A Mass for the Extrasolar Planet Gl 876b Determined from Hubble Space Telescope Fine Guidan.pdf
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to appear in Ap. J. Letters
A Mass for the Extrasolar Planet Gl 876b Determined from Hubble
Space Telescope Fine Guidance Sensor 3 Astrometry and
High-Precision Radial Velocities1
G. F. Benedict1, B. E. McArthur1, T. Forveille 2 ,3, X. Delfosse3, E. Nelan 4, R. P. Butler5,
W. Spiesman1, G. Marcy6, B. Goldman8, C. Perrier3, W. H. Jefferys7, and M. Mayor9
ABSTRACT
We report the first astrometrically determined mass of an extrasolar planet,
a companion previously detected by Doppler spectroscopy. Radial velocities first
provided an ephemeris with which to schedule a significant fraction of the HST
observations near companion peri- and apastron. The astrometry residuals at
these orbital phases exhibit a systematic deviation consistent with a perturba-
tion due to a planetary mass companion. Combining HST astrometry with radial
velocities, we solve for the proper motion, parallax, perturbation size, inclination,
and position angle of the line of nodes, while constraining period, velocity ampli-
tude, longitude of periastron, and eccentricity to values determined from radial
1McDonald Observatory, University of Texas, 1 University Station C1402, Austin, TX 78712, fritz @as-
tro.as.utexas.edu, mca@astro.as.utexas.edu
2Canada-France-Hawaii Telescope, P.O. Box 1597, Kamuela, HI 96743, forveill@cfht.hawaii.edu
3Observatoire de Grenoble, B.P. 53X, 38041 Grenoble Cedex, France, delfosse@obs.ujf-
grenoble.fr,perrier@obs.ujf-grenoble.fr
4Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, nelan@stsci.edu
5Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road
NW, Washington, DC 20015, paul@dtm.ciw.edu
6Department of Astronomy, University of California, Berkeley, 601 Campbell Hall, Berkeley, CA 94720,
gmarcy@etoile.berkeley.edu
7Astronomy Dept., University of Texas, 1 University Station C1400, Austin, TX 78712,
bill@astro.as.utexas.edu
8Departmen
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