Olivine is named for its typically olive-green color, thought to be a result of traces of
nickel, though it may alter to a reddish color from the oxidation of iron. Translucent olivine is sometimes used as a
gemstone called
peridot (
péridot, the
French word for olivine). It is also called chrysolite (or
chrysolithe, from the
Greek words for
gold and stone), though this name is now rarely used in the English language. Some of the finest gem-quality olivine has been obtained from a body of
mantle rocks on
Zabargad Island in the
Red Sea. Olivine occurs in both
mafic and
ultramafic igneous rocks and as a primary mineral in certain
metamorphic rocks. Mg-rich olivine crystallizes from
magma that is rich in magnesium and low in
silica. That magma crystallizes to mafic rocks such as
gabbro and
basalt. Ultramafic rocks usually contain substantial olivine, and those with an olivine content of over 40% are described as
peridotites.
Dunite has an olivine content of over 90% and is likely a
cumulate formed by olivine crystallizing and settling out of magma or a
vein mineral lining magma conduits. Olivine and high pressure structural variants constitute over 50% of the Earth's upper mantle, and olivine is one of the Earth's most common minerals by volume. The
metamorphism of impure
dolomite or other
sedimentary rocks with high magnesium and low silica content also produces Mg-rich olivine, or
forsterite. Fe-rich olivine
fayalite is relatively much less common, but it occurs in
igneous rocks in small amounts in rare
granites and
rhyolites, and extremely Fe-rich olivine can exist stably with
quartz and
tridymite. In contrast, Mg-rich olivine does not occur stably with
silica minerals, as it would react with them to form
orthopyroxene (). Mg-rich olivine is stable to pressures equivalent to a depth of about within Earth. Because it is thought to be the most abundant mineral in Earth's mantle at shallower depths, the properties of olivine have a dominant influence upon the
rheology of that part of Earth and hence upon the solid flow that drives
plate tectonics. Experiments have documented that olivine at high pressures (12
GPa, the pressure at depths of about ) can contain at least as much as about 8900 parts per million (weight) of water, and that such water content drastically reduces the resistance of olivine to solid flow. Moreover, because olivine is so abundant, more water may be dissolved in olivine of the mantle than is contained in Earth's oceans. Olivine pine forest (a
plant community) is unique to Norway. It is rare and found on dry olivine ridges in the fjord districts of Sunnmøre and Nordfjord. File:Papakolea Beach sand high mag 052915.jpg|Olivine grains that eroded from
lava on
Papakolea Beach,
Hawaii File:Peridot in basalt.jpg|Light green olivine crystals in peridotite xenoliths in basalt from Arizona File:Lunar Olivine Basalt 15555 from Apollo 15 in National Museum of Natural History.jpg|Olivine
basalt from the Moon, collected in 1971 by the crew of
Apollo 15 File:Forsterite-158776.jpg|Bright green olivine from Pakistan, showing chisel termination and silky luster File:Lava - Olivine - Azores.jpg|Olivine in lava from the
Azores Extraterrestrial occurrences , a
pallasite meteorite Mg-rich olivine has also been discovered in
meteorites, on the
Moon and
Mars, falling into infant stars, as well as on asteroid
25143 Itokawa. Such meteorites include
chondrites, collections of debris from the early
Solar System; and
pallasites, mixes of iron-nickel and olivine. The rare
A-type asteroids are suspected to have a surface dominated by olivine. The
spectral signature of olivine has been seen in the dust disks around young stars. The tails of comets (which formed from the dust disk around the young
Sun) often have the spectral signature of olivine, and the presence of olivine was verified in samples of a comet from the
Stardust spacecraft in 2006. Comet-like (magnesium-rich) olivine has also been detected in the
planetesimal belt around the star
Beta Pictoris. ==Crystal structure==