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Bilder zu 'Heart' gefunden, 10,846

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Inside the archaeological complex of Machu Picchu, Peru (photo)

Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584743

Peru Machu Picchu (photo)

Peru Machu Picchu (photo)

Sergi Reboredo

SRB3585204

Terraces inside the archaeological complex of Machu Picchu, Peru (photo)

Terraces inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584747

Planetary nebula M57 (NGC 6720) in Lyra - M57 (NGC 6720) planetary nebula in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained by different telescopes. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Planetary nebula are shells of gas shed by stars late in their life cycles after using up all of their nuclear fuel. The star then ejects a significant portion of its mass in a gaseous shell, which is illuminated by its extremely

Planetary nebula M57 (NGC 6720) in Lyra - M57 (NGC 6720) planetary nebula in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained by different telescopes. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Planetary nebula are shells of gas shed by stars late in their life cycles after using up all of their nuclear fuel. The star then ejects a significant portion of its mass in a gaseous shell, which is illuminated by its extremely

PIX4623359

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

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

Total Eclipse of Moon 27 - 09 - 1996 - Total lunar eclipse September 27, 1996 - This montage illustrates the progression of the Moon in Earth's shadow cone. The image on the right corresponds to its complete entry into the shadow (beginning of the totalite), the central at the maximum of the totalite and the one on the left at the end of the totalite. During this eclipse, the southern pole of the Moon is passing a little above the center of the Earth's shadow cone. Thus, the southern pole of the Moon is the darkest, while the north pole is brighter. Note the color degrade for the right and left poses: from dark red towards the center of the shadow cone to white on the periphery of this cone, with an intermediate greenish orange degrade. This highlights the fact that blue is more diffuse than green by the Earth's atmosphere - hence the absence of blue on the image, because this color is lost in the Earth's atmosphere and therefore does not reach the surface of the Moon - and that green

Total Eclipse of Moon 27 - 09 - 1996 - Total lunar eclipse September 27, 1996 - This montage illustrates the progression of the Moon in Earth's shadow cone. The image on the right corresponds to its complete entry into the shadow (beginning of the totalite), the central at the maximum of the totalite and the one on the left at the end of the totalite. During this eclipse, the southern pole of the Moon is passing a little above the center of the Earth's shadow cone. Thus, the southern pole of the Moon is the darkest, while the north pole is brighter. Note the color degrade for the right and left poses: from dark red towards the center of the shadow cone to white on the periphery of this cone, with an intermediate greenish orange degrade. This highlights the fact that blue is more diffuse than green by the Earth's atmosphere - hence the absence of blue on the image, because this color is lost in the Earth's atmosphere and therefore does not reach the surface of the Moon - and that green

Laurent Laveder

PIX4579217

Fountain from the Monastery of Saint-Michel-de-Cuxa, Roussillon, France, 1125-50 (marble)

Fountain from the Monastery of Saint-Michel-de-Cuxa, Roussillon, France, 1125-50 (marble)

French School, (12th century)

PHL434225

Markarian Galaxy 817 - Galaxy Markarian 817 - The spiral galaxy Markarian 817 is located 430 million light years ago in the constellation Dragon. This galaxy houses in its heart a supermassive black hole. Image obtained by the Hubble Space Telescope on August 2, 2009. Rings of brilliant blue stars encircle the bright, active core of this spiral galaxy, whose monster black hole is blasting material into space at over 14 million kilometers per hour. Viewed nearly face - on, the galaxy, called Markarian 817, shows intense star - forming regions and dark bands of interstellar dust along its spiral arms. Observations by the new Cosmic Origins Spectrograph (COS) aboard the NASA/ESA Hubble Space Telescope captured the powerful outflow of material from this galaxy. The COS spectrum of Markarian 817 highlights the outflow's dynamic nature. A gas cloud containing hydrogen that was detected in Hubble data taken in 1997 does not appear in the COS observation because the cloud has apparently been d

