Thursday, August 25, 2022

Stars Alpha Centauri A and B: Closest Star System to Earth | Hubble

Stars Alpha Centauri A and B: Closest Star System to Earth | Hubble


The closest star system to the Earth is the famous Alpha Centauri group. Located in the constellation of Centaurus (The Centaur), at a distance of 4.3 light-years, this system is made up of the binary formed by the stars Alpha Centauri A and Alpha Centauri B, plus the faint red dwarf Alpha Centauri C, also known as Proxima Centauri.

The NASA/European Space Agency Hubble Space Telescope has given us this stunning view of the bright Alpha Centauri A (on the left) and Alpha Centauri B (on the right), flashing like huge cosmic headlamps in the dark. The image was captured by the Wide Field and Planetary Camera 2 (WFPC2). WFPC2 was Hubble’s most used instrument for the first 13 years of the space telescope’s life, being replaced in 2009 by WFC3 during Servicing Mission 4. This portrait of Alpha Centauri was produced by observations carried out at optical and near-infrared wavelengths.

Compared to the Sun, Alpha Centauri A is of the same stellar type G2, and slightly bigger, while Alpha Centauri B, a K1-type star, is slightly smaller. They orbit a common center of gravity once every 80 years, with a minimum distance of about 11 times the distance between the Earth and the Sun. Because these two stars are, together with their sibling Proxima Centauri, the closest to Earth, they are among the best studied by astronomers. And they are also among the prime targets in the hunt for habitable exoplanets. Using the HARPS instrument astronomers already discovered a planet orbiting Alpha Centauri B. August 24, 2016, astronomers announced the discovery of an Earth-like planet in the habitable zone orbiting the star Proxima Centauri.


Credit: European Space Agency (ESA)/Hubble & NASA

Release Date: August 29, 2016


#NASA #ESA #Astronomy #Space #Science #StarSystem #Stars #AlphaCentauri #AlphaCentauriA #AlphaCentauriB #BetaCentauri #Exoplanet #ProximaCentauri #Centaurus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #GSFC #STScI #UnitedStates #Europe #STEM #Education

Stars Alpha Centauri & Proxima Centauri (labeled): Wide-field View | ESO

Stars Alpha Centauri & Proxima Centauri (labeled): Wide-field View | ESO

This image of the sky around the bright star Alpha Centauri AB also shows the much fainter red dwarf star, Proxima Centauri, the closest star to the Solar System. The picture was created from pictures forming part of the Digitized Sky Survey 2. The blue halo around Alpha Centauri AB is an artifact of the photographic process, the star is really pale yellow in color like the Sun.

Distance: about 4 light years


Credit: Digitized Sky Survey 2

Acknowledgement: Davide De Martin/Mahdi Zamani

Release Date: August 24, 2016


#NASA #ESO #Astronomy #Space #Science #StarSystem #Stars #AlphaCentauri #AlphaCentauriA #AlphaCentauriB #BetaCentauri #Exoplanet #ProximaCentauri #Centaurus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Chile #Europe #Infographic #STEM #Education

A Tour of Alpha Centauri | NASA's Chandra X-ray Observatory

A Tour of Alpha Centauri | NASA's Chandra X-ray Observatory

In humanity's search for life outside our Solar System, one of the best places to look is Alpha Centauri, a system containing the three nearest stars beyond the Sun.

A new study that has involved monitoring of Alpha Centauri for more than a decade by NASA's Chandra X-ray Observatory provides encouraging news about one key aspect of planetary habitability. It indicates that any planets orbiting the two brightest stars in the Alpha Cen system are likely not being pummeled by large amounts of X-ray radiation from their host stars.

Alpha Centauri is a triple star system located just over four light years, or about 25 trillion miles, from Earth. While this is a large distance in terrestrial terms, it is three times closer than the next nearest Sun-like star.

The stars in the Alpha Centauri system include a pair called "A" and "B," that we'll call AB, which orbit relatively close to each other. Alpha Cen A is a near twin of our Sun in almost every way, including age, while Alpha Cen B is somewhat smaller and dimmer but still quite similar to the Sun. The third member, Alpha Cen C (also known as Proxima), is a much smaller red dwarf star that travels around the AB pair in a much larger orbit that takes it more than 10 thousand times farther from the AB pair than the Earth-Sun distance. Proxima currently holds the title of the nearest star to Earth, although AB is a very close second.

