Planet Hunters X. KIC 8462852 - Where's the Flux?

Authors:
  • TBT. S. Boyajian
    T. S. Boyajian
  • DLD. M. LaCourse
    D. M. LaCourse
  • SRS. A. Rappaport
    S. A. Rappaport
  • DFD. Fabrycky
    D. Fabrycky
  • DFD. A. Fischer
    D. A. Fischer
  • DGD. Gandolfi
    D. Gandolfi
  • GKG. M. Kennedy
    G. M. Kennedy
  • MLM. C. Liu
    M. C. Liu
  • AMA. Moor
    A. Moor
  • KOK. Olah
    K. Olah
  • KVK. Vida
    K. Vida
  • MWM. C. Wyatt
    M. C. Wyatt
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Abstract
Over the duration of the Kepler mission, KIC 8462852 was observed to undergo irregularly shaped, aperiodic dips in flux down to below the 20% level. The dipping activity can last for between 5 and 80 days. We characterize the object with high-resolution spectroscopy, spectral energy distribution fitting, and Fourier analyses of the Kepler light curve. We determine that KIC 8462852 is a main-sequence F3 V/IV star, with a rotation period ~0.88 d, that exhibits no significant IR excess. In this paper, we describe various scenarios to explain the mysterious events in the Kepler light curve, most of which have problems explaining the data in hand. By considering the observational constraints on dust clumps orbiting a normal main-sequence star, we conclude that the scenario most consistent with the data is the passage of a family of exocomet fragments, all of which are associated with a single previous breakup event. We discuss the necessity of future observations to help interpret the system.