  We report the discovery of eight hot-Jupiter exoplanets from the WASP-South
transit survey. WASP-144b has a mass of 0.44 Mj, a radius of 0.85 Rj, and is in
a 2.27-d orbit around a V = 12.9, K2 star which shows a 21-d rotational
modulation. WASP-145Ab is a 0.89 Mj planet in a 1.77-d orbit with a grazing
transit, which means that the planetary radius is not well constrained. The
host is a V = 11.5, K2 star with a companion 5 arcsecs away and 1.4 mags
fainter. WASP-158b is a relatively massive planet at 2.8 Mj with a radius of
1.1 Rj and a 3.66-d orbit. It transits a V = 12.1, F6 star. WASP-159b is a
bloated hot Jupiter (1.4 Rj and 0.55 Mj) in a 3.8-d orbit around a V = 12.9, F9
star. WASP-162b is a massive planet in a relatively long and highly eccentric
orbit (5.2 Mj, P = 9.6 d, e = 0.43). It transits a V = 12.2, K0 star. WASP-168b
is a bloated hot Jupiter (0.42 Mj, 1.5 Rj) in a 4.15-d orbit with a grazing
transit. The host is a V = 12.1, F9 star. WASP-172b is a bloated hot Jupiter
(0.5 Mj; 1.6 Rj) in a 5.48-d orbit around a V = 11.0, F1 star. It is likely to
be the best planet of those reported here for atmospheric characterisation.
WASP-173Ab is a massive planet (3.7 Mj) with a 1.2 Rj radius in a circular
orbit with a period of 1.39 d. The host is a V = 11.3, G3 star, being the
brighter component of the double-star system WDS23366-3437, with a companion 6
arcsecs away and 0.8 mags fainter. One of the two stars shows a rotational
modulation of 7.9 d.