The Chandra data reveal that the prospects for life in terms of current X-ray bombardment are actually better around Alpha Cen A than for the Sun, and Alpha Cen B fares only slightly worse. Proxima, on the other hand, is a type of active red dwarf star known to frequently send out dangerous flares of X-ray radiation, and is likely hostile to life.

Distance: about 4 light years


Credit: Chandra X-ray Observatory

Narration: April Hobart, Chandra X-ray Center (CXC)

Duration: 2 minutes, 52 seconds

Release Date: June 6, 2018


#NASA #ESO #Astronomy #Space #Science #StarSystem #Stars #AlphaCentauri #AlphaCentauriA #AlphaCentauriB #BetaCentauri #Exoplanet #ProximaCentauri #Centaurus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Chile #Europe #Chandra #Xray #Observatory #STEM #Education #Visualization #Animation #HD #Video

A Journey to Alpha Centauri | ESO

A Journey to Alpha Centauri | ESO

This video shows an imaginary journey from Earth to the Alpha Centauri system. As we leave the Solar System we see the familiar constellation figures including the Southern Cross (Crux) and the bright stars Alpha and Beta Centauri. As we approach Alpha Centauri, we pass a faint red star, this is Proxima Centauri, the closest star to Earth and the faintest component of a triple star system. The final part shows the bright double star Alpha Centauri A and B with the Sun visible in the background. Alpha Centauri B is known to be orbited by an Earth-mass planet, the closest exoplanet to the Solar System.

Distance: about 4 light years


Credit: European Southern Observatory (ESO)/L. Calçada/Nick Risinger

Duration: 1 minute, 10 seconds

Release Date: October 16, 2012


#NASA #ESO #Astronomy #Space #Science #StarSystem #Stars #AlphaCentauri #AlphaCentauriA #AlphaCentauriB #BetaCentauri #Exoplanet #ProximaCentauri #Centaurus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Chile #Europe #STEM #Education #Visualization #Animation #Art #HD #Video

The Bright Star Alpha Centauri: Our Closest Neighbor | ESO

The Bright Star Alpha Centauri: Our Closest Neighbor | ESO


This wide-field view of the sky around the bright star Alpha Centauri was created from photographic images forming part of the Digitized Sky Survey 2. The star appears so big just because of the scattering of light by the telescope's optics as well as in the photographic emulsion. Alpha Centauri is the closest star system to the Solar System.

Distance: about 4 light years


Credit: European Southern Observatory (ESO)

/Digitized Sky Survey 2

Acknowledgement: Davide De Martin

Release Date: October 16, 2012


#NASA #ESO #Astronomy #Space #Science #StarSystem #Star #AlphaCentauri #Centaurus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #Telescope #Chile #Europe #STEM #Education

NASA Astronaut T-38 Jets Flyover Artemis I Moon Rocket on Launch Pad | Kennedy Space Center

NASA Astronaut T-38 Jets Flyover Artemis I Moon Rocket | Kennedy Space Center








NASA's T-38 jets fly in formation above the Space Launch System (SLS) Moon rocket on Launch Pad 39B at NASA's Kennedy Space Center.

Aircraft designations and passengers:

NASA 901: Chris Condon / Astronaut Zena Cardman.

902: Astronaut Candidate Nicole Ayers / Astronaut Christina Koch.

903: Canadian Space Agency Astronaut Jeremy Hansen / Astronaut Drew Morgan.

904: Chief Astronaut Reid Wiseman / Astronaut Joe Acaba.

905 (Photo Chase): Astronaut Candidate Jack Hathaway / Josh Valcarcel


NASA's Artemis Program:

https://www.nasa.gov/specials/artemis


Credit: NASA/Josh Valcarcel

Capture Date: August 23, 2022


#NASA #ESA #Space #Moon #Artemis #ArtemisI #SLS #Rocket #Orion #Spacecraft #Astronauts #AstronautCandidates #Pilots #Aviators #NorthropT38Talon #T38 #DeepSpace #MoonToMars #Science #Engineering #Technology #Exploration #SolarSystem #LaunchComplex39B #KSC #KennedySpaceCenter #Florida #UnitedStates #Europe #STEM #Education

NASA’s Mars Perseverance Rover Makes New Discoveries in Jezero Crater | JPL

NASA’s Mars Perseverance Rover Makes New Discoveries in Jezero Crater | JPL

The rover found that Jezero Crater’s floor is made up of volcanic rocks that have interacted with water.

