The Vegetation Red Edge Biosignature Through Time on Earth and Exoplanets

TL;DR

This study examines how Earth's vegetation red edge biosignature has evolved over 500 million years, varies with climate and vegetation types, and discusses implications for detecting similar biosignatures on exoplanets.

Contribution

It demonstrates the evolutionary increase of Earth's VRE strength and explores how geological and climatic changes affect its detectability on Earth and exoplanets.

Findings

VRE has increased over 500 million years of plant evolution.

Early plants produce a weaker VRE, about half as strong as modern vegetation.

Hotter, older Earth-like planets are promising targets for VRE detection.

Abstract

The high reflection of land vegetation in the near-infrared, the vegetation red edge (VRE), is often cited as a spectral biosignature for surface vegetation on exoplanets. The VRE is only a few percent change in reflectivity for a disk-integrated observation of present-day Earth. Here we show that the strength of Earth's VRE has increased over the past ~500 million years of land plant evolution and may continue to increase as solar luminosity increases and the planet warms, until either vegetation coverage is reduced, or the planet's atmosphere becomes opaque to light reflected off the surface. Early plants like mosses and liverworts, which dominated on land 500-400 million years ago, produce a weaker VRE, approximately half as strong as that of modern vegetation. We explore how the changes in land plants, as well as geological changes like ice coverage during ice-ages and interglacial periods, influence the detectability of the VRE through Earth's geological past. Our results show that the VRE has varied through the evolutionary history of land plants on Earth, and could continue to change into the future if hotter climate conditions became dominant, encouraging the spread of vegetation. Our findings suggest that older and hotter Earth-like planets are good targets for the search for a VRE signature. In addition, hot exoplanets and dry exoplanets with some water could be the best targets for a successful vegetation biosignature detection. As well as a strong red edge, lower cloud-fractions and low levels of atmospheric water vapor on such planets could make it easier to detect surface features in general.