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Motion of the Star Proxima of Centauri - The proper motion of Proxima Centauri - Proxima of Centauri (in the center of the image) is the closest star to the Sun, located at a distance of 4.2 years - light. This star is a red dwarf, 10,000 times less luminous than our Sun, and is invisible to the naked eye. Its proximity makes it move quickly ahead of the other stars. This composite image made from three images taken in 1976 (blue), 1982 (red) and 1993 (green) shows the shift of the star in 17 years. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Proxima Centauri is the nearest known star to the sun, at a distance of about 4.2 light years. It is an intrinsically faint red star, more than ten magnitudes (ten thousand times) fainter than the Sun. It is also much cooler, with a surface temperature of about 3100 C. Its visual (apparent) magnitude is eleven, so it is only visible with a good telescope, and only then from southern latitudes. Proxima is about one - tenth t

Motion of the Star Proxima of Centauri - The proper motion of Proxima Centauri - Proxima of Centauri (in the center of the image) is the closest star to the Sun, located at a distance of 4.2 years - light. This star is a red dwarf, 10,000 times less luminous than our Sun, and is invisible to the naked eye. Its proximity makes it move quickly ahead of the other stars. This composite image made from three images taken in 1976 (blue), 1982 (red) and 1993 (green) shows the shift of the star in 17 years. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Proxima Centauri is the nearest known star to the sun, at a distance of about 4.2 light years. It is an intrinsically faint red star, more than ten magnitudes (ten thousand times) fainter than the Sun. It is also much cooler, with a surface temperature of about 3100 C. Its visual (apparent) magnitude is eleven, so it is only visible with a good telescope, and only then from southern latitudes. Proxima is about one - tenth t

PIX4571842

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

PIX4610713

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

PIX4610684

Mars: faults in Claritas Fossae. - Mars: fractures in Claritas Fossae - Fracture system in Claritas Fossae, a region south of the Tharsis volcanoes. These fractures, ranging from a few kilometres to a hundred kilometres, are probably associated with the tectonic activity that led to elevation of the Tharsis plateau. Perspective image obtained by the Mars Express probe in 2004. On 29 June 2004 the High Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained image data in orbit 563 with a ground resolution of approximately 62 metres per pixel. The images cover Claritas Fossae at approximately 25* southern latitude and 253* eastern longitude. Claritas Fossae is located on the Tharsis rise, south of the three large volcanoes known as the Tharsis Montes, and extends roughly north to south for approximately 1800 km. Claritas Fossae, which is composed of a series of linear fractures with widths ranging from a few kilometres to 100 km, is roughly 150 km wide in the nor

Mars: faults in Claritas Fossae. - Mars: fractures in Claritas Fossae - Fracture system in Claritas Fossae, a region south of the Tharsis volcanoes. These fractures, ranging from a few kilometres to a hundred kilometres, are probably associated with the tectonic activity that led to elevation of the Tharsis plateau. Perspective image obtained by the Mars Express probe in 2004. On 29 June 2004 the High Resolution Stereo Camera (HRSC) onboard the ESA spacecraft Mars Express obtained image data in orbit 563 with a ground resolution of approximately 62 metres per pixel. The images cover Claritas Fossae at approximately 25* southern latitude and 253* eastern longitude. Claritas Fossae is located on the Tharsis rise, south of the three large volcanoes known as the Tharsis Montes, and extends roughly north to south for approximately 1800 km. Claritas Fossae, which is composed of a series of linear fractures with widths ranging from a few kilometres to 100 km, is roughly 150 km wide in the nor

PIX4616037

Planetary nebula NGC 7027 in the Swan/HST - This NASA Hubble Space Telescope image of planetary nebula NGC 7027 shows remarkable new details of the process by which a star like the Sun dies. New features include: faint, blue, concentric shells surrounding the nebula; an extensive network of red dust clouds throughout the bright inner region; and the hot central white dwarf, visible as a white dot at the center. The nebula is a record of the star's final death throes. Initially the ejection of the star's outer layers, when it was at its red giant stage of evolution, occurred at a low rate and was spherical. The Hubble photo reveals that the initial ejections occurred episodically to produce the concentric shells. This culminated in a vigorous ejection of all of the remaining outer layers, which produced the bright inner regions. At this later stage the ejection was non - spherical, and dense clouds of dust condensed from the ejected material. NGC 7027 is located about 3,000 light - year

Planetary nebula NGC 7027 in the Swan/HST - This NASA Hubble Space Telescope image of planetary nebula NGC 7027 shows remarkable new details of the process by which a star like the Sun dies. New features include: faint, blue, concentric shells surrounding the nebula; an extensive network of red dust clouds throughout the bright inner region; and the hot central white dwarf, visible as a white dot at the center. The nebula is a record of the star's final death throes. Initially the ejection of the star's outer layers, when it was at its red giant stage of evolution, occurred at a low rate and was spherical. The Hubble photo reveals that the initial ejections occurred episodically to produce the concentric shells. This culminated in a vigorous ejection of all of the remaining outer layers, which produced the bright inner regions. At this later stage the ejection was non - spherical, and dense clouds of dust condensed from the ejected material. NGC 7027 is located about 3,000 light - year

