Pallasite

Pallasites
— Class —
A slice of the Esquel pallasite, clearly showing the large olivine crystals suspended in the metal matrix.
Type	Stony-iron
Subgroups	Main group Eagle Station grouplet Pyroxene Pallasite grouplet Ungrouped Pallasites
Composition	Meteoric iron, Silicates
Total known specimens	49 Main group, 4 Eagle Station, 2 Pyroxene grouplet, 38 ungrouped (93 total)

A pallasite is a class of stony–iron meteorite.

Structure and composition

It consists of centimeter-sized olivine crystals of peridot quality in an iron-nickel matrix. Coarser metal areas develop Widmanstätten patterns upon etching. Minor constituents are schreibersite, troilite, chromite, pyroxenes, and phosphates (whitlockite, stanfieldite, farringtonite, and merrillite).^[1][2]

Classification and subgroups

Eagle Station, ES group

Using the oxygen isotopic composition, meteoric iron composition and silicate composition pallasites are divided into 4 subgroups:^[3][4]

• Main group pallasites (PMG): Almost all pallasites
• Eagle Station grouplet (PES): 4 specimens known. They are related to IIF irons.
• Pyroxene Pallasite grouplet (PPX): Counts only Vermillion and Yamato 8451. They take their name from the high orthopyroxene content (about 5%). Metal matrix shows a fine octahedrite Widmanstätten pattern.
• Pallasite ungrouped (P-ung): Specimens that don't fit into any groups or grouplets

Origin

Pallasites were once thought to originate at the core-mantle boundary of differentiated asteroids that were subsequently shattered through impacts. An alternative recent hypothesis is that they are impact-generated mixtures of core and mantle materials.^[5]

History

Krasnojarsk meteorite

A common error is to associate their name with the asteroid 2 Pallas but their actual name is after the German naturalist Peter Pallas (1741–1811), who studied in 1772 a specimen found earlier near Krasnoyarsk in the mountains of Siberia that had a mass of 680 kilograms (1,500 lb).^[6] The Krasnoyarsk mass described by Pallas in 1776 was one of the examples used by E.F.F. Chladni in the 1790s to demonstrate the reality of meteorite falls on the Earth, which were at his time considered by most scientists as fairytales. This rock mass was dissimilar to all rocks or ores found in this area (and the large piece could not have been accidentally transported to the find site), but its content of native metal was similar to other finds known from completely different areas.^[7]

Pallasite falls

Pallasites are a rare type of meteorite. Only 61 are known to date, including 10 from Antarctica, with four being observed falls.^[8][9] The following four falls are in chronological order:

• Mineo, Sicily, Italy. A luminous meteor was observed and an object seen to fall with a loud roar in May 1826. Only 46 grams (1.6 oz) are preserved in collections.
• Zaisho, Japan. 330 g were found on February 1, 1898,^[10] after the appearance of a fireball.
• Marjalahti, Karelia, Russia. After the appearance of a bright meteor and detonations, a large mass was seen to fall and 45 kilograms (99 lb) were recovered in June 1902. At this date the fall site belonged to Finland, and the main mass of Marjalahti is now at the Geological Museum of the University of Helsinki.
• Omolon, Magadan Region, Russia. A reindeer-breeder observed the fall on May 16, 1981, and found the 250 kilograms (550 lb) meteorite two years later. The fall was confirmed by a meteorological station that had observed a fireball on the same date.

Notable pallasite finds

Brenham

Imilac full slice

Although pallasites are a rare meteorite type, enough pallasite material is found in museums and meteorite collections and is available for research. This is due to large finds, some of which yielded more than a metric ton. The following are the largest finds:

