Thursday, September 22, 2022

Center of The Milky Way: Wide-field View | ESO

Center of The Milky Way: Wide-field View | ESO


This visible light wide-field view shows the rich star clouds in the constellation of Sagittarius (the Archer) in the direction of the center of our Milky Way galaxy. The entire image is filled with vast numbers of stars—but far more remain hidden behind clouds of dust and are only revealed in infrared images. This view was created from photographs in red and blue light and form part of the Digitized Sky Survey 2. The field of view is approximately 3.5 degrees x 3.6 degrees.

Distance: 25,000 light years


Credit: European Southern Observatory (ESO) and Digitized Sky Survey 2

Acknowledgment: Davide De Martin and S. Guisard

Release Date: May 12, 2022


#NASA #ESO #Astronomy #Space #Science #BlackHole #SagittariusA #SagittariusAAsterisk #Sagittarius #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Telescope #Chile #Europe #STEM #Education

Hot Gas Bubble Swirling Around Our Supermassive Black Hole | ESO

Hot Gas Bubble Swirling Around Our Supermassive Black Hole | ESO

ESOcast 256 Light: Using the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers have found a hot bubble of gas that swirls around Sagittarius A*, the black hole at the center of our galaxy, at 30% of the speed of light.


Credit: European Southern Observatory (ESO)

Directed by: Herbert Zodet and Martin Wallner

Editing: Herbert Zodet

Web and technical support: Gurvan Bazin and Raquel Yumi Shida

Written by: Rebecca Forsberg and Rory Harris

Footage and photos: ESO, Event Horizon Telescope (EHT) Collaboration, M. Kornmesser, L. Calçada (Acknowledgment: M. Wielgus), Jordy Davelaar et al./Radboud University/BlackHoleCam, ALMA (ESO/NAOJ/NRAO) and C. Malin

Scientific consultant: Mariya Lyubenova

Release Date: September 22, 2022

Duration: 1 minute, 27 seconds


#NASA #ESO #ALMA #EHT #Astronomy #Space #Science #GasBubble #BlackHole #SagittariusA #SagittariusAAsterisk #MilkyWay #Galaxy #Cosmos #Universe #Telescope #Chile #Europe #Infographics #STEM #Education #HD #Video

Hot Gas Bubble Detected Swirling around Milky Way’s Black Hole | ESO

Hot Gas Bubble Detected Swirling around Milky Way’s Black Hole | ESO




Using the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers have spotted signs of a ‘hot spot’ orbiting Sagittarius A*, the black hole at the center of our galaxy. The finding helps us better understand the enigmatic and dynamic environment of our supermassive black hole.

“We think we're looking at a hot bubble of gas zipping around Sagittarius A* on an orbit similar in size to that of the planet Mercury, but making a full loop in just around 70 minutes. This requires a mind blowing velocity of about 30% of the speed of light!” says Maciek Wielgus of the Max Planck Institute for Radio Astronomy in Bonn, Germany, who led the study published today in Astronomy & Astrophysics.

The observations were made with ALMA in the Chilean Andes—a radio telescope co-owned by the European Southern Observatory (ESO)—during a campaign by the Event Horizon Telescope (EHT) Collaboration to image black holes. In April 2017 the EHT linked together eight existing radio telescopes worldwide, including ALMA, resulting in the recently released first ever image of Sagittarius A*. To calibrate the EHT data, Wielgus and his colleagues, who are members of the EHT Collaboration, used ALMA data recorded simultaneously with the EHT observations of Sagittarius A*. To the team's surprise, there were more clues to the nature of the black hole hidden in the ALMA-only measurements.

By chance, some of the observations were done shortly after a burst or flare of X-ray energy was emitted from the center of our galaxy, which was spotted by NASA’s Chandra Space Telescope. These kinds of flares, previously observed with X-ray and infrared telescopes, are thought to be associated with so-called ‘hot spots’, hot gas bubbles that orbit very fast and close to the black hole. 

“What is really new and interesting is that such flares were so far only clearly present in X-ray and infrared observations of Sagittarius A*. Here we see for the first time a very strong indication that orbiting hot spots are also present in radio observations,” says Wielgus, who is also affiliated with the Nicolaus Copernicus Astronomical Center, Poland and the Black Hole Initiative at Harvard University, USA. 

