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'Four Star' images and/or videos results page 91 of 13

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Images of 'Four Star' found, 1,120

 
Andromede and Triangle Constellations - Constellations of Andromeda and Triangulum - The constellation of Andromede begins at the brilliant star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegase. Alpheratz is the brightest star in the picture, on the right, and is located about 97 light years away from Earth. Mirach star, in the center of the image, is a giant red star situated about 200 years ago - light. The galaxy of Andromede, M31, is visible at the top of the picture. At the bottom of the mage, in the middle, the galaxy M33. The large open cluster NGC 752 is at the bottom left. The constellations of Andromeda, the Princess, and Triangulum, the Triangle, point the way to several deep - sky delights in the fall sky. Andromeda begins at the bright star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegasus. Alpheratz is the brightest star in the image, near the right side of the frame and is located about 97 light years away f

Jerry Lodriguss

PIX4588980

Andromede and Triangle Constellations - Constellations of Andromeda and Triangulum - The constellation of Andromede begins at the brilliant star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegase. Alpheratz is the brightest star in the picture, on the right, and is located about 97 light years away from Earth. Mirach star, in the center of the image, is a giant red star situated about 200 years ago - light. The galaxy of Andromede, M31, is visible at the top of the picture. At the bottom of the mage, in the middle, the galaxy M33. The large open cluster NGC 752 is at the bottom left. The constellations of Andromeda, the Princess, and Triangulum, the Triangle, point the way to several deep - sky delights in the fall sky. Andromeda begins at the bright star Alpheratz, or Alpha Andromedae, one of the corners of the great square of Pegasus. Alpheratz is the brightest star in the image, near the right side of the frame and is located about 97 light years away f

Jerry Lodriguss

PIX4588980

 
Autumn lactee route - Pointe du Raz - Autumn Milky way - Pointe du Raz - The lactee route above Notre Dame des Shipwrecks, Pointe du Raz. Brittany, 27 September 2008. Milky Way above the statue dedicated to “” Our Lady of the Shipwrecks”””. The zodiacal band is visible under the aspect of a fuzzy and pale band extending from the top of the statue to the upper right. A the top of the picture is the powerful lighthouse of the Sein Island. at Pointe du Raz, the western tip of France. Brittany, 27 September 2008

Laurent Laveder

PIX4637152

Autumn lactee route - Pointe du Raz - Autumn Milky way - Pointe du Raz - The lactee route above Notre Dame des Shipwrecks, Pointe du Raz. Brittany, 27 September 2008. Milky Way above the statue dedicated to “” Our Lady of the Shipwrecks”””. The zodiacal band is visible under the aspect of a fuzzy and pale band extending from the top of the statue to the upper right. A the top of the picture is the powerful lighthouse of the Sein Island. at Pointe du Raz, the western tip of France. Brittany, 27 September 2008

Laurent Laveder

PIX4637152

 
Autumn lactee route - Pointe du Raz - Autumn Milky way - Pointe du Raz - The lactee route above Notre Dame des Shipwrecks, Pointe du Raz. Brittany, 27 September 2008. Milky Way above the statue dedicated to “” Our Lady of the Shipwrecks”””. The zodiacal band is visible under the aspect of a fuzzy and pale band extending from the top of the statue to the upper right. A the top of the picture is the powerful lighthouse of the Sein Island. at Pointe du Raz, the western tip of France. Brittany, 27 September 2008

Laurent Laveder

PIX4637204

Autumn lactee route - Pointe du Raz - Autumn Milky way - Pointe du Raz - The lactee route above Notre Dame des Shipwrecks, Pointe du Raz. Brittany, 27 September 2008. Milky Way above the statue dedicated to “” Our Lady of the Shipwrecks”””. The zodiacal band is visible under the aspect of a fuzzy and pale band extending from the top of the statue to the upper right. A the top of the picture is the powerful lighthouse of the Sein Island. at Pointe du Raz, the western tip of France. Brittany, 27 September 2008

Laurent Laveder

PIX4637204

 
Walk under the Lactee Way - Nigth sky observation - Two back girls observe the lactee path standing in the dunes. Two girls watching milky way above the ocean

Laurent Laveder

PIX4566247

Walk under the Lactee Way - Nigth sky observation - Two back girls observe the lactee path standing in the dunes. Two girls watching milky way above the ocean

Laurent Laveder

PIX4566247

 
Map of the Autumn sky in France - Illustration - Autumn sky map. Artwork - Map plotted for a latitude of 45 degrees north, showing the sky visible in France in late October at about 9 pm, and more broadly in Europe and the world inside a strip stretching from 38 degrees to 52 degrees north latitude. This map also corresponds to the sky visible in mid-night September and early November. The position of the planet Jupiter is given for the beginning of November 2010. Map showing the sky visible in France in october in the end of the evening at 9 p.m (english hour) for a latitude of 45 degrees north. This map also shows the sky in the whole world between 38 degrees and 52 degrees north. This map also refers to september in the middle of the night and to november in the beginning of the evening. Planet Jupiter is shown for the beginning of november 2010

G. Cannat

PIX4594823

Map of the Autumn sky in France - Illustration - Autumn sky map. Artwork - Map plotted for a latitude of 45 degrees north, showing the sky visible in France in late October at about 9 pm, and more broadly in Europe and the world inside a strip stretching from 38 degrees to 52 degrees north latitude. This map also corresponds to the sky visible in mid-night September and early November. The position of the planet Jupiter is given for the beginning of November 2010. Map showing the sky visible in France in october in the end of the evening at 9 p.m (english hour) for a latitude of 45 degrees north. This map also shows the sky in the whole world between 38 degrees and 52 degrees north. This map also refers to september in the middle of the night and to november in the beginning of the evening. Planet Jupiter is shown for the beginning of november 2010

