Thursday, February 16, 2023

Galaxy NGC 1433 | James Webb Space Telescope

Galaxy NGC 1433 | James Webb Space Telescope


This image taken by the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope shows one of a total of 19 galaxies targeted for study by the Physics at High Angular resolution in Nearby Galaxies (PHANGS) collaboration. Nearby barred spiral galaxy NGC 1433 takes on a completely new look when observed by Webb’s Mid-Infrared Instrument (MIRI).

Image Description: A large galaxy takes up the entirety of the image. The core is mostly bright white, but there are also swirling, detailed structures that resemble water circling a drain. There is white and light blue colored dust that emanates from the core’s center, but it is tightly contained to the core. The rings are wispy and highlight filaments of dust around cavernous black bubbles. The dust in the outer rings contains dots that are navy blue, pinkish, reddish, and white.

NGC 1433’s spiral arms are littered with evidence of extremely young stars releasing energy and, in some cases, blowing out the gas and dust of the interstellar medium they plough into. Areas that once appeared dark and dim in optical imaging light up under Webb’s infrared eye, as clumps of dust and gas in the interstellar medium absorb the light from forming stars and emit it back out in the infrared.

Webb’s image of NGC1433 is a dramatic display of the role that dynamic processes within the forming stars, dust, and gas play in the larger structure of an entire galaxy.

At the center of the galaxy, a tight, bright core featuring a unique double ring structure shines in exquisite detail, revealed by Webb’s extreme resolution. In this case, that double ring is actually tightly wrapped spiral arms that wind into an oval shape along the galaxy’s bar axis.

NGC 1433 is classified as a Seyfert galaxy, a galaxy relatively close to Earth that has a bright, active core. The brightness and lack of dust in the MIRI image of NGC 1433 could hint at a recent merger or even collision with another galaxy.

In the image of NGC 1433, blue, green, and red were assigned to Webb’s MIRI data at 7.7, 10 and 11.3, and 21 microns (the F770W, F1000W and F1130W, and F2100W filters, respectively).

MIRI was contributed by ESA and NASA, with the instrument designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) and NASA’s Jet Propulsion Laboratory, in partnership with the University of Arizona.


Credit: NASA, ESA, CSA, and J. Lee (NOIRLab), A. Pagan (STScI)

Release Date: Feb.16, 2023


#NASA #ESA #Astronomy #Space #Science #Galaxy #NGC1433 #Seyfert #Horologium #Constellation #JamesWebb #SpaceTelescope #JWST #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #NOIRLab #UnitedStates #STEM #Education

Galaxy NGC 1365 | James Webb Space Telescope

Galaxy NGC 1365 | James Webb Space Telescope

Scientists are getting their first look with the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope’s powerful resolution at how the formation of young stars influences the evolution of nearby galaxies. NGC 1365, observed here by Webb’s Mid-Infrared Instrument (MIRI) is one of a total of 19 galaxies targeted for study by the Physics at High Angular resolution in Nearby Galaxies (PHANGS) collaboration.

NGC 1365 is a double-barred spiral galaxy that lies about 56 million light-years away from Earth. It is one of the largest galaxies currently known to astronomers, spanning twice the length of the Milky Way.

Image Description: A large spiral galaxy takes up the entirety of the image, with the lower right portion of the galaxy’s spiral arms extending out of frame. The core of the galaxy is just off center to the lower right of the image. The bright core is an elongated oval with narrow, diffuse arms extending a short way out each narrow end of the oval. The main spiral arm to the upper left of the core is waspy and highlights filaments of dust around cavernous black bubbles.

As revealed by the MIRI observations of NGC 1365, clumps of dust and gas in the interstellar medium have absorbed the light from forming stars and emitted it back out in the infrared, lighting up an intricate network of cavernous bubbles and filamentary shells influenced by young stars releasing energy into the galaxy’s spiral arms.

Webb’s exquisite resolution also picks up several extremely bright star clusters not far from the core and newly observed recently formed clusters along the outer edges of the spiral arms.

