Thursday, December 19, 2024

Saturnian Grooves | NASA's Cassini Mission

Saturnian Grooves | NASA's Cassini Mission

Saturn - August 19, 2009
Saturn - June 12, 2007
Saturn - November 4, 2006
Saturn - April 25, 2008

Planet Saturn's rings can appear similar to the grooves of a vinyl record. The first 12-inch, 33-revolutions per minute (RPM) record was produced by the American company Columbia Broadcasting System (CBS) in 1948. Twelve-inch albums could hold an album’s worth of songs on each side. They arrived on the market when the postwar entertainment industry was booming. Consumers were ready to buy these 12-inch LP (long-play) records. They quickly became the industry standard. Instead of the hard shellac that 78s were made from, 12-inch LPs consisted of polyvinyl carbonate, the material that gives vinyl records their name.

Source: "The History of Vinyl Records: An In-Depth Guide"
https://thesoundofvinyl.us/blogs/vinyl-101/the-history-of-vinyl-records

NASA's Cassini spacecraft arrived in the Saturn system in 2004 and ended its mission in 2017 by deliberately plunging into Saturn's atmosphere. 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.

The Cassini-Huygens mission was a cooperative project of NASA, European Space Agency (ESA) and the Italian Space Agency. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the mission for NASA's Science Mission Directorate, Washington. JPL designed, developed and assembled the Cassini orbiter. The Cassini radar instrument was built by JPL and the Italian Space Agency, working with team members from the U.S. and several European countries.

NASA Cassini Mission information: 
https://solarsystem.nasa.gov/cassini


Image Credit: NASA/JPL-Caltech/SSI/CICLOPS
Processing: Kevin M. Gill
Image Dates: Nov. 4, 2006-Aug. 19, 2009


#NASA #Astronomy #Space #Science #Planet #Saturn #Rings #Astrobiology #SolarSystem #CassiniMission #CassiniSpacecraft #JPL #Caltech #UnitedStates #ESA #Italy #Italia #ASI #Europe #Records #VinyRecords #History #STEM #Education

Planet Mars: 'Texoli' Butte on Mount Sharp | NASA Curiosity Mars Rover

Planet Mars: 'Texoli' Butte on Mount Sharp | NASA Curiosity Mars Rover

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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

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

NASA's Curiosity Mars rover used its right Mast Camera, or Mastcam, to capture this panorama on Nov. 26, 2024, the 4,375th Martian day, or sol, of the mission. Made from 251 individual images containing 393 million pixels, the panorama's color has been adjusted to match lighting conditions as the human eye would see them on Earth. This is one of the largest high-resolution panoramas Curiosity has taken during its mission.

Curiosity is making its way up the foothills of Mount Sharp, a 3-mile-tall (5-kilometer-tall) mountain found within Mars' Gale Crater. Dominating the scene in this image is a butte on Mount Sharp nicknamed "Texoli". It has many stratigraphic layers that scientists can study to learn more about the formation of this region of Mars. Texoli stands about 525 feet (160 meters) tall.

A butte is "an isolated hill with steep, often vertical sides and a small, relatively flat top."

To the right of Texoli is another butte nicknamed "Wilkerson." It is 262 feet (80 meters) tall. Curiosity will travel between the two buttes as it drives away from Gediz Vallis channel. It has been investigating this area for the past year, and from Gediz Vallis (Gediz valley) itself, where it has been for four years.

On the horizon beyond Texoli on the left side of the image is the Yardang Unit—a higher-elevation geologic region that Curiosity's scientists hope to visit in the years to come. On the horizon on the right side of the image, beyond Wilkerson, is the floor of Gale Crater and, visible through a dusty haze, the crater's distant northern rim.

For more about Curiosity, visit: 
science.nasa.gov/mission/msl-curiosity

Curiosity was built by NASA's Jet Propulsion Laboratory (JPL). It is managed by Caltech in Pasadena, California. JPL leads the mission on behalf of NASA's Science Mission Directorate in Washington. Malin Space Science Systems in San Diego built and operates Mastcam.


