Schreibersite | |
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General | |
Category | Phosphide mineral Meteorite mineral |
Formula (repeating unit) | (Fe,Ni)3P |
IMA symbol | Scb [1] |
Strunz classification | 1.BD.05 |
Dana classification | 01.01.21.02 |
Crystal system | Tetragonal |
Crystal class | Disphenoidal (4) H-M symbol: (4) |
Space group | I4 |
Identification | |
Color | Silver-white to tin-white, tarnishes brass-yellow or brown |
Crystal habit | Rarely in crystals, hoppered, plates, tablets, rods or needles |
Cleavage | {001} perfect, {010} indistinct, {110} indistinct |
Tenacity | Very brittle |
Mohs scale hardness | 6.5–7 |
Luster | Brilliant metallic |
Streak | Dark gray |
Diaphaneity | Opaque |
Specific gravity | 7.0–7.3 |
Optical properties | Uniaxial |
References | [2] [3] [4] |
Schreibersite is generally a rare iron nickel phosphide mineral, (Fe,Ni)3P, though common in iron-nickel meteorites. It has been found on Disko Island in Greenland [5] and Illinois. [6] [7]
Another name used for the mineral is rhabdite. It forms tetragonal crystals with perfect 001 cleavage. Its color ranges from bronze to brass yellow to silver white. It has a density of 7.5 and a hardness of 6.5 – 7. It is opaque with a metallic luster and a dark gray streak. It was named after the Austrian scientist Carl Franz Anton Ritter von Schreibers (1775–1852), who was one of the first to describe it from iron meteorites. [3]
Schreibersite is reported from the Magura Meteorite, Arva-(present name – Orava), Slovak Republic; the Sikhote-Alin Meteorite in eastern Russia; the São Julião de Moreira Meteorite, Viana do Castelo, Portugal; the Gebel Kamil (meteorite) in Egypt; and numerous other locations including the Moon. [8]
In 2007, researchers reported that schreibersite and other meteoric phosphorus bearing minerals may be the ultimate source for the phosphorus that is so important for life on Earth. [9] [10] [11] In 2013, researchers reported that they had successfully produced pyrophosphite, a possible precursor to pyrophosphate, the molecule associated with ATP, a co-enzyme central to energy metabolism in all life on Earth. Their experiment consisted of subjecting a sample of schreibersite to a warm, acidic environment typically found in association with volcanic activity, activity that was far more common on the primordial Earth. They hypothesized that their experiment might represent what they termed "chemical life", a stage of evolution which may have led to the emergence of fully biological life as exists today. [12]
In 1986 researchers found lightning can create schreibersite [13] and may have been the source of phosphorus for early life. [14] [6] [7]
Fulgurites, commonly known as "fossilized lightning", are natural tubes, clumps, or masses of sintered, vitrified, and/or fused soil, sand, rock, organic debris and other sediments that sometimes form when lightning discharges into ground. When composed of silica, fulgurites are classified as a variety of the mineraloid lechatelierite.
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An iron meteorite fell on the Sikhote-Alin Mountains, in southeastern Russia, in 1947. Large iron meteorite falls have been witnessed and fragments recovered but never before, in recorded history, a fall of this magnitude. An estimated 23 tonnes of fragments survived the fiery passage through the atmosphere and reached the Earth.
Cohenite is a naturally occurring iron carbide mineral with the chemical structure (Fe, Ni, Co)3C. This forms a hard, shiny, silver mineral which was named by E. Weinschenk in 1889 after the German mineralogist Emil Cohen, who first described and analysed material from the Magura meteorite found near Slanica, Žilina Region, Slovakia. Cohenite is found in rod-like crystals in iron meteorites.
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Tetrataenite is a native metal alloy composed of chemically-ordered L10-type FeNi, recognized as a mineral in 1980. The mineral is named after its tetragonal crystal structure and its relation to the iron-nickel alloy, taenite. It is one of the mineral phases found in meteoric iron.
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Carlsbergite is a nitride mineral that has the chemical formula CrN, or chromium nitride.
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