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A NEW CHANNEL TO SEARCH FOR EXTRA-SOLAR SYSTEMS WITH MULTIPLE PLANETS VIA GRAVITATIONAL MICROLENSING

  • HAN CHEONGHO (Department of Physics, Chungbuk National University) ;
  • PARK MYEONG-GU (Department of Astronomy & Atmospheric Sciences, Kyungpook National University)
  • 발행 : 2002.03.01

초록

Gaudi, Naber & Sackett pointed out that if an event is caused by a lens system containing more than two planets, all planets will affect the central region of the magnification pattern, and thus the existence of the multiple planets can be inferred by detecting additionally deformed anomalies from intensive monitoring of high magnification microlensing events. Unfortunately, this method has important limitations in identifying the existence of multiple planets and determining their parameters (the mass ratio and the instantaneous projected separation) due to the degeneracy of the resulting light curve anomalies from those induced by a single planet and the complexity of multiple planet lensing models. In this paper, we propose a new channel to search for multiple planets via microlensing. The method is based on the fact that the lensing light curve anomalies induced by multiple planets are well approximated by the superposition of those of the single planet systems where the individual planet-primary pairs act as independent lens systems. Then, if the source trajectory passes both of the outer deviation regions induced by the individual planets, one can unambiguously identify the existence of the multiple planets. We illustrate that the probability of successively detecting light curve anomalies induced by two Jovian-mass planets located in the lensing zone through this channel will be substantial. Since the individual anomalies can be well described by much simpler single planet lensing models, the proposed method has an important advantage of allowing one to accurately determine the parameters of the individual planets.

키워드

참고문헌

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피인용 문헌

  1. Microlensing Surveys for Exoplanets vol.50, pp.1, 2012, https://doi.org/10.1146/annurev-astro-081811-125518
  2. CRITICAL CURVES AND CAUSTICS OF TRIPLE-LENS MODELS vol.806, pp.1, 2015, https://doi.org/10.1088/0004-637X/806/1/99
  3. On the Feasibility of Detecting Satellites of Extrasolar Planets via Microlensing vol.580, pp.1, 2002, https://doi.org/10.1086/343082
  4. A Likely Detection of a Two-planet System in a Low-magnification Microlensing Event vol.155, pp.6, 2018, https://doi.org/10.3847/1538-3881/aabd7a