The Best Chelyabinsk Meteorite found days after fall 2013 Russia. 47. 7 gm

Description: Genuine Russian 2013 Meteorite discovered days after the fall in Chelyabinsk, Russia. 47. 7 gm (large) Feb. 15, 2013Guaranteed authentic Chelyabinsk MeteoriteFrom Wikipedia, the free encyclopediaJump to navigationJump to searchNot to be confused with Chelyabinsk meteor.ChelyabinskLargest fragment of the meteorite at the exhibition of The State Museum of the South Ural History.TypeOrdinary chondrite LL5[1]Shock stageS4[2]Weathering gradeW0 (pristine)CountryRussiaRegionChelyabinsk OblastCoordinates54°57′18″N 60°19′30″ECoordinates: 54°57′18″N 60°19′30″EObserved fallYesFall date15 February 2013, 09:20 YEKT(UTC+06:00)Found date27 February 2013TKWapproximately 1,000 kg (2,200 lb)[3]Strewn fieldYes Related media on Wikimedia CommonsThe Chelyabinsk meteorite (Russian: Челябинский метеорит, Chelyabinskii meteorit) is the fragmented remains of the large Chelyabinsk meteor of 15 February 2013 which reached the ground after the meteor's passage through the atmosphere. The descent of the meteor, visible as a brilliant superbolide in the morning sky, caused a series of shock waves that shattered windows, damaged approximately 7,200 buildings and left 1,500 people injured.[4][5] The resulting fragments were scattered over a wide area.The largest fragment raised from the bottom of Lake Chebarkul on 16 October 2013 had a mass of 540 kg (1,190 lb)[6] and the total mass of other 7 meteorite fragments found nearby was 84.4 kg (186 lb).[6] Composition and classification[edit]The meteorite has been classified as an LL5 ordinary chondrite. First estimates of its composition indicate about 10% of meteoric iron, as well as olivine and sulfides.[4][8]Asteroid[edit]The impacting asteroid started to brighten up in the general direction of the Pegasus constellation, close to the East horizon where the Sun was starting to rise.[9] The impactor belonged to the Apollo group of near-Earth asteroids.[9][10]The asteroid had an approximate size of 18 m (59 ft) and a mass of about 9,100 t (10,000 short tons) before it entered the denser parts of Earth's atmosphere and started to ablate.[11] At an altitude of about 23.3 km (14.5 miles) the body exploded in a meteor air burst.[11] Meteorite fragments of the body landed on the ground.[12][13]Analysis of three fragments using optical microscopy, electron microscopy, Raman spectroscopy, and isotopic compositiontechniques used to date Solar System objects, showed the isotopic clocks in the asteroids (rubidium and strontium ratios, argonisotope ratios) appear to have partially or totally reset in past collisions. The isotopic clock resets may result from thermal effects changing isotopic ratios, and changes to cosmic radiation exposure. The asteroid appears to have had eight major collisions, around 4.53, 4.45, 3.73, 2.81, and 1.46 billion years ago, then at 852, 312, and 27 million years ago.[14][15]Meteorite[edit]Scientists collected 53 samples from near a 6-metre-wide hole in the ice of Lake Chebarkul, thought to be the result of a single meteorite fragment impact. The specimens are of various sizes, with the largest being 5 kg (11 lb),[16] and initial laboratory analysis confirmed their meteoric origin.[1]In June 2013, Russian scientists reported that further investigation by magnetic imaging below the location of the ice hole in Lake Chebarkul had identified a 60 cm-large (2 ft) meteorite buried in the mud at the bottom of the lake. An operation to recover it from the lake began on 10 September 2013,[17] and concluded on 16 October 2013, with the raising of the rock with the mass of 540 kg (1,190 lb).[6] It was examined by scientists and handed over to the local authorities,[18][19] who put it on display at the Chelyabinsk State Museum of Local Lore, causing protests from the followers of the recently established "Church of Chelyabinsk Meteorite".[20]In the aftermath of the superbolide air burst, a large number of small meteorite fragments fell on areas west of Chelyabinsk, including Deputatskoye, generally at terminal velocity, about the speed of a piece of gravel dropped from a skyscraper.[12] Local residents and schoolchildren located and picked up some of the meteorites, many located in snowdrifts, by following a visible hole that had been left in the outer surface of the snow. Speculators became active in the informal market for meteorite fragments that rapidly emerged.[12]

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