| Giroux | is an instance of main group pallasite |  |
| has olivine SiO2 content 40.8 % by weight |  |
| has olivine FeO content 10.7 % by weight |  |
| has olivine MgO content 48.9 % by weight |  |
| has olivine MnO content 0.25 % by weight |  |
| has olivine Cr2O3 content 0.052 % by weight |  |
| has olivine CaO content 0.017 % by weight |  |
| has olivine Fe/Mn ratio 42 |  |
| has olivine magnesium content 89.1 mg# or 100 * Mg/(Mg + Fe) |  |
| has olivine scandium content 1.09 microgram/gram using Instrumental Neutron Activation Analysis |  |
| has olivine chromium content 312 microgram/gram using Instrumental Neutron Activation Analysis |  |
| has olivine manganese content 2.14 milligram/gram using Instrumental Neutron Activation Analysis |  |
| has olivine cobalt content 6.40 microgram/gram using Instrumental Neutron Activation Analysis |  |
| has olivine nickel content 18.3 microgram/gram using Instrumental Neutron Activation Analysis |  |
| has olivine zinc content 7.0 microgram/gram using Instrumental Neutron Activation Analysis |  |
| main group pallasite | has olivine composition Fo 88+-1 |  |
| has olivine composition uniformity heterogeneous elements are zoned between grain rim and core |  |
| has minor mineral troilite |  |
| has minor mineral schreibersite |  |
| has troilite content 0.1 to 7.3 % by volume |  |
| has schreibersite content 0.3 to 2.8 % by volume |  |
| pallasite | has composition metallic iron plus olivine; core/mantle boundary samples |  |
| has letter designation PAL |  |
| has olivine content 35 to 85 % by volume |  |
| has phosphate content 1 % or less by volume |  |
| has chromite content 1 % or less by volume |  |
| has olivine grain shape from angular fragments to rounded |  |
| has olivine grain size typically one centimeter |  |
| has olivine crystal distribution from homogeneous to heterogeneous |  |
| has formation cooling rate 2.5 to 4 degrees C per million years |  |
| parent body radius 78 to 97 kilometers |  |
| has total mass of finds 7207 kg |  |
| has number of finds 33 |  |
| stony iron meteorite | has distinguishing feature mixture of iron-nickel alloy and non-metallic minerals |  |
| has relative abundance 1.5 % of meteorite falls |  |
| metal-rich meteorite | has metal content higher than that of average solar system material |  |
| has nickel content always greater than 4 % |  |
| differentiated meteorite | has origin planet or asteroid much larger than 100 km in diameter |  |
| 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 impact velocity when it hits the ground which is smaller than its velocity before it enters the atmosphere |  |
| has impact angle |  |
| has weather resistance which depends on its composition |  |
| 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 |  |
| has ablative mass loss depending on composition, more friable stony meteoroids loses more mass than iron meteoroid |  |
| has ablative mass loss directly proportional to initial velocity |  |
| can shatter during impact phase |  |
| can fragment during meteor phase |  |
| has fragmentation probability during meteor phase which depends on composition |  |
| igneous rock | has solidification mechanism |  |
| has solidification timescale |  |
| rock | has part mineral |  |
| has texture |  |
| has genesis |  |