Additionally, the Webb images provide insights into how the orbits of stars and gas vary depending on where they form, and how this results in the population of older clusters outside the inner star-formation ring.

In this image of NGC 1356, blue, green, and red were assigned to Webb’s MIRI data at 7.7, 10 and 11.3, and 21 microns (the F770W, F1000W and F1130W, and F2100W filters, respectively).

MIRI was contributed by ESA and NASA, with the instrument designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) and NASA’s Jet Propulsion Laboratory, in partnership with the University of Arizona.


Credit: NASA, ESA, CSA, and J. Lee (NOIRLab), A. Pagan (STScI)

Release Date: Feb. 16, 2023


#NASA #ESA #Astronomy #Space #Science #Galaxy #NGC1365 #Fornax #Constellation #JamesWebb #SpaceTelescope #JWST #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education

Galaxy NGC 7496 | James Webb Space Telescope

Galaxy NGC 7496 | James Webb Space Telescope

Scientists are getting their first look with the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope’s powerful resolution at how the formation of young stars influences the evolution of nearby galaxies. The spiral arms of NGC 7496, one of a total of 19 galaxies targeted for study by the Physics at High Angular resolution in Nearby Galaxies (PHANGS) collaboration, are filled with cavernous bubbles and shells overlapping one another in this image from Webb’s Mid-Infrared Instrument (MIRI). These filaments and hollow cavities are evidence of young stars releasing energy and, in some cases, blowing out the gas and dust of the interstellar medium they plough into.

NGC 7496 lies over 24 million light-years away from Earth in the constellation Grus.

Image Description: A large galaxy takes up the entirety of the image. Six reddish diffraction spikes extend from the core. The spiral arms of the galaxy outstretch to the upper left and the lower right. The arms are wispy and highlight filaments of dust around cavernous black bubbles. That dust in the outer rings contains diffuse dots that are navy blue, pinkish, reddish, and white.

Until Webb’s high resolution at infrared wavelengths came along, stars at the earliest point of their lifecycle in nearby galaxies like NGC 7496 remained obscured by gas and dust. Webb’s specific wavelength coverage (7.7 and 11.3 microns), allows for the detection of polycyclic aromatic hydrocarbons, which play a critical role in the formation of stars and planets. In Webb’s MIRI image, these are mostly found within the main dust lanes in the spiral arms.

In their analysis of the new data from Webb, scientists were able to identify nearly 60 new, undiscovered embedded cluster candidates in NGC 7496. These newly identified clusters could be among the youngest stars in the entire galaxy.

At the center of NGC 7496, a barred spiral galaxy, is an active galactic nucleus (AGN). An AGN is a supermassive black hole that is emitting jets and winds. The AGN glows brightly at the center of this Webb image. Additionally, Webb’s extreme sensitivity also picks up various background galaxies,far distant from NGC 7496, which appear green or red in some instances.

In this image of NGC 7496, blue, green, and red were assigned to Webb’s MIRI data at 7.7, 10 and 11.3, and 21 microns (the F770W, F1000W and F1130W, and F2100W filters, respectively).

MIRI was contributed by ESA and NASA, with the instrument designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) and NASA’s Jet Propulsion Laboratory, in partnership with the University of Arizona.


Credit: NASA, ESA, CSA, and J. Lee (NOIRLab), A. Pagan (STScI)

Release Date: Feb. 16, 2023


#NASA #ESA #Astronomy #Space #Science #NGC7496 #AGN #Grus #Constellation #JamesWebb #SpaceTelescope #JWST #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education

Practicing Moonwalks for Future Artemis Missions | NASA's Johnson Space Center

Practicing Moonwalks for Future Artemis Missions | NASA's Johnson Space Center









JETT3 was the third simulated moonwalk in preparation for future Artemis missions; during Artemis III, astronauts will visit the lunar South Pole region, which has never been explored by humans. The S P Crater has unique terrain and geology, as well as minimal communications infrastructure that make it a great location for an analog mission.

