PLANET-PLANET SCATTERING LEADS TO TIGHTLY PACKED PLANETARY SYSTEMS
- Center for Astrophysics and Space Astronomy, 389 UCB, University of Colorado, Boulder, CO 80309 (United States)
- Department of Astronomy, University of Washington, Seattle, WA 98195 (United States)
- Astronomy Department, University of Florida, Gainesville, FL 32111 (United States)
- JILA, University of Colorado, Boulder, CO 80309 (United States)
- Google, Inc., 1600 Amphitheatre Parkway, Mountain View, CA 94043 (United States)
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ (United States)
The known extrasolar multiple-planet systems share a surprising dynamical attribute: they cluster just beyond the Hill stability boundary. Here we show that the planet-planet scattering model, which naturally explains the observed exoplanet eccentricity distribution, can reproduce the observed distribution of dynamical configurations. We calculated how each of our scattered systems would appear over an appropriate range of viewing geometries; as Hill stability is weakly dependent on the masses, the mass-inclination degeneracy does not significantly affect our results. We consider a wide range of initial planetary mass distributions and find that some are poor fits to the observed systems. In fact, many of our scattering experiments overproduce systems very close to the stability boundary. The distribution of dynamical configurations of two-planet systems may provide better discrimination between scattering models than the distribution of eccentricity. Our results imply that, at least in their inner regions which are weakly affected by gas or planetesimal disks, planetary systems should be 'packed', with no large gaps between planets.
- OSTI ID:
- 21300739
- Journal Information:
- Astrophysical Journal (Online), Vol. 696, Issue 1; Other Information: DOI: 10.1088/0004-637X/696/1/L98; Country of input: International Atomic Energy Agency (IAEA); ISSN 1538-4357
- Country of Publication:
- United States
- Language:
- English
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