  Context. The CoRoT space mission routinely provides high-precision
photometric measurements of thousands of stars that have been continuously
observed for months.
  Aims. The discovery and characterization of the first very massive transiting
planetary companion with a short orbital period is reported.
  Methods. A series of 34 transits was detected in the CoRoT light curve of an
F3V star, observed from May to October 2007 for 152 days. The radius was
accurately determined and the mass derived for this new transiting, thanks to
the combined analysis of the light curve and complementary ground-based
observations: high-precision radial-velocity measurements, on-off photometry,
and high signal-to-noise spectroscopic observations.
  Results. CoRoT-Exo-3b has a radius of 1.01+-0.07 RJup and transits around its
F3-type primary every 4.26 days in a synchronous orbit. Its mass of 21.66+-1.0
MJup, density of 26.4+-5.6 g cm^-3, and surface gravity of log g = 4.72 clearly
distinguish it from the regular close-in planet population, making it the most
intriguing transiting substellar object discovered so far.
  Conclusions. With the current data, the nature of CoRoT-Exo-3b is ambiguous,
as it could either be a low-mass brown-dwarf or a member of a new class of
"superplanets". Its discovery may help constrain the evolution of close-in
planets and brown-dwarfs better. Finally, CoRoT-Exo-3b confirms the trend that
massive transiting giant planets (M >= 4 MJup) are found preferentially around
more massive stars than the Sun.
