Image:Magellan Eistla Regio.jpg

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Magellan 3D perspective of Venus surface in western Eistla Regio

Image source: http://images.jsc.nasa.gov/luceneweb/caption.jsp?photoId=S91-50687

Original caption: Magellan synthetic aperture radar data was used to create this three- dimensional (3D) perspective view of Venus' western Eistla Regio. This viewpoint is located at 1,310 kilometers (812 miles) southwest of Gula Mons at an elevation of 0.178 kilometers (0.48 miles). The view is of the northeast with Gula Mons appearing on the horizon. Gula Mons, a 3 kilometer (1.86 mile) high volcano, is located at approximately 22 degrees north latitude, 359 degrees east longitude. The impact crater Cunitz, named for the astronomer and mathematician Maria Cunitz, is visible in the center of the image. The crater is 48.5 kilometers (30 miles) in diameter and is 215 kilometers (133 miles) from the viewer's position. Magellan synthetic aperture radar data is combined with radar altimetry to develop a 3D map of the surface. Rays cast in a computer intersect the surface to create a 3D view.

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(del) (cur) 16:11, 11 July 2005 . . Keithlard (Talk | contribs) . . 640×480 (40,558 bytes) (Magellan 3D perspective of Venus surface in western Eistla Regio)