The on/off nature of star-planet interactions

Evgenya Shkolnik, David A. Bohlender, Gordon A H Walker, Andrew Collier Cameron

Research output: Contribution to journalArticle

154 Citations (Scopus)

Abstract

Evidence suggesting an observable magnetic interaction between a star and its hot Jupiter appears as a cyclic variation of stellar activity synchronized to the planet's orbit. In this study we monitored the chromospheric activity using several stellar activity indicators of seven stars with hot Jupiters using new high-resolution echelle spectra collected with ESPaDOnS over a few nights in 2005 and 2006 from the CFHT (Ca II H λ3968, K λ3933, the Ca II infrared triplet [IRT] λ8662 line, Hα λ6563, and He I λ5876). Synchronicity of the Ca II H and K emission of HD 179949 with its planet's orbit is clearly seen in four out of six epochs, while rotational modulation with Prot = 7 days is apparent in the other two seasons. We observe a similar phenomenon on v And. This on/off nature of star-planet interaction (SPI) in the two systems is likely a function of the changing stellar magnetic field structure throughout its activity cycle. Variability in the transiting system HD 189733 is likely associated with an active region rotating with the star; however, the flaring in excess of the rotational modulation may be associated with its hot Jupiter. As for HD 179949, the peak variability as measured by the mean absolute deviation (MAD) for both HD 189733 and τ Boo leads the subplanetary longitude by ∼70°. The tentative correlation between this activity and the ratio of Mp sin i to the planet's rotation period, a quantity proportional to the hot Jupiter's magnetic moment, first presented by Shkolnik and coworkers remains viable. This work furthers the characterization of SPI, improving its otential as a probe of extrasolar planetary magnetic fields.

Original languageEnglish (US)
Pages (from-to)628-638
Number of pages11
JournalAstrophysical Journal
Volume676
Issue number1
DOIs
StatePublished - Mar 20 2008
Externally publishedYes

Fingerprint

planets
Jupiter (planet)
planet
Jupiter
stars
stellar activity
interactions
planetary magnetic fields
stellar magnetic fields
magnetic field
orbits
modulation
longitude
night
magnetic moments
time measurement
probe
deviation
probes
high resolution

Keywords

  • Planetary systems
  • Radiation mechanisms: nonthermal
  • Stars: activity
  • Stars: chromospheres
  • Stars: individual (τ Boo, HD 179949, HD 209458, HD 189733, HD 217107, HD 149143)
  • Stars: late-type

ASJC Scopus subject areas

  • Nuclear and High Energy Physics
  • Space and Planetary Science

Cite this

Shkolnik, E., Bohlender, D. A., Walker, G. A. H., & Cameron, A. C. (2008). The on/off nature of star-planet interactions. Astrophysical Journal, 676(1), 628-638. https://doi.org/10.1086/527351

The on/off nature of star-planet interactions. / Shkolnik, Evgenya; Bohlender, David A.; Walker, Gordon A H; Cameron, Andrew Collier.

In: Astrophysical Journal, Vol. 676, No. 1, 20.03.2008, p. 628-638.

Research output: Contribution to journalArticle

Shkolnik, E, Bohlender, DA, Walker, GAH & Cameron, AC 2008, 'The on/off nature of star-planet interactions', Astrophysical Journal, vol. 676, no. 1, pp. 628-638. https://doi.org/10.1086/527351
Shkolnik E, Bohlender DA, Walker GAH, Cameron AC. The on/off nature of star-planet interactions. Astrophysical Journal. 2008 Mar 20;676(1):628-638. https://doi.org/10.1086/527351
Shkolnik, Evgenya ; Bohlender, David A. ; Walker, Gordon A H ; Cameron, Andrew Collier. / The on/off nature of star-planet interactions. In: Astrophysical Journal. 2008 ; Vol. 676, No. 1. pp. 628-638.
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