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Volumn 288, Issue 5469, 2000, Pages 1204-1208

Prometheus: Io's wandering plume

Author keywords

[No Author keywords available]

Indexed keywords

SULFUR DIOXIDE;

EID: 0034685999     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.288.5469.1204     Document Type: Article
Times cited : (75)

References (23)
  • 1
    • 0034685793 scopus 로고    scopus 로고
    • A. McEwen et al., Science 288, 1193 (2000).
    • (2000) Science , vol.288 , pp. 1193
    • McEwen, A.1
  • 3
    • 0001471362 scopus 로고    scopus 로고
    • A. McEwen et al., Icarus 135, 181 (1998).
    • (1998) Icarus , vol.135 , pp. 181
    • McEwen, A.1
  • 4
    • 0342355709 scopus 로고    scopus 로고
    • note
    • 3 and some other S-compounds can be ruled out as major components based on the spectral data in the literature.
  • 7
    • 85040847975 scopus 로고    scopus 로고
    • Springer-Verlag, Berlin
    • _ and H.-U. Schmincke, Pyroclastic Rocks (Springer-Verlag, Berlin, 1984), pp. 263-254.
    • Pyroclastic Rocks , vol.1984 , pp. 263-1254
    • Schmincke, H.-U.1
  • 12
    • 0343225306 scopus 로고    scopus 로고
    • note
    • If the lava flows in the western delta were thinner than 1 m, they could not produce the extensive sheet flows observed in the 124 and 127 SSI images (1). If they were much thicker than 100 m, shadowed scarps would be visible at the flow margins. Based on the interpretation that the Prometheus lavas are inflated pahoehoe (1), and observations of similar inflated flows in the same size range on Earth, we suggest that the thickness of warm lava in the Prometheus lava "delta" is likely to be a few tens of meters.
  • 13
    • 0343660934 scopus 로고    scopus 로고
    • note
    • We have based the density estimate on the assumption that the observed high temperatures for the lava flows (2) indicate a lava of mafic, that is, relatively dense, composition.
  • 14
    • 0003897291 scopus 로고
    • Dover, New York
    • -1. Under the fortuitous conditions considered here, the latent heat supplied by crystallization of the lava is almost exactly equal to the heat required for melting of the snow and the terms cancel in the conservation equations [M. Necati Ozisik, Boundary Value Problems of Heat Conduction (Dover, New York, 1968)]. Thermal conductivity could be appreciably lower if the lava is porous, or if temperatures are extremely high, perhaps by an order of magnitude. Lower values of thermal conductivity would extend the time scales calculated here.
    • (1968) Boundary Value Problems of Heat Conduction
    • Ozisik, M.N.1
  • 16
    • 0039825163 scopus 로고
    • D. Morrison, Ed. Univ. of Arizona Press, Tucson, AZ, fig. 18.5
    • S. W. Kieffer, in Satellites of Jupiter, D. Morrison, Ed. (Univ. of Arizona Press, Tucson, AZ, 1982), fig. 18.5, p. 17.
    • (1982) Satellites of Jupiter , pp. 17
    • Kieffer, S.W.1
  • 20
    • 0040417714 scopus 로고
    • D. Morrison, Ed. Univ. of Arizona Press, Tucson, AZ
    • T. V. Johnson and L. A. Soderblom, in Satellites of Jupiter, D. Morrison, Ed. (Univ. of Arizona Press, Tucson, AZ, 1982), chap. 17, p. 637.
    • (1982) Satellites of Jupiter , pp. 637
    • Johnson, T.V.1    Soderblom, L.A.2
  • 23
    • 0342790729 scopus 로고    scopus 로고
    • note
    • Portions of this work were performed at the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA. We also thank T. Johnson for pointing out that we had Prometheus bound if we had a mechanism to stop the motion of the plume.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.