In Search of Terrestrial Planets in the Habitable Zone of M Dwarfs

Details In Search of Terrestrial Planets in the Habitable Zone of M Dwarfs In Search of Terrestrial Planets in the Habitable Zone of M Dwarfs

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006msngr.123...21k&link_type=abstract

The Messenger, volume 123, page 21

Computer Science

2

Scientific paper

After the availability of UVES at the VLT in 2000, we began a survey of M-dwarf stars in order to find low-mass planetarycompanions. This ongoing survey, which currently enjoys ESO Large Programme status, provides a time baseline of up to six years. It is thus capable of finding planets of just a few Earth masses in close-in orbits that correspond to the habitable zones around these stars.

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