Constraints on the formation age and evolution of the Moon from 142Nd–143 Nd systematics of Apollo 12 basalts. Earth
The Moon likely formed as a result of a giant impact between proto-Earth and another large body. The timing of this event and the subsequent lunar differentiation timescales are actively debated. New high-precision Nd isotope data of Apollo mare basalts are used to evaluate the Low-Ti, High-Ti and K...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.1077.959 2023-05-15T18:23:17+02:00 Constraints on the formation age and evolution of the Moon from 142Nd–143 Nd systematics of Apollo 12 basalts. Earth Claire L Mcleod Alan D Brandon Rosalind M G Armytage The Pennsylvania State University CiteSeerX Archives 2014 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1077.959 http://eps.harvard.edu/files/eps/files/mcleodetal.2014epsl.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1077.959 http://eps.harvard.edu/files/eps/files/mcleodetal.2014epsl.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://eps.harvard.edu/files/eps/files/mcleodetal.2014epsl.pdf text 2014 ftciteseerx 2020-05-03T00:17:27Z The Moon likely formed as a result of a giant impact between proto-Earth and another large body. The timing of this event and the subsequent lunar differentiation timescales are actively debated. New high-precision Nd isotope data of Apollo mare basalts are used to evaluate the Low-Ti, High-Ti and KREEP mantle source reservoirs within the context of lunar formation and evolution. The resulting models are assessed using both reported 146 146 Sm = 103 Myr). The lunar mantle source reservoir closure ages <4.5 Ga may be reconciled by 3 potential scenarios. First, the Moon formed later than currently favored models indicate, such that the lunar mantle closure age is near or at the time of lunar formation. Second, the Moon formed ca. 4.55 to 4.47 Ga and small amounts of residual melts were sustained within a crystallizing lunar magma ocean (LMO) for up to ca. 200 Myr from tidal heating or asymmetric LMO evolution. Third, the LMO crystallized rapidly after early Moon formation. Thus the Sm-Nd mantle closure age represents a later resetting of isotope systematics. This may have resulted from a global wide remelting event. While current Earth-Moon formation constraints cannot exclusively advocate or dismiss any of these models, the fact that U-Pb ages and Hf isotopes for Jack Hills zircons from Australia are best explained by an Earth that re-equilibrated at 4.4 Ga or earlier following the Moon-forming impact, does not favor a later forming Moon. If magma oceans crystallize in a few million years as currently advocated, then a global resetting, possibly by a large impact at 4.40 to 4.34 Ga, such as that which formed the South Pole Aitken Basin, best explains the late mantle closure age for the coupled Sm-Nd isotope systematics presented here. Text South pole Unknown Aitken ENVELOPE(-44.516,-44.516,-60.733,-60.733) South Pole |
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Open Polar |
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Unknown |
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ftciteseerx |
language |
English |
description |
The Moon likely formed as a result of a giant impact between proto-Earth and another large body. The timing of this event and the subsequent lunar differentiation timescales are actively debated. New high-precision Nd isotope data of Apollo mare basalts are used to evaluate the Low-Ti, High-Ti and KREEP mantle source reservoirs within the context of lunar formation and evolution. The resulting models are assessed using both reported 146 146 Sm = 103 Myr). The lunar mantle source reservoir closure ages <4.5 Ga may be reconciled by 3 potential scenarios. First, the Moon formed later than currently favored models indicate, such that the lunar mantle closure age is near or at the time of lunar formation. Second, the Moon formed ca. 4.55 to 4.47 Ga and small amounts of residual melts were sustained within a crystallizing lunar magma ocean (LMO) for up to ca. 200 Myr from tidal heating or asymmetric LMO evolution. Third, the LMO crystallized rapidly after early Moon formation. Thus the Sm-Nd mantle closure age represents a later resetting of isotope systematics. This may have resulted from a global wide remelting event. While current Earth-Moon formation constraints cannot exclusively advocate or dismiss any of these models, the fact that U-Pb ages and Hf isotopes for Jack Hills zircons from Australia are best explained by an Earth that re-equilibrated at 4.4 Ga or earlier following the Moon-forming impact, does not favor a later forming Moon. If magma oceans crystallize in a few million years as currently advocated, then a global resetting, possibly by a large impact at 4.40 to 4.34 Ga, such as that which formed the South Pole Aitken Basin, best explains the late mantle closure age for the coupled Sm-Nd isotope systematics presented here. |
author2 |
The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
Claire L Mcleod Alan D Brandon Rosalind M G Armytage |
spellingShingle |
Claire L Mcleod Alan D Brandon Rosalind M G Armytage Constraints on the formation age and evolution of the Moon from 142Nd–143 Nd systematics of Apollo 12 basalts. Earth |
author_facet |
Claire L Mcleod Alan D Brandon Rosalind M G Armytage |
author_sort |
Claire L Mcleod |
title |
Constraints on the formation age and evolution of the Moon from 142Nd–143 Nd systematics of Apollo 12 basalts. Earth |
title_short |
Constraints on the formation age and evolution of the Moon from 142Nd–143 Nd systematics of Apollo 12 basalts. Earth |
title_full |
Constraints on the formation age and evolution of the Moon from 142Nd–143 Nd systematics of Apollo 12 basalts. Earth |
title_fullStr |
Constraints on the formation age and evolution of the Moon from 142Nd–143 Nd systematics of Apollo 12 basalts. Earth |
title_full_unstemmed |
Constraints on the formation age and evolution of the Moon from 142Nd–143 Nd systematics of Apollo 12 basalts. Earth |
title_sort |
constraints on the formation age and evolution of the moon from 142nd–143 nd systematics of apollo 12 basalts. earth |
publishDate |
2014 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1077.959 http://eps.harvard.edu/files/eps/files/mcleodetal.2014epsl.pdf |
long_lat |
ENVELOPE(-44.516,-44.516,-60.733,-60.733) |
geographic |
Aitken South Pole |
geographic_facet |
Aitken South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
http://eps.harvard.edu/files/eps/files/mcleodetal.2014epsl.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1077.959 http://eps.harvard.edu/files/eps/files/mcleodetal.2014epsl.pdf |
op_rights |
Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766202845498966016 |