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rock > igneous rock > differentiated meteorite > metal-rich meteorite > iron meteorite > nonmagmatic iron meteorite > type IAB/IIICD iron meteorite > type IIICD iron meteorite
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type IIICD iron meteorite
subjectfact 
type IIICD iron meteoriteis a kind of type IAB/IIICD iron meteorite2000-12-14 14:18:40.0
is a kind of iron meteorite2000-12-14 14:18:40.0
has composition kamacite, taenite, carbides2000-12-14 14:18:40.0
has structural class Of, Off-D octahedrite, ataxite2000-12-14 14:18:40.0
has formation cooling rate 10 degrees C per million years    has source: Yang, CW. Williams,D.B. Goldstein,J.I. 1997, Meteoritics Planet Sci 32, 423, 2000-12-14 14:18:40.0
parent body radius 51 kilometers    has source: Yang, CW. Williams,D.B. Goldstein,J.I. 1997, Meteoritics Planet Sci 32, 423, 2000-12-14 14:18:40.0
has total mass of finds 199 kg2000-12-14 14:18:40.0
has number of finds 112000-12-14 14:18:40.0
type IAB/IIICD iron meteoritehas origin impact melting2000-12-14 14:18:39.0
has origin asteroid wide partial melting2000-12-14 14:18:39.0
iron meteoritehas relative abundance 5.7 % of meteorite falls2000-12-14 14:18:32.0
has weather resistance high2000-12-14 14:18:32.0
has fragmentation probability low because it is tougher than stony meteorite2000-12-14 14:18:32.0
has ablative mass loss low because it has higher tensile strength than stony meteorite2000-12-14 14:18:32.0
metal-rich meteoritehas metal content higher than that of average solar system material2000-12-14 14:18:32.0
has nickel content always greater than 4 %2000-12-14 14:18:32.0
meteoritehas fall date recorded by eyewitness or inferred from dating methods2000-12-14 14:18:31.0
has fall location strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity2000-12-14 14:18:31.0
has fall coordinates in degrees, minutes and seconds of lattitude and longitude2000-12-14 14:18:31.0
has fall map which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity2000-12-14 14:18:31.0
can have crater image2000-12-14 14:18:31.0
has original mass which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site2000-12-14 14:18:31.0
has impact velocity when it hits the ground which is smaller than its velocity before it enters the atmosphere2000-12-14 14:18:31.0
has impact angle2000-12-14 14:18:31.0
has monetary value large if the fall was witnessed2000-12-14 14:18:31.0
has name based on the locale, region, or nearby town in which the fall occurred2000-12-14 14:18:31.0
often produce power outages and failures in electrical equipment due to EMP (electromagnetic pulse)2000-12-14 14:18:31.0
can be associated with crater2000-12-14 14:18:31.0
vaporizes completely if size is between 3 micrometers and 3 millimeters2000-12-14 14:18:31.0
can survive fall if size is larger than 3 mm and velocity is less than 24 km per second2000-12-14 14:18:31.0
can survive fall if it fragments because smaller pieces with less mass are more easily slowed by the atmosphere2000-12-14 14:18:31.0
can shatter during impact phase2000-12-14 14:18:31.0
can fragment during meteor phase2000-12-14 14:18:31.0
igneous rockhas solidification mechanism2000-12-14 14:18:21.0
has solidification timescale2000-12-14 14:18:21.0
rockhas part mineral2000-12-14 14:18:20.0
has texture2000-12-14 14:18:20.0
has genesis2000-12-14 14:18:20.0

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