Astronomers anticipate 100 billion Earth-like planets

April 4, 2013

Milky Way Galaxy (credit: NASA/JPL-Caltech)

University of Auckland researchers have proposed a new method for finding Earth-like planets in our galaxy and they anticipate that the number will be on the order of 100 billion.

The research supports an earlier estimate based on extrapolations of Kepler data.

The new research 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.

“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,” says Dr. Phil Yock from the University of Auckland’s Department of Physics. 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.”

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.

“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.”

In recent years, microlensing has been used to detect several planets as large as Neptune and Jupiter. Dr Yock and colleagues have proposed a new microlensing strategy for detecting the tiny deflection caused by an Earth-sized planet. Simulations carried out by Yock and his colleagues showed that Earth-sized planets could be detected more easily if a worldwide network of moderate-sized, robotic telescopes was available to monitor them.

Coincidentally, just such a network of 1m and 2m telescopes is now being deployed by Las Cumbres Observatory Global Telescope Network (LCOGT) in collaboration with SUPA/St Andrews (Scottish Universities Physics Alliance), with three telescopes in Chile, three in South Africa, three in Australia, and one each in Hawaii and Texas.  This network is used to study microlensing events in conjunction with the Liverpool Telescope in the Canary Islands which is owned and operated by Liverpool John Moores University.

It is expected that the data from this suite of telescopes will be supplemented by measurements using the existing 1.8m MOA telescope at Mt John, the 1.3m Polish telescope in Chile known as OGLE, and the recently opened 1.3m Harlingten telescope in Tasmania.

The new work will appear in Monthly Notices of the Royal Astronomical Society (Oxford University Press):