WASP-38b: A Transiting Exoplanet in an Eccentric, 6.87d Period Orbit

TL;DR

WASP-38b is a newly discovered long-period, eccentric transiting exoplanet orbiting a bright F8 dwarf star, with detailed characterization of its orbital and physical parameters enabled by upgraded detection instruments.

Contribution

This paper reports the discovery and detailed characterization of WASP-38b, the longest period planet found by SuperWASP-North, including precise measurements of its orbit and physical properties.

Findings

WASP-38b has a mass of 2.69 Mjup and radius of 1.09 Rjup.

The planet's orbit has a low eccentricity of 0.0314.

The host star is a bright F8 dwarf with Teff=6150K.

Abstract

We report the discovery of WASP-38b, a long period transiting planet in an eccentric 6.871815 day orbit. The transit epoch is 2455335.92050 +/- 0.00074 (HJD) and the transit duration is 4.663 hours. WASP-38b's discovery was enabled due to an upgrade to the SuperWASP-North cameras. We performed a spectral analysis of the host star HD 146389/BD+10 2980 that yielded Teff = 6150 +/- 80K, logg =4.3 +/- 0.1, vsini=8.6 +/- 0.4 km/s, M*=1.16 +/- 0.04 Msun and R* =1.33 +/- 0.03 Rsun, consistent with a dwarf of spectral type F8. Assuming a main-sequence mass-radius relation for the star, we fitted simultaneously the radial velocity variations and the transit light curves to estimate the orbital and planetary parameters. The planet has a mass of 2.69 +/- 0.06 Mjup and a radius of 1.09 +/-0.03 Rjup giving a density, rho_p = 2.1 +/-0.1 rho_jup. The high precision of the eccentricity e=0.0314 +/- 0.0044 is due to the relative transit timing from the light curves and the RV shape. The planet equilibrium temperature is estimated at 1292 +/- 33K. WASP-38b is the longest period planet found by SuperWASP-North and with a bright host star (V =9.4 mag), is a good candidate for followup atmospheric studies.