HAT-P-25 b is a sizzling hot Jupiter orbiting a star called HAT-P-25, discovered back in 2010 using the trusty transit method from the ground-based HATNet survey. This gas giant is a real close-in companion, circling so tightly it's scorched by its star's relentless heat, making it a fascinating target for astronomers eager to study the atmospheres of such fiery worlds. Detected with a 2K CCD sensor, HAT-P-25 b showcases the power of ground-based telescopes to find distant planets even without space-based help. While it might not have a catchy nickname yet, this world is a shining example of how far exoplanet hunting has come, revealing exotic planetary systems far beyond our solar neighborhood.
