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Volumn 317, Issue 5838, 2007, Pages 653-656

The source of Saturn's G ring

Author keywords

[No Author keywords available]

Indexed keywords

COLLISION; RESONANCE; SATURN; SPACECRAFT;

EID: 34547792488     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1143964     Document Type: Article
Times cited : (68)

References (22)
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    • Mimas' 7:6 inner Lindblad resonance also lies nearby at 445.411°/day (a = 167,511 km).
    • Mimas' 7:6 inner Lindblad resonance also lies nearby at 445.411°/day (a = 167,511 km).
  • 10
  • 14
    • 33644853764 scopus 로고    scopus 로고
    • G. H. Jones et al., Science 311, 1412 (2006).
    • (2006) Science , vol.311 , pp. 1412
    • Jones, G.H.1
  • 17
    • 0012550293 scopus 로고    scopus 로고
    • E. Grün, B. Gustafson, S. Dermott, H. Fecthig, Eds, Springer, New York
    • 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.
    • (2001) Interplanetary Dust , pp. 641-725
    • Burns, J.A.1    Hamilton, D.P.2    Showalter, M.R.3
  • 18
    • 34547793261 scopus 로고    scopus 로고
    • 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.
    • 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.
  • 20
    • 0002596394 scopus 로고
    • R. Greenberg, A. Brahic, Eds, Univ. of Arizona Press, Tucson, AZ
    • 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.
    • (1984) Planetary Rings , pp. 200-272
    • Burns, J.A.1    Showalter, M.R.2    Morfill, G.E.3
  • 21
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    • D. Gurnett et al., Science 316, 442 (2007).
    • (2007) Science , vol.316 , pp. 442
    • Gurnett, D.1
  • 22
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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
    • 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.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.