Isochrone tracks from Demarque et al. (2004) for WASP-56 using the metallicity [Fe/H] = 0.12 dex from our spectral analysis and the best-fit stellar density 0.88 ρ_⊙. From left to right the solid lines are for isochrones of: 1.8, 2.0, 2.5, 3.0, 4.0, 5.0, 6.0, 7.0, 8.0, 9.0, 10.0, 11.0, 12.0, 13.0 and 14.0 Gyr. From left to right, dashed lines are for mass tracks of: 1.2, 1.1, 1.0, 0.9 and 0.8 M_⊙.