Trace Elements in Manganese Minerals as Potential Biosignatures on Mars
Abstract
Observations from the Curiosity rover in Gale crater, Mars have shown the presence of high abundances of manganese (>3 wt% MnO) within sedimentary rocks throughout the traverse. Such high Mn abundances point to the past presence of abundant liquid water and strongly oxidizing conditions. On Earth, these types of environments are almost always habitable and are frequently inhabited by microbes. Given its close association with life and habitable environments on Earth, manganese has long been considered a potential biosignature for Mars. However, high concentrations of martian Mn have only recently been observed. In addition to the observations in Gale crater, high abundances of Mn have also been observed in Endeavor crater by the Opportunity rover and in the paired martian meteorites NWA 7034 and 7533 (`Black Beauty'), suggesting that Mn deposits may be more widespread on Mars than previously thought. The goal of this work is to determine whether there are unique signatures from rover payload instruments that can distinguish Mn-rich deposits as biogenic in origin (i.e., produced by life) from abiogenic Mn deposits. Importantly, Mn-oxides are known to scavenge trace metals from water because of their surface charge properties. We hypothesize that the presence and abundance of specific trace elements are the critical, distinguishing evidence for identifying the biogenic origin of Mn-bearing materials. A suite of natural rocks containing Mn-rich minerals with a range of Mn redox states was selected for analysis with laser-induced breakdown spectroscopy (LIBS). Samples with a biogenic origin had mixed valence redox states between Mn3+ and Mn4+ as inferred by mineralogy. Trace elements Ba, Li, Sr, and Rb were quantified and the presence or absence of Zn and Cu was ascertained by examining key LIBS peaks. Results show that samples with a known microbial origin had moderate Mn abundances >30 wt% MnO and higher Li and Ba. These results suggest that high Mn abundance alone is not sufficient evidence of a biosignatures. However, the presence of trace elements may help to infer the redox state of Mn, which may in turn point to samples that are more likely to have a biogenic origin.
- Publication:
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AGU Fall Meeting Abstracts
- Pub Date:
- December 2017
- Bibcode:
- 2017AGUFM.P53E2679L
- Keywords:
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- 0406 Astrobiology and extraterrestrial materials;
- BIOGEOSCIENCES;
- 1065 Major and trace element geochemistry;
- GEOCHEMISTRY;
- 2784 Solar wind/magnetosphere interactions;
- MAGNETOSPHERIC PHYSICS;
- 6296 Extra-solar planets;
- PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS