The Pioneer of Transit Method Discoveries: OGLE-TR-56b

 Transit methodology, where an exoplanet crosses its star during its orbit, has proven to be a powerful tool for planet discovery. The regular dips in the star's brightness, caused by the planet obstructing some of its light, reveal the existence of these exoplanets. This predictable pattern of light curves has enabled the discovery of almost 4,000 exoplanets to date, many of which were observed by the Kepler telescope.

OGLE-TR-56b, discovered in 2002, holds the honor of being the first planet discovered through transits. Technically, exoplanet Osiris was the first to be observed through this method, but it had already been discovered through the radial velocity method, making OGLE-TR-56b the true pioneer.

Unveiled within the OGLE project, OGLE-TR-56b's discovery was announced in July 2002 and confirmed the following year. The planet orbits an F-type star and at the time of its discovery, it was the most distant known exoplanet from Earth, located 1,500 light-years away.

Classified as a "hot Jovian," OGLE-TR-56b is a gas giant slightly larger than Jupiter, with a mass 1.4 times that of Jupiter and a diameter 1.3 times that of the Jovian planet. Its close proximity to its star, with a semi-major axis of only 0.02 AU and completing one revolution in just 1.2 days, makes the conditions on OGLE-TR-56b inhospitable for life as we know it. 

Credit: NASA.