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Bilder zu 'Atlante' gefunden, 9,227

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Maori artefacts, New Zealand, 1826-1829

Maori artefacts, New Zealand, 1826-1829

UIS5077717

Men from New Ireland and Fiji, 1826-1829

Men from New Ireland and Fiji, 1826-1829

UIS5077739

Three types of volutes or sea molluscs, 1837-1840

Three types of volutes or sea molluscs, 1837-1840

UIS5098172

Proboscis monkey, Borneo, 1837-1840

Proboscis monkey, Borneo, 1837-1840

UIS5098120

Dolphin foetus and gnarled whale, 1837-1840

Dolphin foetus and gnarled whale, 1837-1840

UIS5098163

Two types of owl, 1837-1840

Two types of owl, 1837-1840

UIS5098068

Five types of frog and toad, 1837-1840

Five types of frog and toad, 1837-1840

UIS5098117

Seal with small claws, 1837-1840

Seal with small claws, 1837-1840

UIS5098136

Taurus, c.1825 (card, paper, tissue )

Taurus, c.1825 (card, paper, tissue )

Hall, Sydney (fl.1826)

MMM7340884

Interacting galaxies Arp 81

Interacting galaxies Arp 81

Adam Block

PIX5620161

New York harbour, 1779 (coloured engraving)

New York harbour, 1779 (coloured engraving)

DesBarres, Joseph Frederick Wallet (1721-1824)

MMM7337582

Galaxies NGC 4631 and NGC 4656 - 57 in Hunting Dogs - Galaxies NGC 4631 and NGC 4656 - 57 - The spiral galaxy NGC 4631 (upper right) is a galaxy seen by the slice that is located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. Below the irregular galaxies NGC 4656 and NGC 4657. Galaxies NGC 4631 (top right) and NGC 4656 (bottom left) are two unusual galaxies in Canes Venatici. A small companion galaxy, NGC 4627, can be seen next to NGC 4631. The galaxies, which are located about 30 million lights years away, get their unusual shapes from gravitational interactions with each other. NGC 6431 and NGC 4627 are also listed in ARP's Atlas of Peculiar Galaxies as Arp 281

Galaxies NGC 4631 and NGC 4656 - 57 in Hunting Dogs - Galaxies NGC 4631 and NGC 4656 - 57 - The spiral galaxy NGC 4631 (upper right) is a galaxy seen by the slice that is located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. Below the irregular galaxies NGC 4656 and NGC 4657. Galaxies NGC 4631 (top right) and NGC 4656 (bottom left) are two unusual galaxies in Canes Venatici. A small companion galaxy, NGC 4627, can be seen next to NGC 4631. The galaxies, which are located about 30 million lights years away, get their unusual shapes from gravitational interactions with each other. NGC 6431 and NGC 4627 are also listed in ARP's Atlas of Peculiar Galaxies as Arp 281

Jerry Lodriguss

PIX4611740

Cormorants, 1837-1840

Cormorants, 1837-1840

UIS5098100

North celestial pole and circumpolar constellations - North celestial pole and circumpolar constellations - The northern celestial pole is marked by the polar star of the Little Bear. Around, the so-called circumpolar constellations with from top to bottom: The Great Bear on the left, the Dragon that encircles the Little Bear, Cephee below and the Swan on its right, then Cassiopee snaps everything against a big rock. In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. May 20, 2007, Ploumanach (Cotes d'Armor - France). Pole star Polaris (near the center of the image) and circumpolar constellations; from left to right and top to bottom: Big Dipper, Draco with Little Dipper, Cygnus, Cepheus and Cassiopeia. Constellation mythological forms from “” Uranographia”” star atlas by Hevelius (1690) have been added. May 20, 2007, Ploumanach (Cotes d'Armor - France)

North celestial pole and circumpolar constellations - North celestial pole and circumpolar constellations - The northern celestial pole is marked by the polar star of the Little Bear. Around, the so-called circumpolar constellations with from top to bottom: The Great Bear on the left, the Dragon that encircles the Little Bear, Cephee below and the Swan on its right, then Cassiopee snaps everything against a big rock. In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. May 20, 2007, Ploumanach (Cotes d'Armor - France). Pole star Polaris (near the center of the image) and circumpolar constellations; from left to right and top to bottom: Big Dipper, Draco with Little Dipper, Cygnus, Cepheus and Cassiopeia. Constellation mythological forms from “” Uranographia”” star atlas by Hevelius (1690) have been added. May 20, 2007, Ploumanach (Cotes d'Armor - France)

