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rock > igneous rock > differentiated meteorite > differentiated achondrite > asteroidal achondrite > HED meteorite > eucrite > Camel Donga 003
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Camel Donga 003
subjectfact 
Camel Donga 003is an instance of CK3 chondrite2000-12-14 14:19:13.0
has image
  
2000-12-14 14:19:13.0
has name Camel Donga2000-12-14 14:19:13.0
is an instance of eucrite    2000-12-14 14:19:13.0
has find date 19842000-12-14 14:19:13.0
has fall location Camel Donga, West Australia, Australia2000-12-14 14:19:13.0
eucritehas letter designation AUEC2000-12-14 14:18:46.0
has characteristic mineral anorthite-pigeonite Ca-rich2000-12-14 14:18:46.0
has total mass of finds 231 kg2000-12-14 14:18:46.0
has number of finds 232000-12-14 14:18:46.0
CK chondritehas petrologic type 3 to 62000-12-14 14:18:51.0
has prototype ??? meteorite2000-12-14 14:18:51.0
has chondrule abundance 15 % by volume2000-12-14 14:18:51.0
has matrix abundance 75 % by volume2000-12-14 14:18:51.0
has refractory inclusion abundance 4 % by volume2000-12-14 14:18:51.0
has metal abundance 0.01 % by volume2000-12-14 14:18:51.0
has chondrule mean diameter 0.7 millimeters2000-12-14 14:18:51.0
type 3 chondritehas petrologic type 32000-12-14 14:18:49.0
has degree of aqueous alteration none2000-12-14 14:18:49.0
has degree of thermal metamorphism none2000-12-14 14:18:49.0
has olivine and low Ca pyroxene homogeneity greater than 5 % deviations2000-12-14 14:18:49.0
has structural state of low Ca pyroxene predominantly monoclinic2000-12-14 14:18:49.0
has chondrule glass type clear, isotropic, variable abundance2000-12-14 14:18:49.0
has part feldspar minor primary grains only2000-12-14 14:18:49.0
has part maximum bulk Ni in metal greater than 20 % by weight, kamacite and taenite in exsolution relationship2000-12-14 14:18:49.0
has part sulfide Ni content less than 0.5 % by weight2000-12-14 14:18:49.0
has part matrix clastic and minor opaque2000-12-14 14:18:49.0
has part chondrule chondrules very sharply defined2000-12-14 14:18:49.0
has part carbon 0.2 to 1 % by weight2000-12-14 14:18:49.0
has part water 0.3 to 3 % by weight2000-12-14 14:18:49.0
HED meteoriteis an acronym for Howardite, Eucrite, Diogenite2000-12-14 14:18:45.0
has origin 4 Vesta2000-12-14 14:18:45.0
has minerology orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica2000-12-14 14:18:45.0
has petrology coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated2000-12-14 14:18:45.0
has likely origin cumulates, crystallized melts, impact mixing2000-12-14 14:18:45.0
carbonaceous chondritehas relative abundance 8 % of meteorite falls2000-12-14 14:18:50.0
has distinguishing feature elemental carbon2000-12-14 14:18:50.0
has abundance rare relative to other chondrite types2000-12-14 14:18:50.0
volcanic rockhas solidification mechanism extrusion onto the surface of the planet or asteroid via a volcanic eruption2000-12-14 14:18:22.0
has solidification timescale very rapid2000-12-14 14:18:22.0
chondritehas petrologic type range which depends on degree of aqueous alteration and thermal metamorphism2000-12-14 14:18:47.0
has homogeneity of olivine and low Ca pyroxene definition goes here2000-12-14 14:18:47.0
has part metal maximum bulk in weight %2000-12-14 14:18:47.0
has part mean Ni content of sulfides in weight %2000-12-14 14:18:47.0
igneous rockhas composition silicates (with very few exceptions)2000-12-14 14:18:21.0
stony meteoritehas weather resistance low2000-12-14 14:18:32.0
has fragmentation probability high because it is more friable than iron meteorite2000-12-14 14:18:32.0
has ablative mass loss high because it is more friable than iron meteorite2000-12-14 14:18:32.0
undifferentiated meteoritehas peak temperature less than 950 degree Celsius during its entire history since solidification2000-12-14 14:18:47.0
has parent body asteroid smaller than 100 km in diameter2000-12-14 14:18:47.0
has age oldest and most primitive rock in solar system2000-12-14 14:18:47.0
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
meteoritehas fall date recorded by eyewitness or inferred from dating methods2000-12-14 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
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
conglomeratehas sediment mechanism agglomeration of particles, many of which record individual, diverse histories2000-12-14 14:18:20.0

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