Two Joint Extravehicular Activity Test Team Field Test #3 (JETT3) mission members work on sample collection on the remote, rocky, high-desert terrain of the S P Crater near Flagstaff, Arizona, on Oct. 5, 2022.

Credit: NASA's Johnson Space Center (JSC)
Release Date: Feb. 15, 2023

#NASA #Space #Astronomy #Science #Earth #Moon #SouthPole #Artemis #JETT3 #Analog #AnalogAstronauts #Astronauts #Technology #Engineering #JSC #Flagstaff #Arizona #UnitedStates #STEM #Education 

Galactic Crash Course | Hubble Space Telescope

Galactic Crash Course | Hubble Space Telescope

A spectacular trio of merging galaxies in the constellation Boötes takes center stage in this image from the NASA/European Space Agency Hubble Space Telescope. These three galaxies, known to astronomers as SDSSCGB 10189, are set on a collision course and will eventually merge into a single larger galaxy, distorting one another’s spiral structure through mutual gravitational interaction in the process. An unrelated foreground galaxy appears to float serenely alongside the collision, and the smudged shapes of much more distant galaxies are visible in the background.


Credit: European Space Agency/Hubble & NASA, M. Sun

Duration: 30 seconds

Release Date: Feb. 15, 2023

#NASA #Hubble #Astronomy #Space #Science #Stars #Galaxies #SDSSCGB10189 #BCG #Bootes #Constellation #Galaxy #Galaxies #Cosmos #Universe #HST #SpaceTelescope #ESA #Europe #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Wednesday, February 15, 2023

Moon Mountain Name Honors NASA Mathematician Melba Mouton

Moon Mountain Name Honors NASA Mathematician Melba Mouton

Scientists recently named a mesa-like lunar mountain that towers above the landscape carved by craters near the Moon’s South Pole. This unique feature will now be referred to as “Mons Mouton,” after NASA mathematician and computer programmer Melba Roy Mouton.

Learn more about Melba Roy Mouton:

https://www.nasa.gov/feature/ames/moon-mountain-name-honors-nasa-mathematician-melba-mouton/


NASA's Ames Research Center is located in California's Silicon Valley.


Credit: NASA's Ames Research Center 

Duration: 1 minutes, 46 seconds

Release Date: Feb. 15, 2023


#NASA #Space #Astronomy #Science #Earth #Apollo #Artemis #Moon #SouthPole #Mountain #MonsMouton #Landmark #Mathematician #MelbaRoyMouton #Women #AfricanAmerican #Leaders #Pioneers #Ames #California #UnitedStates #STEM #Education #History #HD #Video

NASA Astronaut Victor Glover: New Eyes | Johnson Space Center

NASA Astronaut Victor Glover: New Eyes | Johnson Space Center

Down to Earth - S2:E7: In this episode of Down to Earth, astronaut Victor Glover sits down with his daughter, Corinne, to discuss the important lessons he took away from his time in space.


Credit: NASA's Johnson Space Center (JSC)

Duration: 4 minutes, 19 seconds

Release Date: Feb. 15, 2023


NASA Astronaut Victor Glover's Official Biography

https://www.nasa.gov/astronauts/biographies/victor-j-glover

https://www.nasa.gov/astronauts/biographies/victor-j-glover/biography


Credit: NASA's Johnson Space Center

Duration: 4 minutes, 31 seconds

Release Date: Sept. 20, 2022


#NASA #Space #ISS #Artemis #Moon #SpaceX #SpaceXCrew1 #CrewDragon #Spacecraft #Astronaut #VictorGlover #Pilot #Aviator #Engineer #Leader #USNavy #HumanSpaceflight #Expedition64 #AfricanAmerican #JSC #Houston #Texas #UnitedStates #STEM #Education #HD #Video

