1. Home
  2. Search Results

Print Friendly Version Page

Print this page or go back to standard view.

2501742 Search Results

Martian panorama taken by the rover Opportunity - Martian panorama seen from rover Opportunity - 360 degres panorama obtained by the rover Opportunity from the position where the rover remained for five weeks in November and December 2008. The 276 images that make up this panorama were taken from November 21 to 24, 2008. In this image the rover, whose top of its antenna can be seen in the center of the image, is located about 1 km southwest of the Victoria crater. Opportunity returned to Endeavour crater on December 23, 2008. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows the vista from the location where Nasa's Mars Exploration Rover Opportunity spent five weeks in November and December 2008 while the sun was almost directly in between Mars and Earth, limiting communications. Opportunity is approaching the fifth Earth - year anniversary of its landing on Mars, continuing a surface mission that was initially scheduled to last three months. The rover landed on Jan. 24, 2004 (Pacific Standard Time; Jan. 25, 2004 Universal Time). When it reached the location from which its panoramic camera (Pancam) captured this view, it had driven a total of 13,616 meters (8.46 miles) since its landing. The view combines 276 different exposures taken with Opportunity's panoramic camera (Pancam) - - 92 pointings, with three filters at each pointing. The component images were taken during the period from the rover's 1,716th Martian day, or sol, to the mission's Sol 1719 (Nov. 21 to 24, 2008). Opportunity has driven 1.83 kilometers (1.14 miles) since it exited Victoria Crater on Sol 1634 (Aug. 28, 2008). It skirted the west rim of Victoria and, at the point from which this panorama was taken, had reached a position about a kilometer (six - tenths of a mile) southwest of the south rim of the crater. North is in the center of the panorama. Rover tracks are visible from the drive to th
Martian panorama taken by the rover Opportunity - Martian panorama seen from rover Opportunity - 360 degres panorama obtained by the rover Opportunity from the position where the rover remained for five weeks in November and December 2008. The 276 images that make up this panorama were taken from November 21 to 24, 2008. In this image the rover, whose top of its antenna can be seen in the center of the image, is located about 1 km southwest of the Victoria crater. Opportunity returned to Endeavour crater on December 23, 2008. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows the vista from the location where Nasa's Mars Exploration Rover Opportunity spent five weeks in November and December 2008 while the sun was almost directly in between Mars and Earth, limiting communications. Opportunity is approaching the fifth Earth - year anniversary of its landing on Mars, continuing a surface mission that was initially scheduled to last three months. The rover landed on Jan. 24, 2004 (Pacific Standard Time; Jan. 25, 2004 Universal Time). When it reached the location from which its panoramic camera (Pancam) captured this view, it had driven a total of 13,616 meters (8.46 miles) since its landing. The view combines 276 different exposures taken with Opportunity's panoramic camera (Pancam) - - 92 pointings, with three filters at each pointing. The component images were taken during the period from the rover's 1,716th Martian day, or sol, to the mission's Sol 1719 (Nov. 21 to 24, 2008). Opportunity has driven 1.83 kilometers (1.14 miles) since it exited Victoria Crater on Sol 1634 (Aug. 28, 2008). It skirted the west rim of Victoria and, at the point from which this panorama was taken, had reached a position about a kilometer (six - tenths of a mile) southwest of the south rim of the crater. North is in the center of the panorama. Rover tracks are visible from the drive to th

PIX4615883: Martian panorama taken by the rover Opportunity - Martian panorama seen from rover Opportunity - 360 degres panorama obtained by the rover Opportunity from the position where the rover remained for five weeks in November and December 2008. The 276 images that make up this panorama were taken from November 21 to 24, 2008. In this image the rover, whose top of its antenna can be seen in the center of the image, is located about 1 km southwest of the Victoria crater. Opportunity returned to Endeavour crater on December 23, 2008. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows the vista from the location where Nasa's Mars Exploration Rover Opportunity spent five weeks in November and December 2008 while the sun was almost directly in between Mars and Earth, limiting communications. Opportunity is approaching the fifth Earth - year anniversary of its landing on Mars, continuing a surface mission that was initially scheduled to last three months. The rover landed on Jan. 24, 2004 (Pacific Standard Time; Jan. 25, 2004 Universal Time). When it reached the location from which its panoramic camera (Pancam) captured this view, it had driven a total of 13,616 meters (8.46 miles) since its landing. The view combines 276 different exposures taken with Opportunity's panoramic camera (Pancam) - - 92 pointings, with three filters at each pointing. The component images were taken during the period from the rover's 1,716th Martian day, or sol, to the mission's Sol 1719 (Nov. 21 to 24, 2008). Opportunity has driven 1.83 kilometers (1.14 miles) since it exited Victoria Crater on Sol 1634 (Aug. 28, 2008). It skirted the west rim of Victoria and, at the point from which this panorama was taken, had reached a position about a kilometer (six - tenths of a mile) southwest of the south rim of the crater. North is in the center of the panorama. Rover tracks are visible from the drive to th / Bridgeman Images

