Schreibersite
| Schreibersite | |
|---|---|
 | |
| General | |
| Category |
Phosphide mineral Meteorite mineral |
| Formula (repeating unit) | (Fe,Ni)3P |
| Strunz classification | 01.BD.05 |
| Dana classification | 01.01.21.02 |
| Identification | |
| Color | Silver-white to tin-white, tarnishes brass-yellow or brown |
| Crystal habit | Rarely in crystals, hoppered, plates, tablets, rods or needles |
| Crystal system | Tetragonal - Disphenoidal H-M Symbol (4) |
| 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 | [1][2][3] |
Schreibersite is generally a rare iron nickel phosphide mineral, (Fe,Ni)3P, though common in iron-nickel meteorites. The only known occurrence of the mineral on Earth is located on Disko Island in Greenland.[4]
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.[2]
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; and numerous other locations including the Moon.[5]
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.[6][7][8] 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.[9]
See also
References
- ↑ Mindat.org
- ↑ 2.0 2.1 Webmineral.com
- ↑ http://rruff.geo.arizona.edu/doclib/hom/schreibersite.pdf Handbook of Mineralogy
- ↑ "Power behind primordial soup discovered", Eurekalert, April 4, 2013
- ↑ Hunter R. H. and Taylor L. A. 1981: Rust and schreibersite in Apollo 16 highland rocks - Manifestations of volatile-element mobility -
- ↑ Report of U of A Extra-terrestrial Phosphorus
- ↑ The Limits of Organic Life in Planetary Systems (2007): The Origin of Phosphorus
- ↑ Life's Fifth Element Came From Meteors: Discover Magazine (January 2005)
- ↑ "Hydrothermal modification of the Sikhote-Alin iron meteorite under low pH geothermal environments. A plausibly prebiotic route to activated phosphorus on the early Earth", Bryant et al, Geochimica et Cosmochimica Acta, Volume 109, 15 May 2013, Pages 90-112, ISSN 0016-7037, 10.1016/j.gca.2012.12.043
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