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Centro Habana district in Havana, Cuba.
Centro Habana district in Havana, Cuba.

TEC4593269: Centro Habana district in Havana, Cuba. / Bridgeman Images

ID: TEC4593269

Centro Habana district in Havana, Cuba.

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: 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 / Bridgeman Images

ID: PIX4593306

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

Church of Saint Thibault in Burgundy (Cote d'Or).
Church of Saint Thibault in Burgundy (Cote d'Or).

ITR4593355: Church of Saint Thibault in Burgundy (Cote d'Or). / Bridgeman Images

ID: ITR4593355

Church of Saint Thibault in Burgundy (Cote d'Or).

Little Fox Constellation - Constellation of Vulpecula - Uranographia by Johann Bode (1801) recolorized by us Uranographia by Johann Bode (1801), recolored
Little Fox Constellation - Constellation of Vulpecula - Uranographia by Johann Bode (1801) recolorized by us Uranographia by Johann Bode (1801), recolored

PIX4593409: Little Fox Constellation - Constellation of Vulpecula - Uranographia by Johann Bode (1801) recolorized by us Uranographia by Johann Bode (1801), recolored / Bridgeman Images

ID: PIX4593409

Little Fox Constellation - Constellation of Vulpecula - Uranographia by Johann Bode (1801) recolorized by us Uranographia by Johann Bode (1801), recolored

Abbey of Pontigny in the Yonne. Photography 15/11/03.
Abbey of Pontigny in the Yonne. Photography 15/11/03.

ITR4593443: Abbey of Pontigny in the Yonne. Photography 15/11/03. / Bridgeman Images

ID: ITR4593443

Abbey of Pontigny in the Yonne. Photography 15/11/03.

Batobus on the Seine in Paris.
Batobus on the Seine in Paris.

TEC4593619: Batobus on the Seine in Paris. / Bridgeman Images

ID: TEC4593619

Batobus on the Seine in Paris.

The Pont de la Concorde (1787-1791). Built with the stones of the Bastille fortress, it connected the faubourg Saint-Germain to the faubourg Saint-Honore, architect Jean Rodolphe (Jean-Rodolphe) Perronet.
The Pont de la Concorde (1787-1791). Built with the stones of the Bastille fortress, it connected the faubourg Saint-Germain to the faubourg Saint-Honore, architect Jean Rodolphe (Jean-Rodolphe) Perronet.

LBY4593673: The Pont de la Concorde (1787-1791). Built with the stones of the Bastille fortress, it connected the faubourg Saint-Germain to the faubourg Saint-Honore, architect Jean Rodolphe (Jean-Rodolphe) Perronet. / Bridgeman Images

ID: LBY4593673

The Pont de la Concorde (1787-1791). Built with the stones of the Bastille fortress, it connected the faubourg Saint-Germain to the faubourg Saint-Honore, architect Jean Rodolphe (Jean-Rodolphe) Perronet.

Constellation of Sagittarius - Constellation of Sagittarius - The constellation of Sagittarius with its mythological form extracted from the Uranographia of Hevelius. Map showing the constellation of Sagittarius with its mythological form from “Uranographia”” star atlas by Hevelius (1690) added
Constellation of Sagittarius - Constellation of Sagittarius - The constellation of Sagittarius with its mythological form extracted from the Uranographia of Hevelius. Map showing the constellation of Sagittarius with its mythological form from “Uranographia”” star atlas by Hevelius (1690) added

PIX4593678: Constellation of Sagittarius - Constellation of Sagittarius - The constellation of Sagittarius with its mythological form extracted from the Uranographia of Hevelius. Map showing the constellation of Sagittarius with its mythological form from “Uranographia”” star atlas by Hevelius (1690) added / Bridgeman Images

ID: PIX4593678

Constellation of Sagittarius - Constellation of Sagittarius - The constellation of Sagittarius with its mythological form extracted from the Uranographia of Hevelius. Map showing the constellation of Sagittarius with its mythological form from “Uranographia”” star atlas by Hevelius (1690) added

Pont Bir Hakeim (Bir-Hakeim), Paris 15th arrondissement. Ex Passy Viaduct, it became in 1949 the bridge of Bir Hakeim. One of the most beautiful sites of metal architecture. The 237-metre bridge has the particularity of being both metropolitan, automobile and pedestrian. Architect Louis Biette (1860-1939) and Jean Camille Formige (1845-1926), 1903-1905.
Pont Bir Hakeim (Bir-Hakeim), Paris 15th arrondissement. Ex Passy Viaduct, it became in 1949 the bridge of Bir Hakeim. One of the most beautiful sites of metal architecture. The 237-metre bridge has the particularity of being both metropolitan, automobile and pedestrian. Architect Louis Biette (1860-1939) and Jean Camille Formige (1845-1926), 1903-1905.

