DOI:
10.1007/s10686-021-09800-1
Authors:
Shi, Xian;Castillo-Rogez, Julie;Hsieh, Henry;Hui, Hejiu;Ip, Wing-Huen;Lei, Hanlun;Li, Jian-Yang;Tosi, Federico;Zhou, Liyong;Agarwal, Jessica;Barucci, Antonella;Beck, Pierre;Bagatin, Adriano Campo;Capaccioni, Fabrizio;Coates, Andrew J.;Cremonese, Gabriele;Duffard, Rene;Grande, Manuel;Jaumann, Ralf;Jones, Geraint H.;Kallio, Esa;Lin, Yangting;Mousis, Olivier;Nathues, Andreas;Oberst, Jürgen;Sierks, Holger;Ulamec, Stephan;Wang, Mingyuan;Gauss Team
Abstract:
The goal of Project GAUSS (Genesis of Asteroids and evolUtion of the Solar System) is to return samples from the dwarf planet Ceres. Ceres is the most accessible candidate of ocean worlds and the largest reservoir of water in the inner Solar System. It shows active volcanism and hydrothermal activities in recent history. Recent evidence for the existence of a subsurface ocean on Ceres and the complex geochemistry suggest past habitability and even the potential for ongoing habitability. GAUSS will return samples from Ceres with the aim of answering the following top-level scientific questions: What is the origin of Ceres and what does this imply for the origin of water and other volatiles in the inner Solar System?
URL:
https://ui.adsabs.harvard.edu/#abs/2021ExA...tmp..123S/abstract
Keywords:
Ceres;Dwarf planet;Sample return;Ocean world;Habitability;Voyage 2050