An impact crater, subsequently modified by a wrinkle ridge in Mare Imbrium. Field of view 3.2 meters wide from LROC Narrow Angle Camera (NAC) observation M1114391184R, LRO orbit 16466, February 1, 2013; 1.23 meters resolution [NASA/GSFC/Arizona State University]. |
Sarah Braden
LROC News System
Stratigraphic relationships in today's Featured Image tell a story of complex geologic events on the lunar surface.
Planetary geologists interpret images taken from orbit and piece together a narrative. Initially a bolide impacted the lunar surface, creating a crater.
Subsequently mare basalt flows buried parts of the impact crater. In the above image you can see darker material around the edges of the crater's rim and also areas where mare basalt material covered parts of the rim and the crater interior. Finally, tectonic deformation created a wrinkle ridge which is better seen in the context image and topography below. Boulders from the wrinkle ridge fell into the impact crater where the edge of the wrinkle ridge intersects with the crater's rim (upper right hand corner of the Featured Image). This impact crater has seen better days!
Explore the entire NAC frame to see more of the wrinkle ridge and surrounding mare, HERE.
Related Posts:
Posidonius Y
Boulders in the Sea of Serenity
Up and Down / Back and Forth
A Wrinkly Crater
LROC News System
Stratigraphic relationships in today's Featured Image tell a story of complex geologic events on the lunar surface.
Planetary geologists interpret images taken from orbit and piece together a narrative. Initially a bolide impacted the lunar surface, creating a crater.
Subsequently mare basalt flows buried parts of the impact crater. In the above image you can see darker material around the edges of the crater's rim and also areas where mare basalt material covered parts of the rim and the crater interior. Finally, tectonic deformation created a wrinkle ridge which is better seen in the context image and topography below. Boulders from the wrinkle ridge fell into the impact crater where the edge of the wrinkle ridge intersects with the crater's rim (upper right hand corner of the Featured Image). This impact crater has seen better days!
LROC WAC topography showing the same region, contour interval is 140 meters elevation [NASA/GSFC/Arizona State University]. |
Related Posts:
Posidonius Y
Boulders in the Sea of Serenity
Up and Down / Back and Forth
A Wrinkly Crater
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