We review the origin and evolution of the atmospheres of Earth, Venus and Mars from the
time when their accreting bodies were released from the protoplanetary disk a few million …

The current state and surface conditions of the Earth and its twin planet Venus are drastically
different. Whether these differences are directly inherited from the earliest stages of …

Earth has had oceans for nearly four billion years and Mars had lakes and rivers 3.5–3.8
billion years ago. However, it is still unknown whether water has ever condensed on the …

We demonstrate that the deep volatile storage capacity of magma oceans has significant
implications for the bulk composition, interior, and climate state inferred from exoplanet mass …

ABSTRACT A new hot line list for the main isotopologue of CO2, 12C16O2 is presented. The
line list consists of almost 2.5 billion transitions between 3.5 million rotation-vibration states …

The earliest atmospheres of rocky planets originate from extensive volatile release during
magma ocean epochs that occur during assembly of the planet. These establish the initial …

The discovery of thousands of highly irradiated, low-mass, exoplanets has led to the idea
that atmospheric escape is an important process that can drive their evolution. Of particular …

The aim of this article is to provide the reader with an overview of the different possible
scenarios for the emergence of life, to critically assess them and, according to the …

The CHONS elements that constitute the outgassed atmosphere and exosphere have likely
been delivered by chondritic materials to the Earth during planetary accretion and …

Abstract Planets with 2 R⊕< R< 3 R⊕ and orbital period< 100 days are abundant; these
sub-Neptune exoplanets are not well understood. For example, Kepler sub-Neptunes are …