| Sikhote-Alin | |
|---|---|
Thumbprinted Sikhote-Alin sample
| |
| Type | Iron |
| Structural classification | Octahedrite, coarsest |
| Group | IIAB |
| Composition | 93% Fe, 5.9% Ni, 0.42% Co, 0.46% P, 0.28% S |
| Country | Russia |
| Region | Sikhote-Alin Mountains, Primorsky Krai, Far Eastern Federal District |
| Coordinates | 46°09′36″N 134°39′12″ECoordinates: 46°09′36″N 134°39′12″E |
| Observed fall | Yes |
| Fall date | February 12, 1947 |
| TKW | >23 tonnes (25 short tons) |
| Strewn field | Yes |
An iron meteorite fell on the Sikhote-Alin Mountains, in southeastern Russia, in 1947. Though large iron meteorite falls had been witnessed previously and fragments recovered, never before in recorded history had a fall of this magnitude been observed. An estimated 23 tonnes of fragments survived the fiery passage through the atmosphere and reached the Earth, but still less than the largest meteorite find, the Hoba meteorite of 60 tonnes.
Impact
The 10th anniversary stamp. It reproduces a painting by P. J. Medvedev.
At around 10:30 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 deafening sound of the fall were
observed for 300 kilometres (190 mi) around the point of impact not far
from Luchegorsk and approximately 440 km (270 mi) northeast of Vladivostok. A smoke trail, estimated at 32 km (20 mi) long, remained in the sky for several hours.
As the meteor, traveling at a speed of about 14 km/s (8.7 mi/s),
entered the atmosphere, it began to break apart, and the fragments fell
together. At an altitude of about 5.6 km (3.5 mi), the largest mass
apparently broke up in a violent explosion called an air burst.
On November 20, 1957 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, so he immediately began
drawing what he saw.
Orbit
Because the meteor fell during 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.
Such an orbit was probably created by collisions within the asteroid
belt.
Size
Sikhote-Alin is a massive fall with the pre-atmospheric mass of the meteoroid estimated at approximately 90,000 kg (200,000 lb). A more recent estimate by Tsvetkov (and others) puts the mass at around 100,000 kg (220,000 lb).
Krinov had estimated the post-atmospheric mass of the meteoroid at some 23,000 kg (51,000 lb).
Strewn field and craters
The strewn field for this meteorite covered an elliptical area of about 1.3 km2 (0.50 sq mi). Some of the fragments made impact craters, the largest of which was about 26 m (85 ft) across and 6 m (20 ft) deep. Fragments of the meteorite were also driven into the surrounding trees.
Composition and classification
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.
Specimens
Specimens of the Sikhote-Alin Meteorite are basically of two types:
- 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 thumb prints) in 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 were
probably the result of 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 a great number of smaller specimens have made their way into the collector's market.
Thumbprinted individual
Oriented individual
Shrapnel sample