“Perhaps these hot spots detected at infrared wavelengths are a manifestation of the same physical phenomenon: as infrared-emitting hot spots cool down, they become visible at longer wavelengths, like the ones observed by ALMA and the EHT,” adds Jesse Vos, a PhD student at Radboud University, the Netherlands, who was also involved in this study.

The flares were long thought to originate from magnetic interactions in the very hot gas orbiting very close to Sagittarius A*, and the new findings support this idea. “Now we find strong evidence for a magnetic origin of these flares and our observations give us a clue about the geometry of the process. The new data are extremely helpful for building a theoretical interpretation of these events,” says co-author Monika Mościbrodzka from Radboud University.

ALMA allows astronomers to study polarized radio emission from Sagittarius A*, which can be used to unveil the black hole’s magnetic field. The team used these observations together with theoretical models to learn more about the formation of the hot spot and the environment it is embedded in, including the magnetic field around Sagittarius A*. Their research provides stronger constraints on the shape of this magnetic field than previous observations, helping astronomers uncover the nature of our black hole and its surroundings.

The observations confirm some of the previous discoveries made by the GRAVITY instrument at ESO’s Very Large Telescope (VLT), which observes in the infrared. The data from GRAVITY and ALMA both suggest the flare originates in a clump of gas swirling around the black hole at about 30% of the speed of light in a clockwise direction in the sky, with the orbit of the hot spot being nearly face-on.

“In the future we should be able to track hot spots across frequencies using coordinated multiwavelength observations with both GRAVITY and ALMA—the success of such an endeavor would be a true milestone for our understanding of the physics of flares in the Galactic center,” says Ivan Marti-Vidal of the University of València in Spain, co-author of the study.

The team is also hoping to be able to directly observe the orbiting gas clumps with the EHT, to probe ever closer to the black hole and learn more about it. “Hopefully, one day, we will be comfortable saying that we ‘know’ what is going on in Sagittarius A*,” Wielgus concludes.


Credit: EHT Collaboration, European Southern Observatory (ESO)/M. Kornmesser (Acknowledgment: M. Wielgus)

Release Date: September 22, 2022


#NASA #ESO #ALMA #EHT #Astronomy #Space #Science #GasBubble #BlackHole #SagittariusA #SagittariusAAsterisk #MilkyWay #Galaxy #Cosmos #Universe #Telescope #Chile #Europe #Infographic #STEM #Education

Touring an Enigmatic Astronomical Explosion | Hubble

Touring 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/Hubble & NASA, R. Sahai

Duration: 30 seconds

Release Date: September 21, 2022


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

Wednesday, September 21, 2022

Orbital Views of Expedition 68 Soyuz Rocket Launch | International Space Station

Orbital Views of Expedition 68 Soyuz Rocket Launch | International Space Station


European Space Agency (ESA) astronaut Samantha Cristoforetti of Italy shared orbital views from the International Space Station of the Expedition 68 Soyuz MS-22 rocket launch with astronaut Frank Rubio of NASA, and cosmonauts Sergey Prokopyev and Dmitri Petelin of Roscosmos (Russia) onboard. Launch occurred Wednesday, Sept. 21, 2022,  at 13:54 UTC (18:54 local time, 09:54 EDT) from the Baikonur Cosmodrome in Kazakhstan. Rubio, Prokopyev, and Petelin will spend approximately six months on the orbital complex, returning to Earth in March 2023. 

Samantha sent an accompanying message stating: "We had a spectacular view of the Soyuz launch! Sergey, Dmitry and Frank will come knocking on our door in just a couple of hours . . . looking forward to welcoming them to their new home!"

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

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: Samantha Cristoforetti/ESA/NASA-JSC

Release Date: September 21, 2022


#NASA #ISS #Earth #Science #Roscomos #Роскосмос #Soyuz #Rocket #Launch #SoyuzMS22 #Spacecraft #Cosmonauts #SergeyProkopyev #DmitriPetelin #Russia #Россия #Astronauts #SamanthaCristoforetti #FrankRubio #UnitedStates #BaikonurCosmodrome #Kazakhstan #Қазақстан #Human #Spaceflight #Expedition68 #Photography #STEM #Education

Expedition 68 Soyuz MS-22 Spacecraft Docking | International Space Station

Expedition 68 Soyuz MS-22 Spacecraft Docking | International Space Station

The Expedition 68 Soyuz MS-22 spacecraft autonomously docked to the Rassvet module of the International Space Station (ISS) on September 21, 2022, at 17:06 UTC (13:06 EDT). The Soyuz MS-22 spacecraft, with Roscosmos (Russia) cosmonauts Sergey Prokopyev, Dmitri Petelin and NASA astronaut Frank Rubio, opened the hatch to the station at 3:34 p.m. EDT.

