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'Very Large Array' images and/or videos results page 1 of 1

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Images of 'Very Large Array' found, 34

Sun and Radiotelescopes - Sun above Radiotelescopes - VLA Radio Observatory, New Mexico, USA. Radiotelescope consists of 27 antennas 25 m in diameter. Illustration. The Very Large Array, one of the world's premier astronomical radio observatories, consists of 27 radio antennas in a Y - shaped configuration. Each antenna is 25 meters (82 feet) in diameter. Illustration
 
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Sun and Radiotelescopes - Sun above Radiotelescopes - VLA Radio Observatory, New Mexico, USA. Radiotelescope consists of 27 antennas 25 m in diameter. Illustration. The Very Large Array, one of the world's premier astronomical radio observatories, consists of 27 radio antennas in a Y - shaped configuration. Each antenna is 25 meters (82 feet) in diameter. Illustration

Gregoire Cirade

PIX4656596

Sun and Radiotelescopes - Sun above Radiotelescopes - VLA Radio Observatory, New Mexico, USA. Radiotelescope consists of 27 antennas 25 m in diameter. Illustration. The Very Large Array, one of the world's premier astronomical radio observatories, consists of 27 radio antennas in a Y - shaped configuration. Each antenna is 25 meters (82 feet) in diameter. Illustration

Gregoire Cirade

PIX4656596

Crab Nebula seen in different wavelength - The Crab Nebula in multi wavelength: M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 6500 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, different observatories and telescopes combined their observations; the VLA provided the radio image (in red), the Spitzer telescope the infrared image (in yellow), the Hubble telescope for the visible part (here in green), XMM-Newton the ultraviolet image (in blue) and the Chandra telescope for X-ray data (purple). The pulsar is the bright spot in the center of the image. The unusual image was produced by combining data from telescopes spanning almost the entire electromagnetic spectrum, from radio waves to X-rays. The Karl G. Jansky Very Large Array (VLA) provided information about the nebula gathered in the radio regime (colored in red). Nasa's Spitzer Space Telescope took images in the infrared (yellow). The NASA/ESA Hubble Space Telescope provided the images made in optical wavelengths (colored in green). ESA's XMM-Newton telescope observed the Crab Nebula in the ultraviolet (blue) and Nasa's Chandra X-ray Observatory provided the data for X-ray radiation (purple). The Crab Nebula, located 6500 light-years from Earth in the constellation of Taurus, is the result of a supernova explosion which was observed by Chinese and other astronomers in 1054. At its centre is a pulsar: a super-dense neutron star, spinning once every 33 milliseconds, shooting out rotating light-like beams of radio waves and visible light. Surrounding the pulsar lies a mix of material; some of it was originally expelled from the star before it went supernova, and the rest was ejected during the explosion itself. Fast-moving winds of particles fly off from the neutron star, energising the dust and gas around it.
 
Crab Nebula seen in different wavelength - The Crab Nebula in multi wavelength: M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 6500 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, different observatories and telescopes combined their observations; the VLA provided the radio image (in red), the Spitzer telescope the infrared image (in yellow), the Hubble telescope for the visible part (here in green), XMM-Newton the ultraviolet image (in blue) and the Chandra telescope for X-ray data (purple). The pulsar is the bright spot in the center of the image. The unusual image was produced by combining data from telescopes spanning almost the entire electromagnetic spectrum, from radio waves to X-rays. The Karl G. Jansky Very Large Array (VLA) provided information about the nebula gathered in the radio regime (colored in red). Nasa's Spitzer Space Telescope took images in the in

PIX4626499

Crab Nebula seen in different wavelength - The Crab Nebula in multi wavelength: M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 6500 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, different observatories and telescopes combined their observations; the VLA provided the radio image (in red), the Spitzer telescope the infrared image (in yellow), the Hubble telescope for the visible part (here in green), XMM-Newton the ultraviolet image (in blue) and the Chandra telescope for X-ray data (purple). The pulsar is the bright spot in the center of the image. The unusual image was produced by combining data from telescopes spanning almost the entire electromagnetic spectrum, from radio waves to X-rays. The Karl G. Jansky Very Large Array (VLA) provided information about the nebula gathered in the radio regime (colored in red). Nasa's Spitzer Space Telescope took images in the in

PIX4626499

Composite image of the dwarf galaxy Henize 2-10 (photo)
 
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Composite image of the dwarf galaxy Henize 2-10 (photo)

