HATS-6b: A WARM SATURN TRANSITING AN EARLY M DWARF STAR, AND A SET OF EMPIRICAL RELATIONS FOR CHARACTERIZING K AND M DWARF PLANET HOSTS
We report the discovery by the HATSouth survey of HATS-6b, an extrasolar planet transiting a V = 15.2 mag, i = 13.7 mag M1V star with a mass of 0.57 M sub([middot in circle]) and a radius of 0.57 R sub([middot in circle]). HATS-6b has a period of P = 3.3253 d, mass of M sub(p) = 0.32 M sub(J) , radi...
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creator | Hartman, J D Bayliss, D Brahm, R Bakos, G A Mancini, L Jordan, A Penev, K Rabus, M Zhou, G Butler, R P |
description | We report the discovery by the HATSouth survey of HATS-6b, an extrasolar planet transiting a V = 15.2 mag, i = 13.7 mag M1V star with a mass of 0.57 M sub([middot in circle]) and a radius of 0.57 R sub([middot in circle]). HATS-6b has a period of P = 3.3253 d, mass of M sub(p) = 0.32 M sub(J) , radius of R sub(p) = 1.00 R sub(J) , and zero-albedo equilibrium temperature of T sub(eq) = 712.8 + or - 5.1 K. HATS-6 is one of the lowest mass stars known to host a close-in gas giant planet, and its transits are among the deepest of any known transiting planet system. We show that from the transit-based stellar density alone it is possible to measure the mass and radius of a ~0.6 M sub([middot in circle]) star to ~7 and ~2% precision, respectively. |
doi_str_mv | 10.1088/0004-6256/149/5/166 |
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HATS-6b has a period of P = 3.3253 d, mass of M sub(p) = 0.32 M sub(J) , radius of R sub(p) = 1.00 R sub(J) , and zero-albedo equilibrium temperature of T sub(eq) = 712.8 + or - 5.1 K. HATS-6 is one of the lowest mass stars known to host a close-in gas giant planet, and its transits are among the deepest of any known transiting planet system. 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subjects | ALBEDO ASTROPHYSICS, COSMOLOGY AND ASTRONOMY BOLOMETERS CORRECTIONS DENSITY DWARF STARS ECLIPSE Empirical analysis EQUILIBRIUM Extrasolar planets Gas giant planets MAIN SEQUENCE STARS MASS Red dwarf stars SATURN PLANET Stars Transits TRANSMISSION |
title | HATS-6b: A WARM SATURN TRANSITING AN EARLY M DWARF STAR, AND A SET OF EMPIRICAL RELATIONS FOR CHARACTERIZING K AND M DWARF PLANET HOSTS |
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