ID: PIX4615883

Martian panorama taken by the rover Opportunity - Martian panorama seen from rover Opportunity - 360 degres panorama obtained by the rover Opportunity from the position where the rover remained for five weeks in November and December 2008. The 276 images that make up this panorama were taken from November 21 to 24, 2008. In this image the rover, whose top of its antenna can be seen in the center of the image, is located about 1 km southwest of the Victoria crater. Opportunity returned to Endeavour crater on December 23, 2008. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows the vista from the location where Nasa's Mars Exploration Rover Opportunity spent five weeks in November and December 2008 while the sun was almost directly in between Mars and Earth, limiting communications. Opportunity is approaching the fifth Earth - year anniversary of its landing on Mars, continuing a surface mission that was initially sch

Paris. Photography 25/08/07.
Paris. Photography 25/08/07.

TEC4615886: Paris. Photography 25/08/07. / Bridgeman Images

ID: TEC4615886

Paris. Photography 25/08/07.

March: Faults and impact crater in Acheron Fossae. - Fracture system around a 55 km diametre and 2000m deep impact crater. Image obtained by the Mars Express probe in 2004
March: Faults and impact crater in Acheron Fossae. - Fracture system around a 55 km diametre and 2000m deep impact crater. Image obtained by the Mars Express probe in 2004

PIX4615921: March: Faults and impact crater in Acheron Fossae. - Fracture system around a 55 km diametre and 2000m deep impact crater. Image obtained by the Mars Express probe in 2004 / Bridgeman Images

ID: PIX4615921

March: Faults and impact crater in Acheron Fossae. - Fracture system around a 55 km diametre and 2000m deep impact crater. Image obtained by the Mars Express probe in 2004

Traces of the passage of water on Mars - Ancient river beds on Mars. Observation of sedimentary rocks shows that water is in the liquid state to dig these furrows. Region of 14 km by 19 km Mosaic of images obtained by the Mars Global Surveyor probe between August 2000 and September 2003
Traces of the passage of water on Mars - Ancient river beds on Mars. Observation of sedimentary rocks shows that water is in the liquid state to dig these furrows. Region of 14 km by 19 km Mosaic of images obtained by the Mars Global Surveyor probe between August 2000 and September 2003

PIX4615391: Traces of the passage of water on Mars - Ancient river beds on Mars. Observation of sedimentary rocks shows that water is in the liquid state to dig these furrows. Region of 14 km by 19 km Mosaic of images obtained by the Mars Global Surveyor probe between August 2000 and September 2003 / Bridgeman Images

ID: PIX4615391

Traces of the passage of water on Mars - Ancient river beds on Mars. Observation of sedimentary rocks shows that water is in the liquid state to dig these furrows. Region of 14 km by 19 km Mosaic of images obtained by the Mars Global Surveyor probe between August 2000 and September 2003

Peniche on the Canal Saint Martin in Paris 10th.
Peniche on the Canal Saint Martin in Paris 10th.

TEC4615405: Peniche on the Canal Saint Martin in Paris 10th. / Bridgeman Images

ID: TEC4615405

Peniche on the Canal Saint Martin in Paris 10th.

Boulevard de Srtasbourg overlooking the Cafe de France with the Gare de l'Est in Paris 10th.
Boulevard de Srtasbourg overlooking the Cafe de France with the Gare de l'Est in Paris 10th.

TEC4615441: Boulevard de Srtasbourg overlooking the Cafe de France with the Gare de l'Est in Paris 10th. / Bridgeman Images

ID: TEC4615441

Boulevard de Srtasbourg overlooking the Cafe de France with the Gare de l'Est in Paris 10th.

