Monday, August 15, 2022

Pan across Supernova Remnant N103B | Hubble

Pan across Supernova Remnant N103B | Hubble

The supernova remnant N103B can be found in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. The elliptical-shaped gas cloud is the leftover of the past explosion and astronomers investigate it in the hope of finding the remains of the exploded star’s companion.

Distance: 150,000 light years

This pan shows N103B as well as the outskirts of the star cluster NGC 1850.


Credit: European Space Agency (ESA)/Hubble

Duration: 50 seconds

Release Date: March 30, 2017


#NASA #ESA #Astronomy #Space #Hubble #SupernovaRemnant #N103B #TypeIa #SNR0509687 #Star #StarCluster #NGC1850 #Dorado #Constellation #LargeMagellanicCloud #LMC #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Zoom into Supernova Remnant N103B | Hubble

Zoom into Supernova Remnant N103B | Hubble

This video starts with a wide-field view of the night sky, as seen from the ground, displaying the Large and the Small Magellanic Clouds. It zooms in on the Large Magellanic Cloud, a satellite galaxy of the Milky Way, and onto the star cluster NGC 1850. Just next to the bright cluster Hubble observed the supernova remnant N103B. In the remnant of this supernova astronomers hope to find the surviving star of a supernova explosion.

Distance: 150,000 light years


Credit: European Space Agency/Hubble, Nick Risinger, R. Gendler & European Southern Observatory (ESO)  

Duration: 50 seconds

Release Date: March 30, 2017


#NASA #ESA #Astronomy #Space #Hubble #SupernovaRemnant #N103B #TypeIa #SNR0509687 #Star #StarCluster #NGC1850 #Dorado #Constellation #LargeMagellanicCloud #LMC #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Supernova Remnant N103B in Large Magellanic Cloud | Hubble

Supernova Remnant N103B in Large Magellanic Cloud | Hubble


This image, taken with the NASA/European Space Agency Hubble Space Telescope, shows the supernova remnant SNR 0509-68.7, also known as N103B (top of the image). N103B was a Type Ia supernova, located in the Large Magellanic Cloud—a neighboring galaxy of the Milky Way. Owing to its relative proximity to Earth, astronomers observe the remnant to search for a potential stellar survivor of the explosion.

Distance: 150,000 light years

The orange-red filaments visible in the image show the shock fronts of the supernova explosion. These filaments allow astronomers to calculate the original center of the explosion. The filaments also show that the explosion is no longer expanding as a sphere, but is elliptical in shape. Astronomers assume that part of material ejected by the explosion hit a denser cloud of interstellar material, which slowed its speed. The shell of expanding material being open to one side supports this idea.

The gas in the lower half of the image and the dense concentration of stars in the lower left are the outskirts of the star cluster NGC 1850.


Credit: European Space Agency/Hubble, NASA

Release Date: March 30, 2017


#NASA #ESA #Astronomy #Space #Hubble #SupernovaRemnant #N103B #TypeIa #SNR0509687 #Star #StarCluster #NGC1850 #Dorado #Constellation #LargeMagellanicCloud #LMC #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

The Moon above the Pacific Ocean | International Space Station

The Moon above the Pacific Ocean | International Space Station


The waxing gibbous Moon is pictured from the International Space Station as it orbited 260 miles above the Pacific Ocean south of Alaska's Aleutian Islands.

Expedition 67 Crew

Commander Oleg Artemyev (Russia)

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

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

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

An international partnership of space agencies provides and operates the elements of the  International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada. The ISS has been the most politically complex space exploration program ever undertaken.

Learn more about the important research being operated on Station:

For more information about STEM on Station:


Credit: NASA's Johnson Space Center (JSC)

Image Date: August 9, 2022


#NASA #Space #Earth #ISS #Moon #UnitedStates #Alaska #AleutianIslands #PacificOcean #Astronauts #Europe #Italia #Italy #Canada #Japan #日本 #Russia #Россия #Science #Research #International #Expedition67 #STEM #Education

NASA’s Europa Clipper Spacecraft Kicks Assembly Into High Gear | JPL

NASA’s Europa Clipper Spacecraft Kicks Assembly Into High Gear | JPL


The Europa Clipper spacecraft will occupy the main production facility of NASA’s Jet Propulsion Laboratory (JPL) as it prepares for its 2024 launch to Jupiter’s moon Europa.