LBY4593703: Pont Bir Hakeim (Bir-Hakeim), Paris 15th arrondissement. Ex Passy Viaduct, it became in 1949 the bridge of Bir Hakeim. One of the most beautiful sites of metal architecture. The 237-metre bridge has the particularity of being both metropolitan, automobile and pedestrian. Architect Louis Biette (1860-1939) and Jean Camille Formige (1845-1926), 1903-1905. / Bridgeman Images

ID: LBY4593703

Pont Bir Hakeim (Bir-Hakeim), Paris 15th arrondissement. Ex Passy Viaduct, it became in 1949 the bridge of Bir Hakeim. One of the most beautiful sites of metal architecture. The 237-metre bridge has the particularity of being both metropolitan, automobile and pedestrian. Architect Louis Biette (1860-1939) and Jean Camille Formige (1845-1926), 1903-1905.

Universe has 11 dimensions - 11-dimension Universe - Many universes could coexist and evolve in completely different ways. Artwork showing multiple universes
Universe has 11 dimensions - 11-dimension Universe - Many universes could coexist and evolve in completely different ways. Artwork showing multiple universes

PIX4634649: Universe has 11 dimensions - 11-dimension Universe - Many universes could coexist and evolve in completely different ways. Artwork showing multiple universes / Bridgeman Images

ID: PIX4634649

Universe has 11 dimensions - 11-dimension Universe - Many universes could coexist and evolve in completely different ways. Artwork showing multiple universes

Cathedrale Saint Corentin (Saint Corentin) in Quimper, Brittany.
Cathedrale Saint Corentin (Saint Corentin) in Quimper, Brittany.

TEC4634661: Cathedrale Saint Corentin (Saint Corentin) in Quimper, Brittany. / Bridgeman Images

ID: TEC4634661

Cathedrale Saint Corentin (Saint Corentin) in Quimper, Brittany.

The Infinite Universe - Artist's view
The Infinite Universe - Artist's view

PIX4634691: The Infinite Universe - Artist's view / Bridgeman Images

ID: PIX4634691

The Infinite Universe - Artist's view

Uranus - true and false colors - Voyager 2 - Uranus in true and false colors - Images obtained by the Voyager 2 probe on January 17, 1986 at 9.1 million km from Uranus. On the left image in real colors, the blue color is due to the presence of methane in the atmosphere of the planet; on the right, the false colours show a thick layer of fog around the south pole. The axis of rotation of the planet is different from that of all other planets in the solar system. While for most planets this axis is almost vertical, for Uranus it is almost lying on the plane of its orbit. These two pictures of Uranus - - one in true color (left) and the other in false color - - were compiled from images returned Jan. 17, 1986, by the narrow - angle camera of Voyager 2. The spacecraft was 9.1 million kilometers (5.7 million miles) from the planet, several days from closest approach. The picture at left has been processed to show Uranus as human eyes would see it from the vantage point of the spacecraft. The picture is a composite of images taken through blue, green and orange filters. The darker shadings at the upper right of the disk correspond to the day - night boundary on the planet. Beyond this boundary lies the hidden northern hemisphere of Uranus, which currently remains in total darkness as the planet rotates. The blue - green color results from the absorption of red light by methane gas in Uranus' deep, cold and remarkably clear atmosphere. The picture at right uses false color and extreme contrast enhancement to bring out subtle details in the polar region of Uranus. Images obtained through ultraviolet, violet and orange filters were respectively converted to the same blue, green and red colors used to produce the picture at left
Uranus - true and false colors - Voyager 2 - Uranus in true and false colors - Images obtained by the Voyager 2 probe on January 17, 1986 at 9.1 million km from Uranus. On the left image in real colors, the blue color is due to the presence of methane in the atmosphere of the planet; on the right, the false colours show a thick layer of fog around the south pole. The axis of rotation of the planet is different from that of all other planets in the solar system. While for most planets this axis is almost vertical, for Uranus it is almost lying on the plane of its orbit. These two pictures of Uranus - - one in true color (left) and the other in false color - - were compiled from images returned Jan. 17, 1986, by the narrow - angle camera of Voyager 2. The spacecraft was 9.1 million kilometers (5.7 million miles) from the planet, several days from closest approach. The picture at left has been processed to show Uranus as human eyes would see it from the vantage point of the spacecraft. The picture is a composite of images taken through blue, green and orange filters. The darker shadings at the upper right of the disk correspond to the day - night boundary on the planet. Beyond this boundary lies the hidden northern hemisphere of Uranus, which currently remains in total darkness as the planet rotates. The blue - green color results from the absorption of red light by methane gas in Uranus' deep, cold and remarkably clear atmosphere. The picture at right uses false color and extreme contrast enhancement to bring out subtle details in the polar region of Uranus. Images obtained through ultraviolet, violet and orange filters were respectively converted to the same blue, green and red colors used to produce the picture at left

