"Our proposal is to measure the number of Earth-mass planets orbiting stars at distances typically twice the Sun-Earth distance. Our planets will therefore be cooler than the Earth."
The Kepler data will combine with the observatory's data from a technique called gravitational microlensing - that detects the mass of a planet or star.
The microlensing is currently used by a Japan-New Zealand collaboration called Microlensing Observations in Astrophysics (MOA).
"By interpolating between the Kepler and MOA results, we should get a good estimate of the number of Earth-like, habitable planets in the Galaxy. We anticipate a number in the order of 100 billion.
"Of course, it will be a long way from measuring this number to actually finding inhabited planets, but it will be a step along the way."
A network of 12 telescopes in Chile, South Africa, Australia, Hawaii, Texas and the Canary Islands will also help to detect the planets.