After 50 years of dreaming about it, space-based
microlensing observations are now underway. A 2014 100-hr Spitzer Pilot
Program generated "microlens parallaxes" for dozens of lenses, opening
the prospect of measuring the Galactic distribution of planets. This
program will be expanded 8-fold in 2015. Analogous observations by
Kepler will measure the mass function of free-floating planets. WFIRST
microlensing observations will, as advertised, "complete the planetary
census" but they will do an immense amount of astrophysics as well. I
discuss how microlensing's take off builds on rapid, ongoing,
ground-based developments.
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