|
Whetstone Mountains | |||||||||
---|---|---|---|---|---|---|---|---|---|
Basic information | Name: Whetstone Mountains This is an OFFICIAL meteorite name. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: Yes Year fell: 2009 Country: United States Mass: 2.14 kg | ||||||||
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 1 Sep 2009 Revised 31 Jul 2012: Released coordinates | ||||||||
Writeup |
Writeup from MB 99:
Whetstone Mountains 31.938626°N, 110.424477°W Cochise County, Arizona, United States Fall: June 23, 2009 at 9:22 p.m. MST (UTC -7 hours) Classification: Ordinary chondrite (H5 breccia) History: A bright fireball with detonations and rumblings was observed by many witnesses. Carl Hergenrother estimated magnitude -11 fireball that created shadows, lasted for at least ~2 seconds moving from the southeast part of the sky to the east and downward. Part of the path was recorded by the All-Sky camera at the UA-Multiple-Mirror Telescope facility on Mt. Hopkins and a security camera in Marana, AZ. Jack L. Schrader interviewed eye-witnesses and recovered the first 155.86 g stone on the surface of the high desert less than 45 hours after the fall. Within a month of its fall, additional stones were found by Chuck Schrader, Shauna Russell, Robert Ward, Todd Parker, and Michael Farmer. Strewnfield occupies an ~3 x 6 km ellipse, trending N 30° E. Coordinates given are approximately at the center of the strewnfield. Physical characteristics: Total known mass as of July 15, 2009 is 2138.74 g among 10 stones. All except one were recovered as intact individuals with complete fusion crust. Some stones exhibit regmaglypts. Fusion crust is fresh, matte black. One stone exhibits a fusion crust with a reddish hue (not oxidation) and others contain a few “bluish” spots. Petrography D. H. Hill (UAz): Well-defined chondrules (200-700 μm) with porphyritic olivine and pyroxene chondrules being most abundant. Metal grains up to 800 μm and troilite up to 300 μm occur between chondrules in approximately 1:1 proportion. Many metal grains exhibit fingerlike intergrowth of kamacite and taenite. Mg-bearing phosphates ~100 x 200 μm occur between chondrules. A crushed texture is observed that corresponds to a lighter lithology in a darker groundmass. Shock veins are visible in the hand specimen. There are two 350 μm chromite-rich clasts. Mineral compositions and geochemistry: D. H. Hill (UAz) EMP: Olivine (Fa18.82±0.25); pyroxene (Fs16.56±0.49Wo1.77±1.7); kamacite (Ni 6.71% ± 0.28; Co 0.49% ± 0.03), taenite (26% Ni and ~40 % Ni (tetrataenite?); phosphates are mostly Mg-rich with a few Cl-bearing. Classification: Ordinary chondrite (H5) breccia; W0 | ||||||||
Institutions and collections |
ASU: Center for Meteorite Studies, Arizona State University, Tempe, Arizona 85287-1404, United States; Website (institutional address; updated 14 Jan 2012) UAz: Lunar and Planetary Laboratory, University of Arizona, 1629 E. University Blvd., Tucson, AZ 85721, United States (institutional address; updated 14 Jan 2012) |
||||||||
Catalogs: |
| ||||||||
References: | Published in Meteoritical Bulletin, No. 99, April 2012, MAPS 47, E1-E52 (2012) [published online only]
| ||||||||
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: |