A Decade of Hα Transits for HD 189733 b: Stellar Activity versus Absorption in the Extended Atmosphere

P. Wilson Cauley, Seth Redfield, Adam G. Jensen

Research output: Contribution to journalArticle

16 Citations (Scopus)

Abstract

HD 189733 b is one of the most well studied exoplanets due to its large transit depth and host star brightness. The focus on this object has produced a number of high-cadence transit observations using high-resolution optical spectrographs. Here we present an analysis of seven full Hα transits of HD 189733 b using HARPS on the 3.6 meter La Silla telescope and HIRES on Keck I, taken over the course of nine years from 2006 to 2015. Hα transmission signals are analyzed as a function of the stellar activity level, as measured using the normalized core flux of the Ca ii H and K lines. We find strong variations in the strength of the Hα transmission spectrum from epoch to epoch. However, there is no clear trend between the Ca ii core emission and the strength of the in-transit Hα signal, although the transit showing the largest absorption value also occurs when the star is the most active. We present simulations of the in-transit contrast effect and find that the planet must consistently transit active latitudes with very strong facular and plage emission regions in order to reproduce the observed line strengths. We also investigate the measured velocity centroids with models of planetary rotation and show that the small line profile velocities could be due to large velocities in the upper atmosphere of the planet. Overall, we find it more likely that the measured Hα signals arise in the extended planetary atmosphere, although a better understanding of active region emission for active stars such as HD 189733 is needed.

Original languageEnglish (US)
Article number217
JournalAstronomical Journal
Volume153
Issue number5
DOIs
StatePublished - May 2017

Fingerprint

stellar activity
transit
atmospheres
atmosphere
planet
planetary rotation
planetary atmosphere
upper atmosphere
velocity profile
stars
planets
time measurement
H lines
faculae
planetary atmospheres
K lines
signal transmission
extrasolar planets
simulation
centroids

Keywords

  • planets and satellites: atmospheres
  • planets and satellites: individual (HD 189733 b)
  • stars: activity
  • stars: individual (HD 189733)
  • techniques: spectroscopic

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

A Decade of Hα Transits for HD 189733 b : Stellar Activity versus Absorption in the Extended Atmosphere. / Cauley, P. Wilson; Redfield, Seth; Jensen, Adam G.

In: Astronomical Journal, Vol. 153, No. 5, 217, 05.2017.

Research output: Contribution to journalArticle

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