Susceptibility of planetary atmospheres to mass-loss and growth by planetesimal impacts: the impact shoreline.

This paper considers how planetesimal impacts affect planetary atmospheres. Atmosphere evolution depends on the ratio of gain from volatiles to loss from atmosphere stripping f v; for constant bombardment, atmospheres with f v < 1 are destroyed in finite time, but grow linearly with time for f v > 1. An impact outcome prescription is used to characterize how f v depends on planetesimal impact velocities, size distribution, and composition. Planets that are low mass and/or close to the star have atmospheres that deplete in impacts, while high-mass and/or distant planets grow secondary atmospheres. Dividing these outcomes is an f v = 1 impact shoreline analogous to Zahnle and Catling's cosmic shoreline. The impact shoreline's location depends on assumed impacting planetesimal properties, so conclusions for the atmospheric evolution of a planet like the Earth with f v ≈ 1 are only as strong as those assumptions. Application to the exoplanet population shows that the gap in the planet radius distribution at ∼1.5 R⊕ is coincident with the impact shoreline, which has a similar dependence on orbital period and stellar mass to the observed gap. Given sufficient bombardment, planets below the gap would be expected to lose their atmospheres, while those above could have atmospheres enhanced in volatiles. The level of atmosphere alteration depends on the total bombardment a planet experiences, and so on the system's (usually unknown) other planets and planetesimals, though massive distant planets would have low accretion efficiency. Habitable zone planets around lower luminosity stars are more susceptible to atmosphere stripping, disfavouring M stars as hosts of life-bearing planets if Earth-like bombardment is conducive to the development of life. [ABSTRACT FROM AUTHOR]