partially made of
chrysotile, from
Dobšiná,
Slovakia Serpentinization is a form of low-temperature (0 to ~600 °C)
metamorphism of ferromagnesian minerals in mafic and
ultramafic rocks, such as
dunite,
harzburgite, or
lherzolite. These are rocks low in
silica and composed mostly of
olivine (),
pyroxene (), and
chromite (approximately ). Serpentinization is driven largely by
hydration and
oxidation of olivine and pyroxene to
serpentine group minerals (antigorite, lizardite, and chrysotile),
brucite (),
talc (), and
magnetite (). Under the unusual chemical conditions accompanying serpentinization, water is the oxidizing agent, and is itself reduced to hydrogen, . This leads to further reactions that produce rare
iron group native element minerals, such as
awaruite () and
native iron;
methane and other
hydrocarbon compounds; and
hydrogen sulfide. During serpentinization, large amounts of water are absorbed into the rock, increasing the volume, reducing the density and destroying the original structure. The density changes from with a concurrent volume increase on the order of 30-40%. The reaction is highly
exothermic, releasing up to per mole of water reacting with the rock, and rock temperatures can be raised by about , providing an energy source for formation of non-volcanic
hydrothermal vents. The hydrogen, methane, and hydrogen sulfide produced during serpentinization are released at these vents and provide energy sources for deep sea
chemotroph microorganisms.
Serpentine can form from
olivine via several reactions: {{NumBlk|: {{NumBlk|: Reaction 1a tightly binds silica, lowering its
chemical activity to the lowest values seen in common rocks of the
Earth's crust. Serpentinization then continues through the hydration of olivine to yield serpentine and brucite (Reaction 1b). The mixture of brucite and serpentine formed by Reaction 1b has the lowest silica activity in the
serpentinite, so that the brucite phase is very important in understanding serpentinization. {{NumBlk|: Studies of serpentinites suggest that in nature iron minerals are first converted to
ferroan brucite, that is, brucite containing , which then undergoes the
Schikorr reaction in the anaerobic conditions of serpentinization: {{NumBlk|: Maximum reducing conditions, and the maximum rate of production of hydrogen, occur when the temperature of serpentinization is between and when fluids are carbonate undersaturated. Chromite present in the protolith will be altered to chromium-rich magnetite at lower serpentinization temperatures. At higher temperatures, it will be altered to iron-rich chromite (ferrit-chromite). During serpentinization, the rock is enriched in
chlorine,
boron,
fluorine, and sulfur. Sulfur will be reduced to hydrogen sulfide and sulfide minerals, though significant quantities are incorporated into serpentine minerals, and some may later be reoxidized to sulfate minerals such as
anhydrite. The sulfides produced include nickel-rich sulfides, such as
mackinawite.
Methane and other hydrocarbons Laboratory experiments have confirmed that at a temperature of and pressure of 500 bars, olivine serpentinizes with release of hydrogen gas. In addition, methane and complex hydrocarbons are formed through reduction of carbon dioxide. The process may be catalyzed by magnetite formed during serpentinization. Its presence in a serpentinite indicates either that serpentinization took place at unusually high pressure and temperature or that the rock experienced higher grade metamorphism after serpentinization was complete. Brucite rapidly converts to
magnesite and serpentine minerals (other than antigorite) are converted to talc. The presence of
pseudomorphs of the original serpentinite minerals shows that this alteration takes place after serpentinization. In 2022, it was reported that microscopic examination of the
ALH 84001 meteorite, which came from Mars, shows that indeed the organic matter it contains was formed by serpentinization, not by life processes. Using data from the
Cassini probe flybys obtained in 2010–12, scientists were able to confirm that Saturn's moon
Enceladus likely has a liquid water ocean beneath its frozen surface. A model suggests that the ocean on Enceladus has an alkaline
pH of 11–12. The high pH is interpreted to be a key consequence of serpentinization of
chondritic rock, that leads to the generation of , a geochemical source of energy that can support both abiotic and biological synthesis of organic molecules. ==Environment of formation==