
Mathematics Webinar
Mathematical Modeling in Solar System Dynamics
I am pleased to invite you to attend the following webinar, Mathematical Modeling in Solar System Dynamics. We are excited to hold three talks on new results pertaining to the size of our solar system and the mechanisms by which objects from interstellar space are captured into it using dynamical systems/chaos modeling, in addition to exploring how objects moving within it can eventually escape using random walk and Arnold diffusion. In addition, we will discuss how the size of the solar system is far larger than previously thought, extending far beyond the Oort cloud. Gravitational models for dark matter in our galaxy play a key role in modeling. The capture mechanism we discuss is called ‘weak capture’, which utilizes hyperbolic manifolds in phase space about our Sun. We also address the following question: What can be captured into our solar system?
Our speakers are Dr. James Green, former Chief Scientist of NASA, who will discuss the size of our solar system, capture into it, and what could actually be captured, and the second speaker will be Prof. Marian Gidea, Chair of Yeshiva Univ.’s mathematics department, who will discuss how instabilities can occur from seemingly stable orbits via Arnold diffusion.
Mathematical Methods of Astrophysics and Space Science
Edited by Prof. Dr. Edward A. Belbruno and Dr. James Lauer Green
Deadline for manuscript submissions: 1 October 2026