Zoom into Pandora’s Cluster: Abell 2744 | James Webb Space Telescope

Zoom into Pandora’s Cluster: Abell 2744 | James Webb Space Telescope

Astronomers estimate 50,000 sources of near-infrared light are represented in this image from the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope. Their light has traveled through various distances to reach the telescope’s detectors, representing the vastness of space in a single image. A foreground star in our own galaxy, to the right of the image center, displays Webb’s distinctive diffraction spikes. Bright white sources surrounded by a hazy glow are the galaxies of Pandora’s Cluster, a conglomeration of already-massive clusters of galaxies coming together to form a mega cluster. The concentration of mass is so great that the fabric of spacetime is warped by gravity, creating a natural, super-magnifying glass called a 'gravitational lens' that astronomers can use to see very distant sources of light beyond the cluster that would otherwise be undetectable, even to Webb.


Credit: NASA, ESA, CSA, I. Labbe (Swinburne University of Technology), R. Bezanson (University of Pittsburgh), A. Pagan (STScI). Dark Energy Survey/DOE/FNAL/NOIRLab/NSF/AURA, DSS, N. Bartmann, E. Slawik, N. Risinger, D. de Martin, M. Zamani  

Duration: 1 minute

Release Date: Feb. 15, 2023

#NASA #ESA #Astronomy #Space #Science #PandorasCluster #Abell2744 #Astrophysics #GravitationalLensing #Sculptor #Constellation #JamesWebb #SpaceTelescope #JWST #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Take a Tour of Pandora's Cluster | James Webb Space Telescope

Take a Tour of Pandora's Cluster | James Webb Space Telescope

This video tours Pandora’s Cluster (Abell 2744), a region where multiple clusters of galaxies are in the process of merging to form a megacluster. Astronomers estimate 50,000 sources of near-infrared light are represented in this image from NASA’s James Webb Space Telescope.

The concentration of mass in Pandora’s Cluster is so great that the fabric of spacetime is warped by gravity, creating an effect that makes the region of special interest to astronomers: a natural, super-magnifying glass called a “gravitational lens” that they can use to see very distant sources of light beyond the cluster that would otherwise be undetectable, even to Webb. These lensed sources, which are particularly prominent in the lower right area, appear red in the image, and often as elongated arcs distorted by the gravitational lens.

The video also highlights a mysterious object that appears to be no more than a red dot. One theory is that this source of infrared light is a glowing disk of gas surrounding a supermassive black hole in the early universe.


Credits:

Video: STScI, Danielle Kirshenblat

Music: PremiumBeat Music, Klaus Hergersheimer

Science: Ivo Labbe (Swinburne), Rachel Bezanson (University of Pittsburgh)

Image Processing: STScI, Alyssa Pagan

Duration: 1 minute, 38 seconds

Release Date: Feb. 15, 2023

#NASA #ESA #Astronomy #Space #Science #PandorasCluster #Abell2744 #Astrophysics #GravitationalLensing #Sculptor #Constellation #JamesWebb #SpaceTelescope #JWST #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Pan of Pandora’s Cluster: Abell 2744 | James Webb Space Telescope

Pan of Pandora’s Cluster: Abell 2744 | James Webb Space Telescope

Astronomers estimate 50,000 sources of near-infrared light are represented in this image from the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope. Their light has traveled through various distances to reach the telescope’s detectors, representing the vastness of space in a single image. 

A foreground star in our own galaxy, to the right of the image center, displays Webb’s distinctive diffraction spikes. Bright white sources surrounded by a hazy glow are the galaxies of Pandora’s Cluster, a conglomeration of already-massive clusters of galaxies coming together to form a mega cluster. The concentration of mass is so great that the fabric of spacetime is warped by gravity, creating a natural, super-magnifying glass called a 'gravitational lens' that astronomers can use to see very distant sources of light beyond the cluster that would otherwise be undetectable, even to Webb.


