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Colony meteorite, Washita Co., Oklahoma, USA

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Carbonaceous Chondrite [CO3.0; S1; W3]
Primitive; weathered

In 1975 a single odd-looking 3.91 kg stone was caught in the tines of a cotton cultivator, set aside, and later identified as a meteorite. Colony is a CO3.0 (Ornans-like) Carbonaceous Chondrite. Carbonaceous Chondrites are classified and sub-classified on the basis of their near solar bulk Mg-Si ratios and their oxygen isotope ratios. The CO class are further distinguished by their small chondrules and matrix of small minerals, comminuted fragments, and glassy components.

Colony is the largest known petrologic type CO3.0 meteorite. For the past 4.5 billion years its abundant and varied chondrules — rich in unequilibrated Olivine and/or Pyroxene — have largely escaped the mild or severe metamorphism experienced by the vast majority of chondrules in other chondrites. In a word, Colony is a very primitive meteorite. It contains, for example, a small number of ancient refractory spinel-rich and hibonite-rich inclusions from the earliest epochs of solar system formation. Within its micro-mineralogical niches there are also tiny ‘nano’ diamonds and silicon carbide grains produced in pre-solar system times.

On the other hand, since reaching the earth Colony has experienced significant weathering. The weathering, of course, further complicates our ability to understand this already complicated object.

Mineral List



16 entries listed. 12 valid minerals.

The above list 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.

References

Graham, A. L. (ed.) (1984) Meteoritical Bulletin, no. 62, Meteoritics 19 (1): 49-57. (March 1984)

Rubin, A. E., James, J. A., Keck, B. D., Weeks, K. S., Sears, D. W. G. & Jarosewich, E. (1985) The Colony meteorite and variations in CO3 chondrite properties. Meteoritics 20(2, part 1): 175-196. (June 1985)

Greenwood, R. C., Hutchison, R., Huss, G. R. & Hutcheon, I. D. (1992). CAIs in CO3 Meteorites: Parent Body or Nebular Alteration? Meteoritics 27 (3): 229. (July 1992)

Newton J., Arden, J. W. & Pillinger, C. T. 1992b. Metamorphism of CO3 chondrites: A carbon and nitrogen isotope study (abstract). Meteoritics 27 (3):267–268. (July 1992)

Weber, D. & Bischoff, A. (1994) Geochimica et Cosmochimica Acta 58 (18): 3855-3877. (Sept 1994)

Brearley, A. J. & Jones, R. H. (1998): Chondritic Meteorites. In: Planetary Materials (Papike, J. J., Editor): Chapter 3, 398 pages. Mineralogical Society of America: Washington, DC, USA.

Chizmadia, J., Rubin, A. E. & Wasson, J. T. (2002). Mineralogy and petrology of amoeboid olivine inclusions in CO3 chondrites: relationship to parent-body aqueous alteration. Meteoritics & Planetary Science 37 (12): 1781-1796 (Dec 2002)

Grady, M. M., Pratesi, G. & Moggi-Cecchi, V. (2015) Atlas of Meteorites. Cambridge University Press: Cambridge, United Kingdom. 373 pages.


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