Grand canyons on the Moon

Abstract High energy streams of rock ejected from the Schrödinger impact basin carved two canyons in the lunar crust that are comparable in size to the Grand Canyon of North America. Here we use photogeologic mapping of those canyons and related impact ejecta deposits to show the trajectory of the i...

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Main Authors: David A. Kring, Danielle P. Kallenborn, Gareth S. Collins
Format: Article
Language:English
Published: Nature Portfolio 2025-02-01
Series:Nature Communications
Online Access:https://doi.org/10.1038/s41467-024-55675-z
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author David A. Kring
Danielle P. Kallenborn
Gareth S. Collins
author_facet David A. Kring
Danielle P. Kallenborn
Gareth S. Collins
author_sort David A. Kring
collection DOAJ
description Abstract High energy streams of rock ejected from the Schrödinger impact basin carved two canyons in the lunar crust that are comparable in size to the Grand Canyon of North America. Here we use photogeologic mapping of those canyons and related impact ejecta deposits to show the trajectory of the impacting asteroid or comet, which produced an asymmetrical pattern of crater excavation and transport of ejected debris. The flow directions of that ejected debris and the speed of its subsequent impact with the lunar surface are calculated, as is the energy that carved the canyons in less than ten minutes. The study implies that most of the excavated debris was ejected away from the lunar south pole, minimizing the amount of debris that covers the > 4 billion year old units that will be explored by Artemis astronauts.
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spelling doaj-art-2c814bc846934a28bd027255591f9a9e2025-02-09T12:46:17ZengNature PortfolioNature Communications2041-17232025-02-011611710.1038/s41467-024-55675-zGrand canyons on the MoonDavid A. Kring0Danielle P. Kallenborn1Gareth S. Collins2Lunar and Planetary Institute, Universities Space Research AssociationLunar and Planetary Institute, Universities Space Research AssociationDepartment of Earth Science and Engineering, Imperial College LondonAbstract High energy streams of rock ejected from the Schrödinger impact basin carved two canyons in the lunar crust that are comparable in size to the Grand Canyon of North America. Here we use photogeologic mapping of those canyons and related impact ejecta deposits to show the trajectory of the impacting asteroid or comet, which produced an asymmetrical pattern of crater excavation and transport of ejected debris. The flow directions of that ejected debris and the speed of its subsequent impact with the lunar surface are calculated, as is the energy that carved the canyons in less than ten minutes. The study implies that most of the excavated debris was ejected away from the lunar south pole, minimizing the amount of debris that covers the > 4 billion year old units that will be explored by Artemis astronauts.https://doi.org/10.1038/s41467-024-55675-z
spellingShingle David A. Kring
Danielle P. Kallenborn
Gareth S. Collins
Grand canyons on the Moon
Nature Communications
title Grand canyons on the Moon
title_full Grand canyons on the Moon
title_fullStr Grand canyons on the Moon
title_full_unstemmed Grand canyons on the Moon
title_short Grand canyons on the Moon
title_sort grand canyons on the moon
url https://doi.org/10.1038/s41467-024-55675-z
work_keys_str_mv AT davidakring grandcanyonsonthemoon
AT daniellepkallenborn grandcanyonsonthemoon
AT garethscollins grandcanyonsonthemoon