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Degtevo | |||||||||||||||||||||||||||||||||||||||||
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Basic information | Name: Degtevo This is an OFFICIAL meteorite name. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: Yes, confirmed fall Year fell: 2016 Country: Russia Mass: 2.1 kg | ||||||||||||||||||||||||||||||||||||||||
Classification history: |
This is 1 of 12099 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 26 Feb 2017 | ||||||||||||||||||||||||||||||||||||||||
Writeup |
Writeup from MB 106:
Degtevo 49°09.6’N, 40°39.7’E Rostovskaya oblast’, Russia Confirmed fall: 20 March 2016 Classification: Ordinary chondrite (H5) History: Imamkulov Toir Mamazoirovich was working on a farm near Degtevo when he heard a whistling sound and saw a stone falling. Slezhuk Dmitry Vasilyevich, working on the same farm, also heard a loud whistling sound from the sky, went to the place of the fall and saw the piece. Several other people working on the farm confirm having heard a whistling sound and a trace in the sky. The first two aforementioned witnesses live in the town of Millerovo. A single piece of 2092 g and a fragment of 5.85 g were retrieved. Find information collected by Dmitry Sadilenko, Russian Academy of Sciences. The complete mass was purchased at the Ensisheim show 2016 by Marc Jost, Switzerland. Physical characteristics: Single stone with dimensions 19.3 × 13.5 × 6.5 cm. This is an oriented meteorite with well-developed regmaglypts on the cone-shaped front side and an irregular back side. Nearly completely covered by fusion crust. Fusion crust shows a thickened rim 2-10 mm wide around the edge of the back side. On one edge, a fracture surface of approx. 7 × 4 cm exposing the interior is present; another edge shows a fresh fracture surface of approx. 3 × 2 cm, exposing a pre-existing fracture with a surface reminiscent of a shatter cone. These broken edges indicate that about 50 to 100 g are missing and probably were not recovered. Some brownish coloration around metal grains. Some regmaglypts contain traces of brown organic material, probably cattle manure. Petrography: (B. Hofmann, NMBE, Å. Rosén, UBE/NMBE): Mean chondrule size 0.52±0.28 mm (n=125). Typical size of plagioclase grains is 10-20 μm. Troilite is polycrystalline. Shock stage is S2, some shock veins and shock-blackened areas are visible, no weathering (W0), some rusty coloration around metal grains. Fusion crust melt is invading fractures near the surface. Geochemistry: Electron microprobe analysis yielded: olivine Fa17.9±0.5 (Fa17.4-19.5; n=28), pyroxene Fs15.7±0.3Wo1.2±0.2 (Fs15.4-16.6Wo0.4-1.9; n=27). Cosmogenic radionuclides: (Å. Rosén, GEMSE): Gamma-spectroscopy performed in September 2016 showed the presence of the following short-lived radionuclides: 46Sc, 56Co, 54Mn, 58Co, 7Be, 57Co, 22Na, 44Ti, 26Al and 60Co. Recalculated to 15 March 2016, 22Na was 65.0(+8.9,-4.8) dpm/kg and 26Al 48.5(+7.8,-3.7) dpm/kg. The 22Na/26Al activity ratio of 1.3(+0.3,-0.1) is consistent with a fall in March 2016. Classification: Ordinary chondrite (H5), shock stage S2, no weathering (W0). Specimens: 25.3 g and two polished thin sections at NMBE. Main mass with Marc Jost. | ||||||||||||||||||||||||||||||||||||||||
Data from: MB106 Table 0 Line 0: |
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Institutions and collections |
NMBE: Natural History Museum Bern
Bernastrasse 15
CH-3005 Bern
Switzerland, Switzerland; Website (institutional address; updated 2 Mar 2012) UBE: University of Bern, University of Bern, Hochschulstrasse 4, CH-3012 Bern, Switzerland (institutional address) |
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Catalogs: |
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References: | Published in Gattacceca J., Bouvier A., Grossman J., Metzler K., and Uehara M. (2019) Meteoritical Bulletin, no. 106. Meteorit. Planet. Sci. 54 in press.
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Geography: |
Statistics: This is 1 of 4 approved meteorites from Rostovskaya oblast', Russia (plus 2 impact craters) This is 1 of 158 approved meteorites from Russia (plus 5 unapproved names) (plus 19 impact craters) | ||||||||||||||||||||||||||||||||||||||||
Proximity search: |