The Mars Global Surveyor spacecraft obtained globally-distributed vector ma
gnetic field measurements approximately 400 km above the surface of Mars. T
hese have been compiled to produce the first complete global magnetic field
maps of Mars. Crustal magnetization appears dichotomized, with intense mag
netization mainly confined to the ancient, heavily cratered highlands in th
e south. The global distribution of sources is consistent with a reversing
dynamo that halted early in Mars evolution. Intense crustal magnetization r
equires an increased oxidation state relative to mantle-derived rock, consi
stent with assimilation of an aqueous component at crustal depths.