Laurent Laveder

PIX4593365

Constellations of the Little Horse, Dauphin, Fleche and Petite Fox - Constellation of Equuleus and Vulpecula - At the top right, the constellation of the Little Fox, below, the Fleche, on the left, the Dolphin; at the bottom left, the Little Horse. Equuleus (the Little Horse or colt) is a small and undistinguished constellation located about 10 degrees north of the celestial equator. It is the second smallest constellation in the sky: only Crux is smaller. It contains no bright stars, so, unlike Crux, it is difficult to find, though Delphinus is a useful guide. There is little of astronomical interest here that is accessible to small telescopes. Vulpecula, the Fox, first appears in Johannes Hevelius' atlas of 1690 and was originally called Vulpecula Cum Anser, the fox with goose, but the bird has flown and the fox is hardly obvious. The constellation crosses part of the northern Milky Way and lies just south of Cygnus. The main stars of Sagitta are also well seen here

Constellations of the Little Horse, Dauphin, Fleche and Petite Fox - Constellation of Equuleus and Vulpecula - At the top right, the constellation of the Little Fox, below, the Fleche, on the left, the Dolphin; at the bottom left, the Little Horse. Equuleus (the Little Horse or colt) is a small and undistinguished constellation located about 10 degrees north of the celestial equator. It is the second smallest constellation in the sky: only Crux is smaller. It contains no bright stars, so, unlike Crux, it is difficult to find, though Delphinus is a useful guide. There is little of astronomical interest here that is accessible to small telescopes. Vulpecula, the Fox, first appears in Johannes Hevelius' atlas of 1690 and was originally called Vulpecula Cum Anser, the fox with goose, but the bird has flown and the fox is hardly obvious. The constellation crosses part of the northern Milky Way and lies just south of Cygnus. The main stars of Sagitta are also well seen here

PIX4593306

Two types of dolphin, 1837-1840

Two types of dolphin, 1837-1840

UIS5098162

Couple d'Aborigenes de Tasmanie (Australie), 1826-1829

Couple d'Aborigenes de Tasmanie (Australie), 1826-1829

UIS5077756

Two types of dolphin, 1837-1840

Two types of dolphin, 1837-1840

UIS5098159

Constellations of the Little Horse, Dauphin, Fleche and Petite Fox - Constellation of Equuleus and Vulpecula - At the top right, the constellation of the Little Fox, below, the Fleche, on the left, the Dolphin; at the bottom left, the Little Horse. Equuleus (the Little Horse or colt) is a small and undistinguished constellation located about 10 degrees north of the celestial equator. It is the second smallest constellation in the sky: only Crux is smaller. It contains no bright stars, so, unlike Crux, it is difficult to find, though Delphinus is a useful guide. There is little of astronomical interest here that is accessible to small telescopes. Vulpecula, the Fox, first appears in Johannes Hevelius' atlas of 1690 and was originally called Vulpecula Cum Anser, the fox with goose, but the bird has flown and the fox is hardly obvious. The constellation crosses part of the northern Milky Way and lies just south of Cygnus. The main stars of Sagitta are also well seen here

Constellations of the Little Horse, Dauphin, Fleche and Petite Fox - Constellation of Equuleus and Vulpecula - At the top right, the constellation of the Little Fox, below, the Fleche, on the left, the Dolphin; at the bottom left, the Little Horse. Equuleus (the Little Horse or colt) is a small and undistinguished constellation located about 10 degrees north of the celestial equator. It is the second smallest constellation in the sky: only Crux is smaller. It contains no bright stars, so, unlike Crux, it is difficult to find, though Delphinus is a useful guide. There is little of astronomical interest here that is accessible to small telescopes. Vulpecula, the Fox, first appears in Johannes Hevelius' atlas of 1690 and was originally called Vulpecula Cum Anser, the fox with goose, but the bird has flown and the fox is hardly obvious. The constellation crosses part of the northern Milky Way and lies just south of Cygnus. The main stars of Sagitta are also well seen here

PIX4593321

Isolario, in verse, with coloured drawings and a chart of the eastern Mediterranean on vellum., c.1480 (drawing on vellum)

Isolario, in verse, with coloured drawings and a chart of the eastern Mediterranean on vellum., c.1480 (drawing on vellum)

Sonetti, Bartolomeo da li (fl.1485)

