z-logo
open-access-imgOpen Access
Science Drivers for the Future Exploration of Ceres: From Solar System Evolution to Ocean World Science
Author(s) -
Julie CastilloRogez,
Marc Neveu,
Vassilissa Vinogradoff,
Kelly E. Miller,
Michael M. Sori,
F. Tosi,
B. E. Schmidt,
J. E. C. Scully,
Mohit Melwani Daswani,
K. Hughson,
H. Y. McSween,
M. C. De Sanctis,
L. C. Quick,
A. Ermakov,
G. Thangjam,
Katharina A. Otto,
Katrin Krohn,
P. Schenk,
A. Nathues,
C. A. Raymond
Publication year - 2022
Publication title -
the planetary science journal
Language(s) - English
Resource type - Journals
ISSN - 2632-3338
DOI - 10.3847/psj/ac502b
Subject(s) - astrobiology , planet , solar system , earth science , geology , brine , planetary science , oceanography , geography , astronomy , physics , thermodynamics
Dawn revealed that Ceres is a compelling target whose exploration pertains to many science themes. Ceres is a large ice- and organic-rich body, potentially representative of the population of objects that brought water and organics to the inner solar system, as well as a brine-rich body whose study can contribute to ocean world science. The Dawn observations have led to a renewed focus on planetary brine physics and chemistry based on the detection of many landforms built from brines or suspected to be emplaced via brine effusion. Ceres’ relative proximity to Earth and direct access to its surface of evaporites that evolved from a deep brine reservoir make this dwarf planet an appealing target for follow-up exploration. Future exploration, as described here, would address science questions pertinent to the evolution of ocean worlds and the origin of volatiles and organics in the inner solar system.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom