![Maps of average lensing parameters of simulated microlensing events due to different BFFPs over the 2D space log10[s(AU)]−log10[Mtot(M⊕)]. Here, Fi and Fw are fractions of simulated microlensing events due to BFFPs with intermediate and wide caustic topologies, respectively. ρ? shows the source radius projected on the lens plane and normalized to the Einstein radius, Lc is a length scale for caustic curves, ∆c represents the caustic area, τ is a time scale for microlensing events due to BFFPs, and P is the orbital period of binary lenses. -- Monthly Notices of the Royal Astronomical Society](https://i0.wp.com/astrobiology.com/wp-content/uploads/2025/10/On-the-Detection-of-Binary-Free-Floating-Planets.png?resize=1200%2C720&ssl=1)
The recent discovery of 40 binary Jupiter-mass free-floating planets in the Trapezium cluster by the James Webb Space Telescope (Pearson & McCaughrean 2023) has opened new windows and questions in […]
Trapezium Cluster
Posted inAstronomy & Telescopes, Brown Dwarfs, Exoplanets, -moons, -comets, Gas Giants, Interstellar, Press Release
New Study Reveals How Rogue Planetary-mass Objects Form In Young Star Clusters
A groundbreaking study published in Science Advances sheds new light on the mysterious origins of free-floating planetary-mass objects (PMOs)—celestial bodies with masses between stars and planets.