2025/04/24 by Weicheng Zang, Youn Kil Jung, Jennifer C. Yee +88 · 2 voices · 33 citations
Physics and Astronomy · #Astro and Planetary Science #Astrobiology #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Exoplanet #Galaxy #Gas giant #Gravitational microlensing #Jupiter (rocket family) #Mass distribution #Orbit (dynamics) #Physics #Planet #Planetary system #Stars #Stellar, planetary, and galactic studies
paper · pdf · doi:10.1126/science.adn6088
published in Science 388(6745), 400-404 (American Association for the Advancement of Science)
openalex publication_date 2025/04/24 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06
Exoplanets classified as super-Earths are commonly observed on short-period orbits, close to their host stars, but their abundance on wider orbits is poorly constrained. Gravitational microlensing is sensitive to exoplanets on wide orbits. We observed the microlensing event OGLE-2016-BLG-0007, which indicates an exoplanet with a planet-to-star mass ratio roughly double the Earth-Sun mass ratio, on an orbit longer than Saturn's. We combined this event with a larger sample from a microlensing survey to determine the distribution of mass ratios for planets on wide orbits. We infer that there are ~0.35 super-Earth planets per star on Jupiter-like orbits. The observations are most consistent with a bimodal distribution, with separate peaks for super-Earths and gas giants. We suggest that this reflects differences in their formation processes.