MetSoc Home            Publications            Contacts  
Search the Meteoritical Bulletin Database
Last update: 23 May 2024
Search for: Search type: Search limits: Display: Publication:
Text help
Starts with
Sounds like
Falls  Non-NWAs
What's new
  in the last:
Limit to approved meteorite names
Search text:  
Basic information Name: Ozerki
     This is an OFFICIAL meteorite name.
Abbreviation: There is no official abbreviation for this meteorite.
Observed fall: Yes, confirmed fall
Year fell: 2018
Country: Russia
Mass:help 6.5 kg
Meteoritical Bulletin:  MB 107  (2018)  L6
Recommended:  L6    [explanation]

This is 1 of 12896 approved meteorites (plus 11 unapproved names) classified as L6.   [show all]
Search for other: L chondrites, L chondrites (type 4-7), Ordinary chondrites, and Ordinary chondrites (type 4-7)
Comments: Approved 20 Jul 2018
Writeup from MB 107:

Ozerki        52°48.084’N, 38°10.268’E

Lipetskaya oblast’, Russia

Confirmed fall: 21 June 2018

Classification: Ordinary chondrite (L6)

History: The first meteorite fragments were recovered based on analysis of the fireball observed over the Lipetskaya oblast’ in Russia on June 21, 2018, at 01:16:20 UT. The fireball was widely observed from many places in Russia, including Moscow. The scientists from UrFU, UHelsinki, and the Finnish Fireball Network formed a consortium enabling quick prediction and the actual discovery of the meteorite. Collection of the observational data and trajectory analysis were done by Esko Lyytinen, Maria Gritsevich, Nikolai Kruglikov, and Mikhail Larionov. The derived parameters, characterizing the trajectory were clearly indicative of a number of  meteorite fragments landing on the ground. Using these results, a comprehensive model of the strewn field providing the expected locations of fragments was done by Jarmo Moilanen. The area of the meteorite shower was predicted to be on the line Ozerki – Zlobino - Druzhba, Stanovlyansky district, northwest of Yelets town, Lipetskaya oblast’. The modeling assumed about 100 meteorites (excepting the main body) with total mass ~7 kg. With the support of these data, a meteorite recovery campaign was initiated by Victor I. Grokhovsky. Five samples of the meteorite (1176 g) were recovered during the UrFU meteorite expedition-2018 (23-27 June 2018; Pastukhovich A.Yu., Yakovlev G.A., Petrova E.V. and volunteer Usenkov A.V.) in the Lipetskaya oblast’. The first sample was found 25 June 2018 by G.A. Yakovlev (59.85 g). The UrFU finds were near Ozerki village. During the next few weeks, more meteorite samples (>5500 g) were recovered by institutional groups (Vernad - GEOKHI RAS, IA RAS, IDG RAS) and private collectors in the area Ozerki – Zlobino. The total mass and number of stones may increase due to additional finds.

Physical characteristics: The meteorites have roughly rounded shapes, covered by dark fusion crust; the interior is light colored and contains visible opaque shock veins. The samples are fresh, but halos of Fe-hydroxides were already present around metal grains. Some samples contain impact melt.

Petrography: (V.V. Sharygin, SIGM and UrFU, and D.A. Zamyatin, RAS-UB and UrFU): Petrographic observation of a polished section shows very rare chondrules in a coarse recrystallized matrix. Most chondrules are very poorly defined and their apparent sizes vary from 200 µm to 1 mm. Only the largest chondrules (up to 4 mm) are clearly delineated. The PO, POP and BO chondrules are most common and mainly consist of olivine, plagioclase, low-Ca pyroxene ± chromite and blebs of troilite and FeNi-metal. Other textural types of chondrules were not observed. Olivine, low-Ca-pyroxene, plagioclase, FeNi-metal and troilite are the main minerals in the matrix. Clinopyroxene, chromite, chlorapatite and merrillite (100-300 µm) occur locally in the matrix. Plagioclase grains are larger than 50-100 µm. Shock features include undulatory extinction, irregular and planar fractures (three directions) in olivine and the presence of opaque shock veins. The presence of impact melt suggests shock stage S5. Grains of FeNi metal (up to 1 mm) are represented by both individual phases (kamacite, taenite or plessite) and their intergrowths (kamacite + taenite, kamacite + plessite + tetrataenite, kamacite + tetrataenite + pentlandite) ± troilite. Grains of troilite (100-500 µm) are spongy, fine-grained aggregates of micrometer-sized individuals (<5 µm). Some pentlandite grains occur in such aggregates, especially on contacts with FeNi-metal. Opaque shock veins (up to 100 µm in thick) are not very abundant and contain metal-sulfide intergrowths in fine-grained low-Ca pyroxene matrix. The thickness of fusion crust is up to 600 µm. It is highly vesicular and zoned in texture: the outmost zone is a cryptocrystalline aggregate of skeletal crystals of zoned olivine and magnetite (up to 5 µm) and glass (44-47 wt.% SiO2); the inner zone is represented by larger skeletal crystals of newly formed olivine + glass + minor magnetite. Both zones contain rounded relics of initial olivine and chromite and newly formed Ni-rich metal-sulfide globules (10-20 µm). Magnetic susceptibility log χ (× 10-9 m3/kg) = 4.8 (analyst Yakovlev G.A.).

