HAT-P-50b - Wikipedia
HAT-P-50b is an exoplanet orbiting HAT-P-50 star located in the Gemini constellation. [1] [2] It was discovered in 2015. [3]
HAT-P-50 b - Science@NASA
2024年10月24日 · HAT-P-50 b is a gas giant exoplanet that orbits a F-type star. Its mass is 1.35 Jupiters, it takes 3.1 days to complete one orbit of its star, and is 0.0453 AU from its star. Its discovery was announced in 2015.
HAT-P-50 | NASA Exoplanet Archive
Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets.
[1503.04149] HAT-P-50b, HAT-P-51b, HAT-P-52b, and HAT-P …
2015年3月13日 · We report the discovery and characterization of four transiting exoplanets by the HATNet survey. The planet HAT-P-50b has a mass of 1.35 M_J and a radius of 1.29 R_J, and orbits a bright (V = 11.8...
HAT-P-50b, HAT-P-51b, HAT-P-52b, and HAT-P-53b: Three …
The low stellar jitter and favorable {R} p /{R} \star ratio for HAT-P-51 make it a promising target for measuring the Rossiter-McLaughlin effect for a Saturn-mass planet. Based on observations obtained with the Hungarian-made Automated Telescope Network.
HAT-P-50b, HAT-P-51b, HAT-P-52b, AND HAT-P-53b: THREE …
2015年11月4日 · In this paper we presented the discovery and characterization of four TEPs from the HATNet survey, including three hot Jupiters (HAT-P-50b, HAT-P-52b and HAT-P-53b) and a hot Saturn (HAT-P-51b). All four planets have masses and …
HAT-P-50b, HAT-P-51b, HAT-P-52b, AND HAT-P-53b: THREE …
We report the discovery and characterization of four transiting exoplanets by the HATNet survey. The planet HAT-P-50b has a mass of 1.35 M-J and radius of 1.29 R-J, and orbits a bright (V = 11.8 mag) M = 1.27 M-circle dot, R = 1.70 R-circle dot star every P = 3.1220 days. The planet HAT-P-51b has a mass of 0.31 M-J and radius of 1.29 R-J, and orbits a V = 13.4 mag, M = 0.98 M-circle dot, R = 1 ...
HAT-P-50b, HAT-P-51b, HAT-P-52b, and HAT-P-53b: Three …
All four planets are consistent with having circular orbits and have masses and radii measured to better than 10% precision. The low stellar jitter and favorable {R} p / {R} \star ratio for HAT-P …
(PDF) HAT-P-50b, HAT-P-51b, HAT-P-52b, and HAT-P-53b
2015年3月13日 · We report the discovery and characterization of four transiting exoplanets by the HATNet survey. The planet HAT-P-50b has a mass of 1.35 M_J and a radius of 1.29 R_J, and orbits a bright (V =...
p/R ratio for HAT-P-51 make it a promising target for measuring the Rossiter–McLaughlin effect for a Saturn-mass planet. Key words: planetary systems – stars: individual (HAT-P-50, HAT-P-51, HAT-P-52, HAT-P-53) – techniques: photometric – techniques: spectroscopic Supporting material: machine-readable and VO table 1. INTRODUCTION
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