G. Cannat

PIX4594823

 
Map of the autumn sky in France - Illustration - Autumn sky map. Artwork - Map plotted for a latitude of 45 degrees north, showing the sky in October at about 9 pm French time. This card can also be consulted in mid-night September or early November. Jupiter's position at the beginning of November. Map showing the sky in october at 9 p.m (english hour) for a latitude of 45 degrees north (metropolitan France). This map also refers to september in the middle of the night and to november at the beginning of evening. Jupiter is shown for the beginning of november

G. Cannat

PIX4594767

Map of the autumn sky in France - Illustration - Autumn sky map. Artwork - Map plotted for a latitude of 45 degrees north, showing the sky in October at about 9 pm French time. This card can also be consulted in mid-night September or early November. Jupiter's position at the beginning of November. Map showing the sky in october at 9 p.m (english hour) for a latitude of 45 degrees north (metropolitan France). This map also refers to september in the middle of the night and to november at the beginning of evening. Jupiter is shown for the beginning of november

G. Cannat

PIX4594767

 
Map of the Autumn sky in France - Illustration - Autumn sky map. Artwork - Map plotted for a latitude of 45 degrees north, showing the sky visible in France in late October at about 9 pm, and more broadly in Europe and the world inside a strip stretching from 38 degrees to 52 degrees north latitude. This map also corresponds to the sky visible in mid-night September and early November. The position of the planet Jupiter is given for the beginning of November 2010. Map showing the sky visible in France in october in the end of the evening at 9 p.m (english hour) for a latitude of 45 degrees north. This map also shows the sky in the whole world between 38 degrees and 52 degrees north. This map also refers to september in the middle of the night and to november in the beginning of the evening. Planet Jupiter is shown for the beginning of november 2010

G. Cannat

PIX4594829

Map of the Autumn sky in France - Illustration - Autumn sky map. Artwork - Map plotted for a latitude of 45 degrees north, showing the sky visible in France in late October at about 9 pm, and more broadly in Europe and the world inside a strip stretching from 38 degrees to 52 degrees north latitude. This map also corresponds to the sky visible in mid-night September and early November. The position of the planet Jupiter is given for the beginning of November 2010. Map showing the sky visible in France in october in the end of the evening at 9 p.m (english hour) for a latitude of 45 degrees north. This map also shows the sky in the whole world between 38 degrees and 52 degrees north. This map also refers to september in the middle of the night and to november in the beginning of the evening. Planet Jupiter is shown for the beginning of november 2010

G. Cannat

PIX4594829

 
Fin de nuit etoilee - End of an automn night - 19 November 2006, Quimper (Finistere - France)

Laurent Laveder

PIX4581621

Fin de nuit etoilee - End of an automn night - 19 November 2006, Quimper (Finistere - France)

Laurent Laveder

PIX4581621

 
Map of the autumn sky in France - Illustration - Autumn sky map. Artwork - Map plotted for a latitude of 45 degrees north, showing the sky in October at about 9 pm French time. This card can also be consulted in mid-night September or early November. Jupiter's position at the beginning of November. Map showing the sky in october at 9 p.m (english hour) for a latitude of 45 degrees north (metropolitan France). This map also refers to september in the middle of the night and to november at the beginning of evening. Jupiter is shown for the beginning of november

G. Cannat

PIX4594777

Map of the autumn sky in France - Illustration - Autumn sky map. Artwork - Map plotted for a latitude of 45 degrees north, showing the sky in October at about 9 pm French time. This card can also be consulted in mid-night September or early November. Jupiter's position at the beginning of November. Map showing the sky in october at 9 p.m (english hour) for a latitude of 45 degrees north (metropolitan France). This map also refers to september in the middle of the night and to november at the beginning of evening. Jupiter is shown for the beginning of november

G. Cannat

PIX4594777

 
Star watching - Night sky observation - Two girls look at the sky sitting in the dunes, with the Big Bear in the background. Two girls watching the starry sky

Laurent Laveder

PIX4566248

Star watching - Night sky observation - Two girls look at the sky sitting in the dunes, with the Big Bear in the background. Two girls watching the starry sky

Laurent Laveder

PIX4566248

 
Entrance to Restaurant, Dieu Donne Guest House, Franschhoek (photo)

UIG804536

Entrance to Restaurant, Dieu Donne Guest House, Franschhoek (photo)

UIG804536

 
Flag of the Federated States of Micronesia

UIG533688

Flag of the Federated States of Micronesia

UIG533688

 
From Gemeaux to Andromede - Pointe du Raz - From Gemini to Andromeda - Pointe du Raz - Directon de l'Est, Les Gemeaux are getting up, cut in half by the semaphore tower of Pointe du Raz. The cluster of stars M 35, in the lactee lane, is surmounted by the Coach and its 3 star clusters (on the right, above the antenna). Then it is Persee (with Nebula California on the bottom right), the Double Cluster of Persee and finally Cassiopee with the Galaxy of Andromede on its right. Brittany, 27 September 2008. Toward East, Gemini is rising, cut in two by the semaphore tower. The star cluster M35, in the Milky Way, is surmounted by Auriga and its 3 star clusters (above the antenna, on the right). Then, it's Perseus and its double cluster and finally Cassiopeia with the Great Andromeda Galaxy on the right. Pointe du Raz, Brittany, 27 September 2008

Laurent Laveder

PIX4594895

From Gemeaux to Andromede - Pointe du Raz - From Gemini to Andromeda - Pointe du Raz - Directon de l'Est, Les Gemeaux are getting up, cut in half by the semaphore tower of Pointe du Raz. The cluster of stars M 35, in the lactee lane, is surmounted by the Coach and its 3 star clusters (on the right, above the antenna). Then it is Persee (with Nebula California on the bottom right), the Double Cluster of Persee and finally Cassiopee with the Galaxy of Andromede on its right. Brittany, 27 September 2008. Toward East, Gemini is rising, cut in two by the semaphore tower. The star cluster M35, in the Milky Way, is surmounted by Auriga and its 3 star clusters (above the antenna, on the right). Then, it's Perseus and its double cluster and finally Cassiopeia with the Great Andromeda Galaxy on the right. Pointe du Raz, Brittany, 27 September 2008

