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The promenade planted on the High Line in New York (New York), United States (United States). Photography 26/09/10
The promenade planted on the High Line in New York (New York), United States (United States). Photography 26/09/10

TEC4612174: The promenade planted on the High Line in New York (New York), United States (United States). Photography 26/09/10 / Bridgeman Images

Centaurus A elliptical galaxy (NGC 5128) in Centaurus - Elliptical galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This giant galaxy is a powerful radio source known as Centaurus A. NGC 5128 is the nearest large elliptical galaxies to our sun located at about 13 million light years. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky
Centaurus A elliptical galaxy (NGC 5128) in Centaurus - Elliptical galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This giant galaxy is a powerful radio source known as Centaurus A. NGC 5128 is the nearest large elliptical galaxies to our sun located at about 13 million light years. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky

PIX4612265: Centaurus A elliptical galaxy (NGC 5128) in Centaurus - Elliptical galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This giant galaxy is a powerful radio source known as Centaurus A. NGC 5128 is the nearest large elliptical galaxies to our sun located at about 13 million light years. It is also the nearest of the giant radio galaxies, possessing an active galactic nucleus (AGN) and optically one of the most luminous galaxies in the sky / Bridgeman Images

Centaurus A elliptical galaxy (NGC 5128) in Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This Giant Galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. The green dot visible in the dust strip is a supernova, the supernova 1986g. It appears green because the red filter image that made this trichromy image was only taken a year after the event and the supernova had weakened. Image obtained from the 3.9m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy. The circular, uniformly bright portion is composed of several thousand million stars, most of them old and yellowish. The galaxy is girded by a dense dust lane which obscures and reddens the light of stars behind it. Some younger, blue stars can be seen at the edges of the dust cloud. One of the nearer galaxies, 13 million light years away, Centaurus A is the most powerful nearby radio source and is also a copious source of X - and gamma rays as well as visible and infrared radiation. The curious green star in the dust lane is because the blue and green - light plates were taken when supernova 1986g had just appeared, while the red - light plate was taken a year later when the supernova had faded
Centaurus A elliptical galaxy (NGC 5128) in Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This Giant Galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. The green dot visible in the dust strip is a supernova, the supernova 1986g. It appears green because the red filter image that made this trichromy image was only taken a year after the event and the supernova had weakened. Image obtained from the 3.9m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy. The circular, uniformly bright portion is composed of several thousand million stars, most of them old and yellowish. The galaxy is girded by a dense dust lane which obscures and reddens the light of stars behind it. Some younger, blue stars can be seen at the edges of the dust cloud. One of the nearer galaxies, 13 million light years away, Centaurus A is the most powerful nearby radio source and is also a copious source of X - and gamma rays as well as visible and infrared radiation. The curious green star in the dust lane is because the blue and green - light plates were taken when supernova 1986g had just appeared, while the red - light plate was taken a year later when the supernova had faded

PIX4612278: Centaurus A elliptical galaxy (NGC 5128) in Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. This Giant Galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. The green dot visible in the dust strip is a supernova, the supernova 1986g. It appears green because the red filter image that made this trichromy image was only taken a year after the event and the supernova had weakened. Image obtained from the 3.9m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy. The circular, uniformly bright portion is composed of several thousand million stars, most of them old and yellowish. The galaxy is girded by a dense dust lane which obscures and reddens the light of stars behind it. Some younger, blue stars can be seen at the edges of the dust cloud. One of the nearer galaxies, 13 million light years away, Centaurus A is the most powerful nearby radio source and is also a copious source of X - and gamma rays as well as visible and infrared radiation. The curious green star in the dust lane is because the blue and green - light plates were taken when supernova 1986g had just appeared, while the red - light plate was taken a year later when the supernova had faded / Bridgeman Images