SMT1217252

Composite image of the dwarf galaxy Henize 2-10 (photo)

SMT1217252

Active Galaxy NGC 1068 in the Whale - Active galaxy NGC 1068 - This composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068 or resides a massive black hole. NGC 1068 is located about 50 million light years away from Earth. Images obtained in X-ray by the Chandra satellite (red), visible by the Hubble space telescope (green) and radio waves (blue). This is a composite image of NGC 1068, one of the nearest and brightest galaxies containing a rapidly growing supermassive black hole. X - ray data from the Chandra X - ray Observatory are shown in red, optical data from the Hubble Space Telescope in green and radio data from the Very Large Array in blue. The spiral structure of NGC 1068 is shown by the X - ray and optical data, and a jet powered by the central supermassive black hole is shown by the radio data. The X - ray images and spectra obtained using Chandra's High Energy Transmission Grating Spectrometer show that a strong wind is being driven away from the center of NGC 1068 at a rate of about a million miles per hour. This wind is likely generated as surrounding gas is accelerated and heated as it swirls toward the black hole. A portion of the gas is pulled into the black hole, but some of it is blown away. High energy X - rays produced by the gas near the black hole heat the ouflowing gas, causing it to glow at lower X - ray energies. NGC 1068 is located about 50 million light years from Earth and contains a supermassive black hole about twice as massive as the one in the middle of the Milky Way Galaxy
 
Active Galaxy NGC 1068 in the Whale - Active galaxy NGC 1068 - This composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068 or resides a massive black hole. NGC 1068 is located about 50 million light years away from Earth. Images obtained in X-ray by the Chandra satellite (red), visible by the Hubble space telescope (green) and radio waves (blue). This is a composite image of NGC 1068, one of the nearest and brightest galaxies containing a rapidly growing supermassive black hole. X - ray data from the Chandra X - ray Observatory are shown in red, optical data from the Hubble Space Telescope in green and radio data from the Very Large Array in blue. The spiral structure of NGC 1068 is shown by the X - ray and optical data, and a jet powered by the central supermassive black hole is shown by the radio data. The X - ray images and spectra obtained using Chandra's High Energy Transmission Grating Spectrometer show that a strong wind is being driven aw

PIX4609662

Active Galaxy NGC 1068 in the Whale - Active galaxy NGC 1068 - This composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068 or resides a massive black hole. NGC 1068 is located about 50 million light years away from Earth. Images obtained in X-ray by the Chandra satellite (red), visible by the Hubble space telescope (green) and radio waves (blue). This is a composite image of NGC 1068, one of the nearest and brightest galaxies containing a rapidly growing supermassive black hole. X - ray data from the Chandra X - ray Observatory are shown in red, optical data from the Hubble Space Telescope in green and radio data from the Very Large Array in blue. The spiral structure of NGC 1068 is shown by the X - ray and optical data, and a jet powered by the central supermassive black hole is shown by the radio data. The X - ray images and spectra obtained using Chandra's High Energy Transmission Grating Spectrometer show that a strong wind is being driven aw

PIX4609662

Barree spiral galaxy NGC 7098 - Barred spiral galaxy NGC 7098: The barree spiral galaxy NGC 7098 is located about 95 million light years away from Earth in the southern constellation of the octant. Image obtained by the Very Large Telescope (VLT). Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 - an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098's double features is a duo of distinct ring-like structures that loop around the galaxy's hazy heart. This central region hosts a second double feature: a double bar. NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity - they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the brim with stars. This image is formed from data gathered by the Focal Reducer and low dispersion Spectrograph (FORS) instrument, installed on Eso's Very Large Telescope at Paranal Observatory. An array of distant galaxies are also visible throughout the frame, the most prominent being the small, edge-on, spiral galaxy visible to the left of NGC 7098, known as ESO 048-G007
 
Barree spiral galaxy NGC 7098 - Barred spiral galaxy NGC 7098: The barree spiral galaxy NGC 7098 is located about 95 million light years away from Earth in the southern constellation of the octant. Image obtained by the Very Large Telescope (VLT). Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 - an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098's double features is a duo of distinct ring-like structures that loop around the galaxy's hazy heart. This central region hosts a second double feature: a double bar. NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity - they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the bri