Laurent Laveder

PIX4594895

 
Lactee route - Pointe du Raz - Milky way - Pointe du Raz - The lactee route above the semaphore of Pointe du Raz. Visible in the sky are the nebula North America, the Great Galaxy of Andromede, the Double Cluster of Persee and the Galaxy of the Triangle. Brittany, 27 September 2008. Milky Way above a control tower at Pointe du Raz, the western tip of France. In the sky are some of the most famous objects in the sky: North America Nebula, the Great Andromeda Galaxy, the Double Star Cluster in Perseus and the Triangulum Galaxy. Brittany, 27 September 2008

Laurent Laveder

PIX4637182

Lactee route - Pointe du Raz - Milky way - Pointe du Raz - The lactee route above the semaphore of Pointe du Raz. Visible in the sky are the nebula North America, the Great Galaxy of Andromede, the Double Cluster of Persee and the Galaxy of the Triangle. Brittany, 27 September 2008. Milky Way above a control tower at Pointe du Raz, the western tip of France. In the sky are some of the most famous objects in the sky: North America Nebula, the Great Andromeda Galaxy, the Double Star Cluster in Perseus and the Triangulum Galaxy. Brittany, 27 September 2008

Laurent Laveder

PIX4637182

 
Lactee route - Pointe du Raz - Milky Way - Pointe du Raz - The Great Bear is almost entirely masked by the semaphore tower at Pointe du Raz. The “Two Guards” located on the right of the tower point towards the Polar Star, vertical of the antenna. Higher, our eye cuts the lactee path near the zenith. As we descend towards the southern horizon, we can see the Great Galaxy of Andromede and that of the Triangle. Brittany, 27 September 2008. The Big Dipper is almost completely masked by the tower of the semaphore. Its two stars on the right are pointing towards the star Polaris, at the vertical of the antenna. Higher, our eye cross the Milky Way near the zenith. Then, descending towards the South, we can see the Great Andromeda Galaxy and the Triangulum Galaxy. Pointe du Raz, Brittany, 27 September 2008

Laurent Laveder

PIX4637219

Lactee route - Pointe du Raz - Milky Way - Pointe du Raz - The Great Bear is almost entirely masked by the semaphore tower at Pointe du Raz. The “Two Guards” located on the right of the tower point towards the Polar Star, vertical of the antenna. Higher, our eye cuts the lactee path near the zenith. As we descend towards the southern horizon, we can see the Great Galaxy of Andromede and that of the Triangle. Brittany, 27 September 2008. The Big Dipper is almost completely masked by the tower of the semaphore. Its two stars on the right are pointing towards the star Polaris, at the vertical of the antenna. Higher, our eye cross the Milky Way near the zenith. Then, descending towards the South, we can see the Great Andromeda Galaxy and the Triangulum Galaxy. Pointe du Raz, Brittany, 27 September 2008

Laurent Laveder

PIX4637219

 
From Gemeaux to Andromede - Pointe du Raz - From Gemini to Andromeda - Pointe du Raz - Directon de l'Est, Les Gemeaux are getting up, cut in half by the semaphore tower of Pointe du Raz. The cluster of stars M 35, in the lactee lane, is surmounted by the Coach and its 3 star clusters (on the right, above the antenna). Then it is Persee (with Nebula California on the bottom right), the Double Cluster of Persee and finally Cassiopee with the Galaxy of Andromede on its right. Brittany, 27 September 2008. Toward East, Gemini is rising, cut in two by the semaphore tower. The star cluster M35, in the Milky Way, is surmounted by Auriga and its 3 star clusters (above the antenna, on the right). Then, it's Perseus and its double cluster and finally Cassiopeia with the Great Andromeda Galaxy on the right. Pointe du Raz, Brittany, 27 September 2008

Laurent Laveder

PIX4594908

From Gemeaux to Andromede - Pointe du Raz - From Gemini to Andromeda - Pointe du Raz - Directon de l'Est, Les Gemeaux are getting up, cut in half by the semaphore tower of Pointe du Raz. The cluster of stars M 35, in the lactee lane, is surmounted by the Coach and its 3 star clusters (on the right, above the antenna). Then it is Persee (with Nebula California on the bottom right), the Double Cluster of Persee and finally Cassiopee with the Galaxy of Andromede on its right. Brittany, 27 September 2008. Toward East, Gemini is rising, cut in two by the semaphore tower. The star cluster M35, in the Milky Way, is surmounted by Auriga and its 3 star clusters (above the antenna, on the right). Then, it's Perseus and its double cluster and finally Cassiopeia with the Great Andromeda Galaxy on the right. Pointe du Raz, Brittany, 27 September 2008

Laurent Laveder

PIX4594908

 
Milky Way behind control tower of Pointe du Raz - Milky Way behind control tower of Pointe du Raz - In this photo, the North America nebula is visible in the upper left corner of the star Deneb. Two soldiers stand on the semaphore bridge at Point du Raz. Brittany, 27 September 2008. People in the control tower are working, monitoring the ships with their binoculars. In this picture, the North America Nebula is visible in the upper left corner, near the star Deneb. Two people are standing on the footbridge. Pointe du Raz, Brittany, 27 September 2008

Laurent Laveder

PIX4637200

Milky Way behind control tower of Pointe du Raz - Milky Way behind control tower of Pointe du Raz - In this photo, the North America nebula is visible in the upper left corner of the star Deneb. Two soldiers stand on the semaphore bridge at Point du Raz. Brittany, 27 September 2008. People in the control tower are working, monitoring the ships with their binoculars. In this picture, the North America Nebula is visible in the upper left corner, near the star Deneb. Two people are standing on the footbridge. Pointe du Raz, Brittany, 27 September 2008

Laurent Laveder

PIX4637200

 
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. 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, crossing the Milky Way. Brittany, 27 September 2008

