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Hydrogen isotope analysis of thermal-desorption from activated-carbon filter sample OREX-103001-14

Authors

Ewerton SantosYongsong Huang



Description

This study applies gas chromatography–isotope ratio mass spectrometry (GC-IRMS) to analyze volatile and pyrolysis-derived organic compounds released from activated-carbon filter sample OREX-103001-14. These samples represent processed filter materials collected for assessment of organic contamination backgrounds. Sample was analyzed using pyrolysis at 600 C to obtain the Hydrogen isotope signature of weakly bound volatiles and thermally generated decomposition products. Sample preparation involved isolating activated-carbon fragments, weighing approximately 2 mg, and loading them into prebaked quartz tubes packed with combusted quartz wool. No GC-MS analysis were done for these samples due to limited sample quantity, but the identification was done by previous filter samples analysis using GC-MS and GC-C-IRMS. The thermal desorption runs primarily released low-molecular-weight hydrocarbons and oxygenated volatiles (e.g, isopropanol, acetone, and phenol), with isotopoe varying between -107 permil (isopropanol) to +230 permil (acetic acid). While pyrolysis generated a broader suite of decomposition products, including small hydrocarbons, aromatics, and nitrogen, sulfur, and oxygenbearing compounds.


Info

Mission
OSIRIS-REx
Sample
OREX-103001-14
Session
20260521_GC-C-IRMS_HU_OREX-103001-14_1

Analytical Methods

Laboratory
Hokkaido University
Instrument
Agilent 7890B with Thermo Delta V GC-C-IRMS instrument
Technique
Gas Chromatography-Combustion-Isotopic Ratio Mass Spectrometry

How To Cite

Santos, E., Huang, Y., 2026. Hydrogen isotope analysis of thermal-desorption from activated-carbon filter sample OREX-103001-14, Version 1.0. Astromaterials Data Archive. https://doi.org/10.60707/7prs-j403 Accessed 2026-07-01.

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Type

Dataset

Date Created

May 21, 2026

Size

1.82 MB

License
Review Status

Pending External Review


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Funding Sources

This research is funded by NASA grant 80NSSC22K1691 and under Contract NNM10AA11C issued through the New Frontiers Program.

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