Gravitational Microlensing: A Tool for Detecting and Characterizing Free‐Floating Planets
Author(s) -
Cheongho Han,
SunJu Chung,
Doeon Kim,
ByeongGon Park,
YoonHyun Ryu,
Sang-jun Kang,
Dong Wook Lee
Publication year - 2004
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/381429
Subject(s) - gravitational microlensing , planet , exoplanet , physics , astronomy , jupiter mass , planetary mass , astrobiology , jupiter (rocket family) , orbit (dynamics) , gravitation , astrophysics , stars , space exploration , aerospace engineering , engineering
Various methods have been proposed to search for extrasolar planets. Comparedto the other methods, microlensing has unique applicabilities to the detectionsof Earth-mass and free-floating planets. However, the microlensing method isseriously flawed by the fact that the masses of the detected planets cannot beuniquely determined. Recently, Gould, Gaudi, & Han introduced an observationalsetup that enables one to resolve the mass degeneracy of the Earth-massplanets. The setup requires a modest adjustment to the orbit of an alreadyproposed Microlensing planet-finder satellite combined with ground-basedobservations. In this paper, we show that a similar observational setup canalso be used for the mass determinations of free-floating planets with massesranging from ~0.1 M_J to several Jupiter masses. If the proposed observationalsetup is realized, the future lensing surveys will play important roles in thestudies of Earth-mass and free-floating planets, which are the populations ofplanets that have not been previously probed.Comment: total 8 pages, including 3 figures, ApJ, in press (Mar 1, 2004
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