PIX4634727: Uranus - true and false colors - Voyager 2 - Uranus in true and false colors - Images obtained by the Voyager 2 probe on January 17, 1986 at 9.1 million km from Uranus. On the left image in real colors, the blue color is due to the presence of methane in the atmosphere of the planet; on the right, the false colours show a thick layer of fog around the south pole. The axis of rotation of the planet is different from that of all other planets in the solar system. While for most planets this axis is almost vertical, for Uranus it is almost lying on the plane of its orbit. These two pictures of Uranus - - one in true color (left) and the other in false color - - were compiled from images returned Jan. 17, 1986, by the narrow - angle camera of Voyager 2. The spacecraft was 9.1 million kilometers (5.7 million miles) from the planet, several days from closest approach. The picture at left has been processed to show Uranus as human eyes would see it from the vantage point of the spacecraft. The picture is a composite of images taken through blue, green and orange filters. The darker shadings at the upper right of the disk correspond to the day - night boundary on the planet. Beyond this boundary lies the hidden northern hemisphere of Uranus, which currently remains in total darkness as the planet rotates. The blue - green color results from the absorption of red light by methane gas in Uranus' deep, cold and remarkably clear atmosphere. The picture at right uses false color and extreme contrast enhancement to bring out subtle details in the polar region of Uranus. Images obtained through ultraviolet, violet and orange filters were respectively converted to the same blue, green and red colors used to produce the picture at left / Bridgeman Images

ID: PIX4634727

Uranus - true and false colors - Voyager 2 - Uranus in true and false colors - Images obtained by the Voyager 2 probe on January 17, 1986 at 9.1 million km from Uranus. On the left image in real colors, the blue color is due to the presence of methane in the atmosphere of the planet; on the right, the false colours show a thick layer of fog around the south pole. The axis of rotation of the planet is different from that of all other planets in the solar system. While for most planets this axis is almost vertical, for Uranus it is almost lying on the plane of its orbit. These two pictures of Uranus - - one in true color (left) and the other in false color - - were compiled from images returned Jan. 17, 1986, by the narrow - angle camera of Voyager 2. The spacecraft was 9.1 million kilometers (5.7 million miles) from the planet, several days from closest approach. The picture at left has been processed to show Uranus as human eyes would see it from the vantage point of the spacecraft. Th

