메뉴 건너뛰기




Volumn 307, Issue 5706, 2005, Pages 71-75

The Kuiper belt and the solar system's comet disk

Author keywords

[No Author keywords available]

Indexed keywords

CLOUDS; PLANETS;

EID: 11844305930     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1100553     Document Type: Review
Times cited : (59)

References (35)
  • 3
    • 0001963429 scopus 로고    scopus 로고
    • V. Mannings, A. Boss, S. Russell, Eds. (Univ. Arizona Press, Tucson, AZ)
    • G. Wuchterl, T. Guillot, J. Lissauer, in Protostars and Planets IV, V. Mannings, A. Boss, S. Russell, Eds. (Univ. Arizona Press, Tucson, AZ, 2000), pp. 1081-1109.
    • (2000) Protostars and Planets IV , pp. 1081-1109
    • Wuchterl, G.1    Guillot, T.2    Lissauer, J.3
  • 4
    • 0032506537 scopus 로고    scopus 로고
    • B. Gladman, Nature 396, 513 (1998).
    • (1998) Nature , vol.396 , pp. 513
    • Gladman, B.1
  • 6
    • 11844269451 scopus 로고    scopus 로고
    • note
    • The semimajor axis is the average orbital distance (half the long axis of the elliptical orbit). Mean-motion resonances occur when the orbital period of the trans-neptunian object is near a fractional multiple of a planet. For example, objects near a = 39.4 AU may be in the 3:2 mean-motion resonance with Neptune; Pluto and the so-called plutino population are examples. The 2:1 resonance with Neptune at a = 48 currently marks the outer edge of known objects with low orbital eccentricity.
  • 17
    • 0036329391 scopus 로고    scopus 로고
    • B. Gladman et al., Icarus 157, 269 (2002).
    • (2002) Icarus , vol.157 , pp. 269
    • Gladman, B.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.