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Image of the Arcadia quadrangle (MC-3). The southern part contains the large shield volcano Alba Patera and the highly faulted Tempe Terra province, w
Image of the Arcadia quadrangle (MC-3). The southern part contains the large shield volcano Alba Patera and the highly faulted Tempe Terra province, which includes many small volcanoes.
Graben near Alba Patera, as seen by THEMIS. Graben and catenae, collapse features, both caused by faults. When the crust is stretched, faults form and
Graben near Alba Patera, as seen by THEMIS. Graben and catenae, collapse features, both caused by faults. When the crust is stretched, faults form and material falls into voids created by the stretching. Uranius Tholus (upper) and Ceraunius Tholus (largest) volcanoes are visible in wide context view, below and to the right of Alba Patera.
Forces from different directions caused this complex of grabens to form. Picture taken by THEMIS.
Forces from different directions caused this complex of grabens to form. Picture taken by THEMIS.
Mareotis Fossae Region, as seen by HiRISE
Mareotis Fossae Region, as seen by HiRISE
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Viking image of Alba Mons. The volcano's relief is barely visible in orbital photographs. The broad system of fractures on the volcano's eastern side
Viking image of Alba Mons. The volcano's relief is barely visible in orbital photographs. The broad system of fractures on the volcano's eastern side (right) is called Tantalus Fossae. The narrower fracture system on the western flank is Alba Fossae. (Viking color MDIM 2.1)
MOLA exaggerated relief view of Alba Mons central edifice and summit dome viewed from south (top) and north (bottom). Vertical exaggeration is 10x.
MOLA exaggerated relief view of Alba Mons central edifice and summit dome viewed from south (top) and north (bottom). Vertical exaggeration is 10x.
Central caldera complex of Alba Mons. The calderas are shallow compared to those on other Tharsis volcanoes. Within the larger caldera is a small shie
Central caldera complex of Alba Mons. The calderas are shallow compared to those on other Tharsis volcanoes. Within the larger caldera is a small shield capped by a concentric circular feature (near center). Image is about 200 km (120 mi) across (THEMIS daytime IR mosaic).
Dust mantle at the SW edge of small caldera on Alba Mons (HiRISE).
Dust mantle at the SW edge of small caldera on Alba Mons (HiRISE).