The arrival of three new crew members to the existing seven people already aboard for Expedition 67 temporarily increases the station’s population to 10.

Roscosmos cosmonauts Oleg Artemyev, Denis Matveev, and Sergey Korsakov will return to Earth Sept. 29 on the Soyuz MS-21 spacecraft, which is currently docked at the International Space Station, for a parachute-assisted landing on the Kazakh steppe.

Expedition 67 astronauts Bob Hines, Kjell Lindgren, and Jessica Watkins of NASA and astronaut Samantha Cristoforetti of the European Space Agency (ESA) have been aboard since arriving April 27, 2022, on the SpaceX Dragon Freedom. Freedom and its crew are currently planned to return early-to-mid October.

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/Roscosmos

Acknowledgement: SciNews

Duration: 5 minutes

Release Date: September 21, 2022


#NASA #ISS #Earth #Science #Roscomos #Роскосмос #Soyuz #Союз #СоюзMS22 #SoyuzMS22 #Spacecraft #Docking #Cosmonauts #Commander #SergeyProkopyev #DmitriPetelin #Russia #Россия #Astronaut #FrankRubio #UnitedStates #JSC #Human #Spaceflight #Expedition68 #STEM #Education #HD #Video

Expedition 68 Crew Photos: Prelaunch | International Space Station

Expedition 68 Crew Photos: Prelaunch | International Space Station

NASA astronaut Frank Rubio (left), Roscosmos cosmonaut Sergey Prokopyev (center) and Roscosmos cosmonaut Dmitri Petelin (right) in front of their Soyuz MS-22 spacecraft

NASA astronaut Frank Rubio left Roscosmos cosmonaut Sergey Prokopyev center and Roscosmos cosmonaut Dmitri Petelin right complete training preparations in front of their Soyuz MS 22 spacecraft

NASA astronaut Frank Rubio (left), Roscosmos cosmonaut Sergey Prokopyev (center) and Roscosmos cosmonaut Dmitri Petelin (right)

NASA astronaut Frank Rubio undergoes preflight spacesuit fit checkouts

NASA astronaut Frank Rubio is seated in front of the Soyuz MS-22 spacecraft

NASA astronaut Frank Rubio performs preflight checkouts in the Soyuz MS-22 spacecraft

Soyuz MS-22 spacecraft in Integration Facility at the Baikonur Cosmodrome

Soyuz MS-22 spacecraft in Integration Facility at the Baikonur Cosmodrome


At the Baikonur Cosmodrome in Kazakhstan, NASA astronaut Frank Rubio, Roscosmos cosmonaut Sergey Prokopyev and Roscosmos cosmonaut Dmitri Petelin completed training preparations as they prepared for their launch on Sept. 21, 2022, for a six-month mission on the International Space Station. The Soyuz spacecraft bears the name of Konstantin Tsiolkovsky, the “father” of cosmonautics. 


Credit: NASA/Victor Zelentsov

Release Date: September 7, 2022


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

Expedition 68 Soyuz Rocket Launch in Kazakhstan | International Space Station

Expedition 68 Soyuz Rocket Launch in Kazakhstan | International Space Station






The Soyuz MS-22 rocket launched to the International Space Station with Expedition 68 astronaut Frank Rubio of NASA, and cosmonauts Sergey Prokopyev and Dmitri Petelin of Roscosmos (Russia) onboard, Wednesday, Sept. 21, 2022,  at 13:54 UTC (18:54 local time, 09:54 EDT) from the Baikonur Cosmodrome in Kazakhstan. Rubio, Prokopyev, and Petelin will spend approximately six months on the orbital complex, returning to Earth in March 2023. 