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.

TEC4615473: 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: TEC4615473

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.
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.

TEC4615479: 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: TEC4615479

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.

Quai de Valmy in Paris 10th.
Quai de Valmy in Paris 10th.

TEC4615517: Quai de Valmy in Paris 10th. / Bridgeman Images

ID: TEC4615517

Quai de Valmy in Paris 10th.

Convent of Recollets, 150-154 rue du Faubourg Saint Martin, Paris 10th. Built in 1604, the convent was abandoned for many years. Rehabilitates an international reception centre for artists, researchers, intellectuals and academics since 2004. There are eighty one furniture dwellings and workshops dwellings available to them. The Centre also houses the Maison de l'Architecture of France and a cultural animation association. Photography 2005.
Convent of Recollets, 150-154 rue du Faubourg Saint Martin, Paris 10th. Built in 1604, the convent was abandoned for many years. Rehabilitates an international reception centre for artists, researchers, intellectuals and academics since 2004. There are eighty one furniture dwellings and workshops dwellings available to them. The Centre also houses the Maison de l'Architecture of France and a cultural animation association. Photography 2005.

TEC4615550: Convent of Recollets, 150-154 rue du Faubourg Saint Martin, Paris 10th. Built in 1604, the convent was abandoned for many years. Rehabilitates an international reception centre for artists, researchers, intellectuals and academics since 2004. There are eighty one furniture dwellings and workshops dwellings available to them. The Centre also houses the Maison de l'Architecture of France and a cultural animation association. Photography 2005. / Bridgeman Images

ID: TEC4615550

Convent of Recollets, 150-154 rue du Faubourg Saint Martin, Paris 10th. Built in 1604, the convent was abandoned for many years. Rehabilitates an international reception centre for artists, researchers, intellectuals and academics since 2004. There are eighty one furniture dwellings and workshops dwellings available to them. The Centre also houses the Maison de l'Architecture of France and a cultural animation association. Photography 2005.

March: Columbia memorial station - Columbia memorial station, the landing base of the rover Spirit, photographed by the rover during his 16th Martian day (18 - 19 January 2004). The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004
March: Columbia memorial station - Columbia memorial station, the landing base of the rover Spirit, photographed by the rover during his 16th Martian day (18 - 19 January 2004). The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

PIX4615559: March: Columbia memorial station - Columbia memorial station, the landing base of the rover Spirit, photographed by the rover during his 16th Martian day (18 - 19 January 2004). The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004 / Bridgeman Images

ID: PIX4615559

March: Columbia memorial station - Columbia memorial station, the landing base of the rover Spirit, photographed by the rover during his 16th Martian day (18 - 19 January 2004). The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

March: Cratere Bonneville seen by Spirit - Panorama of 360 degres obtained by Spirit on 12 and 13 March 2004. Bonneville is an impact crater 200m in diameter. Far on the right, Columbia Hills; near the horizon line in the center of the image, a bright point, the thermal shield of the probe. On the left, the traces left by the rover. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004
March: Cratere Bonneville seen by Spirit - Panorama of 360 degres obtained by Spirit on 12 and 13 March 2004. Bonneville is an impact crater 200m in diameter. Far on the right, Columbia Hills; near the horizon line in the center of the image, a bright point, the thermal shield of the probe. On the left, the traces left by the rover. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

PIX4615587: March: Cratere Bonneville seen by Spirit - Panorama of 360 degres obtained by Spirit on 12 and 13 March 2004. Bonneville is an impact crater 200m in diameter. Far on the right, Columbia Hills; near the horizon line in the center of the image, a bright point, the thermal shield of the probe. On the left, the traces left by the rover. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004 / Bridgeman Images

ID: PIX4615587

March: Cratere Bonneville seen by Spirit - Panorama of 360 degres obtained by Spirit on 12 and 13 March 2004. Bonneville is an impact crater 200m in diameter. Far on the right, Columbia Hills; near the horizon line in the center of the image, a bright point, the thermal shield of the probe. On the left, the traces left by the rover. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