Image Credit: NASA/JPL-Caltech/MSSS
Release Date: Dec. 16, 2024


#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #CuriosityRover #MSL #Sol4375 #TexoliButte #MountSharp #GaleCrater #Robotics #SpaceTechnology #SpaceEngineering #MSSS #JPL #Caltech #UnitedStates #CitizenScience #KevinGill #STEM #Education

Cosmic Jingles: "Listen" to Euclid Space Telescope’s Image of Nebula M78 in Orion

Cosmic Jingles: "Listen" to Euclid Space Telescope’s Image of Nebula M78 in Orion

An ethereal dance of misty clouds of interstellar dust with a myriad of distant stars and galaxies speckled like paint drops over a black canvas. This is a sonification of a breathtaking image taken by the European Space Agency's Euclid space telescope of the young star-forming region Messier 78. 

The sonification offers a unique representation of the data collected by Euclid. It lets us explore the stellar nurseries in M78 through sound. Close your eyes and listen to let the cosmic image be drawn by your mind’s eye, or watch as the traceback line in this video follows the sounds to color the image from left to right.  

The twinkling sounds of pitches and volumes represent the galaxies and stars in the frame. The pitch of the sound points towards where we see the dot of light in the image. Higher pitches tell us that a star or galaxy appears further at the top in the image along the traceback line.  

The brightness of these objects in and around M78 are represented by the volume of the twinkles. Whenever we hear a particularly loud clink, the star or galaxy that Euclid observed appears particularly bright in the image. 

Underlying these jingling sounds, we can hear a steady undertone, made up of two chords which represent regions in Messier 78. This sound intensifies as the traceback line approaches first the brightest, and later the densest regions in the nebula.  

The first two deeper crescendos in this undertone indicate two patches in the image where the most intense color is blue/purple. These appear as two ‘cavities’ in M78, where newly forming stars carve out and illuminate the dust and gas in which they were born. 

The chords intensify a third time at a slightly higher pitch corresponding to the red-orange colors in the image, as the sound draws over the densest star-forming region of the frame. This stellar nursery is hidden by a layer of dust and gas that is so thick that it obscures almost all the light of the young stars within it.  

As the sound traces over the entire Euclid image, these different tones together form a cosmic symphony that represents the image of Messier 78, and the stars and galaxies that lie behind and within it.

Image Description: A filamentary orange veil covers a bright region of star formation. The background is dark, stippled with stars and galaxies ranging from small bright dots to starry shapes. The foreground veil spans from upper left to the bottom right and resembles a seahorse. Bright stars light up the ‘eye’ and ‘chest’ regions of the seahorse with purple light. Within the tail, three bright spots sit in a traffic-light like formation.

Many thanks to Klaus Nielsen (DTU Space/Maple Pools) for making the sonification in this video. If you would like to hear more sonifications and music by this artist, please visit:
https://linktr.ee/maplepools 


Credits: ESA/Euclid/Euclid Consortium/NASA Image Processing: J.-C. Cuillandre (CEA Paris-Saclay) and G. Anselmi, sonification by K. Nielsen (DTU Space/Maple Pools)
Duration: 1 minute, 29 seconds
Release Date: Dec. 19, 2024

#NASA #ESA #ESAEuclid #Astronomy #Space #Science #Stars #Nebulae #StellarNursery #Messier78 #Orion #Cosmos #Universe #EST #EuclidSpaceTelescope #Infrared #SpaceTelescopes #Sonification #Europe #STEM #Education #HD #Video

Aurora Australis in Antarctica | European Space Agency

Aurora Australis in Antarctica | European Space Agency


A mesmerizing display of Aurora Australis (southern lights) glows over the Concordia research station in Antarctica with yellow hues shimmering near the horizon and red lights stretching upwards into the vast polar sky.

These beautiful colors result from the interaction of charged particles from the Sun with gases in our atmosphere, guided by Earth's magnetic field to the polar regions. Green aurorae, the most common display, form at altitudes between 100 and 200 km, where oxygen atoms are highly concentrated and require less energy to emit light. During periods of high solar activity, charged particles become more energetic and can interact with oxygen at higher altitudes above 200 km, where oxygen atoms are less concentrated and need more energy to emit light. This higher energy corresponds to light with a longer wavelength, producing the stunning red aurorae. The beautiful yellow hues seen on the horizon occur when green and red aurorae mix in areas of overlap.

Standing beneath this incredible natural phenomenon is Jessica Studer, the European Space Agency-sponsored medical doctor for Concordia's 2024 winter-over. Jessica lived with a small team in complete isolation during the harsh Antarctic winter where the Sun does not rise for four months and temperatures plunge as low as –85°C. Concordia is one of the most remote places on Earth; the closest humans are at Russia's Vostok research station 600 km away, making it more isolated than the International Space Station. The station is an unique platform for research in fields like astronomy, glaciology, and human physiology, offering insights into how humans adapt to extreme isolation, cold, and darkness—conditions that mirror those faced by astronauts in space.