The city of Algiers Algiers - Algeria -
The city of Algiers Algiers - Algeria -

TEC4634760: The city of Algiers Algiers - Algeria - / Bridgeman Images

ID: TEC4634760

The city of Algiers Algiers - Algeria -

The city of Algiers Algiers - Algeria -
The city of Algiers Algiers - Algeria -

TEC4634798: The city of Algiers Algiers - Algeria - / Bridgeman Images

ID: TEC4634798

The city of Algiers Algiers - Algeria -

Venus Crescent - Crescent Venus - The planet Venus in crescent seen in broad daylight March 31, 2009. Crescent Venus shimmers in the daytime afternoon sky due to poor seeing conditions. This image was taken on March 31, 2009 just 4 days after inferior conjunction. The planet was at magnitude, - 4.1, and subtended an angle of 58.7 arc seconds, with a phase of 0.014, at an elongation of 9.9 degrees from the Sun
Venus Crescent - Crescent Venus - The planet Venus in crescent seen in broad daylight March 31, 2009. Crescent Venus shimmers in the daytime afternoon sky due to poor seeing conditions. This image was taken on March 31, 2009 just 4 days after inferior conjunction. The planet was at magnitude, - 4.1, and subtended an angle of 58.7 arc seconds, with a phase of 0.014, at an elongation of 9.9 degrees from the Sun

PIX4634838: Venus Crescent - Crescent Venus - The planet Venus in crescent seen in broad daylight March 31, 2009. Crescent Venus shimmers in the daytime afternoon sky due to poor seeing conditions. This image was taken on March 31, 2009 just 4 days after inferior conjunction. The planet was at magnitude, - 4.1, and subtended an angle of 58.7 arc seconds, with a phase of 0.014, at an elongation of 9.9 degrees from the Sun / Bridgeman Images

ID: PIX4634838

Venus Crescent - Crescent Venus - The planet Venus in crescent seen in broad daylight March 31, 2009. Crescent Venus shimmers in the daytime afternoon sky due to poor seeing conditions. This image was taken on March 31, 2009 just 4 days after inferior conjunction. The planet was at magnitude, - 4.1, and subtended an angle of 58.7 arc seconds, with a phase of 0.014, at an elongation of 9.9 degrees from the Sun

Representation of St. Paul ( Relief)
Representation of St. Paul ( Relief)

LRI4635119: Representation of St. Paul ( Relief) / Bridgeman Images

ID: LRI4635119

Representation of St. Paul ( Relief)

Image based on radar images obtained by the Magellan probe - The left edge of the image is at 52.5 degrees east longitude, the right edge at 67.5 degrees east longitude. The top and bottom of the image are at 90 degrees north latitude and 90 degrees south latitude, respectively. Magellan synthetic aperture radar mosaics from the first cycle of Magellan mapping are mapped onto a rectangular latitude-longitude grid to create this image. Data gaps are filled with Pioneer Venus Orbiter altimetric data, or a constant mid-range value. Simulated color is used to enhance small-scale structure. The simulated hues are based on color images recorded by the Soviet Venera 13 and 14 spacecraft -: Venus Surface Map - Cylindrical map of the surface of Venus
Image based on radar images obtained by the Magellan probe - The left edge of the image is at 52.5 degrees east longitude, the right edge at 67.5 degrees east longitude. The top and bottom of the image are at 90 degrees north latitude and 90 degrees south latitude, respectively. Magellan synthetic aperture radar mosaics from the first cycle of Magellan mapping are mapped onto a rectangular latitude-longitude grid to create this image. Data gaps are filled with Pioneer Venus Orbiter altimetric data, or a constant mid-range value. Simulated color is used to enhance small-scale structure. The simulated hues are based on color images recorded by the Soviet Venera 13 and 14 spacecraft -: Venus Surface Map - Cylindrical map of the surface of Venus

PIX4635162: Image based on radar images obtained by the Magellan probe - The left edge of the image is at 52.5 degrees east longitude, the right edge at 67.5 degrees east longitude. The top and bottom of the image are at 90 degrees north latitude and 90 degrees south latitude, respectively. Magellan synthetic aperture radar mosaics from the first cycle of Magellan mapping are mapped onto a rectangular latitude-longitude grid to create this image. Data gaps are filled with Pioneer Venus Orbiter altimetric data, or a constant mid-range value. Simulated color is used to enhance small-scale structure. The simulated hues are based on color images recorded by the Soviet Venera 13 and 14 spacecraft -: Venus Surface Map - Cylindrical map of the surface of Venus / Bridgeman Images