Rover Spirit - Self Portrait - The Rover Spirit used his panoramic camera to take several images and create this mosaic on December 7, 2004. The mat on which the camera is mounted has been erased. This self-portrait shows the accumulation of Martian dust on the rover and its solar panels. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004
Rover Spirit - Self Portrait - The Rover Spirit used his panoramic camera to take several images and create this mosaic on December 7, 2004. The mat on which the camera is mounted has been erased. This self-portrait shows the accumulation of Martian dust on the rover and its solar panels. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

PIX4615651: Rover Spirit - Self Portrait - The Rover Spirit used his panoramic camera to take several images and create this mosaic on December 7, 2004. The mat on which the camera is mounted has been erased. This self-portrait shows the accumulation of Martian dust on the rover and its solar panels. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004 / Bridgeman Images

ID: PIX4615651

Rover Spirit - Self Portrait - The Rover Spirit used his panoramic camera to take several images and create this mosaic on December 7, 2004. The mat on which the camera is mounted has been erased. This self-portrait shows the accumulation of Martian dust on the rover and its solar panels. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

March: Rover Spirit - Self Portrait - The Rover Spirit used his panoramic camera to take several images and create this mosaic on August 27, 2005. This self-portrait shows the accumulation of Martian dust on the rover and its solar panels. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004
March: Rover Spirit - Self Portrait - The Rover Spirit used his panoramic camera to take several images and create this mosaic on August 27, 2005. This self-portrait shows the accumulation of Martian dust on the rover and its solar panels. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

PIX4615673: March: Rover Spirit - Self Portrait - The Rover Spirit used his panoramic camera to take several images and create this mosaic on August 27, 2005. This self-portrait shows the accumulation of Martian dust on the rover and its solar panels. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004 / Bridgeman Images

ID: PIX4615673

March: Rover Spirit - Self Portrait - The Rover Spirit used his panoramic camera to take several images and create this mosaic on August 27, 2005. This self-portrait shows the accumulation of Martian dust on the rover and its solar panels. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004

Cinema Luxor Pathe in Paris 10th. Construction 1920, architect Henri Zipcy, decor of the Amedee Tiberi facade. Photography 1990.
Cinema Luxor Pathe in Paris 10th. Construction 1920, architect Henri Zipcy, decor of the Amedee Tiberi facade. Photography 1990.

MDA4616209: Cinema Luxor Pathe in Paris 10th. Construction 1920, architect Henri Zipcy, decor of the Amedee Tiberi facade. Photography 1990. / Bridgeman Images

ID: MDA4616209

Cinema Luxor Pathe in Paris 10th. Construction 1920, architect Henri Zipcy, decor of the Amedee Tiberi facade. Photography 1990.

Mars - Satellite Phobos - Martian moon Phobos - View of the satellite Phobos obtained by the Mars Express probe on July 23, 2008 at a distance of 97 km from the Martian moon. The resolution is 3.7 meters per pixel. On 23 July 2008, the High Resolution Stereo Camera on board the ESA's Mars Express took the highest - resolution full - disc image yet of the surface of the moon Phobos. The image data was acquired from a distance of 97 km with a spatial resolution of about 3.7 m/pixel in orbit 5851. These images have surpassed all previous images from other missions in continuous coverage of the illuminated surface at the highest spatial resolution of 3.7 m/pixel. This image is photometrically enhanced to bring out the features in the less illuminated part
Mars - Satellite Phobos - Martian moon Phobos - View of the satellite Phobos obtained by the Mars Express probe on July 23, 2008 at a distance of 97 km from the Martian moon. The resolution is 3.7 meters per pixel. On 23 July 2008, the High Resolution Stereo Camera on board the ESA's Mars Express took the highest - resolution full - disc image yet of the surface of the moon Phobos. The image data was acquired from a distance of 97 km with a spatial resolution of about 3.7 m/pixel in orbit 5851. These images have surpassed all previous images from other missions in continuous coverage of the illuminated surface at the highest spatial resolution of 3.7 m/pixel. This image is photometrically enhanced to bring out the features in the less illuminated part

