메뉴 건너뛰기




Volumn 156, Issue 1, 2002, Pages 152-161

A melt-through model for chaos formation on Europa

Author keywords

Europa; Satellites; Satellites of Jupiter; Surfaces; Thermal histories

Indexed keywords


EID: 0036264793     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1006/icar.2001.6777     Document Type: Article
Times cited : (108)

References (28)
  • 5
    • 0003559368 scopus 로고
    • Properties of Ordinary Water-Substance in all its Phases: Water-Vapor, Water, and all the Ices
    • Reinhold, New York
    • (1940)
    • Dorsey, N.E.1
  • 7
    • 0039572480 scopus 로고    scopus 로고
    • Europa: Initial Galileo geological observations
    • and 20 colleagues
    • (1998) Icarus , vol.135 , pp. 4-24
    • Greeley, R.1
  • 11
    • 0033499760 scopus 로고    scopus 로고
    • Brine mobilization during lithospheric heating on Europa: Implications for formation of chaos terrain, lenticulae texture, and color variations
    • (1999) J. Geophys. Res , vol.104 , pp. 27143-27155
    • Head, J.W.1    Pappalardo, R.T.2
  • 18
    • 0033604183 scopus 로고    scopus 로고
    • Does Europa have a subsurface ocean? Evaluation of the geological evidence
    • and 31 colleagues
    • (1999) J. Geophys. Res , vol.104 , pp. 24015-24056
    • Pappalardo, R.T.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.