WASP-37b: A 1.8<i>M</i><sub>J</sub>EXOPLANET TRANSITING A METAL-POOR STAR

E. K. Simpson, F. Faedi, S. C. C. Barros, D. J. A. Brown, A. Collier Cameron, Leslie Hebb, D. Pollacco, B. Smalley, Ian A. Todd, O. W. Butters,

The Astronomical Journal · 2010 · 54 citations · 72 references

DOIFull text

Open access

Concepts

Abstract

We report on the discovery of WASP-37b, a transiting hot Jupiter orbiting an mv = 12.7 G2-type dwarf, with a period of 3.577469 ± 0.000011 d, transit epoch T0 = 2455338.6188 ± 0.0006 (HJD; dates throughout the paper are given in Coordinated Universal Time (UTC)), and a transit duration 0.1304-0.0017 +0.0018 d. The planetary companion has a mass Mp = 1.80 ± 0.17 MJ and radius R p = 1.16-0.06 +0.07 RJ, yielding a mean density of 1.15-0.15 +0.12 ρJ. From a spectral analysis, we find that the host star has M* = 0.925 ± 0.120M⊙, R* = 1.003 ± 0.053 R⊙, Teff = 5800 ± 150 K, and [Fe/H] = -0.40 ± 0.12. WASP-37 is therefore one of the lowest metallicity stars to host a transiting planet

References

72