PIX4616278: Mars - Satellite Phobos - Martian moon Phobos - View of the satellite Phobos obtained by the Mars Express probe on July 23, 2008 at a distance of 97 km from the Martian moon. The resolution is 3.7 meters per pixel. On 23 July 2008, the High Resolution Stereo Camera on board the ESA's Mars Express took the highest - resolution full - disc image yet of the surface of the moon Phobos. The image data was acquired from a distance of 97 km with a spatial resolution of about 3.7 m/pixel in orbit 5851. These images have surpassed all previous images from other missions in continuous coverage of the illuminated surface at the highest spatial resolution of 3.7 m/pixel. This image is photometrically enhanced to bring out the features in the less illuminated part / Bridgeman Images

ID: PIX4616278

Mars - Satellite Phobos - Martian moon Phobos - View of the satellite Phobos obtained by the Mars Express probe on July 23, 2008 at a distance of 97 km from the Martian moon. The resolution is 3.7 meters per pixel. On 23 July 2008, the High Resolution Stereo Camera on board the ESA's Mars Express took the highest - resolution full - disc image yet of the surface of the moon Phobos. The image data was acquired from a distance of 97 km with a spatial resolution of about 3.7 m/pixel in orbit 5851. These images have surpassed all previous images from other missions in continuous coverage of the illuminated surface at the highest spatial resolution of 3.7 m/pixel. This image is photometrically enhanced to bring out the features in the less illuminated part

Cycle on the life of Saint Stephen: “” The funeral of Saint Stephen”” (The esequie di santo Stefano) Detail. Fresco by Filippo Lippi (ca. 1406-1469) 1452-1465 Prato, Cattedrale di Santo Stefano (Duomo) Italy - Stories from the Life of St. Stephen. Funeral, by Filippo Lippi (c.1406-1469). Detail. Fresco, 1452-65. Cathedral of Santo Stefano, Prato, Italy
Cycle on the life of Saint Stephen: “” The funeral of Saint Stephen”” (The esequie di santo Stefano) Detail. Fresco by Filippo Lippi (ca. 1406-1469) 1452-1465 Prato, Cattedrale di Santo Stefano (Duomo) Italy - Stories from the Life of St. Stephen. Funeral, by Filippo Lippi (c.1406-1469). Detail. Fresco, 1452-65. Cathedral of Santo Stefano, Prato, Italy

LRI4616050: Cycle on the life of Saint Stephen: “” The funeral of Saint Stephen”” (The esequie di santo Stefano) Detail. Fresco by Filippo Lippi (ca. 1406-1469) 1452-1465 Prato, Cattedrale di Santo Stefano (Duomo) Italy - Stories from the Life of St. Stephen. Funeral, by Filippo Lippi (c.1406-1469). Detail. Fresco, 1452-65. Cathedral of Santo Stefano, Prato, Italy, Lippi, Filippo (c.1406-69) / Bridgeman Images

ID: LRI4616050

Cycle on the life of Saint Stephen: “” The funeral of Saint Stephen”” (The esequie di santo Stefano) Detail. Fresco by Filippo Lippi (ca. 1406-1469) 1452-1465 Prato, Cattedrale di Santo Stefano (Duomo) Italy - Stories from the Life of St. Stephen. Funeral, by Filippo Lippi (c.1406-1469). Detail. Fresco, 1452-65. Cathedral of Santo Stefano, Prato, Italy

Lippi, Filippo (c.1406-69)

March - Spirit - Panorama McMurdo 10 - 2006 - March: McMurdo panorama - Spirit 10 - 2006 - Panorama of 360 degres “” Mac Murdo”” obtained by the Spirit rover from April to October 2006. Spirit stayed in the same place directing its solar panels towards the Sun to recharge its batteries. Many dark, porous volcanic rocks are visible in this image. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. This 360 - degree view, called the “” McMurdo”” panorama, comes from the panoramic camera (Pancam) on Nasa's Mars Exploration Rover Spirit. From April through October 2006, Spirit has stayed on a small hill known as “Low Ridge.”” There, the rover's solar panels are tilted towards the sun to maintain enough solar power for Spirit to keep making scientific observations throughout the winter on southern Mars. This view of the surroundings from Spirit's “” Winter Haven”” is presented in approximately true color. Many dark, porous - textured volcanic rocks can be seen around the rover, including many on Low Ridge. Two rocks to the right of center, brighter and smoother - looking in this image and more reflective in infrared observations by Spirit's miniature thermal emission spectrometer, are thought to be meteorites
March - Spirit - Panorama McMurdo 10 - 2006 - March: McMurdo panorama - Spirit 10 - 2006 - Panorama of 360 degres “” Mac Murdo”” obtained by the Spirit rover from April to October 2006. Spirit stayed in the same place directing its solar panels towards the Sun to recharge its batteries. Many dark, porous volcanic rocks are visible in this image. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. This 360 - degree view, called the “” McMurdo”” panorama, comes from the panoramic camera (Pancam) on Nasa's Mars Exploration Rover Spirit. From April through October 2006, Spirit has stayed on a small hill known as “Low Ridge.”” There, the rover's solar panels are tilted towards the sun to maintain enough solar power for Spirit to keep making scientific observations throughout the winter on southern Mars. This view of the surroundings from Spirit's “” Winter Haven”” is presented in approximately true color. Many dark, porous - textured volcanic rocks can be seen around the rover, including many on Low Ridge. Two rocks to the right of center, brighter and smoother - looking in this image and more reflective in infrared observations by Spirit's miniature thermal emission spectrometer, are thought to be meteorites