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Gl 581c: discovery of a habitable planet - Gl 581c: discovery of an habitable planet - Artist's view of the exoplanet Gliese 581c. Gliese 581c, with a radius of 1.5 times that of the Earth, is the first exoplanet gathering the necessary elements to imagine the existence of a possible extra-terrestrial life. From its surface, its star, about 100 times less bright than our Sun, must be large in the sky because of its proximity to the planet. In April 2007 the Geneva Observatory in Switzerland announced the discovery of a “super - earth”” extrasolar planet orbiting the red dwarf star Gliese 581. Dubbed Gliese 581 c, it's been called a super - earth because it is one of the few known extrasolar planets that has a mass near Earth's, and the only one to occupy its sun's “” habitable zone.”” Gliese 581 c is believed to be about five times more massive than the Earth with a diameter about half - again as large as Earth's. Depending upon the planet's composition, whether mostly rock or a combin

Gl 581c: discovery of a habitable planet - Gl 581c: discovery of an habitable planet - Artist's view of the exoplanet Gliese 581c. Gliese 581c, with a radius of 1.5 times that of the Earth, is the first exoplanet gathering the necessary elements to imagine the existence of a possible extra-terrestrial life. From its surface, its star, about 100 times less bright than our Sun, must be large in the sky because of its proximity to the planet. In April 2007 the Geneva Observatory in Switzerland announced the discovery of a “super - earth”” extrasolar planet orbiting the red dwarf star Gliese 581. Dubbed Gliese 581 c, it's been called a super - earth because it is one of the few known extrasolar planets that has a mass near Earth's, and the only one to occupy its sun's “” habitable zone.”” Gliese 581 c is believed to be about five times more massive than the Earth with a diameter about half - again as large as Earth's. Depending upon the planet's composition, whether mostly rock or a combin

Walter B Myers

PIX4573770

Jeju volcanic island, South Korea - Jeju volcanic island, South Korea - Jeju volcanic island seen by Landsat satellite - 7 on April 6, 2000. This island, classified as a World Heritage Site, is home to the highest peak of South Korea, Mount Halla (1950 m), a volcano shield whose last eruption dates back to 1007. Cheju Island, is an oval - shaped volcanic landmass covering 1,845 square kilometers (712 square miles) off the southern tip of the Korean Peninsula. Geologists estimate the island's age at 2 million years, and archaeological finds suggest that people have lived on the island since prehistoric times. Today, Cheju is both a tourist attraction and home to an UNESCO World Heritage site. The Enhanced Thematic Mapper Plus on Nasa's Landsat - 7 satellite captured this image of Cheju Island on April 6, 2000. In this photo - like image, cloudless skies allow a clear view of the island and the swirling blue hues of the surrounding waters. Urbanized areas, such as the capital city, Cheju

Jeju volcanic island, South Korea - Jeju volcanic island, South Korea - Jeju volcanic island seen by Landsat satellite - 7 on April 6, 2000. This island, classified as a World Heritage Site, is home to the highest peak of South Korea, Mount Halla (1950 m), a volcano shield whose last eruption dates back to 1007. Cheju Island, is an oval - shaped volcanic landmass covering 1,845 square kilometers (712 square miles) off the southern tip of the Korean Peninsula. Geologists estimate the island's age at 2 million years, and archaeological finds suggest that people have lived on the island since prehistoric times. Today, Cheju is both a tourist attraction and home to an UNESCO World Heritage site. The Enhanced Thematic Mapper Plus on Nasa's Landsat - 7 satellite captured this image of Cheju Island on April 6, 2000. In this photo - like image, cloudless skies allow a clear view of the island and the swirling blue hues of the surrounding waters. Urbanized areas, such as the capital city, Cheju

PIX4660095

Star Formation in Galaxy M83 - Star Birth in Spiral galaxy M83 - Close-up of star-forming zones in the arms and near the nucleus (white region on the right) of the M83 galaxy. In red appear the hydrogen clouds in which the stars are born. The new stars are concentrated in blue clusters visible by hundreds on this image. The galaxy M83 (NGC 5236) is located about 15 million light years away from Earth in the constellation Hydra. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained by the Hubble space telescope with its wide field camera 3 (WFC3) in August 2009. Nicknamed the Southern Pinwheel, M83 is undergoing more rapid star formation than our own Milky Way galaxy, especially in its nucleus. The sharp “” eye”” of the Wide Field Camera 3 (WFC3) has captured hundreds of young star clusters, ancient swarms of globular star clusters, and hundreds of thousands of individual stars, mostly blue supergiants and red supergiants. The image, taken in August 20

Star Formation in Galaxy M83 - Star Birth in Spiral galaxy M83 - Close-up of star-forming zones in the arms and near the nucleus (white region on the right) of the M83 galaxy. In red appear the hydrogen clouds in which the stars are born. The new stars are concentrated in blue clusters visible by hundreds on this image. The galaxy M83 (NGC 5236) is located about 15 million light years away from Earth in the constellation Hydra. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained by the Hubble space telescope with its wide field camera 3 (WFC3) in August 2009. Nicknamed the Southern Pinwheel, M83 is undergoing more rapid star formation than our own Milky Way galaxy, especially in its nucleus. The sharp “” eye”” of the Wide Field Camera 3 (WFC3) has captured hundreds of young star clusters, ancient swarms of globular star clusters, and hundreds of thousands of individual stars, mostly blue supergiants and red supergiants. The image, taken in August 20

