribbean Sea | International Space Station

The Soyuz MS-21 crew ship is pictured attached to the Prichal docking module as the International Space Station orbited 259 miles above the Caribbean Sea in between the island nations of Grenada and Trinidad and Tobago.

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. The ISS has been the most politically complex space exploration program ever undertaken.

Learn more about the important research being operated on the International Space Station:

https://www.nasa.gov/iss-science 

For more information about STEM on Station:

https://www.nasa.gov/stemonstation

Science, Technology, Engineering, Math (STEM) Education

Credit: NASA's Johnson Space Center (JSC)

Image Date: Sept. 15, 2022

#NASA #Space #ISS #Earth #Roscosmos #Cosmonauts #Soyuz #Союз #SoyuzMS21 #Spacecraft #Роскосмос #Russia #Россия #JSC #Houston #Texas #UnitedStates #Grenada #Trinidad #Tobago #Caribbean #CaribbeanSea #AtlanticOcean #Expedition67 #InternationalCooperation #UNOOSA #STEM #Education

An Enigmatic Astronomical Explosion | Hubble

An Enigmatic Astronomical Explosion | Hubble

A bright young star is surrounded by a shroud of thick gas and dust in this image from the NASA/European Space Agency Hubble Space Telescope. Hubble’s Wide Field Camera 3 inspected a young stellar object, over 9,000 light years away in the constellation Taurus, to help astronomers understand the earliest stages in the lives of massive stars. This object—which is known to astronomers as IRAS 05506+2414—is thought to be an example of an explosive event caused by the disruption of a massive young star system. If so, it would only be the second such example known.

Usually the swirling discs of material surrounding a young star are funnelled into twin outflows of gas and dust from the star. In the case of IRAS 05506+2414, however, a fan-like spray of material traveling at velocities of up to 350 kilometers per second is spreading outwards from the center of this image.

Astronomers turned to Hubble’s Wide Field Camera 3 to measure the distance to IRAS 05506+2414. While it is possible to measure the velocity of material speeding outwards from the star, astronomers cannot tell how far from Earth the star actually is from a single observation. However, by measuring the distance that the outflow travels between successive images, they will be able to infer the distance to IRAS 05506+2414. This will allow astronomers to determine how bright the star is and how much energy it is emitting, and hence to estimate its mass—all vital information that will help to understand the origin of this bright young star’s unusual outflow.

Credit: European Space Agency (ESA)/Hubble & NASA, R. Sahai

Release Date: September 19, 2022

#NASA #ESA #Astronomy #Space #Science #Hubble #Star #IRAS055062414 #Taurus #Constellation #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #STEM #Education

SpaceX Starlink Mission: Sept. 18, 2022 | Cape Canaveral Space Force Station

SpaceX Starlink Mission: Sept. 18, 2022 | Cape Canaveral Space Force Station

On Sunday, September 18, 2022, at 8:18 p.m. ET, SpaceX launched 54 Starlink satellites to orbit from Space Launch Complex 40 (SLC-40) at Cape Canaveral Space Force Station in Florida.

This was the sixth launch and landing of this Falcon 9 first stage booster, which previously launched CRS-22, Crew-3, Turksat 5B, Crew-4, CRS-25, and now one Starlink mission.

Credit: Space Exploration Technologies Corp. (SpaceX)

Capture Date: September 18, 2022

#NASA #Space #Earth #Orbit #LEO #SpaceX #Falcon9 #Rocket #Satellites #Starlink #Broadband #Internet #ElonMusk #GwynneShotwell #Spaceflight #Technology #Engineering #CommercialSpace #Spaceport #CapeCanaveral #SpaceForce #Florida #UnitedStates #STEM #Education

A Globular Cluster’s Striking Red Eye: NGC 2108 | Hubble

A Globular Cluster’s Striking Red Eye: NGC 2108 | Hubble

This image shows the colorful globular cluster NGC 2108. The cluster is nestled within the Large Magellanic Cloud, in the constellation of the Swordfish (Dorado). It was discovered in 1835 by the astronomer, mathematician, chemist and inventor John Herschel, son of the famous William Herschel.

The most striking feature of this globular cluster is the gleaming ruby-red spot at the center left of the cluster. What looks like the cluster’s watchful eye is actually a carbon star. Carbon stars are almost always cool red giants, with atmospheres containing more carbon than oxygen—the opposite to our Sun. Carbon monoxide forms in the outer layer of the star through a combination of these elements, until there is no more oxygen available. Carbon atoms are then free to form a variety of other carbon compounds, such as C2, CH, CN, C3 and SiC2, which scatter blue light within the star, allowing red light to pass through undisturbed.

This image was captured by the NASA/ESA Hubble Space Telescope’s Advanced Camera for Surveys (ACS), using three different filters.