Laurent Laveder

PIX4637852

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. 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, crossing the Milky Way. Brittany, 27 September 2008

Laurent Laveder

PIX4637852

 
From Gemeaux to Andromede - Pointe du Raz - From Gemini to Andromeda - Pointe du Raz - Directon de l'Est, Les Gemeaux are getting up, cut in half by the semaphore tower of Pointe du Raz. The cluster of stars M 35, in the lactee lane, is surmounted by the Coach and its 3 star clusters (on the right, above the antenna). Then it is Persee (with Nebula California on the bottom right), the Double Cluster of Persee and finally Cassiopee with the Galaxy of Andromede on its right. Brittany, 27 September 2008. Toward East, Gemini is rising, cut in two by the semaphore tower. The star cluster M35, in the Milky Way, is surmounted by Auriga and its 3 star clusters (above the antenna, on the right). Then, it's Perseus and its double cluster and finally Cassiopeia with the Great Andromeda Galaxy on the right. Pointe du Raz, Brittany, 27 September 2008

Laurent Laveder

PIX4594888

From Gemeaux to Andromede - Pointe du Raz - From Gemini to Andromeda - Pointe du Raz - Directon de l'Est, Les Gemeaux are getting up, cut in half by the semaphore tower of Pointe du Raz. The cluster of stars M 35, in the lactee lane, is surmounted by the Coach and its 3 star clusters (on the right, above the antenna). Then it is Persee (with Nebula California on the bottom right), the Double Cluster of Persee and finally Cassiopee with the Galaxy of Andromede on its right. Brittany, 27 September 2008. Toward East, Gemini is rising, cut in two by the semaphore tower. The star cluster M35, in the Milky Way, is surmounted by Auriga and its 3 star clusters (above the antenna, on the right). Then, it's Perseus and its double cluster and finally Cassiopeia with the Great Andromeda Galaxy on the right. Pointe du Raz, Brittany, 27 September 2008

Laurent Laveder

PIX4594888

 
Orion to Andromede - Pointe du Raz - From Orion to Andromeda - Pointe du Raz - Directon south - east, Orion is standing behind the semaphore of Pointe du Raz. Higher, the Taurus and the Pleiades, then Persee and the Triangle, and finally Andromede (and Cassiope all left). Brittany, 27 September 2008. Toward South - East, Orion is rising behind the semaphore. Higher, the Taurus and the Pleiades, then Perseus and the Triangulum and finally Andromeda (and Cassiopeia on the far left). Pointe du Raz, Brittany, 27 September 2008

Laurent Laveder

PIX4594919

Orion to Andromede - Pointe du Raz - From Orion to Andromeda - Pointe du Raz - Directon south - east, Orion is standing behind the semaphore of Pointe du Raz. Higher, the Taurus and the Pleiades, then Persee and the Triangle, and finally Andromede (and Cassiope all left). Brittany, 27 September 2008. Toward South - East, Orion is rising behind the semaphore. Higher, the Taurus and the Pleiades, then Perseus and the Triangulum and finally Andromeda (and Cassiopeia on the far left). Pointe du Raz, Brittany, 27 September 2008

Laurent Laveder

PIX4594919

 
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

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

 
Orion to Andromede - Pointe du Raz - From Orion to Andromeda - Pointe du Raz - Directon south - east, Orion is standing behind the semaphore of Pointe du Raz. Higher, the Taurus and the Pleiades, then Persee and the Triangle, and finally Andromede (and Cassiope all left). Brittany, 27 September 2008. Toward South - East, Orion is rising behind the semaphore. Higher, the Taurus and the Pleiades, then Perseus and the Triangulum and finally Andromeda (and Cassiopeia on the far left). Pointe du Raz, Brittany, 27 September 2008

Laurent Laveder

PIX4594912

Orion to Andromede - Pointe du Raz - From Orion to Andromeda - Pointe du Raz - Directon south - east, Orion is standing behind the semaphore of Pointe du Raz. Higher, the Taurus and the Pleiades, then Persee and the Triangle, and finally Andromede (and Cassiope all left). Brittany, 27 September 2008. Toward South - East, Orion is rising behind the semaphore. Higher, the Taurus and the Pleiades, then Perseus and the Triangulum and finally Andromeda (and Cassiopeia on the far left). Pointe du Raz, Brittany, 27 September 2008

Laurent Laveder

PIX4594912

 
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Usage restrictions from our Content Partners
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Rosy feather Star (Antedon bifida), Antedonidae, drawing

DGA1262261

Rosy feather Star (Antedon bifida), Antedonidae, drawing

DGA1262261

 
Orion to Andromede - Pointe du Raz - From Orion to Andromeda - Pointe du Raz - Directon south - east, Orion is standing behind the semaphore of Pointe du Raz. Higher, the Taurus and the Pleiades, then Persee and the Triangle, and finally Andromede (and Cassiopee all left). Brittany, 27 September 2008. In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. Toward South - East, Orion is rising behind the semaphore. Higher, the Taurus and the Pleiades, then Perseus and the Triangulum and finally Andromeda (and Cassiopeia on the far left). Pointe du Raz, Brittany, 27 September 2008. Mythological Constellations forms from “Uranographia” star atlas by Hevelius (1690) have been added

Laurent Laveder

PIX4594938

Orion to Andromede - Pointe du Raz - From Orion to Andromeda - Pointe du Raz - Directon south - east, Orion is standing behind the semaphore of Pointe du Raz. Higher, the Taurus and the Pleiades, then Persee and the Triangle, and finally Andromede (and Cassiopee all left). Brittany, 27 September 2008. In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. Toward South - East, Orion is rising behind the semaphore. Higher, the Taurus and the Pleiades, then Perseus and the Triangulum and finally Andromeda (and Cassiopeia on the far left). Pointe du Raz, Brittany, 27 September 2008. Mythological Constellations forms from “Uranographia” star atlas by Hevelius (1690) have been added

