首页    期刊浏览 2024年12月12日 星期四
登录注册

文章基本信息

  • 标题:TESS Observations of the Hot Jupiter Exoplanet XO-6b: No Evidence of Transit Timing Variations
  • 本地全文:下载
  • 作者:Andrew Ridden-Harper ; Jake D.Turner ; Ray Jayawardhana
  • 期刊名称:The Astronomical journal
  • 印刷版ISSN:0004-6256
  • 电子版ISSN:1538-3881
  • 出版年度:2020
  • 卷号:160
  • 期号:6
  • 页码:1-12
  • DOI:10.3847/1538-3881/abba1e
  • 语种:English
  • 出版社:American Institute of Physics
  • 摘要:From previous ground-based observations, the hot Jupiter exoplanet XO-6b was reported to exhibit apparently periodic transit timing variations (TTVs), with a semi-amplitude of 14 minutes and a period of about 450 days. These variations were interpreted as being due to a resonant perturbation between XO-6b and a hitherto unknown low-mass planet orbiting the same star. To understand this enigmatic planetary system better, we analyzed three sectors of data, spanning over seven months, from the Transiting Exoplanet Survey Satellite (TESS), which produces high-quality light curves that are well suited to characterizing exoplanets and searching for TTVs. Here we present an updated orbital period of 3.7649893 ± 0.0000037 days and a transit epoch of 2456652.7157 ± 0.0022 BJDTDB. The planetary parameters we report, while consistent with their discovery values, have greatly improved precision. Notably, we find no evidence for TTVs: we can rule out TTVs ≳2.5 minutes at the 3σ level. Therefore, the TESS data have sufficient precision and time baseline to readily reveal the previously reported TTVs of approximately 10 minutes. Our findings highlight the capability of TESS for robust follow-up, and confirm that TTVs are rarely seen in hot Jupiters, unlike is the case with small planets.
国家哲学社会科学文献中心版权所有