ID: PIX4635162

Image based on radar images obtained by the Magellan probe - The left edge of the image is at 52.5 degrees east longitude, the right edge at 67.5 degrees east longitude. The top and bottom of the image are at 90 degrees north latitude and 90 degrees south latitude, respectively. Magellan synthetic aperture radar mosaics from the first cycle of Magellan mapping are mapped onto a rectangular latitude-longitude grid to create this image. Data gaps are filled with Pioneer Venus Orbiter altimetric data, or a constant mid-range value. Simulated color is used to enhance small-scale structure. The simulated hues are based on color images recorded by the Soviet Venera 13 and 14 spacecraft -: Venus Surface Map - Cylindrical map of the surface of Venus

Venus: volcanic domes in Alpha Regio seen by the Magellan probe - lava domes with a diameter of about 25 km from a few hundred meters of altitude. View obtained by the Magellan probe and processed by computer to generate a 3-dimensional view. The relief is exaggerated
Venus: volcanic domes in Alpha Regio seen by the Magellan probe - lava domes with a diameter of about 25 km from a few hundred meters of altitude. View obtained by the Magellan probe and processed by computer to generate a 3-dimensional view. The relief is exaggerated

PIX4635222: Venus: volcanic domes in Alpha Regio seen by the Magellan probe - lava domes with a diameter of about 25 km from a few hundred meters of altitude. View obtained by the Magellan probe and processed by computer to generate a 3-dimensional view. The relief is exaggerated / Bridgeman Images

ID: PIX4635222

Venus: volcanic domes in Alpha Regio seen by the Magellan probe - lava domes with a diameter of about 25 km from a few hundred meters of altitude. View obtained by the Magellan probe and processed by computer to generate a 3-dimensional view. The relief is exaggerated

Mars - Cerberus - Mosaic of 104 images obtained by the Viking probe 1. The image is deformed by a fish-eye effect. You can see a dark region on the left: Cerberus. Inside it there are major flaws. To the north of Cerberus is Elysium Mons
Mars - Cerberus - Mosaic of 104 images obtained by the Viking probe 1. The image is deformed by a fish-eye effect. You can see a dark region on the left: Cerberus. Inside it there are major flaws. To the north of Cerberus is Elysium Mons

PIX4615170: Mars - Cerberus - Mosaic of 104 images obtained by the Viking probe 1. The image is deformed by a fish-eye effect. You can see a dark region on the left: Cerberus. Inside it there are major flaws. To the north of Cerberus is Elysium Mons / Bridgeman Images

ID: PIX4615170

Mars - Cerberus - Mosaic of 104 images obtained by the Viking probe 1. The image is deformed by a fish-eye effect. You can see a dark region on the left: Cerberus. Inside it there are major flaws. To the north of Cerberus is Elysium Mons

Mars - Dust Tempete - These two images show the same view of Mars before and during a dust storm. Images obtained by the Mars Global Surveyor probe on 10 June 2001 on the left and on 31 July 2001 on the right
Mars - Dust Tempete - These two images show the same view of Mars before and during a dust storm. Images obtained by the Mars Global Surveyor probe on 10 June 2001 on the left and on 31 July 2001 on the right

PIX4615244: Mars - Dust Tempete - These two images show the same view of Mars before and during a dust storm. Images obtained by the Mars Global Surveyor probe on 10 June 2001 on the left and on 31 July 2001 on the right / Bridgeman Images

ID: PIX4615244

Mars - Dust Tempete - These two images show the same view of Mars before and during a dust storm. Images obtained by the Mars Global Surveyor probe on 10 June 2001 on the left and on 31 July 2001 on the right

Image made from altimetric data obtained by the Mars Global Surveyor probe. The northern polar cap is mostly made up of water ice. It measures about 1100 km - Altimetric image of north pole made from MOLA instrument observations on the Mars Global Surveyor spacecraft. This image is colored according to the relative height of the surface features: North Mars pole seen by Mars Global Surveyor - Mars north pole
Image made from altimetric data obtained by the Mars Global Surveyor probe. The northern polar cap is mostly made up of water ice. It measures about 1100 km - Altimetric image of north pole made from MOLA instrument observations on the Mars Global Surveyor spacecraft. This image is colored according to the relative height of the surface features: North Mars pole seen by Mars Global Surveyor - Mars north pole