Scientists got a surprise when NASA’s Perseverance Mars rover began examining rocks on the floor of Jezero Crater in spring 2021: Because the crater held a lake billions of years ago, they had expected to find sedimentary rock, which would have formed when sand and mud settled in a once-watery environment. Instead, they discovered the floor was made of two types of igneous rock—one that formed deep underground from magma, the other from volcanic activity at the surface.

The findings are described in four new papers published Thursday, Aug. 25, 2022. In Science, one offers an overview of Perseverance’s exploration of the crater floor before it arrived at Jezero’s ancient river delta in April 2022; a second study in the same journal details distinctive rocks that appear to have formed from a thick body of magma. The other two papers, published in Science Advances, detail the unique ways that Perseverance’s rock-vaporizing laser and ground-penetrating radar established that igneous rocks cover the crater floor.

Rock of Ages

Igneous rocks are excellent timekeepers: Crystals within them record details about the precise moment they formed.

“One great value of the igneous rocks we collected is that they will tell us about when the lake was present in Jezero. We know it was there more recently than the igneous crater floor rocks formed,” said Ken Farley of Caltech, Perseverance’s project scientist and the lead author of the first of the new Science papers. “This will address some major questions: When was Mars’ climate conducive to lakes and rivers on the planet’s surface, and when did it change to the very cold and dry conditions we see today?”

However, because of how it forms, igneous rock is not ideal for preserving the potential signs of ancient microscopic life Perseverance is searching for. In contrast, determining the age of sedimentary rock can be challenging, particularly when it contains rock fragments that formed at different times before the rock sediment was deposited. However, sedimentary rock often forms in watery environments suitable for life and is better at preserving ancient signs of life.

This is why the sediment-rich river delta Perseverance has been exploring since April 2022 has been so tantalizing to scientists. The rover has begun drilling and collecting core samples of sedimentary rocks there so that the Mars Sample Return campaign could potentially return them to Earth to be studied by powerful lab equipment too large to bring to Mars.

Mysterious Magma-Formed Rocks

A second paper published in Science solves a longstanding mystery on Mars. Years ago, Mars orbiters spotted a rock formation filled with the mineral olivine. Measuring roughly 27,000 square miles (70,000 square kilometers)—nearly the size of South Carolina—this formation extends from the inside edge of Jezero Crater into the surrounding region.

Scientists have offered various theories why olivine is so plentiful over such a large area of the surface, including meteorite impacts, volcanic eruptions, and sedimentary processes. Another theory is that the olivine formed deep underground from slowly cooling magma—molten rock—before being exposed over time by erosion.

Yang Liu of NASA’s Jet Propulsion Laboratory in Southern California and her co-authors have determined that last explanation is the most likely. Perseverance abraded a rock to reveal its composition; studying the exposed patch, the scientists homed in on the olivine’s large grain size, along with the rock’s chemistry and texture.

Using Perseverance’s Planetary Instrument for X-ray Lithochemistry, or PIXL, they determined the olivine grains in the area measure 1 to 3 millimeters—much larger than would be expected for olivine that formed in rapidly cooling lava at the planet’s surface.

Unique Science Tools

The two Science Advances papers detail the findings of science instruments that helped establish that igneous rocks cover the crater floor. The instruments include Perseverance’s SuperCam laser and a ground-penetrating radar called RIMFAX (Radar Imager for Mars’ Subsurface Experiment).

SuperCam is equipped with rock-vaporizing laser that can zap a target as small as a pencil tip from up to 20 feet (7 meters) away. It studies the resulting vapor using a visible-light spectrometer to determine a rock’s chemical composition. SuperCam zapped 1,450 points during Perseverance’s first 10 months on Mars, helping scientists arrive at their conclusion about igneous rocks on the crater floor.

In addition, SuperCam used near-infrared light—it is the first instrument on Mars with that capability—to find that water altered minerals in the crater floor rocks. However, the alterations were not pervasive throughout the crater floor, according to the combination of laser and infrared observations.

RIMFAX marks another first: Mars orbiters carry ground-penetrating radars, but no spacecraft on the surface of Mars have before Perseverance. Being on the surface, RIMFAX can provide unparalleled detail, and surveyed the crater floor as deep as 50 feet (15 meters).

