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Indian Butte | |||||||||||||||||||||||||||||||||||||||
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Basic information | Name: Indian Butte This is an OFFICIAL meteorite name. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: Yes Year fell: 1998 Country: United States Mass: 1721 g | ||||||||||||||||||||||||||||||||||||||
Classification history: |
This is 1 of 12055 approved meteorites (plus 23 unapproved names) classified as H5. [show all] Search for other: H chondrites, H chondrites (type 4-7), Ordinary chondrites, and Ordinary chondrites (type 4-7) | ||||||||||||||||||||||||||||||||||||||
Comments: | Approved 29 May 2013 | ||||||||||||||||||||||||||||||||||||||
Writeup |
Writeup from MB 102:
Indian Butte 32°51.860’N, 112°2.920’W Pinal County, Arizona, USA Fell: 7 June 1998 Classification: Ordinary chondrite (H5) History: The following lines of evidence support a connection between the Indian Butte stones and the "Casa Grande" fireball of 7 June 1998: 1) The discovery location is consistent with the triangulated endpoint based on fireball reports; 2) The location is directly under a Doppler radar return; 3) The stones are fresh (weathering grade W0 to 1). Doppler radar was first used in 2009 to locate the Ash Creek meteorite fall. The Indian Butte radar signal was recently identified during a search of historic falls. Some stones have been marketed under the synonym "Stanfield". A 128 gram stone was discovered by Robert Reisener, Sonny Clary, and Fredric Stephan while investigating a doppler radar signal corresponding to the "Casa Grande" fireball of 7 June 1998. At least 30 other stones were subsequently found. The Doppler signature was identified by Marc Fries and Robert Matson using fireball witness reports collected by Robert Ward. The location of discovery is near the area searched by David Kring and others immediately after the fireball. Physical characteristics: At least 30 fusion-crusted stones have been recovered, with a total mass of 1721 grams. The fusion crust is fresh, although many stones display slight oxidation on the bottom where they lay on the desert surface. The interior metal is free of limonite rinds, indicative of weathering grade W0. Petrography: (A.Rubin, UCLA) The chondrite is moderately recrystallized. Polysynthetically twinned low-Ca pyroxene is absent. A few small grains of diopside have grown large enough to be analyzed with the electron microprobe. Plagioclase has also grown fairly coarse; grains up to 25 µm across are present. Geochemistry: Olivine, Fa17.9±0.3; pyroxene, Fs16.0±0.2Wo1.5±0.2. Mineralogical equilibrium has occurred. Classification: Ordinary chondrite (H5). Shock stage = S1 and weathering grade = W0. Specimens: Most stones are privately held; 22.2 grams have been deposited at UCLA. | ||||||||||||||||||||||||||||||||||||||
Data from: MB102 Table 0 Line 0: |
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Institutions and collections |
UCLA: Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095-1567, United States (institutional address; updated 17 Oct 2011) Clary: Ralph "Sonny" Clary, Las Vegas, NV 89131 , United States; Website (private address; updated 3 Jan 2010) |
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Catalogs: |
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References: | Published in Meteoritical Bulletin, no. 102, MAPS 50, 1662, September 2015
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Photos: |
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Geography: |
Statistics: This is 1 of 180 approved meteorites from Arizona, United States (plus 1 impact crater) This is 1 of 1934 approved meteorites from United States (plus 866 unapproved names) (plus 28 impact craters) | ||||||||||||||||||||||||||||||||||||||
Proximity search: | |||||||||||||||||||||||||||||||||||||||
Synonyms: |
Casa Grande (In MB102) Stanfield (In MB102) |