DocumentCode :
2067145
Title :
Preparing for a future in situ mission to Titan
Author :
Reh, Kim R. ; Elliott, John
Author_Institution :
Jet Propulsion Lab., California Inst. of Technol., Pasadena, CA, USA
fYear :
2010
fDate :
6-13 March 2010
Firstpage :
1
Lastpage :
9
Abstract :
It is becoming clear that any future mission to Titan will require the delivery and support of in situ elements to address high priority science questions raised by both the Cassini-Huygens mission and the international science community participating in recent NASA-ESA mission studies. The most recent studies have specifically identified the Montgolfie¿re hot air balloon (Titan´s rover) and lake lander as providing the highest value science return for future missions to Titan. Furthermore, results from science, technical, and management review of recent studies have focused current technical efforts on key areas for increasing the readiness of these in situ elements for launch. The purpose of this paper is to provide a technical overview of the Titan Saturn System Mission (TSSM) architecture and its elements and the progress and plans toward reducing risk and increasing readiness.
Keywords :
Saturn; planetary atmospheres; planetary rovers; planetary satellites; planetary surfaces; Cassini-Huygens mission follow-on; Saturnian satellite; Titan Saturn System Mission; Titan rover; in situ measurements; montgolfiere hot air balloon; Biographies; Chemistry; Gravity; Laboratories; Lakes; Magnetosphere; Propulsion; Robustness; Saturn; Space vehicles;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Aerospace Conference, 2010 IEEE
Conference_Location :
Big Sky, MT
ISSN :
1095-323X
Print_ISBN :
978-1-4244-3887-7
Electronic_ISBN :
1095-323X
Type :
conf
DOI :
10.1109/AERO.2010.5446977
Filename :
5446977
Link To Document :
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