Elliptical galaxy Centaurus A (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128). Wide field - The NGC 5128 galaxy is about 13 million light years away from Earth. Image obtained from the 1.2m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy, set in a rich part of the southern sky. not only are there plenty of stars here to catch the eye, but the region is rich in galaxies as well. One of the nearer galaxies, at 13 million light years away, Centaurus A is the most powerful nearby radio source and is also a copious source of X - and gamma rays as well as visible and infrared radiation
Elliptical galaxy Centaurus A (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128). Wide field - The NGC 5128 galaxy is about 13 million light years away from Earth. Image obtained from the 1.2m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy, set in a rich part of the southern sky. not only are there plenty of stars here to catch the eye, but the region is rich in galaxies as well. One of the nearer galaxies, at 13 million light years away, Centaurus A is the most powerful nearby radio source and is also a copious source of X - and gamma rays as well as visible and infrared radiation

PIX4612296: Elliptical galaxy Centaurus A (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128). Wide field - The NGC 5128 galaxy is about 13 million light years away from Earth. Image obtained from the 1.2m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy, set in a rich part of the southern sky. not only are there plenty of stars here to catch the eye, but the region is rich in galaxies as well. One of the nearer galaxies, at 13 million light years away, Centaurus A is the most powerful nearby radio source and is also a copious source of X - and gamma rays as well as visible and infrared radiation / Bridgeman Images

Chelsea district, New York (New York), United States (USA).
Chelsea district, New York (New York), United States (USA).

TEC4612307: Chelsea district, New York (New York), United States (USA). / Bridgeman Images

Detail of a building in the neighborhood of Chelsea in New York (New York), United States (United States). Photography 26/09/10
Detail of a building in the neighborhood of Chelsea in New York (New York), United States (United States). Photography 26/09/10

TEC4612326: Detail of a building in the neighborhood of Chelsea in New York (New York), United States (United States). Photography 26/09/10 / Bridgeman Images

Spiral galaxy M101 in the Great Bear - Spiral galaxy M101 in constellation Ursa Major - The galaxy M101 (NGC 5457) is located about 27 million years ago - light from Earth. Spiral galaxy M101 is a beautiful, large, face - on spiral galaxy located about 27 million light - year away in the constellation Ursa Major
Spiral galaxy M101 in the Great Bear - Spiral galaxy M101 in constellation Ursa Major - The galaxy M101 (NGC 5457) is located about 27 million years ago - light from Earth. Spiral galaxy M101 is a beautiful, large, face - on spiral galaxy located about 27 million light - year away in the constellation Ursa Major

PIX4612702: Spiral galaxy M101 in the Great Bear - Spiral galaxy M101 in constellation Ursa Major - The galaxy M101 (NGC 5457) is located about 27 million years ago - light from Earth. Spiral galaxy M101 is a beautiful, large, face - on spiral galaxy located about 27 million light - year away in the constellation Ursa Major / Bridgeman Images

Spiral galaxy NGC 5474 in the Great Bear - Spiral galaxy NGC 5474 in Ursa Majo
Spiral galaxy NGC 5474 in the Great Bear - Spiral galaxy NGC 5474 in Ursa Majo

PIX4612755: Spiral galaxy NGC 5474 in the Great Bear - Spiral galaxy NGC 5474 in Ursa Majo / Bridgeman Images

Galaxies NGC 5560, NGC 5566 and NGC 5569 in the Virgin - Galaxies NGC 5560, NGC 5566 and NGC 5569 in Virgo - This group of galaxies also called Arp 286 is located about 80 million years ago - light from Earth in the constellation of the Virgin. At the top is the galaxy NGC 5560, below, in the center, the galaxy NGC 5566, with the galaxy NGC 5569 on the left. This galaxy group is about 80 million light years from Earth in the contellation of Virgo. To the top of the image, the galaxy NGC 5560; below, in center, galaxy NGC 5566 with NGC 5569 to the left
Galaxies NGC 5560, NGC 5566 and NGC 5569 in the Virgin - Galaxies NGC 5560, NGC 5566 and NGC 5569 in Virgo - This group of galaxies also called Arp 286 is located about 80 million years ago - light from Earth in the constellation of the Virgin. At the top is the galaxy NGC 5560, below, in the center, the galaxy NGC 5566, with the galaxy NGC 5569 on the left. This galaxy group is about 80 million light years from Earth in the contellation of Virgo. To the top of the image, the galaxy NGC 5560; below, in center, galaxy NGC 5566 with NGC 5569 to the left

