NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Science Goals and New Mission Concepts for Future Exploration of Titan’s Atmosphere, Geology and Habitability: Titan POlar Scout/orbitEr and in Situ Lake Lander and DrONe Explorer (POSEIDON)In response to ESA’s “Voyage 2050” announcement of opportunity, we propose an ambitious L-class mission to explore one of the most exciting bodies in the Solar System, Saturn’s largest moon Titan. Titan, a “world with two oceans”, is an organic-rich body with interior-surface-atmosphere interactions that are comparable in complexity to the Earth. Titan is also one of the few places in the Solar System with habitability potential. Titan’s remarkable nature was only partly revealed by the Cassini-Huygens mission and still holds mysteries requiring a complete exploration using a variety of vehicles and instruments. The proposed mission concept POSEI-DON (Titan POlar Scout/orbitEr and In situ lake lander DrONe explorer) would perform joint orbital and in situ investigations of Titan. It is designed to build on and exceed the scope and scientific/technological accomplishments of Cassini-Huygens, exploring Titan in ways that were not previously possible, in particular through full close-up and in situ coverage over long periods of time. In the proposed mission architecture, POSEIDON consists of two major elements: a spacecraft with a large set of instruments that would orbit Titan, preferably in a low-eccentricity polar orbit, and a suite of in situ investigation components, i.e. a lake lander, a “heavy” drone (possibly amphibious) and/or a fleet of mini-drones, dedicated to the exploration of the polar regions. The ideal arrival time at Titan would be slightly before the next northern Spring equinox (2039), as equinoxes are the most active periods to moni-tor still largely unknown atmospheric and surface seasonal changes. The exploration of Titan’s northern latitudes with an orbiter and in situ element(s) would be highly complementary in terms of timing (with possible mission timing overlap), locations, and science goals with the upcoming NASA New Frontiers Dragonfly mission that will provide in situ exploration of Titan’s equatorial regions, in the mid-2030s.
Document ID
20220005083
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Sebastien Rodriguez
(Paris Diderot University Paris, France)
Sandrine Vinatier
(Sorbonne University Paris, France)
Daniel Cordier
(University of Reims Champagne-Ardenne Reims, Champagne-Ardenne, France)
Gabriel Tobie
(University of Nantes Nantes, France)
Richard K Achterberg
(University of Maryland, College Park College Park, Maryland, United States)
Carrie M Anderson
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Murthy Satyanarayana Gudipati
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Ralph D Lorenz
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
Conor A Nixon
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Date Acquired
March 30, 2022
Publication Date
January 11, 2022
Publication Information
Publication: Experimental Astronomy
Publisher: Springer
Issue Publication Date: January 11, 2022
ISSN: 0922-6435
e-ISSN: 1572-9508
Subject Category
Astronomy
Funding Number(s)
WBS: 811073.02.55.01.12
CONTRACT_GRANT: 80NM0018D0004P00002
CONTRACT_GRANT: 80MSFC20F0146
CONTRACT_GRANT: 80GSFC21M0002
CONTRACT_GRANT: J-090011
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
No Preview Available