The aurorae visible here were captured in May 2024, during a period of heightened solar activity associated with the ongoing solar activity maximum, a phase in the Sun’s 11-year cycle that increases the intensity and frequency of auroral displays. These vibrant skies are just one of the benefits of living and working in Concordia, alongside the opportunity to contribute to groundbreaking science in a challenging environment.

Would you like to experience these breathtaking sights yourself? The European Space Agency (ESA) is currently accepting applications for a medical doctor to spend the winter of 2026 at Concordia station—apply here: https://bit.ly/3P4WXWc


Image Credits: ESA/IPEV/PNRA-J. Studer
Image Date: May 2024

#NASA #ESA #Space #Astronomy #Science #Sun #Magnetosphere #Planet #Earth #Atmosphere #Aurora #AuroraAustralis #SouthernLights #Antarctica #SouthPole #ConcordiaStation #Europe #Stars #MilkyWayGalaxy #Cosmos #Universe #STEM #Education

NASA "Espacio a Tierra" | Un satélite de madera: 13 de diciembre de 2024

NASA "Espacio a Tierra" | Un satélite de madera: 13 de diciembre 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: NASA's Johnson Space Center (JSC)
Duration: 4 minutes
Release Date: Dec. 18, 2024

#NASA #Space #Science #ISS #Earth #NASAenespañol #español #Satellites #LingoSat #SpaceXCargoDragon #CRS31 #Astrobee #Astronauts #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #LongDurationMissions #HumanSpaceflight #SpaceLaboratory #UnitedStates #Expedition72 #STEM #Education #HD #Video

Shenzhou-19 Crew Sets New Record for Longest Spacewalk by Chinese Astronauts

Shenzhou-19 Crew Sets New Record for Longest Spacewalk by Chinese Astronauts

Shenzhou-19 crew members aboard China's orbiting Tiangong Space Station successfully completed a marathon nine-hour spacewalk at 21:57 Beijing Time on Tuesday, December 17, 2024, setting a new long duration record for Chinese astronauts' extravehicular activities (EVAs). 

The previous record for the longest spacewalk in Earth orbit was set by the Russian space agency Roscosmos after its cosmonauts completed a spacewalk lasting 8 hours and 13 minutes in 2018. It was set by Expedition 54 Commander Alexander Misurkin and Flight Engineer Anton Shkaplerov of the International Space Station.

Astronauts Cai Xuzhe, Song Lingdong were assigned the EVA duty, while Wang Haoze assisted the pair throughout the mission from inside the space station. It was the 17th spacewalk carried out by Chinese astronauts.

At the end of the mission, before closing the hatch, the Shenzhou-19 crew expressed their joy at completing the mission and their gratitude to the ground team.

"Congratulations to 02 for completing your first spacewalk and moreover, for becoming the first Chinese astronaut born after 1990 to carry out EVAs. My appreciation also goes to the full collaboration of 03 inside the module, and to the extensive support of Shuguang and the entire technical team. From the assigned tasks to the more flexible assignments, we feel greater and greater confidence in conducting extravehicular activities. China's space station will always remain something to look forward to," said Cai, commander of Shenzhou-19 spaceflight mission crew.

"I express my gratitude to 01, Shuguang, and all the ground staff. Today, our crew and the ground team worked together to make the extravehicular activities a success. As I admired the spectacular view in space, I felt deep in my heart how important and great a cause the manned spaceflight is. I want to take this opportunity to thank all those who dedicate themselves to this cause—those who were here before us and who are with us along the way. Thank you all for your hard work, so that we were given the chance to conduct a spacewalk. The cause of the manned spaceflight is a relay race, and we are in it every step of the way. Let us keep striving and head for the future together," said Song.

"Congratulations to 01 and 02 for successfully completing your talks. Both of you made breakthroughs and I'm proud of your excellent performance. Meanwhile, my thanks also go to Shuguang and all the staff who worked day and night on this mission. Everybody up in space and on Earth work as one in our exploration and joint efforts for a promising tomorrow. I wish everyone sweet dreams tonight," Wang said.

China launched the Shenzhou-19 crewed spaceship on Oct. 30, 2024, sending three astronauts—including the country's first female space engineer—to its orbiting space station for a six-month mission.