PIX4612765: Galaxies NGC 5560, NGC 5566 and NGC 5569 in the Virgin - Galaxies NGC 5560, NGC 5566 and NGC 5569 in Virgo - This group of galaxies also called Arp 286 is located about 80 million years ago - light from Earth in the constellation of the Virgin. At the top is the galaxy NGC 5560, below, in the center, the galaxy NGC 5566, with the galaxy NGC 5569 on the left. This galaxy group is about 80 million light years from Earth in the contellation of Virgo. To the top of the image, the galaxy NGC 5560; below, in center, galaxy NGC 5566 with NGC 5569 to the left / Bridgeman Images

Lenticular Galaxy M102 (NGC 5866) in the Dragon - Lenticular galaxy M102 (NGC 5866) in Drac
Lenticular Galaxy M102 (NGC 5866) in the Dragon - Lenticular galaxy M102 (NGC 5866) in Drac

PIX4612811: Lenticular Galaxy M102 (NGC 5866) in the Dragon - Lenticular galaxy M102 (NGC 5866) in Drac / Bridgeman Images

Spiral galaxy NGC 5907 in the Dragon - Spiral galaxy NGC 5907 in Draco - The galaxy NGC 5907 is about 35 million years away - light from Earth. Image obtained in 2006 in several cumulative long poses, with a large amateur instrument, a 50 cm telescope. Edge - on spiral galaxy located at 35 million light years away
Spiral galaxy NGC 5907 in the Dragon - Spiral galaxy NGC 5907 in Draco - The galaxy NGC 5907 is about 35 million years away - light from Earth. Image obtained in 2006 in several cumulative long poses, with a large amateur instrument, a 50 cm telescope. Edge - on spiral galaxy located at 35 million light years away

PIX4612832: Spiral galaxy NGC 5907 in the Dragon - Spiral galaxy NGC 5907 in Draco - The galaxy NGC 5907 is about 35 million years away - light from Earth. Image obtained in 2006 in several cumulative long poses, with a large amateur instrument, a 50 cm telescope. Edge - on spiral galaxy located at 35 million light years away / Bridgeman Images

Spiral Galaxies NGC 5963 and NGC 5965 in the Dragon - NGC 5963 and NGC 5965 spiral galaxies in Draco - NGC 5965 is a spiral galaxy seen by the slice located about 179 million years ago - light in the constellation of Dragon. Above it, the spiral galaxy NGC 5963. The edge - on NGC 5965 spiral galaxy located about 179 million light years in the constellation Drago. Just above it, the NGC 5963 galaxy spiral
Spiral Galaxies NGC 5963 and NGC 5965 in the Dragon - NGC 5963 and NGC 5965 spiral galaxies in Draco - NGC 5965 is a spiral galaxy seen by the slice located about 179 million years ago - light in the constellation of Dragon. Above it, the spiral galaxy NGC 5963. The edge - on NGC 5965 spiral galaxy located about 179 million light years in the constellation Drago. Just above it, the NGC 5963 galaxy spiral

PIX4612882: Spiral Galaxies NGC 5963 and NGC 5965 in the Dragon - NGC 5963 and NGC 5965 spiral galaxies in Draco - NGC 5965 is a spiral galaxy seen by the slice located about 179 million years ago - light in the constellation of Dragon. Above it, the spiral galaxy NGC 5963. The edge - on NGC 5965 spiral galaxy located about 179 million light years in the constellation Drago. Just above it, the NGC 5963 galaxy spiral / Bridgeman Images

Spiral Galaxy NGC 6503 in the Dragon - Spiral galaxy NGC 6503 in Draco - The galaxy NGC 6503 is about 16 million years away - light from Earth
Spiral Galaxy NGC 6503 in the Dragon - Spiral galaxy NGC 6503 in Draco - The galaxy NGC 6503 is about 16 million years away - light from Earth

PIX4612930: Spiral Galaxy NGC 6503 in the Dragon - Spiral galaxy NGC 6503 in Draco - The galaxy NGC 6503 is about 16 million years away - light from Earth / Bridgeman Images

