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|Latitude & Longitude (WGS84):||41° 47' 59'' North , 91° 52' 0'' West|
|Latitude & Longitude (decimal):||41.80000,-91.86667|
|Non-native locality type:||Meteorite|
|Meteorite Class:||L5 chondrite meteorite|
|Meteoritical Society Class:||L5|
|Metbull:||View entry in Meteoritical Bulletin Database|
|Köppen climate type:||Dfa : Hot-summer humid continental climate|
Ordinary chondrite (L5,br; S3; W0)
Fell, 12 February 1875: ~10:30 PM; 226.8 kg, meteorite shower
Late in the evening on a clear winter night, an unusually bright bolide was seen over a 600 km long path moving from the SE towards the NE over northern Missouri and southern Iowa. Detonations were heard — and, on the third day afterwards a single stone was found lying on the snow. After the snow had melted in March and in subsequent months over 300 meteoritic stones were recovered over a 10x5 km ellipse. Almost all the stones were covered with a black fusion crust. The mass of the largest stone largest stone was 33.5 kg, but a large number of very small stones were found.
The Homestead meteorite is a thoroughly brecciated meteorite. Presumably at least partially due to earlier pre-terrestrial impacts, the meteorite had already begun to break into smaller fragments well before it struck the earth. Its largely equilibrated olivine and low Ca-orthopyroxene (Fa23.1; Fs20, resp.) and its indistinct chondrules are characteristic of type L5 chondrites. Chondrules (mostly barred olivine [BO], porphyritic olivine [PO], and porphyritic pyroxene [PP]) are similar to those in many meteorites. In addition to the dominant olivine and pyroxene of both chondrules and matrix, minor amounts of Fe-Ni metal and troilite (almost entirely as aggregates within the matrix) account for most of the mass. Lesser amounts of albitic plagioclase plus accessory chromite and phosphate are present. However, close studies of textures and accessory constituents provide clear evidence of pre-terrestrial disruption. Small veins, minute pools of opaques, and weak mosaicism in olivine are but the most obvious indicators of preterrestrial shock (level S3). Whether pre-terrestrial post-shock annealing has partially obscured even stronger shock event(s) is a somewhat open question.
The L (relatively low in total iron) chondrites are the largest group of ordinary chondrites and represent ~45% of classified and witnessed falls. The L5 petrologic type subgroup represent ~20 % of the total L group. Although a few more massive L5 finds have been found, Homestead is in fact the most massive of the 80 witnessed and documented meteorite falls classified exactly as 'L5' chondrites (as of early May 2016).
The largest stones and fragments of the Homestead shower were acquired by museums in the United States (Yale University; Field Museum of Natural History in Chicago; Harvard University; American Museum of Natural History in New York). However, moderate sized masses in the 1-5 kg range were distributed to several other U.S. and European museums and institutions.
Commodity ListThis is a list of exploitable or exploited mineral commodities recorded at this locality.
8 valid minerals.
Meteorite/Rock Types Recorded
Note: this is a very new system on mindat.org and data is currently VERY limited. Please bear with us while we work towards adding this information!
Select Rock List TypeAlphabetical List Tree Diagram
Entries shown in red are rocks recorded for this region.
This page contains all mineral locality references listed on mindat.org. This does not claim to be a complete list. If you know of more minerals from this site, please register so you can add to our database. This locality information is for reference purposes only. You should never attempt to visit any sites listed in mindat.org without first ensuring that you have the permission of the land and/or mineral rights holders for access and that you are aware of all safety precautions necessary.
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Leonard, N.R. (1875) Iowa County meteor and its Meteorites. American Journal of Science (3rd Series) 10: 357-363.
Farrington, O.C. (1915) Catalogue of the Meteorites of North America: Memoirs of the National Academy of Sciences, Vol. 23: Washington. 545 pages.
Prior, G.T. (1918) On the Chemical Composition of the Meteorites Amana (=Homestead) and Eagle Station: Mineralogical Magazine 18(85): 173-179. (Aug 1918).
Mason, B. (1962) Classification of Chondritic Meteorites: American Museum Novitates, #2085. 20 pages. (May 1962).
Mason, B. (1963) Olivine in ordinary chondrites: Geochimica et Cosmochimica Acta 27(9): 1011-1023. (Sept 1963).
Ramdohr, P. (1973). The Opaque Minerals in Stony Meteorites. Elsevier Publishing Company: Amsterdam; London: New York. 245 pages.
Crozaz G., Pellas, P., Bourot-Denise, M., de Chazal, S.M., Fieni, C., Lundberg, L.L. & Zinner, E. (1989) Plutonium, uranium and rare earths in the phosphates of ordinary chondrites—the quest for a chronometer: Earth and Planetary Science Letters 93: 157-169.
Rubin, A. (1990) Olivine & Kamacite in Ordinary Chondrites: Intergroup and Intragroup relationships. Geochimica et Cosmochimica Acta 54: 1217-1230.
Ivanova, M.A., Krot, A.N., Mitreikina, O.B. & Zinovieva, N.G. (1992) Chromite-rich Inclusions in the Homestead (L5) Chondrite (abstract): Lunar and Planetary Science Conference XXIII: page 585. (March 1992).
Rubin, A.E. (1994) Metallic copper in ordinary chondrites. Meteoritics 29 (1): 93-98. (Jan 1994).
Heide, F. & Wlotzka, F. (1995) Meteorites: Messengers from Space. Springer-Verlag: Berlin, Heidelberg, New York. 231 pages.
Grady, M.M. (2000). Catalogue of Meteorites (5/e). Cambridge University Press: Cambridge; New York; Oakleigh; Madrid; Cape Town. 689 pages.
Grady, M.M., Pratesi, G. & Moggi-Cecchi, V. (2015) Atlas of Meteorites. Cambridge University Press: Cambridge, United Kingdom. 373 pages.