Its high-resolution “radargrams” show rock layers unexpectedly inclined up to 15 degrees underground. Understanding how these rock layers are ordered can help scientists build a timeline of Jezero Crater’s formation.

The science team is excited by what they have found so far, but they are even more excited about the science that lies ahead.

More About the Mission

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

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

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

JPL, which is managed for NASA by Caltech in Pasadena, California, built and manages operations of the Perseverance rover.

For more about Perseverance: 

mars.nasa.gov/mars2020/


Credit: NASA/JPL/Caltech/MSSS

Release Date: August 25, 2022


#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #Jezero #Crater #PerseveranceRover #Robotics #Technology #Engineering #JPL #California #UnitedStates #JourneyToMars #GIF #STEM #Education

Hot Gas Giant Exoplanet WASP-39 b: CO2 Found | James Webb Space Telescope

Hot Gas Giant Exoplanet WASP-39 b: CO2 Found | James Webb Space Telescope

A transmission spectrum of the hot gas giant exoplanet WASP-39 b, captured by Webb’s Near-Infrared Spectrograph (NIRSpec) on July 10, 2022, reveals the first definitive evidence for carbon dioxide in the atmosphere of a planet outside the Solar System. This is the first detailed transmission spectrum ever captured that covers wavelengths between 3 and 5.5 microns.

A transmission spectrum is made by comparing starlight filtered through a planet’s atmosphere as it moves in front of the star, to the unfiltered starlight detected when the planet is beside the star. Each of the 95 data points (white circles) on this graph represents the amount of a specific wavelength of light that is blocked by the planet and absorbed by its atmosphere.

This spectrum was made by measuring the change in brightness of each wavelength over time as the planet transited its star. The planet’s atmosphere absorbs some wavelengths more than others.

Wavelengths absorbed by the atmosphere appear as peaks in the transmission spectrum. The hill centered around 4.3 microns represents the light absorbed by carbon dioxide.

The grey lines extending above and below each data point are error bars that show the uncertainty of each measurement, or the reasonable range of possible values. For a single observation, the error on these measurements is extremely small.

The blue line is a best-fit model that takes into account the data, the known properties of WASP-39 b and its star (e.g., size, mass, temperature), and the assumed characteristics of the atmosphere. Researchers can vary the parameters in the model —changing unknown characteristics like cloud height in the atmosphere and abundances of various gases—to get a better fit and further understand what the atmosphere is really like. The model shown here assumes that the planet is made primarily of hydrogen and helium with small amounts of water and carbon dioxide, with a thin veil of clouds.

The observation was made using the NIRSpec PRISM bright object time-series mode, which involves using a prism to spread out light from a single bright object (like the star WASP-39) and measuring the brightness of each wavelength at set intervals of time.

WASP-39 b is a hot gas giant exoplanet that orbits a Sun-like star roughly 700 light-years away, in the constellation Virgo. The planet orbits extremely close to its star (less than 1/20 of the distance between Earth and the Sun) and completes one orbit in just over four Earth-days. The planet’s discovery, based on ground-based observations, was announced in 2011. The star, WASP-39, is roughly the same size, mass, temperature, and color as the Sun.

The background illustration of WASP-39 b and its star is based on current understanding of the planet from Webb spectroscopy and previous ground- and space-based observations. Webb has not captured a direct image of the planet or its atmosphere.

NIRSpec was built for the European Space Agency (ESA) by a consortium of European companies led by Airbus Defence and Space (ADS) with NASA’s Goddard Space Flight Center providing its detector and micro-shutter subsystems.


Credit: NASA, European Space Agency, Canadian Space Agency, and L. Hustak (STScI)

Science: The JWST Transiting Exoplanet Community Early Release Science Team

Release Date: August 25, 2022


#NASA #ESA #Astronomy #Space #JWST #NIRSpec #Star #WASP39 #WASP39b #Exoplanet #Atmosphere #CarbonDioxide #Science #JamesWebb #WebbTelescope #UnfoldTheUniverse #Europe #CSA #Canada #Goddard #GSFC #STScI #UnitedStates #Infographic #STEM #Education

James Webb Space Telescope Detects Carbon Dioxide in Exoplanet Atmosphere

James Webb Space Telescope Detects Carbon Dioxide in Exoplanet Atmosphere


The NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope has found definitive evidence for carbon dioxide in the atmosphere of a gas giant planet orbiting a Sun-like star 700 light-years away. The result provides important insights into the composition and formation of the planet, and is indicative of Webb’s ability to also detect and measure carbon dioxide in the thinner atmospheres of smaller rocky planets.

