Tuesday, August 16, 2022

Zooming into Galaxy Centaurus A | ESO

Zooming into Galaxy Centaurus A | ESO

This video zoom sequence starts with a broad view of the Milky Way. We close in on a region not far from the plane of a the galaxy and can soon see a strange fuzz with a dark band across it. This is the famous peculiar radio galaxy Centaurus A. The final view shows a very detailed image from the MPG/ESO 2.2-meter telescope at the La Silla Observatory in Chile.

Distance: 13 million light years


Credit: European Southern Observatory (ESO)/Nick Risinger

Duration: 1 minute

Release Date: May 16, 2012


#NASA #ESO #Astronomy #Space #Science #Stars #Galaxy #AGNGalaxy #NGC5128 #CentaurusA #Centaurus #Constellation #Cosmos #Universe #Telescope #VLT #FORS2 #LaSillaObservatory #Chile #Europe #STEM #Education #HD #Video

Radio Galaxy Centaurus A | ESO

Radio Galaxy Centaurus A | ESO


This FORS2 image of Centaurus A, also known as NGC 5128, is an example of how frontier science can be combined with esthetic aspects. This galaxy is a most interesting object for the present attempts to understand active galaxies. It is being investigated by means of observations in all spectral regions, from radio via infrared and optical wavelengths to X- and gamma-rays. It is one of the most extensively studied objects in the southern sky. FORS2, with its large field-of-view and excellent optical resolution, makes it possible to study the global context of the active region in Centaurus A in great detail. Note for instance the great number of massive and luminous blue stars that are well resolved individually, in the upper right and lower left. 

Distance: 13 million light years

Centaurus A is one of the foremost examples of a radio-loud active galactic nucleus (AGN). On images obtained at optical wavelengths, thick dust layers almost completely obscure the galaxy's center. This structure was first reported by Sir John Herschel in 1847. Until 1949, NGC 5128 was thought to be a strange object in the Milky Way, but it was then identified as a powerful radio galaxy and designated Centaurus A. The distance is about 10-13 million light-years (3-4 Mpc) and the apparent visual magnitude is about 8, or 5 times too faint to be seen with the unaided eye.There is strong evidence that Centaurus A is a merger of an elliptical with a spiral galaxy, since elliptical galaxies would not have had enough dust and gas to form the young, blue stars seen along the edges of the dust lane. The core of Centaurus A is the smallest known extragalactic radio source, only 10 light-days across. A jet of high-energy particles from this center is observed in radio and X-ray images. The core probably contains a supermassive black hole with a mass of about 100 million solar masses.

This image is a composite of three exposures in B (300 sec exposure, image quality 0.60 arcsec; here rendered in blue color), V (240 sec, 0.60 arcsec; green) and R (240 sec, 0.55 arcsec; red). 


Credit: European Southern Observatory (ESO)

Release Date: February 8, 2000


#NASA #ESO #Astronomy #Space #Science #Stars #Galaxy #AGNGalaxy #NGC5128 #CentaurusA #Centaurus #Constellation #Cosmos #Universe #Telescope #VLT #FORS2 #LaSillaObservatory #Chile #Europe #STEM #Education

Spiral Galaxy NGC 3621: Wide-field View | ESO

Spiral Galaxy NGC 3621: Wide-field View | ESO


This picture of the spiral galaxy NGC 3621 was taken using the Wide Field Imager (WFI) at the European Southern Observatory’s La Silla Observatory in Chile. NGC 3621 is about 22 million light-years away in the constellation of Hydra (The Sea Snake). It is comparatively bright and can be well seen in moderate-sized telescopes.

The data from the Wide Field Imager on the MPG/ESO 2.2-meter telescope at ESO’s La Silla Observatory in Chile used to make this image were selected from the ESO archive by Joe DePasquale as part of the Hidden Treasures competition.