Aug. 15, 2022: The core of NASA’s Europa Clipper spacecraft has taken center stage in the Spacecraft Assembly Facility at the agency’s Jet Propulsion Laboratory in Southern California. Standing 10 feet (3 meters) high and 5 feet (1.5 meters) wide, the craft’s main body will for the next two years be the focus of attention in the facility’s ultra-hygienic High Bay 1 as engineers and technicians assemble the spacecraft for its launch to Jupiter’s moon Europa in October 2024.

Scientists believe the ice-enveloped moon harbors a vast internal ocean that may have conditions suitable for supporting life. During nearly 50 flybys of Europa, the spacecraft’s suite of science instruments will gather data on the moon’s atmosphere, surface, and interior—information that scientists will use to gauge the depth and salinity of the ocean, the thickness of the ice crust, and potential plumes that may be venting subsurface water into space.

Several of Europa Clipper’s science instruments already have been completed and will be installed on the spacecraft at JPL. Most recently, the plasma-detection instrument, called the Plasma Instrument for Magnetic Sounding, and the Europa Imaging System wide-angle camera arrived from the Johns Hopkins Applied Physics Laboratory (APL), in Laurel, Maryland. The thermal-emission imaging instrument, called E-THEMIS, and the ultraviolet spectrograph, Europa-UVS, have already been installed on the spacecraft’s nadir deck, which will support many of the instrument sensors by stabilizing them to ensure they are oriented correctly.

Fabricated at JPL, this key piece of hardware will soon move into the Spacecraft Assembly Facility’s High Bay 1, the same clean room where historic missions such as Galileo, Cassini, and all of NASA’s Mars rovers were built.

Also moving soon to High Bay 1 will be the aluminum electronics vault, which will be bolted to the main body of the spacecraft, protecting the electronics inside from Jupiter’s intense radiation. The electronics enable Europa Clipper’s computer to communicate with the spacecraft’s antennae, science instruments, and the subsystems that will keep them alive.

Bright copper cabling snaking around the orbiter’s aluminum core contains thousands of wires and connectors handcrafted at APL. If placed end to end, the cabling would stretch almost 2,100 feet (640 meters)—enough to wrap around a U.S. football field twice.

Inside the core are Europa Clipper’s two propulsion tanks. The fuel and oxidizer they will hold will flow to an array of 24 engines, where they will create a controlled chemical reaction to produce thrust in deep space.

By the end of 2022, most of the flight hardware and the remainder of the science instruments are expected to be complete. Then, the next steps will be a wide variety of tests as the spacecraft moves toward its 2024 launch period. After traveling for nearly six years and over 1.8 billion miles (2.9 billion kilometers), it will achieve orbit around Jupiter in 2030.

More About the Mission

Missions such as Europa Clipper contribute to the field of astrobiology, the interdisciplinary research field that studies the conditions of distant worlds that could harbor life as we know it. While Europa Clipper is not a life-detection mission, it will conduct a detailed exploration of Europa and investigate whether the icy moon, with its subsurface ocean, has the capability to support life. Understanding Europa’s habitability will help scientists better understand how life developed on Earth and the potential for finding life beyond our planet.

Managed by Caltech in Pasadena, California, JPL leads the development of the Europa Clipper mission in partnership with APL for NASA’s Science Mission Directorate in Washington. APL designed the main spacecraft body in collaboration with JPL and NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The Planetary Missions Program Office at NASA’s Marshall Space Flight Center in Huntsville, Alabama, executes program management of the Europa Clipper mission.

