Characteristics of Extrasolar Planets

Details Characteristics of Extrasolar Planets Characteristics of Extrasolar Planets

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..324..133f&link_type=abstract

Debris Disks and the Formation of Planets: A Symposium in Memory of Fred Gillett, ASP Conference Series, Vol. 324, Proceedings o

Astronomy and Astrophysics

Astronomy

2

Scientific paper

One hundred extrasolar planets have been discovered, all with ground-based Doppler observations. Most of the detected planets have masses (M sin i) greater than Jupiter. However, with improved precision the Doppler technique should eventually reach down to Neptune-mass planets at separations of 1 AU or less. Here we present the characteristics of discovered planets and their host stars and we report two multiple planet discoveries.

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