PIX4574313

Barree spiral galaxy NGC 7098 - Barred spiral galaxy NGC 7098: The barree spiral galaxy NGC 7098 is located about 95 million light years away from Earth in the southern constellation of the octant. Image obtained by the Very Large Telescope (VLT). Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 - an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098's double features is a duo of distinct ring-like structures that loop around the galaxy's hazy heart. This central region hosts a second double feature: a double bar. NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity - they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the bri

PIX4574313

Very Large Array Radio Telescopes near Soccoro 1/2
 
Very Large Array Radio Telescopes near Soccoro 1/2

DWB809881

Very Large Array Radio Telescopes near Soccoro 1/2

DWB809881

Very Large Array Radio Telescopes near Soccoro
 
Very Large Array Radio Telescopes near Soccoro

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Very Large Array Radio Telescopes near Soccoro

DWB694034

Very Large Array Radio Telescopes near Soccoro
 
Very Large Array Radio Telescopes near Soccoro

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Very Large Array Radio Telescopes near Soccoro

DWB694033

Very Large Array Radio Telescopes near Soccoro
 
Very Large Array Radio Telescopes near Soccoro

DWB694028

Very Large Array Radio Telescopes near Soccoro

DWB694028

Time lapse, very Large Array Radio Telescopes near Soccoro
 
Time lapse, very Large Array Radio Telescopes near Soccoro

DWB694036

Time lapse, very Large Array Radio Telescopes near Soccoro

DWB694036

Time lapse, very Large Array Radio Telescopes near Soccoro
 
Time lapse, very Large Array Radio Telescopes near Soccoro

DWB694037

Time lapse, very Large Array Radio Telescopes near Soccoro

DWB694037

Very Large Array Radio Telescopes near Soccoro at sunset
 
Very Large Array Radio Telescopes near Soccoro at sunset

DWB694030

Very Large Array Radio Telescopes near Soccoro at sunset

DWB694030

Very Large Array Radio Telescopes near Soccoro at sunset
 
Very Large Array Radio Telescopes near Soccoro at sunset

DWB694032

Very Large Array Radio Telescopes near Soccoro at sunset

DWB694032

Time lapse, dusk to night, Very Large Array Radio Telescopes near Soccoro
 
Time lapse, dusk to night, Very Large Array Radio Telescopes near Soccoro

DWB694031

Time lapse, dusk to night, Very Large Array Radio Telescopes near Soccoro

DWB694031

Time lapse, day to night, very Large Array Radio Telescopes near Soccoro
 
Time lapse, day to night, very Large Array Radio Telescopes near Soccoro

DWB694029

Time lapse, day to night, very Large Array Radio Telescopes near Soccoro

DWB694029

Very Large Array National Radio Astronomy Observatory, New Mexico
 
Very Large Array National Radio Astronomy Observatory, New Mexico

UIG536095

Very Large Array National Radio Astronomy Observatory, New Mexico

UIG536095

Very Large Array National Radio Astronomy Observatory, New Mexico
 
Very Large Array National Radio Astronomy Observatory, New Mexico

UIG536098

Very Large Array National Radio Astronomy Observatory, New Mexico

UIG536098

A grazing encounter between two spiral galaxies, 1999
 
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A grazing encounter between two spiral galaxies, 1999

UIS5093348

A grazing encounter between two spiral galaxies, 1999

UIS5093348

The elliptical galaxy M84 - The elliptical galaxy M84 - The M84 galaxy (NGC 4374) is 55 million light years away from Earth, in the Virgin's cluster. This image is a composite obtained in X-rays (blue), radio (red) and visible (yellow and white). Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This composite image shows M84, a massive elliptical galaxy in the Virgo Cluster, about 55 million light years from Earth. Hot gas around M84 is shown in a Chandra X - ray Observatory image in blue and a radio image from the Very Large Array is shown in red. A background image from the Sloan Digital Sky Survey is shown in yellow and white. A number of bubbles are visible in the hot gas, outlined with blue X - ray emission. These bubbles were blown by relativistic particles generated by the central supermassive black hole in M84. These particles travel outwards in the form of a two - sided jet. Because smaller bubbles are found inside large bubbles, the impression given by the image is that of Russian dolls, where smaller dolls can be found inside large ones. These nested bubbles provide clear evidence for repeated outbursts from the central black hole
 
