NASA has given the go-ahead to a project to search for Earth-like planets
beyond the Solar System. The space-borne telescope, called Kepler, will enable
us to search the Galaxy for planets the size of Earth or smaller, and is
scheduled for launch in 2006.
Around 80 planets outside our Solar System have been discovered. Late last
year, the Hubble Space Telescope detected the atmosphere of one of them
(91av, 1 December 2001, p 16).
But techniques used so far are only sensitive enough to find gas giants like Jupiter,
which are unlikely to harbour life.
Kepler should be able to detect planets as small as Mercury, says deputy
principal investigator David Koch of the NASA Ames Research Center in
California. The project was first proposed in the 1990s
(91av, 18 September 1999, p 32),
and has now been chosen as part of NASA’s Discovery
Program of relatively low-cost missions. It will share $299 million with
a project called Dawn, which will study asteroid formation.
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Kepler will follow the Earth in an orbit around the Sun. Using a telescope
measuring 1 metre across, it will monitor hundreds of thousands of stars
simultaneously to look for tiny changes in their brightness caused by planets
passing in front of them.
“From the [planet’s] orbit and temperature of the star, we can then calculate
the characteristic temperature of the planet, and determine if liquid water
could exist on the surface,” explains Koch. “That is, determine if it is
ٲ.”
The technique will only detect planets that pass exactly between the
telescope and their parent star. For Earth-sized planets, the odds of that
orbital alignment are just 1 in 200, but Koch still hopes that Kepler will find
“many hundreds” of planets like our own during its four-year mission.
“It is the first step on a long road,” says Malcolm Friedlund from the
European Space Agency in Noordwijk, the Netherlands. Friedlund is working on
ESA’s Darwin mission, due for launch in 2015, which will attempt to find planets
and analyse their atmospheres by detecting their light directly.