This is an illustration (artist’s impression) showing what the exoplanet WASP-39 b could look like, based on current understanding of the planet.

WASP-39 b is a hot, puffy gas giant planet with a mass 0.28 times that of Jupiter (0.94 times that of Saturn) and a diameter 1.3 times that of Jupiter, orbiting just 0.0486 astronomical units (4 520 000 miles) from its host star. The star, WASP-39, is fractionally smaller and less massive than the Sun. Because it is so close to its star, WASP-39 b is very hot and is likely to be tidally locked, meaning that one side faces the star at all times.

Data collected by Webb’s Near-Infrared Spectrograph (NIRSpec) show unambiguous evidence for carbon dioxide in the atmosphere, while previous observations from Hubble, Spitzer, and other telescopes indicate the presence of water vapour, sodium, and potassium, as well. The planet probably has clouds and some form of weather, but may not have atmospheric bands like those of Jupiter and Saturn.

This illustration is based on indirect transit observations from Webb as well as other space and ground-based telescopes. Webb has not captured a direct image of this planet.

NIRSpec was built for the European Space Agency (ESA) by a consortium of European companies led by Airbus Defence and Space (ADS) with NASA’s Goddard Space Flight Centre providing its detector and micro-shutter subsystems.


Credit: NASA, ESA, CSA, and J. Olmsted (STScI)

Release Date: August 25, 2022


#NASA #ESA #Astronomy #Space #JWST #NIRSpec #Star #WASP39 #WASP39b #Exoplanet #Atmosphere #CarbonDioxide #Science #JamesWebb #WebbTelescope #UnfoldTheUniverse #Europe #CSA #Canada #Goddard #GSFC #STScI #UnitedStates #Illustration #STEM #Education

James Webb Space Telescope Detects Carbon Dioxide in Exoplanet Atmosphere

James Webb Space Telescope Detects Carbon Dioxide in Exoplanet Atmosphere

Space Sparks Episode 4: Watch this Space Sparks episode to learn more about how the James Webb Space Telescope has found definitive evidence for carbon dioxide in the atmosphere of a gas giant planet orbiting a Sun-like star 700 light-years away.


Credits: NASA/ESA/CSA/STScI

Directed by: Bethany Downer and Nico Bartmann  

Editing: Nico Bartmann  

Web and technical support: Enciso Systems  

Written by: Bethany Downer  

Music: STAN DART - Organic Life  

Footage and photos: NASA, ESA, CSA, and STScI, NASA's Goddard Space Flight Center Conceptual Image Lab, ESO, E. Slawik, N. Risinger, D. De Martin, D. Lennon, E. Sabbi, N. Bartmann, M. Zamani

Duration: 2 minutes

Release Date: August 25, 2022


#NASA #ESA #Astronomy #Space #JWST #NIRSpec #Star #WASP39 #WASP39b #Exoplanet #Atmosphere #CarbonDioxide #Science #JamesWebb #WebbTelescope #UnfoldTheUniverse #Europe #CSA #Canada #Goddard #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Galaxy Pair Arp 116: Wide-field View | Hubble

Galaxy Pair Arp 116: Wide-field View | Hubble


This image from a ground-based telescope shows the galaxy pair Arp 116 (made up of the elliptical galaxy M60 and the spiral galaxy NGC 4647) and its surroundings.

Distance: 50 million light years


Credit: NASA, European Space Agency, Digitized Sky Survey 2 

Acknowledgement: Davide De Martin

Release Date: September 6, 2012


#NASA #ESA #Astronomy #Space #Science #Hubble #Galaxies #Galaxy #EllipticalGalaxy #Arp116 #Messier60 #M60UCD1 #Virgo #Constellation #SMC #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Galaxy Pair Arp 116 (annotated) | Hubble

Galaxy Pair Arp 116 (annotated) | Hubble


This image shows Arp 116, which is composed of a giant elliptical galaxy known as Messier 60, and a much smaller spiral galaxy, NGC 4647. Also included in the image is an annotated pointer to their even smaller neighbor M60-UCD1.

