  Precision Doppler velocity measurements from the Anglo-Australian Tele- scope
reveal a planet with a 9.4+/-0.4 year period orbiting the M1.5 dwarf GJ 832.
Within measurement uncertainty the orbit is circular, and the minimum mass (m
sin i) of the planet is 0.64+/-0.06 MJUP. GJ 832 appears to be depleted in met-
als by at least 50% relative to the Sun, as are a significant fraction of the M
dwarfs known to host exoplanets. GJ 832 adds another Jupiter-mass planet to the
known census of M dwarf exoplanets, which currently includes a significant
number of Neptune-mass planets. GJ 832 is an excellent candidate for astromet-
ric orbit determination with alpha sin i = 0.95 mas. GJ 832b has the second
largest angular distance from its star among radial velocity detected
exoplanets (0.69 arc sec) making it a potentially interesting target for future
direct detection.