The elliptical galaxy M84 - The elliptical galaxy M84 - The M84 galaxy (NGC 4374) is 55 million light years away from Earth, in the Virgin's cluster. This image is a composite obtained in X-rays (blue), radio (red) and visible (yellow and white). Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This composite image shows M84, a massive elliptical galaxy in the Virgo Cluster, about 55 million light years from Earth. Hot gas around M84 is shown in a Chandra X - ray Observatory image in blue and a radio image from the Very Large Array is shown in red. A background image from the Sloan Digital Sky Survey is shown in yellow and white. A number of bubbles are visible in the hot gas, outlined with blue X - ray emission. These bubbles were blown by relativistic particles generated by the central supermassive black hole in M84. These particles travel outwards in the form of a two - sided jet. Because smaller bubbles are found inside lar

PIX4611313

The elliptical galaxy M84 - The elliptical galaxy M84 - The M84 galaxy (NGC 4374) is 55 million light years away from Earth, in the Virgin's cluster. This image is a composite obtained in X-rays (blue), radio (red) and visible (yellow and white). Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This composite image shows M84, a massive elliptical galaxy in the Virgo Cluster, about 55 million light years from Earth. Hot gas around M84 is shown in a Chandra X - ray Observatory image in blue and a radio image from the Very Large Array is shown in red. A background image from the Sloan Digital Sky Survey is shown in yellow and white. A number of bubbles are visible in the hot gas, outlined with blue X - ray emission. These bubbles were blown by relativistic particles generated by the central supermassive black hole in M84. These particles travel outwards in the form of a two - sided jet. Because smaller bubbles are found inside lar

PIX4611313

Juno Probe - Solar Panels - Juno Solar Panels - View of the solar panels of the Juno probe in operation verification. Launched in 2011, the Juno probe will reach Jupiter in 2016. It will then hold the record for the farthest solar power probe ever sent. Technicians at Astrotech's payload processing facility in Titusville, Fla. stow solar array # 2 against the body of Nasa's Juno spacecraft. Launching from Earth in 2011, the Juno spacecraft will arrive at Jupiter in 2016 to study the giant planet from an elliptical, polar orbit. When Juno arrives at Jupiter in 2016, it will be farther from the sun than any previous solar powered mission. The choice of solar power for Juno necessitates very large solar arrays with dimensions of 2.65 meters wide by 8.9 meters long (about 9 feet wide by 29 feet long). Once in orbit at the giant planet, the three arrays will provide about 450 watts of electricity for Juno
 
Juno Probe - Solar Panels - Juno Solar Panels - View of the solar panels of the Juno probe in operation verification. Launched in 2011, the Juno probe will reach Jupiter in 2016. It will then hold the record for the farthest solar power probe ever sent. Technicians at Astrotech's payload processing facility in Titusville, Fla. stow solar array # 2 against the body of Nasa's Juno spacecraft. Launching from Earth in 2011, the Juno spacecraft will arrive at Jupiter in 2016 to study the giant planet from an elliptical, polar orbit. When Juno arrives at Jupiter in 2016, it will be farther from the sun than any previous solar powered mission. The choice of solar power for Juno necessitates very large solar arrays with dimensions of 2.65 meters wide by 8.9 meters long (about 9 feet wide by 29 feet long). Once in orbit at the giant planet, the three arrays will provide about 450 watts of electricity for Juno

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Juno Probe - Solar Panels - Juno Solar Panels - View of the solar panels of the Juno probe in operation verification. Launched in 2011, the Juno probe will reach Jupiter in 2016. It will then hold the record for the farthest solar power probe ever sent. Technicians at Astrotech's payload processing facility in Titusville, Fla. stow solar array # 2 against the body of Nasa's Juno spacecraft. Launching from Earth in 2011, the Juno spacecraft will arrive at Jupiter in 2016 to study the giant planet from an elliptical, polar orbit. When Juno arrives at Jupiter in 2016, it will be farther from the sun than any previous solar powered mission. The choice of solar power for Juno necessitates very large solar arrays with dimensions of 2.65 meters wide by 8.9 meters long (about 9 feet wide by 29 feet long). Once in orbit at the giant planet, the three arrays will provide about 450 watts of electricity for Juno

