Apparent Stellar Wobble by a Planet in a Circumstellar Disk: Limitations   on Planet Detection by Astrometry
  Astrometric detection of a stellar wobble on the plane of the sky will provide us a next breakthrough in searching extrasolar planets. The Space Interferometry Mission (SIM) is expected to achieve a high-precision astrometry as accurate as 1 micro-as, which is precise enough to discover a new-born Jupiter mass planet around a pre-main-sequence (PMS) star in the Taurus-Auriga star forming region. PMS stars, however, have circum-stellar disks that may be obstacles to the precise measurement of the stellar position. We present results on disk influences to the stellar wobble. The density waves excited by a planet move both of the disk's mass center and the photo-center. The motion of the disk mass center induces an additional wobble of the stellar position, and the motion of the disk photo-center causes a contamination in the measurement of the stellar position. We show that the additional stellar motion dynamically caused by the disk's gravity is always negligible, but that the contamination of the disk light can interfere with the precise measurement of the stellar position, if the planet's mass is smaller than ~10 Jupiter mass. The motion of the disk photo-center is sensitive to a slight change in the wave pattern and the disk properties. Measurements by interferometers are generally insensitive to extended sources such as disks. Because of this property SIM will not suffer significant contaminations of the disk light, even if the planet's mass is as small as 1 Jupiter mass. 
Taku Takeuchi (Kobe University), T. Velusamy (JPL), and D. N. C. Lin   (UCO/Lick Observatory)