Sikhote-Alin meteorite
Template:Short description Template:Infobox meteorite In southeastern Russia, an iron meteorite fell on the Sikhote-Alin mountains in 1947. Large iron meteorite falls have been witnessed, and fragments have been recovered, but never before in recorded history has a fall of this magnitude occurred.<ref name="rocks">Template:Cite book</ref> An estimated 23 tonnes<ref name="metbull"/> of fragments survived the fiery passage through the atmosphere and reached the Earth.
ImpactEdit
At around 10:30 AM on 12 February 1947, eyewitnesses in the Sikhote-Alin Mountains, Primorye, Soviet Union, observed a large bolide brighter than the sun that came out of the north and descended at an angle of about 41 degrees. The bright flash and the loud sound of the fall were observed for Template:Convert around the point of impact not far from Luchegorsk and approximately Template:Convert northeast of Vladivostok. A smoke trail, estimated at Template:Convert long, remained in the sky for several hours.
As the meteor, traveling at a speed of about Template:Convert, entered the atmosphere, it began to break apart, and the fragments fell together, some burying themselves Template:Convert deep.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> At an altitude of about Template:Convert, the largest mass apparently broke up in an explosion called an air burst.
On November 20, 1957<ref name="stamps">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> the Soviet Union issued a stamp for the 10th anniversary of the Sikhote-Alin meteorite shower. It reproduces a painting by P. I. Medvedev, a Soviet artist who witnessed the fall: he was sitting in his window starting a sketch when the fireball appeared and immediately began drawing what he saw.<ref name="montreal">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>
OrbitEdit
Because the meteor fell during the daytime, it was observed by many eyewitnesses. Evaluation of this observational data allowed V. G. Fesenkov, then chairman of the meteorite committee of the USSR Academy of Science, to estimate the meteoroid's orbit before it encountered the Earth. This orbit was ellipse-shaped, with its point of greatest distance from the sun situated within the asteroid belt, similar to many other small bodies crossing the orbit of the Earth.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> Such an orbit was probably created by collisions within the asteroid belt.
MassEdit
Sikhote-Alin is a massive fall, with the pre-atmospheric mass of the meteoroid estimated at approximately Template:Convert.<ref name="fieldguide">Template:Cite book</ref> A more recent estimate by Tsvetkov (and others) puts the mass at around Template:Convert.<ref name="metmag">Template:Cite journal</ref>
Krinov estimated the post-atmospheric mass of the meteoroid to be some Template:Convert.
Strewn field and cratersEdit
The strewn field for this meteorite covered an elliptical area of about Template:Convert. Some of the fragments made impact craters, the largest of which was about Template:Convert across and Template:Convert deep.<ref name="eidb">Template:Cite Earth Impact DB Template:Dead link</ref> Fragments of the meteorite were also driven into the surrounding trees, embedding themselves.
Composition and classificationEdit
The Sikhote-Alin meteorite is classified as an iron meteorite belonging to the meteorite group IIAB and with a coarse octahedrite structure. It is composed of approximately 93% iron, 5.9% nickel, 0.42% cobalt, 0.46% phosphorus, and 0.28% sulfur, with trace amounts of germanium and iridium. Minerals present include taenite, plessite, troilite, chromite, kamacite, and schreibersite.<ref>Template:Cite book</ref>
SpecimensEdit
Specimens of the Sikhote-Alin Meteorite are basically of two types:<ref name="metmag"/>
- individual, thumbprinted or regmaglypted specimens, showing fusion crust and signs of atmospheric ablation
- shrapnel or fragmented specimens, sharp-edged pieces of torn metal showing evidence of violent fragmentation
The first type probably broke off the main object early in the descent. These pieces are characterized by regmaglypts (cavities resembling thumbprints) on the surface of each specimen. The second type are fragments which were either torn apart during the atmospheric explosions or blasted apart upon impact on the frozen ground. Most resulted from the explosion at 5.6 km (3.5 mi) altitude.
A large specimen is on display in Moscow. Many other specimens are held by Russian Academy of Science and many smaller specimens exist in the collectors' market.
- Sikhote Alin Eisenmeteorit 1.3kg.JPG
Thumbprinted individual
- Sikalin179.jpg
Oriented individual
- Sikhote-Alin meteorite, shrapnel.jpg
Shrapnel sample
- Barringer Crater 2015 039.jpg
A piece on display at Meteor Crater, Arizona
See alsoEdit
ReferencesEdit
External linksEdit
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