PIX4615739: March - Spirit - Panorama McMurdo 10 - 2006 - March: McMurdo panorama - Spirit 10 - 2006 - Panorama of 360 degres “” Mac Murdo”” obtained by the Spirit rover from April to October 2006. Spirit stayed in the same place directing its solar panels towards the Sun to recharge its batteries. Many dark, porous volcanic rocks are visible in this image. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. This 360 - degree view, called the “” McMurdo”” panorama, comes from the panoramic camera (Pancam) on Nasa's Mars Exploration Rover Spirit. From April through October 2006, Spirit has stayed on a small hill known as “Low Ridge.”” There, the rover's solar panels are tilted towards the sun to maintain enough solar power for Spirit to keep making scientific observations throughout the winter on southern Mars. This view of the surroundings from Spirit's “” Winter Haven”” is presented in approximately true color. Many dark, porous - textured volcanic rocks can be seen around the rover, including many on Low Ridge. Two rocks to the right of center, brighter and smoother - looking in this image and more reflective in infrared observations by Spirit's miniature thermal emission spectrometer, are thought to be meteorites / Bridgeman Images

ID: PIX4615739

March - Spirit - Panorama McMurdo 10 - 2006 - March: McMurdo panorama - Spirit 10 - 2006 - Panorama of 360 degres “” Mac Murdo”” obtained by the Spirit rover from April to October 2006. Spirit stayed in the same place directing its solar panels towards the Sun to recharge its batteries. Many dark, porous volcanic rocks are visible in this image. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. This 360 - degree view, called the “” McMurdo”” panorama, comes from the panoramic camera (Pancam) on Nasa's Mars Exploration Rover Spirit. From April through October 2006, Spirit has stayed on a small hill known as “Low Ridge.”” There, the rover's solar panels are tilted towards the sun to maintain enough solar power for Spirit to keep making scientific observations throughout the winter on southern Mars. This view of the surroundings from Spirit's “” Winter Haven”” is presented in approximately true color. Many dark, porous - textured volcanic rocks can be seen around t

Fragrant island (Watercolour, 1929)
Fragrant island (Watercolour, 1929)

LRI4615742: Fragrant island (Watercolour, 1929), Klee, Paul (1879-1940) / Bridgeman Images

ID: LRI4615742

Fragrant island (Watercolour, 1929)

Klee, Paul (1879-1940)

La rue du Buisson Saint Louis in Paris 10th.
La rue du Buisson Saint Louis in Paris 10th.

TEC4615751: La rue du Buisson Saint Louis in Paris 10th. / Bridgeman Images

ID: TEC4615751

La rue du Buisson Saint Louis in Paris 10th.

Le quai de Valmy in Paris 10th.
Le quai de Valmy in Paris 10th.

TEC4615833: Le quai de Valmy in Paris 10th. / Bridgeman Images

ID: TEC4615833

Le quai de Valmy in Paris 10th.

Le quai de Jemmapes in Paris 10th.
Le quai de Jemmapes in Paris 10th.

TEC4615874: Le quai de Jemmapes in Paris 10th. / Bridgeman Images

ID: TEC4615874

Le quai de Jemmapes in Paris 10th.

House in Paris 20th.
House in Paris 20th.

