CARBON and hydrogen are only trace constituents of the Earth's mantle,
yet carbon- and hydrogen-bearing fluids have an important effect on m
agma genesis, mantle rheology and mantle chemistry. Many mantle-derive
d rocks record interactions with such fluids, but direct samples of th
e fluids themselves are rare. Diamonds, owing to their robust nature,
constitute effective sampling devices for such deep-seated fluids1; fo
r example, carbonates and water have been found2,3 in fluid inclusions
in fibrous diamonds4. In addition, CO2, H2O, CO, CH4, H-2 and N2 have
been detected in gases released from diamonds by crushing5 or heating
6,7, but their primary nature could not be confirmed beyond doubt1. He
re we report the discovery of solid CO2 in a natural diamond. Infrared
spectroscopy indicates that the CO2 is presently at a pressure of 5 G
Pa (50 kbar), and must therefore have been trapped at even greater pre
ssures in the hot mantle, corresponding to depths of about 220-270 km.
At these pressures, free CO2 should react with olivine and pyroxene;
thus, its survival indicates the presence at depth of an environment o
f different mineralogy such as a fully carbonated metasomatic vein, or
a block of subducted sediments.