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8
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-
34547812247
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Mimas' 7:6 inner Lindblad resonance also lies nearby at 445.411°/day (a = 167,511 km).
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Mimas' 7:6 inner Lindblad resonance also lies nearby at 445.411°/day (a = 167,511 km).
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10
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-
0000210932
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C. C. Porco, Science 253, 995 (1991).
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(1991)
Science
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Porco, C.C.1
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14
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33644853764
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G. H. Jones et al., Science 311, 1412 (2006).
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(2006)
Science
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Jones, G.H.1
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17
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0012550293
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E. Grün, B. Gustafson, S. Dermott, H. Fecthig, Eds, Springer, New York
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J. A. Burns, D. P. Hamilton, M. R. Showalter, in Interplanetary Dust, E. Grün, B. Gustafson, S. Dermott, H. Fecthig, Eds. (Springer, New York, 2001), pp. 641-725.
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(2001)
Interplanetary Dust
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Burns, J.A.1
Hamilton, D.P.2
Showalter, M.R.3
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18
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34547793261
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Slight deviations from an exponential profile occur around 168,200 and 169,800 km. The latter feature shows longitudinal structure and is probably associated with the Mimas 8:7 inner Lindblad resonance.
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Slight deviations from an exponential profile occur around 168,200 and 169,800 km. The latter feature shows longitudinal structure and is probably associated with the Mimas 8:7 inner Lindblad resonance.
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20
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0002596394
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R. Greenberg, A. Brahic, Eds, Univ. of Arizona Press, Tucson, AZ
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J. A. Burns, M. R. Showalter, G. E. Morfill, in Planetary Rings, R. Greenberg, A. Brahic, Eds. (Univ. of Arizona Press, Tucson, AZ, 1984), pp. 200-272.
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(1984)
Planetary Rings
, pp. 200-272
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-
Burns, J.A.1
Showalter, M.R.2
Morfill, G.E.3
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21
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34247488340
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D. Gurnett et al., Science 316, 442 (2007).
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(2007)
Science
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Gurnett, D.1
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22
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34547783649
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We thank the staff at the Space Science Institute, Jet Propulsion Laboratory, and Cornell University for planning and delivering the imaging data, and M. Kusterer of the Johns Hopkins University Applied Physics Laboratory (JHUAPL) for LEMMS data reduction. We also acknowledge the support of the Cassini Project and NASA's Planetary Geology & Geophysics program. MIMI/LEMMS was in part financed by the German Bundesministerium für Bildung und Forschung through the German Aerospace Center (DLR) under contract 50 OH 0103 and by the Max Planck Gesellschaft. The work at JHUAPL was supported by NASA under contract NAS5-97271 with the Johns Hopkins University. G.H.J. was partially supported by the Science and Technology Facilities Council, UK
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We thank the staff at the Space Science Institute, Jet Propulsion Laboratory, and Cornell University for planning and delivering the imaging data, and M. Kusterer of the Johns Hopkins University Applied Physics Laboratory (JHUAPL) for LEMMS data reduction. We also acknowledge the support of the Cassini Project and NASA's Planetary Geology & Geophysics program. MIMI/LEMMS was in part financed by the German Bundesministerium für Bildung und Forschung through the German Aerospace Center (DLR) under contract 50 OH 0103 and by the Max Planck Gesellschaft. The work at JHUAPL was supported by NASA under contract NAS5-97271 with the Johns Hopkins University. G.H.J. was partially supported by the Science and Technology Facilities Council, UK.
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