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RELAX Xenon Isotopic Analysis of Neutron Irradiated OSIRIS-REX sample OREX-803064-0

Authors

Jamie GilmourSarah Crowther



Description

The dataset includes numbers of atoms of 132Xe and isotope ratios of the other xenon isotopes to 132Xe for each of a series of laser step heating analyses of sample OREX-803064-0. OREX-803064-0 is a single particle separated from aggregate sample OREX-803021-0. Xenon was released from the sample and admitted into the RELAX (Refrigerator Enhanced Laser Analyser for Xenon) time-of-flight, resonance ionization mass spectrometer at the University of Manchester for xenon isotopic analysis. 111 distinct, sequentially increasing temperature steps were analysed and calibrated with reference to air aliquots and blanks. Temperature was increased by increasing the power delivered to the sample by a fiber laser. The purpose of this dataset is to investigate the I-Xe system, and therefore the sample was artificially neutron irradiated prior to analysis (irradiation MN2025a). Aliquots of Shallowater enstatite were irradiated and analysed alongside the sample, to monitor the conversion of 127I to 128Xe; those data are also incorporated in this dataset. The Xe isotopic composition is similar to average carbonaceous chondrite (AVCC) xenon, with excesses of 129Xe from decay of 129I and 128Xe produced in the reactor. An I-Xe age ~15 Myr after CAI formation is determined, which may record a late halogen mobilising episode.


Info

Mission
OSIRIS-REx
Sample
OREX-803064-0
Session
20251007_RI-TOF-NGMS_UoM_OREX-803064-0_1

Analytical Methods

Laboratory
University of Manchester
Instrument
RELAX
Technique
Resonance ionization time of flight noble gas mass spectrometry

How To Cite

Gilmour, J., Crowther, S., 2026. RELAX Xenon Isotopic Analysis of Neutron Irradiated OSIRIS-REX sample OREX-803064-0, Version 1.0. Astromaterials Data Archive. https://doi.org/10.60707/9v2n-5839 Accessed 2026-07-20.

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Type

Dataset

Date Created

June 9, 2026

Size

2.27 MB

License
Review Status

Pending External Review


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Funding Sources

This material is supported by NASA under contract NNM10AA11C issued through the New Frontiers program. Work at the University of Manchester (UK) is funded by Science and Technology Facilities Council (STFC) grants ST/V000675/1 and ST/Y002369/1.

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