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Abstract EANA2025-152



Is it Alive? An Investigation into Mineral False Positives in the Search for Exoplanet Reflectance Biosignatures

Mia Belle Frothingham (1), Sean McMahon (1,2), Beth Biller (1,3), Lisa Kaltenegger (4)
(1) University of Edinburgh School of Physics & Astronomy, Scotland (2) University of Edinburgh School of Geosciences, Scotland (3) Royal Observatory at the University of Edinburgh, Scotland (4) Carl Sagan Institute at Cornell University, United States


Direct imaging by the next generation of space telescope instruments is expected to obtain disk-integrated spectra of Earth-like exoplanets in the visible-to-near-infrared. These spectra may capture reflected light from surface materials, potentially including biomass. Photosynthetic life is detectable in Earthshine via the “vegetation red edge” (VRE): a sharp, step-like increase in reflectance with increasing wavelength at ~700 nm. Other forms of biomass display analogous step-like reflectance “edges”. However, some minerals of non-biological origin are also known to show reflectance edges, suggesting a risk of false positives in exoplanet biosignature detection. We investigate edge-like features in mineral reflectance spectra using existing databases. We identify several sulfide and tectosilicate minerals with VRE-like features, as well as the prebiotically important cyanide salt, potassium ferrocyanide. We conclude that the future evaluation of the biogenicity of VRE-like features in exoplanet reflectance spectra may reduce to a judgement about the relative prior probability of a non-Earth-like planetary mineralogy versus Earth-like planetary biology. Current ongoing work involves expanding our understanding of the extent of false positives, testing the potential quantitative relationship between life and non-life, and exploring agnostic biosignatures in future telescope detections.