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In Situ Zircon Lu-Hf Isotopic Analyses on the Sapphire 1700 MC-ICPMS: Example from the San Gabriel Anorthosite, CA and Implications for Planetary AnalogsThe mineral zircon is the primary choice for U-Pb geochronology and the coupling of these ages to the zircon’s Lu-Hf isotopic composition provides a powerful tool for elucidating magmatic sources, as well as elucidating the temporal evolution of the crust-mantle system. The number of published studies with Lu-Hf in zircon measurements has increased rapidly with the development and improvement of laser ablation inductively coupled mass spectrometry (LA-ICPMS) [e.g., 1]. On a smaller scale, there has also been an increase in studies using the Lu-Hf isotopic system in zircon to advance our understanding of the formation of non-terrestrial planetary bodies (e.g. petrogenesis of lunar [2] and martian zircon [3]).
From a precious extraterrestrial sample perspective, with limited amount of sample available, there is a need to continuously to document the capabilities and limitations of semi-destructive in-situ geochemical measurement techniques. Here, we report the in-situ zircon Lu-Hf measurement capabilities of the Sapphire 1700 MC-ICPMS, a first, and discuss a Mesoproterozoic analog sample. Namely, a pegmatitic zircon from the San Gabriel Mountain anorthosite, CA.
Document ID
20240016138
Acquisition Source
Johnson Space Center
Document Type
Extended Abstract
Authors
J B Setera
(The University of Texas at El Paso El Paso, United States)
J I Simon
(Johnson Space Center Houston, United States)
Date Acquired
December 16, 2024
Subject Category
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: 56th Lunar and Planetary Science Conference (LPSC)
Location: The Woodlands, TX
Country: US
Start Date: March 10, 2025
End Date: March 14, 2025
Sponsors: Lunar and Planetary Institute
Funding Number(s)
CONTRACT_GRANT: 80JSC022DA035
WBS: 811073
Distribution Limits
Public
Copyright
Public Use Permitted.
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