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Updated: Sep 10, 2025
![Measuring the Spin-Lattice Relaxation Magnetic Field Dependence of Hyperpolarized [1-13C]pyruvate](/_next/image?url=https%3A%2F%2Fcloudfront.jove.com%2FCDNSource%2Fteasers%2F59399.jpg&w=3840&q=50)
Measuring the Spin-Lattice Relaxation Magnetic Field Dependence of Hyperpolarized [1-13C]pyruvate
Published on: September 13, 2019
Molecular Average and Intramolecular δ13C Measurements of Pyruvic Acid and Acetic Acid Using Gas Chromatography
Youki J Sato1, Allison A Baczynski1, Hao Xie2
1Astrobiology Center for Isotopologue Research, Department of Geosciences, Pennsylvania State University, University Park, Pennsylvania 16802, United States.
Abstract:
We developed a novel method using gas chromatography - Orbitrap mass spectrometry (GC Orbitrap MS) to measure the intramolecular carbon isotope value of pyruvic acid and acetic acid with high mass accuracy and mass resolution with nanomole (10-100) injections of analyte. Previous efforts to analyze intramolecular isotope patterns of small organic acids have been limited by labor-intensive chemical degradation steps, a narrow potential analyte pool, or large sample mass requirements. We present a new way to trap an analyte peak, which is then tested by measuring the molecular average and intramolecular carbon isotope values of pyruvic acid and acetic acid standards. Molecular average (MA) δ13C measurements with our method agreed with complementary methods within 2.2-2.6‰ relative mean standard deviation (RMSD) for 0.1 micromoles of compound, whereas intramolecular δ13C values varied from the complementary method from 1.9 to 4.9‰ RMSD. Intramolecular δ13C measurements of pyruvic acid and acetic acid yielded acquisition errors (σAE) of better than 0.2‰ and an experimental reproducibility (σER) of <2.8‰ and <3.4‰, respectively, for 0.1 micromoles of analyte. This method enables measurements of the intramolecular δ13C values of small organic acids sufficiently precise to differentiate synthesis pathways for these compounds, including for pathways within the central metabolism, and in extracts of carbonaceous meteorites, which are theorized to have formed in interstellar ices.
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