Published March 12, 2024
| Version 1.0.2
Dataset
Open
Spherical harmonic models of the gravity field of Enceladus
Description
This archive contains previously published models of the gravitational field of Saturn's moon Enceladus.
- Iess2014.sh (SOL1)
- Park2024.sh (Case 2)
All models make use of unnormalized spherical harmonic functions that exclude the Condon-Shortley phase factor of (-1)^m.
Files
Files
(665 Bytes)
| Name | Size | Download all |
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md5:3a093a42b9e53c52ce0530add0cf15fd
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326 Bytes | Download |
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md5:f57df986866354ae92fd3538df7f6105
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339 Bytes | Download |
Additional details
Related works
- Is documented by
- Publication: 10.1029/2023JE008054 (DOI)
- Publication: 10.1126/science.1250551 (DOI)
Dates
- Available
-
2024-03-11
References
- Park, R. S., Mastrodemos, N., Jacobson, R. A., Berne, A., Vaughan, A. T., Hemingway, D. J., Leonard, E. J., Castillo-Rogez, J. C., Cockell, C. S., Keane, J. T., Konopliv, A. S., Nimmo, F., Riedel, J. E., Simons, M., & Vance, S. (2024). The Global Shape, Gravity Field, and Libration of Enceladus. Journal of Geophysical Research: Planets, 129(1), e2023JE008054. https://doi.org/10.1029/2023JE008054
- Iess, L., Stevenson, D. J., Parisi, M., Hemingway, D., Jacobson, R. A., Lunine, J. I., Nimmo, F., Armstrong, J. W., Asmar, S. W., Ducci, M., & Tortora, P. (2014). The Gravity Field and Interior Structure of Enceladus. Science, 344(6179), 78–80. https://doi.org/10.1126/science.1250551