The orbiting probe
detects small dips in the brightness of a star that occur when a planet crosses its face.
It is being done by the people who launched the Kepler satellite to
detect small dips in the brightness of distant stars in order to detect the presence of now ~ 1000 new planets in the last several years, completely re-writing the textbooks on the parameter space of planetary atmospheres, solar system formation, etc..
Not exact matches
Seeing transits is not enough; periodic
dips in a star's light could be caused by a
small companion star too dim to
detect directly.
That parts - per - million sensitivity should allow Corot to
detect the
dips in a star's light caused by a transiting planet with a radius just twice that of Earth — and perhaps an even
smaller one, provided its orbit is tighter than Mercury's, so that the planet completes three transits during the 150 - day viewing period.
But with needle - in - haystack projects, I always wonder whether they saw nothing because there was nothing to
detect or because they missed the rare and transient brightness
dips that
small KBOs would cause.»
They can
detect brightness
dips as
small as 1 %, which is sufficient to find giant gaseous planets that are like our own Jupiter and Saturn.