Shenzhou-19 Crew:
Commander Cai Xuzhe (蔡旭哲)
Mission Specialist Wang Haoze (王浩泽)
Mission Specialist Song Lingdong (宋令东)


Video Credit: CCTV
Duration: 2 minutes
Release Date: Dec. 17, 2024

#NASA #Space #Science #Earth #China #中国 #Shenzhou19 #神舟十九号 #Taikonauts #Astronauts #Spacewalk #EVA #CSS #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #SpaceLaboratory #CMSA #中国载人航天工程办公室 #LongDurationMissions #HumanSpaceflight #History #STEM #Education #HD #Video

Russian Cosmonaut Spacewalk: Walkthrough Animation | International Space Station

Russian Cosmonaut Spacewalk: Walkthrough Animation | International Space Station

[No Audio]: NASA coverage is underway for today’s spacewalk with Roscosmos cosmonauts Alexey Ovchinin and Ivan Vagner of Russia. The duo are venturing outside the station’s Poisk airlock to install an experiment package designed to monitor celestial x-ray sources and new electrical connector patch panels, remove several experiments for disposal,  and relocate a control panel for the European Robotic Arm that is attached to the Nauka multipurpose laboratory module. Additionally, the two cosmonauts will relocate a control panel for the European robotic arm, which is attached to the Nauka multipurpose laboratory module. Roscosmos cosmonaut Alexsandr Gorbunov will operate the arm during the spacewalk from inside the station.

The spacewalk is scheduled to last about six hours and 45 minutes. Roscosmos spacewalk 63 will be the second for Ovchinin and the first for Vagner. Ovchinin will wear an Orlan spacesuit with red stripes, and Vagner will wear a spacesuit with blue stripes. It will be the 272nd spacewalk in support of space station assembly, maintenance, and upgrades.

It will be the 272nd spacewalk in support of station maintenance and upgrades, the second for Ovchinin and the first for Vagner. 

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.


Video Credit: NASA's Johnson Space Center (JSC)
Duration: 9 minutes
Release Date: Dec. 19, 2024


#NASA #Space #Science #ISS #Earth #Spacewalk #EVA #Cosmonauts # IvanVagner #Russia #Россия #Roscosmos #Роскосмос #Astronauts #InternationalCooperation #LongDurationMissions #SpaceLaboratory #HumanSpaceflight #UnitedStates #Expedition72 #STEM #Education #Animation #HD #Video

Wednesday, December 18, 2024

Transition video: Hubble & Webb views of Spiral Galaxy NGC 2566 in Puppis

Transition video: Hubble & Webb views of Spiral Galaxy NGC 2566 in Puppis


Spiral galaxy NGC 2566 sits 76 million light-years away in the constellation Puppis.

The first view of the galaxy shown is a new image that is a combination of data from the James Webb Space Telescope's MIRI and NIRCam instruments. It shows off NGC 2566’s well-defined spiral arms, long central bar and delicate tracery of gas, dust and stars.

The second image is an also-new image from the NASA/European Space Agency Hubble Space Telescope and shows the galaxy’s star clusters and star-forming regions, bright in visible and ultraviolet light.


Credit: ESA/Webb/Hubble, NASA & CSA, A. Leroy, D. Thilker, N. Bartmann (ESA/Webb)
Duration: 30 seconds
Release Date: Dec. 18, 2024

#NASA #Astronomy #Space #Science #Stars #Galaxies #NGC2566 #SpiralGalaxy #Puppis #Constellation #Universe #JWST #MIRI #NIRCam #Infrared #Hubble #HST #SpaceTelescopes #ESA #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Spiral Galaxy NGC 2566: NirCam+MIRI views | James Webb Space Telescope

Spiral Galaxy NGC 2566: NirCam+MIRI views | James Webb Space Telescope


The galaxy filling the frame in this NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope picture is NGC 2566, a spiral galaxy located in the constellation Puppis. The image combines observations from two of Webb’s instruments, the Near-InfraRed Camera (NIRCam) and Mid-InfraRed Instrument (MIRI), to show off NGC 2566’s well-defined spiral arms, long central bar and delicate tracery of gas, dust and stars.

At 76 million light-years away, NGC 2566 is considered a nearby galaxy, making it an excellent target for studying fine details like star clusters and gas clouds. The new Webb images of NGC 2566 were collected as part of an observing program (#3707) dedicated to understanding the connections between stars, gas and dust in nearby star-forming galaxies. NGC 2566 is just one of the 55 galaxies in the local Universe examined by Webb for this program.

The mid-infrared wavelengths captured by MIRI highlight NGC 2566’s warm interstellar dust, including complex, sooty molecules called polycyclic aromatic hydrocarbons. The near-infrared NIRCam data give a detailed view of the galaxy’s stars, even those that are deeply embedded within clouds of gas. The NIRCam data also captured light from the hydrocarbon molecules.

To gain a full understanding of the star-formation process in nearby galaxies, astronomers will combine Webb data with observations from other telescopes. At the long-wavelength end of the electromagnetic spectrum, the 66 radio dishes of the Atacama Large Millimeter/submillimeter Array (ALMA) provide a detailed view of the cold, turbulent clouds where stars are born. 

The NASA/ESA Hubble Space Telescope has also cast its gaze on NGC 2566, and a new Hubble image of this galaxy was released earlier this week. The Hubble data will help researchers take a census of the stars in nearby galaxies, especially the young stars that are bright at the ultraviolet and visible wavelengths to which Hubble is sensitive. Together, the Webb, Hubble and ALMA data provide a rich view of the cold gas, warm dust and brilliant stars in NGC 2566.

Image Description: An oval-shaped spiral galaxy, seen close-up. Its core is a compact, pale spot that glows brightly, filling the disc with bluish light. Faint strands of pale reddish dust swirl out from the core to the far sides of the disc. They each join up with an arm of thick, cloudy, red dust with brighter orange patches, that follows the edge of the disc around to the opposite end and a little off the galaxy.


Credit: ESA/Webb, NASA & CSA, A. Leroy
Duration: 30 seconds
Release Date: Dec. 17, 2024


#NASA #Astronomy #Space #Science #NASAWebb #Stars #Galaxies #NGC2566 #SpiralGalaxy #Puppis #Constellation #Cosmos #Universe #UnfoldTheUniverse #JWST #MIRI #NIRCam #Infrared #SpaceTelescope #ESA #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Spiral Galaxy NGC 2566: NirCam+MIRI view | James Webb Space Telescope

Spiral Galaxy NGC 2566: NirCam+MIRI view | James Webb Space Telescope


The galaxy filling the frame in this NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope picture is NGC 2566, a spiral galaxy located in the constellation Puppis. The image combines observations from two of Webb’s instruments, the Near-InfraRed Camera (NIRCam) and Mid-InfraRed Instrument (MIRI), to show off NGC 2566’s well-defined spiral arms, long central bar and delicate tracery of gas, dust and stars.

At 76 million light-years away, NGC 2566 is considered a nearby galaxy, making it an excellent target for studying fine details like star clusters and gas clouds. The new Webb images of NGC 2566 were collected as part of an observing program (#3707) dedicated to understanding the connections between stars, gas and dust in nearby star-forming galaxies. NGC 2566 is just one of the 55 galaxies in the local Universe examined by Webb for this program.

The mid-infrared wavelengths captured by MIRI highlight NGC 2566’s warm interstellar dust, including complex, sooty molecules called polycyclic aromatic hydrocarbons. The near-infrared NIRCam data give a detailed view of the galaxy’s stars, even those that are deeply embedded within clouds of gas. The NIRCam data also captured light from the hydrocarbon molecules.

To gain a full understanding of the star-formation process in nearby galaxies, astronomers will combine Webb data with observations from other telescopes. At the long-wavelength end of the electromagnetic spectrum, the 66 radio dishes of the Atacama Large Millimeter/submillimeter Array (ALMA) provide a detailed view of the cold, turbulent clouds where stars are born. The NASA/ESA Hubble Space Telescope has also cast its gaze on NGC 2566, and a new Hubble image of this galaxy was released earlier this week. The Hubble data will help researchers take a census of the stars in nearby galaxies, especially the young stars that are bright at the ultraviolet and visible wavelengths to which Hubble is sensitive. Together, the Webb, Hubble and ALMA data provide a rich view of the cold gas, warm dust and brilliant stars in NGC 2566.

Image Description: An oval-shaped spiral galaxy, seen close-up. Its core is a compact, pale spot that glows brightly, filling the disc with bluish light. Faint strands of pale reddish dust swirl out from the core to the far sides of the disc. They each join up with an arm of thick, cloudy, red dust with brighter orange patches, that follows the edge of the disc around to the opposite end and a little off the galaxy.