Markarian Galaxy 817 - Galaxy Markarian 817 - The spiral galaxy Markarian 817 is located 430 million light years ago in the constellation Dragon. This galaxy houses in its heart a supermassive black hole. Image obtained by the Hubble Space Telescope on August 2, 2009. Rings of brilliant blue stars encircle the bright, active core of this spiral galaxy, whose monster black hole is blasting material into space at over 14 million kilometers per hour. Viewed nearly face - on, the galaxy, called Markarian 817, shows intense star - forming regions and dark bands of interstellar dust along its spiral arms. Observations by the new Cosmic Origins Spectrograph (COS) aboard the NASA/ESA Hubble Space Telescope captured the powerful outflow of material from this galaxy. The COS spectrum of Markarian 817 highlights the outflow's dynamic nature. A gas cloud containing hydrogen that was detected in Hubble data taken in 1997 does not appear in the COS observation because the cloud has apparently been d

PIX4613665

Fountain from the Monastery of Saint-Michel-de-Cuxa, Roussillon, France, 1125-50 (marble)

Fountain from the Monastery of Saint-Michel-de-Cuxa, Roussillon, France, 1125-50 (marble)

French School, (12th century)

PHL434224

Fountain from the Monastery of Saint-Michel-de-Cuxa, Roussillon, France, 1125-50 (marble)

Fountain from the Monastery of Saint-Michel-de-Cuxa, Roussillon, France, 1125-50 (marble)

French School, (12th century)

PHL434223

Fountain from the Monastery of Saint-Michel-de-Cuxa, Roussillon, France, 1125-50 (marble)

Fountain from the Monastery of Saint-Michel-de-Cuxa, Roussillon, France, 1125-50 (marble)

French School, (12th century)

PHL434226

Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula (M57) in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Despite their name, planetary nebulae have nothing to do with planets. They were named originally because their discoverers observed them visually and they did not appear as stellar point sources, but rather as small diffuse objects that resembled the outer planets in our solar system such

Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula (M57) in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Despite their name, planetary nebulae have nothing to do with planets. They were named originally because their discoverers observed them visually and they did not appear as stellar point sources, but rather as small diffuse objects that resembled the outer planets in our solar system such

Jerry Lodriguss

PIX4623312

Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula (M57) in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Despite their name, planetary nebulae have nothing to do with planets. They were named originally because their discoverers observed them visually and they did not appear as stellar point sources, but rather as small diffuse objects that resembled the outer planets in our solar system such

Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula (M57) in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Despite their name, planetary nebulae have nothing to do with planets. They were named originally because their discoverers observed them visually and they did not appear as stellar point sources, but rather as small diffuse objects that resembled the outer planets in our solar system such

Sebastian Voltmer

PIX4623321

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

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

Auckland Region (New Zealand) satellite view - Auckland, New Zealand - Auckland Region, the largest urban area in New Zealand, in the North Island, viewed by Landsat satellite - 7 August 27, 2002. Auckland, New Zealand's largest city, is located on the country's North Island. Nearly a third of New Zealand's population lives in Auckland - - more than three million people. This natural - color (photo - like) image of Auckland was acquired on August 27, 2002, by Nasa's Landsat 7 satellite. The most densely developed areas appear white and gray, while suburban areas appear grayish green - - a mixture of houses, streets, and lawns. The city spreads out across various peninsulas surrounding Tamaki Strait and other bays and inlets. The city has been built up around the Auckland Volcanic Field; within a 20 - kilometer (12.4 - mile) radius of the heart of the city, there are 49 volcanoes, most of them small cones less than 150 meters (492 feet) high. Many of them have been protected as parks or

Auckland Region (New Zealand) satellite view - Auckland, New Zealand - Auckland Region, the largest urban area in New Zealand, in the North Island, viewed by Landsat satellite - 7 August 27, 2002. Auckland, New Zealand's largest city, is located on the country's North Island. Nearly a third of New Zealand's population lives in Auckland - - more than three million people. This natural - color (photo - like) image of Auckland was acquired on August 27, 2002, by Nasa's Landsat 7 satellite. The most densely developed areas appear white and gray, while suburban areas appear grayish green - - a mixture of houses, streets, and lawns. The city spreads out across various peninsulas surrounding Tamaki Strait and other bays and inlets. The city has been built up around the Auckland Volcanic Field; within a 20 - kilometer (12.4 - mile) radius of the heart of the city, there are 49 volcanoes, most of them small cones less than 150 meters (492 feet) high. Many of them have been protected as parks or

