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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Nature Portfolio
2025-02-01
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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. |
format | Article |
id | doaj-art-2c814bc846934a28bd027255591f9a9e |
institution | Kabale University |
issn | 2041-1723 |
language | English |
publishDate | 2025-02-01 |
publisher | Nature Portfolio |
record_format | Article |
series | Nature Communications |
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 |