Tightly packed planetary systems

Research output: Chapter in Book/Report/Conference proceedingChapter

Abstract

Many exoplanet systems are tightly packed on orbits unnervingly near instability. Here we review theories for the origin of tightly packed systems and how their properties constrain how planetary systems form and evolve. We begin with a pedagogical overview of packing metrics and their connection to resonance overlap and instability. We highlight an additional scale, the escape velocity from the surface of the planet, that causes dynamical behavior to vary with host star separation. Next we discuss how tightly packed systems inform us about planet formation conditions, if and how planets migrate, and survival in chaotic configurations. Along the way, we highlight several examples of packed exoplanet systems-the Kepler-11, Kepler-36, and HR 8799-and compare them to Solar System benchmarks. We conclude with a discussion about unifying the three packing perspectives of formation, migration, and stability.

Original languageEnglish (US)
Title of host publicationHandbook of Exoplanets
PublisherSpringer International Publishing
Pages2713-2730
Number of pages18
ISBN (Electronic)9783319553337
ISBN (Print)9783319553320
DOIs
StatePublished - Nov 3 2018

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)
  • Earth and Planetary Sciences(all)

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    Dawson, R. I. (2018). Tightly packed planetary systems. In Handbook of Exoplanets (pp. 2713-2730). Springer International Publishing. https://doi.org/10.1007/978-3-319-55333-7_114