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Discovering planetary systems through gravitational microlenses

Gould, Andrew, Loeb, Abraham·1992·The Astrophysical Journal

Abstract

Planetary systems of Galactic disk stars can be detected as microlenses of stars in the Galactic bulge. Planets in a solar-like system positioned half-way to the Galactic center should leave a noticeable signature (magnification larger than 5 percent) on the light curve of a gravitationally lensed bulge star in about 20 percent of the microlensing events. This high probability results from a coincidence between Jupiter's orbital radius and the solar Einstein radius at this distance. Typical planetary signals last for about 1 day, a small fraction of the approximately 1 month duration of the entire microlensing event. Dedicated monitoring of microlensing candidates is suggested as a method to discover planetary systems in conjunction with forthcoming observations toward the Galactic bulge.

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Metadata

Authors
Gould, A., & Loeb, A.
Venue
The Astrophysical Journal
Published
1992-09
Volume
396
Pages
104
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2060501361
Cited by
577
References
0
FWCI
1.97
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Discovering planetary systems through gravitational microlenses. https://app.cochat.ai/papers/10.1086/171700
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Gould, A., & Loeb, A. (1992). Discovering planetary systems through gravitational microlenses. The Astrophysical Journal. https://doi.org/10.1086/171700

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.