WASP-74 is a star in the constellation of Aquila, located approximately 487 light-years (149 parsecs) from the Sun. At least one exoplanet is known to orbit the star.
Stellar characteristics WASP-74 is a yellow-white subgiant of spectral type F9. Its apparent magnitude is 9.75, making it invisible to the naked eye. Based on spectroscopic analysis with the HARPS-N spectrograph and Bayesian modelling using PARSEC isochrones, the star has a mass of 1.236 ± 0.026 solar masses, a radius of 1.444±0.044 solar radii, and an effective temperature of 5,883±57 K. Its metallicity ([Fe/H]) is +0.38±0.03, indicating it is notably more metal-rich than the Sun. Stellar models give an age of 3.49±0.65 billion years, and the star's projected rotational velocity is 5.85±0.50 km/s. The star's proper motion is 1.350±0.082 mas/yr in right ascension and −64.604±0.060 mas/yr in declination, with a radial velocity of −15.32±0.27 km/s.
Planetary system In 2015, one exoplanet was announced orbiting WASP-74, designated WASP-74 b, discovered by the SuperWASP survey using the transit method. It is a hot Jupiter with a mass of 0.72 Jupiter masses and a radius of 1.312 Jupiter radii, completing one orbit every 2.13775138 days at a distance of 0.0334 AU from its host star, with an equilibrium temperature of approximately 1,865 K. The planet's orbit is circular and well-aligned with the stellar equator, with a measured sky-projected spin-orbit angle of 0.77±0.99 degrees.
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