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rock > igneous rock > differentiated meteorite > metal-rich meteorite > iron meteorite > magmatic iron meteorite > type IIIAB iron meteorite
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type IIIAB iron meteorite
subjectfact 
type IIIAB iron meteoriteis a kind of magmatic iron meteorite2000-12-14 14:18:36.0
is a kind of Om octahedrite2000-12-14 14:18:36.0
has composition kamacite, taenite, trolite, phosphides2000-12-14 14:18:36.0
has formation cooling rate 3 to 75 degrees C per million years    has source: Haack,H. Rasmussen,K.L., Warren,P.H. 1990, J Geophys Res 95, 5111, 2000-12-14 14:18:36.0
parent body radius 20 to 90 kilometers    has source: Haack,H. Rasmussen,K.L., Warren,P.H. 1990, J Geophys Res 95, 5111, 2000-12-14 14:18:36.0
has total mass of finds 128986 kg2000-12-14 14:18:36.0
has number of finds 1572000-12-14 14:18:36.0
has nickel content 8.49 % by weight    has source: Willis, J. 1980 PhD Dissertation, Univ. California, 2000-12-14 14:18:36.0
has gallium content 19.7 microgram/gram    has source: Willis, J. 1980 PhD Dissertation, Univ. California, 2000-12-14 14:18:36.0
has germanium content 38.9 microgram/gram    has source: Willis, J. 1980 PhD Dissertation, Univ. California, 2000-12-14 14:18:36.0
has iridium content 4.1 microgram/gram    has source: Willis, J. 1980 PhD Dissertation, Univ. California, 2000-12-14 14:18:36.0
has carbon content 140 microgram/gram    has source: Willis, J. Goldstein, 1982, 13th Lunar and Planetary Sci Conf, 435 (final composition, table 5), 2000-12-14 14:18:36.0
has phosphor content 5.6 milligram/gram    has source: Willis, J. 1980 PhD Dissertation, Univ. California, 2000-12-14 14:18:36.0
has sulfur content 1.4 % by weight    has source: Willis, J. Goldstein, 1982, 13th Lunar and Planetary Sci Conf, 435 (final composition, table 5), 2000-12-14 14:18:36.0
has chromium content 40 microgram/gram    has source: Willis, J. 1980 PhD Dissertation, Univ. California, 2000-12-14 14:18:36.0
has cobalt content 5.0 milligram/gram    has source: Willis, J. 1980 PhD Dissertation, Univ. California, 2000-12-14 14:18:36.0
has copper content 160 microgram/gram    has source: Willis, J. 1980 PhD Dissertation, Univ. California, 2000-12-14 14:18:36.0
has molydbenum content 7.2 microgram/gram    has source: Willis, J. 1980 PhD Dissertation, Univ. California, 2000-12-14 14:18:36.0
has tungsten content 1 microgram/gram    has source: Willis, J. 1980 PhD Dissertation, Univ. California, 2000-12-14 14:18:37.0
has palladium content 3.5 microgram/gram    has source: Willis, J. 1980 PhD Dissertation, Univ. California, 2000-12-14 14:18:37.0
has gold content 1.2 microgram/gram    has source: Willis, J. 1980 PhD Dissertation, Univ. California, 2000-12-14 14:18:37.0
has arsenic content 10.5 microgram/gram    has source: Willis, J. 1980 PhD Dissertation, Univ. California, 2000-12-14 14:18:37.0
has antimony content 265 nanogram/gram    has source: Willis, J. 1980 PhD Dissertation, Univ. California, 2000-12-14 14:18:37.0
Om octahedritehas structural class Om2000-12-14 14:18:33.0
has crystal size 0.5 to 1.3 mm (medium)2000-12-14 14:18:33.0
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
structural iron meteoritehas distinguishing feature crystalline iron-nickel alloy2000-12-14 14:18:33.0
differentiated meteoritehas origin planet or asteroid much larger than 100 km in diameter2000-12-14 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

Kinds of type IIIAB iron meteorite :

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