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Lava Flows (possible Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)
This is a full resolution mosaic centered at 25° North Latitude and 351° East Longitude.

The Region is approximately 160 Km (100 miles) across. It shows a series of complex Lava Flows which emerge from the Northern Flank of Sif Mons, a large Southern Venusian Volcano.
Several of the Flows occupy narrow troughs formed by long fractures. A sequence of events that can be inferred from this image is the formation of the dark background Plains by eruptions of extremely fluid volcanic material, and the formation of the small Shield Volcanoes on the Plains' Surface that can be seen in the upper left part of the image.

Next, the Region was domed upward probably by heat from the interior of Venus that ultimately caused magmas to break out from the Surface near the Summit Regions forming the Sif volcanic structure and its associated flank eruptions which can be seen in this image.
North_Polar_Regions-Ishtar_Terra.jpg Venusian_Surface-Venera_13-06-DPM-PCF-LXTT-IPF-1.jpg Volcanic_Features-Lava_Flows-PIA00471.jpg Venusian_Surface-Venera_13-09a.jpg 7-Venus_orbit31V3_fc_H.jpg
Informazioni File
Nome file:Volcanic_Features-Lava_Flows-PIA00471.jpg
Nome Album:MareKromium / Venus
Valutazione (6 voti): (Dettagli)
Keywords:Venus from orbit - Volcanic Features - Lava Flows
Copyright:NASA/JPL - Magellan Probe Project e Paolo C. Fienga/Lunexit Team per l'additional process. e la colorizzazione
Dimensione file:1016 KB
Aggiunto il:Gen 30, 2010
Dimensioni:2082 x 1736 pixels
Visto:53 volte
URL:http://www.lunexit.it/gallery/displayimage.php?pos=-26207
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