PIX4675653

Blue stragglers in cluster 47 Toucan - Blue stragglers in globular cluster 47 Tucanae - This image obtained by the Hubble space telescope shows a detail of the 47 Toucan cluster near its center (the field is indicated on the left image taken from the ground). The yellow circles on the right image indicate the position of stars identified by the telescope as blue trainers. Because of the high density of stars within a globular cluster, a collision between two stars sometimes occurs, merging into a single young, bright and warm star called a blue straggler. The core of globular cluster 47 Tucanae is home to many blue stragglers, rejuvenated stars that glow with the blue light of young stars. A ground - based telescope image (on the left) shows the entire crowded core of 47 Tucanae, located 15,000 light - years away in the constellation Tucana. Peering into the heart of the globular cluster's bright core, the Hubble Space Telescope's Wide Field and Planetary Camera 2 separated the dense c

Blue stragglers in cluster 47 Toucan - Blue stragglers in globular cluster 47 Tucanae - This image obtained by the Hubble space telescope shows a detail of the 47 Toucan cluster near its center (the field is indicated on the left image taken from the ground). The yellow circles on the right image indicate the position of stars identified by the telescope as blue trainers. Because of the high density of stars within a globular cluster, a collision between two stars sometimes occurs, merging into a single young, bright and warm star called a blue straggler. The core of globular cluster 47 Tucanae is home to many blue stragglers, rejuvenated stars that glow with the blue light of young stars. A ground - based telescope image (on the left) shows the entire crowded core of 47 Tucanae, located 15,000 light - years away in the constellation Tucana. Peering into the heart of the globular cluster's bright core, the Hubble Space Telescope's Wide Field and Planetary Camera 2 separated the dense c

PIX4564265

Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope and the Large Binocular Telescope. In this composite image, visible - light observations by Nasa's Hubble Space Telescope are combined with infrared data from the ground - based Large Binocular Telescope in Arizona to assemble a dramatic view of the well - known Ring Nebula. Called a planetary nebula, the Ring Nebula is the glowing remains of a Sun - like star. The object is tilted towards Earth so that astronomers see the ring face - on. The Hubble observations reveal that the nebula's shape is more complicated than astronomers thought. The blue gas in the nebula's center is actually a football - shaped structure that pierces the red doug

Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope and the Large Binocular Telescope. In this composite image, visible - light observations by Nasa's Hubble Space Telescope are combined with infrared data from the ground - based Large Binocular Telescope in Arizona to assemble a dramatic view of the well - known Ring Nebula. Called a planetary nebula, the Ring Nebula is the glowing remains of a Sun - like star. The object is tilted towards Earth so that astronomers see the ring face - on. The Hubble observations reveal that the nebula's shape is more complicated than astronomers thought. The blue gas in the nebula's center is actually a football - shaped structure that pierces the red doug

PIX4623411

Mir station 01/1997 - Mir station seen from the shuttle Atlantis before docking 01/1997 - Mir space station seen from the shuttle Atlantis approaching for mooring. 14/01/1997. In the upper center: a Progress ship, the Kvant module - and the central module; centre left: the Priroda module; centre right: the Spektr module; bottom left: the Kvant module - 2; centre low: a Soyuz ship; bottom right, the Kristall module and the mooring module. This is a view of the Russian Mir Space Station photographed by a crewmember of the fifth Shuttle/Mir docking mission, STS-81. The image shows: upper center - Progress supply vehicle, Kvant - 1 module, and Core module; center left - Priroda module; center right - Spektr module; bottom left - Kvant - 2 module; bottom center - Soyuz; and bottom right - Kristall module and Docking module. The Progress was an unmarned, automated version of the Soyuz crew transfer vehicle, designed to resupply the Mir. The Kvant - 1 provided research in the physics of galax

Mir station 01/1997 - Mir station seen from the shuttle Atlantis before docking 01/1997 - Mir space station seen from the shuttle Atlantis approaching for mooring. 14/01/1997. In the upper center: a Progress ship, the Kvant module - and the central module; centre left: the Priroda module; centre right: the Spektr module; bottom left: the Kvant module - 2; centre low: a Soyuz ship; bottom right, the Kristall module and the mooring module. This is a view of the Russian Mir Space Station photographed by a crewmember of the fifth Shuttle/Mir docking mission, STS-81. The image shows: upper center - Progress supply vehicle, Kvant - 1 module, and Core module; center left - Priroda module; center right - Spektr module; bottom left - Kvant - 2 module; bottom center - Soyuz; and bottom right - Kristall module and Docking module. The Progress was an unmarned, automated version of the Soyuz crew transfer vehicle, designed to resupply the Mir. The Kvant - 1 provided research in the physics of galax

