Reexamination of Early Lunar Chronology With GRAIL Data: Terranes, Basins, and Impact Fluxes ...

Flooding of the lunar surface by ancient mare basalts has rendered uncertain the ages of lunar geochemical terranes and several impact basins. Here we combine craters having recognizable surface expressions with craters identified only by their gravitational signatures in Gravity Recovery and Interi...

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Main Authors: Evans, Alexander J., Andrews-Hanna, Jeffrey C., Head, James W., Soderblom, Jason M., Solomon, Sean C., Zuber, Maria T.
Format: Article in Journal/Newspaper
Language:unknown
Published: Columbia University 2018
Subjects:
Online Access:https://dx.doi.org/10.7916/d8-9k87-2b47
https://academiccommons.columbia.edu/doi/10.7916/d8-9k87-2b47
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author Evans, Alexander J.
Andrews-Hanna, Jeffrey C.
Head, James W.
Soderblom, Jason M.
Solomon, Sean C.
Zuber, Maria T.
author_facet Evans, Alexander J.
Andrews-Hanna, Jeffrey C.
Head, James W.
Soderblom, Jason M.
Solomon, Sean C.
Zuber, Maria T.
author_sort Evans, Alexander J.
collection DataCite
description Flooding of the lunar surface by ancient mare basalts has rendered uncertain the ages of lunar geochemical terranes and several impact basins. Here we combine craters having recognizable surface expressions with craters identified only by their gravitational signatures in Gravity Recovery and Interior Laboratory data to reassess the chronological sequence of lunar impact basins and the ages of major lunar geochemical terranes. Our results indicate that although volcanically flooded regions are deficient in craters with diameters greater than 20 km by more than 50% relative to unflooded regions, craters with diameters greater than 90 km can be readily recognized either by topography or by gravity anomaly. On the basis of the areal density of craters with diameters greater than 90 km we conclude that (1) the Serenitatis basin could be as young as the Imbrium basin; (2) the areal density of craters within the Procellarum KREEP Terrane is significantly lower than that for the South Pole‐Aitken basin and the ...
format Article in Journal/Newspaper
genre South pole
genre_facet South pole
geographic Aitken
South Pole
geographic_facet Aitken
South Pole
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institution Open Polar
language unknown
long_lat ENVELOPE(-44.516,-44.516,-60.733,-60.733)
op_collection_id ftdatacite
op_doi https://doi.org/10.7916/d8-9k87-2b4710.1029/2017je005421
op_relation https://dx.doi.org/10.1029/2017je005421
publishDate 2018
publisher Columbia University
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spelling ftdatacite:10.7916/d8-9k87-2b47 2025-01-17T00:52:11+00:00 Reexamination of Early Lunar Chronology With GRAIL Data: Terranes, Basins, and Impact Fluxes ... Evans, Alexander J. Andrews-Hanna, Jeffrey C. Head, James W. Soderblom, Jason M. Solomon, Sean C. Zuber, Maria T. 2018 https://dx.doi.org/10.7916/d8-9k87-2b47 https://academiccommons.columbia.edu/doi/10.7916/d8-9k87-2b47 unknown Columbia University https://dx.doi.org/10.1029/2017je005421 Moon Lunar geology Geochemistry FOS: Earth and related environmental sciences Impact craters Text article-journal Articles ScholarlyArticle 2018 ftdatacite https://doi.org/10.7916/d8-9k87-2b4710.1029/2017je005421 2024-10-01T11:49:36Z Flooding of the lunar surface by ancient mare basalts has rendered uncertain the ages of lunar geochemical terranes and several impact basins. Here we combine craters having recognizable surface expressions with craters identified only by their gravitational signatures in Gravity Recovery and Interior Laboratory data to reassess the chronological sequence of lunar impact basins and the ages of major lunar geochemical terranes. Our results indicate that although volcanically flooded regions are deficient in craters with diameters greater than 20 km by more than 50% relative to unflooded regions, craters with diameters greater than 90 km can be readily recognized either by topography or by gravity anomaly. On the basis of the areal density of craters with diameters greater than 90 km we conclude that (1) the Serenitatis basin could be as young as the Imbrium basin; (2) the areal density of craters within the Procellarum KREEP Terrane is significantly lower than that for the South Pole‐Aitken basin and the ... Article in Journal/Newspaper South pole DataCite Aitken ENVELOPE(-44.516,-44.516,-60.733,-60.733) South Pole
spellingShingle Moon
Lunar geology
Geochemistry
FOS: Earth and related environmental sciences
Impact craters
Evans, Alexander J.
Andrews-Hanna, Jeffrey C.
Head, James W.
Soderblom, Jason M.
Solomon, Sean C.
Zuber, Maria T.
Reexamination of Early Lunar Chronology With GRAIL Data: Terranes, Basins, and Impact Fluxes ...
title Reexamination of Early Lunar Chronology With GRAIL Data: Terranes, Basins, and Impact Fluxes ...
title_full Reexamination of Early Lunar Chronology With GRAIL Data: Terranes, Basins, and Impact Fluxes ...
title_fullStr Reexamination of Early Lunar Chronology With GRAIL Data: Terranes, Basins, and Impact Fluxes ...
title_full_unstemmed Reexamination of Early Lunar Chronology With GRAIL Data: Terranes, Basins, and Impact Fluxes ...
title_short Reexamination of Early Lunar Chronology With GRAIL Data: Terranes, Basins, and Impact Fluxes ...
title_sort reexamination of early lunar chronology with grail data: terranes, basins, and impact fluxes ...
topic Moon
Lunar geology
Geochemistry
FOS: Earth and related environmental sciences
Impact craters
topic_facet Moon
Lunar geology
Geochemistry
FOS: Earth and related environmental sciences
Impact craters
url https://dx.doi.org/10.7916/d8-9k87-2b47
https://academiccommons.columbia.edu/doi/10.7916/d8-9k87-2b47