PIX4612521

Field of distant galaxies - Distant galaxies - Image of distant galaxies obtained by the Hubble space telescope in the furnace constellation. 7500 galaxies, some of which are more than 13 billion years old - light are visible on this image. Some closer galaxies also appear. This image covers a field equivalent to one third of a full moon. This image, taken by Nasa's Hubble Space Telescope, was made from mosaics taken in September and October 2009 with the newly installed Wide Field Camera 3 (WFC3) and in 2004 with the Advanced Camera for Surveys (ACS). The view covers a portion of the southern field of a large galaxy census called the Great Observatories Origins Deep Survey (GOODS), a deep - sky study by several observatories to trace the formation and evolution of galaxies. The final image combines a broad range of colors, from the ultraviolet, through visible light, and into the near - infrared. The image reveals galaxy shapes that appear increasingly chaotic at each earlier epoch, a

Field of distant galaxies - Distant galaxies - Image of distant galaxies obtained by the Hubble space telescope in the furnace constellation. 7500 galaxies, some of which are more than 13 billion years old - light are visible on this image. Some closer galaxies also appear. This image covers a field equivalent to one third of a full moon. This image, taken by Nasa's Hubble Space Telescope, was made from mosaics taken in September and October 2009 with the newly installed Wide Field Camera 3 (WFC3) and in 2004 with the Advanced Camera for Surveys (ACS). The view covers a portion of the southern field of a large galaxy census called the Great Observatories Origins Deep Survey (GOODS), a deep - sky study by several observatories to trace the formation and evolution of galaxies. The final image combines a broad range of colors, from the ultraviolet, through visible light, and into the near - infrared. The image reveals galaxy shapes that appear increasingly chaotic at each earlier epoch, a

PIX4613824

Earth's atmosphere and setting sun - Earth's atmosphere and setting sun - Earth's atmosphere seen at sunset from the International Space Station (ISS) on May 25, 2010. This spectacular image of sunset on the Indian Ocean was taken by astronauts aboard the International Space Station (ISS). The image presents an edge - on, or limb view, of the Earth's atmosphere as seen from orbit. The Earth's curvature is visible along the horizon line, or limb, that extends across the image from center left to lower right. Above the darkened surface of the Earth, a brilliant sequence of colors roughly denotes several layers of the atmosphere. Deep oranges and yellows appear in the troposphere, which extends from the Earth's surface to 6 - 20 km high. This layer contains over 80 percent of the mass of the atmosphere and almost all of the water vapor, clouds, and precipitation. Several dark cloud layers are visible within this layer. Variations in the colors are due mainly to varying concentrations of e

Earth's atmosphere and setting sun - Earth's atmosphere and setting sun - Earth's atmosphere seen at sunset from the International Space Station (ISS) on May 25, 2010. This spectacular image of sunset on the Indian Ocean was taken by astronauts aboard the International Space Station (ISS). The image presents an edge - on, or limb view, of the Earth's atmosphere as seen from orbit. The Earth's curvature is visible along the horizon line, or limb, that extends across the image from center left to lower right. Above the darkened surface of the Earth, a brilliant sequence of colors roughly denotes several layers of the atmosphere. Deep oranges and yellows appear in the troposphere, which extends from the Earth's surface to 6 - 20 km high. This layer contains over 80 percent of the mass of the atmosphere and almost all of the water vapor, clouds, and precipitation. Several dark cloud layers are visible within this layer. Variations in the colors are due mainly to varying concentrations of e

PIX4675392

Star Vega in the Lyre - Star Vega in infrared - Vega (Alpha Lyrae) is the main star of the constellation Lyra, located only 25.4 light years from the Sun. It is the second brightest star after Sirius in the northern hemisphere. It's seen here in infrared by the Spitzer space telescope. Observed in this wavelength, the dust cloud surrounding the star appears. Nasa's Spitzer Space Telescope captured these images of the star Vega, located 25 light years away in the constellation Lyra. Spitzer was able to detect the heat radiation from the cloud of dust around the star and found that the debris disk is much larger than previously thought. This side - by - side comparison, taken by Spitzer's multiband imaging photometer, shows the warm infrared glows from dust particles orbiting the star at wavelengths of 24 microns (on the left in blue) and 70 microns (on the right in red). Both images show a very large, circular and smooth debris disk. The disk radius extends to at least 815 astronomical

Star Vega in the Lyre - Star Vega in infrared - Vega (Alpha Lyrae) is the main star of the constellation Lyra, located only 25.4 light years from the Sun. It is the second brightest star after Sirius in the northern hemisphere. It's seen here in infrared by the Spitzer space telescope. Observed in this wavelength, the dust cloud surrounding the star appears. Nasa's Spitzer Space Telescope captured these images of the star Vega, located 25 light years away in the constellation Lyra. Spitzer was able to detect the heat radiation from the cloud of dust around the star and found that the debris disk is much larger than previously thought. This side - by - side comparison, taken by Spitzer's multiband imaging photometer, shows the warm infrared glows from dust particles orbiting the star at wavelengths of 24 microns (on the left in blue) and 70 microns (on the right in red). Both images show a very large, circular and smooth debris disk. The disk radius extends to at least 815 astronomical

PIX4571758

Traces of the impact crater Chicxulub - Chicxulub impact crater - Excessive relief view of the Yucatan peninsula obtained from radar altimetric data acquired by the SRTM instrument aboard the space shuttle Endeavour in 2000. An arc of circle is visible to the north-west of the peninsula, marking the outer edge of the Chicxulub impact crater whose centre is located off the Mexican coast. This meteorite impact would have caused the disappearance of dinosaurs 65 million years ago. This shaded relief image of Mexico's Yucatan Peninsula show a subtle, but unmistakable, indication of the Chicxulub impact crater. Most scientists now agree that this impact was the cause of the Cretatious - Tertiary Extinction, the event 65 million years ago that marked the sudden extinction of the dinosaurs as well as the majority of life then on Earth. Most of the peninsula is visible here, along with the island of Cozumel off the east coast. The Yucatan is a plateau composed mostly of limestone and is an are