Laurent Laveder

PIX4594938

 
The Milky Way above The Isle of Sein, Brittany, 27 September 2008

Laurent Laveder

PIX4637202

The Milky Way above The Isle of Sein, Brittany, 27 September 2008

Laurent Laveder

PIX4637202

 
Birkenhead House, Hermanus, Western Cape (photo)

UIG805524

Birkenhead House, Hermanus, Western Cape (photo)

UIG805524

 
Orion's Trapeze - Trapezium Multiple Star System in Orion - Orion's Trapeze is one of the youngest open clusters known, with new stars still forming in this region. The Trapezium is the most famous multiple star system in the entire night sky. Located at the very heart of M42, the Orion Nebula, it is one of the youngest star clusters known. The four brightest stars in the Trapezium (A, B, C and D) are easily visible in a four inch telescope with decent optical quality under good seeing conditions. They range in brightness from magnitude 5 to magnitude 8. They can be seen merged together as one star to the unaided eye as the middle star in the sword of Orion. The image above shows the four brightest stars of the Trapezium at the center of the photo. The core of M42 surrounding the Trapezium is a blue - green color from the predominantly green spectral emission line of Oxygen III, with a smaller amount of blue - green mixed in from the hydrogen - beta emission line. These particular wave

Jerry Lodriguss

PIX4617879

Orion's Trapeze - Trapezium Multiple Star System in Orion - Orion's Trapeze is one of the youngest open clusters known, with new stars still forming in this region. The Trapezium is the most famous multiple star system in the entire night sky. Located at the very heart of M42, the Orion Nebula, it is one of the youngest star clusters known. The four brightest stars in the Trapezium (A, B, C and D) are easily visible in a four inch telescope with decent optical quality under good seeing conditions. They range in brightness from magnitude 5 to magnitude 8. They can be seen merged together as one star to the unaided eye as the middle star in the sword of Orion. The image above shows the four brightest stars of the Trapezium at the center of the photo. The core of M42 surrounding the Trapezium is a blue - green color from the predominantly green spectral emission line of Oxygen III, with a smaller amount of blue - green mixed in from the hydrogen - beta emission line. These particular wave

Jerry Lodriguss

PIX4617879

 
Permissions
  • Permission required for immersive exhibition use - Please contact us;Permission required for TV use - Please contact us
Usage restrictions from our Content Partners
  • Not available to clients invoiced in Italy
Meeting of military vehicles, Willys MB 8 Jeep, 1941

DGA550228

Meeting of military vehicles, Willys MB 8 Jeep, 1941

DGA550228

 
End of an Autumn Night - End of an Autumn Night - In this photo taken at the end of the night at the end of autumn, the winter constellations lie to the right (the Big Dog, Orion and the Gems) while rise to the left of the spring constellations: the Boreale Crown, the Bovier above, followed by the tail of the Great Bear, the Virgin then the Raven with the Lion higher. In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. 19 November 2006, Quimper (Finistere - France). End of an automn night with at right, winter constellations setting and at left spring constellations rising. Constellation mythological forms from “” Uranographia”” star atlas by Hevelius (1690) have been added. November 19 2006, Quimper (Finistere - France)

Laurent Laveder

PIX4594561

End of an Autumn Night - End of an Autumn Night - In this photo taken at the end of the night at the end of autumn, the winter constellations lie to the right (the Big Dog, Orion and the Gems) while rise to the left of the spring constellations: the Boreale Crown, the Bovier above, followed by the tail of the Great Bear, the Virgin then the Raven with the Lion higher. In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. 19 November 2006, Quimper (Finistere - France). End of an automn night with at right, winter constellations setting and at left spring constellations rising. Constellation mythological forms from “” Uranographia”” star atlas by Hevelius (1690) have been added. November 19 2006, Quimper (Finistere - France)

Laurent Laveder

PIX4594561

 
Usage restrictions from our Content Partners
  • Not available to clients invoiced in Japan
Sea star or starfish with five arms, upper side, Asterias rubens B, another starfish species 1,2, sea star with four arms 3,4, and small sea star 5. Handcoloured copperplate engraving from Georg Wolfgang Knorr's Deliciae Naturae Selectae of Kabinet van Zeldzaamheden der Natuur, Blusse and Son, Nuremberg, 1771.

FLO4652648

Sea star or starfish with five arms, upper side, Asterias rubens B, another starfish species 1,2, sea star with four arms 3,4, and small sea star 5. Handcoloured copperplate engraving from Georg Wolfgang Knorr's Deliciae Naturae Selectae of Kabinet van Zeldzaamheden der Natuur, Blusse and Son, Nuremberg, 1771.

FLO4652648

 
Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - The galaxy NGC 4038 - 39 (antenna galaxy) is located about 45 million years ago - light. These two galaxies are interacting. The collision started at least 100 million years ago causes intense star formation. These images made by the Hubble space telescope on 20 January 1996 show in detail the nuclei of these two twin galaxies (right) as well as clusters of blue stars, consisting of young and massive stars (left). The scale bar at the top of each image represents 1500 years - light. These four close - up views are taken from a head - on collision between two spiral galaxies, called the Antennae galaxies, seen at image center. The scale bar at the top of each image is 1,500 light - years across. Left: the collision triggers the birth of new stars in brilliant blue star clusters, the brightest of which contains roughly a million stars. The star clusters are blue because they are very young, the youngest b

PIX4611053

Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - The galaxy NGC 4038 - 39 (antenna galaxy) is located about 45 million years ago - light. These two galaxies are interacting. The collision started at least 100 million years ago causes intense star formation. These images made by the Hubble space telescope on 20 January 1996 show in detail the nuclei of these two twin galaxies (right) as well as clusters of blue stars, consisting of young and massive stars (left). The scale bar at the top of each image represents 1500 years - light. These four close - up views are taken from a head - on collision between two spiral galaxies, called the Antennae galaxies, seen at image center. The scale bar at the top of each image is 1,500 light - years across. Left: the collision triggers the birth of new stars in brilliant blue star clusters, the brightest of which contains roughly a million stars. The star clusters are blue because they are very young, the youngest b

