Photometric Orbits of Extrasolar Planets
arXiv:0905.2365 · doi:10.1088/0004-637X/702/2/1237
Abstract
We define and analyze the photometric orbit (PhO) of an extrasolar planet observed in reflected light. In our definition, the PhO is a Keplerian entity with six parameters: semimajor axis, eccentricity, mean anomaly at some particular time, argument of periastron, inclination angle, and effective radius, which is the square root of the geometric albedo times the planetary radius. Preliminarily, we assume a Lambertian phase function. We study in detail the case of short-period giant planets (SPGPs) and observational parameters relevant to the Kepler mission: 20 ppm photometry with normal errors, 6.5 hour cadence, and three-year duration. We define a relevant "planetary population of interest" in terms of probability distributions of the PhO parameters. We perform Monte Carlo experiments to estimate the ability to detect planets and to recover PhO parameters from light curves. We calibrate the completeness of a periodogram search technique, and find structure caused by degeneracy. We recover full orbital solutions from synthetic Kepler data sets and estimate the median errors in recovered PhO parameters. We treat in depth a case of a Jupiter body-double. For the stated assumptions, we find that Kepler should obtain orbital solutions for many of the 100-760 SPGP that Jenkins & Doyle (2003) estimate Kepler will discover. Because most or all of these discoveries will be followed up by ground-based radial-velocity observations, the estimates of inclination angle from the PhO may enable the calculation of true companion masses: Kepler photometry may break the "m sin i" degeneracy.
V1: 27 pages, 12 figures, 2 tables - submitted to ApJ; V2: 31 pages, 16 figures, 2 tables - accepted by ApJ
References in corpus (9)
- Photometric Light Curves and Polarization of Close-in Extrasolar Giant Planets
- The Very Low Albedo of an Extrasolar Planet: MOST Spacebased Photometry of HD 209458
- TrES-4: A Transiting Hot Jupiter of Very Low Density
- Photometric and Obscurational Completeness
- Phase Functions and Light Curves of Wide Separation Extrasolar Giant Planets
- Optical Albedo Theory of Strongly-Irradiated Giant Planets: The Case of HD 209458b
- Phase light curves for extrasolar Jupiters and Saturns
- Detecting Reflected Light from Close-In Extrasolar Giant Planets with the Kepler Photometer
- On the Completeness of Reflex Astrometry on Extrasolar Planets near the Sensitivity Limit
Cited by in corpus (6)
- Exoplanet albedo spectra and colors as a function of planet phase, separation, and metallicity
- New Completeness Methods for Estimating Exoplanet Discoveries by Direct Detection
- EXONEST: Bayesian Model Selection Applied to the Detection and Characterization of Exoplanets Via Photometric Variations
- True Masses of Radial-Velocity Exoplanets
- Analytical formulation of the single-visit completeness joint probability density function
- EXONEST: The Bayesian Exoplanetary Explorer