Journal Article 1 Mention
One or more bound planets per Milky Way star from microlensing observations
A. Cassan•2012
D. KubasJean‐Philippe Beaulieu
Top 1% · 99th Percentile
588 citations · Astronomy and Astrophysics
Open AccessAstrophysics in St Andrews/SUPASearch for Earth mass exoplanet and free-floating planet via gravitational microlensing

TLDR

The Milky Way likely has at least one planet for every star, on average. Smaller planets are more common than giant planets, especially in wide orbits.

Summary

1 Study Aim

The authors aimed to measure how often stars have bound planets orbiting 0.5–10 astronomical units (AU, with one AU equal to the Sun–Earth distance). They focused on planets from roughly five Earth masses to ten Jupiter masses. The study tested whether planets are common or unusual around Milky Way stars. The research asked how many cool, distant planets exist around typical stars.

2 Study Design

The authors analyzed gravitational microlensing (brief brightening caused by a foreground star bending light) observations from 2002–07. The Optical Gravitational Lensing Experiment and Microlensing Observations in Astrophysics surveys found events, while the Probing Lensing Anomalies Network monitored them closely. Of 98 events observed in 2004, 43 met quality standards, with 26 providing most sensitivity. Three compatible planet detections were included. The team calculated detection efficiency (the chance of finding a planet signal), then fitted a planetary mass function (planet numbers across masses and orbits). A Bayesian analysis (probability updated using the observations) and Poisson model (a model for counting rare events) produced occurrence estimates. The researchers measured planet numbers using consistent observations and statistical corrections.

3 Findings

The study estimates that 17% of stars host Jupiter-mass planets between 0.5 and 10 AU, while 52% host cool Neptunes. Super-Earths occur at an estimated 62% rate. Across planets from five Earth masses to ten Jupiter masses, stars average 1.6 planets, with substantial uncertainty. The fitted mass distribution increases toward lower masses, showing that smaller planets are more common than giant ones. The authors conclude that planets are the rule rather than the exception around Milky Way stars. Their result also agrees with expectations from core-accretion theory (planet formation by gradually collecting solid material). Stars usually have worlds circling them, and smaller worlds are more common than very large ones.

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