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rock > igneous rock > differentiated meteorite > metal-rich meteorite > stony iron meteorite > pallasite > main group pallasite > Giroux
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Giroux
subjectfact 
Girouxis an instance of main group pallasite2000-12-14 14:19:22.0
has olivine SiO2 content 40.8 % by weighthas source: Mittlefehldt, 2000-12-14 14:19:22.0
has olivine FeO content 10.7 % by weighthas source: Mittlefehldt, 2000-12-14 14:19:22.0
has olivine MgO content 48.9 % by weighthas source: Mittlefehldt, 2000-12-14 14:19:23.0
has olivine MnO content 0.25 % by weighthas source: Mittlefehldt, 2000-12-14 14:19:23.0
has olivine Cr2O3 content 0.052 % by weighthas source: Mittlefehldt, 2000-12-14 14:19:23.0
has olivine CaO content 0.017 % by weighthas source: Mittlefehldt, 2000-12-14 14:19:23.0
has olivine Fe/Mn ratio 42has source: Mittlefehldt, 2000-12-14 14:19:23.0
has olivine magnesium content 89.1 mg# or 100 * Mg/(Mg + Fe)has source: Mittlefehldt, 2000-12-14 14:19:23.0
has olivine scandium content 1.09 microgram/gram using Instrumental Neutron Activation Analysishas source: Mittlefehldt, 2000-12-14 14:19:23.0
has olivine chromium content 312 microgram/gram using Instrumental Neutron Activation Analysishas source: Mittlefehldt, 2000-12-14 14:19:23.0
has olivine manganese content 2.14 milligram/gram using Instrumental Neutron Activation Analysishas source: Davis, A.M. 1977, PhD Yale Univ., 2000-12-14 14:19:23.0
has olivine cobalt content 6.40 microgram/gram using Instrumental Neutron Activation Analysishas source: Mittlefehldt, 2000-12-14 14:19:23.0
has olivine nickel content 18.3 microgram/gram using Instrumental Neutron Activation Analysishas source: Mittlefehldt, 2000-12-14 14:19:23.0
has olivine zinc content 7.0 microgram/gram using Instrumental Neutron Activation Analysishas source: Mittlefehldt, 2000-12-14 14:19:23.0
main group pallasitehas olivine composition Fo 88+-12000-12-14 14:18:41.0
has olivine composition uniformity heterogeneous elements are zoned between grain rim and core2000-12-14 14:18:41.0
has minor mineral troilite2000-12-14 14:18:41.0
has minor mineral schreibersite2000-12-14 14:18:41.0
has troilite content 0.1 to 7.3 % by volume2000-12-14 14:18:41.0
has schreibersite content 0.3 to 2.8 % by volume2000-12-14 14:18:41.0
pallasitehas composition metallic iron plus olivine; core/mantle boundary samples2000-12-14 14:18:41.0
has letter designation PAL2000-12-14 14:18:41.0
has olivine content 35 to 85 % by volume2000-12-14 14:18:41.0
has phosphate content 1 % or less by volume2000-12-14 14:18:41.0
has chromite content 1 % or less by volume2000-12-14 14:18:41.0
has olivine grain shape from angular fragments to rounded2000-12-14 14:18:41.0
has olivine grain size typically one centimeter2000-12-14 14:18:41.0
has olivine crystal distribution from homogeneous to heterogeneous2000-12-14 14:18:41.0
has formation cooling rate 2.5 to 4 degrees C per million years2000-12-14 14:18:41.0
parent body radius 78 to 97 kilometers2000-12-14 14:18:41.0
has total mass of finds 7207 kg2000-12-14 14:18:41.0
has number of finds 332000-12-14 14:18:41.0
stony iron meteoritehas distinguishing feature mixture of iron-nickel alloy and non-metallic minerals2000-12-14 14:18:41.0
has relative abundance 1.5 % of meteorite falls2000-12-14 14:18:41.0
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
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 weather resistance which depends on its composition2000-12-14 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
has ablative mass loss depending on composition, more friable stony meteoroids loses more mass than iron meteoroid2000-12-14 14:18:31.0
has ablative mass loss directly proportional to initial velocity2000-12-14 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
has fragmentation probability during meteor phase which depends on composition2000-12-14 14:18:32.0
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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