HAT-P-7 b is a sizzling hot Jupiter orbiting the star HAT-P-7, discovered back in 2008 using the trusty ground-based HATNet telescope and its 2K CCD sensor. This planet is no wallflower—it’s a gas giant so close to its star that it completes orbits faster than many other planets take to finish a year! Being a "transit" discovery, we catch glimpses of this world as it passes in front of its star, causing tiny dips in starlight. Its tight, fiery embrace with its star makes HAT-P-7 b an exciting target for astronomers interested in extreme planetary weather and scorching atmospheres. If you’re looking for a wild ride in exoplanet exploration, HAT-P-7 b is definitely one to watch!