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Young stars in Rho Ophiuchi - Young stars in Rho Ophiuchi - Image of the central part of Rho Ophiuchi obtained in infrared by the Spitzer space telescope. Rho Ophiuchi is a vast dark cloud of molecular hydrogen located 407 years - light from Earth in the constellations of Ophiuchus and Scorpio. More than 300 young stars aged only 300,000 years have been observed. On this picture in false colors highlighting the temperature differences present in this cloud, the younger stars appear in red, the more evolute stars in blue. Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from Nasa's Spitzer Space Telescope. Called “” Rho Oph””” by astronomers, it's one of the closest star - forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth. Rho Oph is a complex made up of a large main cloud of molecular hydrogen, a key molecule allowing new stars to form from cold cosmic gas, with two long streamers trailing off in different directions. Recent studies using the latest X - ray and infrared observations reveal more than 300 young stellar objects within the large central cloud. Their median age is only 300,000 years, very young compared to some of the university's oldest stars, which are more than 12 billion years old. This false - color image of Rho Oph's main cloud, Lynds 1688, was created with data from Spitzer's infrared array camera, and its multiband imaging photometer, best for detecting cooler materials. Blue represents 3.6 - micron light; green shows light of 8 microns; and red is 24 - micron light. The multiple wavelengths reveal different aspects of the dust surrounding and between the embedded stars, yielding information about the stars and their birthplace. The colors in this image reflect the relative temperatures and evolutionary states of the
 
Young stars in Rho Ophiuchi - Young stars in Rho Ophiuchi - Image of the central part of Rho Ophiuchi obtained in infrared by the Spitzer space telescope. Rho Ophiuchi is a vast dark cloud of molecular hydrogen located 407 years - light from Earth in the constellations of Ophiuchus and Scorpio. More than 300 young stars aged only 300,000 years have been observed. On this picture in false colors highlighting the temperature differences present in this cloud, the younger stars appear in red, the more evolute stars in blue. Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from Nasa's Spitzer Space Telescope. Called “” Rho Oph””” by astronomers, it's one of the closest star - forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth. Rho Oph is a complex made up of a large main cloud of molecular hydrogen, a key molecule allowing new

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Young stars in Rho Ophiuchi - Young stars in Rho Ophiuchi - Image of the central part of Rho Ophiuchi obtained in infrared by the Spitzer space telescope. Rho Ophiuchi is a vast dark cloud of molecular hydrogen located 407 years - light from Earth in the constellations of Ophiuchus and Scorpio. More than 300 young stars aged only 300,000 years have been observed. On this picture in false colors highlighting the temperature differences present in this cloud, the younger stars appear in red, the more evolute stars in blue. Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from Nasa's Spitzer Space Telescope. Called “” Rho Oph””” by astronomers, it's one of the closest star - forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth. Rho Oph is a complex made up of a large main cloud of molecular hydrogen, a key molecule allowing new

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Remains of supernova SN 1006 - Supernova remnant SN 1006 - Remains of supernova SN 1006 located 7000 years ago - light in the constellation Wolf. This supernova that appeared in 1006 is the result of a white dwarf star that absorbs the matter of a companion star became unstable and eventually exploded. This image is a composite of X-ray images obtained by the Chandra telescope (blue), by Cerro Tololo's 90 cm telescope (yellow) and by the Digitized Sky Survey (orange and light blue), and by the VLA and the Green Bank's telescope radio (red). Just over a thousand years ago, the stellar explosion known as supernova SN 1006 was observed. It was brighter than Venus, and visible during the day for weeks. The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world. Astronomers now understand that SN 1006 was caused by a white dwarf star that captured mass from a companion star until the white dwarf became unstable and exploded. Recent observations of the remnant of SN 1006 reveal the liberation of elements such as iron that were previously locked up inside the star. Because no material falls back into a neutron star or black hole after this type of supernova explosion, the liberation of this star's contents is complete. This is a composite image of the SN 1006 supernova remnant, which is located about 7000 light years from Earth. Shown here are X - ray data from Nasa's Chandra X - ray Observatory (blue), optical data from the University of Michigan's 0.9 meter Curtis Schmidt telescope at the NSF's Cerro Tololo Inter - American Observatory (CTIO; yellow) and the Digitized Sky Survey (orange and light blue), plus radio data from the NRAO's Very Large Array and Green Bank Telescope (VLA/GB/GBV T ; red)
 
Remains of supernova SN 1006 - Supernova remnant SN 1006 - Remains of supernova SN 1006 located 7000 years ago - light in the constellation Wolf. This supernova that appeared in 1006 is the result of a white dwarf star that absorbs the matter of a companion star became unstable and eventually exploded. This image is a composite of X-ray images obtained by the Chandra telescope (blue), by Cerro Tololo's 90 cm telescope (yellow) and by the Digitized Sky Survey (orange and light blue), and by the VLA and the Green Bank's telescope radio (red). Just over a thousand years ago, the stellar explosion known as supernova SN 1006 was observed. It was brighter than Venus, and visible during the day for weeks. The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world. Astronomers now understand that SN 1006 was caused by a white dwarf star that captured mass from a companion star until the white dwarf became unstable and

