Radial velocity detection of extra-solar planetary systems

Details Radial velocity detection of extra-solar planetary systems Radial velocity detection of extra-solar planetary systems

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991plas.rept...33c&link_type=abstract

In NASA, Washington, Reports of Planetary Astronomy, 1991 p 33-34 (SEE N92-12792 03-89)

Astronomy and Astrophysics

Astronomy

Center Of Gravity, Planetary Composition, Planetary Evolution, Planetary Orbits, Radial Velocity, Stellar Mass, G Stars, Geochronology, Main Sequence Stars, Planetary Systems, Precision

Scientific paper

The goal of this program was to detect planetary systems in orbit around other stars through the ultra high precision measurement of the orbital motion of the star around the star-planet barycenter. The survey of 33 nearby solar-type stars is the essential first step in understanding the overall problem of planet formation. The program will accumulate the necessary statistics to determine the frequency of planet formation as a function of stellar mass, age, and composition.

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