  This paper outlines a simple approach to evaluate the atmospheric composition
of hot rocky planets by assuming different types of planetary composition and
using corresponding model calculations. To explore hot atmospheres above 1000
K, we model the vaporization of silicate magma and estimate the range of
atmospheric compositions according to the planet's radius and semi-major axis
for the Kepler February 2011 data release. Our results show 5 atmospheric types
for hot, rocky super-Earth atmospheres, strongly dependent on the initial
composition and the planet's distance to the star. We provide a simple set of
parameters that can be used to evaluate atmospheric compositions for current
and future candidates provided by the Kepler mission and other searches.
