File:Volcanoes in Lacus Mortis (LROC213 - M131488521RE-2 thumb).png

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Captions

Captions

Most of the craters on the Moon formed through impact processes. However, some craters, like the one visible in this portion of LROC NAC frame M131488521R, may be a volcano summit pit crater.

Summary

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Description
English: Most of the craters on the Moon formed through impact processes. However, some craters, like the one visible in this portion of LROC NAC frame M131488521R, may be a volcano summit pit crater. Crater diameter is ~400 m, the image width is 923 m, and illumination is from the right [NASA/GSFC/Arizona State University].
Date 10 August 2010 (upload date)
Source Volcanoes in Lacus Mortis
Author NASA/GSFC/Arizona State University
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Keywords
InfoField
Volcanism; Pits
This media is a product of the
Lunar Reconnaissance Orbiter Camera
Credit and attribution belongs to the Lunar Reconnaissance Orbiter Camera (LROC) team, NASA/GSFC/Arizona State University
This image or video was catalogued by Goddard Space Flight Center of the United States National Aeronautics and Space Administration (NASA) under Photo ID: lroc:213.

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Licensing

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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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