The Influence of Stellar Phosphorus On Our Understanding of Exoplanets and Astrobiology
Natalie R. Hinkel, Hilairy E. Hartnett, and Patrick A. Young

TL;DR
This paper examines stellar phosphorus abundance and its implications for exoplanet habitability, highlighting the need for more P data to understand planetary composition and potential for life.
Contribution
It compares stellar and planetary elemental ratios, emphasizing the importance of phosphorus data for assessing exoplanet habitability.
Findings
Stars generally have lower N and P compared to Earth and plankton.
P abundance data is scarce, limiting trend analysis.
High stellar P may support surface life on rocky exoplanets.
Abstract
When searching for exoplanets and ultimately considering their habitability, it is necessary to consider the planet's composition, geophysical processes, and geochemical cycles in order to constrain the bioessential elements available to life. Determining the elemental ratios for exoplanetary ecosystems is not yet possible, but we generally assume that planets have compositions similar to those of their host stars. Therefore, using the Hypatia Catalog of high-resolution stellar abundances for nearby stars, we compare the C, N, Si, and P abundance ratios of main sequence stars with those in average marine plankton, Earth's crust, as well as bulk silicate Earth and Mars. We find that, in general, plankton, Earth, and Mars are N-poor and P-rich compared with nearby stars. However, the dearth of P abundance data, which exists for only ~1% of all stars and 1% of exoplanet hosts, makes it…
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