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rock > igneous rock > differentiated meteorite > metal-rich meteorite > iron meteorite > nonmagmatic iron meteorite > type IAB/IIICD iron meteorite > type IAB iron meteorite > IAB iron with angular silicate inclusions and winonaites

IAB iron with angular silicate inclusions and winonaites
subject			fact

IAB iron with angular silicate inclusions and winonaites	is a kind of type IAB iron meteorite
type IAB iron meteorite	has formation cooling rate 25 degrees C per million years
	parent body radius 33 kilometers
	has shape of inclusion
	has texture
	has mafic minerals includes olivine, orthopyroxene and clinopyroxene in % by volume
	has plagioclase % by volume
	has troilite % by volume
	has metal % by volume
	has W.P. % by volume
	has chr % by volume
	has daubreelite % by volume
	has schreibersite % by volume
	has graphite % by volume
	has cohenite % by volume
	has nickel content 6.4 % by weight
	has gallium content 96 microgram/gram
	has germanium content 400 microgram/gram
	has iridium content 2.7 microgram/gram
	has phosphor content 2.1 milligram/gram
	has chromium content 16 microgram/gram
	has cobalt content 4.6 milligram/gram
	has copper content 132 microgram/gram
	has molydbenum content 8.2 microgram/gram
	has tungsten content 1.6 microgram/gram
	has palladium content 3.5 microgram/gram
	has gold content 1.5 microgram/gram
	has arsenic content 11 microgram/gram
	has antimony content 270 nanogram/gram
type IAB/IIICD iron meteorite	has origin impact melting
	has origin asteroid wide partial melting
iron meteorite	has relative abundance 5.7 % of meteorite falls
	has total mass of finds 454624 kg
	has number of finds 532
	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
meteorite	has fall date recorded by eyewitness or inferred from dating methods
	has fall location strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity
	has fall coordinates in degrees, minutes and seconds of lattitude and longitude
	has fall map which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity
	can have crater image
	has original mass which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site
	has composition often minerals not found on Earth
	has impact velocity when it hits the ground which is smaller than its velocity before it enters the atmosphere
	has impact angle
	has monetary value large if the fall was witnessed
	has name based on the locale, region, or nearby town in which the fall occurred
	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 composition silicates (with very few exceptions)
	has solidification mechanism
	has solidification timescale
rock	has part mineral
	has genesis

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