dc.contributor.author
Rodriguez, Sébastien
dc.contributor.author
Vinatier, Sandrine
dc.contributor.author
Cordier, Daniel
dc.contributor.author
Tobie, Gabriel
dc.contributor.author
Achterberg, Richard K.
dc.contributor.author
Anderson, Carrie M.
dc.contributor.author
Badman, Sarah V.
dc.contributor.author
Barnes, Jason W.
dc.contributor.author
Barth, Erika L.
dc.contributor.author
Jaumann, Ralf
dc.date.accessioned
2023-04-11T11:04:41Z
dc.date.available
2023-04-11T11:04:41Z
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/33935
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-33654
dc.description.abstract
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 POSEIDON (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 monitor 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.
en
dc.format.extent
63 Seiten
dc.rights.uri
https://creativecommons.org/licenses/by/4.0/
dc.subject
Habitability
en
dc.subject.ddc
500 Naturwissenschaften und Mathematik::520 Astronomie::520 Astronomie und zugeordnete Wissenschaften
dc.title
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)
dc.type
Wissenschaftlicher Artikel
dcterms.bibliographicCitation.doi
10.1007/s10686-021-09815-8
dcterms.bibliographicCitation.journaltitle
Experimental Astronomy
dcterms.bibliographicCitation.number
2-3
dcterms.bibliographicCitation.pagestart
911
dcterms.bibliographicCitation.pageend
973
dcterms.bibliographicCitation.volume
54
dcterms.bibliographicCitation.url
https://doi.org/10.1007/s10686-021-09815-8
refubium.affiliation
Geowissenschaften
refubium.affiliation.other
Institut für Geologische Wissenschaften / Fachrichtung Planetologie und Fernerkundung
refubium.resourceType.isindependentpub
no
dcterms.accessRights.openaire
open access
dcterms.isPartOf.eissn
1572-9508
refubium.resourceType.provider
WoS-Alert