THEO Concept Mission: Testing the Habitability of Enceladus's Ocean
Shannon M. MacKenzie, Tess E. Caswell, Charity M. Phillips-Lander, E., Natasha Stavros, Jason D. Hofgartner, Vivian Z. Sun, Kathryn E. Powell, Casey, J. Steuer, Joesph G. O'Rourke, Jasmeet K. Dhaliwal, Cecilia W. S. Leung,, Elaine M. Petro, J. Judson Wynne, Samson Phan

TL;DR
The paper proposes a solar-powered orbiter mission, THEO, to analyze Enceladus's plumes and subsurface ocean for habitability indicators using remote sensing and in situ instruments, addressing key questions about its potential to support life.
Contribution
It introduces the THEO mission concept, combining remote sensing and in situ analysis to assess Enceladus's habitability, developed by student participants under JPL guidance.
Findings
Instrument suite can address key habitability questions.
Mission concept demonstrates feasibility for outer solar system exploration.
Potential to detect signs of biological processes.
Abstract
Saturn's moon Enceladus offers a unique opportunity in the search for life and habitable environments beyond Earth, a key theme of the National Research Council's 2013-2022 Decadal Survey. A plume of water vapor and ice spews from Enceladus's south polar region. Cassini data suggest that this plume, sourced by a liquid reservoir beneath the moon's icy crust, contain organics, salts, and water-rock interaction derivatives. Thus, the ingredients for life as we know it-- liquid water, chemistry, and energy sources-- are available in Enceladus's subsurface ocean. We have only to sample the plumes to investigate this hidden ocean environment. We present a New Frontiers class, solar-powered Enceladus orbiter that would take advantage of this opportunity, Testing the Habitability of Enceladus's Ocean (THEO). Developed by the 2015 Jet Propulsion Laboratory Planetary Science Summer School…
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