Astronaut Frank Rubio’s Official NASA Biography:

https://www.nasa.gov/astronauts/biographies/frank-rubio/biography/

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/Bill Ingalls

Release Date: September 21, 2022


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

Expedition 68 Soyuz MS-22 Rocket Launch | International Space Station

Expedition 68 Soyuz MS-22 Rocket Launch | International Space Station

NASA astronaut Frank Rubio, a member of NASA's 2017 astronaut candidate class, began his first mission to space this Wednesday, Sept. 21, 2022,  at 13:54 UTC (18:54 local time, 09:54 EDT). Rubio lifted off from the Baikonur Cosmodrome in Kazakhstan aboard the Soyuz MS-22 spacecraft, alongside Roscosmos cosmonauts Sergey Prokopyev and Dmitri Petelin. They later docked at the Rassvet module of the International Space Station (ISS).

Rubio, Prokopyev, and Petelin will spend approximately six months on the orbital complex, returning to Earth in March 2023. 

Astronaut Frank Rubio’s Official NASA Biography:

https://www.nasa.gov/astronauts/biographies/frank-rubio/biography/

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/Roscosmos

Acknowledgement: SciNews

Duration: 6 minutes, 21 seconds

Release Date: September 21, 2022


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

Expedition 68 Soyuz Rocket Launch in Kazakhstan | International Space Station

Expedition 68 Soyuz Rocket Launch in Kazakhstan | International Space Station

Expedition 68 crew members Dmitri Petelin of Roscosmos, top, Frank Rubio of NASA, and Sergey  Prokopyev of Roscosmos, bottom, wave farewell 



The Soyuz MS-22 rocket launched to the International Space Station with Expedition 68 astronaut Frank Rubio of NASA, and cosmonauts Sergey Prokopyev and Dmitri Petelin of Roscosmos onboard, Wednesday, Sept. 21, 2022, from the Baikonur Cosmodrome in Kazakhstan. Rubio, Prokopyev, and Petelin will spend approximately six months on the orbital complex, returning to Earth in March 2023. 

Astronaut Frank Rubio’s Official NASA Biography:

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/Bill Ingalls

Release Date: September 21, 2022


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

Pan across Planet Neptune, Its Rings & Moons | James Webb Space Telescope

Pan across Planet Neptune, Its Rings & Moons | James Webb Space Telescope

The NASA/ESA/CSA James Webb Space Telescope is showing off its capabilities closer to home with its first image of Neptune. Not only has Webb captured the clearest view of this peculiar planet’s rings in more than 30 years, but its cameras are also revealing the ice giant in a whole new light.

The James Webb Space Telescope is the world's premier space science observatory. Webb will solve mysteries in our solar system, look beyond to distant worlds around other stars, and probe the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, the European Space Agency (ESA) and the Canadian Space Agency (CSA).


Credit: NASA, European Space Agency (ESA), Canadian Space Agency (CSA) and Space Telescope Science Institute (STScI), N. Bartmann 

Duration: 30 seconds

Release Date: September 21, 2022


#NASA #ESA #Astronomy #Space #Science #Neptune #Planet #Rings #Atmosphere #Moons #Triton #NIRCam #Infrared #JamesWebb #WebbTelescope #JWST #SpaceTelescope #SolarSystem #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #STEM #Education #HD #Video

New Views of Planet Neptune, Its Rings & Moons | James Webb Space Telescope

Planet Neptune, Its Rings & Moons: New Views | James Webb Space Telescope

Space Sparks Episode 6: Watch this Space Sparks episode to learn more about the first views of Neptune from the NASA/ESA/CSA James Webb Space Telescope.

The James Webb Space Telescope is the world's premier space science observatory. Webb will solve mysteries in our solar system, look beyond to distant worlds around other stars, and probe the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, the European Space Agency (ESA) and the Canadian Space Agency (CSA).


Credits:

Directed by: Bethany Downer and Nico Bartmann  

Editing: Nico Bartmann  

Web and technical support: Enciso Systems  

Written by: Bethany Downer  

Footage and photos: NASA, European Space Agency (ESA), Canadian Space Agency (CSA), Space Telescope Science Institute (STScI), N. Bartmann

Duration: 2 minutes

Release Date: September 21, 2022


#NASA #ESA #Astronomy #Space #Science #Neptune #Planet #Rings #Atmosphere #Moons #Triton #NIRCam #Infrared #JamesWebb #WebbTelescope #JWST #SpaceTelescope #SolarSystem #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #STEM #Education #HD #Video

Planet Neptune & Moon Triton: Wide-field View | James Webb Space Telescope

Planet Neptune & Moon Triton: Wide-field View | James Webb Space Telescope

In this image by Webb’s Near-Infrared Camera (NIRCam), a smattering of hundreds of background galaxies, varying in size and shape, appear alongside the Neptune system.