MMM7339139

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

PIX4568732

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

PIX4568741

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

PIX4568852

Galaxy UGC 9618 in Bovier - Galaxy UGC 9618 in Botes - The galaxy UGC 9618, also called VV 340 or Arp 302, is about 450 million years away from Earth. It is a pair of interacting spiral galaxies, VV 340A (view from the edge, bottom) and VV 340B (view from the front, top). Massive stars are formed in abundance. Image obtained by the Hubble Space Telescope in January 2002. UGC 9618, also known as VV 340 or Arp 302 consists of a pair of very gas - rich spiral galaxies in their early stages of interaction: VV 340A is seen edge - on to the left, and VV 340B face - on to the right. An enormous amount of infrared light is radiated by the gas from massive stars that are forming at a rate similar to the most vigorous giant star - forming regions in our own Milky Way. UGC 9618 is 450 million light - years away from Earth, and is the 302nd galaxy in ARP's Atlas of Peculiar Galaxies

Galaxy UGC 9618 in Bovier - Galaxy UGC 9618 in Botes - The galaxy UGC 9618, also called VV 340 or Arp 302, is about 450 million years away from Earth. It is a pair of interacting spiral galaxies, VV 340A (view from the edge, bottom) and VV 340B (view from the front, top). Massive stars are formed in abundance. Image obtained by the Hubble Space Telescope in January 2002. UGC 9618, also known as VV 340 or Arp 302 consists of a pair of very gas - rich spiral galaxies in their early stages of interaction: VV 340A is seen edge - on to the left, and VV 340B face - on to the right. An enormous amount of infrared light is radiated by the gas from massive stars that are forming at a rate similar to the most vigorous giant star - forming regions in our own Milky Way. UGC 9618 is 450 million light - years away from Earth, and is the 302nd galaxy in ARP's Atlas of Peculiar Galaxies

PIX4613610

Image of the globe of the world, 1573 (copperplate engraving on paper)

Image of the globe of the world, 1573 (copperplate engraving on paper)

Ortelius, Abraham (1527-98)

MMM7340119

Interacting Galaxies Arp 256 in the Whale - Interacting galaxies Arp 256 in Cetus - The galaxy Arp 256, also called VV 352, is about 350 million years away from Earth. It's a pair of spiral galaxies interacting. Regions of intense star formations appear in blue. Image obtained by the Hubble Space Telescope on 22 May 2002. Arp 256 is a stunning system of two spiral galaxies in an early stage of merging. The Hubble image displays two galaxies with strongly disrupted shapes and an astonishing number of blue knots of star formation that look like exploding fireworks. The galaxy to the left has two extended ribbon - like tails of gas, dust and stars. The system is a luminous infrared system radiating more than a hundred billion times the luminosity of our Sun. Arp 256 is located in the constellation of Cetus, the Whale, about 350 million light - years away. It is the 256th galaxy in ARP's Atlas of Peculiar Galaxies

Interacting Galaxies Arp 256 in the Whale - Interacting galaxies Arp 256 in Cetus - The galaxy Arp 256, also called VV 352, is about 350 million years away from Earth. It's a pair of spiral galaxies interacting. Regions of intense star formations appear in blue. Image obtained by the Hubble Space Telescope on 22 May 2002. Arp 256 is a stunning system of two spiral galaxies in an early stage of merging. The Hubble image displays two galaxies with strongly disrupted shapes and an astonishing number of blue knots of star formation that look like exploding fireworks. The galaxy to the left has two extended ribbon - like tails of gas, dust and stars. The system is a luminous infrared system radiating more than a hundred billion times the luminosity of our Sun. Arp 256 is located in the constellation of Cetus, the Whale, about 350 million light - years away. It is the 256th galaxy in ARP's Atlas of Peculiar Galaxies

PIX4613619

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are one of the finest and nearest examples of a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus and has been recognised since ancient times. Seven of the brightest stars are quite easy to see with the unaided eye and bear the names of the Seven Sisters, the daughters of Atlas. The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

PIX4568850

Totius Orbis Cogniti Universalis Descriptio, Antwerp, 1593 (engraving)

Totius Orbis Cogniti Universalis Descriptio, Antwerp, 1593 (engraving)

Jode, Cornelis de (1568-1600)

CH3554905

Portrait of Winefred Redmond, 1841 (oil on canvas)

Portrait of Winefred Redmond, 1841 (oil on canvas)

Felton, Maurice (1803-42)