PIX4642225

Eagle Nebula (IC 4703) in the Snake - detail - Young stars in the Eagle nebula - Detail on young stars located in the north - west part of the Eagle Nebula (M16). Image obtained by the Hubble Space Telescope. This picture shows the northwestern part of the Eagle nebula (M16), well away from the centre, and features some very bright young stars that formed from the same cloud of material. These energetic toddlers are part of an open cluster and emit ultraviolet radiation that causes the surrounding nebula to glow. The star cluster is very bright and was discovered in the mid - eighteenth century. The nebula, however, is much more elusive and it took almost a further two decades for it to be first noted by Charles Messier in 1764. Although it is commonly known as the Eagle Nebula, its official designation is Messier 16 and the cluster is also named NGC 6611. One spectacular area of the nebula (outside the field of view) has been nicknamed The Pillars of Creation”” ever since the Hubble S

Eagle Nebula (IC 4703) in the Snake - detail - Young stars in the Eagle nebula - Detail on young stars located in the north - west part of the Eagle Nebula (M16). Image obtained by the Hubble Space Telescope. This picture shows the northwestern part of the Eagle nebula (M16), well away from the centre, and features some very bright young stars that formed from the same cloud of material. These energetic toddlers are part of an open cluster and emit ultraviolet radiation that causes the surrounding nebula to glow. The star cluster is very bright and was discovered in the mid - eighteenth century. The nebula, however, is much more elusive and it took almost a further two decades for it to be first noted by Charles Messier in 1764. Although it is commonly known as the Eagle Nebula, its official designation is Messier 16 and the cluster is also named NGC 6611. One spectacular area of the nebula (outside the field of view) has been nicknamed The Pillars of Creation”” ever since the Hubble S

PIX4620062

Interacting galaxies NGC 2936 and NGC 2937 - Interacting Galaxies NGC 2936 and NGC 2937 in Hydra - These two interacting galaxies also called Arp 142 are located approximately 326 million years ago - light from Earth in the constellation Hydra. NGC 2936 is a spiral galaxy, NGC 2937 is an elliptical galaxy. Above the torque, a blue galaxy UGC 5130, located closer to us is 230 million light years. Image obtained by the Hubble Space Telescope (HST). This interacting galaxy duo is collectively called Arp 142. The pair contains the disturbed, star - forming spiral galaxy NGC 2936, along with its elliptical companion, NGC 2937 at lower left. Once part of a flat, spiral disk, the orbits of the galaxy's stars have become scrambled due to gravitational tidal interactions with the other galaxy. This warps the galaxy's orderly spiral, and interstellar gas is strewn out into giant tails like stretched taffy. Gas and dust drawn from the heart of NGC 2936 becomes compressed during the encounter, whi

Interacting galaxies NGC 2936 and NGC 2937 - Interacting Galaxies NGC 2936 and NGC 2937 in Hydra - These two interacting galaxies also called Arp 142 are located approximately 326 million years ago - light from Earth in the constellation Hydra. NGC 2936 is a spiral galaxy, NGC 2937 is an elliptical galaxy. Above the torque, a blue galaxy UGC 5130, located closer to us is 230 million light years. Image obtained by the Hubble Space Telescope (HST). This interacting galaxy duo is collectively called Arp 142. The pair contains the disturbed, star - forming spiral galaxy NGC 2936, along with its elliptical companion, NGC 2937 at lower left. Once part of a flat, spiral disk, the orbits of the galaxy's stars have become scrambled due to gravitational tidal interactions with the other galaxy. This warps the galaxy's orderly spiral, and interstellar gas is strewn out into giant tails like stretched taffy. Gas and dust drawn from the heart of NGC 2936 becomes compressed during the encounter, whi

PIX4610249

The King Carl XVI Gustaf with crown princess Victoria, 1980 (photo)

The King Carl XVI Gustaf with crown princess Victoria, 1980 (photo)

SJB7350073

Anne of Denmark, c.1611-12 (w/c on vellum laid on playing card (ace of clubs))

Anne of Denmark, c.1611-12 (w/c on vellum laid on playing card (ace of clubs))

Oliver, Isaac (c.1565-1617)

ROC3707675

Portrait of a Gentleman, c.1600 (oil on panel)

Portrait of a Gentleman, c.1600 (oil on panel)

