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Volumn 155, Issue 2, 2002, Pages 375-381

High-resolution 0.33-0.92 μm spectra of Iapetus, Hyperion, Phoebe, Rhea, Dione, and D-type asteroids: How are they related?

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Indexed keywords


EID: 0036109557     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1006/icar.2001.6730     Document Type: Article
Times cited : (51)

References (52)
  • 5
    • 0007392913 scopus 로고
    • Voyager disk resolved photometry of the saturnian satellites
    • (1984) Icarus , vol.59 , pp. 392-405
    • Buratti, B.J.1
  • 13
    • 49149149125 scopus 로고
    • Near-infrared studies of the satellites of Saturm and Uranus
    • (1980) Icarus , vol.41 , pp. 246-258
    • Cruikshank, D.P.1
  • 19
    • 0035849853 scopus 로고    scopus 로고
    • Orbital clustering for twelve newly-discovered saturnian satellites: Clues to their origin
    • and 10 colleagues
    • (2001) Nature , vol.412 , pp. 163-166
    • Gladman, B.1
  • 36
    • 0006145450 scopus 로고
    • An explanation for Iapetus' asymmetric reflectance
    • (1975) Icarus , vol.24 , pp. 499-503
    • Peterson, C.1
  • 38
    • 0040186657 scopus 로고
    • A new look at the Saturn System: The Voyager 2 images
    • and 28 colleagues
    • (1982) Science , vol.215 , pp. 504-536
    • Smith, B.A.1
  • 46
    • 0000275110 scopus 로고
    • Reflectance spectrophotometry (about 0.5 to 1.0 micron) of outer-belt asteroids: Implications for primitive, organic Solar System material
    • (1985) Icarus , vol.64 , pp. 503-516
    • Vilas, F.1    Smith, B.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.