HAT-P-7b (or Kepler-2b) is an exotic exoplanet orbiting the star HAT-P-7, located in the zodiac constellation Cygnus. HATP-7b, discovered in 2008 by the HATNet Project telescope HAT-7, has a radius larger than Jupiter's and an orbital plane that's tilted so much relative to its star (108°) that the planet is nearly in a polar orbit.
As a result of its relatively close orbit, the planet is unique because of its extreme heat (2730 K | 2456,85°C | 4454,33F). It is also unique since of its cloud composition (made of corundum, mineral that forms rubies and sapphires).
The radius of HAT-P-7b is 100,042.641 km (62,163.60 miles) and the area of its surface is 125,770,897,514.3298 km² (48,560,395,072.08 miles²).
Strong winds are moving across HAT-P-7b, which causes catastrophic storms. On the cold night side of the planet, clouds form, but on the hot day side, they evaporate quickly. As a result of strong winds circling the planet, clouds are carried from the nightside to the dayside. Large cloud formations build up and then dissipate as the winds change their speed.
HAT-P-7b has a mass of 1.84 Jupiters (3,492,320,000,000,000,300,000,000,000 tons) and has a density of 0.54 g/cm³.
Studies of the tectonic plates of HAT-P-7b has yet to be made.
HAT-P-7b is 1112.2 light-years away from Earth. Its orbital distance is 0.03676 AU.
It is thought that HAT-P-7b's clouds are composed of vaporized corundum, which is a mineral that forms rubies and sapphires.
The planet is predicted to have a dayside temperature of 2,630-2,880 K (4,270-4,720°F | 2,360-2,610°C), while nightside temperatures are 2,211-2,238 K (3,520-3,569°F | 1,938-1,965°C).
We do not know its age.
This extra solar planet has a surface gravity of 17.36 m/s² (56.955381 ft/s²).
Simulation of magnetic field lines in the atmosphere of HD209458 b with a similar temperature structure to HAT-P-7 b. Azimuthal (toroidal) magnetic field lines are colour-coded, with blue representing a negatively-directed field (with saturation at -50 G) and magenta representing a positively-directed field (with saturation at 50 G), then green and yellow corresponding to -5 and 5 G, respectively. From this vantage point, you can see the east-side terminator.
It takes 2.2 days for HAT-P-7b to complete one orbit around its star.
HAT-P-7b is a tidally locked exoplanet.
HAT-P-7b does not have any moons.
HAT-P-7b does not possess any rings.