Credit: European Space Agency (ESA)/Hubble & NASA

Release Date: August 6, 2018

#NASA #ESA #Astronomy #Space #Science #Hubble #CarbonStar #StarCluster #GlobularCluster #NGC2108 #Dorado #Constellation #LMC #Galaxy #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #Astronomer #JohnHerschel #History #STEM #Education

A Great Ball of Stars: NGC 1806 | Hubble

A Great Ball of Stars: NGC 1806 | Hubble

The NASA/European Space Agency Hubble Space Telescope has turned its sharp eye towards a tight collection of stars, first seen 174 years ago. The result is a sparkling image of NGC 1806, tens of thousands of stars gravitationally bound into a rich cluster. Commonly called globular clusters, most of these objects are very old, having formed in the distant past when the Universe was only a fraction of its current age. NGC 1806 lies within the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. It can be observed within the constellation of Dorado (the dolphin-fish), an area of the sky best seen from the Earth’s southern hemisphere.

NGC 1806 was discovered in 1836 by the British astronomer John Herschel. He had travelled to South Africa in order to catalog astronomical objects visible best from southern latitudes, and thereby complete work begun by his father William, the man who coined the term “globular cluster”. Using a large telescope John Herschel carefully scanned the night sky and noted objects of interest, of which NGC 1806 was one. In the same year that he documented NGC 1806 he was visited by the naturalist Charles Darwin after the HMS Beagle stopped over in Cape Town. Darwin later referred to John Herschel as “one of our greatest philosophers”.

The Wide Field Channel of Hubble's Advanced Camera for Surveys was used to obtain this picture that was created from images taken through blue (F435W, colored blue), yellow (F555W, colored green) and near-infrared (F814W, colored red) filters. The exposure times were 770 s, 720 s and 688 s, respectively, and the field of view is  3.1 by 1.9 arcminutes. Surely Herschel, who made great contributions to the sciences of both astronomy and photography, would have been immensely impressed by this glittering Hubble picture.

Credit: European Space Agency (ESA)/Hubble & NASA

Release Date: October 25, 2010

#NASA #ESA #Astronomy #Space #Science #Hubble #StarCluster #GlobularCluster #NGC1806 #Dorado #Constellation #LMC #Galaxy #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #Astronomer #JohnHerschel #History #STEM #Education

Different Generations Standing Together: Star Cluster NGC 1866 | Hubble

Different Generations Standing Together: Star Cluster NGC 1866 | Hubble

Star clusters are common structures throughout the Universe, each made up of hundreds of thousands of stars all bound together by gravity. This star-filled image, taken with the NASA/European Space Agency Hubble Space Telescope’s Wide Field Camera 3 (WFC3), shows one of them: NGC 1866.

NGC 1866 is found at the very edges of the Large Magellanic Cloud, a small galaxy located near to the Milky Way. The cluster was discovered in 1826 by Scottish astronomer James Dunlop, who catalogued thousands of stars and deep-sky objects during his career.

However, NGC 1866 is no ordinary cluster. It is a surprisingly young globular cluster situated close enough to us that its stars can be studied individually—no mean feat given the mammoth distances involved in studying the cosmos! There is still debate over how globular clusters form, but observations such as this have revealed that most of their stars are old and have a low metallicity. In astronomy, ‘metals’ are any elements other than hydrogen and helium; since stars form heavier elements within their core as they carry out nuclear fusion throughout their lifetimes, a low metallicity indicates that a star is very old, as the material from which it formed was not enriched with many heavy elements. It is possible that the stars within globular clusters are so old that they were actually some of the very first to form after the Big Bang.

In the case of NGC 1866, though, not all stars are the same. Different populations, or generations, of stars are thought to coexist within the cluster. Once the first generation of stars formed, the cluster may have encountered a giant gas cloud that sparked a new wave of star formation and gave rise to a second, younger, generation of stars—explaining why it seems surprisingly youthful.

Credit: European Space Agency (ESA)/Hubble & NASA

Release Date: November 19, 2018

#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #GlobularStarCluster #StarCluster #NGC1866 #Dorado #Constellation #LMC #Galaxy #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #History #STEM #Education

Pan across a Scattering of Stars: Open Star Cluster NGC 330 | Hubble

Pan across a Scattering of Stars: Open Star Cluster NGC 330 | Hubble

This video showcases the open star cluster NGC 330, which lies around 180,000 light-years away inside the Small Magellanic Cloud. The cluster—which is in the constellation Tucana (The Toucan)—contains a multitude of stars, many of which are scattered across this striking image.

