Rb-Sr, Sm-Nd and Lu-Hf isotope systematics of the lunar Mg-suite: the age of the lunar crust and its relation to the time of Moon formation
New Rb-Sr, 146,147Sm-142,143Nd and Lu-Hf isotopic analyses of Mg-suite lunar crustal rocks 67667, 76335, 77215 and 78238, including an internal isochron for norite 77215, were undertaken to better define the time and duration of lunar crust formation and the history of the source materials of the Mg...
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| Published in | Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences Vol. 372; no. 2024; p. 20130246 |
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| Main Authors | , , , |
| Format | Journal Article |
| Language | English |
| Published |
England
The Royal Society Publishing
13.09.2014
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| Subjects | |
| Online Access | Get full text |
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| Abstract | New Rb-Sr, 146,147Sm-142,143Nd and Lu-Hf isotopic analyses of Mg-suite lunar crustal rocks 67667, 76335, 77215 and 78238, including an internal isochron for norite 77215, were undertaken to better define the time and duration of lunar crust formation and the history of the source materials of the Mg-suite. Isochron ages determined in this study for 77215 are: Rb-Sr=4450±270 Ma, 147Sm-143Nd=4283±23 Ma and Lu-Hf=4421±68 Ma. The data define an initial 146Sm/144Sm ratio of 0.00193±0.00092 corresponding to ages between 4348 and 4413 Ma depending on the half-life and initial abundance used for 146Sm. The initial Nd and Hf isotopic compositions of all samples indicate a source region with slight enrichment in the incompatible elements in accord with previous suggestions that the Mg-suite crustal rocks contain a component of KREEP. The Sm/Nd-142Nd/144Nd correlation shown by both ferroan anorthosite and Mg-suite rocks is coincident with the trend defined by mare and KREEP basalts, the slope of which corresponds to ages between 4.35 and 4.45 Ga. These data, along with similar ages for various early Earth differentiation events, are in accord with the model of lunar formation via giant impact into Earth at ca 4.4 Ga. |
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| AbstractList | New Rb-Sr, 146,147Sm-142,143Nd and Lu-Hf isotopic analyses of Mg-suite lunar crustal rocks 67667, 76335, 77215 and 78238, including an internal isochron for norite 77215, were undertaken to better define the time and duration of lunar crust formation and the history of the source materials of the Mg-suite. Isochron ages determined in this study for 77215 are: Rb-Sr=4450±270 Ma, 147Sm-143Nd=4283±23 Ma and Lu-Hf=4421±68 Ma. The data define an initial 146Sm/144Sm ratio of 0.00193±0.00092 corresponding to ages between 4348 and 4413 Ma depending on the half-life and initial abundance used for 146Sm. The initial Nd and Hf isotopic compositions of all samples indicate a source region with slight enrichment in the incompatible elements in accord with previous suggestions that the Mg-suite crustal rocks contain a component of KREEP. The Sm/Nd-142Nd/144Nd correlation shown by both ferroan anorthosite and Mg-suite rocks is coincident with the trend defined by mare and KREEP basalts, the slope of which corresponds to ages between 4.35 and 4.45 Ga. These data, along with similar ages for various early Earth differentiation events, are in accord with the model of lunar formation via giant impact into Earth at ca 4.4 Ga. New Rb-Sr, (146,147)Sm-(142,143)Nd and Lu-Hf isotopic analyses of Mg-suite lunar crustal rocks 67667, 76335, 77215 and 78238, including an internal isochron for norite 77215, were undertaken to better define the time and duration of lunar crust formation and the history of the source materials of the Mg-suite. Isochron ages determined in this study for 77215 are: Rb-Sr=4450±270 Ma, (147)Sm-(143)Nd=4283±23 Ma and Lu-Hf=4421±68 Ma. The data define an initial (146)Sm/(144)Sm ratio of 0.00193±0.00092 corresponding to ages between 4348 and 4413 Ma depending on the half-life and initial abundance used for (146)Sm. The initial Nd and Hf isotopic compositions of all samples indicate a source region with slight enrichment in the incompatible elements in accord with previous suggestions that the Mg-suite crustal rocks contain a component of KREEP. The Sm/Nd-(142)Nd/(144)Nd correlation shown by both ferroan anorthosite and Mg-suite rocks is coincident with the trend defined