Еще одна новая планета - KELT-2A b
Jun. 11th, 2012 04:41 pmKELT-2Ab: A Hot Jupiter Transiting the Bright (V=8.77) Primary Star of a Binary System
(Submitted on 7 Jun 2012)
We report the discovery of KELT-2Ab, a hot Jupiter transiting the bright (V=8.77) primary star of the HD 42176 binary system. The host is a slightly evolved late F-star likely in the very short-lived "blue-hook" stage of evolution, with $\teff=6151\pm50{\rm K}$, $\log{g_*}=4.030_{-0.028}^{+0.013}$ and $\feh=-0.018\pm0.069$. The inferred stellar mass is $M_*=1.308_{-0.025}^{+0.028}$\msun\ and the star has a relatively large radius of $R_*=1.828_{-0.034}^{+0.070}$\rsun. The planet is a typical hot Jupiter with period $4.113791\pm0.00001$ days and a mass of $M_P=1.522\pm0.078$\mj\ and radius of $R_P=1.286_{-0.047}^{+0.065}$\rj. This is mildly inflated as compared to models of irradiated giant planets at the $\sim$4 Gyr age of the system. KELT-2A is the third brightest star with a transiting planet identified by ground-based transit surveys, and the ninth brightest star overall with a transiting planet. KELT-2Ab's mass and radius are unique among the subset of planets with $V<9$ host stars, and therefore increases the diversity of bright benchmark systems. We also measure the relative motion of KELT-2A and -2B over a baseline of 38 years, robustly demonstrating for the first time that the stars are bound. This allows us to infer that KELT-2B is an early K dwarf. We hypothesize that through the eccentric Kozai mechanism KELT-2B may have emplaced KELT-2Ab in its current orbit. This scenario is potentially testable with Rossiter-McLaughlin measurements, which should have an amplitude of $\sim$44 m s$^{-1}$.
http://arxiv.org/abs/1206.1592
Planet : KELT-2A b
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| THE STAR |
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HD 42176
Созвездие:Возничий
Каталоги и обозначения:
Собственные (Edit)
имена:
HD 1989 HD 42176
TYCHO-2 2000 TYC 2420-899-1
USNO-A2.0 USNO-A2 1200-04436596
HIP HIP 29301
http://www.skymap2.sky-map.org/starview?object_type=1&object_id=570159&object_name=HD+42176