Expanding the Timeline for Earth's Photosynthetic Red Edge Biosignature
Jack T. O'Malley-James, Lisa Kaltenegger

TL;DR
This paper explores how the Earth's photosynthetic red edge biosignature can be detected earlier in Earth's history by considering lichens, algae, and cyanobacteria, thus broadening the timeline for detecting life on exoplanets.
Contribution
It demonstrates that the red edge biosignature could have been present for over 2 billion years due to various life forms, extending its applicability in astrobiology.
Findings
Lichens could extend the red edge biosignature to 1.2 Gyr ago.
Ocean algae and cyanobacteria could extend it to over 2 Gyr ago.
The red edge is a broad biosignature applicable to diverse life forms.
Abstract
When Carl Sagan observed the Earth during a Gallileo fly-by in 1993, he found a widely distributed surface pigment with a sharp reflection edge in the red part of the spectrum, which, together with the abundance of gaseous oxygen and methane in extreme thermodynamic disequilibrium, were strongly suggestive of the presence of life on Earth. This widespread pigmentation that could not be explained by geological processes alone, is caused by the cellular structure of vegetation - a mechanism for potentially limiting damage to chlorophyll and/or limiting water loss. The distinctive increase in the red portion of Earth's global reflectance spectrum is called the vegetation red edge in astrobiology literature and is one of the proposed surface biosignatures to search for on exoplanets and exomoons. Earth's surface vegetation has only been widespread for about half a billion years, providing a…
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