  We report 33 V-band observations by the Hereford Arizona Observatory (HAO) of
the enigmatic star KIC 8462852 during the two week period 3-17 August 2017. We
find a striking resemblance of these observations to the Kepler day 1540 dip
with HAO observations tracking the Kepler light curve (adjusted for egress
symmetry). A possible explanation of this potential repeat transit is a brown
dwarf and extensive ring system in a 1601-day eccentric orbit. We suggest this
object may be detectable through radial velocity observations in October and
November 2017, with an amplitude of ~ 1-2 kms-1.
