Astronomers anticipate 100 billion Earth-like planets

galaxy

The strategy uses a technique called gravitational microlensing, currently used by a Japan-New Zealand collaboration called MOA (Microlensing Observations in Astrophysics) at New Zealand’s Mt John Observatory. Their work will appear in the Oxford University Press journal Monthly Notices of the Royal Astronomical Society. Lead author Dr Phil Yock from the University of Auckland’s Department of Physics explains that the work will require a combination of data from microlensing and the NASA Kepler space telescope.

“Kepler finds Earth-sized planets that are quite close to parent stars, and it estimates that there are 17 billion such planets in the Milky Way. These planets are generally hotter than Earth, although some could be of a similar temperature (and therefore habitable) if they’re orbiting a cool star called a red dwarf.” “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. 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.” The first planet orbiting a Sun-like star was not found until 1995, despite strenuous efforts by astronomers. Dr Yock explains that this reflects the difficulty of detecting from a distance a tiny non-luminous object like Earth orbiting a bright object like the Sun.

The planet is lost in the glare of the star, so indirect methods of detection must be used. Whereas Kepler measures the loss of light from a star when a planet orbits between us and the star, microlensing measures the deflection of light from a distant star that passes through a planetary system en route to Earth – an effect predicted by Einstein in 1936. In recent years, microlensing has been used to detect several planets as large as Neptune and Jupiter.

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