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21 médias trouvés pour 'Valles Occidental'

Axes belonging to the Catalan Grave Culture, 2800-2500BC (stone)

Axes belonging to the Catalan Grave Culture, 2800-2500BC (stone)

IBE291978

Pre-romanesque Church of Saint Peter. Terrassa. Spain.

Pre-romanesque Church of Saint Peter. Terrassa. Spain.

TRK831670

Pre-romanesque Church of Saint Peter. Terrassa. Spain.

Pre-romanesque Church of Saint Peter. Terrassa. Spain.

TRK831687

Pre-romanesque Church of Saint Peter. Terrassa. Spain.

Pre-romanesque Church of Saint Peter. Terrassa. Spain.

TRK831669

Pre-romanesque Church of Saint Peter. Terrassa. Spain.

Pre-romanesque Church of Saint Peter. Terrassa. Spain.

TRK831668

Pre-romanesque Church of Saint Peter. Terrassa. Spain.

Pre-romanesque Church of Saint Peter. Terrassa. Spain.

TRK831673

Pre-romanesque Church of Saint Peter. Terrassa. Spain.

Pre-romanesque Church of Saint Peter. Terrassa. Spain.

TRK831671

Pre-romanesque Church of Saint Peter. Terrassa. Spain.

Pre-romanesque Church of Saint Peter. Terrassa. Spain.

TRK831672

The fjords of Sogn og Fjordane, 2003

The fjords of Sogn og Fjordane, 2003

UIG1580003

Building an Empire in the Fascist age: western lower plain, 09/05/1936 (b/w photo)

Building an Empire in the Fascist age: western lower plain, 09/05/1936 (b/w photo)

Baldinetti, Modestino (fl.1930)

FAF1249798

ninnus, 2007, (ice from the Western Antarctic Ice Sheet, sediment from Antarctica’s Dry Valleys and mixed media on paper)

premium — ninnus, 2007, (ice from the Western Antarctic Ice Sheet, sediment from Antarctica’s Dry Valleys and mixed media on paper)

ninnus, 2007, (ice from the Western Antarctic Ice Sheet, sediment from Antarctica’s Dry Valleys and mixed media on paper)

Cortada, Xavier

CTD1121519

leverett, 2007, (ice from the Western Antarctic Ice Sheet, sediment from Antarctica's Dry Valleys and mixed media on paper)

premium — leverett, 2007, (ice from the Western Antarctic Ice Sheet, sediment from Antarctica's Dry Valleys and mixed media on paper)

leverett, 2007, (ice from the Western Antarctic Ice Sheet, sediment from Antarctica's Dry Valleys and mixed media on paper)

Cortada, Xavier

CTD1121521

Mars: Noctis Labyrinthus - Illustration - Artist's view of Noctis Labyrinthus, a Martian canyon located in the western part of Valles Marineris. Panorama of Noctis Labyrinthus, a giant fault system on Mar

Mars: Noctis Labyrinthus - Illustration - Artist's view of Noctis Labyrinthus, a Martian canyon located in the western part of Valles Marineris. Panorama of Noctis Labyrinthus, a giant fault system on Mar

Steven Hobbs

PIX4616993

March: Chaotic terrain between Kasei Valles and Sacra Fossae - Mars: Chaotic terrain between Kasei Valles and Sacra Fossae - Region bordering Kasei Valles (top) and Sacra Fossae (bottom). Kasei Valles is one of the largest Martian canal systems. The large impact crater on the right is 35 km in diameter. The image covering an area of 225 km by 95 km was obtained by the Mars Express probe. Mars Express flew over the boundary between Kasei Valles and Sacra Fossae and imaged the region, acquiring spectacular views of the chaotic terrain in the area. The images are centred at 12* N/285* E and have a ground resolution of about 21 m/pixel. They cover 225 x 95 km or 21.375 sq km, an area roughly half the size of the Netherlands. The upper portion of the image swath shows the eastern margin of Kasei Valles and the western margin of the Lunae Planum plateau and the adjoining Sacra Fossae. Kasei Valles is one of the largest outflow channels on Mars, spanning 3000 km, from the Chryse Planitia basin in the north to Etus Chasma to the south. The impact crater at right is 35 km diameter — March: Chaotic terrain between Kasei Valles and Sacra Fossae - Mars: Chaotic terrain between Kasei Valles and Sacra Fossae - Region bordering Kasei Valles (top) and Sacra Fossae (bottom). Kasei Valles is one of the largest Martian canal systems. The large impact crater on the right is 35 km in diameter. The image covering an area of 225 km by 95 km was obtained by the Mars Express probe. Mars Express flew over the boundary between Kasei Valles and Sacra Fossae and imaged the region, acquiring spectacular views of the chaotic terrain in the area. The images are centred at 12* N/285* E and have a ground resolution of about 21 m/pixel. They cover 225 x 95 km or 21.375 sq km, an area roughly half the size of the Netherlands. The upper portion of the image swath shows the eastern margin of Kasei Valles and the western margin of the Lunae Planum plateau and the adjoining Sacra Fossae. Kasei Valles is one of the largest outflow channels on Mars, spanning 3000 km, from the Chryse Planitia basi

