A comprehensive statistical assessment of star-planet interaction

Brendan P. Miller, Elena Gallo, Jason Wright, Elliott G. Pearson

Research output: Contribution to journalArticle

25 Citations (Scopus)

Abstract

We investigate whether magnetic interaction between close-in giant planets and their host stars produce observable statistical enhancements in stellar coronal or chromospheric activity. New Chandra observations of 12 nearby (d < 60 pc) planet-hosting solar analogs are combined with archival Chandra, XMM-Newton, and ROSAT coverage of 11 similar stars to construct a sample inoculated against inherent stellar class and planet-detection biases. Survival analysis and Bayesian regression methods (incorporating both measurements errors and X-ray upper limits; 13/23 stars have secure detections) are used to test whether "hot Jupiter" hosts are systematically more X-ray luminous than comparable stars with more distant or smaller planets. No significant correlations are present between common proxies for interaction strength (M P/a 2 or 1/a) versus coronal activity (L X or L X/L bol). In contrast, a sample of 198 FGK main-sequence stars does show a significant (99% confidence) increase in X-ray luminosity with M P/a 2. While selection biases are incontrovertibly present within the main-sequence sample, we demonstrate that the effect is primarily driven by a handful of extreme hot-Jupiter systems with M P/a 2 > 450 M Jup AU-2, which here are all X-ray luminous but to a degree commensurate with their Ca II H and K activity, in contrast to presented magnetic star-planet interaction scenarios that predict enhancements relatively larger in L X. We discuss these results in the context of cumulative tidal spin-up of stars hosting close-in gas giants (potentially followed by planetary infall and destruction). We also test our main-sequence sample for correlations between planetary properties and UV luminosity or Ca II H and K emission, and find no significant dependence.

Original languageEnglish (US)
Article number163
JournalAstrophysical Journal
Volume799
Issue number2
DOIs
StatePublished - Feb 1 2015

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planets
planet
magnetic stars
stars
augmentation
destruction
luminosity
interactions
gases
gas
x rays
test

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Miller, Brendan P. ; Gallo, Elena ; Wright, Jason ; Pearson, Elliott G. / A comprehensive statistical assessment of star-planet interaction. In: Astrophysical Journal. 2015 ; Vol. 799, No. 2.
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A comprehensive statistical assessment of star-planet interaction. / Miller, Brendan P.; Gallo, Elena; Wright, Jason; Pearson, Elliott G.

In: Astrophysical Journal, Vol. 799, No. 2, 163, 01.02.2015.

Research output: Contribution to journalArticle

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