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GAUSS - genesis of asteroids and evolution of the solar system: A sample return mission to Ceres.
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.
Affiliation
  • Shi X; Max Planck Institute for Solar System Research, Göttingen, Germany.
  • Castillo-Rogez J; Present Address: Shanghai Astronomical Observatory, Shanghai, China.
  • Hsieh H; NASA Jet Propulsion Laboratory, La Cañada Flintridge, CA USA.
  • Hui H; Planetary Science Institute, Tucson, AZ USA.
  • Ip WH; School of Earth Sciences and Engineering, Nanjing University, Nanjing, China.
  • Lei H; Institute of Astronomy and Space Science, National Central University, Chung Li, Taiwan.
  • Li JY; School of Astronomy and Space Science, Nanjing University, Nanjing, China.
  • Tosi F; Planetary Science Institute, Tucson, AZ USA.
  • Zhou L; Istituto Nazionale di AstroFisica - Istituto di Astrofisica e Planetologia Spaziali (INAF-IAPS), Rome, Italy.
  • Agarwal J; School of Astronomy and Space Science, Nanjing University, Nanjing, China.
  • Barucci A; Max Planck Institute for Solar System Research, Göttingen, Germany.
  • Beck P; Institute for Geophysics and Extraterrestrial Physics, Technical University Braunschweig, Braunschweig, Germany.
  • Bagatin AC; LESIA-Observatoire de Paris, Université PSL, CNRS, Université de Paris, Sorbonne Université, F-92195 Meudon, Principal Cedex, France.
  • Capaccioni F; CNRS Institut de Planétologie et d'Astrophysique, Univ. Grenoble Alpes, Grenoble, France.
  • Coates AJ; Universidad de Alicante, Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Alicante, Spain.
  • Cremonese G; Istituto Nazionale di AstroFisica - Istituto di Astrofisica e Planetologia Spaziali (INAF-IAPS), Rome, Italy.
  • Duffard R; Mullard Space Science Laboratory, University College London, Surrey, UK.
  • Grande M; INAF - Osservatorio Astronomico di Padova, Padova, Italy.
  • Jaumann R; Instituto de Astrofísica de Andalucía (CSIC), Granada, Spain.
  • Jones GH; University of Aberystwyth, Aberystwyth, UK.
  • Kallio E; Institute of Geological Sciences, Free University of Berlin, Berlin, Germany.
  • Lin Y; Mullard Space Science Laboratory, University College London, Surrey, UK.
  • Mousis O; School of Electrical Engineering, Aalto University, Aalto, Finland.
  • Nathues A; Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.
  • Oberst J; Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France.
  • Sierks H; Max Planck Institute for Solar System Research, Göttingen, Germany.
  • Ulamec S; DLR Institute of Planetary Research, Berlin, Germany.
  • Wang M; Max Planck Institute for Solar System Research, Göttingen, Germany.
Exp Astron (Dordr) ; 54(2-3): 713-744, 2022.
Article in En | MEDLINE | ID: mdl-36915624
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?What are the physical properties and internal structure of Ceres? What do they tell us about the evolutionary and aqueous alteration history of dwarf planets?What are the astrobiological implications of Ceres? Is it still habitable today?What are the mineralogical connections between Ceres and our current collections of carbonaceous meteorites?
Key words

Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: Exp Astron (Dordr) Year: 2022 Document type: Article Affiliation country: Germany

Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: Exp Astron (Dordr) Year: 2022 Document type: Article Affiliation country: Germany
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