Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007dda....38.1506t&link_type=abstract
American Astronomical Society, DDA meeting #38, #15.06
Astronomy and Astrophysics
Astronomy
Scientific paper
Planets locked in mean-motion resonances are a natural outcome of migration in a gas disk, but how durable are such configurations? I will show how mean-motion resonances may commonly be disrupted later in a system's evolution, sometimes violently so. The extrasolar planets observed to be in mean-motion resonances may thus be just the survivors of an originally larger resonant population. Even our own Solar System may have started out this way.
Bryden Geoff
Rasio Fred
Thommes Edward
Wu Yihong
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