Spiral Galaxy M51 in Hunting Dogs and Supernova - The Whirlpool Galaxy (M51) in Canes Venatici with SN 2005cs - The spiral galaxy M51 (NGC 5194) is located about 37 million years ago - light from Earth. This galaxy is double; two galaxies interact: the largest, NGC 5194, the smallest NGC 5195. On June 28, 2005 a supernova of type II appeared in M51; this supernova (SN 2005cs) is visible just under the nucleus, in the first arm. Image obtained with two telescopes of 50 cm and 30 cm, composite of several poses. The Whirlpool Galaxy lies approximately 31 million light years from earth. This spectacular galaxy is paired with a smaller, more distant companion whose matter is being disrupted by the larger spiral in a gravitational tug of war. Eventually, the shape of both will be altered over many more millions of years. On June 28, 2005, a new star was noticed in this galaxy. It was confirmed to be a bright supernova, one of the brightest in recent years and similar to the brightest supernova of modern times: 1987A. This rare event, SN 2005cs, is visible on the first spiral arm, directly below the nucleus, as a bright star
Spiral Galaxy M51 in Hunting Dogs and Supernova - The Whirlpool Galaxy (M51) in Canes Venatici with SN 2005cs - The spiral galaxy M51 (NGC 5194) is located about 37 million years ago - light from Earth. This galaxy is double; two galaxies interact: the largest, NGC 5194, the smallest NGC 5195. On June 28, 2005 a supernova of type II appeared in M51; this supernova (SN 2005cs) is visible just under the nucleus, in the first arm. Image obtained with two telescopes of 50 cm and 30 cm, composite of several poses. The Whirlpool Galaxy lies approximately 31 million light years from earth. This spectacular galaxy is paired with a smaller, more distant companion whose matter is being disrupted by the larger spiral in a gravitational tug of war. Eventually, the shape of both will be altered over many more millions of years. On June 28, 2005, a new star was noticed in this galaxy. It was confirmed to be a bright supernova, one of the brightest in recent years and similar to the brightest supernova of modern times: 1987A. This rare event, SN 2005cs, is visible on the first spiral arm, directly below the nucleus, as a bright star

PIX4612380: Spiral Galaxy M51 in Hunting Dogs and Supernova - The Whirlpool Galaxy (M51) in Canes Venatici with SN 2005cs - The spiral galaxy M51 (NGC 5194) is located about 37 million years ago - light from Earth. This galaxy is double; two galaxies interact: the largest, NGC 5194, the smallest NGC 5195. On June 28, 2005 a supernova of type II appeared in M51; this supernova (SN 2005cs) is visible just under the nucleus, in the first arm. Image obtained with two telescopes of 50 cm and 30 cm, composite of several poses. The Whirlpool Galaxy lies approximately 31 million light years from earth. This spectacular galaxy is paired with a smaller, more distant companion whose matter is being disrupted by the larger spiral in a gravitational tug of war. Eventually, the shape of both will be altered over many more millions of years. On June 28, 2005, a new star was noticed in this galaxy. It was confirmed to be a bright supernova, one of the brightest in recent years and similar to the brightest supernova of modern times: 1987A. This rare event, SN 2005cs, is visible on the first spiral arm, directly below the nucleus, as a bright star / Bridgeman Images

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. M83 (NGC 5236) is an intermediate spiral galaxy at approximately 15 million light - years away in the constellation Hydra
Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. M83 (NGC 5236) is an intermediate spiral galaxy at approximately 15 million light - years away in the constellation Hydra

PIX4612435: Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. M83 (NGC 5236) is an intermediate spiral galaxy at approximately 15 million light - years away in the constellation Hydra / Bridgeman Images

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained by the 2.2m ESO/MPG telescope of La Silla in Chile. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. Colour - composite image made using data from the Wide Field Imager on the ESO/MPG 2.2 - m telescope at La Silla. The WFI stared at M83 for four periods of 25 minutes through different filters (B, V, R, Halpha)
Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained by the 2.2m ESO/MPG telescope of La Silla in Chile. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. Colour - composite image made using data from the Wide Field Imager on the ESO/MPG 2.2 - m telescope at La Silla. The WFI stared at M83 for four periods of 25 minutes through different filters (B, V, R, Halpha)

PIX4612524: Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained by the 2.2m ESO/MPG telescope of La Silla in Chile. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. Colour - composite image made using data from the Wide Field Imager on the ESO/MPG 2.2 - m telescope at La Silla. The WFI stared at M83 for four periods of 25 minutes through different filters (B, V, R, Halpha) / Bridgeman Images

