New research proposes that a single cosmic event, such as a flyby of a massive interstellar object, could provide answers to the mystery about the slightly eccentric and tilted orbits of the Solar System’s gas giants.
Planetary orbits today reflects billions of years of interactions, as planets coalesced from a rotating disk of gas and dust around the Sun, following conservation of angular momentum shaped their orbits into a flat plane.
While planet-planet interactions were common, rare visits by interstellar objects likely played pivotal roles in shaping planet formation.
A study by a team from the University of Toronto suggests that a single encounter with an object between two and fifty times the mass of Jupiter could explain the observed eccentricities and tilts of the Solar System’s giant planets.
The flyby hypothesis addresses gaps in traditional theories that struggle to explain the orbits of Jupiter, Saturn, Uranus, and Neptune which deviate from perfect circles and alignments.
The researchers have found one-in-one-hundred odds that such scenario involving a massive interstellar object passing at a perihelion distance of less than 20 astronomical units would have occurred.
The flyby hypothesis is a theoretical model that requires further validation and observational campaigns could identify remnants of past interstellar visitors, lending credibility to the theory.
The recognition of an interconnected galaxy where planets and interstellar objects frequently influence one another could provide a better understanding of potential life-sustaining environments elsewhere in the universe.
Future research will likely focus on identifying other systems where rogue planets have played similar roles.
Advances in telescopes and detection methods could reveal more interstellar objects, providing opportunities to study their interactions with established planetary systems.