THEO

THEO (Testing the Habitability of Enceladus's Ocean) is a feasibility study for a New Frontiers class orbiter mission to Enceladus that would directly sample its south pole water plumes in order to study its internal habitability and to search for biosignatures. Specifically, it would take advantage of the direct sampling opportunities of a subsurface ocean.

The study concept was produced by the 2015 Jet Propulsion Laboratory Planetary Science Summer School under the guidance of TeamX. The study has not yet been formally proposed for funding.

Mission concept
A plume of water vapor and ice spews from Enceladus's south polar region, offering a unique opportunity for a low-cost mission in the search for life and habitable environments beyond Earth. The THEO mission would further understanding of life and habitability in our solar system by addressing (i) the limits of life under colder, fainter Sun conditions, (ii) the importance of hydrothermal alteration in the origin of life, and (iii) the distribution of molecules in the Solar System that may have served as the precursors for life.

The Cassini mission 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 are available in Enceladus's subsurface ocean.

The THEO mission would primarily focus on whether Enceladus is habitable. It would not look for life forms directly, but for higher abundances of certain molecules, ratios of organic compounds, or chains of amino acids could all be biosignatures that all give away the presence of life.

Mission design
The trajectory of THEO would obtain the needed kinetic energy with one Venus and two Earth gravity assists. THEO would reduce its velocity (delta-v) by making flybys of Saturn moons Titan, Rhea, Dione, Tethys, and Enceladus before the Enceladus orbit insertion. The data would be collected from three orbital attitudes (500 km, 100 km, 30 km) with each representing a separate mission phase. More than 600 science orbits are expected over the span of nominal six-month mission. At the end of the mission, and according to planetary protection protocols, the orbiter will be sent on an impact trajectory to Tethys, where it will be discarded.

Proposed payload
This mission concept includes remote sensing and in situ analyses with: These instruments (total mass ≈80 kg) were selected to address four key questions for ascertaining the habitability of Enceladus's ocean within the context of the moon's geological activity:
 * a mass spectrometer (SWAMP)
 * a sub-mm radiometer-spectrometer (WAVES)
 * a camera (DRIPS)
 * a magnetometer (OSMOSIS)
 * doppler tracking (GEISER)
 * 1) How are the plumes and ocean connected?
 * 2) Are the abiotic conditions of the ocean suitable for habitability?
 * 3) How stable is the ocean environment?
 * 4) Is there evidence of biological processes?