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - 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. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies
Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - 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. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies

PIX4612535: Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - 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. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies / Bridgeman Images

Galaxy M83 in Hydra - Galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is about 15 million years away from Earth. This galaxy is a barred spiral. Image obtained by the Hubble Space Telescope (HST). M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. The vibrant magentas and blues reveal the galaxy is ablaze with star formation. This photograph captures thousands of star clusters, hundreds of thousands of individual stars, and “” ghosts”” of dead stars called supernova remnants. The galactic panorama unveils a tapestry of the drama of stellar birth and death spread across 50,000 light - years.Image taken with the Hubble space telescope (HST)
Galaxy M83 in Hydra - Galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is about 15 million years away from Earth. This galaxy is a barred spiral. Image obtained by the Hubble Space Telescope (HST). M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. The vibrant magentas and blues reveal the galaxy is ablaze with star formation. This photograph captures thousands of star clusters, hundreds of thousands of individual stars, and “” ghosts”” of dead stars called supernova remnants. The galactic panorama unveils a tapestry of the drama of stellar birth and death spread across 50,000 light - years.Image taken with the Hubble space telescope (HST)

PIX4612543: Galaxy M83 in Hydra - Galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is about 15 million years away from Earth. This galaxy is a barred spiral. Image obtained by the Hubble Space Telescope (HST). M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. The vibrant magentas and blues reveal the galaxy is ablaze with star formation. This photograph captures thousands of star clusters, hundreds of thousands of individual stars, and “” ghosts”” of dead stars called supernova remnants. The galactic panorama unveils a tapestry of the drama of stellar birth and death spread across 50,000 light - years.Image taken with the Hubble space telescope (HST) / Bridgeman Images

Suprematist element: two squares  (oil on canvas, 20th century)
Suprematist element: two squares  (oil on canvas, 20th century)

LRI4616317: Suprematist element: two squares (oil on canvas, 20th century), Malevich, Kazimir Severinovich (1878-1935) / Bridgeman Images

Blue horse and rainbow (drawing in pencil and watercolor, 1913)
Blue horse and rainbow (drawing in pencil and watercolor, 1913)

LRI4616526: Blue horse and rainbow (drawing in pencil and watercolor, 1913), Marc, Franz (1880-1916) / Bridgeman Images

Renovation of the Gare de l'Est (built in 1852), Paris 10th. Realisation 2007, architect Jean Marie Duthilleul. Photography 06/06/07.
Renovation of the Gare de l'Est (built in 1852), Paris 10th. Realisation 2007, architect Jean Marie Duthilleul. Photography 06/06/07.

RCT4616293: Renovation of the Gare de l'Est (built in 1852), Paris 10th. Realisation 2007, architect Jean Marie Duthilleul. Photography 06/06/07., Duthilleul, Jean Marie (b.1952) / Bridgeman Images

Volcano Arsia Mons - Arsia Mons volcano. - Arsia Mons is one of the largest known volcanoes. It stands more than 9 km above the surrounding plains and its caldera extends for 110 km. Mosaic of infrared images obtained by the Mars Odyssey probe. Arsia Mons is the southernmost of the Tharsis volcanoes. It is 270 miles in diameter, almost 12 miles high, and the summit caldera is 72 miles wide. For comparison, the largest volcano on Earth is Mauna Loa. From its base on the sea floor, Mauna Loa measures only 6.3 miles high and 75 miles in diameter. The image here is a mosaic of several daytime IR images taken by the Mars Odyssey spacecraft
Volcano Arsia Mons - Arsia Mons volcano. - Arsia Mons is one of the largest known volcanoes. It stands more than 9 km above the surrounding plains and its caldera extends for 110 km. Mosaic of infrared images obtained by the Mars Odyssey probe. Arsia Mons is the southernmost of the Tharsis volcanoes. It is 270 miles in diameter, almost 12 miles high, and the summit caldera is 72 miles wide. For comparison, the largest volcano on Earth is Mauna Loa. From its base on the sea floor, Mauna Loa measures only 6.3 miles high and 75 miles in diameter. The image here is a mosaic of several daytime IR images taken by the Mars Odyssey spacecraft

