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We report the discovery by WASP of five planets orbiting moderately bright($V$ = 11.0-12.9) Solar-type stars. WASP-137b, WASP-143b and WASP-146b aretypical hot Jupiters in orbits of 3-4 d and with masses in the range 0.68--1.11$M_{\rm Jup}$. WASP-134 is a metal-rich ([Fe/H] = +0.40 $\pm$ 0.07]) G4 starorbited by two warm Jupiters: WASP-134b ($M_{\rm pl}$ = 1.41 $M_{\rm Jup}$; $P= 10.1$ d; $e = 0.15 \pm 0.01$; $T_{\rm eql}$ = 950 K) and WASP-134c ($M_{\rmpl} \sin i$ = 0.70 $M_{\rm Jup}$; $P = 70.0$ d; $e = 0.17 \pm 0.09$; $T_{\rmeql}$ = 500 K). From observations of the Rossiter-McLaughlin effect ofWASP-134b, we find its orbit to be misaligned with the spin of its star($\lambda = -44 \pm 10^\circ$). WASP-134 is a rare example of a system with ashort-period giant planet and a nearby giant companion. In-situ formation ordisc migration seem more likely explanations for such systems than doeshigh-eccentricity migration.

The discovery of WASP-134b, WASP-134c, WASP-137b, WASP-143b and WASP-146b: three hot Jupiters and a pair of warm Jupiters orbiting Solar-type stars