Traces of the impact crater Chicxulub - Chicxulub impact crater - Excessive relief view of the Yucatan peninsula obtained from radar altimetric data acquired by the SRTM instrument aboard the space shuttle Endeavour in 2000. An arc of circle is visible to the north-west of the peninsula, marking the outer edge of the Chicxulub impact crater whose centre is located off the Mexican coast. This meteorite impact would have caused the disappearance of dinosaurs 65 million years ago. This shaded relief image of Mexico's Yucatan Peninsula show a subtle, but unmistakable, indication of the Chicxulub impact crater. Most scientists now agree that this impact was the cause of the Cretatious - Tertiary Extinction, the event 65 million years ago that marked the sudden extinction of the dinosaurs as well as the majority of life then on Earth. Most of the peninsula is visible here, along with the island of Cozumel off the east coast. The Yucatan is a plateau composed mostly of limestone and is an are

PIX4630564

Cone Nebula NGC 2264 in the Unicorn - The Cone Nebula NGC 2264 in Monoceros - The Cone Nebula is a region H II located about 2600 years from Earth. It is accompanied by a cluster of stars called the Christmas tree. The bright star at the top is S Monocerotis, a star of magnitude 4.7. Image obtained by the 2.2m telescope of La Silla. NGC 2264 and the Christmas Tree cluster lies about 2600 light - years from Earth in the constellation of Monoceros, the Unicorn, not far from the more familiar figure of Orion, the Hunter. The image shows a region of space about 30 light - years across. The cluster is very bright and can easily be seen with binoculars. With a small telescope (whose lenses will turn the view upside down) the stars resemble the glittering lights on a Christmas tree. The dazzling star at the top is S Monocerotis, bright enough to be seen with the unaided eye. It is a massive multiple star system that only emerged from the dust and gas a few million years ago. At the bottom of

Cone Nebula NGC 2264 in the Unicorn - The Cone Nebula NGC 2264 in Monoceros - The Cone Nebula is a region H II located about 2600 years from Earth. It is accompanied by a cluster of stars called the Christmas tree. The bright star at the top is S Monocerotis, a star of magnitude 4.7. Image obtained by the 2.2m telescope of La Silla. NGC 2264 and the Christmas Tree cluster lies about 2600 light - years from Earth in the constellation of Monoceros, the Unicorn, not far from the more familiar figure of Orion, the Hunter. The image shows a region of space about 30 light - years across. The cluster is very bright and can easily be seen with binoculars. With a small telescope (whose lenses will turn the view upside down) the stars resemble the glittering lights on a Christmas tree. The dazzling star at the top is S Monocerotis, bright enough to be seen with the unaided eye. It is a massive multiple star system that only emerged from the dust and gas a few million years ago. At the bottom of

PIX4618657

Planetary nebula NGC 2818 - Planetary nebula NGC 2818 in Pyxis - The open cluster NGC 2818A in the southern constellation of the Compsole is distinguished by the fact that most of its bright stars have already become supernovae; this indicates that this cluster must be very old, perhaps a billion years. It has a planetary nebula, NGC 2818, photographed here by the Hubble space telescope in November 2008. A planetary nebula is an end-of-life star. NGC 2818 (also called PLN 261+8.1) is located about 10,000 light years from Earth. The unique planetary nebula NGC 2818 is nested inside the open star cluster NGC 2818A. Both the cluster and the nebula reside over 10,000 light - years away, in the southern constellation Pyxis (the Compasss). NGC 2818 is one of very few planetary nebulae in our galaxy located within an open cluster. Open clusters, in general, are loosely bound and they disperse over hundreds of millions of years. Stars that form planetary nebulae typically live for billions of

Planetary nebula NGC 2818 - Planetary nebula NGC 2818 in Pyxis - The open cluster NGC 2818A in the southern constellation of the Compsole is distinguished by the fact that most of its bright stars have already become supernovae; this indicates that this cluster must be very old, perhaps a billion years. It has a planetary nebula, NGC 2818, photographed here by the Hubble space telescope in November 2008. A planetary nebula is an end-of-life star. NGC 2818 (also called PLN 261+8.1) is located about 10,000 light years from Earth. The unique planetary nebula NGC 2818 is nested inside the open star cluster NGC 2818A. Both the cluster and the nebula reside over 10,000 light - years away, in the southern constellation Pyxis (the Compasss). NGC 2818 is one of very few planetary nebulae in our galaxy located within an open cluster. Open clusters, in general, are loosely bound and they disperse over hundreds of millions of years. Stars that form planetary nebulae typically live for billions of

PIX4622959

Planetary nebula NGC 6543 in the Dragon - Planetary nebula NGC 6543 in Draco - Composite view of the planetary nebula NGC 6543 in the Dragon obtained by the Hubble space telescope and X-ray (blue) by the Chandra satellite. NGC 6543 is located about 3000 years of light from Earth. This composite of data from Nasa's Chandra X - ray Observatory and Hubble Space Telescope is a new look for NGC 6543, better known as the Cat's Eye nebula. This famous object is a so - called planetary nebula that represents a phase of stellar evolution that the Sun should experience several billion years from now. When a star like the Sun begins to run out of fuel, it becomes what is known as a red giant. In this phase, a star sheds some of its outer layers, eventually leaving behind a hot core that collapses to form a dense white dwarf star. A fast wind emanating from the hot core rams into the ejected atmosphere, pushes it outward, and creates the graceful filamentary structures seen with optical telescopes

