Sikhote-Alin | has image
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has name Sikhote-Alin |  |
is an instance of Ogg octahedrite  |  |
is an instance of type IIAB iron meteorite |  |
has fall date February 12, 1947, 10:38 a.m. local time  |  |
has fall location Sikhote-Alin Mountains, Maritime Province, Russia, 270 miles northeast of Vladivostok |  |
has fall coordinates 46° 9' 36" N, 134° 39' 12" E |  |
has fall map
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has original mass greater than 14000 kg |  |
have composition 5.9% Ni, 0.42% Co, 0.46% P, about 0.28% S, 52 ppm Ga, 161 ppm Ge, 0.03 ppm Ir |  |
has crystal size 9 ± 5 mm (coarsest) |  |
has impact velocity 14.5 kilometers per second |  |
Ogg octahedrite | has structural class Ogg |  |
type IIAB iron meteorite | has composition kamacite, daubreelite |  |
has formation cooling rate 0.8 to 3 degrees C per million years |  |
parent body radius 90 to 165 kilometers |  |
has total mass of finds 3563 kg |  |
has number of finds 43 |  |
has nickel content 6.15 % by weight |  |
has gallium content 58.3 microgram/gram |  |
has germanium content 173 microgram/gram |  |
has iridium content 10 microgram/gram |  |
has carbon content 2000 microgram/gram |  |
has phosphor content 6 milligram/gram |  |
has sulfur content 0.20 % by weight |  |
has chromium content 28 microgram/gram |  |
has cobalt content 5.3 milligram/gram |  |
has copper content 129 microgram/gram |  |
has molydbenum content 6.9 microgram/gram |  |
has tungsten content 2.1 microgram/gram |  |
has palladium content 2.6 microgram/gram |  |
has gold content 1.1 microgram/gram |  |
has arsenic content 9.9 microgram/gram |  |
has antimony content 201 nanogram/gram |  |
structural iron meteorite | has distinguishing feature crystalline iron-nickel alloy |  |
iron meteorite | has relative abundance 5.7 % of meteorite falls |  |
has weather resistance high |  |
has fragmentation probability low because it is tougher than stony meteorite |  |
has ablative mass loss low because it has higher tensile strength than stony meteorite |  |
metal-rich meteorite | has metal content higher than that of average solar system material |  |
differentiated meteorite | has origin planet or asteroid much larger than 100 km in diameter |  |
meteorite | can have crater image |  |
has impact angle |  |
has monetary value large if the fall was witnessed |  |
often produce power outages and failures in electrical equipment due to EMP (electromagnetic pulse) |  |
can be associated with crater |  |
vaporizes completely if size is between 3 micrometers and 3 millimeters |  |
can survive fall if size is larger than 3 mm and velocity is less than 24 km per second |  |
can survive fall if it fragments because smaller pieces with less mass are more easily slowed by the atmosphere |  |
can shatter during impact phase |  |
can fragment during meteor phase |  |
igneous rock | has solidification mechanism |  |
has solidification timescale |  |
rock | has part mineral |  |
has texture |  |
has genesis |  |