Credit: ESA/Webb, NASA & CSA, A. Leroy
Release Date: Dec. 17, 2024


#NASA #Astronomy #Space #Science #NASAWebb #Stars #Galaxies #NGC2566 #SpiralGalaxy #Puppis #Constellation #Cosmos #Universe #UnfoldTheUniverse #JWST #MIRI #NIRCam #Infrared #SpaceTelescope #ESA #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education

Close-up view: Spiral Galaxy NGC 2566 in Puppis | James Webb Space Telescope

Close-up view: Spiral Galaxy NGC 2566 in Puppis | James Webb Space Telescope


The galaxy filling the frame in this NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope picture is NGC 2566, a spiral galaxy located in the constellation Puppis. In this image, Webb’s Mid-InfraRed Instrument (MIRI) puts the thick clouds of interstellar dust throughout NGC 2566 on display, as well as the galaxy’s compact, bright core.

At 76 million light-years away, NGC 2566 is considered a nearby galaxy, making it an excellent target for studying fine details like star clusters and gas clouds. The new Webb images of NGC 2566 were collected as part of an observing program (#3707) dedicated to understanding the connections between stars, gas and dust in nearby star-forming galaxies. NGC 2566 is just one of the 55 galaxies in the local Universe examined by Webb for this program.

To gain a full understanding of the star-formation process in nearby galaxies, astronomers will combine Webb data with observations from other telescopes. At the long-wavelength end of the electromagnetic spectrum, the 66 radio dishes of the Atacama Large Millimeter/submillimeter Array (ALMA) provide a detailed view of the cold, turbulent clouds where stars are born. The NASA/ESA Hubble Space Telescope has also cast its gaze on NGC 2566. The Hubble data will help researchers take a census of the stars in nearby galaxies, especially the young stars that are bright at the ultraviolet and visible wavelengths that Hubble is sensitive to. Together, the Webb, Hubble and ALMA data provide a comprehensive view of the cold gas, warm dust, and brilliant stars in NGC 2566.

Image Description: A spiral galaxy, seen close-up. Its core is a round spot that glows intensely bright, crowned by eight long and spikes that extend across the galaxy, artefacts of the telescope’s structure. Its disc is an oval shape with edges made of very thick and cloudy arms of gas and dust, mostly blue but paler and brighter around patches of stars. Wisps of darker dust also fill the inner disc and swirl off the ends of the arms.


Credit: ESA/Webb, NASA & CSA, A. Leroy
Duration: 30 seconds
Release Date: Dec. 17, 2024


#NASA #Astronomy #Space #Science #NASAWebb #Stars #Galaxies #NGC2566 #SpiralGalaxy #Puppis #Constellation #Cosmos #Universe #UnfoldTheUniverse #JWST #MIRI #Infrared #SpaceTelescope #ESA #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Spiral Galaxy NGC 2566 in Puppis | James Webb Space Telescope

Spiral Galaxy NGC 2566 in Puppis | James Webb Space Telescope

The galaxy filling the frame in this NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope picture is NGC 2566, a spiral galaxy located in the constellation Puppis. In this image, Webb’s Mid-InfraRed Instrument (MIRI) puts the thick clouds of interstellar dust throughout NGC 2566 on display, as well as the galaxy’s compact, bright core.

At 76 million light-years away, NGC 2566 is considered a nearby galaxy, making it an excellent target for studying fine details like star clusters and gas clouds. The new Webb images of NGC 2566 were collected as part of an observing program (#3707) dedicated to understanding the connections between stars, gas and dust in nearby star-forming galaxies. NGC 2566 is just one of the 55 galaxies in the local Universe examined by Webb for this program.

To gain a full understanding of the star-formation process in nearby galaxies, astronomers will combine Webb data with observations from other telescopes. At the long-wavelength end of the electromagnetic spectrum, the 66 radio dishes of the Atacama Large Millimeter/submillimeter Array (ALMA) provide a detailed view of the cold, turbulent clouds where stars are born. The NASA/ESA Hubble Space Telescope has also cast its gaze on NGC 2566. The Hubble data will help researchers take a census of the stars in nearby galaxies, especially the young stars that are bright at the ultraviolet and visible wavelengths that Hubble is sensitive to. Together, the Webb, Hubble and ALMA data provide a comprehensive view of the cold gas, warm dust, and brilliant stars in NGC 2566.