Lying about 50 million light-years away, M60-UCD1 is a tiny galaxy with a diameter of 300 light-years—just 1/500th of the diameter of the Milky Way! Despite its size it is pretty crowded, containing some 140 million stars.

An international team of astronomers have found a supermassive black hole at the center of M60-UCD1 with the mass of 20 million Suns.


Credit: European Space Agency, NASA and the Hubble Heritage (STScI/AURA)

Release Date: September 6, 2012


#NASA #ESA #Astronomy #Space #Science #Hubble #Galaxies #Galaxy #EllipticalGalaxy #Arp116 #Messier60 #M60UCD1 #Virgo #Constellation #SMC #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Pan across Galaxy Pair Arp 116 | Hubble

Pan across Galaxy Pair Arp 116 | Hubble

This video shows Hubble observations of Arp 116, a pair of galaxies in the constellation of Virgo. It is made up of M60, a large elliptical galaxy, and a smaller, bluer spiral galaxy, NGC 4647. It has long been unclear whether the two galaxies are actually interacting, or whether they simply appear close together from our distant vantage point. However, detailed studies of Hubble pictures suggest that the pair are beginning to experience tidal forces.

Distance: 50 million light years


Credit: NASA, European Space Agency

Duration: 1 minute

Release Date: September 6, 2012


#NASA #ESA #Astronomy #Space #Science #Hubble #Galaxies #Galaxy #EllipticalGalaxy #Arp116 #Messier60 #M60 #M60UCD1 #NGC4647 #Virgo #Constellation #SMC #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Zoom into Galaxy Pair Arp 116 | Hubble

Zoom into Galaxy Pair Arp 116 | Hubble

This video zooms in from a view of the night sky, through the constellation of Virgo, and into a Hubble view of galaxy pair Arp 116.

Distance: 50 million light years


Credit: NASA, European Space Agency, A. Fujii, Digitized Sky Survey 2

Duration: 1 minute

Release Date: September 6, 2012


#NASA #ESA #Astronomy #Space #Science #Hubble #Galaxies #Galaxy #EllipticalGalaxy #Arp116 #Messier60 #M60UCD1 #Virgo #Constellation #SMC #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Galaxy Pair Arp 116 | Hubble

Galaxy Pair Arp 116 | Hubble


This NASA/ESA Hubble Space Telescope image shows the peculiar galaxy pair called Arp 116. 

Distance: 50 million light years

Arp 116 is composed of a giant elliptical galaxy known as Messier 60, and a much smaller spiral galaxy, NGC 4647.

Astronomers have long tried to determine whether these two galaxies are actually interacting. Although they overlap as seen from Earth, there is no evidence of new star formation, which would be one of the clearest signs that the two galaxies are indeed interacting. However, recent studies of very detailed Hubble images suggest the onset of some tidal interaction between the two.

Also included in the image, just below and to the right of M60, is their even smaller neighbor M60-UCD1.

M60-UCD1 is a very tiny galaxy, just 1/500th of the diameter of our Milky Way, that lies about 50 million light-years away. Despite its size, it is pretty crowded, with about 140 million stars crammed into its diameter of just 300 light-years.

An international team of astronomers have found a supermassive black hole at the centre of M60-UCD1 with the mass of 20 million Suns.


Credit: European Space Agency, NASA

Release Date: September 6, 2012


#NASA #ESA #Astronomy #Space #Science #Hubble #Galaxies #Galaxy #EllipticalGalaxy #Arp116 #Messier60 #M60UCD1 #Virgo #Constellation #SMC #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education

Zoom in on Glowing Nebula NGC 248 | Hubble

Zoom in on Glowing Nebula NGC 248 | Hubble

This zoom video starts with a wide-field view of both the Small and the Large Magellanic Clouds before zooming into the emission nebula NGC 248, located on the southern end of the Small Magellanic Cloud, as it is seen with the NASA/European Space Agency Hubble Space Telescope.

Distance: 200,000 light years


Credit: NASA, European Space Agency/Hubble, A. Fujii and Digitized Sky Survey 2 

Duration: 50 seconds

Release Date: December 20, 2016


#NASA #ESA #ESO #Astronomy #Space #Hubble #Nebula #NGC248 #EmissionNebula #Tucana #Constellation #SMC #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education