bredigite
Formula: Ca4[Mg8Fe3+2Ti2]O4[Si6Al6O36]
Inosilicate (chain silicate), rhönite group
Crystal System: Triclinic
Specific gravity: 3.4 to 3.76 measured
Hardness: 5 to 6
Colour: Brown-red, black to reddish black
Environments
Igneous environments
Extraterrestrial environments
Rhönite occurs in silica-undersaturated, alkalic, mafic to
intermediate igneous rocks, as a primary mineral, or as an
alteration of amphiboles. It is also developed at the contact of alkalic
basalt and limestone.
Associated minerals include titanium-bearing
augite,
kaersutite, alkalic feldspar,
diopside, forsterite,
spinel, perovskite,
titanium-bearing
magnetite and magnesioferrite
(HOM).
Localities
At the Hut Point Peninsula, Ross Island, Ross Archipelago, Victoria Land, Eastern Antarctica, the McMurdo Volcanic
Group consists of undersaturated alkaline volcanics which range in composition from alkali
olivine basalt and
basanite to trachyte
and phonolite.
A detailed examination revealed no primary rhönite in the surface flows, but rhönite grains were found
in three samples of porphyritic
olivine basanite as
microphenocrysts which rarely reach 0.2 mm in length. The rhönite is usually intergrown with or surrounded by
pyroxene
(AM 60.722-725).
At Puy de Barbeire, Massif Central, France, rhönite occurs in
nepheline dolerites
(Dana).
at Puy Foretier, Haute-Loire, Auvergne-Rhône-Alpes, France, rhönite occurs in an inclusion of
pyroxenite in basalt
(Dana).
At the type locality, the Rhön Mountains, Germany, rhönite occurs in
nepheline basanite
(Dana).
At the Allende meteorite, Pueblito de Allende, Chihuahua, Mexico, rhönite has been found which contains both
Ti3+ ande Ti4+
(Dana).
At Pulling Point, Dunedin City, Otago Region, South Island, New Zealand, rhönite occurs within alteration rims on
kaersutite crystals, together with
titanium-bearing augite,
olivine, plagioclase,
apatite and titanium-bearing
magnetite. These minerals make up coarse-grained xenoliths to 1 cm in a
nepheline hawaiite. The host
rock is composed of a groundmass of plagioclase, pale green
clinopyroxene, interstitial nepheline
and titanium-bearing
magnetite, in which are set phenocrysts of
titanium-bearing augite,
olivine, and kaersutite
(AM 60.722-725).
In the Koloa Volcanic Series, Kauai Island, Kauai County, Hawaii, USA, rhönite occurs only in the alkali
gabbro as tiny phenocrysts or as epitaxial overgrowths on
crystals of Fe-bearing diopside
(AM 69.57-68).
At Location 159, Big Bend National Park, Brewster county, Texas, USA, the intrusion in which rhönite is found is
a sill composed of two rock types, a variety of basanite and a dark
syenite overlying it. The rhönite is found only in the
syenite, where it is present in significant amounts of 5% to 15%. The
syenite is usually
porphyritic with phenocrysts of
titanium-bearing augite, rhönite,
olivine, nepheline and
plagioclase, set in a groundmass of
K-felspar, microlites and
zeolites. Phenocrysts of rhönite up to 4 mm in length have been observed.
Rhönite, titanium-bearing augite,
and plagioclase crystallised early, preceding
nepheline and K-felspar. The
rhönite is commonly intergrown with
titanium-bearing augite, and rarely with
olivine
(AM 55.864-874).
On the Moon, grains of rhönite have been discovered in magmatic inclusions in
augite grains of the lunar regolith from
Mare Crisium, returned to Earth by the Russian Luna 24 spacecraft. These rhönite grains are up to 8 μm long
(AM 93.488-491).
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