More information about Europa can be found here: europa.nasa.gov


Credit: NASA/JPL

Release Date: August 15, 2022


#NASA #Astronomy #Space #Science #Jupiter #Europa #Moon #Ocean #Astrobiology #Biosignatures #Habitability #Radiation #EuropaClipper #Spacecraft #SolarSystem #Exploration #APL #Marshall #MSFC #JPL #California #UnitedStates #STEM #Education

How NASA Moves a Spacecraft: Europa Clipper Arrives in Its New Home | JPL

How NASA Moves a Spacecraft: Europa Clipper Arrives in Its New Home | JPL

This time-lapse video follows NASA’s Europa Clipper spacecraft as it moves into the storied High Bay 1 clean room from a smaller clean room at the agency’s Jet Propulsion Laboratory in Southern California. The multiday transport between rooms at the Lab’s Spacecraft Assembly Facility and the unwrapping and positioning of the spacecraft core required thorough planning and careful choreography. 

In this new location, engineers and technicians will complete assembly of the spacecraft in preparation for its launch to Jupiter’s moon Europa in October 2024. 

Scientists believe the ice-enveloped moon harbors a vast internal ocean that may have conditions suitable for supporting life. During nearly 50 flybys of Europa, the spacecraft’s suite of science instruments will gather data on the moon’s atmosphere, surface, and interior—information that scientists will use to gauge the depth and salinity of the ocean, the thickness of the ice crust, and potential plumes that may be venting subsurface water into space.

Managed by Caltech in Pasadena, California, JPL leads the development of the Europa Clipper mission in partnership with Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland.

For more information about Europa, visit: europa.nasa.gov

Download Europa Clipper Ocean World poster: go.nasa.gov/3Gsjzt5


Credit: NASA's Jet Propulsion Laboratory (JPL)/Caltech

Duration: 46 seconds

Release Date: August 15, 2022


#NASA #Astronomy #Space #Science #Jupiter #Europa #Moon #Ocean #Astrobiology #Biosignatures #Habitability #Radiation #EuropaClipper #Spacecraft #SolarSystem #Exploration #APL #Marshall #MSFC #JPL #Pasadena #California #UnitedStates #STEM #Education #HD #Video

The Cometary Globule CG4: Wide-field View

The Cometary Globule CG4: Wide-field View | ESO


This wide-field image shows a rich region of the sky in the constellation of Puppis (The Poop Deck). At the center lies the strange cometary globule CG4. Other interesting objects are also seen, including several much more distant spiral galaxies. This color view was produced from images forming part of the Digitized Sky Survey 2.

Distance: 1,300 light years


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

Release Date: January 28, 2015


#NASA #ESO #Astronomy #Space #Science #Galaxies #Stars #Nebula #CometaryGlobule #CometaryGlobuleCG4 #Puppis #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Telescope #VLT #LaSillaObservatory #Chile #Europe #STEM #Education

Panning over The Cometary Globule CG4

Panning over The Cometary Globule CG4 | ESO

The cometary globule CG4 glows menacingly, like the gaping mouth of a gigantic celestial creature, in this pan video based on an image from the European Southern Observatory’s Very Large Telescope. What looks huge and bright in this image is actually a faint nebula and not easy to observe. The exact nature of CG4 remains a mystery.

Distance: 1,300 light years


Credit: European Southern Observatory (ESO)

Duration: 50 seconds

Release Date: February 9, 2015


#NASA #ESO #Astronomy #Space #Science #Stars #Nebula #CometaryGlobule #CometaryGlobuleCG4 #Puppis #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Telescope #VLT #LaSillaObservatory #Chile #Europe #STEM #Education #HD #Video

Zooming in on Cometary Globule CG4 | ESO

Zooming in on Cometary Globule CG4 | ESO

This zoom video sequence goes from a wide view of the southern Milky Way deep into the constellation of Puppis close to the site of the Vela supernova remnant. The final view shows a new close-up view of the cometary globule CG4. It glows menacingly, like the gaping mouth of a gigantic celestial creature, in this this new image from the European Southern Observatory’s Very Large Telescope (VLT). What looks huge and bright in this image is actually a faint nebula and not easy to observe. The exact nature of CG4 remains a mystery.

