2007. The American Astronomical Society. All rights reserved. Printed in U.S.A. TrES-3: A NEARBY, MASSIVE, TRANSITING HOT JUPITER IN A 31 HOUR ORBIT1

We describe the discovery of a massive transiting hot Jupiter with a very short orbital period (1.30619 days), which we name TrES-3. From spectroscopy of the host star GSC 0308900929, we measure T p 5720eff K, , and km s1 and derive a stellar mass of. We estimate a150 log gp 4.6 0.3 v sin i! 2 0.90 0.15 M, planetary mass of, based on the sinusoidal variation of our high-precision radial velocity1.92 0.23 MJup measurements. This variation has a period and phase consistent with our transit photometry. Our spectra show no evidence of line bisector variations that would indicate a blended eclipsing binary star. From detailed modeling of our B and z photometry of the 2.5 % deep transits, we determine a stellar radius and a0.802 0.046 R, planetary radius. TrES-3 has one of the shortest orbital periods of the known transiting1.295 0.081 RJup exoplanets, facilitating studies of orbital decay and mass loss due to evaporation, and making it an excellent target for future studies of infrared emission and reflected starlight