Distance: 22 million light years


Credit: European Southern Observatory (ESO) and Joe DePasquale

Release Date: February 2, 2011


#NASA #ESO #Astronomy #Space #Science #Stars #Galaxy #NGC3621 #BlackHoles #Hydra #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Telescope #VLT #LaSillaObservatory #Chile #Europe #STEM #Education

Zooming in on Spiral Galaxy NGC 3621 | ESO

Zooming in on Spiral Galaxy NGC 3621 | ESO

Travel 22 million light years to spiral galaxy NGC 3621 in less than 50 seconds!

This zoom sequence starts with a view of the southern parts of the Milky Way. As we zoom in we can see the spiral galaxy NGC 3621, lying about 22 million light-years from us. The final detailed view shows a new image from the MPG/ESO 2.2-meter telescope at ESO's La Silla Observatory in Chile. The data used to make this image were selected from the European Southern Observatory archive by Joe DePasquale as part of the Hidden Treasures competition.


Credit: European Southern Observatory (ESO)

Duration: 50 seconds

Release Date: February 2, 2011


#NASA #ESO #Astronomy #Space #Science #Stars #Galaxy #NGC3621 #BlackHoles #Hydra #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Telescope #VLT #LaSillaObservatory #Chile #Europe #STEM #Education #HD #Video

Galaxy NGC 3621: Full of Surprises & Three Black Holes | ESO

Galaxy NGC 3621: Full of Surprises & Three Black Holes | ESO


This image, from the European Southern Observatory’s Very Large Telescope (VLT), shows a truly remarkable galaxy known as NGC 3621. To begin with, it is a pure-disc galaxy. Like other spirals, it has a flat disc permeated by dark lanes of material and with prominent spiral arms where young stars are forming in clusters (the blue dots seen in the image). But while most spiral galaxies have a central bulge—a large group of old stars packed in a compact, spheroidal region—NGC 3621 does not. In this image, it is clear that there is simply a brightening to the center, but no actual bulge.

Distance: 22 million light years

NGC 3621 is also interesting as it is believed to have an active supermassive black hole at its center that is engulfing matter and producing radiation. This is somewhat unusual because most of these so-called active galactic nuclei exist in galaxies with prominent bulges. In this particular case, the supermassive black hole is thought to have a relatively small mass, of around 20,000 times that of the Sun.

Another interesting feature is that there are also thought to be two smaller black holes, with masses of a few thousand times that of the Sun, near the nucleus of the galaxy. Therefore, NGC 3621 is an extremely interesting object which, despite not having a central bulge, has a system of three black holes in its central region.

This galaxy is located in the constellation of Hydra (The Sea Snake) and can be seen with a moderate-sized telescope. This image, taken using B, V, and I filters with the FORS1 instrument on the powerful Very Large Telescope (VLT), shows striking detail in this odd object and also reveals a multitude of background galaxies. A number of bright foreground stars that belong to our own Milky Way are also visible.


Credit: European Southern Observatory (ESO)

Release Date: November 28, 2011


#NASA #ESO #Astronomy #Space #Science #Stars #Galaxy #NGC3621 #BlackHoles #Hydra #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Telescope #VLT #LaSillaObservatory #Chile #Europe #STEM #Education

Monday, August 15, 2022

New Delhi, Capital of India, at Night | International Space Station

New Delhi, Capital of India, at Night | International Space Station

Night image of the city of New Delhi, capital of India, as seen by European Space Agency (ESA) astronaut Samantha Cristoforetti aboard the International Space Station for her Minerva Mission.

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:

https://www.nasa.gov/iss-science 

For more information about STEM on Station:

https://www.nasa.gov/stemonstation


Credit: ESA/NASA-S.Cristoforetti

Release Date: August 15, 2022


#NASA #Space #Earth #ISS #NewDelhi #India #ISRO #SamanthaCristoforetti #Italy #Italia #MissionMinerva #Astronauts #Europe #Italia #Italy #Canada #Japan #日本 #Russia #Россия #Science #Research #International #Expedition67 #STEM #Education #Bhārat #Gaṇarājya

Zoom to Galaxy UGC 2885 | Hubble

Zoom to Galaxy UGC 2885 | Hubble

Travel 232 million light-years to galaxy UGC 2885!