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Remains of supernova SN 1006 - Supernova remnant SN 1006 - Remains of supernova SN 1006 located 7000 years ago - light in the constellation Wolf. This supernova that appeared in 1006 is the result of a white dwarf star that absorbs the matter of a companion star became unstable and eventually exploded. This image is a composite of X-ray images obtained by the Chandra telescope (blue), by Cerro Tololo's 90 cm telescope (yellow) and by the Digitized Sky Survey (orange and light blue), and by the VLA and the Green Bank's telescope radio (red). Just over a thousand years ago, the stellar explosion known as supernova SN 1006 was observed. It was brighter than Venus, and visible during the day for weeks. The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world. Astronomers now understand that SN 1006 was caused by a white dwarf star that captured mass from a companion star until the white dwarf became unstable and

PIX4583213

The galactic center seen by Spitzer Space Telescope - The galactic center region seen by Spitzer satellite. The area photographed extends over 890 light-years and over 640 light-years high. In visible light, this area is hidden by a large amount of interstellar dust. This picture in false colors shows the old and cold stars in blue, and the red regions the hot and massive stars. Dark and bright filamentous clouds are star-forming regions. The brightest area in the center of the image is the center of our galaxy which houses a supermassive black hole. This infrared image from Nasa's Spitzer Space Telescope shows hundreds of thousands of stars crowded into the swirling core of our spiral Milky Way galaxy. In visible-light pictures, this region cannot be seen at all because dust lying between Earth and the galactic center blocks our view. In this false-color picture, old and cool stars are blue, while dust features lit up by blazing hot, massive stars are shown in a reddish hue. Both bright and dark filamentary clouds can be seen, many of which harbor stellar nurseries. The plane of the Milky Way's flat disk is apparent as the main, horizontal band of clouds. The brightest white spot in the middle is the very center of the galaxy, which also marks the site of a supermassive black hole. The region pictured here is immense, with a horizontal span of 890 light-years and a vertical span of 640 light-years. Earth is located 26,000 light-years away, out in one of the Milky Way's spiral arms. Though most of the objects seen in this image are located at the galactic center, the features above and below the galactic plane tend to lie closer to Earth. This image is a mosaic of thousands of short exposures taken by Spitzer's Infrared Array Camera. The entire region was imaged in less than 16 hours
 
The galactic center seen by Spitzer Space Telescope - The galactic center region seen by Spitzer satellite. The area photographed extends over 890 light-years and over 640 light-years high. In visible light, this area is hidden by a large amount of interstellar dust. This picture in false colors shows the old and cold stars in blue, and the red regions the hot and massive stars. Dark and bright filamentous clouds are star-forming regions. The brightest area in the center of the image is the center of our galaxy which houses a supermassive black hole. This infrared image from Nasa's Spitzer Space Telescope shows hundreds of thousands of stars crowded into the swirling core of our spiral Milky Way galaxy. In visible-light pictures, this region cannot be seen at all because dust lying between Earth and the galactic center blocks our view. In this false-color picture, old and cool stars are blue, while dust features lit up by blazing hot, massive stars are shown in a reddish hue. Both brig

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The galactic center seen by Spitzer Space Telescope - The galactic center region seen by Spitzer satellite. The area photographed extends over 890 light-years and over 640 light-years high. In visible light, this area is hidden by a large amount of interstellar dust. This picture in false colors shows the old and cold stars in blue, and the red regions the hot and massive stars. Dark and bright filamentous clouds are star-forming regions. The brightest area in the center of the image is the center of our galaxy which houses a supermassive black hole. This infrared image from Nasa's Spitzer Space Telescope shows hundreds of thousands of stars crowded into the swirling core of our spiral Milky Way galaxy. In visible-light pictures, this region cannot be seen at all because dust lying between Earth and the galactic center blocks our view. In this false-color picture, old and cool stars are blue, while dust features lit up by blazing hot, massive stars are shown in a reddish hue. Both brig

PIX4637936

Gladstone collection 3: Northern Territories, Ghana Part 3 c.1961
 
Gladstone collection 3: Northern Territories, Ghana Part 3 c.1961

BAF8619159

Gladstone collection 3: Northern Territories, Ghana Part 3 c.1961

BAF8619159

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