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|  |  |  |  | | | Una pareja de volcanes en Marte 1 abril 2011
| | | |  | A wider contextual image showing the region around Ceraunius Tholus and Uranius Tholus. Together with Uranius Patera, a large volcano 120 km to the northeast, the volcanoes form the Uranius group. They are aligned with three large volcanoes known collectively as the Tharsis Montes. One of them, Ascraeus Mons, can be seen in the bottom left of this image. The others are Pavonis and Arsia. The Mars Express data were acquired in the Tharsis region at approximately 25°N / 263°E.
Credits: NASA MGS MOLA Science Team |  |  |  |  |
| | | | | | | |  | Ceraunius Tholus and Uranius Tholus are two volcanoes in the Tharsis region of Mars. Ceraunius Tholus is 130 km across and rises 5.5 km above its surroundings. Its neighbour, Uranius Tholus is a smaller volcano, with a base diameter of 62 km and a height of 4.5 km. The image was created using a Digital Terrain Model (DTM) obtained from the High Resolution Stereo Camera on ESA’s Mars Express spacecraft. Elevation data from the DTM is colour coded: purple indicates the lowest lying regions and grey the highest. The scale is in metres.
Credits: ESA/DLR/FU Berlin (G. Neukum) |  |  |  |  |
| | | | | | | |  | Ceraunius Tholus is 130 km across and rises 5.5 km above its surroundings. Its flanks display deeply incised valleys of which the longest and deepest is about 3.5 km wide and 300 m deep. It terminates with a fan of deposited material in the north of the Rahe crater. The crater itself is 35 km by 18 km and was created by the oblique impact of a meteorite. The High Resolution Stereo Camera on ESA’s Mars Express took this image. The perspective view has been calculated from the digital terrain model derived from the stereo channels.
Credits: ESA/DLR/FU Berlin (G. Neukum) |  |  |  |  |
| | | |  | Ceraunius Tholus and Uranius Tholus are two volcanoes in the Tharsis region of Mars. Ceraunius Tholus is 130 km across and rises 5.5 km above its surroundings. Its neighbour, Uranius Tholus is a smaller volcano, with a base diameter of 62 km and a height of 4.5 km. The High Resolution Stereo Camera on ESA’s Mars Express took this image. The perspective view has been calculated from the digital terrain model derived from the stereo channels.
Credits: ESA/DLR/FU Berlin (G. Neukum) |  |  |  |  |
| | | |  | Ceraunius Tholus and Uranius Tholus are two volcanoes in the Tharsis region of Mars. Ceraunius Tholus is 130 km across and rises 5.5 km above its surroundings. Its neighbour, Uranius Tholus is a smaller volcano, with a base diameter of 62 km and a height of 4.5 km. The High Resolution Stereo Camera on ESA’s Mars Express took this image. The perspective view has been calculated from the digital terrain model derived from the stereo channels.
Credits: ESA/DLR/FU Berlin (G. Neukum) |  |  |  |  |
| | | |  | Ceraunius Tholus and Uranius Tholus are two volcanoes in the Tharsis region of Mars. Ceraunius Tholus is 130 km across and rises 5.5 km above its surroundings. Its neighbour, Uranius Tholus is a smaller volcano, with a base diameter of 62 km and a height of 4.5 km. The High Resolution Stereo Camera (HRSC) on ESA’s Mars Express took this image. It combines data from HRSC’s nadir channel and one stereo channel to produce this 3D image. Stereoscopic glasses are required to see the 3D effect.
Credits: ESA/DLR/FU Berlin (G. Neukum) |  |  |  |  |
| | | |  | Ceraunius Tholus and Uranius Tholus are two volcanoes in the Tharsis region of Mars. Ceraunius Tholus is 130 km across and rises 5.5 km above its surroundings. Its neighbour, Uranius Tholus is a smaller volcano, with a base diameter of 62 km and a height of 4.5 km. The High Resolution Stereo Camera (HRSC) on ESA’s Mars Express took this image. It combines data from HRSC’s nadir channel and one stereo channel to produce this 3D image. Stereoscopic glasses are required to see the 3D effect.
Credits: ESA/DLR/FU Berlin (G. Neukum) |  |  |  |  |
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