Ekta Patel, Villanova University
When
Refreshments served at 2:00 pm in the 3rd floor atrium
TAP Dynamics Initiative Lecture
Ekta Patel, Villanova University
Title: Assembling Andromeda: What Orbital Dynamics Reveal About the M31 System
Abstract: The Milky Way–Large Magellanic Cloud interaction has reshaped our understanding of how massive satellites drive disequilibrium in their host systems — and Andromeda (M31) tells a strikingly parallel, yet distinct, story. With 6D phase space data now available for nearly a dozen M31 satellites, we can for the first time begin to reconstruct the complex interaction history of the M31 system in detail.
In this talk, I will present orbital modeling results for M31 and its most massive satellite, M33. Contrary to the long-held assumption that M33 experienced a recent close encounter with M31, I will show that M33 is most likely on its first infall into M31's halo — a result further corroborated by M33's untruncated HI disk and the orbital histories of cosmological analogs. I will also present preliminary orbital results on M32, a prominent dwarf elliptical galaxy situated near M31's disk. Drawing on insights from the MW-LMC system, I will discuss how M33's passage may be displacing M31's barycenter and influencing the dynamics of its broader satellite population, and what this means for interpreting M31's assembly history.
Bio: Dr. Ekta Patel received her Ph.D. in Astronomy & Astrophysics from the University of Arizona in 2019, and she holds a B.A. in Physics from New York University. From 2019-2023 she was a Miller Fellow at UC Berkeley and then a NASA Hubble Fellow at the University of Utah. She has been an Assistant Professor in the Department of Astrophysics and Planetary Science at Villanova University since Fall 2025. Dr. Patel's research focuses on galactic dynamics and the evolution of satellite galaxies and their host galaxies in the Local Group.
Articles/press: Scientific American, ESA, Sky&Telescope, UA Press Release