The Kepler mission from Nasa is the most modern technique for the hunt of Earth like planets. Till today thousands of planets are discovered and this discovery is still going on. The kepler satellite that was launched 2 years ago, scans a particular portion of the sky with high precision and captures the pixels on a high quality CCD. The pixel data recorded on the CCD is then transfered to Earth in the Nasa Laboratories. The main trick behind finding a planet from the data returned by Kepler is to look for stars that blink periodically on the CCD. From this periodicity we can determine the radial velocity and distance of the planet from the star. Again the blinking of the star provide us the drop of brightness during the blink or the transit. The drop of brightness, radial velocity, planet distance from the star and the star type help us to determine the surface temperature of the planet.
The proper values will yield a planet that is in the habitable zone and also earth like. But these studies are only for the stars whose plane of rotation is perpendicular to the field of view of the Kepler Telescope. It cannot be used for the stars whose plane of rotation is in the field of view of the telescope. I want to know the perfect parameter that can be used to detect a planet for the stars with rotational plane in the field of view. This is the only discrepancy in this mission. I hope sooner or later this will also be erased.