NSW5914763

Galaxies NGC 3718 in the Great Bear - Galaxy NGC 3718 in Ursa Major - NGC 3718 (Arp 214) is a special galaxy located about 42 million years ago - light from the Earth in the constellation Big Bear. It's an active nucleus galaxy. Its tormented form is probably due to the attraction exerted by another galaxy, NGC 3729 (off-field). On the right, Arp 322 (or Hickson 56), is a group of 5 galaxies far farther away, located about 300 million years from Earth. NGC 3718 (Arp 214) seems to have a rudimentary bar and spiral structure although it is recognized as a peculiar galaxy and as such is listed within ARP's Atlas of Peculiar Galaxies. NGC 3718 contains an active galactic nucleus (AGN) and is known as a Seyfert type 1.9 galaxy. Its strange shape is probably due to a gravitational interaction with its companion NGC 3729 (out of field). A grouping of 5 background galaxies 300 million light years distant are projected at right of NGC 3718 and are designated Arp 322 (also Hickson 56). Several m

Galaxies NGC 3718 in the Great Bear - Galaxy NGC 3718 in Ursa Major - NGC 3718 (Arp 214) is a special galaxy located about 42 million years ago - light from the Earth in the constellation Big Bear. It's an active nucleus galaxy. Its tormented form is probably due to the attraction exerted by another galaxy, NGC 3729 (off-field). On the right, Arp 322 (or Hickson 56), is a group of 5 galaxies far farther away, located about 300 million years from Earth. NGC 3718 (Arp 214) seems to have a rudimentary bar and spiral structure although it is recognized as a peculiar galaxy and as such is listed within ARP's Atlas of Peculiar Galaxies. NGC 3718 contains an active galactic nucleus (AGN) and is known as a Seyfert type 1.9 galaxy. Its strange shape is probably due to a gravitational interaction with its companion NGC 3729 (out of field). A grouping of 5 background galaxies 300 million light years distant are projected at right of NGC 3718 and are designated Arp 322 (also Hickson 56). Several m

Jim Misti

PIX4610955

La Voie lactee from one horizon to the other- Pointe du Raz - Milky way - 180* panorama - Pointe du Raz - At the end of September, at the end of the night, the horizon East presents a scattered and inclined light band: it is the zodiacal light generated by dust near the Sun located in the plane of the solar system. This glow is visible at the top of the photo. It extends to the lactee road over forty degrees high. Here, on this view of more than 180*, it is easily visible despite the glows of the city of Audierne. In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. Brittany, 27 September 2008. At the end of September, at the end of the night, the East horizon is displaying a faint, fuzzy and tilted glow: it's the zodiacal light formed by the dust near the Sun along the plan of the Solar System. It extends to about 40* of elevation. In this 180* panorama, the zodiacal light is easily visible despite the glow of the city of Audierne,

La Voie lactee from one horizon to the other- Pointe du Raz - Milky way - 180* panorama - Pointe du Raz - At the end of September, at the end of the night, the horizon East presents a scattered and inclined light band: it is the zodiacal light generated by dust near the Sun located in the plane of the solar system. This glow is visible at the top of the photo. It extends to the lactee road over forty degrees high. Here, on this view of more than 180*, it is easily visible despite the glows of the city of Audierne. In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. Brittany, 27 September 2008. At the end of September, at the end of the night, the East horizon is displaying a faint, fuzzy and tilted glow: it's the zodiacal light formed by the dust near the Sun along the plan of the Solar System. It extends to about 40* of elevation. In this 180* panorama, the zodiacal light is easily visible despite the glow of the city of Audierne,

Laurent Laveder

PIX4637858

Galaxy IC 883 - Galaxy IC 883 - The particular galaxy IC 883 (Arp 193) is located about 300 million light years away from Earth in the constellation Hunting Dogs. Its shape presents two antennas, maree tails, suggesting that IC 883 is the fusion of two galaxies. The collision caused a burst of star formations as evidenced by the presence of star clusters in the central region. Image obtained by the Hubble Space Telescope on January 10, 2002. IC 883 displays a very disturbed, complex central region with two tidal tails of approximately the same length emerging at nearly right angles: one diagonally to the top right of the frame and the other to the bottom right. The twin tidal tails suggest that IC 883 is the remnant of the merger of two gas - rich disk galaxies. The collision appears to have triggered a burst of star formation, indicated by a number of bright star clusters in the central region. IC 883 is 300 million light - years away towards the constellation of Canes Venatici, the H

Galaxy IC 883 - Galaxy IC 883 - The particular galaxy IC 883 (Arp 193) is located about 300 million light years away from Earth in the constellation Hunting Dogs. Its shape presents two antennas, maree tails, suggesting that IC 883 is the fusion of two galaxies. The collision caused a burst of star formations as evidenced by the presence of star clusters in the central region. Image obtained by the Hubble Space Telescope on January 10, 2002. IC 883 displays a very disturbed, complex central region with two tidal tails of approximately the same length emerging at nearly right angles: one diagonally to the top right of the frame and the other to the bottom right. The twin tidal tails suggest that IC 883 is the remnant of the merger of two gas - rich disk galaxies. The collision appears to have triggered a burst of star formation, indicated by a number of bright star clusters in the central region. IC 883 is 300 million light - years away towards the constellation of Canes Venatici, the H

