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