Bhanu Kumar Picture
Bhanu Kumar


Department of Mathematics
University of Michigan
Ann Arbor, MI 48109

Email: bhkumar (at) umich.edu


Curriculum Vitae (updated 22 Oct 2025)


I am currently a James Van Loo Postdoctoral Assistant Professor in the Department of Mathematics at the University of Michigan. Previously, I was a postdoctoral researcher in the research station "Geometry + Dynamics" at the Institute for Mathematics, Heidelberg University, working with JProf. Agustin Moreno on the AFOSR-funded project "Symplectic Methods in Space Mission Design". From October 2022 - April 2024 and May - August 2025, I was an NSF Mathematical Sciences Postdoctoral Research Fellow in the Mission Design and Navigation (MDNav) Section of the NASA Jet Propulsion Laboratory, California Institute of Technology. I completed my Ph.D. in 2022 from the School of Mathematics at Georgia Tech, advised by Prof. Rafael de la Llave and supported by a NASA NSTRF fellowship. I also spent time during my Ph.D. as an NSTRF visiting technologist in MDNav at JPL, working with mentor Dr. Rodney Anderson. Prior to that, from 2014-2017 I was a co-op student in the Radio Science Systems Group at JPL. I hold an M.S. degree in Aerospace Engineering as well, also from Georgia Tech.


Research Interests

At a broad level, my interests lie in the application of tools and results from mathematical dynamical systems theory and symplectic geometry, both analytical and computational, to various problems in celestial mechanics and applied astrodynamics for space mission design. In brief, there are geometric structures, such as periodic orbits, invariant tori, and stable and unstable manifolds, which govern many of the important dynamical properties of multi-body celestial systems. I am interested in developing fast and accurate methods for computing these objects as well as for investigating the dynamics induced by them. I am also working on applications of these methods to current and relevant problems in astrodynamics, with a current focus on mission design in cislunar space and outer planet moon systems using mean motion resonances.


Selected Journal and Conference Papers