  We present the discovery and characterization of a giant planet orbiting the
young Sun-like star Kepler-63 (KOI-63, $m_{\rm Kp} = 11.6$, $T_{\rm eff} =
5576$ K, $M_\star = 0.98\, M_\odot$). The planet transits every 9.43 days, with
apparent depth variations and brightening anomalies caused by large starspots.
The planet's radius is $6.1 \pm 0.2 R_{\earth}$, based on the transit light
curve and the estimated stellar parameters. The planet's mass could not be
measured with the existing radial-velocity data, due to the high level of
stellar activity, but if we assume a circular orbit we can place a rough upper
bound of $120 M_{\earth}$ (3$\sigma$). The host star has a high obliquity
($\psi$ = $104^{\circ}$), based on the Rossiter-McLaughlin effect and an
analysis of starspot-crossing events. This result is valuable because almost
all previous obliquity measurements are for stars with more massive planets and
shorter-period orbits. In addition, the polar orbit of the planet combined with
an analysis of spot-crossing events reveals a large and persistent polar
starspot. Such spots have previously been inferred using Doppler tomography,
and predicted in simulations of magnetic activity of young Sun-like stars.
