GAUSS - genesis of asteroids and evolution of the solar system View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2021-10-15

AUTHORS

Xian Shi, Julie Castillo-Rogez, Henry Hsieh, Hejiu Hui, Wing-Huen Ip, Hanlun Lei, Jian-Yang Li, Federico Tosi, Liyong Zhou, Jessica Agarwal, Antonella Barucci, Pierre Beck, Adriano Campo Bagatin, Fabrizio Capaccioni, Andrew J. Coates, Gabriele Cremonese, Rene Duffard, Manuel Grande, Ralf Jaumann, Geraint H. Jones, Esa Kallio, Yangting Lin, Olivier Mousis, Andreas Nathues, Jürgen Oberst, Holger Sierks, Stephan Ulamec, Mingyuan Wang,

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? More... »

PAGES

1-32

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  • Journal

    TITLE

    Experimental Astronomy

    ISSUE

    N/A

    VOLUME

    N/A

    Author Affiliations

  • Shanghai Astronomical Observatory, Shanghai, China
  • NASA Jet Propulsion Laboratory, La Cañada Flintridge, CA, USA
  • Planetary Science Institute, Tucson, AZ, USA
  • School of Earth Sciences and Engineering, Nanjing University, Nanjing, China
  • Institute of Astronomy and Space Science, National Central University, Chung Li, Taiwan
  • School of Astronomy and Space Science, Nanjing University, Nanjing, China
  • Istituto Nazionale di AstroFisica – Istituto di Astrofisica e Planetologia Spaziali (INAF-IAPS), Rome, Italy
  • Institute for Geophysics and Extraterrestrial Physics, Technical University Braunschweig, Braunschweig, Germany
  • LESIA-Observatoire de Paris, Université PSL, CNRS, Université de Paris, Sorbonne Université, Principal Cedex, F-92195, Meudon, France
  • CNRS Institut de Planétologie et d’Astrophysique, Univ. Grenoble Alpes, Grenoble, France
  • Universidad de Alicante, Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Alicante, Spain
  • Mullard Space Science Laboratory, University College London, Surrey, UK
  • INAF - Osservatorio Astronomico di Padova, Padova, Italy
  • Instituto de Astrofísica de Andalucía (CSIC), Granada, Spain
  • University of Aberystwyth, Aberystwyth, UK
  • Institute of Geological Sciences, Free University of Berlin, Berlin, Germany
  • School of Electrical Engineering, Aalto University, Aalto, Finland
  • Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China
  • Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France
  • Max Planck Institute for Solar System Research, Göttingen, Germany
  • DLR Institute of Planetary Research, Berlin, Germany
  • DLR Space Operations and Astronaut Training, Cologne, Germany
  • National Astronomical Observatory, Chinese Academy of Science, Beijing, China
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/s10686-021-09800-1

    DOI

    http://dx.doi.org/10.1007/s10686-021-09800-1

    DIMENSIONS

    https://app.dimensions.ai/details/publication/pub.1141917035


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