A portion of the eastern edge of Alpha Regio is
displayed in this three-dimensional perspective view of the surface of Venus.
The viewpoint is located at approximately 30 degrees south latitude, 11.8
degrees east longitude at an elevation of 2.4 kilometers (3.8 miles). The view
is to the northeast at the center of an area containing seven circular dome-like
hills. The average diameter of the hills is 25 kilometers (15 miles) with
maximum heights of 750 meters (2,475 feet). Three of the hills are visible in
the center of the image. Fractures on the surrounding plains are both older and
younger than the domes. The hills may be the result of viscous or thick
eruptions of lava coming from a vent on the relatively level ground, allowing
the lava to flow in an even lateral pattern. The concentric and radial fracture
patterns on their surfaces suggests that a chilled outer layer formed, then
further intrusion in the interior stretched the surface. An alternative
interpretation is that domes are the result of shallow intrusions of molten lava
causing the surface to rise. If they are intrusive, then magma withdrawal near
the end of the eruptions produced the fractures. The bright margins possibly
indicate the presence of rock debris or talus at the slopes of the domes.
Resolution of the Magellan data is about 120 meters (400 feet). Magellan's
synthetic aperture radar is combined with radar altimetry to develop a
three-dimensional map of the surface. A perspective view is then generated from
the map. Simulated color and a process called radar-clinometry are used to
enhance small-scale structures. The simulated hues are based on color images
recorded by the Soviet Venera 13 and 14 spacecraft. The image was produced by
the JPL Multimission Image Processing Laboratory by Eric De Jong, Jeff Hall,
Myche McAuley, and Randy Kirk of the United States Geological Survey, and is a
single frame from the movie released at the May 29, 1991 Magellan news
conference.