Copyright © 2014 Elsevier Ltd. All rights reserved. This document is the author’s final accepted version of the journal article. You are advised to consult the published version if you wish to cite from it.NHM Repositor
Funding: TEJ acknowledges support from the State Key Laboratory for Geological Processes and Mineral...
While on Earth the processes of early differentiation and crust formation have been largely overprin...
Isotopic studies of mare basalts have led workers to conclude that their sources are heterogeneous o...
Copyright © 2014 Elsevier Ltd. All rights reserved. This document is the author’s final accepted ver...
The heterogeneous-source model of mare basalt formation indicates that Lunar Magma Ocean (LMO) overt...
The heterogeneous-source model of mare basalt formation indicates that Lunar Magma Ocean (LMO) overt...
Corresponding author. E-mail address: cshearer@unm.edu (C.K. Shearer).early mantle dynamics and melt...
The Earth and the Moon are observed to be almost indistinguishable over a range of refractory isotop...
The primordial differentiation of the Moon via a global magma ocean has become the paradigm under wh...
Mare basalts comprise less than 1% of the lunar crust, but they constitute our primary source of inf...
Lunar rocks are inferred to tap the different fossil cumulate layers formed during crystallisation o...
A scenario for the formation of the Moon is advanced and is argued to be consistent with both known ...
The Apollo 17 high-Ti mare basalts are derived from source regions containing plagioclase that was n...
Lunar sample 15474,4 is a tiny fragment of olivine-augite vitrophyre that is a mare basalt. Although...
Early studies of mare basalts from the Apollo 15 site established that two distinct groups are repre...
Funding: TEJ acknowledges support from the State Key Laboratory for Geological Processes and Mineral...
While on Earth the processes of early differentiation and crust formation have been largely overprin...
Isotopic studies of mare basalts have led workers to conclude that their sources are heterogeneous o...
Copyright © 2014 Elsevier Ltd. All rights reserved. This document is the author’s final accepted ver...
The heterogeneous-source model of mare basalt formation indicates that Lunar Magma Ocean (LMO) overt...
The heterogeneous-source model of mare basalt formation indicates that Lunar Magma Ocean (LMO) overt...
Corresponding author. E-mail address: cshearer@unm.edu (C.K. Shearer).early mantle dynamics and melt...
The Earth and the Moon are observed to be almost indistinguishable over a range of refractory isotop...
The primordial differentiation of the Moon via a global magma ocean has become the paradigm under wh...
Mare basalts comprise less than 1% of the lunar crust, but they constitute our primary source of inf...
Lunar rocks are inferred to tap the different fossil cumulate layers formed during crystallisation o...
A scenario for the formation of the Moon is advanced and is argued to be consistent with both known ...
The Apollo 17 high-Ti mare basalts are derived from source regions containing plagioclase that was n...
Lunar sample 15474,4 is a tiny fragment of olivine-augite vitrophyre that is a mare basalt. Although...
Early studies of mare basalts from the Apollo 15 site established that two distinct groups are repre...
Funding: TEJ acknowledges support from the State Key Laboratory for Geological Processes and Mineral...
While on Earth the processes of early differentiation and crust formation have been largely overprin...
Isotopic studies of mare basalts have led workers to conclude that their sources are heterogeneous o...
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