PIX4616305: Volcano Arsia Mons - Arsia Mons volcano. - Arsia Mons is one of the largest known volcanoes. It stands more than 9 km above the surrounding plains and its caldera extends for 110 km. Mosaic of infrared images obtained by the Mars Odyssey probe. Arsia Mons is the southernmost of the Tharsis volcanoes. It is 270 miles in diameter, almost 12 miles high, and the summit caldera is 72 miles wide. For comparison, the largest volcano on Earth is Mauna Loa. From its base on the sea floor, Mauna Loa measures only 6.3 miles high and 75 miles in diameter. The image here is a mosaic of several daytime IR images taken by the Mars Odyssey spacecraft / Bridgeman Images

Mars: Tooting crater - View of the Tooting impact crater obtained by the Mars Odyssey probe. It is a “recent” impact crater (a few hundred thousand years) with a diameter of about 29 km
Mars: Tooting crater - View of the Tooting impact crater obtained by the Mars Odyssey probe. It is a “recent” impact crater (a few hundred thousand years) with a diameter of about 29 km

PIX4616308: Mars: Tooting crater - View of the Tooting impact crater obtained by the Mars Odyssey probe. It is a “recent” impact crater (a few hundred thousand years) with a diameter of about 29 km / Bridgeman Images

Mars - Satellite Phobos - Martian moon Phobos - View of the satellite Phobos obtained by the Mars Express probe on January 9, 2011, at a distance of 100 km from the satellite. The south pole is indicated. Mars Express took this image of the surface of the moon Phobos on January 9, 2011. Mars Express passed Mars' largest moon at a distance of 100 km. South pole is indicated
Mars - Satellite Phobos - Martian moon Phobos - View of the satellite Phobos obtained by the Mars Express probe on January 9, 2011, at a distance of 100 km from the satellite. The south pole is indicated. Mars Express took this image of the surface of the moon Phobos on January 9, 2011. Mars Express passed Mars' largest moon at a distance of 100 km. South pole is indicated

PIX4616339: Mars - Satellite Phobos - Martian moon Phobos - View of the satellite Phobos obtained by the Mars Express probe on January 9, 2011, at a distance of 100 km from the satellite. The south pole is indicated. Mars Express took this image of the surface of the moon Phobos on January 9, 2011. Mars Express passed Mars' largest moon at a distance of 100 km. South pole is indicated / Bridgeman Images

Crater Bacolor on Mars - Bacolor Crater on planet Mars - View of the impact crater Bacolor obtained by the Mars Odyssey probe. It's an impact crater about 20 km in diameter. Bacolor Crater is a magnificent impact feature about 20 kilometers (12 miles) wide. The lines on the ejecta blanket surrounding the crater rim come from a surge of superheated gas and debris flying outward in the wake of the meteorite impact that made the crater. This view combines images taken during the period from September 2002 to October 2005 by the Thermal Emission Imaging System instrument on Nasa's Mars Odyssey orbiter. The pictured location on Mars is 33 degrees north latitude, 118.6 degrees east longitude
Crater Bacolor on Mars - Bacolor Crater on planet Mars - View of the impact crater Bacolor obtained by the Mars Odyssey probe. It's an impact crater about 20 km in diameter. Bacolor Crater is a magnificent impact feature about 20 kilometers (12 miles) wide. The lines on the ejecta blanket surrounding the crater rim come from a surge of superheated gas and debris flying outward in the wake of the meteorite impact that made the crater. This view combines images taken during the period from September 2002 to October 2005 by the Thermal Emission Imaging System instrument on Nasa's Mars Odyssey orbiter. The pictured location on Mars is 33 degrees north latitude, 118.6 degrees east longitude

PIX4616373: Crater Bacolor on Mars - Bacolor Crater on planet Mars - View of the impact crater Bacolor obtained by the Mars Odyssey probe. It's an impact crater about 20 km in diameter. Bacolor Crater is a magnificent impact feature about 20 kilometers (12 miles) wide. The lines on the ejecta blanket surrounding the crater rim come from a surge of superheated gas and debris flying outward in the wake of the meteorite impact that made the crater. This view combines images taken during the period from September 2002 to October 2005 by the Thermal Emission Imaging System instrument on Nasa's Mars Odyssey orbiter. The pictured location on Mars is 33 degrees north latitude, 118.6 degrees east longitude / Bridgeman Images

