winonaite | is a kind of primitive achondrite |  |
has composition IAB-silica related |  |
has inclusion minerology troilite, metal, daubreilite, schreibersite, graphite |  |
has prototype Winona meteorite |  |
primitive achondrite | has minerology olivine, orthopyroxene, clinopyroxene, metal with some troilite and some sodic plagioclase |  |
has petrology fine- to coarse-grained equigranular |  |
has likely origin ultrametamorphism, partial melting with some melt migration |  |
achondrite | has relative abundance 7.1 % of meteorite falls |  |
has distinguishing feature no chondrules |  |
has number of finds 70 |  |
has total mass of finds 1606 kg |  |
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 |  |
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 |  |
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 |  |
stony meteorite | has weather resistance low |  |
has fragmentation probability high because it is more friable than iron meteorite |  |
has ablative mass loss high because it is more friable than iron meteorite |  |
conglomerate | has sediment mechanism agglomeration of particles, many of which record individual, diverse histories |  |
rock | has part mineral |  |
has texture |  |
has genesis |  |