File:Korolev X and Z (LROC1076 - content M1168158470 LRmos warp str01 1100p).png

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Captions

Captions

Sharing a melt flow: visible in the right part of this oblique image is the bright wall of Korolev Z crater, the source of a 12.5-kilometer-long dark melt flow that drapes across the ancient floor of the degraded crater Korolev X.

Summary

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Description
English: Sharing a melt flow: visible in the right part of this oblique image is the bright wall of Korolev Z crater, the source of a 12.5-kilometer-long dark melt flow that drapes across the ancient floor of the degraded crater Korolev X. South is to the left. The image covers an area measuring about 20 kilometers from left to right and 40 kilometers from bottom to top. NAC image M1168158470LR [NASA/GSFC/Arizona State University].
Date 14 December 2018, 16:43:00 (upload date)
Source Korolev X and Z
Author NASA/GSFC/Arizona State University
Other versions
Keywords
InfoField
Anaglyph; Oblique; 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:1076.

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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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current16:02, 9 March 2024Thumbnail for version as of 16:02, 9 March 20241,100 × 1,100 (692 KB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://www.lroc.asu.edu/ckeditor_assets/pictures/701/content_M1168158470_LRmos.warp.str01.1100p.png via Commons:Spacemedia

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