Credit: ESA/Hubble & NASA, J. Kalirai, A. Milone  

Duration: 30 seconds

Release Date: July 25, 2021

#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #OpenStarCluster #StarClusters #NGC330 #GALFOR1 #Tucana #Constellation #LMC #Galaxy #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #STEM #Education #HD #Video

A Scattering of Stars: Open Star Cluster NGC 330 | Hubble

A Scattering of Stars: Open Star Cluster NGC 330 | Hubble

This image depicts the open star cluster NGC 330, which lies around 180,000 light-years away inside the Small Magellanic Cloud. The cluster—which is in the constellation Tucana (The Toucan)—contains a multitude of stars, many of which are scattered across this striking image.

The most stunning object in this image is actually the very small star cluster in the lower left corner of the image, surrounded by a nebula of ionized hydrogen (red) and dust (blue). Named GALFOR 1, the cluster was discovered in 2018 in Hubble's archival data, which was used to create this latest image from Hubble. To better understand this star cluster, specifically whether the nebula surrounding the cluster also contains a bow shock, scientists will need high resolution infrared imagery from the upcoming NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope.

This image also contains clues about the inner workings of Hubble itself. The criss-cross patterns surrounding the stars in this image—known as diffraction spikes—were created when starlight interacted with the four thin vanes supporting Hubble’s secondary mirror.

As star clusters form from a single primordial cloud of gas and dust, all the stars they contain are roughly the same age. This makes them useful natural laboratories for astronomers to learn how stars form and evolve. This image uses observations from Hubble’s Wide Field Camera 3, and incorporates data from two very different astronomical investigations. The first aimed to understand why stars in star clusters appear to evolve differently from stars elsewhere, a peculiarity first observed by the Hubble Space Telescope. The second aimed to determine how large stars can be before they become doomed to end their lives in cataclysmic supernova explosions.

Credit: European Space Agency (ESA)/Hubble & NASA, J. Kalirai, A. Milone

Release Date: June 28, 2021

#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #OpenStarCluster #StarClusters #NGC330 #GALFOR1 #Tucana #Constellation #LMC #Galaxy #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #STEM #Education

A Pocketful of Stars: Globular Cluster NGC 1805 | Hubble

A Pocketful of Stars: Globular Cluster NGC 1805 | Hubble

Many colorful stars are packed close together in this image of the globular cluster NGC 1805, taken by the NASA/European Space Agency Hubble Space Telescope. This tight grouping of thousands of stars is located near the edge of the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. The stars orbit closely to one another, like bees swarming around a hive. In the dense center of one of these clusters, stars are 100 to 1000 times closer together than the nearest stars are to our Sun, making planetary systems around them unlikely.

The striking difference in star colors is illustrated beautifully in this image, which combines two different types of light: blue stars, shining brightest in near-ultraviolet light, and red stars, illuminated in red and near-infrared. Space telescopes like Hubble can observe in the ultraviolet because they are positioned above Earth’s atmosphere, which absorbs most of this wavelength, making it inaccessible to ground-based facilities.

This young globular cluster can be seen from the southern hemisphere, in the Dorado constellation, which is Portugese for dolphinfish. Usually, globular clusters contain stars which are born at the same time. However, NGC 1805 is unusual as it appears to host two different populations of stars with ages millions of years apart. Observing such clusters of stars can help astronomers understand how stars evolve, and what factors determine whether they end their lives as white dwarfs, or explode as supernovae.

Credit: European Space Agency (ESA)/Hubble & NASA, J. Kalirai

Release Date: September 7, 2020

#NASA #ESA #Astronomy #Space #Science #Hubble #Ultraviolet #Infrared #Stars #GlobularCluster #NGC1805 #Dorado #Constellation #LMC #Galaxy #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #STEM #Education

Faint Afterglow of Nearby Stellar Explosion: Supernova Remnant N132D | Hubble

Faint Afterglow of Nearby Stellar Explosion: Supernova Remnant N132D | Hubble

Intricate wisps of glowing gas float amid a myriad of stars in this image created by combining data from the NASA/European Space Agency Hubble Space Telescope and Chandra X-ray Observatory. The gas is a supernova remnant, cataloged as N132D, ejected from the explosion of a massive star that occurred some 3,000 years ago. This titanic explosion took place in the Large Magellanic Cloud, a nearby neighbor galaxy of our own Milky Way.

Distance: 170,000 light years

Credit: NASA, European Space Agency (ESA), and The Hubble Heritage Team STScI/AURA

Release Date: October 4, 2005

#NASA #ESA #Astronomy #Space #Science #Hubble #Chandra #Observatory #Xray #Star #Supernova #SupernovaRemnant #Nebula #N132D #Dorado #Constellation #LMC #Galaxy #Cosmos #Universe #SpaceTelescopes #STScI #GSFC #UnitedStates #Europe #STEM #Education

A Vapor of Stars: Galaxy DDO 82 | Hubble

A Vapor of Stars: Galaxy DDO 82 | Hubble

Relatively few galaxies possess the sweeping, luminous spiral arms or brightly glowing center of our home galaxy the Milky Way. In fact, most of the Universe's galaxies look like small, amorphous clouds of vapor. One of these galaxies is DDO 82, captured here in an image from the NASA/European Space Agency Hubble Space Telescope. Though tiny compared to the Milky Way, such dwarf galaxies still contain between a few million and a few billion stars.

