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ON THE INCLINATION OF EXTRA-SOLAR PLANETARY ORBITS
BRUCE CAMPBELL and R. F. GARRISON
Publications of the Astronomical Society of the Pacific
Vol. 97, No. 588 (February 1985), pp. 180-182
Published by: Astronomical Society of the Pacific
Stable URL: http://www.jstor.org/stable/40678471
Page Count: 3
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We show that the inclination of a planetary orbital axis can be determined, on the assumption that it is the same as the inclination of the stellar rotation axis. The latter may be derived from the apparent stellar rotation speed (v sin i) and the rotation period determined from the modulation or strength of Ca II emission.
Publications of the Astronomical Society of the Pacific © 1985 The University of Chicago Press