TEC4616406: House in Paris 20th. / Bridgeman Images

ID: TEC4616406

House in Paris 20th.

Church Notre Dame de la Croix, Place Maurice Chevalier in Paris 20th. Architect Louis Antoineæheret, construction 1863-1880. She's in a neo-romanthic Gothic transition style.
Church Notre Dame de la Croix, Place Maurice Chevalier in Paris 20th. Architect Louis Antoineæheret, construction 1863-1880. She's in a neo-romanthic Gothic transition style.

TEC4616433: Church Notre Dame de la Croix, Place Maurice Chevalier in Paris 20th. Architect Louis Antoineæheret, construction 1863-1880. She's in a neo-romanthic Gothic transition style. / Bridgeman Images

ID: TEC4616433

Church Notre Dame de la Croix, Place Maurice Chevalier in Paris 20th. Architect Louis Antoineæheret, construction 1863-1880. She's in a neo-romanthic Gothic transition style.

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

TEC4616490: The cemetery of Pere Lachaise in Paris. The cemetery opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere-Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it counts about 70 000 monuments.ÆPhotograph 06/06/05. / Bridgeman Images

ID: TEC4616490

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

The tomb of Francois-Joseph (Francois Joseph) Talma (1763-1826) at the Pere Lachaise cemetery in Paris 20th. Opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it has nearly 70,000 monuments. Photography 06/06/05.
The tomb of Francois-Joseph (Francois Joseph) Talma (1763-1826) at the Pere Lachaise cemetery in Paris 20th. Opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it has nearly 70,000 monuments. Photography 06/06/05.

TEC4616522: The tomb of Francois-Joseph (Francois Joseph) Talma (1763-1826) at the Pere Lachaise cemetery in Paris 20th. Opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it has nearly 70,000 monuments. Photography 06/06/05. / Bridgeman Images

ID: TEC4616522

The tomb of Francois-Joseph (Francois Joseph) Talma (1763-1826) at the Pere Lachaise cemetery in Paris 20th. Opened around 1804 on a land formerly owned by the Jesuit. The architect Alexandre Theodore Brongniart conceived the plans of 1810. Many artists worked at Pere Lachaise in the first half of the 19th century. With an area of almost 44 hectares, it has nearly 70,000 monuments. Photography 06/06/05.

The eye and the human spirit (oil on canvas, 1930)
The eye and the human spirit (oil on canvas, 1930)

LRI4616590: The eye and the human spirit (oil on canvas, 1930), Martini, Alberto (1876-1954) / Bridgeman Images

ID: LRI4616590

The eye and the human spirit (oil on canvas, 1930)

Martini, Alberto (1876-1954)

A comet seen in the sky of the planet Mars - illustration - Comet Over Candor on Mars - Illustration - A comet passes over Candor Chasma, one of the canyons of Valles Marineris. In the sky, the bright spot is the planet Earth. A comet lights up the Martian predawn over the twisted landscape of Candor Chasma. The distant mountains are several kilometers high. The planet Earth shines as a bright blue star in the sky
A comet seen in the sky of the planet Mars - illustration - Comet Over Candor on Mars - Illustration - A comet passes over Candor Chasma, one of the canyons of Valles Marineris. In the sky, the bright spot is the planet Earth. A comet lights up the Martian predawn over the twisted landscape of Candor Chasma. The distant mountains are several kilometers high. The planet Earth shines as a bright blue star in the sky

PIX4617044: A comet seen in the sky of the planet Mars - illustration - Comet Over Candor on Mars - Illustration - A comet passes over Candor Chasma, one of the canyons of Valles Marineris. In the sky, the bright spot is the planet Earth. A comet lights up the Martian predawn over the twisted landscape of Candor Chasma. The distant mountains are several kilometers high. The planet Earth shines as a bright blue star in the sky / Bridgeman Images

ID: PIX4617044

A comet seen in the sky of the planet Mars - illustration - Comet Over Candor on Mars - Illustration - A comet passes over Candor Chasma, one of the canyons of Valles Marineris. In the sky, the bright spot is the planet Earth. A comet lights up the Martian predawn over the twisted landscape of Candor Chasma. The distant mountains are several kilometers high. The planet Earth shines as a bright blue star in the sky