DDO 82, also known by the designation UGC 5692, is not without a hint of structure, however. Astronomers classify it as an Sm galaxy, or Magellanic spiral galaxy, named after the Large Magellanic Cloud, a dwarf galaxy that orbits the Milky Way. That galaxy, like DDO 82, is said to have one spiral arm.

In the case of DDO 82, gravitational interactions over its history seem to have discombobulated it so that this structure is not as evident as in the Large Magellanic Cloud. Accordingly, astronomers also refer to DDO 82 and others of a similar unshapely nature as dwarf irregular galaxies.       

DDO 82 can be found in the constellation of Ursa Major (the Great Bear) approximately 13 million light-years away. The object is considered part of the M81 Group of around three dozen galaxies. DDO 82 gets its name from its entry number in the David Dunlap Observatory Catalogue. Canadian astronomer Sidney van den Bergh originally compiled this list of dwarf galaxies in 1959.

The image is made up of exposures taken in visible and infrared light by Hubble’s Advanced Camera for Surveys. The field of view is approximately 3.3 by 3.3 arcminutes.

Credit: European Space Agency (ESA)/Hubble & NASA

Distance: 13 million light years

Release Date: June 25, 2012

#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #Galaxy #DDO82 #UGC5692 #SmGalaxy #MagellanicSpiralGalaxy #UrsaMajor #Constellation #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #DavidDunlapObservatory #Canada #History #STEM #Education

NASA Astronaut Frank Rubio Prepares for Russian Soyuz Rocket Launch

NASA Astronaut Frank Rubio Prepares for Russian Soyuz Rocket Launch

U.S. astronaut Frank Rubio prepares for launch to the International Space Station on a Russian Soyuz rocket. Expedition 68 astronaut Frank Rubio of NASA, and cosmonauts Sergey Prokopyev and Dmitri Petelin of Roscosmos are scheduled to launch aboard their Soyuz MS-22 spacecraft on Sept. 21, 2022. In this image, Frank Rubio performs preflight checkouts in the Soyuz MS-22 spacecraft at the Baikonur Cosmodrome in Kazakhstan. Rubio is scheduled for a six-month mission on the International Space Station.

A Soyuz rocket was raised to vertical after having rolled out by train to the launch pad, Sunday, Sept. 18, at site 31 of the Baikonur Cosmodrome in Kazakhstan. 

Launch coverage will begin at 9 a.m. on NASA Television’s Public Channel, the NASA app, and on the agency’s website. 

Watch the Soyuz MS-22 launch online at: https://www.nasa.gov/live

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. The ISS has been the most politically complex space exploration program ever undertaken.

Credit: NASA/Victor Zelentsov

Release Date: September 16, 2022

#NASA #ISS #Earth #Science #Soyuz #Rocket #SoyuzMS22 #Spacecraft #Cosmonauts #Commander #SergeyProkopyev #DmitriPetelin #Russia #Россия #Astronaut #FrankRubio #UnitedStates #JSC #BaikonurCosmodrome #Kazakhstan ##Қазақстан #Human #Spaceflight #Expedition68 #STEM #Education

Expedition 68 Soyuz Rocket Rollout in Kazakhstan | International Space Station

Expedition 68 Soyuz Rocket Rollout in Kazakhstan | International Space Station

U.S. astronaut Frank Rubio prepares for launch to the International Space Station on a Russian Soyuz rocket. A Soyuz rocket is raised to vertical after having rolled out by train to the launch pad, Sunday, Sept. 18, 2022, at site 31 of the Baikonur Cosmodrome in Kazakhstan. Expedition 68 astronaut Frank Rubio of NASA, and cosmonauts Sergey Prokopyev and Dmitri Petelin of Roscosmos are scheduled to launch aboard their Soyuz MS-22 spacecraft on Sept. 21.

Coverage will begin at 9 a.m. on NASA Television’s Public Channel, the NASA app, and on the agency’s website. 

Watch the Soyuz MS-22 launch online at: https://www.nasa.gov/live

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. The ISS has been the most politically complex space exploration program ever undertaken.

Image Credit: NASA/Bill Ingalls/Victor Zelentsov

Image Date: September 18, 2022

#NASA #ISS #Earth #Science #Soyuz #Rocket #SoyuzMS22 #Spacecraft #Cosmonauts #Commander #SergeyProkopyev #DmitriPetelin #Russia #Россия #Astronaut #FrankRubio #UnitedStates #JSC #BaikonurCosmodrome #Kazakhstan #Қазақстан #Human #Spaceflight #Expedition68 #STEM #Education