Dusty tails of evaporating exoplanets. I. Constraints on the dust composition

TL;DR

This study constrains the dust composition in evaporating exoplanets with comet-like tails by analyzing transit light curves, finding that corundum and iron-rich silicates fit observations best, and estimating dust mass loss rates.

Contribution

It introduces a semi-analytical model linking dust sublimation properties to tail length, constraining dust composition from light curve analysis.

Findings

Tail lengths are consistent with corundum or iron-rich silicate dust.

Pure iron and carbonaceous dust are disfavoured by the data.

Estimated dust mass loss rates are approximately 1.7 M_earth/Gyr for KIC 12557548b.

Abstract

Recently, two exoplanet candidates have been discovered, KIC 12557548b and KOI-2700b, whose transit profiles show evidence for a comet-like tail of dust trailing the planet, thought to be fed by the evaporation of the planet's surface. We aim to put constraints on the composition of the dust ejected by these objects from the shape of their transit light curves. We derive a semi-analytical expression for the attenuation of dust cross-section in the tail, incorporating the sublimation of dust grains as well as their drift away from the planet. This expression shows that the length of the tail is highly sensitive to the sublimation properties of the dust material. We compute tail lengths for several possible dust compositions, and compare these to observational estimates of the tail lengths of KIC 12557548b and KOI-2700b, inferred from their light curves. The observed tail lengths are consistent with dust grains composed of corundum (Al2O3) or iron-rich silicate minerals (e.g., fayalite, Fe2SiO4). Pure iron and carbonaceous compositions are disfavoured. In addition, we estimate dust mass loss rates of 1.7 +/- 0.5 M_earth/Gyr for KIC 12557548b, and > 0.007 M_earth/Gyr (1-sigma lower limit) for KOI-2700b.