Mercury by Mariner 10 - Mercury by Mariner 10 - Mosaic of images obtained by the Mariner 10 probe on 29 March 1974 during its first flight
Mercury by Mariner 10 - Mercury by Mariner 10 - Mosaic of images obtained by the Mariner 10 probe on 29 March 1974 during its first flight

PIX4617124: Mercury by Mariner 10 - Mercury by Mariner 10 - Mosaic of images obtained by the Mariner 10 probe on 29 March 1974 during its first flight / Bridgeman Images

ID: PIX4617124

Mercury by Mariner 10 - Mercury by Mariner 10 - Mosaic of images obtained by the Mariner 10 probe on 29 March 1974 during its first flight

Mercury by Mariner 10 - Mercury by Mariner 10 - Basin Caloris - The Basin Caloris is the rest of a large impact crater; visible half on the left of the image, it measures 1300 km in diameter. Mosaic of images obtained by the Mariner 10 probe
Mercury by Mariner 10 - Mercury by Mariner 10 - Basin Caloris - The Basin Caloris is the rest of a large impact crater; visible half on the left of the image, it measures 1300 km in diameter. Mosaic of images obtained by the Mariner 10 probe

PIX4617148: Mercury by Mariner 10 - Mercury by Mariner 10 - Basin Caloris - The Basin Caloris is the rest of a large impact crater; visible half on the left of the image, it measures 1300 km in diameter. Mosaic of images obtained by the Mariner 10 probe / Bridgeman Images

ID: PIX4617148

Mercury by Mariner 10 - Mercury by Mariner 10 - Basin Caloris - The Basin Caloris is the rest of a large impact crater; visible half on the left of the image, it measures 1300 km in diameter. Mosaic of images obtained by the Mariner 10 probe

Avenue Frochot in Paris 9th.
Avenue Frochot in Paris 9th.

TEC4617168: Avenue Frochot in Paris 9th. / Bridgeman Images

ID: TEC4617168

Avenue Frochot in Paris 9th.

Mercury by Mariner 10 - Mercury by Mariner 10 - Region cratere Kuiper - Mosaic of images made by the Mariner 10 probe. Region around the Kuiper crater (small bright white crater at the bottom right of the picture) and the Lermontov crater (large white crater at the top left center)
Mercury by Mariner 10 - Mercury by Mariner 10 - Region cratere Kuiper - Mosaic of images made by the Mariner 10 probe. Region around the Kuiper crater (small bright white crater at the bottom right of the picture) and the Lermontov crater (large white crater at the top left center)

PIX4617192: Mercury by Mariner 10 - Mercury by Mariner 10 - Region cratere Kuiper - Mosaic of images made by the Mariner 10 probe. Region around the Kuiper crater (small bright white crater at the bottom right of the picture) and the Lermontov crater (large white crater at the top left center) / Bridgeman Images

ID: PIX4617192

Mercury by Mariner 10 - Mercury by Mariner 10 - Region cratere Kuiper - Mosaic of images made by the Mariner 10 probe. Region around the Kuiper crater (small bright white crater at the bottom right of the picture) and the Lermontov crater (large white crater at the top left center)

Avenue Frochot in Paris 9th.
Avenue Frochot in Paris 9th.

TEC4617195: Avenue Frochot in Paris 9th. / Bridgeman Images

ID: TEC4617195

Avenue Frochot in Paris 9th.

Window in Paris 9th.
Window in Paris 9th.

TEC4617221: Window in Paris 9th. / Bridgeman Images

ID: TEC4617221

Window in Paris 9th.

Paris seen from the 20th arrondissement.
Paris seen from the 20th arrondissement.

OMG4616946: Paris seen from the 20th arrondissement. / Bridgeman Images

ID: OMG4616946

Paris seen from the 20th arrondissement.

Reconstruction of a building grid in Paris 20th. Photography 20/04/00.
Reconstruction of a building grid in Paris 20th. Photography 20/04/00.

OMG4617036: Reconstruction of a building grid in Paris 20th. Photography 20/04/00. / Bridgeman Images

ID: OMG4617036

Reconstruction of a building grid in Paris 20th. Photography 20/04/00.


Back to top

Bridgeman Images • 17-19 Garway Road • London W2 4PH • United Kingdom • +44 (0)20 7727 4065

All contents © 1972-2015 Bridgeman Art Library Limited, All rights reserved.