PIX4611053

 
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Untitled, 1915 (w/c with pen on paper mounted on cardboard)

Klee, Paul (1879-1940)

PCD282353

Untitled, 1915 (w/c with pen on paper mounted on cardboard)

Klee, Paul (1879-1940)

PCD282353

 
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Postage stamps from series honoring Constellations visible from Namibia, 1996, depicting, from left to right and from top to bottom: Orion, Southern Cross, Sagittarius, Scorpio, Namibia, 20th century

DGA2582876

Postage stamps from series honoring Constellations visible from Namibia, 1996, depicting, from left to right and from top to bottom: Orion, Southern Cross, Sagittarius, Scorpio, Namibia, 20th century

DGA2582876

 
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Reed Birney, on-set of the Film, "Four Friends", Filmways Pictures, 1981 (b/w photo)

Unknown photographer, (20th century)

GLH6326575

Reed Birney, on-set of the Film, "Four Friends", Filmways Pictures, 1981 (b/w photo)

Unknown photographer, (20th century)

GLH6326575

 
Nebula N44 in the Large Magellan Cloud - Superbubble LHA 120 - N 44 in the Large Magellanic Cloud - This image obtained by the Very Large Telescope (VLT) shows the nebula N44 surrounding the cluster of stars NGC 1929. It is a star-forming region located in the galaxy of the Great Magellan Cloud, about 170,000 light years from Earth. Eso's Very Large Telescope captured this striking view of the nebula around the star cluster NGC 1929 within the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. A colossal example of what astronomers call a superbubble dominates this stellar nursery. It is being carved by the winds from bright young stars and the shockwaves from supernova explosions. This nebula is officially known as LHA 120 - N 44, or just N 44 for short. Hot young stars in NGC 1929 are emitting intense ultraviolet light and causing the gas to glow. This effect highlights the aptly - named superbubble, a vast shell of material around 325 by 250 light - years across. For c

PIX4620802

Nebula N44 in the Large Magellan Cloud - Superbubble LHA 120 - N 44 in the Large Magellanic Cloud - This image obtained by the Very Large Telescope (VLT) shows the nebula N44 surrounding the cluster of stars NGC 1929. It is a star-forming region located in the galaxy of the Great Magellan Cloud, about 170,000 light years from Earth. Eso's Very Large Telescope captured this striking view of the nebula around the star cluster NGC 1929 within the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. A colossal example of what astronomers call a superbubble dominates this stellar nursery. It is being carved by the winds from bright young stars and the shockwaves from supernova explosions. This nebula is officially known as LHA 120 - N 44, or just N 44 for short. Hot young stars in NGC 1929 are emitting intense ultraviolet light and causing the gas to glow. This effect highlights the aptly - named superbubble, a vast shell of material around 325 by 250 light - years across. For c

PIX4620802

 
Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - On the left, seen from the ground of the galaxy NGC 4038 - 39 (antenna galaxy), located about 45 million years ago - light. These two galaxies are interacting. The collision started at least 100 million years ago causes intense star formation. On the right, the image made by the space telescope Hubble on 20 January 1996 shows in detail the nuclei of these two twin galaxies surrounded by young clusters of blue stars, more than 1000, made up of young and massive stars. At left, a ground - based telescopic view of the Antennae galaxies (known formally as NGC 4038/4039) - so named because a pair of long tails of luminous matter, formed by the gravitational tidal forces of their encounter, resemble an insect's antennae. The galaxies are located 45 million light - years away in the southern constellation Corvus. At right, the respective cores of the twin galaxies are the orange blobs, left and right of image

PIX4611051

Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - On the left, seen from the ground of the galaxy NGC 4038 - 39 (antenna galaxy), located about 45 million years ago - light. These two galaxies are interacting. The collision started at least 100 million years ago causes intense star formation. On the right, the image made by the space telescope Hubble on 20 January 1996 shows in detail the nuclei of these two twin galaxies surrounded by young clusters of blue stars, more than 1000, made up of young and massive stars. At left, a ground - based telescopic view of the Antennae galaxies (known formally as NGC 4038/4039) - so named because a pair of long tails of luminous matter, formed by the gravitational tidal forces of their encounter, resemble an insect's antennae. The galaxies are located 45 million light - years away in the southern constellation Corvus. At right, the respective cores of the twin galaxies are the orange blobs, left and right of image

PIX4611051

 
Nebula NGC 3372 in the Carene - NGC 3372, Eta Carinae nebula - The nebula of the Carene is located about 8000 years - light from the Earth. It is home to many hot massive stars, including the star Eta Carinae in the centre of the nebula. This nebula is larger than the Great Nebula in Orion, but is not visible from most northern latitudes. It is a giant complex of emission and dark nebulae surrounding the unique variable star Eta Carinae, which scientists believe is the most massive and energetic star in the Milky Way galaxy. Located about 8,500 light years from the Earth, the star is about 100 times as massive as our own Sun, but produces 6 million times the light output. It was observed producing a remarkable burst of X - ray emissions that doubled its X - ray output in only four months. In the 1840's, Eta Carinae erupted visibly and was the second brightest star in the sky during this time

Jerry Lodriguss

PIX4618875

Nebula NGC 3372 in the Carene - NGC 3372, Eta Carinae nebula - The nebula of the Carene is located about 8000 years - light from the Earth. It is home to many hot massive stars, including the star Eta Carinae in the centre of the nebula. This nebula is larger than the Great Nebula in Orion, but is not visible from most northern latitudes. It is a giant complex of emission and dark nebulae surrounding the unique variable star Eta Carinae, which scientists believe is the most massive and energetic star in the Milky Way galaxy. Located about 8,500 light years from the Earth, the star is about 100 times as massive as our own Sun, but produces 6 million times the light output. It was observed producing a remarkable burst of X - ray emissions that doubled its X - ray output in only four months. In the 1840's, Eta Carinae erupted visibly and was the second brightest star in the sky during this time

Jerry Lodriguss

PIX4618875

 
C. Aubrey Smith, (standing), on-set of the Film "The Four Feathers", 1939

GLH2559277

C. Aubrey Smith, (standing), on-set of the Film "The Four Feathers", 1939

GLH2559277

 
Orion nebula centre - Trapeze - Orion nebula center - Mosaic of images obtained by the space telescope in 1994 and 1995 showing the center of Orion nebula, the region around the Trapeze, a cluster of 4 very young and massive stars that make this nebula shine. The picture shows a churning turbulent star factory set within a maelstrom of flowing, luminescent gas. Although this 2.5 light - years wide view is still a small portion of the entire Orion nebula, it includes almost all of the light from the bright glowing clouds of gas and a star cluster associated with the nebula. Hubble reveals details as small as 4.1 billion miles across. Hubble Space Telescope observing time was devoted to making this panorama because the nebula is a vast laboratory for studying the processes which gave birth to our own Sun and solar system 4.5 billion years ago. Gas are illuminated and heated by a torrent of energetic ultraviolet light from its four hottest and most massive stars, called the Trapezium, whi

PIX4617855

Orion nebula centre - Trapeze - Orion nebula center - Mosaic of images obtained by the space telescope in 1994 and 1995 showing the center of Orion nebula, the region around the Trapeze, a cluster of 4 very young and massive stars that make this nebula shine. The picture shows a churning turbulent star factory set within a maelstrom of flowing, luminescent gas. Although this 2.5 light - years wide view is still a small portion of the entire Orion nebula, it includes almost all of the light from the bright glowing clouds of gas and a star cluster associated with the nebula. Hubble reveals details as small as 4.1 billion miles across. Hubble Space Telescope observing time was devoted to making this panorama because the nebula is a vast laboratory for studying the processes which gave birth to our own Sun and solar system 4.5 billion years ago. Gas are illuminated and heated by a torrent of energetic ultraviolet light from its four hottest and most massive stars, called the Trapezium, whi

PIX4617855

 
Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavi

PIX4621160

Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavi

PIX4621160

 
Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavi

PIX4621152

Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavi

PIX4621152

 
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Sea star or starfish with five arms, Asterias rubens 1, starfish from America 2, sea star regenerating one arm 3, four-armed starfish 4, five-armed starfish 5.6. Handcoloured copperplate engraving by Johann Sebastian Leitner after an illustration by Christian Leinberger from Georg Wolfgang Knorr's Deliciae Naturae Selectae of Kabinet van Zeldzaamheden der Natuur, Blusse and Son, Nuremberg, 1771. Specimens from a Wunderkammer or Cabinet of Curiosities of P.L. Muller.

FLO4652653

Sea star or starfish with five arms, Asterias rubens 1, starfish from America 2, sea star regenerating one arm 3, four-armed starfish 4, five-armed starfish 5.6. Handcoloured copperplate engraving by Johann Sebastian Leitner after an illustration by Christian Leinberger from Georg Wolfgang Knorr's Deliciae Naturae Selectae of Kabinet van Zeldzaamheden der Natuur, Blusse and Son, Nuremberg, 1771. Specimens from a Wunderkammer or Cabinet of Curiosities of P.L. Muller.

FLO4652653

 
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Meeting of armored military vehicles, M8 Greyhound, 1942

DGA550246

Meeting of armored military vehicles, M8 Greyhound, 1942

DGA550246

 
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Meeting of armored military vehicles, M8 Greyhound, 1942

DGA550249

Meeting of armored military vehicles, M8 Greyhound, 1942

DGA550249

 
Barree spiral galaxy NGC 6744 in the constellation Peacock - Barred spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is located about 25 million years ago - light from Earth. The morphology of this galaxy is very similar to that of our galaxy, the Lactee Way. Image obtained from the 3.9m telescope of Siding Spring, Australia. This beautiful galaxy is about 25 million light years away in the direction of Pavo, a constellation of the southern hemisphere winter. NGC 6744 is believed to one of the most Milky Way - like of all the nearby spirals, with fluffy (flocculent) spiral arms and a large and distinctly elongated nucleus. It also has other similarities to the Milky Way that are not visible here (but seen on a deep image) with at least one distorted companion galaxy superficially similar to one of the Magellanic Clouds. The CCD chip that made this picture at the prime focus of the AAT (Siding Spring) covers about 7 arc minutes of sky. But the galaxy has a much bigger angular size t

PIX4612955

Barree spiral galaxy NGC 6744 in the constellation Peacock - Barred spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is located about 25 million years ago - light from Earth. The morphology of this galaxy is very similar to that of our galaxy, the Lactee Way. Image obtained from the 3.9m telescope of Siding Spring, Australia. This beautiful galaxy is about 25 million light years away in the direction of Pavo, a constellation of the southern hemisphere winter. NGC 6744 is believed to one of the most Milky Way - like of all the nearby spirals, with fluffy (flocculent) spiral arms and a large and distinctly elongated nucleus. It also has other similarities to the Milky Way that are not visible here (but seen on a deep image) with at least one distorted companion galaxy superficially similar to one of the Magellanic Clouds. The CCD chip that made this picture at the prime focus of the AAT (Siding Spring) covers about 7 arc minutes of sky. But the galaxy has a much bigger angular size t

PIX4612955

 
Spiral Galaxy NGC 253 in Sculptor - Spiral galaxy NGC 253 in Sculptor - NGC 253 is the brightest galaxy of the Sculptor's group, the closest galaxy group to the Local Group. It is about 13 million light years away. Image obtained with the 2,2m MPG/ESO telescope of La Silla. Measuring 70 000 light - years across and lying 13 million light - years away, the nearly edge - on spiral galaxy NGC 253 is revealed here in an image from the Wide Field Imager (WFI) of the MPG/ESO 2.2 m telescope at the La Silla Observatory. The image is based on data obtained through four different filters (R, V, H - alpha and OIII). North is up and East to the left. The field of view is 30 arcminutes