Planetary nebula NGC 6543 in the Dragon - Planetary nebula NGC 6543 in Draco - Composite view of the planetary nebula NGC 6543 in the Dragon obtained by the Hubble space telescope and X-ray (blue) by the Chandra satellite. NGC 6543 is located about 3000 years of light from Earth. This composite of data from Nasa's Chandra X - ray Observatory and Hubble Space Telescope is a new look for NGC 6543, better known as the Cat's Eye nebula. This famous object is a so - called planetary nebula that represents a phase of stellar evolution that the Sun should experience several billion years from now. When a star like the Sun begins to run out of fuel, it becomes what is known as a red giant. In this phase, a star sheds some of its outer layers, eventually leaving behind a hot core that collapses to form a dense white dwarf star. A fast wind emanating from the hot core rams into the ejected atmosphere, pushes it outward, and creates the graceful filamentary structures seen with optical telescopes

PIX4623257

Djorgovski globular cluster 1 in Scorpio - Globular cluster Djorgovski 1 in Scorpius - The Djorgovski globular cluster 1 is a cluster of light stars located near the galactic center, 40,000 years - light from Earth. Its discovery is recent (1987) and studies show that its stars are composed only of hydrogene and helium. The absence of heavier elements that are usually present in stars remains an enigma. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has imaged an area so jam - packed with stars that they almost overwhelm the inky blackness of space. This includes the globular star cluster Djorgovski 1, which was only discovered in 1987 Djorgovski 1 is located close to the centre of our Milky Way Galaxy, within the bulge. If the galaxy is thought of as being like a city, then this bulge is the very busiest district at its centre. Djorgovski 1's proximity to this hub - - within just a few degrees - - explains why the picture is teeming with stars.

Djorgovski globular cluster 1 in Scorpio - Globular cluster Djorgovski 1 in Scorpius - The Djorgovski globular cluster 1 is a cluster of light stars located near the galactic center, 40,000 years - light from Earth. Its discovery is recent (1987) and studies show that its stars are composed only of hydrogene and helium. The absence of heavier elements that are usually present in stars remains an enigma. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has imaged an area so jam - packed with stars that they almost overwhelm the inky blackness of space. This includes the globular star cluster Djorgovski 1, which was only discovered in 1987 Djorgovski 1 is located close to the centre of our Milky Way Galaxy, within the bulge. If the galaxy is thought of as being like a city, then this bulge is the very busiest district at its centre. Djorgovski 1's proximity to this hub - - within just a few degrees - - explains why the picture is teeming with stars.

PIX4565206

Open cluster Westerlund 2 in Carene - Open cluster Westerlund 2 in Carina - The open cluster Westerlund 2 is located about 20,000 years - light in the southern constellation of Carene, within the nebula Gum 29. About 3000 stars form this cluster. It contains a significant number of massive stars including one of the most massive stars known to date: WR 20a. Image obtained by the Hubble Space Telescope. The sparkling centerpiece of this image taken by the Hubble space telescope is a giant cluster of about 3,000 stars called Westerlund 2, named for Swedish astronomer Bengt Westerlund, who discovered the grouping in the 1960s. The cluster resides in a raucous stellar breeding ground known as Gum 29, located 20,000 light - years away from Earth in the constellation Carina. To capture this image, Hubble's near - infrared Wide Field Camera 3 near - infrared pierced through the dusty veil shrouding the stellar nursery, giving astronomers a clear view of the nebula and the dense concentration

Open cluster Westerlund 2 in Carene - Open cluster Westerlund 2 in Carina - The open cluster Westerlund 2 is located about 20,000 years - light in the southern constellation of Carene, within the nebula Gum 29. About 3000 stars form this cluster. It contains a significant number of massive stars including one of the most massive stars known to date: WR 20a. Image obtained by the Hubble Space Telescope. The sparkling centerpiece of this image taken by the Hubble space telescope is a giant cluster of about 3,000 stars called Westerlund 2, named for Swedish astronomer Bengt Westerlund, who discovered the grouping in the 1960s. The cluster resides in a raucous stellar breeding ground known as Gum 29, located 20,000 light - years away from Earth in the constellation Carina. To capture this image, Hubble's near - infrared Wide Field Camera 3 near - infrared pierced through the dusty veil shrouding the stellar nursery, giving astronomers a clear view of the nebula and the dense concentration

PIX4569094

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on November 13, 2015. View of the hemisphere oriente towards Saturn - This composite image shows an infrared view of Saturn's moon Titan from Nasa's Cassini spacecraft, acquired during the mission's “” T-114”” flyby on Nov. 13, 2015. The spacecraft's visual and infrared mapping spectrometer (VIMS) instrument made these observations, in which blue represents wavelengths centered at 1.3 microns, green represents 2.0 microns, and red represents 5.0 microns. A view at visible wavelengths (centered around 0.5 microns) would show only Titan's hazy atmosphere (as in PIA14909). The near-infrared wavelengths in this image allow Cassini's vision to penetrate the haze and reveal the moon's surface - During this Titan flyby, the spacecraft's close-approach altitude was 6,200 miles (10,000 kilometers), which is considerably higher than