Geochemistry: SEM-EDS-WDS (V. V. Sharygin, SIGM and UrFU) and EMPA-WDS (D.A. Zamyatin, RAS-UB and UrFU). Olivine Fa25.6±0.3 (N=51), low-Ca pyroxene Fs21.4±0.2Wo1.6±0.3 (N=44), plagioclase Ab83.5An10.5Or6.0 (N=35), Cr-bearing clinopyroxene En45.8Fs9.0Wo45.2 (Cr2O3 – 0.8-1.0 wt.%, N=6), chromite Crt82.8Spl12.1 (N=17), chlorapatite, merrillite, FeNi-metals, troilite and pentlandite. Chlorapatite contains F (up to 0.5 wt.%); Cl – 5.5, Na2O – 0.5 wt.% (N=11). Merrillite is poor in FeO (0.3-0.7 wt.%, N=8). Composition of metal (in wt.%): kamacite (N=32) – Fe 93.2±1.4, Ni – 5.89±1.44, Co – 0.92±0.13; taenite (N=20) – Fe 68.6±5.1, Ni 31.0±5.1, Co 0.36±0.09; tetrataenite (N=3) – Fe 48.5, Ni 51.2, Co 0.16. Composition of sulfides (in wt.%): pentlandite (N=10, in association with troilite) – Fe 50.6±0.8, Ni 15.4±1.0, Co 0.15±0.02, Cu 0.61±0.26, S 33.6±0.3; heazlewoodite (N=10, from fusion crust) – Fe 2.62±0.46, Ni 71.4±0.8, Co 0.11±0.01, Cu 0.37±0.09, S 25.6±0.5.

Classification: Ordinary chondrite. L6, S5, W0.

Specimens: UrFU - 798.6 g (3 samples: 550.4, 188.3, 59.9 g); Vernad - 603 g (3 samples); SIGM - 31.7 g fragment; RAS-UB - 15 g fragment; UHelsinki - 15 g fragment.

Data from:
  Table 0
  Line 0:
State/Prov/County:Lipetskaya oblast'
Origin or pseudonym:plain, plowed land
Date:21 June 2018
Mass (g):>6500
Shock stage:S4/5
Weathering grade:W0
Fayalite (mol%):25.6±0.3 (N=51)
Ferrosilite (mol%):21.4±0.2 (N=44)
Wollastonite (mol%):1.61±0.26 (N=44)
Magnetic suscept.:4.80
Classifier:V. V. Sharygin, SIGM and UrFU, V. I. Grokhovsky, UrFU
Type spec mass (g):798.6
Type spec location:UrFU
Main mass:798.6 g (3 samples) – UrFU; 603 g (3 samples) - Vernad; 31.7 g fragment– SIGM; 15 g fragment – RAS-UB; 15 g fragment - UHelsinki.
Finder:UrFU meteorite expedition – Lipetsk-2018
Comments:Submitted by Victor V. Sharygin
   and collections
Vernad: Vernadsky Institute of Geochemistry and Analytical Chemistry, Russia (institutional address; updated 21 Feb 2016)
UrFU: Ural Federal University, 620002, 19 Mira street, Ekaterinburg, Russia (institutional address; updated 14 Jan 2015)
UHelsinki: University of Helsinki, Department of Physics, P.O. Box 64, 00014 Helsinki University, Finland (institutional address; updated 25 Apr 2015)
SIGM: V.S. Sobolev Institute of Geology and Mineralogy SB RAS, pr. Akademika Koptyuga, 3 Novosibirsk, 630090, Russia; Website (institutional address; updated 10 May 2017)
RAS-UB: Zavaritsky Institute of Geology and Geochemistry Russian Academy of Sciences, Ural Branch 15 Akademika Vonsovskogo str., Ekaterinburg, 620016, Russia (institutional address; updated 19 Apr 2018)
References: Published in Meteoritical Bulletin, no. 107, MAPS 55, 460-462
Find references in NASA ADS:
Find references in Google Scholar:
Photos from the Encyclopedia of Meteorites:
Sergey Vasiliev   
Photos uploaded by members of the Encyclopedia of Meteorites.
    (Caution, these are of unknown reliability)
chen wang               
Chunliang Zhang               
Cute child   
Domjan Svilkovic   
Paulo Anselmo Matioli (JN Science Museum)   
Qi Lv      
Solar Anamnesis         
Wojciech Moscinski   
Woreczko Jan & Wadi   
Ziyao Wang                        
Public domain photographs:
Victor V. Sharygin      

     Recommended::   (52° 48' 5"N, 38° 10' 16"E)

     This is the only approved meteorite from Lipetskaya oblast', Russia
     This is 1 of 156 approved meteorites from Russia (plus 5 unapproved names) (plus 19 impact craters)
Proximity search:
Find nearby meteorites: enter search radius (km):

Direct link to this page