simulations

Chromatic transit light curves of disintegrating rocky planets

Context. Kepler observations have revealed a class of short-period exoplanets, of which Kepler-1520 b is the prototype, which have comet-like dust tails thought to be the result of small, rocky planets losing mass. The shape and chromaticity of the …

Dusty tails of evaporating exoplanets. II. Physical modelling of the KIC 12557548b light curve

Context. Evaporating rocky exoplanets, such as KIC 12557548b, eject large amounts of dust, which can trail the planet in a comet- like tail. When such objects occult their host star, the resulting transit signal contains information about the dust in …