Constraints on Aquatic Photosynthesis for Terrestrial Planets around Other Stars

Aquatic photosynthesis plays a major role in carbon fixation and O2 production on Earth. In this Letter, we analyze the prospects for oxygenic photosynthesis in aquatic environments on modern Earth-analogs around F-, G-, K-, and M-type stars. Our analysis takes into account the spectral type of the host star, attenuation of light by aquatic organisms, and rates of respiration and photosynthesis. We study the compensation depth (${{ \mathcal Z }}_{\mathrm{CO}}$) and the critical depth (${{ \mathcal Z }}_{\mathrm{CR}}$), defined respectively as the locations where the net growth rates and vertically integrated net growth rates of photoautotrophs become zero. Our analysis suggests that ${{ \mathcal Z }}_{\mathrm{CO}}$ declines by more than an order of magnitude as one moves from the habitable zones around Sun-like stars to late-type M-dwarfs, but ${{ \mathcal Z }}_{\mathrm{CR}}$ decreases by only a modest amount (∼40%). For M-dwarf exoplanets, we propose that the photosynthetic red edge may constitute a more robust biosignature of aquatic photosynthesis compared to atmospheric O2.