Murchison | has image
 |  |
is an instance of CM chondrite |  |
is an instance of meteorite fall |  |
is an instance of S1 shock stage chondrite |  |
has name Murchison |  |
has fall date September 28, 1969 10:45 am |  |
has fall coordinates 36° 37' S., 145° 12' E. |  |
has fall location Murchison, Victoria, Australia  |  |
have composition contain amino acids |  |
has image
 |  |
CM chondrite | has prototype Mighei meteorite |  |
has chondrule abundance 20 % by volume |  |
has matrix abundance 70 % by volume |  |
has refractory inclusion abundance 5 % by volume |  |
has metal abundance 0.1 % by volume |  |
has chondrule mean diameter 0.3 millimeters |  |
has chondrule glass type rare |  |
has tenacity friable |  |
meteorite fall | has value higher because the fall was witnessed |  |
has fall description what witnesses saw or what was recorded by instruments |  |
has weathering negligible due to quick recovery of meteorite before corrosion begins |  |
S1 shock stage chondrite | has olivine shock metamorphism sharp optical extinction, irregular fractures |  |
has plagioclase shock metamorphism sharp optical extinction, irregular fractures |  |
has orthopyroxene shock metamorphism sharp optical extinction, irregular fractures |  |
carbonaceous chondrite | has relative abundance 8 % of meteorite falls |  |
has total mass of finds 2577 kg |  |
has number of finds 36 |  |
has distinguishing feature elemental carbon |  |
has abundance rare relative to other chondrite types |  |
type 2 chondrite | has petrologic type 2 |  |
has degree of aqueous alteration moderate |  |
has olivine and low Ca pyroxene homogeneity greater than 5 % deviations |  |
has structural state of low Ca pyroxene predominantly monoclinic |  |
has part feldspar minor primary grains only |  |
has part maximum bulk Ni in metal less than 20 % by weight; taenite minor or absent |  |
has part sulfide Ni content greater than 0.5 % by weight |  |
has part matrix mostly fine, opaque |  |
has part chondrule chondrules very sharply defined |  |
has part carbon 0.8 to 2.6 % by weight |  |
has part water 2 to 16 % by weight |  |
meteorite | 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 composition often minerals not found on Earth |  |
has relative abundance |  |
has total mass of finds 485755 kg |  |
has number of finds 1691 |  |
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 |  |
often produce power outages and failures in electrical equipment due to EMP (electromagnetic pulse) |  |
can be associated with crater |  |
has origin meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal |  |
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 |  |
shocked chondrite | is independent of the nature and degree of thermal metamorphism or aqueous alteration |  |
can be shocked before, during or after other types of metamorphism |  |
has shock pressure the equilibration peak shock pressure in GPa (gigapascals) for ordinary chondrites only |  |
has shock diagnostic mineral olivine and plagioclase for ordinary chondrite |  |
has shock diagnostic mineral olivine for carbonaceous chondrite |  |
has shock diagnostic mineral orthopyroxene for enstatite chondrite |  |
S1 shock stage meteorite | has shock stage S1 |  |
has shock pressure less than 5 GPa |  |
has degree of shock metamorphism unshocked |  |
chondrite | has petrologic type range which depends on degree of aqueous alteration and thermal metamorphism |  |
has homogeneity of olivine and low Ca pyroxene definition goes here |  |
has part metal maximum bulk in weight % |  |
has part mean Ni content of sulfides in weight % |  |
water altered chondrite | has metamorphism mechanism aqueous altermation |  |
rock | has part mineral |  |
has texture |  |
has genesis |  |
altered chondrite | has degree of secondary processing providing insight into geological evolution of parent asteroid |  |
shocked meteorite | has metamorphism mechanism shock metamorphism |  |
undifferentiated meteorite | has peak temperature less than 950 degree Celsius during its entire history since solidification |  |
has parent body asteroid smaller than 100 km in diameter |  |
has age oldest and most primitive rock in solar system |  |
conglomerate | has sediment mechanism agglomeration of particles, many of which record individual, diverse histories |  |