Published September 2019
| Published
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Detection of rapid orbital expansion of Saturn's moon Titan
Abstract
The Saturn satellite system is a complex dynamical system with several gravitational interactions happening between the satellites, the rings and the central body, such as resonances, librations and tides. These intricate dynamics carry information on the formation and evolution of the Saturn and Solar systems.
Additional Information
© Author(s) 2019. CC Attribution 4.0 license. V.L.'s research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. This work has been supported by the ENCELADE team of the International Space Science Institute (ISSI). Support for this work was provided by the Italian Space Agency (LGC, MZ, PT, and DM) through the Agreement 2017-10-H.O in the context of the NASA/ESA/ASI Cassini/Huygens mission. JF's research is funded in part by a Rose Hills Innovator Grant. N.C. and C.M. were supported by the UK Science and Technology Facilities Council (Grant No. ST/M001202/1) and are grateful to them for financial assistance. N.C. thanks the Scientific Council of the Paris Observatory for funding. Q.Z.'s research was supported by the National Natural Science Foundation of China (Grant No. 11873026).Attached Files
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Additional details
- Eprint ID
- 103507
- Resolver ID
- CaltechAUTHORS:20200528-071119369
- NASA/JPL/Caltech
- International Space Science Institute (ISSI)
- Agenzia Spaziale Italiana (ASI)
- 2017-10-H.O
- Rose Hills Foundation
- Science and Technology Facilities Council (STFC)
- ST/M001202/1
- Paris Observatory
- National Natural Science Foundation of China
- 11873026
- Created
-
2020-05-28Created from EPrint's datestamp field
- Updated
-
2020-06-08Created from EPrint's last_modified field
- Caltech groups
- TAPIR, Walter Burke Institute for Theoretical Physics, Astronomy Department
- Series Name
- EPSC Abstracts
- Series Volume or Issue Number
- 13