PIX4615388: Image made from altimetric data obtained by the Mars Global Surveyor probe. The northern polar cap is mostly made up of water ice. It measures about 1100 km - Altimetric image of north pole made from MOLA instrument observations on the Mars Global Surveyor spacecraft. This image is colored according to the relative height of the surface features: North Mars pole seen by Mars Global Surveyor - Mars north pole / Bridgeman Images

ID: PIX4615388

Image made from altimetric data obtained by the Mars Global Surveyor probe. The northern polar cap is mostly made up of water ice. It measures about 1100 km - Altimetric image of north pole made from MOLA instrument observations on the Mars Global Surveyor spacecraft. This image is colored according to the relative height of the surface features: North Mars pole seen by Mars Global Surveyor - Mars north pole

The Canal Saint Martin in Paris 10th. Inaugurated in 1825, the Saint-Martinae Canal connects the Villette basin to the Seine. It has 9 locks and 2 turntables. Photography 2005.
The Canal Saint Martin in Paris 10th. Inaugurated in 1825, the Saint-Martinae Canal connects the Villette basin to the Seine. It has 9 locks and 2 turntables. Photography 2005.

TEC4615495: The Canal Saint Martin in Paris 10th. Inaugurated in 1825, the Saint-Martinae Canal connects the Villette basin to the Seine. It has 9 locks and 2 turntables. Photography 2005. / Bridgeman Images

ID: TEC4615495

The Canal Saint Martin in Paris 10th. Inaugurated in 1825, the Saint-Martinae Canal connects the Villette basin to the Seine. It has 9 locks and 2 turntables. Photography 2005.

Canal Saint Martin, Paris 10th. Inaugurated in 1825, the cananl connects the basin of the Villette to the Seine. It has 9 locks and 2 turntables. Photography 2005.
Canal Saint Martin, Paris 10th. Inaugurated in 1825, the cananl connects the basin of the Villette to the Seine. It has 9 locks and 2 turntables. Photography 2005.

TEC4615614: Canal Saint Martin, Paris 10th. Inaugurated in 1825, the cananl connects the basin of the Villette to the Seine. It has 9 locks and 2 turntables. Photography 2005. / Bridgeman Images

ID: TEC4615614

Canal Saint Martin, Paris 10th. Inaugurated in 1825, the cananl connects the basin of the Villette to the Seine. It has 9 locks and 2 turntables. Photography 2005.

March - Spirit - View from the top of Husband Hill - Panorama of 360 degrees obtained by Spirit from 24 to 27 August 2005. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. Mosaic of 653 images
March - Spirit - View from the top of Husband Hill - Panorama of 360 degrees obtained by Spirit from 24 to 27 August 2005. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. Mosaic of 653 images

PIX4615688: March - Spirit - View from the top of Husband Hill - Panorama of 360 degrees obtained by Spirit from 24 to 27 August 2005. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. Mosaic of 653 images / Bridgeman Images

ID: PIX4615688

March - Spirit - View from the top of Husband Hill - Panorama of 360 degrees obtained by Spirit from 24 to 27 August 2005. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. Mosaic of 653 images

Residential buildings in the 1st arrondissement of Paris. Photography 18/07/09.
Residential buildings in the 1st arrondissement of Paris. Photography 18/07/09.

LBY4593737: Residential buildings in the 1st arrondissement of Paris. Photography 18/07/09. / Bridgeman Images

ID: LBY4593737

Residential buildings in the 1st arrondissement of Paris. Photography 18/07/09.

Constellations of Sagittarius, Scorpio and Jupiter - Sagittarius and Scorpius constellations with Jupiter - Jupiter (the brightest point on the image) in the constellation of Scorpio, on the left, Sagittarius, July 5, 2007, Beg Meil (Finistere - France). In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. Jupiter (brightest spot in the image) in Scorpius constellation and clouds above the sea. Mythological Constellations forms from “” Uranographia”” star atlas by Hevelius (1690) have been added. July 5 2007, Beg Meil (Finistere - France)
Constellations of Sagittarius, Scorpio and Jupiter - Sagittarius and Scorpius constellations with Jupiter - Jupiter (the brightest point on the image) in the constellation of Scorpio, on the left, Sagittarius, July 5, 2007, Beg Meil (Finistere - France). In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. Jupiter (brightest spot in the image) in Scorpius constellation and clouds above the sea. Mythological Constellations forms from “” Uranographia”” star atlas by Hevelius (1690) have been added. July 5 2007, Beg Meil (Finistere - France)

