File:PIA00209 Venus - 3-D Perspective of Golubkina Crater.jpg
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![File:PIA00209 Venus - 3-D Perspective of Golubkina Crater.jpg](https://upload.wikimedia.org/wikipedia/commons/thumb/c/cf/PIA00209_Venus_-_3-D_Perspective_of_Golubkina_Crater.jpg/600px-PIA00209_Venus_-_3-D_Perspective_of_Golubkina_Crater.jpg?20240505101844)
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[edit]DescriptionPIA00209 Venus - 3-D Perspective of Golubkina Crater.jpg |
English: This three dimensional representation of brightness variations in a Magellan radar image of Golubkina crater enhances the structural features of the crater. Golubkina is 34 kilometers (20.4 miles) in diameter, and is located at about 60.5 degrees north latitude, 287.2 degrees east longitude. Golubkina is characterized by terraced inner walls and a central peak, typical of large impact craters on the Earth, Moon and Mars. The terraced inner walls form at late stages in the formation of an impact crater, due to collapse of the initial cavity formed by the meteorite impact. The central peak forms due to rebound of the inner crater floor. |
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Source | https://photojournal.jpl.nasa.gov/catalog/PIA00209 |
Author | NASA/JPL |
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This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | ![]() |
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current | 10:18, 5 May 2024 | ![]() | 1,024 × 1,024 (158 KB) | PlanetUser (talk | contribs) | {{Information |Description={{en|This three dimensional representation of brightness variations in a Magellan radar image of Golubkina crater enhances the structural features of the crater. Golubkina is 34 kilometers (20.4 miles) in diameter, and is located at about 60.5 degrees north latitude, 287.2 degrees east longitude. Golubkina is characterized by terraced inner walls and a central peak, typical of large impact craters on the Earth, Moon and Mars. The terraced inner walls form at late st... |
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