WASP-5 b:一颗致密的、非常热的木星,正穿过一颗南半球的12等恒星。
WASP-5b: a dense, very-hot Jupiter transiting a 12th-mag Southern-hemisphere star
摘要:
我们报告发现了WASP-5 b,这是一颗质量为100亿的行星,在南半球绕着一颗12等G型恒星运行。1.6-d的轨道周期将WASP-5 b置于极热的类星体中,并导致预测的平衡温度为1750 K。WASP-5 b是所有已知木星质量行星的密度,比受到类似恒星日照的TrES-4密度高7倍,比轨道周期类似的WASP-4 b密度高3倍。我们介绍了WASP-5的凌日测光和径向速度测量(= USNO-B1 0487-0799749),从中我们得出了行星的质量,半径和密度:M_P = 1.58 + 0.13 - 0.08 M_J,R_P = 1.090 + 0.094 - 0.058 R_J,Rho_P = 1.22 + 0.19 - 0.24 Rho_J。凌日时刻T_C(HJD)= 2454375.62466 + 0.00026 - 0.00025。
英文摘要:
We report the discovery of WASP-5b, a Jupiter-mass planet orbiting a 12th-mag G-type star in the Southern hemisphere. The 1.6-d orbital period places WASP-5b in the class of very-hot Jupiters and leads to a predicted equilibrium temperature of 1750 K. WASP-5b is the densest of any known Jovian-mass planet, being a factor seven denser than TrES-4, which is subject to similar stellar insolation, and a factor three denser than WASP-4b, which has a similar orbital period. We present transit photometry and radial-velocity measurements of WASP-5 (= USNO-B1 0487-0799749), from which we derive the mass, radius and density of the planet: M_P = 1.58 +0.13 -0.08 M_J, R_P = 1.090 +0.094 -0.058 R_J and Rho_P = 1.22 +0.19 -0.24 Rho_J. The orbital period is P = 1.6284296 +0.0000048 -0.0000037 d and the mid-transit epoch is T_C (HJD) = 2454375.62466 +0.00026 -0.00025.
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