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HAT-P-7b (or Kepler -2b) is an extrasolar planet discovered in 2008. It orbits very close to its host star and is larger and more massive than Jupiter.
HAT-P-7 b is a gas giant exoplanet that orbits a F-type star. Its mass is 1.84 Jupiters, it takes 2.2 days to complete one orbit of its star, and is 0.03676 AU from its star. Its discovery was announced in 2008.
HAT-P-7b (Kepler-2b) – planeta pozasłoneczna typu gorący jowisz znajdująca się w odległości około 1000 lat świetlnych od Ziemi w gwiazdozbiorze Łabędzia. Planeta ta została odkryta 6 marca 2008 w programie HATNet. Obiega ona gwiazdę GSC 03547-01402 (HAT-P-7).
hat-p-7 b Orbital period, transit mid-point, transit duration, Rp/Rs and their errors taken from DR24 KOI table. Planet radius error propagated from stellar radius error in ref. and Rp/Rs error.
Meet the scorching exoplanet that's dark as charcoal with a sapphire sky - BBC Sky at Night Magazine. HAT-P-7b is an ultra-hot exoplanet that's heated to such an extent, its atmosphere is one of the richest in elements yet seen.
12 gru 2016 · HAT-P-7 b is a hot Jupiter of radius 1.4 RJ that transits its host star with a period of 2.20 days 7. It is extremely hot, with a dayside brightness temperature of 2,860 K and an equilibrium ...
15 maj 2017 · A magnetohydrodynamic model is able to explain the peak brightness point offset variations in the atmosphere of the hot giant exoplanet HAT-P-7 b with wind variability. A minimum field...
