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File:Barton crater.jpg

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Barton_crater.jpg (400 × 400 pixels, file size: 27 KB, MIME type: image/jpeg)

Summary

Description
English: This 54-km (32-mi) diameter crater is the size at which craters on Venus begin to possess peak-rings instead of a single central peak. The floor of Barton crater is flat and radar-dark, indicating possible infilling by lava flows sometime following the impact. Barton's central peak-ring is discontinuous and appears to have been disrupted or separated during or following the cratering process. The name Barton has been proposed by the Magellan Science Team, after Clara Barton, founder of the U. S. Red Cross; the name is tentative pending approval by the IAU.
Date
Source pds.jpl.nasa.gov/planets/captions/venus/barton.htm/
Author Magellan Team (NASA-Jet Propulsion Laboratory)
This image or video was catalogued by Jet Propulsion Laboratory of the United States National Aeronautics and Space Administration (NASA) under Photo ID: PIA00463.

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Licensing

Public domain 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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Date/TimeThumbnailDimensionsUserComment
current01:50, 14 December 2007Thumbnail for version as of 01:50, 14 December 2007400 × 400 (27 KB)Bryan Derksen{{Information |Description={{en|This 54-km (32-mi) diameter crater is the size at which craters on Venus begin to possess peak-rings instead of a single central peak. The floor of Barton crater is flat and radar-dark, indicating possible infilling by lava

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