English School, (17th century)

MOU4073718

Crab Pulsar in Nebula M1 - The Crab pulsar: This false-colored image obtained by the Hubble Space Telescope shows the central region of the Crab Nebula or resides its pulsar. The pulsar is visible in the center of the image. It is a very dense neutron star from the explosion of a massive supernova star. This star quickly rotates on itself developing a powerful magnetic field, emitting beams of light and radio waves. M1 is located about 6000 light-years in the constellation Taurus.. In 1054 AD, during the Song dynasty, Chinese astronomers spotted a bright new star in the night sky. This newcomer turned out to be a violent explosion within the Milky Way, caused by the spectacular death of a star some 1600 light-years away. This explosion created one of the most well-studied and beautiful objects in the night sky - the Crab Nebula. The beautiful result of this cataclysmic Type II supernova is shown here, imaged by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys. Unlike m

Crab Pulsar in Nebula M1 - The Crab pulsar: This false-colored image obtained by the Hubble Space Telescope shows the central region of the Crab Nebula or resides its pulsar. The pulsar is visible in the center of the image. It is a very dense neutron star from the explosion of a massive supernova star. This star quickly rotates on itself developing a powerful magnetic field, emitting beams of light and radio waves. M1 is located about 6000 light-years in the constellation Taurus.. In 1054 AD, during the Song dynasty, Chinese astronomers spotted a bright new star in the night sky. This newcomer turned out to be a violent explosion within the Milky Way, caused by the spectacular death of a star some 1600 light-years away. This explosion created one of the most well-studied and beautiful objects in the night sky - the Crab Nebula. The beautiful result of this cataclysmic Type II supernova is shown here, imaged by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys. Unlike m

PIX4583169

Desert of Libya seen by Envisat 11 - 2004 - Libyan dunes fields seen by Envisat. - The desert of Libya observed by ENVISAT satellite on November 24, 2004. The image covers an area 672 km wide and shows the two huge dune fields located south-west of Libya in the Fezzan Desert. At the top of the picture, the Ubari erg (or Awbari) appears reddish. In the middle, Murzuk erg. This Envisat image shows two huge sand dune seas in the Fezzan region of southwestern Libya, close to the border with Algeria. Most of the face of the Sahara desert stretching across Northern Africa is bare stone and pebbles rather than sand dunes, but there are exceptions - sprawling seas of multi - storey sand dunes known as 'ergs'. The Erg Ubari (also called Awbari) is the reddish sand sea towards the top of the image. A dark outcrop of Nubian sandstone separates the Erg Ubari sand from the Erg Murzuq (also called Murzuk) further south. A persistent high - pressure zone centred over Libya keeps the heart of the Saha

Desert of Libya seen by Envisat 11 - 2004 - Libyan dunes fields seen by Envisat. - The desert of Libya observed by ENVISAT satellite on November 24, 2004. The image covers an area 672 km wide and shows the two huge dune fields located south-west of Libya in the Fezzan Desert. At the top of the picture, the Ubari erg (or Awbari) appears reddish. In the middle, Murzuk erg. This Envisat image shows two huge sand dune seas in the Fezzan region of southwestern Libya, close to the border with Algeria. Most of the face of the Sahara desert stretching across Northern Africa is bare stone and pebbles rather than sand dunes, but there are exceptions - sprawling seas of multi - storey sand dunes known as 'ergs'. The Erg Ubari (also called Awbari) is the reddish sand sea towards the top of the image. A dark outcrop of Nubian sandstone separates the Erg Ubari sand from the Erg Murzuq (also called Murzuk) further south. A persistent high - pressure zone centred over Libya keeps the heart of the Saha

PIX4658993

Supernova Sn 2004dj in the galaxy NGC 2403 - The explosion of a massive star blazes with the light of 200 million Suns in this NASA Hubble Space Telescope image. The supernova is so bright in this image that it easily could be mistaken for a foreground star in our Milky Way Galaxy. And yet, this supernova, called SN 2004dj, resides far beyond our galaxy. Its home is in the outskirts of NGC 2403, a galaxy located 11 million light - years from Earth. Although the supernova is far from Earth, it is the closest stellar explosion discovered in more than a decade. The star that became SN 2004dj may have been about 15 times as massive as the Sun, and only about 14 million years old. (Massive stars live much shorter lives than the Sun; they have more fuel to “” burn”” through nuclear fusion, but they use it up at a disproportionately faster rate.) The large number of massive stars in NGC 2403 leads to a high supernova rate. Two other supernovae have been seen in this galaxy during the past hal

