On The Hydrosphere Stability of TESS Targets: Applications to 700 d, 256 b, and 203 b
Paul Bonney (1, 2), Julia Kennefick (1) ((1) Corresponding author:, [email protected], (2) Department of Physics, University of Arkansas)

TL;DR
This paper develops a data-driven method to assess the stability of liquid water on exoplanets, applying it to TESS targets to evaluate their habitability potential over geological timescales.
Contribution
It introduces a novel approach combining observational data and simulations to estimate long-term hydrosphere stability of exoplanets.
Findings
Approximately 51% of TOI 700 d cases are desiccated.
All modeled cases for TOI 256 b retain water.
The method predicts water loss rates and remaining water inventories.
Abstract
A main determinant of the habitability of exoplanets is the presence of stable liquid surface water. In an era of abundant possible targets, the potential to find a habitable world remains a driving force in prioritization. We present here a data-forward method to investigate the likelihood of a stable hydrosphere on the timescales of the formation of life, 1 Gyr, and beyond. As our primary application, we use this method to examine the potential hydrospheres of TESS Objects of Interest 700 d, 256 b, and 203 b. We first present our selection criteria, which is based on an implementation of the Earth Similarity Index, as well as the results of an initial investigation into the desiccation of the targets, which reveals that TOI 203 b is almost certainly desiccated based on TESS observations. We then describe the characterization of the remaining targets and their host stars from 2MASS,…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research