Ellipse within a rectangle (Acrylic on Canvas, 20th century)
Ellipse within a rectangle (Acrylic on Canvas, 20th century)

LRI4616463: Ellipse within a rectangle (Acrylic on Canvas, 20th century), Mangold, Robert (b.1937) / Bridgeman Images

The cemetery of the Pere Lachaise in Paris 20th. Opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it has nearly 70,000 monuments. Photography 06/06/05.
The cemetery of the Pere Lachaise in Paris 20th. Opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it has nearly 70,000 monuments. Photography 06/06/05.

TEC4616465: The cemetery of the Pere Lachaise in Paris 20th. Opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it has nearly 70,000 monuments. Photography 06/06/05. / Bridgeman Images

The cemetery of Pere Lachaise in Paris. The cemetery opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere-Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it counts about 70 000 monuments.ÆPhotograph 06/06/05.
The cemetery of Pere Lachaise in Paris. The cemetery opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere-Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it counts about 70 000 monuments.ÆPhotograph 06/06/05.

TEC4616513: The cemetery of Pere Lachaise in Paris. The cemetery opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere-Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it counts about 70 000 monuments.ÆPhotograph 06/06/05. / Bridgeman Images

The cemetery of Pere Lachaise in Paris. The cemetery opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere-Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it counts about 70 000 monuments.ÆPhotograph 06/06/05.
The cemetery of Pere Lachaise in Paris. The cemetery opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere-Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it counts about 70 000 monuments.ÆPhotograph 06/06/05.

TEC4616527: The cemetery of Pere Lachaise in Paris. The cemetery opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere-Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it counts about 70 000 monuments.ÆPhotograph 06/06/05. / Bridgeman Images

March: Caldera of the volcano Apollinaris Patera - This Martian volcano is 180 to 280 km from its base and rises at about 5000 m altitude. Its caldera seen here by the Mars Express probe on October 26, 2004 measures 80 km in diameter and a depth of 1 km. Faux Color Image
March: Caldera of the volcano Apollinaris Patera - This Martian volcano is 180 to 280 km from its base and rises at about 5000 m altitude. Its caldera seen here by the Mars Express probe on October 26, 2004 measures 80 km in diameter and a depth of 1 km. Faux Color Image

PIX4615989: March: Caldera of the volcano Apollinaris Patera - This Martian volcano is 180 to 280 km from its base and rises at about 5000 m altitude. Its caldera seen here by the Mars Express probe on October 26, 2004 measures 80 km in diameter and a depth of 1 km. Faux Color Image / Bridgeman Images

Composition in blue (Pen drawing and watercolour, 1915)
Composition in blue (Pen drawing and watercolour, 1915)

LRI4616104: Composition in blue (Pen drawing and watercolour, 1915), Lewis, Wyndham (1882-1957) / Bridgeman Images

March: Hebes Chasma - Mars: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Image obtained by the Mars Express probe in 2005. View of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars. A mesa - like mountain is located in the center of Hebes Chasma. It reaches 8000 meters above the graben floor and extends almost to the top of the surrounding plain. The mountain is made up by numerous stacked rock layers. The layering may consists of remnants of the older plateau, lake sediments, wind blown sediments or volcanic rock. The rock layers were exposed by erosional processes. Newest data acquired by the OMEGA spectrometer on - board Mars Express revealed hydratized (water - bearing) minerals like gypsum in some areas of Hebes Chasma. What ever kind of processes led to the formation of the Interior Layered Deposits: at least some water once existed in Hebes Chasma. Hebes Chasma is located at approximately 1* south and 282* east. The HRSC obtained image data on 16 September 2005 with a ground resolution of approximately 15 m/pixel
March: Hebes Chasma - Mars: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Image obtained by the Mars Express probe in 2005. View of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars. A mesa - like mountain is located in the center of Hebes Chasma. It reaches 8000 meters above the graben floor and extends almost to the top of the surrounding plain. The mountain is made up by numerous stacked rock layers. The layering may consists of remnants of the older plateau, lake sediments, wind blown sediments or volcanic rock. The rock layers were exposed by erosional processes. Newest data acquired by the OMEGA spectrometer on - board Mars Express revealed hydratized (water - bearing) minerals like gypsum in some areas of Hebes Chasma. What ever kind of processes led to the formation of the Interior Layered Deposits: at least some water once existed in Hebes Chasma. Hebes Chasma is located at approximately 1* south and 282* east. The HRSC obtained image data on 16 September 2005 with a ground resolution of approximately 15 m/pixel

