首页    期刊浏览 2024年11月30日 星期六
登录注册

文章基本信息

  • 标题:The Aligned Orbit of the Eccentric Warm Jupiter K2-232b
  • 本地全文:下载
  • 作者:Songhu Wang ; Joshua N.Winn ; Brett C.Addison
  • 期刊名称:The Astronomical journal
  • 印刷版ISSN:0004-6256
  • 电子版ISSN:1538-3881
  • 出版年度:2021
  • 卷号:162
  • 期号:2
  • 页码:1-6
  • DOI:10.3847/1538-3881/ac0626
  • 语种:English
  • 出版社:American Institute of Physics
  • 摘要:Measuring the obliquity distribution of stars hosting warm Jupiters may help us to understand the formation of close-orbiting gas giants. Few such measurements have been performed due to practical difficulties in scheduling observations of the relatively infrequent and long-duration transits of warm Jupiters. Here, we report a measurement of the Rossiter–McLaughlin effect for K2-232 b, a warm Jupiter on an 11.17 day orbit with an eccentricity of 0.26. The data were obtained with the Automated Planet Finder during two separate transits. The planet's orbit appears to be well aligned with the spin axis of the host star, with a projected spin–orbit angle of λ = −111 ± 66. Combined with the other available data, we find that high obliquities are almost exclusively associated with planets that either have an orbital separation greater than 10 stellar radii or orbit stars with effective temperatures hotter than 6000 K. This pattern suggests that the obliquities of the closest-orbiting giant planets around cooler stars have been damped by tidal effects.
国家哲学社会科学文献中心版权所有