H chondrite
{{short description|Type of meteorite}}
{{infobox meteorite subdivision
|Subdivision = Group
|Name = H chondrite
|Alternative_names = Bronzite chondrites, Olivine bronzite chondrites
|Image = Weston meteorite.jpg
|Image_caption = Weston meteorite, H4
|Type = Chondrite
|Class = Ordinary chondrite
|Clan =
|Subgroups = {{flatlist|
- H3
- H4
- H5
}}
|Structural_classification = ?
|Parent_body = Possibly 6 Hebe, less likely 3 Juno & 7 Iris
|Composition = Iron ~25–31%, bronzite (an orthopyroxene), olivine (with characteristic fayalite (Fa) content 16 to 20 mol%), nickel-iron 15–19%, troilite 5%
|Petrologic_type = 3 (~2.5%), 5 (40%), 4 & 6 (57.5%)
|Number_of_specimens =
|TKW =
|Image2 = Tetrataenite-138026.jpg
|Image2_caption = Nuevo Mercurio, H5
}}
The H type ordinary chondrites are the most common type of meteorite, accounting for approximately 40% of all those catalogued, 46% of the ordinary chondrites, and 44% of all chondrites.{{Cite web |url=http://internt.nhm.ac.uk/jdsml/research-curation/projects/metcat/metsPerGroup.dsml |title=Natural History Museum, meteorite catalogue |access-date=2005-11-29 |archive-date=2006-05-03 |archive-url=https://web.archive.org/web/20060503223656/http://internt.nhm.ac.uk/jdsml/research-curation/projects/metcat/metsPerGroup.dsml |url-status=dead }} The ordinary chondrites are thought to have originated from three parent asteroids, whose fragments make up the H chondrite, L chondrite and LL chondrite groups respectively.[https://www.youtube.com/watch?v=BNkS1uHUbq8&t=34m39s NASA (YouTube) – Dr. David Kring – Asteroid Initiative Workshop Cosmic Explorations Speakers Session]
Name
The name comes from their High iron abundance, with respect to other ordinary chondrites.
Historically, the H chondrites have been named bronzite chondrites or olivine bronzite chondrites for the dominant minerals, but these terms are now obsolete.
Parent body
A probable parent body for this group is the S-type asteroid 6 Hebe, with less likely candidates being 3 Juno and 7 Iris.[http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1998M%26PS...33.1281G&db_key=AST&data_type=HTML&format=&high=438c93072f28336 M. J. Gaffey & S. L. Gilbert Asteroid 6 Hebe: The probable parent body of the H-Type ordinary chondrites and the IIE iron meteorites], Meteoritics & Planetary Science, Vol. 33, p. 1281 (1998). It is supposed that these meteorites arise from impacts onto small near-Earth asteroids broken off from 6 Hebe in the past, rather than originating from 6 Hebe directly.
The H chondrites have very similar trace element abundances and Oxygen isotope ratios to the IIE iron meteorites, making it likely that they both originate from the same parent body.
Iron
Their high iron abundance is about 25–31% by weight. Over half of this is present in metallic form, making these meteorites strongly magnetic despite the stony chondritic appearance.
Mineralogy
The most abundant minerals are bronzite (an orthopyroxene), and olivine. Characteristic is the fayalite (Fa) content of the olivine of 16 to 20 mol%. They contain also 15–19% of nickel-iron metal and about 5% of troilite. The majority of these meteorites have been significantly metamorphosed, with over 40% being in petrologic class 5, most of the rest in classes 4 and 6. Only a few (about 2.5%) are of the largely unaltered petrologic class 3.
Gallery
File:GaoGuenieMeteorite.jpg|Gao-Guenie, H5
File:Chondrite H5.JPG|H5 Dar Bou Nali South Morocco
See also
References
{{Reflist}}
External links
- [http://internt.nhm.ac.uk/jdsml/research-curation/projects/metcat/metsPerGroup.dsml The Catalogue of Meteorites] {{Webarchive|url=https://web.archive.org/web/20060503223656/http://internt.nhm.ac.uk/jdsml/research-curation/projects/metcat/metsPerGroup.dsml |date=2006-05-03 }}
{{Meteorites}}
{{DEFAULTSORT:H Chondrite}}