<HashMap><database>biostudies-literature</database><scores/><additional><submitter>Chen X</submitter><funding>Swiss National Science Foundation</funding><pagination>36-53</pagination><full_dataset_link>https://www.ebi.ac.uk/biostudies/studies/S-EPMC10801744</full_dataset_link><repository>biostudies-literature</repository><omics_type>Unknown</omics_type><volume>8(1)</volume><pubmed_abstract>Zircons are found in extraterrestrial rocks from the Moon, Mars, and some differentiated meteorite parent-bodies. These zircons are rare, often of small size, and have been affected by neutron capture induced by cosmic ray exposure. The application of the &lt;sup>176&lt;/sup>Lu-&lt;sup>176&lt;/sup>Hf decay system to zircons from planetary bodies such as the Moon can help establish the chronology of large-scale differentiation processes such as the crystallization of the lunar magma ocean. Here, we present methods to measure the isotopic composition of Hf of extraterrestrial zircons dated using ID-TIMS U-Pb after chemical abrasion. We introduce a 2-stage elution scheme to separate Hf from Zr while preserving the unused Zr fraction for future isotopic analysis. The effect of neutron capture is also re-e</pubmed_abstract><journal>ACS earth &amp; space chemistry</journal><pubmed_title>Methodologies for &lt;sup>176&lt;/sup>Lu-&lt;sup>176&lt;/sup>Hf Analysis of Zircon Grains from the Moon and Beyond.</pubmed_title><pmcid>PMC10801744</pmcid><funding_grant_id>196955</funding_grant_id><funding_grant_id>200020</funding_grant_id><pubmed_authors>Zhang ZJ</pubmed_authors><pubmed_authors>Leya I</pubmed_authors><pubmed_authors>Zhang J</pubmed_authors><pubmed_authors>Szymanowski D</pubmed_authors><pubmed_authors>Chen X</pubmed_authors><pubmed_authors>Dauphas N</pubmed_authors><pubmed_authors>Schoene B</pubmed_authors><pubmed_authors>Barboni M</pubmed_authors><pubmed_authors>McKeegan KD</pubmed_authors></additional><is_claimable>false</is_claimable><name>Methodologies for &lt;sup>176&lt;/sup>Lu-&lt;sup>176&lt;/sup>Hf Analysis of Zircon Grains from the Moon and Beyond.</name><description>Zircons are found in extraterrestrial rocks from the Moon, Mars, and some differentiated meteorite parent-bodies. These zircons are rare, often of small size, and have been affected by neutron capture induced by cosmic ray exposure. The application of the &lt;sup>176&lt;/sup>Lu-&lt;sup>176&lt;/sup>Hf decay system to zircons from planetary bodies such as the Moon can help establish the chronology of large-scale differentiation processes such as the crystallization of the lunar magma ocean. Here, we present methods to measure the isotopic composition of Hf of extraterrestrial zircons dated using ID-TIMS U-Pb after chemical abrasion. We introduce a 2-stage elution scheme to separate Hf from Zr while preserving the unused Zr fraction for future isotopic analysis. The effect of neutron capture is also re-e</description><dates><release>2024-01-01T00:00:00Z</release><publication>2024 Jan</publication><modification>2025-04-04T21:16:09.746Z</modification><creation>2025-04-04T21:16:09.746Z</creation></dates><accession>S-EPMC10801744</accession><cross_references><pubmed>38264084</pubmed><doi>10.1021/acsearthspacechem.3c00093</doi></cross_references></HashMap>