Floating binary planets from ejections during close stellar encounters

The discovery of planetary systems beyond our solar system has challenged established theories of planetary formation. Planetary orbits display a variety of unexpected architectures, and free-floating planets appear ubiquitous. The recent detection of candidate Jupiter Mass Binary Objects (JuMBOs) by the James Webb Space Telescope (JWST) has added another puzzling layer. Here, through direct few-body simulations, we demonstrate that JuMBOs could arise from the ejection of double giant planets following a close encounter with a passing star, if the two planets are nearly aligned at the closest approach. These ejected JuMBOs typically possess an average semi-major axis approximately three times the orbital separation within their original planetary system and a high eccentricity, characterized by a superthermal distribution that sets them apart from those formed primordially. We estimate the JuMBO formation rate per planetary system in typical and densely populated clusters, revealing a significant environmental dependence. In dense clusters, this formation rate can reach a few percent for wide planetary systems. Comparative analysis of JuMBO rates and properties with current and forthcoming JWST observations across various environments promises insights into the conditions under which these giant planets formed in protoplanetary disks, thereby imposing constraints on theories of giant planet formation.