activity
19992025
most citedOrbital Evolution of Planets Embedded in a Planetesimal Disk

345 citations · 766 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.EP2025

N-body simulations of the Self-Confinement of Viscous Self-Gravitating Narrow Eccentric Planetary Ringlets

Joseph M. Hahn, Douglas P. Hamilton, Thomas Rimlinger +1

Narrow eccentric planetary ringlets have sharp edges, sizable eccentricity gradients, and a confinement mechanism that prevents radial spreading due to ring viscosity. Most propose…

astro-ph.EP2015★ 6 cited

The Shape of Saturn's Huygens Ringlet Viewed by Cassini ISS

Joseph N. Spitale, Joseph M. Hahn

A new model for the shape of the prominent eccentric ringlet in the gap exterior to Saturn's B-ring is developed based on Cassini imaging observations taken over about 8 years. Unl…

astro-ph.EP2013★ 7 cited

An N-body Integrator for Gravitating Planetary Rings, and the Outer Edge of Saturn's B Ring

Joseph M. Hahn, Joseph N. Spitale

A new symplectic N-body integrator is introduced, one designed to calculate the global 360 degree evolution of a self-gravitating planetary ring that is in orbit about an oblate pl…

astro-ph.EP2010★ 17 cited

Diagnosing Circumstellar Debris Disks

Joseph M. Hahn

(Abridged) A numerical model of a circumstellar debris disk is developed and applied to observations of the circumstellar dust orbiting beta Pictoris. The model accounts for the ra…

astro-ph.EP2009★ 11 cited

Dynamics of the Sharp Edges of Broad Planetary Rings

Joseph M. Hahn, Joseph N. Spitale, Carolyn C. Porco

(Abridged) The following describes a model of a broad planetary ring whose sharp edge is confined by a satellite's m^th Lindblad resonance (LR). This model uses a streamline formal…

astro-ph2008★ 10 cited

The Secular Evolution of a Close Ring-Satellite System: The Excitation of Spiral Density Waves at a Nearby Gap Edge

Joseph M. Hahn

The Lagrange planetary equations are used to study to secular evolution of a small, eccentric satellite that orbits within a narrow gap in a broad, self-gravitating planetary ring.…