• Brenham, Kansas, USA. In 1890 the find of about 20 masses with a total weight of 1,000 kilograms (2,200 lb) around the shallow Haviland Crater were reported. More masses were found later, including one of 454 kilograms (1,001 lb) from a depth of 5 feet (1.5 m), the total amounting to about 4.3 tonnes (4.2 long tons; 4.7 short tons). A piece of 487 kilograms (1,074 lb) is in the Field Museum of Natural History, Chicago. In 2005, Steve Arnold of Arkansas, USA, and Phil Mani of Texas, USA, unearthed a large mass of 650 kilograms (1,430 lb) and in 2006 several new large masses ^[11][12]
• Huckitta, Northern Territory, Australia. A mass of 1,400 kilograms (3,100 lb) was found in 1937 on a cattle station north-east of Alice Springs. Earlier, in 1924, a transported piece of about 1 kilogram (2.2 lb) had been found on Burt Plain north of Alice Springs.
• Fukang, Xinjiang Province, China. A mass of 1,003 kilograms (2,211 lb) was recovered in 2000.
• Imilac, Atacama Desert, Chile; known since 1822. Numerous masses up to 200 kilograms (440 lb) were found, the total weight is about 920 kg.
• Brahin, Gomel Region, Belarus, known since 1810. Many masses were found strewn in a field, with a total weight of about 820 kg. An additional mass of 227 kg was found at a depth of 10 feet (3.0 m) in 2002.
• Esquel, Chubut, Argentina. A large mass of 755 kg was found embedded in soil before 1951.
• Pallasovka, Pallasovka, Russia. A single mass of 198 kg was found near Pallasovka, Russia in 1990. Coincidentally, both the town of Pallasovka and pallasite meteorites were named after the naturalist, Peter Pallas.
• Krasnojarsk, Yeniseisk, Russia. A mass of about 700 kg was detected in 1749 about 145 miles (233 km) south of Krasnojarsk. It was seen by P. S. Pallas in 1772 and transported to Krasnojarsk (see above) The main mass of 515 kg is now in Moscow at the Academy of Sciences. Pallasites are named after Peter Pallas for his study of this meteorite.
• Seymchan, discovered near the town by the same name, in far eastern Russia in 1967. This main group Pallasite has some areas free of olivine crystals, and may have formed near the junction of the core and the mantle of an asteroid. Multiple masses in excess of 1 tonne have been recovered.

See also

• Glossary of meteoritics

References

1. Buseck, P.R. (1977). "Pallasite meteorites: mineralogy, petrology, and geochemistry". Geochimica et Cosmochimica Acta 41 (6): 711–740. Bibcode:1977GeCoA..41..711B. doi:10.1016/0016-7037(77)90044-8.
2. Hsu, W. (2003). "Minor element zoning and trace element geochemistry of pallasites". Meteoritics & Planetary Science 38 (8): 1217–1241. Bibcode:2003M&PS...38.1217H. doi:10.1111/j.1945-5100.2003.tb00309.x.
3. O. Richard Norton. The Cambridge encyclopedia of meteorites. Cambridge, Cambridge University Press, 2002. ISBN 0-521-62143-7.
4. M. K. Weisberg; T. J. McCoy, A. N. Krot (2006). "Systematics and Evaluation of Meteorite Classification". In D. S. Lauretta, H. Y. McSween, Jr. Meteorites and the early solar system II (PDF). Tucson: University of Arizona Press. pp. 19–52. ISBN 978-0816525621. Retrieved 15 December 2012.
5. Edward R.D. Scott, "Impact Origins for Pallasites," Lunar and Planetary Science XXXVIII, 2007.
6. P.S.Pallas, Reise durch die verschiedenen Provinzen des russischen Reichs. St.Petersburg 1776
7. E.F.F.Chladni, Observation on a mass of iron found in Siberia by Professor Pallas, and other masses of the like kind, with some conjectures respecting their connection with certain natural phenomena. Philosophical Magazine and Journal of Science, 1798, vol.2, 1-8.
8. Meteoritical Bulletin Database
9. MetBase
10. Meteorites Japan
11. Mammoth meteorite unearthed, January 2006 about the October 2005 find
12. CNN: Unusual meteorite found in Kansas, October 16, 2006.

External links

• Pallasite images from Meteorites Australia - Meteorites.com.au
• Legend of Glorieta Mountain Discovery of a large pallasite in New Mexico