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20012023
most citedShort-Term Dynamical Interactions Among Extrasolar Planets

198 citations · 1.7k across the 33 of their papers we have counts for

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astro-ph2008★ 154 cited

How eccentric orbital solutions can hide planetary systems in 2:1 resonant orbits

Guillem Anglada-Escude, Mercedes Lopez-Morales, John E. Chambers

The Doppler technique measures the reflex radial motion of a star induced by the presence of companions and is the most successful method to detect exoplanets. If several planets a…

astro-ph2007

N-body integrators for planets in binary star systems

John E. Chambers

Symplectic integrators are the tool of choice for many researchers studying dynamical systems because of their good long-term energy conservation properties. For systems with a dom…

astro-ph2007★ 56 cited

The instability of planetary systems in binaries: how the Kozai mechanism leads to strong planet-planet interactions

Daniel Malmberg, Melvyn B. Davies, John E. Chambers

In this letter we consider the evolution of a planetary system around a star inside a wide binary. We simulate numerically the evolution of the planetary orbits for both co-planar…

astro-ph2007★ 146 cited

Terrestrial Planet Formation Around Individual Stars Within Binary Star Systems

Elisa V. Quintana, Fred C. Adams, Jack J. Lissauer +1

We calculate herein the late stages of terrestrial planet accumulation around a solar type star that has a binary companion with semimajor axis larger than the terrestrial planet r…

astro-ph2002★ 66 cited

A Dynamical Analysis of the 47 UMa Planetary System

Gregory Laughlin, John Chambers, Debra Fischer

The mass and period ratios of the two planets orbiting 47 UMa suggest a possible kinship to the Jupiter-Saturn pair in our solar system. We explore the current dynamical state of t…

astro-ph2002★ 137 cited

Extrasolar Trojans: The Viability and Detectability of Planets in the 1:1 Resonance

Gregory Laughlin, John Chambers

We explore the possibility that extrasolar planets might be found in the 1:1 mean-motion resonance. There are a variety of stable co-orbtial configurations, and we specifically exa…