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on November 13, 2015. View of the hemisphere oriente towards Saturn - This composite image shows an infrared view of Saturn's moon Titan from Nasa's Cassini spacecraft, acquired during the mission's “” T-114”” flyby on Nov. 13, 2015. The spacecraft's visual and infrared mapping spectrometer (VIMS) instrument made these observations, in which blue represents wavelengths centered at 1.3 microns, green represents 2.0 microns, and red represents 5.0 microns. A view at visible wavelengths (centered around 0.5 microns) would show only Titan's hazy atmosphere (as in PIA14909). The near-infrared wavelengths in this image allow Cassini's vision to penetrate the haze and reveal the moon's surface - During this Titan flyby, the spacecraft's close-approach altitude was 6,200 miles (10,000 kilometers), which is considerably higher than

PIX4625361

"Many are called, but few are chosen", St Matthew, xxii, 14 (engraving)

"Many are called, but few are chosen", St Matthew, xxii, 14 (engraving)

English School, (19th century)

LLM2809831

Titan, Saturn satellite seen by Cassini: Visible and infrared composite image of Titan taken by the Cassini probe on September 12, 2013. View of methane and ethane lakes. - This false-color mosaic, made from infrared data collected by Nasa's Cassini spacecraft, reveals the differences in the composition of surface materials around hydrocarbon lakes at Titan, Saturn's largest moon. Titan is the only other place in the solar system that we know has stable liquid on its surface, though its lakes are made of liquid ethane and methane rather than liquid water. While there is one large lake and a few smaller ones near Titan's south pole, almost all of Titan's lakes appear near the moon's north pole - Scientists mapped near-infrared colors onto the visible color spectrum. Red in this image was assigned a wavelength of 5 microns (10 times longer than visible light), green 2.0 microns (four times longer than visible light), and blue 1.3 microns (2.6 times longer than visible light) - The orange

Titan, Saturn satellite seen by Cassini: Visible and infrared composite image of Titan taken by the Cassini probe on September 12, 2013. View of methane and ethane lakes. - This false-color mosaic, made from infrared data collected by Nasa's Cassini spacecraft, reveals the differences in the composition of surface materials around hydrocarbon lakes at Titan, Saturn's largest moon. Titan is the only other place in the solar system that we know has stable liquid on its surface, though its lakes are made of liquid ethane and methane rather than liquid water. While there is one large lake and a few smaller ones near Titan's south pole, almost all of Titan's lakes appear near the moon's north pole - Scientists mapped near-infrared colors onto the visible color spectrum. Red in this image was assigned a wavelength of 5 microns (10 times longer than visible light), green 2.0 microns (four times longer than visible light), and blue 1.3 microns (2.6 times longer than visible light) - The orange

PIX4625336

Curfew (engraving)

Curfew (engraving)

English School, (19th century)

LLM2797552

Jacqueline Kennedy exhibits an ease and serenity on horseback which can be equalled by very few women of her generation. New York.

Jacqueline Kennedy exhibits an ease and serenity on horseback which can be equalled by very few women of her generation. New York.

UIG3730872

Bok's cells in NGC 281 (Cassiopee) - Bok globules in NGC 281 - View of a detail of the nebula NGC 281 in Cassiopee center on Bok's Globules. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. Near these blood cells shine blue stars; they belong to the young cluster of stars IC 1590. Image obtained by the Hubble Space Telescope in October 2005. These opaque, dark knots of gas and dust are called “” Bok globules,””” and they are absorbing light in the center of the nearby emission nebula and star - forming region. Bok hypothesized that giant molecular clouds, on the order of hundreds of light - years in size, can become perturbed and form small pockets where the dust and gas are highly concentrated. These small pockets become gravitationally bound and accumulate dust and gas from the surrounding area. If they can capture enough mass, they have the potential of creating stars in their cores; however, no

Bok's cells in NGC 281 (Cassiopee) - Bok globules in NGC 281 - View of a detail of the nebula NGC 281 in Cassiopee center on Bok's Globules. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. Near these blood cells shine blue stars; they belong to the young cluster of stars IC 1590. Image obtained by the Hubble Space Telescope in October 2005. These opaque, dark knots of gas and dust are called “” Bok globules,””” and they are absorbing light in the center of the nearby emission nebula and star - forming region. Bok hypothesized that giant molecular clouds, on the order of hundreds of light - years in size, can become perturbed and form small pockets where the dust and gas are highly concentrated. These small pockets become gravitationally bound and accumulate dust and gas from the surrounding area. If they can capture enough mass, they have the potential of creating stars in their cores; however, no

PIX4617491

Globular cluster NGC 6401 in Ophiuchus - Globular cluster NGC 6401 in Ophiuchus - The NASA/ESA Hubble Space Telescope has used its powerful optics to separate the globular cluster NGC 6401 into its constituent stars. What was once only visible as a ghostly mist in the eyepieces of astronomical instruments has been transformed into a stunning stellar landscape. NGC 6401 can be found within the constellation of Ophiuchus (The Serpent Bearer). The globular cluster itself is relatively faint, so a telescope and some observational experience are required to see it. Globular clusters are very rich, and generally spherical, collections of stars, hence the name. They orbit the cores of galaxies, with the force of gravity also keeping the stars bound as a group. There are around 160 globular clusters associated with our Milky Way, of which NGC 6401 is one. These objects are very old, containing some of the most ancient stars known. However, there are many mysteries surrounding them, with the or