Credit: NASA, ESA, CSA, I. Labbe (Swinburne University of Technology), R. Bezanson (University of Pittsburgh), A. Pagan (STScI), N. Bartmann (ESA/Webb)  

Duration: 30 seconds

Release Date: Feb. 15, 2023


#NASA #ESA #Astronomy #Space #Science #PandorasCluster #Abell2744 #Astrophysics #GravitationalLensing #Sculptor #Constellation #JamesWebb #SpaceTelescope #JWST #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Pandora’s Cluster: Abell 2744 | James Webb Space Telescope

Pandora’s Cluster: Abell 2744 | James Webb Space Telescope

Astronomers estimate 50,000 sources of near-infrared light are represented in this image from the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope. Their light has traveled through various distances to reach the telescope’s detectors, representing the vastness of space in a single image. A foreground star in our own galaxy, to the right of the image center, displays Webb’s distinctive diffraction spikes. Bright white sources surrounded by a hazy glow are the galaxies of Pandora’s Cluster, a conglomeration of already-massive clusters of galaxies coming together to form a mega cluster. The concentration of mass is so great that the fabric of spacetime is warped by gravity, creating a natural, super-magnifying glass called a 'gravitational lens' that astronomers can use to see very distant sources of light beyond the cluster that would otherwise be undetectable, even to Webb.

Image Description: A crowded galaxy field on a black background, with one large star dominating the image just right of center. Three areas are concentrated with larger white hazy blobs on the left, lower right, and upper right above the single star. Scattered between these areas are many smaller sources of light; some also have a hazy white glow, while many other are red or orange.

These lensed sources appear red in the image, and often as elongated arcs distorted by the gravitational lens. Many of these are galaxies from the early universe, with their contents magnified and stretched out for astronomers to study. Other red sources in the image have yet to be confirmed by follow-up observations with Webb’s Near-Infrared Spectrograph (NIRSpec) instrument to determine their true nature. One intriguing example is an extremely compact source that appears as a tiny red dot, despite the magnifying effect of the gravitational lens. One possibility is that the dot is a supermassive black hole in the early universe. NIRSpec data will provide both distance measurements and compositional details of selected sources, providing a wealth of previously-inaccessible information about the universe and how it has evolved over time.


Credit: NASA, ESA, CSA, I. Labbe (Swinburne University of Technology), R. Bezanson (University of Pittsburgh), A. Pagan (STScI)

Release Date: Feb. 15, 2022


#NASA #ESA #Astronomy #Space #Science #PandorasCluster #Abell2744 #Astrophysics #GravitationalLensing #Sculptor #Constellation #JamesWebb #SpaceTelescope #JWST #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education

Tuesday, February 14, 2023

Uninhabited Atolls of French Polynesia | International Space Station

Uninhabited Atolls of French Polynesia | International Space Station



The uninhabited atolls of (from left) Vahanga, Tenarungo, and Tenanaro, which are part of French Polynesia in the south Pacific Ocean, are pictured from the International Space Station as it orbited 260 miles above.

Follow Expedition 68 crew updates at:

https://blogs.nasa.gov/spacestation/


Expedition 68 Crew

Station Commander: Sergey Prokopyev of Roscosmos (Russia)

Roscosmos (Russia): Flight Engineers Anna Kikina & Dmitri Petelin

NASA: Flight Engineers Nicole Mann, Frank Rubio & Josh Cassada

JAXA (Japan): Flight Engineer Koichi Wakata


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's Johnson Space Center (JSC)

Image Date: Jan. 30, 2023


#NASA #Space #ISS #Earth #Planet #Atolls #Vahanga #Tenarungo #Tenanaro #FrenchPolynesia #France #PacificOcean #Astronauts #Photography #Science #HumanSpaceflight #Expedition68 #Europe #JSC #UnitedStates #Canada #Japan #日本 #Russia #Россия #International #OverviewEffect #OrbitalPerspective #STEM #Education

NASA’s Perseverance Rover Shows Off Collection of Mars Samples

NASA’s Perseverance Rover Shows Off Collection of Mars Samples

NASA's Perseverance Mars rover took a selfie with several of the 10 sample tubes it deposited at a sample depot it is creating within an area of Jezero Crater nicknamed "Three Forks." The image was taken by the WATSON (Wide Angle Topographic Sensor for Operations and eNgineering) camera on the end of the rover's robotic arm.