PIX4613666

Interacting Galaxies Arp 240 - Interacting galaxies Arp 240 - The galaxy Arp 240 is located about 300 million light years away from Earth in the constellation of the Virgin. Composed of spiral galaxies NGC 5257 and NGC 5258, this interacting system presents important star formations. The two galaxies contain a supermassive black hole in the centre. Image obtained by the Hubble Space Telescope on 20 December 2001. NGC 5257/8 (Arp 240) is an astonishing galaxy pair, composed of spiral galaxies of similar mass and size, NGC 5257 and NGC 5258. The galaxies are visibly interacting with each other via a bridge of dim stars connecting the two galaxies, almost like two dancers holding hands while performing a pirouette. Both galaxies harbor supermassive black holes in their centers and are actively forming new stars in their disks. Arp 240 is located in the constellation Virgo, approximately 300 million light - years away, and is the 240th galaxy in ARP's Atlas of Peculiar Galaxies. With the e

Interacting Galaxies Arp 240 - Interacting galaxies Arp 240 - The galaxy Arp 240 is located about 300 million light years away from Earth in the constellation of the Virgin. Composed of spiral galaxies NGC 5257 and NGC 5258, this interacting system presents important star formations. The two galaxies contain a supermassive black hole in the centre. Image obtained by the Hubble Space Telescope on 20 December 2001. NGC 5257/8 (Arp 240) is an astonishing galaxy pair, composed of spiral galaxies of similar mass and size, NGC 5257 and NGC 5258. The galaxies are visibly interacting with each other via a bridge of dim stars connecting the two galaxies, almost like two dancers holding hands while performing a pirouette. Both galaxies harbor supermassive black holes in their centers and are actively forming new stars in their disks. Arp 240 is located in the constellation Virgo, approximately 300 million light - years away, and is the 240th galaxy in ARP's Atlas of Peculiar Galaxies. With the e

PIX4612595

Insurance Plan of London Vol. XII: sheet 364-2, 1891 (coloured engraving)

Insurance Plan of London Vol. XII: sheet 364-2, 1891 (coloured engraving)

English School, (19th century)

BL5899962

Constellation of Taurus - Constellation of Taurus - Taurus, (the Bull) is one of the most ancient constellations, and appears in artefacts as old as western civilisation itself. The bull is still a figure of strength and fertility in cultures around the world. In the sky the distinctive 'V' shape of his head and long horns tipped by beta (ss) and zeta Tau is easily recognised. If the purpose of the horns was in doubt, the English name for ss Tau is Alnath, meaning 'the butting one'. The bull's glowing red eye of Aldebaran completes the picture, and its location between the delicate Pleiades and the aggressive stance of Orion makes Taurus hard to overlook. Despite its masculine connotations, the constellation is rich in female icons; both the Hyades and Pleiades star clusters are daughters of Atlas and both are important astronomically. The Pleiades (or the Seven Sisters) are a group of young stars at a distance of about 440 light years and on long exposure photographs are seen to be em

Constellation of Taurus - Constellation of Taurus - Taurus, (the Bull) is one of the most ancient constellations, and appears in artefacts as old as western civilisation itself. The bull is still a figure of strength and fertility in cultures around the world. In the sky the distinctive 'V' shape of his head and long horns tipped by beta (ss) and zeta Tau is easily recognised. If the purpose of the horns was in doubt, the English name for ss Tau is Alnath, meaning 'the butting one'. The bull's glowing red eye of Aldebaran completes the picture, and its location between the delicate Pleiades and the aggressive stance of Orion makes Taurus hard to overlook. Despite its masculine connotations, the constellation is rich in female icons; both the Hyades and Pleiades star clusters are daughters of Atlas and both are important astronomically. The Pleiades (or the Seven Sisters) are a group of young stars at a distance of about 440 light years and on long exposure photographs are seen to be em

