Deserts and pile-ups in the distribution of exoplanets due to photoevaporative disc clearing

R. D. Alexander, I. Pascucci

Research output: Contribution to journalArticle

47 Scopus citations

Abstract

We present models of giant planet migration in evolving protoplanetary discs. We show that disc clearing by extreme-ultraviolet photoevaporation can have a strong effect on the distribution of giant planet semimajor axes. During disc clearing, planet migration is slowed or accelerated in the region where photoevaporation opens a gap in the disc, resulting in 'deserts' where few giant planets are found and corresponding 'pile-ups' at smaller and larger radii. However, the precise locations and sizes of these features are strong functions of the efficiency of planetary accretion, and therefore also strongly dependent on planet mass. We suggest that photoevaporative disc clearing may be responsible for the pile-up of ~Jupitermass planets at ~1 au seen in exoplanet surveys, and show that observations of the distribution of exoplanet semimajor axes can be used to test models of both planet migration and disc clearing.

Original languageEnglish (US)
Pages (from-to)L82-L86
JournalMonthly Notices of the Royal Astronomical Society: Letters
Volume422
Issue number1
DOIs
StatePublished - May 1 2012

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Keywords

  • Accretion
  • Accretion discs
  • Planet-disc interactions
  • Planetary systems
  • Planets and satellites: formation
  • Protoplanetary discs

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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