  We report the discovery of two transiting exoplanets from the WASP survey,
WASP-150b and WASP-176b. WASP-150b is an eccentric ($e$ = 0.38) hot Jupiter on
a 5.6 day orbit around a $V$ = 12.03, F8 main-sequence host. The host star has
a mass and radius of 1.4 $\rm M_{\odot}$ and 1.7 $\rm R_{\odot}$ respectively.
WASP-150b has a mass and radius of 8.5 $\rm M_J$ and 1.1 $\rm R_J$, leading to
a large planetary bulk density of 6.4 $\rm \rho_J$. WASP-150b is found to be
$\sim3$ Gyr old, well below its circularisation timescale, supporting the
eccentric nature of the planet. WASP-176b is a hot Jupiter planet on a 3.9 day
orbit around a $V$ = 12.01, F9 sub-giant host. The host star has a mass and
radius of 1.3 $\rm M_{\odot}$ and 1.9 $\rm R_{\odot}$. WASP-176b has a mass and
radius of 0.86 $\rm M_J$ and 1.5 $\rm R_J$ respectively, leading to a planetary
bulk density of 0.23 $\rm \rho_J$.