PIX4594061

Constellation of Taurus - Constellation of Taurus - Taurus, (the Bull) is one of the most ancient constellations, and appears in artefacts as old as western civilisation itself. The bull is still a figure of strength and fertility in cultures around the world. In the sky the distinctive 'V' shape of his head and long horns tipped by beta (ss) and zeta Tau is easily recognised. If the purpose of the horns was in doubt, the English name for ss Tau is Alnath, meaning 'the butting one'. The bull's glowing red eye of Aldebaran completes the picture, and its location between the delicate Pleiades and the aggressive stance of Orion makes Taurus hard to overlook. Despite its masculine connotations, the constellation is rich in female icons; both the Hyades and Pleiades star clusters are daughters of Atlas and both are important astronomically. The Pleiades (or the Seven Sisters) are a group of young stars at a distance of about 440 light years and on long exposure photographs are seen to be em

Constellation of Taurus - Constellation of Taurus - Taurus, (the Bull) is one of the most ancient constellations, and appears in artefacts as old as western civilisation itself. The bull is still a figure of strength and fertility in cultures around the world. In the sky the distinctive 'V' shape of his head and long horns tipped by beta (ss) and zeta Tau is easily recognised. If the purpose of the horns was in doubt, the English name for ss Tau is Alnath, meaning 'the butting one'. The bull's glowing red eye of Aldebaran completes the picture, and its location between the delicate Pleiades and the aggressive stance of Orion makes Taurus hard to overlook. Despite its masculine connotations, the constellation is rich in female icons; both the Hyades and Pleiades star clusters are daughters of Atlas and both are important astronomically. The Pleiades (or the Seven Sisters) are a group of young stars at a distance of about 440 light years and on long exposure photographs are seen to be em

PIX4594065

Interacting spiral galaxies Arp 87 - Interacting galaxies Arp 87 - This pair of interaction galaxies called Arp 87 is composed of the galaxy NGC 3808, on the right, and its companion NGC 3808A. Both are spiral galaxies. An arm of NGC 3808, consisting of dust, gas and stars, envelops his companion. The interaction of these galaxies causes intense star formation. Arp 87 is located 300 million light years from Earth in the constellation Lion. This image was taken by the Hubble Space Telescope in February 2007. Arp 87 is a stunning pair of interacting galaxies. Stars, gas, and dust flow from the large spiral galaxy, NGC 3808, forming an enveloping arm around its companion. The shapes of both galaxies have been distorted by their gravitational interaction. Arp 87 is located in the constellation of Leo, the Lion, approximately 300 million light - years away from Earth. Arp 87 appears in ARP's Atlas of Peculiar Galaxies. As also seen in similar interacting galaxies, the corkscrew shape of the

Interacting spiral galaxies Arp 87 - Interacting galaxies Arp 87 - This pair of interaction galaxies called Arp 87 is composed of the galaxy NGC 3808, on the right, and its companion NGC 3808A. Both are spiral galaxies. An arm of NGC 3808, consisting of dust, gas and stars, envelops his companion. The interaction of these galaxies causes intense star formation. Arp 87 is located 300 million light years from Earth in the constellation Lion. This image was taken by the Hubble Space Telescope in February 2007. Arp 87 is a stunning pair of interacting galaxies. Stars, gas, and dust flow from the large spiral galaxy, NGC 3808, forming an enveloping arm around its companion. The shapes of both galaxies have been distorted by their gravitational interaction. Arp 87 is located in the constellation of Leo, the Lion, approximately 300 million light - years away from Earth. Arp 87 appears in ARP's Atlas of Peculiar Galaxies. As also seen in similar interacting galaxies, the corkscrew shape of the

PIX4610957

Map of Palestine, 1926 (colour litho)

Map of Palestine, 1926 (colour litho)

Trietsch, Davis (1870-1935)

CH3482908

Galaxies NGC 3718 and NGC 3729 in the Great Bear - Galaxies NGC 3718 and NGC 3729 in Ursa Major - NGC 3718 is a special galaxy located about 42 million years ago - light from Earth in the constellation of the Great Bear. It's an active nucleus galaxy. Its tormented shape is probably due to the attraction exerted by another galaxy, NGC 3729, visible to its left. To the south, Arp 322 (or Hickson 56), is a group of 5 galaxies far farther away, located about 300 million light years away from Earth. NGC 3718 and its companion NGC 3729 (left) are physically related members of the Ursa Major galaxy cluster. The two galaxies appear to orbit each other at a projected separation of 147,000 light years. NGC 3718 (Arp 214) seems to have a rudimentary bar and spiral structure although it is recognized as a peculiar galaxy and as such is listed within ARP's Atlas of Peculiar Galaxies. NGC 3718 contains an active galactic nucleus (AGN) and is known as a Seyfert type 1.9 galaxy. Its strange shape is