Globular cluster NGC 6401 in Ophiuchus - Globular cluster NGC 6401 in Ophiuchus - The NASA/ESA Hubble Space Telescope has used its powerful optics to separate the globular cluster NGC 6401 into its constituent stars. What was once only visible as a ghostly mist in the eyepieces of astronomical instruments has been transformed into a stunning stellar landscape. NGC 6401 can be found within the constellation of Ophiuchus (The Serpent Bearer). The globular cluster itself is relatively faint, so a telescope and some observational experience are required to see it. Globular clusters are very rich, and generally spherical, collections of stars, hence the name. They orbit the cores of galaxies, with the force of gravity also keeping the stars bound as a group. There are around 160 globular clusters associated with our Milky Way, of which NGC 6401 is one. These objects are very old, containing some of the most ancient stars known. However, there are many mysteries surrounding them, with the or

PIX4564826

Early cars in Belgrave Square, London (b/w photo)

Early cars in Belgrave Square, London (b/w photo)

English Photographer, (20th century)

LLM5987025

Cocoa processing workshop in Kpalime, Togo (photo)

Cocoa processing workshop in Kpalime, Togo (photo)

Philippe Lissac

GNG6279632

The Royal Exchange: Tom pointing out to Jerry a few of the primest features of life in London (coloured engraving)

The Royal Exchange: Tom pointing out to Jerry a few of the primest features of life in London (coloured engraving)

Cruikshank, Isaac Robert (1789-1856) & George (1792-1878)

LLJ586678

Jack the Ripper: Wood's Buildings, Whitechapel Road (photo)

Jack the Ripper: Wood's Buildings, Whitechapel Road (photo)

English Photographer, (20th century)

LLJ607222

Cocoa processing in Kpalime, Togo (photo)

Cocoa processing in Kpalime, Togo (photo)

Philippe Lissac

GNG6279626

Pope Joan (engraving)

Pope Joan (engraving)

English School, (19th century)

LLM5997870

Cocoa processing in Kpalime, Togo (photo)

Cocoa processing in Kpalime, Togo (photo)

Philippe Lissac

GNG6279642

One of the few remaining climbing sweeps (engraving)

One of the few remaining climbing sweeps (engraving)

English School, (19th century)

LLJ604049

satellite view over Northern Australia, shows the northern portion of the Northern Territory, sometimes known as the Top End. There are also a few large islands visible, including Melville and Bathurst Islands to the north and the smaller Groote Eylandt to the east. The Timor Sea is to the west, with the Arafura Sea to the north, and the Gulf of Carpentaria to the east.

satellite view over Northern Australia, shows the northern portion of the Northern Territory, sometimes known as the Top End. There are also a few large islands visible, including Melville and Bathurst Islands to the north and the smaller Groote Eylandt to the east. The Timor Sea is to the west, with the Arafura Sea to the north, and the Gulf of Carpentaria to the east.

UIG529838

Astrolabe about AD 1345 - 1355 An astrolabe is an astronomical instrument that enables the user to determine the time during the day with the help of the sun, and at night with the help of the stars. It can also be used in the preparation of horoscopes and for surveying purposes - to name but a few of its functions.

Astrolabe about AD 1345 - 1355 An astrolabe is an astronomical instrument that enables the user to determine the time during the day with the help of the sun, and at night with the help of the stars. It can also be used in the preparation of horoscopes and for surveying purposes - to name but a few of its functions.

UIG529947

Astrolabe about AD 1345 - 1355 An astrolabe is an astronomical instrument that enables the user to determine the time during the day with the help of the sun, and at night with the help of the stars. It can also be used in the preparation of horoscopes and for surveying purposes - to name but a few of its functions.

Astrolabe about AD 1345 - 1355 An astrolabe is an astronomical instrument that enables the user to determine the time during the day with the help of the sun, and at night with the help of the stars. It can also be used in the preparation of horoscopes and for surveying purposes - to name but a few of its functions.

UIG529946

Planetary nebula CRL 2688 dans le Swan/HST - This image of the Egg Nebula, also known as CRL2688 and located roughly 3,000 light - years from us, was taken in red light with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope.The image shows a pair of mysterious “” searchlight” beams emerging from a hidden star, criss - Yeah. crossed by numerous bright arcs. This image sheds new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. The image is shown in false color. The central star in CRL2688 was a red giant a few hundred years ago. The nebula is really a large cloud of dust and gas ejected by the star, expanding at a speed of 20 km/s (115,000 mph). A dense cocoon of dust (the dark band in the image center) enshrouds the star and hides it from our view. Starlight escapes more easily in directions where the cocoon is thinner, and is reflected towards us by dust particles in the cloud, giving it its

Planetary nebula CRL 2688 dans le Swan/HST - This image of the Egg Nebula, also known as CRL2688 and located roughly 3,000 light - years from us, was taken in red light with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope.The image shows a pair of mysterious “” searchlight” beams emerging from a hidden star, criss - Yeah. crossed by numerous bright arcs. This image sheds new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. The image is shown in false color. The central star in CRL2688 was a red giant a few hundred years ago. The nebula is really a large cloud of dust and gas ejected by the star, expanding at a speed of 20 km/s (115,000 mph). A dense cocoon of dust (the dark band in the image center) enshrouds the star and hides it from our view. Starlight escapes more easily in directions where the cocoon is thinner, and is reflected towards us by dust particles in the cloud, giving it its