PIX4616152: March: Hebes Chasma - Mars: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Image obtained by the Mars Express probe in 2005. View of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars. A mesa - like mountain is located in the center of Hebes Chasma. It reaches 8000 meters above the graben floor and extends almost to the top of the surrounding plain. The mountain is made up by numerous stacked rock layers. The layering may consists of remnants of the older plateau, lake sediments, wind blown sediments or volcanic rock. The rock layers were exposed by erosional processes. Newest data acquired by the OMEGA spectrometer on - board Mars Express revealed hydratized (water - bearing) minerals like gypsum in some areas of Hebes Chasma. What ever kind of processes led to the formation of the Interior Layered Deposits: at least some water once existed in Hebes Chasma. Hebes Chasma is located at approximately 1* south and 282* east. The HRSC obtained image data on 16 September 2005 with a ground resolution of approximately 15 m/pixel / Bridgeman Images

Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater on the left of the image measures 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The surface is mostly smooth, and is covered by several small impact craters measuring 800 to 2800 m in diameter. Smaller craters are scattered across the entire region. The left side of the image shows a large impact crater measuring 20 km in diameter. Covering an area of approximately 150 sq km, a crater of this size on Earth could harbour cities such as Bonn or Kiel. In contrast to the smaller craters, it shows a blanket of ejecta with flow forms surrounding the rim
Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater on the left of the image measures 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The surface is mostly smooth, and is covered by several small impact craters measuring 800 to 2800 m in diameter. Smaller craters are scattered across the entire region. The left side of the image shows a large impact crater measuring 20 km in diameter. Covering an area of approximately 150 sq km, a crater of this size on Earth could harbour cities such as Bonn or Kiel. In contrast to the smaller craters, it shows a blanket of ejecta with flow forms surrounding the rim

PIX4616156: Mars: craters and channels in Hephaestus Fossae - Mars: craters and channels in Hephaestus Fossae - Impact crateres and channel system in Hephaestus Fossae, a region on Mars located on the western flank of Elysium Mons. The large impact crater on the left of the image measures 20 km in diameter. The image covering an area of about 150 square km was obtained by the Mars Express probe on 28 December 2007. This image of Hephaestus Fossae was obtained by Esa's Mars Express orbiter on 28 December 2007. The region is dotted with craters and channel systems and lies at about 21* North and 126* East on the Red Planet. Named after the Greek god of fire, Hephaestus Fossae extends for more than 600 km on the western flank of Elysium Mons in the Utopia Planitia region. The surface is mostly smooth, and is covered by several small impact craters measuring 800 to 2800 m in diameter. Smaller craters are scattered across the entire region. The left side of the image shows a large impact crater measuring 20 km in diameter. Covering an area of approximately 150 sq km, a crater of this size on Earth could harbour cities such as Bonn or Kiel. In contrast to the smaller craters, it shows a blanket of ejecta with flow forms surrounding the rim / Bridgeman Images

The music lesson (Painting, 18th century)
The music lesson (Painting, 18th century)

LRI4616165: The music lesson (Painting, 18th century), Longhi, Pietro (c.1701-85) (after) / Bridgeman Images

Blanter on the Blue Rider (Watercolour, 1913)
Blanter on the Blue Rider (Watercolour, 1913)

LRI4616172: Blanter on the Blue Rider (Watercolour, 1913), Macke, August (1887-1914) / Bridgeman Images

Painting 526  (oil on canvas, 1915)
Painting 526  (oil on canvas, 1915)

LRI4616214: Painting 526 (oil on canvas, 1915), Magnelli, Alberto (1888-1971) / Bridgeman Images


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