March: Chaotic terrain between Kasei Valles and Sacra Fossae - Mars: Chaotic terrain between Kasei Valles and Sacra Fossae - Region bordering Kasei Valles (top) and Sacra Fossae (bottom). Kasei Valles is one of the largest Martian canal systems. The large impact crater on the right is 35 km in diameter. The image covering an area of 225 km by 95 km was obtained by the Mars Express probe. Mars Express flew over the boundary between Kasei Valles and Sacra Fossae and imaged the region, acquiring spectacular views of the chaotic terrain in the area. The images are centred at 12* N/285* E and have a ground resolution of about 21 m/pixel. They cover 225 x 95 km or 21.375 sq km, an area roughly half the size of the Netherlands. The upper portion of the image swath shows the eastern margin of Kasei Valles and the western margin of the Lunae Planum plateau and the adjoining Sacra Fossae. Kasei Valles is one of the largest outflow channels on Mars, spanning 3000 km, from the Chryse Planitia basi

PIX4616154

II. WK, Western Front, Bridge Blasting, 1944 (photo)

II. WK, Western Front, Bridge Blasting, 1944 (photo)

SZT9232487

Mars - Noctis Labyrinthus - Image reconstructed from images taken by the 2001 Mars Odyssey probe.

Mars - Noctis Labyrinthus - Image reconstructed from images taken by the 2001 Mars Odyssey probe.

PIX4616427

Mars: Noctis Labyrinthus - Mars: Noctis Labyrinthus - Perspective view of Noctis Labyrinthus, located in the western part of the great Martian canyon Valles Marineris. This heavily eroded canyon is here 5000 meters deep. Image obtained by the Mars Express probe on June 25, 2006. On 25 June 2006 the High - Resolution Stereo Camera (HRSC), onboard the ESA spacecraft Mars Express obtained image data with a ground resolution of approximately 16 meters per pixel. The data were acquired in the region of Noctis Labyrinthus at approximately 6.5* southern latitude and 260* eastern longitude. The region Noctis Labyrinthus, the Labyrinth of the Night”” is located directly on the western edge of Valles Marineris, the “Grand Canyon of Mars””. It is part of the complex graben system which is associated with the up - arching of Tharsis. Eye - catching is the high density of deeply incised, smaller, maze - like fractures. The scene exhibits parts of those graben structures which are incised up to 5000 meters. They are strongly eroded as can be seen at the bottom of the graben which exhibits detritus. Younger lithologies can be seen on the upper edge of the graben. The fractures are witnesses of so - called extensional tectonics. The intense volcanism in the Tharsis region was associated with an intense up - arching of large areas. This process resulted in tectonic stress, causing the crust to thin out and lead to graben formation. — Mars: Noctis Labyrinthus - Mars: Noctis Labyrinthus - Perspective view of Noctis Labyrinthus, located in the western part of the great Martian canyon Valles Marineris. This heavily eroded canyon is here 5000 meters deep. Image obtained by the Mars Express probe on June 25, 2006. On 25 June 2006 the High - Resolution Stereo Camera (HRSC), onboard the ESA spacecraft Mars Express obtained image data with a ground resolution of approximately 16 meters per pixel. The data were acquired in the region of Noctis Labyrinthus at approximately 6.5* southern latitude and 260* eastern longitude. The region Noctis Labyrinthus, the Labyrinth of the Night”” is located directly on the western edge of Valles Marineris, the “Grand Canyon of Mars””. It is part of the complex graben system which is associated with the up - arching of Tharsis. Eye - catching is the high density of deeply incised, smaller, maze - like fractures. The scene exhibits parts of those graben structures which are incised up to 5000

Mars: Noctis Labyrinthus - Mars: Noctis Labyrinthus - Perspective view of Noctis Labyrinthus, located in the western part of the great Martian canyon Valles Marineris. This heavily eroded canyon is here 5000 meters deep. Image obtained by the Mars Express probe on June 25, 2006. On 25 June 2006 the High - Resolution Stereo Camera (HRSC), onboard the ESA spacecraft Mars Express obtained image data with a ground resolution of approximately 16 meters per pixel. The data were acquired in the region of Noctis Labyrinthus at approximately 6.5* southern latitude and 260* eastern longitude. The region Noctis Labyrinthus, the Labyrinth of the Night”” is located directly on the western edge of Valles Marineris, the “Grand Canyon of Mars””. It is part of the complex graben system which is associated with the up - arching of Tharsis. Eye - catching is the high density of deeply incised, smaller, maze - like fractures. The scene exhibits parts of those graben structures which are incised up to 5000

PIX4616056

II. WK, Eastern Front, Stalingrad, 1942 (photo)

II. WK, Eastern Front, Stalingrad, 1942 (photo)

SZT9240515

Raising the Vietnamese flag, Dien Bien Phu 1954 (b/w photo)

Raising the Vietnamese flag, Dien Bien Phu 1954 (b/w photo)

PFH1773698

Monte Gaina, 1968 (16mm dupe negative, scan 2K/Sound)

Monte Gaina, 1968 (16mm dupe negative, scan 2K/Sound)

MOD6428960

Saxony, GDR, historical, hotel, restaurants, restaurants, cafes, Beer …, 1985 (photo)

Saxony, GDR, historical, hotel, restaurants, restaurants, cafes, Beer …, 1985 (photo)

Sächsische Zeitung

IMO8758572

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