"},"Structural_classification":{"wt":""},"Composition":{"wt":"[[Meteoric iron]] (8 % Ni),[[Silicate]] inclusions"},"Shock":{"wt":""},"Weathering":{"wt":""},"Country":{"wt":"[[Tanzania]]"},"Region":{"wt":"[[Songwe Region|Songwe]]"},"Lat_Long":{"wt":"{{coord|09|06|28|S|33|02|15|E|display=inline,title}}{{cite book |last=Buchwald |first=Vagn F. |author-link=Vagn Buchwald |year=1975 |title=Handbook of Iron Meteorites. Their History,Distribution,Composition and Structure |url=https://evols.library.manoa.hawaii.edu/collections/057021e1-6d10-4cc0-926f-1915445fa95f |volume=2:Iron Meteorites:''Abakan - Mejillones'' |publisher=[[University of California Press]] |page=814 |isbn=0-520-02934-8 |access-date=2024-09-12}}{{efn|Coordinates were verified using satellite images.}}"},"Observed_fall":{"wt":"No"},"Fall_date":{"wt":""},"Found_date":{"wt":"1930"},"TKW":{"wt":"{{convert|16|MT}}"},"Image2":{"wt":""},"Image2_caption":{"wt":""}},"i":0}}]}" id="mwBA">.mw-parser-output .infobox-subbox{padding:0;border:none;margin:-3px;width:auto;min-width:100%;font-size:100%;clear:none;float:none;background-color:transparent}.mw-parser-output .infobox-3cols-child{margin:auto}.mw-parser-output .infobox .navbar{font-size:100%}@media screen{html.skin-theme-clientpref-night .mw-parser-output .infobox-full-data:not(.notheme)>div:not(.notheme)[style]{background:#1f1f23!important;color:#f8f9fa}}@media screen and (prefers-color-scheme:dark){html.skin-theme-clientpref-os .mw-parser-output .infobox-full-data:not(.notheme) div:not(.notheme){background:#1f1f23!important;color:#f8f9fa}}@media(min-width:640px){body.skin--responsive .mw-parser-output .infobox-table{display:table!important}body.skin--responsive .mw-parser-output .infobox-table>caption{display:table-caption!important}body.skin--responsive .mw-parser-output .infobox-table>tbody{display:table-row-group}body.skin--responsive .mw-parser-output .infobox-table tr{display:table-row!important}body.skin--responsive .mw-parser-output .infobox-table th,body.skin--responsive .mw-parser-output .infobox-table td{padding-left:inherit;padding-right:inherit}}
Mbosi | |
---|---|
![]() Main mass near Mbeya, Tanzania | |
Type | Iron |
Group | Ungrouped [1] |
Composition | Meteoric iron (8 % Ni), Silicate inclusions |
Country | Tanzania |
Region | Songwe |
Coordinates | 09°06′28″S33°02′15″E / 9.10778°S 33.03750°E [2] [a] |
Observed fall | No |
Found date | 1930 |
TKW | 16 metric tons (16 long tons; 18 short tons) [1] |
Alternative names | Kimwondo (local name) |
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Mbosi is an ungrouped iron meteorite found in Tanzania. It is one of the world's largest meteorites, variously estimated as the fourth-largest to the eighth-largest, it is located near the city of Mbeya in Tanzania's southern highlands. The meteorite is 3 metres (9.8 ft) long, 1 metre (3 ft 3 in) high, and weighs an estimated 16 metric tons (16 long tons; 18 short tons). [1]
Mbosi has been long known to locals, who call it kimondo, yet became known to outsiders only in the 1930s. It is named after Mbozi District, in Mbeya (Tanzania). When it was discovered by scientists in 1930 it didn't have a crater. [3]
Mbosi consists of meteoric iron with small silicate inclusions. The meteoric iron has a nickel concentration of 8% and shows Widmanstätten pattern. The Germanium-Gallium ratio is larger than 10, which can also be seen in meteorites of the IIF iron meteorite group and the Eagle station pallasites. [4]
The silicate inclusions have a core and mantle structure in thin section. The mantle is made from glass, that partially devitrified into pyroxene and plagioclase. The core consists of quartz. [4]
Currently classified as an ungrouped iron meteorite Mbosi shows similarities with IIF iron meteorites, the Eagle station pallasites and a few other ungrouped iron meteorite (e.g. Bocaiuva meteorite). [1] [4]
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Nonmagmatic meteorite is a deprecated term formerly used in meteoritics to describe iron meteorites that were originally thought to have not formed by igneous processes, to differentiate them from the magmatic meteorites, produced by the crystallization of a metal melt. The concept behind this was developed in the 1970s, but it was quickly realized that igneous processes actually play a vital role in the formation of the so-called "nonmagmatic" meteorites. Today, the terms are still sometimes used, but usage is discouraged because of the ambiguous meanings of the terms magmatic and nonmagmatic. The meteorites that were described to be nonmagmatic are now understood to be the product of partial melting and impact events and are grouped with the primitive achondrites and the achondrites.
This is a glossary of terms used in meteoritics, the science of meteorites.
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