WASP-43b: The closest-orbiting hot Jupiter
Coel Hellier (Keele), D.R. Anderson, A. Collier Cameron, M. Gillon, E., Jehin, M. Lendl, P.F.L. Maxted, F. Pepe, D. Pollacco, D. Queloz, D., Segransan, B. Smalley, A.M.S. Smith, J. Southworth, A.H.M.J. Triaud, S. Udry, and R.G. West

TL;DR
This paper reports the discovery of WASP-43b, a hot Jupiter with the shortest orbital distance known, orbiting a low-mass K7V star, highlighting the existence of such planets around stars with deep convection zones.
Contribution
The discovery of WASP-43b, the closest-orbiting hot Jupiter around a low-mass star, expands understanding of planetary systems around stars with deep convection zones.
Findings
WASP-43b has the shortest known orbital distance for a hot Jupiter.
The host star is the lowest-mass star known to host a hot Jupiter.
The planet's orbit suggests potential for tidal decay studies.
Abstract
We report the discovery of WASP-43b, a hot Jupiter transiting a K7V star every 0.81 d. At 0.6-Msun the host star has the lowest mass of any star hosting a hot Jupiter. It also shows a 15.6-d rotation period. The planet has a mass of 1.8 Mjup, a radius of 0.9 Rjup, and with a semi-major axis of only 0.014 AU has the smallest orbital distance of any known hot Jupiter. The discovery of such a planet around a K7V star shows that planets with apparently short remaining lifetimes owing to tidal decay of the orbit are also found around stars with deep convection zones.
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