Presentation Title
Fourier Transform Infrared (FTIR) Spectrographic Threshold Analysis of Serpentinite vs Stichtite: Implications for Biomarker Detection on Mars
Presentation Type
Poster Presentation/Art Exihibt
College
College of Natural Sciences
Major
Geological Sciences
Location
SMSU Event Center BC
Faculty Mentor
Dr. Erik Melchiorre
Start Date
5-17-2018 9:30 AM
End Date
5-17-2018 11:00 AM
Abstract
Stichtite is a chromium magnesium carbonate hydroxide mineral that forms in environments associated with the earliest life on Earth. This mineral was detectable at levels less than 5% of a sample, using Fourier Transform Infrared Spectroscopy (FTIR), a remote sensing technique which has been used to map Mars. FTIR data was collected from stichtite and its serpentinite host to capture average spectral profiles for each mineral. These endmember profiles were used to calculate synthetic profiles for a range of endmember ratios. Significantly, these synthetic profiles are an excellent match for actual measurements with stichtite-serpentinite mixtures, providing validation for the use of synthetic profiles. A synthetic profile with just 5% stichtite still displays FTIR peaks discernible from serpentinite by at least 1% reflectance intensity at wavelengths of 3500 cm-1, 1366cm-1, and 750cm-1. The association of terrestrial stichtite with early habitable environments, and its ability to be detected with a common remote sensing technique, suggest future work is needed to re-examine Mars FTIR data for the presence of a stichtite biomarker
Fourier Transform Infrared (FTIR) Spectrographic Threshold Analysis of Serpentinite vs Stichtite: Implications for Biomarker Detection on Mars
SMSU Event Center BC
Stichtite is a chromium magnesium carbonate hydroxide mineral that forms in environments associated with the earliest life on Earth. This mineral was detectable at levels less than 5% of a sample, using Fourier Transform Infrared Spectroscopy (FTIR), a remote sensing technique which has been used to map Mars. FTIR data was collected from stichtite and its serpentinite host to capture average spectral profiles for each mineral. These endmember profiles were used to calculate synthetic profiles for a range of endmember ratios. Significantly, these synthetic profiles are an excellent match for actual measurements with stichtite-serpentinite mixtures, providing validation for the use of synthetic profiles. A synthetic profile with just 5% stichtite still displays FTIR peaks discernible from serpentinite by at least 1% reflectance intensity at wavelengths of 3500 cm-1, 1366cm-1, and 750cm-1. The association of terrestrial stichtite with early habitable environments, and its ability to be detected with a common remote sensing technique, suggest future work is needed to re-examine Mars FTIR data for the presence of a stichtite biomarker