PIX4593796: Constellations of Sagittarius, Scorpio and Jupiter - Sagittarius and Scorpius constellations with Jupiter - Jupiter (the brightest point on the image) in the constellation of Scorpio, on the left, Sagittarius, July 5, 2007, Beg Meil (Finistere - France). In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. Jupiter (brightest spot in the image) in Scorpius constellation and clouds above the sea. Mythological Constellations forms from “” Uranographia”” star atlas by Hevelius (1690) have been added. July 5 2007, Beg Meil (Finistere - France) / Bridgeman Images

ID: PIX4593796

Constellations of Sagittarius, Scorpio and Jupiter - Sagittarius and Scorpius constellations with Jupiter - Jupiter (the brightest point on the image) in the constellation of Scorpio, on the left, Sagittarius, July 5, 2007, Beg Meil (Finistere - France). In overprint, the mythological forms of these constellations, extracted from the Uranographia of Hevelius. Jupiter (brightest spot in the image) in Scorpius constellation and clouds above the sea. Mythological Constellations forms from “” Uranographia”” star atlas by Hevelius (1690) have been added. July 5 2007, Beg Meil (Finistere - France)

Constellations of Serpens and Ophiuchus - Constellations of Serpens and Ophiuchus - The constellation of Ophiuchus separates the constellation of the Serpent into two parts. Serpens, the Serpent, is an ancient constellation, unique in being formed from two separate sections, Serpens Caput (the head of the snake) to the west and Serpens Cauda (the tail) to the east. Between them lies the constellation of Ophiuchus, the serpent holder, who is usually identified with the ancient Greek physician Asclepius, around whose shoulders or staff a snake is draped. The stars in both parts of Serpens are mostly quite faint and a snake - like shape is hard to pick out in either section. Serpens Cauda is probably easier to locate since it occupies the dusty part of the Milky Way adjoining the brighter star clouds of Scutum and Aquila
Constellations of Serpens and Ophiuchus - Constellations of Serpens and Ophiuchus - The constellation of Ophiuchus separates the constellation of the Serpent into two parts. Serpens, the Serpent, is an ancient constellation, unique in being formed from two separate sections, Serpens Caput (the head of the snake) to the west and Serpens Cauda (the tail) to the east. Between them lies the constellation of Ophiuchus, the serpent holder, who is usually identified with the ancient Greek physician Asclepius, around whose shoulders or staff a snake is draped. The stars in both parts of Serpens are mostly quite faint and a snake - like shape is hard to pick out in either section. Serpens Cauda is probably easier to locate since it occupies the dusty part of the Milky Way adjoining the brighter star clouds of Scutum and Aquila

PIX4594003: Constellations of Serpens and Ophiuchus - Constellations of Serpens and Ophiuchus - The constellation of Ophiuchus separates the constellation of the Serpent into two parts. Serpens, the Serpent, is an ancient constellation, unique in being formed from two separate sections, Serpens Caput (the head of the snake) to the west and Serpens Cauda (the tail) to the east. Between them lies the constellation of Ophiuchus, the serpent holder, who is usually identified with the ancient Greek physician Asclepius, around whose shoulders or staff a snake is draped. The stars in both parts of Serpens are mostly quite faint and a snake - like shape is hard to pick out in either section. Serpens Cauda is probably easier to locate since it occupies the dusty part of the Milky Way adjoining the brighter star clouds of Scutum and Aquila / Bridgeman Images

ID: PIX4594003

Constellations of Serpens and Ophiuchus - Constellations of Serpens and Ophiuchus - The constellation of Ophiuchus separates the constellation of the Serpent into two parts. Serpens, the Serpent, is an ancient constellation, unique in being formed from two separate sections, Serpens Caput (the head of the snake) to the west and Serpens Cauda (the tail) to the east. Between them lies the constellation of Ophiuchus, the serpent holder, who is usually identified with the ancient Greek physician Asclepius, around whose shoulders or staff a snake is draped. The stars in both parts of Serpens are mostly quite faint and a snake - like shape is hard to pick out in either section. Serpens Cauda is probably easier to locate since it occupies the dusty part of the Milky Way adjoining the brighter star clouds of Scutum and Aquila

