NASA Mission Discovers First Rocky Planet
Monday - 1/17/2011, 12:09pm EST
The size of the exoplanet can be derived from periodic dips in brightness. Kepler's ultra-precise photometer measures the tiny decrease in a star's brightness that happen when a planet crosses in front of it. The distance between the planet and the star is calculated by measuring the time between successive dips as the planet orbits the star.
As a result of the analysis, that star orbited by the planet - Kepler-10 - is now one of the most well-characterized planet-hosting stars in the universe.