by mare and KREEP basalts, the slope of which corresponds to ages between 4.35 and 4.45 Ga. These data, along with similar ages for various early Earth differentiation events, are in accord with the model of lunar formation via giant impact into Earth at ca 4.4 Ga. New Rb-Sr, 146,147 Sm- 142,143 Nd and Lu-Hf isotopic analyses of Mg-suite lunar crustal rocks 67667, 76335, 77215 and 78238, including an internal isochron for norite 77215, were undertaken to better define the time and duration of lunar crust formation and the history of the source materials of the Mg-suite. Isochron ages determined in this study for 77215 are: Rb-Sr=4450±270 Ma, 147 Sm- 143 Nd=4283±23 Ma and Lu-Hf=4421±68 Ma. The data define an initial 146 Sm/ 144 Sm ratio of 0.00193±0.00092 corresponding to ages between 4348 and 4413 Ma depending on the half-life and initial abundance used for 146 Sm. The initial Nd and Hf isotopic compositions of all samples indicate a source region with slight enrichment in the incompatible elements in accord with previous suggestions that the Mg-suite crustal rocks contain a component of KREEP. The Sm/Nd— 142 Nd/ 144 Nd correlation shown by both ferroan anorthosite and Mg-suite rocks is coincident with the trend defined by mare and KREEP basalts, the slope of which corresponds to ages between 4.35 and 4.45 Ga. These data, along with similar ages for various early Earth differentiation events, are in accord with the model of lunar formation via giant impact into Earth at ca 4.4 Ga. |
| Author | Borg, Lars E. Gaffney, Amy M. Carlson, Richard W. Boyet, Maud |
| AuthorAffiliation | 2 Chemical Sciences Division , Lawrence Livermore National Laboratory, 7000 East Avenue L-231 , Livermore, CA 94550, USA 1 Department of Terrestrial Magnetism , Carnegie Institution of Washington, 5241 Broad Branch Road , NW, Washington DC 20015, USA 3 Laboratoire Magmas et Volcans , Universite Blaise Pascal, CNRS UMR 6524, 5 Rue Kessler , Clermont-Ferrand 63038, France |
| AuthorAffiliation_xml | – name: 2 Chemical Sciences Division , Lawrence Livermore National Laboratory, 7000 East Avenue L-231 , Livermore, CA 94550, USA – name: 3 Laboratoire Magmas et Volcans , Universite Blaise Pascal, CNRS UMR 6524, 5 Rue Kessler , Clermont-Ferrand 63038, France – name: 1 Department of Terrestrial Magnetism , Carnegie Institution of Washington, 5241 Broad Branch Road , NW, Washington DC 20015, USA |
| Author_xml | – sequence: 1 givenname: Richard W. surname: Carlson fullname: Carlson, Richard W. email: rcarlson@ciw.edu organization: Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, NW, Washington DC 20015, USA – sequence: 2 givenname: Lars E. surname: Borg fullname: Borg, Lars E. organization: Chemical Sciences Division, Lawrence Livermore National Laboratory, 7000 East Avenue L-231, Livermore, CA 94550, USA – sequence: 3 givenname: Amy M. surname: Gaffney fullname: Gaffney, Amy M. organization: Chemical Sciences Division, Lawrence Livermore National Laboratory, 7000 East Avenue L-231, Livermore, CA 94550, USA – sequence: 4 givenname: Maud surname: Boyet fullname: Boyet, Maud organization: Laboratoire Magmas et Volcans, Universite Blaise Pascal, CNRS UMR 6524, 5 Rue Kessler, Clermont-Ferrand 63038, France |
| BackLink | https://www.ncbi.nlm.nih.gov/pubmed/25114305$$D View this record in MEDLINE/PubMed |
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| Copyright | 2014 The Author(s) Published by the Royal Society. All rights reserved. 2014 The Author(s) Published by the Royal Society. All rights reserved. 2014 |
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| Keywords | giant impact lunar crust age Moon formation magma ocean Mg-suite |
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| Notes | href:rsta20130246.pdf One contribution of 19 to a Discussion Meeting Issue 'Origin of the Moon'. ArticleID:rsta20130246 ark:/67375/V84-NX7ZJNQJ-5 istex:082AD2BA63B03337E590D006AE25B702B2D6E0D2 Discussion Meeting Issue 'Origin of the Moon: challenges and prospects' organised and edited by David J. Stevenson and Alex N. Halliday ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 One contribution of 19 to a Discussion Meeting Issue ‘Origin of the Moon’. |
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| Title | Rb-Sr, Sm-Nd and Lu-Hf isotope systematics of the lunar Mg-suite: the age of the lunar crust and its relation to the time of Moon formation |
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