Supernova Sn 2004dj in the galaxy NGC 2403 - The explosion of a massive star blazes with the light of 200 million Suns in this NASA Hubble Space Telescope image. The supernova is so bright in this image that it easily could be mistaken for a foreground star in our Milky Way Galaxy. And yet, this supernova, called SN 2004dj, resides far beyond our galaxy. Its home is in the outskirts of NGC 2403, a galaxy located 11 million light - years from Earth. Although the supernova is far from Earth, it is the closest stellar explosion discovered in more than a decade. The star that became SN 2004dj may have been about 15 times as massive as the Sun, and only about 14 million years old. (Massive stars live much shorter lives than the Sun; they have more fuel to “” burn”” through nuclear fusion, but they use it up at a disproportionately faster rate.) The large number of massive stars in NGC 2403 leads to a high supernova rate. Two other supernovae have been seen in this galaxy during the past hal

PIX4582457

Irregular dwarf galaxy I Zwicky 18 - Irregular dwarf galaxy I Zwicky 18 - The irregular dwarf galaxy I Zwicky 18 is located 59 million years - light in the Great Bear and extends over about 3000 years - light. The two bright white spots are star-forming regions. At the top left, another galaxy is visible. This galaxy could be interacting with I Zwicky 18. This image is the result of observations made by the Hubble Space Telescope in 2005 and 2006. Called I Zwicky 18, this galaxy has a youthful appearance that resembles galaxies typically found only in the early universe. Hubble has now found faint, older stars within this galaxy, suggesting that the galaxy may have formed at the same time as most other galaxies. I Zwicky 18 is classified as a dwarf irregular galaxy and is much smaller than our Milky Way Galaxy. The concentrated bluish - white knots embedded in the heart of the galaxy are two major starburst regions where stars are forming at a furious rate. The wispy blue filaments sur

Irregular dwarf galaxy I Zwicky 18 - Irregular dwarf galaxy I Zwicky 18 - The irregular dwarf galaxy I Zwicky 18 is located 59 million years - light in the Great Bear and extends over about 3000 years - light. The two bright white spots are star-forming regions. At the top left, another galaxy is visible. This galaxy could be interacting with I Zwicky 18. This image is the result of observations made by the Hubble Space Telescope in 2005 and 2006. Called I Zwicky 18, this galaxy has a youthful appearance that resembles galaxies typically found only in the early universe. Hubble has now found faint, older stars within this galaxy, suggesting that the galaxy may have formed at the same time as most other galaxies. I Zwicky 18 is classified as a dwarf irregular galaxy and is much smaller than our Milky Way Galaxy. The concentrated bluish - white knots embedded in the heart of the galaxy are two major starburst regions where stars are forming at a furious rate. The wispy blue filaments sur

PIX4613873

Scott Glenn, Anthony Hopkins And Jodie Foster.

Scott Glenn, Anthony Hopkins And Jodie Foster.

DIL4059926

The Silence of the Lambs by Jonathan Demme, 1991

The Silence of the Lambs by Jonathan Demme, 1991

DIL4059923

The Silence of the Lambs by Jonathan Demme, 1991

The Silence of the Lambs by Jonathan Demme, 1991

DIL4059929

The Silence of the Lambs by Jonathan Demme, 1991

The Silence of the Lambs by Jonathan Demme, 1991

DIL4059930

The Silence of the Lambs by Jonathan Demme, 1991

The Silence of the Lambs by Jonathan Demme, 1991

DIL4059928

Scott Glenn And Jodie Foster

Scott Glenn And Jodie Foster

DIL4059925

Anthony Hopkins, Jodie Foster And Scott Glenn.

Anthony Hopkins, Jodie Foster And Scott Glenn.

