With
recent progress of observational astronomy, the next generation
of space telescopes (JWST,
ARIEL, OST, HabEx, LUVOIR) will be able to determine the composition
of exoplanetary atmospheres in the next decades. The discovery of
rocky exoplanets, as potentially favorable harbors for life, finds
a particularly strong echo in the scientific community and in the
general audience. The interaction of the surface of a planetary body
with its atmosphere is key to understanding the composition of the
latter and hence to determine whether the planet may host life or
not. In an effort to describe surface–atmosphere interactions
on rocky planets and the heterogeneous reactions occurring on solid
surfaces, in particular mineral dust grains, in such systems it is
necessary to develop a systematic approach to this family of reactions.
Such an approach is proposed in this Perspective on three very distinct
examples of rocky planets: Earth, Mars, and Venus. These bodies have
experienced very different evolutions, although they likely started
from similar initial conditions; the pressure and temperature of their
atmospheres cover a broad range of values, offering an invaluable
set of planet-size laboratories to study the impact of physical and
chemical parameters on the evolution of atmospheres. Systems that
should be investigated in priority with relevance for Earth, Mars,
and Venus are discussed. It is shown that a better knowledge of mineral
dust supporting heterogeneous reactivity is crucial and that the impact
of environmental parameters on these reactions needs to be carefully
investigated. Current and future missions to Mars and Venus will require
such work to better model and understand the observations. In particular,
a strong effort is needed to study Venus, which has only few dedicated
laboratory setups although it will be the target of exploration missions
in the next decades. These studies will pave the way to build robust
models of exoplanetary atmospheres, which will be crucial to account
for the observations of their composition by space telescopes in the
near future.