NASA's Perseverance Mars rover dropped the last of 10 tubes at the "Three Forks" sample depot. 

This photomontage shows each of the sample tubes deposited by NASA’s Perseverance Mars rover at the “Three Forks” sample depot, as viewed by the WATSON camera on the end of the rover’s robotic arm. 
NASA’s Perseverance rover captured this portrait of its recently completed sample depot using its Mastcam-Z camera on Jan. 31, 2023, the 693rd Martian day, or sol, of the mission. Containing 10 samples, the depot is a crucial milestone in the NASA-ESA Mars Sample Return campaign. 
An annotated version of the portrait captured by NASA’s Perseverance shows the location of the 10 sample tubes in the depot. The “Amalik” sample closest to the rover was about 10 feet (3 meters) away; the “Mageik” and “Malay” samples farthest away were approximately 197 feet (60 meters) from the rover. 


NASA’s Perseverance rover captured a portrait of its recently completed sample depot using its Mastcam-Z camera on Jan. 31, 2023, the 693rd Martian day, or sol, of the mission. Containing 10 samples, the depot is a crucial milestone in the NASA-European Space Agency Mars Sample Return campaign. It is humanity’s first collection of samples on another planet. The panorama, stitched together from 368 images that were sent to Earth, captures more than a month of careful placement and mapping of 10 titanium tubes.

Eight of those tubes are filled with rock and regolith (broken rock and dust), while one is an atmospheric sample and one is a “witness” tube. The rover photographed the depot using the Mastcam-Z camera on the top of its mast, or “head,” on Jan. 31, 2023. The color has been adjusted to show the Martian surface approximately as it would look to the human eye.

The depot represents a backup collection of samples that could be recovered in the future by the Mars Sample Return campaign, a joint effort between NASA and European Space Agency (ESA) that aims to bring Mars samples to Earth for closer study. The rover began building the depot on Dec. 21, 2022, precisely spacing the tubes in case they need to be retrieved at a future date.

The primary tubes reside in the belly of Perseverance, which would pass them, along with future samples taken during the mission to a Sample Retrieval Lander as part of the campaign. If anything were to happen to the rover to prevent it from delivering tubes directly to the lander, samples could be retrieved from the depot instead. (Learn more about all 18 samples taken so far.)

Perseverance built the depot at “Three Forks,” a location within Jezero Crater. Billions of years ago, a river flowed into the crater, carrying sediment that formed a steep, fan-shaped delta that the rover will drive up in the months ahead.

While the Martian surface is now cold, dry, and generally inhospitable to life, ancient Mars was likely similar to Earth—and could have supported microbial life, if any ever formed on the Red Planet. The samples Perseverance is collecting could help scientists determine whether life ever left its mark in a place like Jezero Crater.


More About the Mission

A key objective for Perseverance’s mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet’s geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust).

Subsequent NASA missions, in cooperation with the European Space Agency, would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis.

The Mars 2020 Perseverance mission is part of NASA’s Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet.

JPL, which is managed for NASA by Caltech in Pasadena, California, built and manages operations of the Perseverance rover. Arizona State University leads the operations of the Mastcam-Z instrument, working in collaboration with Malin Space Science Systems in San Diego, on the design, fabrication, testing, and operation of the cameras, and in collaboration with the Neils Bohr Institute of the University of Copenhagen on the design, fabrication, and testing of the calibration targets.


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 possible return to Earth.

