Transiting Extrasolar Planet with a Companion: Effects of Orbital Eccentricity and Inclination

Abstract

Continuing work initiated in an earlier publication [Sato and Asada, PASJ, 61, L29 (2009)], we consider light curves influenced by the orbital inclination and eccentricity of a companion in orbit around a transiting extrasolar planet (in a planet-satellite system or a hypothetical true binary). We show that the semimajor axis, eccentricity and inclination angle of a `moon' orbit around the host planet can be determined by transit method alone. For this purpose, we present a formulation for the parameter determinations in a small-eccentricity approximation as well as in the exact form. As a result, the semimajor axis is expressed in terms of observables such as brightness changes, transit durations and intervals in light curves. We discuss also a narrow region of parameters that produce a mutual transit by an extrasolar satellite.

29 pages, 11 figures, 1 table; orbital inclination included, parameter region considered; accepted for publication in PASJ

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• Modeling the Infrared Spectrum of the Earth-Moon System: Implications for the Detection and Characterization of Earthlike Extrasolar Planets and their Moonlike Companions
• Planet-Planet Occultations in TRAPPIST-1 and Other Exoplanet Systems
• LUNA: An algorithm for generating dynamic planet-moon transits
• The Rossiter-McLaughlin effect for exomoons or binary planets
• Possibility for albedo estimation of exomoons: Why should we care about M dwarfs?