Ideas about atmospheric composition and climate on the early Earth have evolved
considerably over the last 30 years, but many uncertainties still remain. It is generally agreed …

Jupiter's icy moon, Europa, harbors a subsurface liquid water ocean; the prospect of this
ocean being habitable motivates further exploration of the moon with the upcoming NASA …

Planet formation ADS Classic is now deprecated. It will be completely retired in October 2019.
This page will automatically redirect to the new ADS interface at that point. SAO/NASA ADS …

Saturn's moon, Enceladus, is a geologically active waterworld. The prevailing paradigm is
that there is a subsurface ocean that erupts to the surface, which leads to the formation of a …

We have considered a wide array of scenarios for Europa's chemical evolution in an attempt
to explain the presence of ice and hydrated materials on its surface and to understand the …

We examine formation conditions for the Galilean satellites in the context of models of late-
stage giant planet accretion and satellite-disk interactions. We first reevaluate the current …

The habitability of Europa is a property within a system, which is driven by a multitude of
physical and chemical processes and is defined by many interdependent parameters, so …

Many carbonaceous chondrites have been aqueously altered within their parent bodies.
From chemical and textural data on these meteorites and from studies of collision …

Carbonaceous chondrites comprise a unique subset of meteorites. Two classes of
carbonaceous chondrites, the so-called CI1 and CM2 chondrites, are particularly interesting …

In this chapter we discuss the structure, composition, and dynamical states of the interiors of
Io, Europa, Ganymede, and Callisto. Interior structure and composition models of the …