Planetary science decadal survey planetary mission concept study report: Ceres: Exploration of Ceres’ habitability

Cooperator Report
By: , and 
Edited by: Timothy N. Titus

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Abstract

Dwarf planet Ceres is a compelling target as an evolved ocean world with, at least, regional brine reservoirs and potentially ongoing geological activity. As the most water-rich body in the inner solar system (in relative abundance), it is a representative of the population of planetesimals that brought volatiles and organics to the inner solar system. Situated in the Main Belt of asteroids, Ceres is accessible enough for a sample return with the resources of a typical medium-class (New Frontiers) NASA mission. Under the Discovery program, Dawn explored Ceres from 2015 to 2018. The extensive dataset revealed the presence of liquid, brine-driven activity, organic matter, and a rich salt chemistry. With this evidence, the overarching goals of the mission concept presented herein are to quantify Ceres’ current habitability potential and origin.

Suggested Citation

Castillo-Rogez, J.C., Brody, J., Bland, M.T., Buczkowski, D., Grimm, R., Hendrix, A., Miller, K., Prettyman, T., Quick, L., Raymond, C., Scully, J., Sori, M.M., Sekine, Y., Williams, D., Zolensky, M., 2020, Planetary science decadal survey planetary mission concept study report: Ceres: Exploration of Ceres’ habitability: Cooperator Report, 360 p.

Publication type Report
Publication Subtype Federal Government Series
Title Planetary science decadal survey planetary mission concept study report: Ceres: Exploration of Ceres’ habitability
Series title Cooperator Report
Year Published 2020
Language English
Publisher NASA
Contributing office(s) Astrogeology Science Center
Description 360 p.
Other Geospatial Ceres
Additional publication details