Galaxies NGC 3718 and NGC 3729 in the Great Bear - Galaxies NGC 3718 and NGC 3729 in Ursa Major - NGC 3718 is a special galaxy located about 42 million years ago - light from Earth in the constellation of the Great Bear. It's an active nucleus galaxy. Its tormented shape is probably due to the attraction exerted by another galaxy, NGC 3729, visible to its left. To the south, Arp 322 (or Hickson 56), is a group of 5 galaxies far farther away, located about 300 million light years away from Earth. NGC 3718 and its companion NGC 3729 (left) are physically related members of the Ursa Major galaxy cluster. The two galaxies appear to orbit each other at a projected separation of 147,000 light years. NGC 3718 (Arp 214) seems to have a rudimentary bar and spiral structure although it is recognized as a peculiar galaxy and as such is listed within ARP's Atlas of Peculiar Galaxies. NGC 3718 contains an active galactic nucleus (AGN) and is known as a Seyfert type 1.9 galaxy. Its strange shape is

R. Gendler

PIX4610948

Interacting Galaxies Arp 299 - Interacting galaxies Arp 299 - The particular galaxy Arp 299 is located about 150 million light years away from Earth in the constellation of the Great Bear. Composed of galaxies IC 694 and NGC 3690, this interacting system presents important star formations. Astronomers also observed the appearance of several supernovae. Arp 299 is an ultra-aluminous infrared galaxy. Image obtained by the Hubble Space Telescope on 18 March 2002. This system consists of a pair of galaxies, dubbed IC 694 and NGC 3690, which made a close pass some 700 million years ago. As a result of this interaction, the system underwent a fierce burst of star formation. In the last fifteen years or so six supernovae have popped off in the outer reaches of the galaxy, making this system a distinguished supernova factory. Arp 299 belongs to the family of ultra - luminous infrared galaxies and is located in the constellation of Ursa Major, the Great Bear, approximately 150 million light - y

Interacting Galaxies Arp 299 - Interacting galaxies Arp 299 - The particular galaxy Arp 299 is located about 150 million light years away from Earth in the constellation of the Great Bear. Composed of galaxies IC 694 and NGC 3690, this interacting system presents important star formations. Astronomers also observed the appearance of several supernovae. Arp 299 is an ultra-aluminous infrared galaxy. Image obtained by the Hubble Space Telescope on 18 March 2002. This system consists of a pair of galaxies, dubbed IC 694 and NGC 3690, which made a close pass some 700 million years ago. As a result of this interaction, the system underwent a fierce burst of star formation. In the last fifteen years or so six supernovae have popped off in the outer reaches of the galaxy, making this system a distinguished supernova factory. Arp 299 belongs to the family of ultra - luminous infrared galaxies and is located in the constellation of Ursa Major, the Great Bear, approximately 150 million light - y

PIX4610926

Galaxies NGC 3718 and NGC 3729 in the Great Bear

Galaxies NGC 3718 and NGC 3729 in the Great Bear

Adam Block

PIX4611005

Interacting galaxies Markarian 533 - Interacting galaxies Markarian 533 - The galaxy NGC 7674 (Markarian 533 or Arp 182) is located about 400 million years ago - light from Earth in the constellation Pegase. It is the most important member of a group of galaxies called Hickson 96 (HCG 96). This spiral galaxy seen from the front is in interaction with other companion galaxies. It has an active core. Image obtained by the Hubble Space Telescope on June 9, 2002. NGC 7674 (seen just above the center), also known as Markarian 533, is the brightest and largest member of the so - called Hickson 96 compact group of galaxies, consisting of four galaxies. This stunning Hubble image shows a spiral galaxy nearly face - on. The central bar - shaped structure is made up of stars. The shape of NGC 7674, including the long narrow streamers seen to the left of and below the galaxy can be accounted for by tidal interactions with its companions. NGC 7674 has a powerful active nucleus of the kind known as

Interacting galaxies Markarian 533 - Interacting galaxies Markarian 533 - The galaxy NGC 7674 (Markarian 533 or Arp 182) is located about 400 million years ago - light from Earth in the constellation Pegase. It is the most important member of a group of galaxies called Hickson 96 (HCG 96). This spiral galaxy seen from the front is in interaction with other companion galaxies. It has an active core. Image obtained by the Hubble Space Telescope on June 9, 2002. NGC 7674 (seen just above the center), also known as Markarian 533, is the brightest and largest member of the so - called Hickson 96 compact group of galaxies, consisting of four galaxies. This stunning Hubble image shows a spiral galaxy nearly face - on. The central bar - shaped structure is made up of stars. The shape of NGC 7674, including the long narrow streamers seen to the left of and below the galaxy can be accounted for by tidal interactions with its companions. NGC 7674 has a powerful active nucleus of the kind known as