Distance: 1,300 light years


Credit: European Southern Observatory (ESO)/J.Perez/Digitized Sky Survey 2/N. Risinger

Duration: 50 seconds

Release Date: February 9, 2015


#NASA #ESO #Astronomy #Space #Science #Stars #Nebula #CometaryGlobule #CometaryGlobuleCG4 #Puppis #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Telescope #VLT #LaSillaObservatory #Chile #Europe #STEM #Education #HD #Video

The Cometary Globule CG4 | ESO

The Cometary Globule CG4 | ESO

Like the gaping mouth of a gigantic celestial creature, the cometary globule CG4 glows menacingly in this image from the European Southern Observatory’s Very Large Telescope (VLT). Although it looks huge and bright in this image, it is actually a faint nebula and not easy to observe. The exact nature of CG4 remains a mystery.


Credit: European Southern Observatory (ESO)

Release Date: January 28, 2015


#NASA #ESO #Astronomy #Space #Science #Stars #Nebula #CometaryGlobule #CometaryGlobuleCG4 #Puppis #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Telescope #VLT #LaSillaObservatory #Chile #Europe #STEM #Education

ALMA Explores Debris Disc Around Fomalhaut Star: A New Solar System? | ESO

ALMA Explores Debris Disc Around Fomalhaut Star: A New Solar System? | ESO

Fomalhaut is one of the brightest stars in the sky. At roughly 25 light-years away the star lies especially close to us, and can be seen shining brightly in the constellation of Piscis Austrinus (The Southern Fish). This image from the Atacama Large Millimeter/submillimeter Array (ALMA) shows Fomalhaut (center) encircled by a ring of dusty debris. This was the first time a scene like this was captured at such a high resolution and sensitivity at millimeter wavelengths.

Fomalhaut’s disc comprises a mix of cosmic dust and gas from comets in the Fomalhaut system (exocomets), released as the exocomets graze past and smash into one another. This turbulent environment resembles an early period in our own Solar System known as the Late Heavy Bombardment, which occurred approximately four billions years ago. This era saw huge numbers of rocky objects hurtle into the inner Solar System and collide with the young terrestrial planets, including Earth, where they formed a myriad of impact craters—many of which remain visible today on the surfaces of planets such as Mercury and Mars.

Fomalhaut is known to be surrounded by several discs of debris—the one visible in this ALMA image is the outermost one. The ring is approximately 20 billion kilometers from the central star and about 2 billion kilometers wide. Such a relative narrow, eccentric disc can only be produced by the gravitational influence of planets in the system, like Jupiter’s gravitational influence on our asteroid belt. 


Credit: ALMA (ESO/NAOJ/NRAO)/L. Matrà/M. A. MacGregor

Release Date: May 22, 2017


#NASA #ESO #ALMA #Astronomy #Space #Science #Star #Ring #Fomalhaut #PiscisAustrinus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Telescope #Chile #Europe #STEM #Education

The Mysteries of Fomalhaut b | Hubble

The Mysteries of Fomalhaut b | Hubble

Data from the NASA/European Space Agency Hubble Space Telescope have revealed an expanding cloud of dust that was likely produced in a collision between two large bodies orbiting the bright nearby star Fomalhaut.


Credit:

Directed by: Bethany Downer and Nico Bartmann  

Editing: Nico Bartmann 

Web and technical support: Gurvan Bazin and Raquel Yumi Shida

Written by: Bethany Downer  

Footage and photos: ESA, NASA, Hubble, M. Kornmesser, P. Kalas, Digitized Sky Survey 2, A. Gáspár and G. Rieke (University of Arizona)

Duration: 1 minute, 36 seconds

Release Date: April 20, 2020


#NASA #ESA #Hubble #Astronomy #Space #Science #Star #Fomalhautb #Fomalhaut #PiscisAustrinus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #SpaceTelescope #UnitedStates #GSFC #Europe #STEM #Education #HD #Video

Zooming in on Fomalhaut Star and its Dusty Disc | ESO

Zooming in on Fomalhaut Star and its Dusty Disc | ESO

This video sequence starts with a wide-field view of the sky around the star Fomalhaut in the constellation of Piscis Austrinus (The Southern Fish). Fomalhaut is the brightest star in the constellation and one of the brightest stars known to have an orbiting planet. It lies about 25 light-years from the Earth and is surrounded by a huge disc of dust. 

