File:Thick and Sticky Melt-Rock (LROC817 - content stretch fresh16 floor2x).png

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Captions

Captions

Cracks and pressure ridges in the surface of the floor support the hypothesis that this material had a component of melted rock when it formed. The pressure ridges formed when the solid surface crust was folded.

Summary

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Description
English: Cracks and pressure ridges in the surface of the floor support the hypothesis that this material had a component of melted rock when it formed. The pressure ridges formed when the solid surface crust was folded. LROC NAC M1112998800 upscaled by a factor of two; melt deposit is roughly 225 m across [NASA/GSFC/Arizona State University].
Date 15 April 2016, 14:17:00 (upload date)
Source Thick and Sticky Melt-Rock
Author NASA/GSFC/Arizona State University
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Keywords
InfoField
Impact Melt; Copernican Crater
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:817.

This tag does not indicate the copyright status of the attached work. A normal copyright tag is still required. See Commons:Licensing.
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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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current15:10, 9 March 2024Thumbnail for version as of 15:10, 9 March 2024952 × 952 (601 KB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://www.lroc.asu.edu/ckeditor_assets/pictures/157/content_stretch_fresh16_floor2x.png via Commons:Spacemedia

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