Oxygen Isotope Signatures of UV Oxidation of Phosphite: Implications for a Biomarker in the Search for Life
Abstract
On the present Earth, phosphorus (P) occurs primarily in fully-oxidized form (P5+) as orthophosphate (PO4), and PO4 derived from igneous apatite minerals is considered as the primary source of P for prebiotic reactions and evolution of first life. Recent discoveries have shown, however, that abundant P compounds with valence <5+, primarily phosphite (PO3 with P3+), are produced from aqueous weathering of phosphides in meteorites(1) and of fulgurites formed by lightning strikes or high-energy impacts(2). These studies concluded that PO3 was likely abundant on the oxygen-free early Earth and extraterrestrial environments, and was possibly the first form of biologically-available P, due to its greater solubility and reactivity relative to PO4 and apatite(1). These findings suggest alternative prebiotic P reservoirs to igneous apatite that would also likely have very different prebiotic/baseline PO4 δ18O values. Here we report results of experimental studies to determine the O-isotope signature of PO4 derived from PO3 oxidation catalyzed by ultraviolet (UV) radiation, which was not blocked on early Earth due to lack of an ozone layer(3). These studies are critical for interpretation of PO4 δ18O biosignatures preserved in ancient terrestrial and extraterrestrial samples. Experiments on UV-catalyzed oxidation of aqueous PO3 to PO4 were conducted using δ18O-labled PO3 and different δ18O-labled waters to gain information on (i) the source(s) of O involved and mechanism of oxidation of PO3 to PO4, and (ii) fractionations accompanying O incorporation into product PO4. Our preliminary results under modern atmospheric conditions indicate incorporation of ca. 15 % O from ambient water and ca. 10 % atmospheric O (δ18O: ~23.5 ‰) into product PO4 with a fractionation between incorporated water O and ambient water O of -20 × 4 ‰ (1 SD), assuming 75 % inheritance of O from PO3 and direct incorporation of atmospheric O into product PO4 without fractionation. If initial δ18O values of PO3 sources were the same as igneous apatite (6 - 8 ‰)(4) and water δ18O = 0 ‰, calculated δ18O values of product PO4 would range from 3.9 to 5.4 ‰, which are lower than that of igneous apatite by 2 - 3 ‰. By investigating abiotic, enzymatic and microbial PO3 oxidation mechanisms under both aerobic and anaerobic conditions and their attendant O-isotope fractionations in future experiments, we will better distinguish reduced-P vs. igneous apatite PO4 sources, abiotic vs. biologically-produced PO4 O-isotope signatures, and also develop a better PO4 biomarker for evolution of P reservoirs on early Earth and extraterrestrial systems. References: (1) Pasek (2008) PNAS 105, 853. (2) Pasek and Block (2009) Nature Geoscience 2, 553. (3) Miller (1953) Science 117, 528. (4) Taylor and Epstein (1962) Geol. Soc. Am. Bull. 73, 461. Acknowledgments: This research was supported by NASA under award No. NNX13AJ36G. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Aeronautics and Space Administration.
- Publication:
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AGU Fall Meeting Abstracts
- Pub Date:
- December 2013
- Bibcode:
- 2013AGUFM.P51F1791C
- Keywords:
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- 5200 PLANETARY SCIENCES: ASTROBIOLOGY;
- 1041 GEOCHEMISTRY Stable isotope geochemistry;
- 0424 BIOGEOSCIENCES Biosignatures and proxies;
- 1060 GEOCHEMISTRY Planetary geochemistry