Image Description: A spiral galaxy, seen close-up. Its core is a round spot that glows intensely bright, crowned by eight long and spikes that extend across the galaxy, artefacts of the telescope’s structure. Its disc is an oval shape with edges made of very thick and cloudy arms of gas and dust, mostly blue but paler and brighter around patches of stars. Wisps of darker dust also fill the inner disc and swirl off the ends of the arms.


Credit: ESA/Webb, NASA & CSA, A. Leroy
Release Date: Dec. 17, 2024


#NASA #Astronomy #Space #Science #NASAWebb #Stars #Galaxies #NGC2566 #SpiralGalaxy #Puppis #Constellation #Cosmos #Universe #UnfoldTheUniverse #JWST #MIRI #Infrared #SpaceTelescope #ESA #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education

Close-up view: Spiral Galaxy NGC 2566 in Puppis | Hubble

Close-up view: Spiral Galaxy NGC 2566 in Puppis | Hubble


Featured in this NASA/European Space Agency Hubble Space Telescope picture is the spiral galaxy NGC 2566. It sits 76 million light-years away in the constellation Puppis. A prominent bar of stars stretches across the center of this galaxy, and spiral arms emerge from each end of the bar. Because NGC 2566 appears tilted from our perspective, its disc takes on an almond shape, giving the galaxy the appearance of a cosmic eye.

As NGC 2566 gazes at us, astronomers gaze right back, using Hubble to survey the galaxy’s star clusters and star-forming regions. The Hubble data are especially valuable for studying stars that are just a few million years old; these stars are bright at the ultraviolet and visible wavelengths to which Hubble is sensitive. Using these data, researchers will measure the ages of NGC 2566’s stars, helping to piece together the timeline of the galaxy’s star formation and the exchange of gas between star-forming clouds and stars themselves.

Several other astronomical observatories have examined NGC 2566, including the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope. The Webb data complement this Hubble image, adding a view of NGC 2566’s warm, glowing dust to Hubble’s stellar portrait. At the long-wavelength end of the electromagnetic spectrum, NGC 2566 has also been observed by the Atacama Large Millimeter/submillimeter Array (ALMA). ALMA is a network of 66 radio telescopes that work together as one to capture detailed images of the clouds of gas in which stars form. Together, Hubble, Webb and ALMA provide an overview of the formation, lives and deaths of stars in galaxies across the Universe.

Image Description: An oval-shaped spiral galaxy. Its core is a compact, glowing blue spot. A bright bar of light, lined with dark reddish dust, extends horizontally to the edge of the disc. A spiral arm emerges from each end of the bar and follows the edge of the disc, lined with blue and red glowing patches of stars, to the opposite end and a little off the galaxy. Blue stars are scattered between us and the galaxy.


Credit: ESA/Hubble & NASA, D. Thilker
Duration: 30 seconds
Release Date: Dec. 16, 2024


#NASA #ESA #Astronomy #Space #Science #Stars #Galaxies #NGC2566 #SpiralGalaxy #Puppis #Constellation #HubbleSpaceTelescope #HST #Cosmos #Universe #Europe #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

New Expedition 72 Crew & International Space Station Images

New Expedition 72 Crew & International Space Station Images

Astronauts Suni Williams and Don Pettit pose for a selfie-portrait
NASA astronauts Suni Williams and Don Pettit, Expedition 72 Commander and Flight Engineer respectively, take a break from science maintenance activities and pose for a selfie-portrait aboard the International Space Station's Harmony module.
NASA astronaut and Expedition 72 Commander Suni Williams photographs the European Materials Ageing (EMA) experiment hardware beng set up inside the International Space Station's Harmony module. EMA contains a variety of samples that will be exposed to the space environment to learn how to improve the development of space hardware and applications for missions to the Moon, Mars, and beyond. The external investigation will operate outside the Columbus laboratory module for about a year.
NASA astronaut and Expedition 72 Commander Suni Williams installs the European Materials Ageing experiment hardware inside the Nanoracks Bishop airlock. The external investigation will be robotically removed from Bishop, installed on the Bartolomeo research platform attached to the outside of the Columbus laboratory module, and expose a variety of materials to the vacuum of space for about a year.
NASA astronaut and Expedition 72 Flight Engineer Nick Hague installs the European Materials Ageing experiment hardware inside the Nanoracks Bishop airlock. The external investigation will be robotically removed from Bishop, installed on the Bartolomeo research platform attached to the outside of the Columbus laboratory module, and expose a variety of materials to the vacuum of space for about a year.
NASA astronauts Suni Williams and Nick Hague, Expedition 72 Commander and Flight Engineer respectively, install the European Materials Ageing experiment hardware inside the Nanoracks Bishop airlock. The external investigation will be robotically removed from Bishop, installed on the Bartolomeo research platform attached to the outside of the Columbus laboratory module, and expose a variety of materials to the vacuum of space for about a year.
The International Space Station is pictured from the SpaceX Dragon crew spacecraft by a SpaceX Crew-8 member shortly after undocking from the Harmony module's space-facing port. The orbital outpost was soaring 272 miles above the cloudy Patagonia region of South America at the time of this photograph on October 23, 2024.
The International Space Station is pictured from a window on the SpaceX Dragon crew spacecraft by a SpaceX Crew-8 member shortly after undocking from the Harmony module's space-facing port. The orbital outpost was soaring 272 miles above a cloudy Pacific Ocean off the coast of Chile at the time of this photograph on October 23, 2024.
The Full Moon is pictured from the International Space Station as it orbited 261 miles above the Pacific Ocean. In the foreground, a portion of one of the orbital outpost's radiators, also known as the External Active Thermal Control System, is seen.