PIX4609140

Spiral Galaxy NGC 253 in Sculptor - Spiral galaxy NGC 253 in Sculptor - NGC 253 is the brightest galaxy of the Sculptor's group, the closest galaxy group to the Local Group. It is about 13 million light years away. Image obtained with the 2,2m MPG/ESO telescope of La Silla. Measuring 70 000 light - years across and lying 13 million light - years away, the nearly edge - on spiral galaxy NGC 253 is revealed here in an image from the Wide Field Imager (WFI) of the MPG/ESO 2.2 m telescope at the La Silla Observatory. The image is based on data obtained through four different filters (R, V, H - alpha and OIII). North is up and East to the left. The field of view is 30 arcminutes

PIX4609140

 
Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds

PIX4572084

Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds

PIX4572084

 
Spiral galaxy NGC 6744 in the constellation Peacock - Spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is about 30 million years away - light from Earth. This galaxy is very similar to our galaxy, the lactee path. Image obtained by the 2.2 meter MPG/ESO telescope at the La Silla Observatory. This picture of the nearby galaxy NGC 6744 was taken with the Wide Field Imager on the MPG/ESO 2.2 - metre telescope at La Silla. The large spiral galaxy is similar to the Milky Way, making this image look like a picture postcard of our own galaxy sent from extragalactic space. The picture was created from exposures taken through four different filters that passed blue, yellow - green, red light, and the glow coming from hydrogen gas. These are shown in this picture as blue, green, orange and red, respectively

PIX4613001

Spiral galaxy NGC 6744 in the constellation Peacock - Spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is about 30 million years away - light from Earth. This galaxy is very similar to our galaxy, the lactee path. Image obtained by the 2.2 meter MPG/ESO telescope at the La Silla Observatory. This picture of the nearby galaxy NGC 6744 was taken with the Wide Field Imager on the MPG/ESO 2.2 - metre telescope at La Silla. The large spiral galaxy is similar to the Milky Way, making this image look like a picture postcard of our own galaxy sent from extragalactic space. The picture was created from exposures taken through four different filters that passed blue, yellow - green, red light, and the glow coming from hydrogen gas. These are shown in this picture as blue, green, orange and red, respectively

PIX4613001

 
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)

PIX4612524

 
Globular cluster NGC 6397 in the Altar - Stars in globular cluster NGC 6397 in Ara - Image of the center of the globular cluster NGC 6397 located 8200 years - light in the southern constellation of the Altar. The density of stars is very important, the stars are distant from each other only a few weeks light (the star closest to our Sun is four years away - light). Sometimes a collision between two stars occurs; they merge into a single, young, bright and warm star called a blue straggler; some of these stars are visible near the center of the image. This Hubble Space Telescope view of the core of one of the nearest globular star clusters, called NGC 6397, located 8,200 light - years away in the constellation Ara. The stellar density is about a million times greater than in our Sun's stellar neighborhood. The stars are only a few light - weeks apart, while the nearest star to our Sun is over four light - years away. The ancient stars are so crowded together that a few of them inevitabl

PIX4564803

Globular cluster NGC 6397 in the Altar - Stars in globular cluster NGC 6397 in Ara - Image of the center of the globular cluster NGC 6397 located 8200 years - light in the southern constellation of the Altar. The density of stars is very important, the stars are distant from each other only a few weeks light (the star closest to our Sun is four years away - light). Sometimes a collision between two stars occurs; they merge into a single, young, bright and warm star called a blue straggler; some of these stars are visible near the center of the image. This Hubble Space Telescope view of the core of one of the nearest globular star clusters, called NGC 6397, located 8,200 light - years away in the constellation Ara. The stellar density is about a million times greater than in our Sun's stellar neighborhood. The stars are only a few light - weeks apart, while the nearest star to our Sun is over four light - years away. The ancient stars are so crowded together that a few of them inevitabl

PIX4564803

 
Star of David on a gravestone at Pere Lachaise cemetery, Paris, France

GNG5257319

Star of David on a gravestone at Pere Lachaise cemetery, Paris, France

GNG5257319

 
Nebula NGC 3372 in the Carene - NGC 3372 Carina nebula - The Carene Nebula (NGC 3372) is a very large region of star formation visible in the southern hemisphere. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). The bright star in the center of the image is Eta Carinae, a super massive star. The Carina Nebula (also known as the Great Nebula in Carina, the Eta Carinae Nebula, or NGC 3372) is a large bright nebula that surrounds several open clusters of stars. Eta Carinae and HD 93129A, two of the most massive and luminous stars in our Milky Way galaxy, are among them. The nebula lies at an estimated distance between 6,500 and 10,000 light years from Earth. It is located in the constellation of Carina. The nebula contains multiple O - type stars. This nebula is one of the largest H II regions in the Milky Way. It has a visual magnitude of 1.0. The nebula is one of the largest diffuse nebulae in our skies. Although it is some fou

Tom Davis

PIX4619112

Nebula NGC 3372 in the Carene - NGC 3372 Carina nebula - The Carene Nebula (NGC 3372) is a very large region of star formation visible in the southern hemisphere. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). The bright star in the center of the image is Eta Carinae, a super massive star. The Carina Nebula (also known as the Great Nebula in Carina, the Eta Carinae Nebula, or NGC 3372) is a large bright nebula that surrounds several open clusters of stars. Eta Carinae and HD 93129A, two of the most massive and luminous stars in our Milky Way galaxy, are among them. The nebula lies at an estimated distance between 6,500 and 10,000 light years from Earth. It is located in the constellation of Carina. The nebula contains multiple O - type stars. This nebula is one of the largest H II regions in the Milky Way. It has a visual magnitude of 1.0. The nebula is one of the largest diffuse nebulae in our skies. Although it is some fou

Tom Davis

PIX4619112

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