The final view of this video shows a new Atacama Large Millimeter Array (ALMA) image of the disc (orange) and the new results from ALMA have given astronomers a major breakthrough in understanding a nearby planetary system and provided valuable clues about how such systems form and evolve. 

Note that ALMA has so far only observed a part of the ring. The underlying blue picture shows an earlier picture obtained by the NASA/ESA Hubble Space Telescope.


Credit: ALMA - European Southern Observatory/National Astronomical Observatory of Japan (NAOJ)/ National Radio Astronomy Observatory (NRAO)

Visible light image: NASA/European Space Agency Hubble Space Telescope A. Fujii/Digitized Sky Survey 2

Acknowledgment: Davide De Martin (ESA/Hubble)

Duration: 56 seconds

Release Date: April 12, 2012


#NASA #ESO #ESA #Hubble #ALMA #Astronomy #Space #Science #Star #Fomalhaut #PiscisAustrinus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Telescope #Chile #Europe #STEM #Education #HD #Video

The Star Fomalhaut: Wide-field View

The Star Fomalhaut: Wide-field View


This wide-field view shows the sky around the bright star Fomalhaut in the constellation of Piscis Austrinus (The Southern Fish). This picture was created from photographs forming part of the Digitized Sky Survey 2. Fomalhaut lies about 25 light-years from the Earth and is surrounded by a huge disc of dust.


Credit: NASA, European Space Agency (ESA), and the Digitized Sky Survey 2

Acknowledgment: Davide De Martin (ESA/Hubble)

Release Date: April 12, 2012


#NASA #ESO #ESA #Hubble #Astronomy #Space #Science #Star #Fomalhaut #PiscisAustrinus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Telescope #Chile #Europe #STEM #Education

Globular Cluster NGC 6540 | Hubble

Globular Cluster NGC 6540 | Hubble


This scintillating image showcases the globular cluster NGC 6540 in the constellation Sagittarius, which was captured by the NASA/European Space Agency Hubble Space Telescope’s Wide Field Camera 3 and Advanced Camera for Surveys. These two instruments have slightly different fields of view—which determines how large an area of sky each instrument captures. This composite image shows the star-studded area of sky that was captured in both instruments’ field of view. 

NGC 6540 is a globular cluster, a stable, tightly bound multitude of stars. The populations of these clusters can range from tens of thousands to millions of stars, all of which are trapped in a closely-packed group by their mutual gravitational attraction.

Distance: about 17,000 light years

The brightest stars in this image are adorned with prominent cross-shaped patterns of light known as diffraction spikes. These astronomical embellishments are a type of imaging artefact, meaning that they are caused by the structure of Hubble rather than the stars themselves. The path taken by the starlight as it enters the telescope is slightly disturbed by its internal structure, causing bright objects to be surrounded by spikes of light.

Hubble peered into the heart of NGC 6540 to help astronomers measure the ages, shapes, and structures of globular clusters towards the center of the Milky Way. The gas and dust shrouding the center of our galaxy block some of the light from these clusters, as well as subtly changing the colors of their stars. Globular clusters contain insights into the earliest history of the Milky Way, and so studying them can help astronomers understand how our galaxy has evolved.


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

Release Date: August 15, 2022


#NASA #ESA #Astronomy #Space #Hubble #Nebula #Stars #NGC6540 #GlobularCluster #StarCluster #Sagittarius #Constellation #MilkyWay #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

The Medusa Nebula: Wide-field view | ESO

The Medusa Nebula: Wide-field view | ESO


This wide-field view shows the sky around the large but faint planetary nebula known as the Medusa Nebula. The full extent of the object can be seen, as well as many faint stars and, far beyond them, numerous distant galaxies.This picture was created from images forming part of the Digitized Sky Survey 2.

Distance: 1,500 light years


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

Release Date: May 20, 2015


#NASA #ESO #Astronomy #Space #Science #Stars #Abell21 #Sharpless2274 #Nebula #MedusaNebula #Gemini #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Telescope #VLT #LaSillaObservatory #Chile #Europe #STEM #Education