DIL4059927

Queen Victoria, 1841 (w/c on ivory laid on card)

Queen Victoria, 1841 (w/c on ivory laid on card)

Ross, William Charles (1794-1860)

ROC5891821

The Unannounced Return by Night of L. Tarquinius Collatinus and his Companions to find his Wife Lucretia Weaving (oil on canvas)

The Unannounced Return by Night of L. Tarquinius Collatinus and his Companions to find his Wife Lucretia Weaving (oil on canvas)

Baleschoux, Jehan Balechouse John (fl.1570) (attr.to)

USB1161917

Eyewitness News Library: April 4, 1978 7PM and 11PM

Eyewitness News Library: April 4, 1978 7PM and 11PM

MOV8614352

Eyewitness News Library: April 6, 1978 6PM

Eyewitness News Library: April 6, 1978 6PM

MOV8614354

(First section) A medallion, partly damaged but containing some drawing in the lower half, atop a blank panel. - a monk-like figure reclining on a grassy platform, clothed in a white hooded robe, with his left eye closed; an angel standing at his feet, bearing a platter of unidentified objects. - a monk-like figure reclining on a grassy platform, clothed in a white hooded robe, awake; an angel standing at his feet, bearing a platter containing a heart with a knife stuck in it. A speech scroll accompanies the angel; the text is partially legible: 'Collirio inunge oculus tuos vi videns'. - a scroll, bearing a largely illegible inscription (from Ashmole Roll 53: 'Est lapis occultus secreto fonte sepultus fermentu variat lapide qui conta colora'); beneath, a frog. (There is a join at this location between two sheets of paper. Comparison with Ashmole Roll 53 shows a small section is missing.) - within a ribboned section, seven roundels connected by laureal wreaths/ropes to a central red sha

(First section) A medallion, partly damaged but containing some drawing in the lower half, atop a blank panel. - a monk-like figure reclining on a grassy platform, clothed in a white hooded robe, with his left eye closed; an angel standing at his feet, bearing a platter of unidentified objects. - a monk-like figure reclining on a grassy platform, clothed in a white hooded robe, awake; an angel standing at his feet, bearing a platter containing a heart with a knife stuck in it. A speech scroll accompanies the angel; the text is partially legible: 'Collirio inunge oculus tuos vi videns'. - a scroll, bearing a largely illegible inscription (from Ashmole Roll 53: 'Est lapis occultus secreto fonte sepultus fermentu variat lapide qui conta colora'); beneath, a frog. (There is a join at this location between two sheets of paper. Comparison with Ashmole Roll 53 shows a small section is missing.) - within a ribboned section, seven roundels connected by laureal wreaths/ropes to a central red sha

BL3292691

The Road to Emmaus, 2009 (oil on canvas)

premium — The Road to Emmaus, 2009 (oil on canvas)

The Road to Emmaus, 2009 (oil on canvas)

Adcock, Rosemarie

RAD8926474

Inauguration of Ronald Reagan 1985

Inauguration of Ronald Reagan 1985

BOF6289618

Victoria Cross, 2nd Lieutenant R P Hallowes, Duke of Cambridge's Own (Middlesex Regiment), 1915 (metal)

Victoria Cross, 2nd Lieutenant R P Hallowes, Duke of Cambridge's Own (Middlesex Regiment), 1915 (metal)

British School, (20th century)

NAM5921596

Victoria Cross, 2nd Lieutenant R P Hallowes, Duke of Cambridge's Own (Middlesex Regiment), 1915 (metal)

Victoria Cross, 2nd Lieutenant R P Hallowes, Duke of Cambridge's Own (Middlesex Regiment), 1915 (metal)

British School, (20th century)

NAM5921595

Release Of Watergate Tapes - President Richard M. Nixon

Release Of Watergate Tapes - President Richard M. Nixon

BOF7336651

Gold Memorial Ring, Silver Buckle, Crystal and Gold Locket, Diamond Locket, Gold Pendant, Sleeve Links of Silver, Silver Heart-Shaped Pendant, Spar Snuff-Bottle, Gold Ring, Gold Memorial Ring, Crystal Locket, Gold Crucifix (chromolitho)

Gold Memorial Ring, Silver Buckle, Crystal and Gold Locket, Diamond Locket, Gold Pendant, Sleeve Links of Silver, Silver Heart-Shaped Pendant, Spar Snuff-Bottle, Gold Ring, Gold Memorial Ring, Crystal Locket, Gold Crucifix (chromolitho)

English School, (19th century)

LLM2812043

The Duke of Burgundy providing a sumptuous feast for Louis, Dauphin of France (colour litho)

The Duke of Burgundy providing a sumptuous feast for Louis, Dauphin of France (colour litho)

Job, pseudonym for Onfray de Breville, Jacques (1858-1931)

LLM3621674

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