Constellation of Taurus - Constellation of Taurus - On the right of the image, nebula NGC 1499, on the top, nebulae IC 1805 and IC 1848
Constellation of Taurus - Constellation of Taurus - On the right of the image, nebula NGC 1499, on the top, nebulae IC 1805 and IC 1848

PIX4594054: Constellation of Taurus - Constellation of Taurus - On the right of the image, nebula NGC 1499, on the top, nebulae IC 1805 and IC 1848 / Bridgeman Images

ID: PIX4594054

Constellation of Taurus - Constellation of Taurus - On the right of the image, nebula NGC 1499, on the top, nebulae IC 1805 and IC 1848

Square Leopold Achilles in Paris.
Square Leopold Achilles in Paris.

TEC4594100: Square Leopold Achilles in Paris. / Bridgeman Images

ID: TEC4594100

Square Leopold Achilles in Paris.

A Parisian kiosk, rue Rambuteau, Paris 3rd arrondissement.
A Parisian kiosk, rue Rambuteau, Paris 3rd arrondissement.

TEC4594161: A Parisian kiosk, rue Rambuteau, Paris 3rd arrondissement. / Bridgeman Images

ID: TEC4594161

A Parisian kiosk, rue Rambuteau, Paris 3rd arrondissement.

Constellations of the Telescopium and Sagittarius - The Telescope is a small constellation of the southern hemisphere located just above Sagittarius
Constellations of the Telescopium and Sagittarius - The Telescope is a small constellation of the southern hemisphere located just above Sagittarius

PIX4594195: Constellations of the Telescopium and Sagittarius - The Telescope is a small constellation of the southern hemisphere located just above Sagittarius / Bridgeman Images

ID: PIX4594195

Constellations of the Telescopium and Sagittarius - The Telescope is a small constellation of the southern hemisphere located just above Sagittarius

Une station de velib, rue Rambuteau, Paris 3rd arrondissement.
Une station de velib, rue Rambuteau, Paris 3rd arrondissement.

TEC4594234: Une station de velib, rue Rambuteau, Paris 3rd arrondissement. / Bridgeman Images

ID: TEC4594234

Une station de velib, rue Rambuteau, Paris 3rd arrondissement.

Constellation of the Southern Triangle - Constellation of Triangulum Austral
Constellation of the Southern Triangle - Constellation of Triangulum Austral

PIX4594270: Constellation of the Southern Triangle - Constellation of Triangulum Austral / Bridgeman Images

ID: PIX4594270

Constellation of the Southern Triangle - Constellation of Triangulum Austral

Constellations of the Virgin, the Raven and the Cup - Constellations of Virgo, Corvus and Crate
Constellations of the Virgin, the Raven and the Cup - Constellations of Virgo, Corvus and Crate

PIX4594435: Constellations of the Virgin, the Raven and the Cup - Constellations of Virgo, Corvus and Crate / Bridgeman Images

ID: PIX4594435

Constellations of the Virgin, the Raven and the Cup - Constellations of Virgo, Corvus and Crate

Constellation of the Virgin - Constellation of Virgo - The constellation of the Virgin with its mythological form extracted from the Uranographia of Hevelius. Map showing the constellation of Virgo with its mythological form from “” Uranographia”” star atlas by Hevelius (1690) added
Constellation of the Virgin - Constellation of Virgo - The constellation of the Virgin with its mythological form extracted from the Uranographia of Hevelius. Map showing the constellation of Virgo with its mythological form from “” Uranographia”” star atlas by Hevelius (1690) added

PIX4594494: Constellation of the Virgin - Constellation of Virgo - The constellation of the Virgin with its mythological form extracted from the Uranographia of Hevelius. Map showing the constellation of Virgo with its mythological form from “” Uranographia”” star atlas by Hevelius (1690) added / Bridgeman Images

ID: PIX4594494

Constellation of the Virgin - Constellation of Virgo - The constellation of the Virgin with its mythological form extracted from the Uranographia of Hevelius. Map showing the constellation of Virgo with its mythological form from “” Uranographia”” star atlas by Hevelius (1690) added


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