PIX4623752

Earth Nut, Fever Few, Knapweed, Frogbit, Fluellin (colour litho)

Earth Nut, Fever Few, Knapweed, Frogbit, Fluellin (colour litho)

English School, (19th century)

LLM6020674

There was a Young Person of Kew, whose virtues and vices were few (litho)

There was a Young Person of Kew, whose virtues and vices were few (litho)

Lear, Edward (1812-88)

LLM966306

'A Few Percussion Common Shell, Passing through the Loose Earth, Exploded in the Pit" (engraving)

'A Few Percussion Common Shell, Passing through the Loose Earth, Exploded in the Pit" (engraving)

English School, (19th century)

LLM666830

View of the Parliamentary buildings from the east (engraving)

View of the Parliamentary buildings from the east (engraving)

English School, (19th century)

LLJ602748

Mexican-American War (1846-48), US recruiting poster, 1846 (engraving)

Mexican-American War (1846-48), US recruiting poster, 1846 (engraving)

American School, (19th century)

PNP3470736

A man from the Stone Age stands amazed at the wonders of the modern world (ie c 1925) (litho)

A man from the Stone Age stands amazed at the wonders of the modern world (ie c 1925) (litho)

English School, (20th century)

LLM5198308

A few young men lost in Glasgow, 1986 (oil on canvas)

A few young men lost in Glasgow, 1986 (oil on canvas)

Conroy, Stephen (b.1964)

NWP3963822

A 17th century parish scene (gouache on paper)

A 17th century parish scene (gouache on paper)

Doughty, C.L. (1913-85)

LLM3641537

Manufatory of Pears' Transparent Soap (engraving)

Manufatory of Pears' Transparent Soap (engraving)

English School, (19th century)

LLJ608723

Charles de France (1523-45), 1524 (pencil on paper)

Charles de France (1523-45), 1524 (pencil on paper)

Clouet, (16th century) (studio of)

CND183099

Bull fighter, taking a few drop of D'Alcool de Menthe de Ricqles (colour litho)

Bull fighter, taking a few drop of D'Alcool de Menthe de Ricqles (colour litho)

Gerbault, Henri (1863-1930)

LLH982917

Compound Headed Kobresia, Creeping Separate-Headed Carex, Prickly Separate-Headed Carex (colour litho)

Compound Headed Kobresia, Creeping Separate-Headed Carex, Prickly Separate-Headed Carex (colour litho)

English School, (19th century)

LLM2797417

FEW Paramount-Duo, 1927, United Kingdom, drawing

FEW Paramount-Duo, 1927, United Kingdom, drawing

DGA2583677

A Shooting Trip at Vigo (engraving)

A Shooting Trip at Vigo (engraving)

English School, (19th century)

LIP1061311

Leaflet advertising the Kineoptikon, Piccadilly Circus (engraving)

Leaflet advertising the Kineoptikon, Piccadilly Circus (engraving)

English School, (19th century)

LLJ607780

Moving house (colour litho)

Moving house (colour litho)

English School, (20th century)

LLM3641733

World War I British poster for the Polish Victims Relief Fund, 1915. Homeless Polish men, women and children carry their few possessions away from a burning village.

World War I British poster for the Polish Victims Relief Fund, 1915. Homeless Polish men, women and children carry their few possessions away from a burning village.

UIG528535

En Route to Bulawayo (b/w photo)

En Route to Bulawayo (b/w photo)

English Photographer, (19th century)

LLM3092347

One of the Few, 1944 (oil on canvas)

One of the Few, 1944 (oil on canvas)

Lush Parry, Ted (1912-93)

NWP3963844

British Wild or Park cattle. Ancient breed surviving in a few small herds in Britain through having been enparked centuries ago. Those shown here are the Hamilton strain (Scottish). The Chillingham is another (English) strain. From William Jardine The Na

British Wild or Park cattle. Ancient breed surviving in a few small herds in Britain through having been enparked centuries ago. Those shown here are the Hamilton strain (Scottish). The Chillingham is another (English) strain. From William Jardine The Na

UIG530751

Trolling for Blue Fish, Currier & Ives, Lithograph, 1866

Trolling for Blue Fish, Currier & Ives, Lithograph, 1866

GLH710444

Air Raid Precautions: Set of 50 cards issued by WD & H0 Wills, Britain 1938, in preparation for the anticipated coming of World War II. Choosing Your Refuge Room in various types of house. Cellar or basement best: if none, use ground floor room with as few windows and outside walls as possible.

Air Raid Precautions: Set of 50 cards issued by WD & H0 Wills, Britain 1938, in preparation for the anticipated coming of World War II. Choosing Your Refuge Room in various types of house. Cellar or basement best: if none, use ground floor room with as few windows and outside walls as possible.

UIG532492

Bombario, the Hunchback, who was used as a Writing-Desk by the Brokers and who, in this Way, earned Pound 6000 in a few days (engraving)

Bombario, the Hunchback, who was used as a Writing-Desk by the Brokers and who, in this Way, earned Pound 6000 in a few days (engraving)

French School, (19th century)

LLM725395

Mr A Merger Hogg is taking a few day's much-needed rest at his country home (litho)

Mr A Merger Hogg is taking a few day's much-needed rest at his country home (litho)

Gibson, Charles Dana (1867-1944)

LLM5209547

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