PIX4613210

Interacting galaxies Arp 81 - Interacting galaxies Arp 81 - Arp 81 is located about 300 million light years away from Earth in the constellation Dragon. This pair of interacting galaxies is composed of NGC 6621 on the left and NGC 6622 on the right. NGC 6621 is the largest of the two galaxies. The collision, seen here about 100 million years later, caused intense star flames. Image obtained by the Hubble Space Telescope on 15 March 1999. NGC 6621/2 (VV 247, Arp 81) is a strongly interacting pair of galaxies, seen about 100 million years after their closest approach. It consists of NGC 6621 (to the left) and NGC 6622 (to the right). NGC 6621 is the larger of the two, and is a very disturbed spiral galaxy. The encounter has pulled a long tail out of NGC 6621 that has now wrapped behind its body. The collision has also triggered extensive star formation between the two galaxies. Scientists believe that Arp 81 has a richer collection of young massive star clusters than the notable Antennae

Interacting galaxies Arp 81 - Interacting galaxies Arp 81 - Arp 81 is located about 300 million light years away from Earth in the constellation Dragon. This pair of interacting galaxies is composed of NGC 6621 on the left and NGC 6622 on the right. NGC 6621 is the largest of the two galaxies. The collision, seen here about 100 million years later, caused intense star flames. Image obtained by the Hubble Space Telescope on 15 March 1999. NGC 6621/2 (VV 247, Arp 81) is a strongly interacting pair of galaxies, seen about 100 million years after their closest approach. It consists of NGC 6621 (to the left) and NGC 6622 (to the right). NGC 6621 is the larger of the two, and is a very disturbed spiral galaxy. The encounter has pulled a long tail out of NGC 6621 that has now wrapped behind its body. The collision has also triggered extensive star formation between the two galaxies. Scientists believe that Arp 81 has a richer collection of young massive star clusters than the notable Antennae

PIX4612937

Center of the particular galaxy Arp 220 in the Serpent - Heart of the galaxy Arp 220 - The galaxy Arp 220 (IC 4553) is about 250 million years away - light from Earth. Designee in the 1960s as a particular galaxy, today it is defined as an ultra-aluminous infrared galaxy. The Hubble space telescope photographed its heart in April 1997 in infrared light and discovered that its nucleus had two spiral galaxies colliding. The two nuclei (the two light points in the center) are 1200 light years apart and orbit around each other. This collision caused a tremendous flare of new stars. The Hubble Space Telescope's Near Infrared Camera and Multi - Object Spectrometer (NICMOS) has uncovered a collision between two spiral galaxies in the heart of the peculiar galaxy called Arp 220. The collision has provided the spark for a burst of star formation. The bright, crescent moon - shaped object is a remnant core of one of the colliding galaxies. The core is a cluster of 1 billion stars. The core's hal

Center of the particular galaxy Arp 220 in the Serpent - Heart of the galaxy Arp 220 - The galaxy Arp 220 (IC 4553) is about 250 million years away - light from Earth. Designee in the 1960s as a particular galaxy, today it is defined as an ultra-aluminous infrared galaxy. The Hubble space telescope photographed its heart in April 1997 in infrared light and discovered that its nucleus had two spiral galaxies colliding. The two nuclei (the two light points in the center) are 1200 light years apart and orbit around each other. This collision caused a tremendous flare of new stars. The Hubble Space Telescope's Near Infrared Camera and Multi - Object Spectrometer (NICMOS) has uncovered a collision between two spiral galaxies in the heart of the peculiar galaxy called Arp 220. The collision has provided the spark for a burst of star formation. The bright, crescent moon - shaped object is a remnant core of one of the colliding galaxies. The core is a cluster of 1 billion stars. The core's hal

PIX4613739

View of Valletta on the island of Malta, seen from Senglea (black chalk, pen & brown ink, brown and grey wash, on three joined sheets)

View of Valletta on the island of Malta, seen from Senglea (black chalk, pen & brown ink, brown and grey wash, on three joined sheets)

Schellinks, Willem (1627-78)

CH3674461

A View of Seringapatam, 1791 circa (oil on canvas)

A View of Seringapatam, 1791 circa (oil on canvas)

Unknown artist, (18th century)

NAM5925042

Salle de spectacle (fol. 11 detail), from 'Atlas du Comte du Nord', 1784 (w/c & ink on paper)

Salle de spectacle (fol. 11 detail), from 'Atlas du Comte du Nord', 1784 (w/c & ink on paper)

Chambe, (fl.1784)

CND898774

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