Journal
ASTROPHYSICAL JOURNAL
Volume 581, Issue 2, Pages L115-L118Publisher
UNIV CHICAGO PRESS
DOI: 10.1086/346073
Keywords
astrometry; planetary systems; stars : distances; techniques : interferometric
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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 Hubble Space Telescope (HST) observations near companion peri- and apastron. The astrometry residuals at these orbital phases exhibit a systematic deviation consistent with a perturbation 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 amplitude, longitude of periastron, and eccentricity to values determined from radial velocities. We find a perturbation semimajor axis and inclination, alpha = 0.25 +/- 0.06 mas, i = 84degrees +/- 6degrees, and G1 876 absolute parallax, pi(abs) = 214.6 +/- 0.2 mas. Assuming that the mass of the primary star is M-* = 0.32 M., we find the mass of the planet, G1 876b, M-b = 1.89 +/- 0.34 M-Jup.
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