Supporting SHERLOC in the Detection of Kerogen as a BiosignatureJuly 06, 2018 / Posted by: Miki Huynh
Left: SHERLOC will be mounted on the arm of the Mars 2020 rover. Right: Scan of a stromatolitic limestone Mars analog sample shows kerogen (dark bands) hosted by carbonate (white areas). Image sources: NASA / SETI Institute.
The upcoming Mars 2020 rover mission will hunt for signs of past microbial life and indications of habitable conditions on Mars. A device mounted on the rover’s arm will aid in the detection of kerogens, fossilized organic materials in sedimentary rocks: a UV-wavelength excitation instrument called SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics & Chemicals).
To inform NASA’s planning strategies for SHERLOC, Svetlana Shkolyar, a 2014 recipient of the NASA Astrobiology Early Career Collaboration Award, and her research team with the NASA Astrobiology Institute team based at SETI analyzed the capabilities of co-located time-gated Raman and fluorescent spectroscopy in detecting and distinguishing kerogen when scanning Mars analogue samples.
The team’s findings, published in Astrobiology reveal promising results and highlight the value of combining co-located Raman and fluorescence spectroscopies, similar to those obtainable by SHERLOC, to strengthen the confidence of kerogen detection as a potential biosignature in complex samples.
Source: [Astrobiology (via SETI Institute)]
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