{ "id": "0911.2008", "version": "v1", "published": "2009-11-10T21:10:58.000Z", "updated": "2009-11-10T21:10:58.000Z", "title": "Starspot Jitter in Photometry, Astrometry and Radial Velocity Measurements", "authors": [ "V. V. Makarov", "C. A. Beichman", "J. H. Catanzarite", "D. A. Fischer", "J. Lebreton", "F. Malbet", "M. Shao" ], "comment": "accepted in ApJ Letters, Nov. 2009", "categories": [ "astro-ph.SR" ], "abstract": "Analytical relations are derived for the amplitude of astrometric, photometric and radial velocity perturbations caused by a single rotating spot. The relative power of the star spot jitter is estimated and compared with the available data for $\\kappa^1$ Ceti and HD 166435, as well as with numerical simulations for $\\kappa^1$ Ceti and the Sun. A Sun-like star inclined at $i=90\\degr$ at 10 pc is predicted to have a RMS jitter of 0.087 \\uas in its astrometric position along the equator, and 0.38 m s$^{-1}$ in radial velocities. If the presence of spots due to stellar activity is the ultimate limiting factor for planet detection, the sensitivity of SIM Lite to Earth-like planets in habitable zones is about an order of magnitude higher that the sensitivity of prospective ultra-precise radial velocity observations of nearby stars.", "revisions": [ { "version": "v1", "updated": "2009-11-10T21:10:58.000Z" } ], "analyses": { "keywords": [ "radial velocity measurements", "starspot jitter", "prospective ultra-precise radial velocity observations", "photometry", "astrometry" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/707/1/L73", "journal": "The Astrophysical Journal", "year": 2009, "month": "Dec", "volume": 707, "number": 1 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 836610, "adsabs": "2009ApJ...707L..73M" } } }