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Extrasolar Planet Interactions

A Tabulation of Dynamical Characteristics. Last Update: 20 July 2012. Website maintained by Miles Timpe. This page lists dynamical properties of published multiple planet systems. So far 2 parameters that quantify dynamical interactions have been identified: proximity to an apsidal separatrix, ε = 0 (see Barnes and Greenberg 2006a. And proximity to the Hill stability boundary for non-resonant systems, β = 1 (see Barnes and Greenberg 2006b. Table 1 - Dynamical Properties of Known Planetary Systems. Wright...

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Extrasolar Planet Interactions | xsp.astro.washington.edu Reviews
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A Tabulation of Dynamical Characteristics. Last Update: 20 July 2012. Website maintained by Miles Timpe. This page lists dynamical properties of published multiple planet systems. So far 2 parameters that quantify dynamical interactions have been identified: proximity to an apsidal separatrix, ε = 0 (see Barnes and Greenberg 2006a. And proximity to the Hill stability boundary for non-resonant systems, β = 1 (see Barnes and Greenberg 2006b. Table 1 - Dynamical Properties of Known Planetary Systems. Wright...
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2 apskier@u washington edu
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5 epsilon;
6 beta;
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Extrasolar Planet Interactions | xsp.astro.washington.edu Reviews

https://xsp.astro.washington.edu

A Tabulation of Dynamical Characteristics. Last Update: 20 July 2012. Website maintained by Miles Timpe. This page lists dynamical properties of published multiple planet systems. So far 2 parameters that quantify dynamical interactions have been identified: proximity to an apsidal separatrix, ε = 0 (see Barnes and Greenberg 2006a. And proximity to the Hill stability boundary for non-resonant systems, β = 1 (see Barnes and Greenberg 2006b. Table 1 - Dynamical Properties of Known Planetary Systems. Wright...

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The Exoplanet Encyclopaedia — Theoretical work

http://www.exoplanet.eu/theory

The Exoplanet Encyclopaedia — Theoretical work. A catalogue for hypothetical terrestrial planets in exoplanetary systems. Debris Disk Radiative Transfer Simulation Tool) Wolf and Hillenbrand. Orbital solutions (Balan and Lahav). 2-D polar hydro code for disk planet tidal interactions. (F. Masset). Evolution of "51 Peg b-like" Planets. The Habitable Zone Gallery. Stephen Kane and Dawn Gelino). Hydrocode Comparison for a Disc-Planet System. EU-RTN Planets and Stockholm Observatory). Burrows et al.).

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Extrasolar Planet Interactions

A Tabulation of Dynamical Characteristics. Last Update: 20 July 2012. Website maintained by Miles Timpe. This page lists dynamical properties of published multiple planet systems. So far 2 parameters that quantify dynamical interactions have been identified: proximity to an apsidal separatrix, ε = 0 (see Barnes and Greenberg 2006a. And proximity to the Hill stability boundary for non-resonant systems, β = 1 (see Barnes and Greenberg 2006b. Table 1 - Dynamical Properties of Known Planetary Systems. Wright...

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