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Volumn 336, Issue 6085, 2012, Pages 1133-1136

The detection and characterization of a nontransiting planet by transit timing variations

Author keywords

[No Author keywords available]

Indexed keywords

COSMOLOGY; DATA SET; DETECTION METHOD; EXTRATERRESTRIAL MATTER; NUMERICAL MODEL; PLANETARY SURFACE; SATELLITE MISSION; SOLAR SYSTEM;

EID: 84861683536     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1221141     Document Type: Article
Times cited : (135)

References (27)
  • 10
    • 2142803437 scopus 로고    scopus 로고
    • Materials and methods are available as supplementary materials on
    • Materials and methods are available as supplementary materials on Science Online.
    • Science Online
  • 19
    • 84889731935 scopus 로고    scopus 로고
    • note
    • We also tested the possibility of planets in the 1:1 mean motion resonance. We used an N-body integrator in this case, because perturbation theory described in (18) is not convergent for crossing orbits.
  • 21
    • 84889745398 scopus 로고    scopus 로고
    • note
    • c < 5° and were inconsistent with the observed TTVs.
  • 22
    • 84889693029 scopus 로고    scopus 로고
    • note
    • We attempted to fit the observed TTVs with a three-planet system. The obtained solutions recovered the two-planet case corresponding to s1 or s2, with the third planet being either too small or too distant to produce significant TTVs.
  • 24
    • 77957371829 scopus 로고    scopus 로고
    • M. J. Holman et al., Science 330, 51 (2010).
    • (2010) Science , vol.330 , pp. 51
    • Holman, M.J.1
  • 25
    • 79551658020 scopus 로고    scopus 로고
    • J. J. Lissauer et al., Nature 470, 53 (2011b).
    • (2011) Nature , vol.470 , pp. 53
    • Lissauer, J.J.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.