Neptune, when compared to Earth, is a big planet. If Earth were the size of a nickel, Neptune would be as big as a basketball. In most portraits, the outer planets of our solar system reflect this otherworldly size. However, Neptune appears relatively small in a wide field of the vast universe.

Towards the bottom left of this image, a barred spiral galaxy comes into focus. Scientists say this particular galaxy, previously unexplored in detail, is about 1,200 million light years away. These types of galaxies at this relative difference are typically dominated by young stars that appear blueish in these wavelengths.

The James Webb Space Telescope is the world's premier space science observatory. Webb will solve mysteries in our solar system, look beyond to distant worlds around other stars, and probe the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, the European Space Agency (ESA) and the Canadian Space Agency (CSA).


Credit: NASA, European Space Agency (ESA), Canadian Space Agency (CSA) and Space Telescope Science Institute (STScI)

Release Date: September 21, 2022


#NASA #ESA #Astronomy #Space #Science #Neptune #Planet #Rings #Atmosphere #Moons #Triton #NIRCam #Infrared #JamesWebb #WebbTelescope #JWST #SpaceTelescope #SolarSystem #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #STEM #Education

Planet Neptune with Triton and Six More Moons | James Webb Space Telescope

Planet Neptune with Triton and Six More Moons | James Webb Space Telescope


In this version of Webb’s Near-Infrared Camera (NIRCam) image of Neptune, the planet’s visible moons are labeled. Neptune has 14 known satellites, and seven of them are visible in this image.

Triton, the bright spot of light in the upper left of this image, far outshines Neptune because the planet’s atmosphere is darkened by methane absorption wavelengths captured by Webb. Triton reflects an average of 70 percent of the sunlight that hits it. Triton, which orbits Neptune in a backward orbit, is suspected to have originally been a Kuiper belt object (KBO) that was gravitationally captured by Neptune.

The James Webb Space Telescope is the world's premier space science observatory. Webb will solve mysteries in our solar system, look beyond to distant worlds around other stars, and probe the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners,  European Space Agency (ESA) and the Canadian Space Agency (CSA).


Credit: NASA, European Space Agency (ESA), Canadian Space Agency (CSA) and Space Telescope Science Institute (STScI)

Release Date: September 21, 2022


#NASA #ESA #Astronomy #Space #Science #Neptune #Planet #Rings #Atmosphere #Moons #Triton #NIRCam #Infrared #JamesWebb #WebbTelescope #JWST #SpaceTelescope #SolarSystem #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #Infographic #STEM #Education

Neptune’s Rings: Clearest View in Decades | James Webb Space Telescope

Neptune’s Rings: Clearest View in Decades | James Webb Space Telescope

Infrared Observations Tease Out Never Seen Atmospheric and Ring Details

The NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope is showing off its capabilities closer to home with its first image of Neptune. Not only has Webb captured the clearest view of this peculiar planet’s rings in more than 30 years, but its cameras are also revealing the ice giant in a whole new light.

Image Description: Webb’s Near-Infrared Camera (NIRCam) image of Neptune, taken on July 12, 2022. The most prominent features of Neptune’s atmosphere in this image are a series of bright patches in the planet’s southern hemisphere that represent high-altitude methane-ice clouds. More subtly, a thin line of brightness circling the planet’s equator could be a visual signature of global atmospheric circulation that powers Neptune’s winds and storms. Additionally, for the first time, Webb has teased out a continuous band of high-latitude clouds surrounding a previously-known vortex at Neptune’s southern pole.

Neptune lurks in one of the dimmest parts of our solar system. With its complex rings, bizarre moon, Triton, and roaring winds faster than the speed of sound here on Earth, Neptune has long perplexed astronomers. Just one spacecraft, Voyager 2, has ever visited this far-flung planet, and observations from both space- and ground-based telescopes over the years have tracked the many turbulent storms.

