Exoplanet hosts reveal lithium depletion: Results from a homogeneous statistical analysis

TL;DR

This study uses a homogeneous statistical approach to show that stars hosting exoplanets tend to have lower lithium abundances than similar stars without planets, indicating a possible link between planet presence and stellar lithium depletion.

Contribution

The paper introduces a multivariable regression method to analyze lithium abundance differences between planet-hosting and non-hosting stars, explicitly accounting for stellar parameters and confirming lithium depletion in hosts.

Findings

Planet-host stars show significant lithium depletion compared to non-hosts.

The lithium depletion offset remains significant under various dataset constraints.

A large increase in lithium uncertainty estimates is needed to nullify the observed depletion.

Abstract

Aims. We study the impact of the presence of planets on the lithium abundance of host stars and evaluate the previous claim that planet hosts exhibit lithium depletion when compared to their non-host counterparts. Methods. Using previously published lithium abundances, we remove the confounding effect of the different fundamental stellar parameters by applying a multivariable regression on our dataset. In doing so, we explicitly make an assumption made implicitly by different authors: that lithium abundance depends linearly on fundamental stellar parameters. Using a moderator variable to distinguish stars with planets from those without, we evaluate the existence of an offset in lithium abundances between the two groups. We perform this analysis first for stars that present a clear lithium detection exclusively and include in a second analysis upper lithium measurements. Results. Our analysis shows that under the above-mentioned assumption of linearity, a statistically significant negative offset in lithium abundance between planet hosts and non-hosts is recovered. We concluded that an inflation on the lithium uncertainty estimations by a factor of larger than 5 is required to render the measured offset compatible with zero at less than 3-4 {\sigma} and make it non-significant. We demonstrated that the offset as delivered by our method depends on the different nature of the stars in the two samples. We did so by showing that the offset is reduced down to zero if the planet-host stars are replaced by comparison stars. Moreover, the measured depletion is still significant when one imposes different constraints on the dataset, such as a limit in planetary mass or constrain the host temperature to around solar value. We conclude then that planet-host stars exhibit enhanced lithium depletion when compared with non-host stars. (abridged)