ERC Consolidator Grant · 2017
Composition of solar system small bodies
The small bodies population (comets, asteroids, KBOs) is today central to Solar System studies. These objects are used to reconstruct the dynamical scenarios of Solar System formation and evolution, and are expected to have played a key role in the habitability of terrestrial planets. Because they are rich in volatile and organics, comets and dark asteroid types (C-, D-) are under intense scrutiny by the Planetary Science community. The objective of this project is to determine the composition of these primitive small bodies and whether or not we have samples available from their surfaces in the form of meteorites and extra-terrestrial dusts (IDPs, micrometeorites). Several decades of…
From the public funding record at EU CORDIS. Describes the funded project, not the reviews below.