Most striking in Webb’s new image is the crisp view of the planet’s rings—some of which have not been detected since NASA’s Voyager 2 became the first spacecraft to observe Neptune during its flyby in 1989. In addition to several bright, narrow rings, the Webb image clearly shows Neptune’s fainter dust bands. 

“It has been three decades since we last saw those faint, dusty bands, and this is the first time we’ve seen them in the infrared,” notes Heidi Hammel, a Neptune system expert and interdisciplinary scientist for Webb. Webb’s extremely stable and precise image quality permits these very faint rings to be detected so close to Neptune.

Neptune has fascinated researchers since its discovery in 1846. Located 30 times farther from the Sun than Earth, Neptune orbits in the remote, dark region of the outer solar system. At that extreme distance, the Sun is so small and faint that high noon on Neptune is similar to a dim twilight on Earth. 

This planet is characterized as an ice giant due to the chemical make-up of its interior. Compared to the gas giants, Jupiter and Saturn, Neptune is much richer in elements heavier than hydrogen and helium. This is readily apparent in Neptune’s signature blue appearance in Hubble Space Telescope images at visible wavelengths, caused by small amounts of gaseous methane. 

Webb’s Near-Infrared Camera (NIRCam) images objects in the near-infrared range from 0.6 to 5 microns, so Neptune does not appear blue to Webb. In fact, the methane gas so strongly absorbs red and infrared light that the planet is quite dark at these near-infrared wavelengths, except where high-altitude clouds are present. Such methane-ice clouds are prominent as bright streaks and spots, which reflect sunlight before it is absorbed by methane gas. Images from other observatories, including the Hubble Space Telescope and the W.M. Keck Observatory, have recorded these rapidly evolving cloud features over the years. 

More subtly, a thin line of brightness circling the planet’s equator could be a visual signature of global atmospheric circulation that powers Neptune’s winds and storms. The atmosphere descends and warms at the equator, and thus glows at infrared wavelengths more than the surrounding, cooler gases. 

Neptune’s 164-year orbit means its northern pole, at the top of this image, is just out of view for astronomers, but the Webb images hint at an intriguing brightness in that area. A previously-known vortex at the southern pole is evident in Webb’s view, but for the first time Webb has revealed a continuous band of high-latitude clouds surrounding it.

Webb also captured seven of Neptune’s 14 known moons. 

The James Webb Space Telescope is the world's premier space science observatory. Webb will solve mysteries in our solar system, look beyond to distant worlds around other stars, and probe the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, the European Space Agency (ESA) and the Canadian Space Agency (CSA).


Credits: NASA, ESA, CSA, Space Telescope Science Institute (STScI)

Image Date: July 12, 2022

Release Date: September 21, 2022


#NASA #ESA #Astronomy #Space #Science #Neptune #Planet #Rings #Atmosphere #Moons #NIRCam #Infrared #JamesWebb #WebbTelescope #JWST #SpaceTelescope #SolarSystem #Cosmos #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #STEM #Education

A Long-dead Star: Supernova Remnant DEM L316A | Hubble

A Long-dead Star: Supernova Remnant DEM L316A | Hubble


This NASA/European Space Agency Hubble Space Telescope image captures the remnants of a long-dead star. These rippling wisps of ionized gas, named DEM L316A, are located some 160,000 light-years away within one of the Milky Way’s closest galactic neighbors—the Large Magellanic Cloud (LMC).

Distance: 150,000 light years

The explosion that formed DEM L316A was an example of an especially energetic and bright variety of supernova, known as a Type Ia. Such supernova events are thought to occur when a white dwarf star steals more material than it can handle from a nearby companion, and becomes unbalanced. The result is a spectacular release of energy in the form of a bright, violent explosion, which ejects the star’s outer layers into the surrounding space at immense speeds. As this expelled gas travels through the interstellar material, it heats it up and ionize it, producing the faint glow that Hubble’s Wide Field Camera 3 has captured here.

The LMC orbits the Milky Way as a satellite galaxy and is the fourth largest in our group of galaxies, the Local Group.


Credit: European Space Agency/Hubble & NASA, Y. Chu

Release Date: July 25, 2016


#NASA #ESA #Hubble #Astronomy #Space #Science #Stars #Supernova #SupernovaRemnant #DEML316A #Nebula #Dorado #Constellation #MilkyWay #Galaxy #Cosmos #Universe #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #STEM #Education