This video zooms into the gigantic galaxy known as UGC 2885, which may just be the largest one in the local universe. It is 2.5 times wider than our Milky Way and contains 10 times as many stars. This galaxy is 232 million light-years away, located in the northern constellation of Perseus.


Credit: NASA, European Space Agency (ESA), Digitized Sky Survey, Nick Risinger

Duration: 50 seconds

Release Date: January 6, 2020


#NASA #ESA #Astronomy #Space #Hubble #Stars #Galaxy #UGC2885 #Perseus #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Galaxy UGC 2885 | Hubble

Galaxy UGC 2885 | Hubble

Galaxy UGC 2885 may be the largest one in the local universe. It is 2.5 times wider than our Milky Way and contains 10 times as many stars. This galaxy is 232 million light-years away, located in the northern constellation of Perseus.


Credit: NASA, European Space Agency (ESA), and B. Holwerda (University of Louisville).

Release Date: January 6, 2020


#NASA #ESA #Astronomy #Space #Hubble #Stars #Galaxy #UGC2885 #Perseus #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

The Small Magellanic Cloud | ESO

The Small Magellanic Cloud | ESO

Wide field image, based on data from Digitized Sky Survey 2, shows the Small Magellanic Cloud galaxy and is centered on the star-forming region NGC 346.

Distance: 7 million light years


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

Acknowledgements: Davide De Martin

Release Date: February 24, 2010


#NASA #ESO #Astronomy #Space #Stars #StarCluster #NGC346 #Tucana #Constellation #SmallMagellanicCloud #SMC #Cosmos #Universe #Telescope #Chile #Europe #STEM #Education

Hubble Finds Infant Stars in Neighboring Galaxy

Hubble Finds Infant Stars in Neighboring Galaxy


The exquisite sharpness of the NASA/European Space Agency  Hubble Space Telescope has plucked out an underlying population of infant stars embedded in the nebula NGC 346 that are still forming from gravitationally collapsing gas clouds. They have not yet ignited their hydrogen fuel to sustain nuclear fusion. The smallest of these infant stars is only half the mass of our Sun.

Distance: 200,000 light years


Credit: NASA, European Space Agency (ESA) and A. Nota (STScI/ESA)

Release Date: January 12, 2005


#NASA #ESA #Astronomy #Space #Hubble #Stars #StarCluster #NGC346 #Tucana #Constellation #SmallMagellanicCloud #SMC #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Young Stars Sculpt Gas with Powerful Outflows | Hubble

Young Stars Sculpt Gas with Powerful Outflows | Hubble


This Hubble Space Telescope view shows one of the most dynamic and intricately detailed star-forming regions in space, located 210,000 light-years away in the Small Magellanic Cloud (SMC), a satellite galaxy of our Milky Way. At the center of the region is a brilliant star cluster called NGC 346. A dramatic structure of arched, ragged filaments with a distinct ridge surrounds the cluster.

A torrent of radiation from the hot stars in the cluster NGC 346, at the center of this Hubble image, eats into denser areas around it, creating a fantasy sculpture of dust and gas. The dark, intricately beaded edge of the ridge, seen in silhouette, is particularly dramatic. It contains several small dust globules that point back towards the central cluster, like windsocks caught in a gale.


Credit: NASA, European Space Agency (ESA) and A. Nota (ESA/STScI, STScI/AURA)

Release Date: November 10, 2005


#NASA #ESA #Astronomy #Space #Hubble #Stars #StarCluster #NGC346 #Tucana #Constellation #SmallMagellanicCloud #SMC #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

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