NASA MAGELLAN MISSION (1989-1994)
Sapas Mons (1,500m or 1, 5km - 4,921ft or 0.93mi)
Venus (Alta Regio)
The mountain
Sapas Mons 1.5 kilometers (0.93 mi) is a large volcano with twin summit, located in the Atla Regio region of planet Venus. Sapas is named after the Canaanite sun goddess. It measures about 400 kilometers (250 mi) across. Its flanks show numerous overlapping lava flows. The dark flows on the lower right of the radar image are thought to be smoother than the brighter ones near the central part of the volcano. Many of the flows appear to have been erupted along the flanks of the volcano rather than from the double summit. This type of flank eruption is common on large volcanoes on Earth, such as the Hawaiian volcanoes. The summit area has two flat-topped mesas, whose smooth tops give a relatively dark appearance in the radar image. Also seen near the summit are groups of pits, some as large as one kilometer (0.6 mile) across. These are thought to have formed when underground chambers of magma were drained through other subsurface tubes and lead to a collapse at the surface. A 20-kilometer-diameter (12 mi) impact crater northeast of the volcano is partially buried by the lava flows. Little was known about Atla Regio prior to the Magellan probe. The new data, acquired in February 1991, show the region to be composed of at least five large volcanoes such as Sapas Mons, which are commonly linked by complex systems of fractures or rift zones. If comparable to similar features on Earth Atla Regio probably formed when large volumes of molten rock upwelled from areas within the interior of Venus known as 'hot spots.'Source:
- NASA
The photographer
Soviet Venera 13 and 14 spacecraft observed in the 1970s have first photographed the twin summit. The Nasa Magellan Mission photographed the region in a more acute way.
- More about NASA Magellan Mission
- Nasa Magellan Mission to Venus
