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Astronomers spot dozens of 'super-Earths'
(Agencies)
Updated: 2008-06-16 22:57

PARIS - European astronomers on Monday said they had located dozens of giant planets in three distant solar systems.


NASA image taken in 2005 from the US spacecraft Messenger en route to the planet Mercury shows Earth. [Agencies] 

The discovery suggests that at least one third of stars similar to our own Sun harbour such planets, multiplying previous estimates by five.

A trio of these 'super-Earths' -- so-called because they are several times the mass of our own planet -- were detected orbiting a star known as HD 40307 some 42 lights away.

One light-year is roughly equivalent to 9.5 trillion kilometres (6 trillion miles).

"Does every single star harbour planets and, if yes, how many?", asked astronomer Michel Mayor of Switzerland's Geneva Observatory. "We may not yet know the answer but we are making huge progress," he said in a statement.

The first planet outside our solar system was detected in 1995, and less than 280 of these exoplanets had been found before today's findings, unveiled at an astronomy conference in Nantes, France.

But a new generation of powerful instruments is almost certain to expand the list rapidly, say scientists.

The recent batch of exoplanets were all spotted with the High-Accuracy Radial-Velocity Planet Searcher (HARPS), a 3.6-metre telescope and spectograph perched atop La Scilla mountain at the southern edge of Chile's Atacama Desert.

"Clearly these planets are only the tip of the iceberg," says Mayor. "The analysis of all the stars studied with HARPS shows that about one third of solar-like stars have either super-Earth or Neptune-like planets with orbital periods shorter than 50 days."

Earth orbits the Sun once every 365 days.

Distant planets, even big ones, are too small to be directly observed, and can only be detected by measuring their impact on the movement of the stars they orbit.

"The mass of the smallest planets is 100,000 times smaller than that of the star, and only the high sensitivity of HARPS made it possible to detect them," says co-author Francois Bouchy, from the Astrophysics Institute of Paris.

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