An Extrasolar Planet Census with a Space-based Microlensing Survey
D.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, M. Rich, K., Sahu, D. Tenerelli, A. Udalski, and P. Yock

TL;DR
A space-based microlensing survey can statistically characterize a wide range of exoplanets, including Earth-mass planets, providing unique insights into planet formation and distribution that other methods cannot achieve.
Contribution
This paper proposes the Microlensing Planet Finder (MPF) mission as a feasible, cost-effective space-based microlensing survey to comprehensively study exoplanet populations.
Findings
Can detect planets down to 0.1 Earth-masses
Provides statistical census of planets from 0.5AU to infinity
Complements other detection methods like Kepler and ground-based microlensing
Abstract
A space-based gravitational microlensing exoplanet survey will provide a statistical census of exoplanets with masses down to 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
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · History and Developments in Astronomy
