A Census of Exoplanets in Orbits Beyond 0.5 AU via Space-based Microlensing
David P. Bennett, J. Anderson, J.-P. Beaulieu, I. Bond, E. Cheng, K., Cook, S. Friedman, B.S. Gaudi, A. Gould, J. Jenkins, R. Kimble, D. Lin, J., Mather, M. Rich, K. Sahu, T. Sumi, D. Tenerelli, A. Udalski, and P. Yock

TL;DR
A space-based microlensing survey can statistically characterize a wide range of exoplanets beyond 0.5 AU, providing unique insights into planetary system architectures and formation theories.
Contribution
This paper advocates for a dedicated space-based microlensing mission, the MPF, to achieve comprehensive exoplanet census beyond 0.5 AU, surpassing other methods in scope and detail.
Findings
Microlensing surveys can detect planets with masses >0.1 Earth-masses beyond 0.5 AU.
Space-based microlensing uniquely covers a broad range of planetary types and orbital distances.
The proposed MPF mission is feasible with proven technology and under $300 million.
Abstract
A space-based gravitational microlensing exoplanet survey will provide a statistical census of exoplanets with masses greater than 0.1 Earth-masses and orbital separations ranging from 0.5AU to infinity. This includes analogs to all the Solar System's planets except for Mercury, as well as most types of planets predicted by planet formation theories. Such a survey will provide results on the frequency of planets around all types of stars except those with short lifetimes. Close-in planets with separations < 0.5 AU are invisible to a space-based microlensing survey, but these can be found by Kepler. Other methods, including ground-based microlensing, cannot approach the comprehensive statistics on the mass and semi-major axis distribution of extrasolar planets that a space-based microlensing survey will provide. The terrestrial planet sensitivity of a ground-based microlensing survey is…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Gamma-ray bursts and supernovae · Astronomy and Astrophysical Research
