The drifting star: Astronomers 'listen' to an exoplanet-host star and find its birthplace

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Using HARPS on ESOs 3.6-m telescope at La Silla astronomers were able to study in great detail the star Iota Horologii known to harbour a giant planet and make a very precise portrait of it: its temperature is 6150 K its mass is 1.25 times that of th ...
Using HARPS on ESO's 3.6-m telescope at La Silla, astronomers were able to study in great detail the star Iota Horologii, known to harbour a giant planet, and make a very precise portrait of it: its temperature is 6150 K, its mass is 1.25 times that of the Sun, and its age is 625 million years. Moreover, the star is found to be more metal-rich than the Sun by about 50%. This means the star must have drifted from the Hyades cluster where it formed. Credit: Digital Sky Survey/VirGO.

By studying in great detail the 'ringing' of a planet-harbouring star, a team of astronomers using ESO's 3.6-m telescope have shown that it must have drifted away from the metal-rich Hyades cluster. This discovery has implications for theories of star and planet formation, and for the dynamics of our Milky Way.


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All News summaries for April 15, 2008

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