Mars Helicopter (Ingenuity)

Launch: July 30, 2020    

Landing: Feb. 18, 2021, Jezero Crater, Mars

For more about Perseverance:

mars.nasa.gov/mars2020/


Credit: NASA/JPL-Caltech/ASU/MSSS

Release Date: Feb. 14, 2023


#NASA #ESA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #PerseveranceRover #Mars2020 #MSR #JezeroCrater #Robotics #Technology #Engineering #JPL #UnitedStates #Europe #MoonToMars #Annotated #STEM #Education

Mexico's Yucatan Peninsula & Isla Pérez | International Space Station

Mexico's Yucatan Peninsula & Isla Pérez | International Space Station

Mexico's Yucatan Peninsula and Isla Pérez (lower right) are pictured from the International Space Station as it orbited 259 miles above the Gulf of Mexico.

Mexico's Isla Pérez of the Yucatan Peninsula is pictured from the International Space Station as it orbited 259 miles above the Gulf of Mexico.

Follow Expedition 68 crew updates at:

https://blogs.nasa.gov/spacestation/

Expedition 68 Crew

Station Commander: Sergey Prokopyev of Roscosmos (Russia)

Roscosmos (Russia): Flight Engineers Anna Kikina & Dmitri Petelin

NASA: Flight Engineers Nicole Mann, Frank Rubio & Josh Cassada

JAXA (Japan): Flight Engineer Koichi Wakata


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's Johnson Space Center (JSC)

Image Date: Jan. 29, 2023


#NASA #Space #ISS #Earth #Planet #Mexico #YucatanPeninsula #IslaPérez #GulfOfMexico #AtlanticOcean #Astronauts #Photography #Science #HumanSpaceflight #Expedition68 #Europe #JSC #UnitedStates #Canada #Japan #日本 #Russia #Россия #International #OverviewEffect #OrbitalPerspective #STEM #Education

Orbital Sunrise above Pacific Ocean | International Space Station

Orbital Sunrise above Pacific Ocean | International Space Station

The soft hues of an orbital sunrise begin revealing the cloud tops above the Pacific Ocean northeast of New Zealand as the International Space Station orbited 260 miles above.

Follow Expedition 68 crew updates at:

https://blogs.nasa.gov/spacestation/


Expedition 68 Crew

Station Commander: Sergey Prokopyev of Roscosmos (Russia)

Roscosmos (Russia): Flight Engineers Anna Kikina & Dmitri Petelin

NASA: Flight Engineers Nicole Mann, Frank Rubio & Josh Cassada

JAXA (Japan): Flight Engineer Koichi Wakata


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's Johnson Space Center (JSC)

Image Date: Feb. 10, 2023


#NASA #Space #ISS #Earth #Planet #Orbital #Sunrise #PacificOcean #Astronauts #Photography #Science #HumanSpaceflight #Expedition68 #Europe #UnitedStates #Canada #Japan #日本 #Russia #Россия #International #OverviewEffect #OrbitalPerspective #STEM #Education

Saturn's Glory | NASA Cassini Mission

Saturn's Glory | NASA Cassini Mission


   Saturn's Rings - May 28, 2009


Saturn's Rings - June 12, 2009


Saturn's Rings - Aug. 31, 2009


Saturn - Feb. 14, 2017


Saturn - June 12, 2017


The Cassini spacecraft ended its mission on Sept. 15, 2017. Cassini's end involved a series of close Saturn passes, approaching within the rings, then an entry into Saturn's atmosphere to destroy the spacecraft. This method was chosen because it is necessary to ensure protection and prevent biological contamination to any of the moons of Saturn thought to offer potential habitability.

For more information about the Cassini-Huygens mission visit: https://saturn.jpl.nasa.gov and www.nasa.gov/cassini

The Cassini-Huygens mission was a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, California, managed the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center was based at the Space Science Institute in Boulder, Colorado.

Credit: NASA/Jet Propuslion Laboratory-Caltech/Space Science Institute (SSI)/Cassini Imaging Central Laboratory for Operations (CICLOPS)
Processing: Kevin M. Gill
Release Date: Feb. 10-13, 2023

#NASA #Astronomy #Science #Space #Saturn #Planet #Rings #SolarSystem #Exploration #Cassini #Spacecraft #JPL #California #UnitedStates #ESA #Europe #ASI #History #STEM #Education