Crew Update: Roscosmos cosmonauts Alexey Ovchinin and Ivan Vagner of Russia are preparing for a spacewalk that will see the duo remove external science experiments and relocate European robotic arm hardware. The pair organized their spacewalking tools and conducted photographic inspections inside the Poisk airlock where they will exit into the vacuum of space at 10:10 a.m. EST on Thursday, December 19, 2024. Ovchinin and Vagner will spend about six hour and 40-minutes wearing their Orlan spacesuits while tethered to the outside of the orbital outpost.

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.

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: Oct. 23-Dec. 14, 2024

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The Christmas Tree Cluster: NGC 2264 with Blinking X-rays | NASA Chandra

The Christmas Tree Cluster: NGC 2264 with Blinking X-rays | NASA Chandra



The “Christmas Tree Cluster,” or NGC 2264, shows a cluster of young stars between one and five million years old. (For comparison, the Sun is a middle-aged star about 5 billion years old—about 1,000 times older.) NGC 2264 is about 2,500 light-years from Earth. NASA Chandra X-ray Telescope data (red, purple, blue, and white) has been combined with optical data (green and violet) captured from by astrophotographer Michael Clow from his telescope in Arizona in November 2024.

Here, wispy green clouds in a conical shape strongly resemble an evergreen tree. Tiny specks of white, blue, purple, and red light, stars within the cluster, dot the structure, turning the cloud into a festive, cosmic Christmas tree!

NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program. The Smithsonian Astrophysical Observatory's Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.


Credits: 
X-ray: NASA/CXC/SAO
Optical: Michael Clow
Image Processing: NASA/CXC/SAO/L. Frattare and K. Arcand 
Video: NASA/CXC/A. Hobart
Duration: 12 seconds
Release Date: Dec. 17, 2024


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NASA Missions Spot Cosmic 'Wreath' Displaying Stellar Circle of Life

NASA Missions Spot Cosmic 'Wreath' Displaying Stellar Circle of Life

Most stars form in collections or groups, called clusters or associations that include very massive stars. Since antiquity, wreaths have symbolized the cycle of life, death, and rebirth. It is fitting then that one of the best places for astronomers to learn more about the stellar lifecycle resembles a giant holiday wreath itself.

The star cluster NGC 602 lies on the outskirts of the Small Magellanic Cloud. It is one of the closest galaxies to the Milky Way about 200,000 light-years from Earth. The stars in NGC 602 have fewer heavier elements compared to the Sun and most of the rest of the Galaxy. Instead, the conditions within NGC 602 mimic those for stars found billions of years ago when the Universe was much younger.

This new image combines data from NASA’s Chandra X-ray Observatory and James Webb Space Telescope (JWST). The dark ring-like outline of the wreath seen in JWST data is made up of dense clouds of filled dust.

Meanwhile, X-rays from Chandra show young, massive stars that are illuminating the wreath, sending high-energy light into interstellar space. These X-rays are powered by winds flowing from the young, massive stars that are sprinkled throughout the cluster. The extended cloud in the Chandra data likely comes from the overlapping X-ray glow of thousands of young, low-mass stars in the cluster.


Video Credit: NASA's Chandra X-ray Observatory
Duration: 1 minute, 45 seconds
Release Date: Dec. 17, 2024


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