EET 83309 | is an instance of polymict ureilite |  |
is an instance of meteorite find |  |
has olivine composition Fo% 80-84 for monomict ureilitic clasts |  |
has pigeonite composition Wo% variable En% variable for monomict ureilitic clasts |  |
has pyroxene content 0.27 in modal pyroxene/(pryroxene+olivine) for monomict ureilitic clasts |  |
has reference Prinz et al. (1987) |  |
is an instance of polymict ureilite |  |
is an instance of Antarctic meteorite |  |
has name EET 83309 |  |
has fall location Elephant Moraine, Antarctica |  |
has find date 1983 |  |
polymict ureilite | has lithic clast composition typical monomict ureilite material plus a variety of other lithic clasts |  |
has matrix composition smaller mineral fragments, carbon, suessite (Fe3Si), sulfides, minor chromite and minor apatite |  |
has plagioclase common in clasts |  |
meteorite find | has value lower because the fall was not witnessed |  |
has weathering can be severe due to long exposure time to environmental corrosion agents |  |
Antarctic meteorite | has identification date |  |
ureilite | has letter designation AURE |  |
has characteristic mineral olivine-pigeonite about 90% by volume |  |
has total mass of finds 9 kg (out of date) |  |
has number of finds 6 (out of date) |  |
has minerology olivine, pyroxene (some combination of pigeonite, orthopyroxene, augite) |  |
has petrology coarse-grained granular |  |
has likely origin partial melting residue |  |
has olivine grain characteristic reduced rims contacting carbonaceous matrix material 0.1 mm FeO-free olivine and/or enstatite rims riddled with tiny inclusions of low-Ni metal |  |
meteorite | has fall date recorded by eyewitness or inferred from dating methods |  |
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 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 |  |
breccia | has pronunciation bre - chia |  |
rock | has part mineral |  |
has texture |  |
has genesis |  |
plutonic rock | has solidification mechanism cooling in deep underground chambers |  |
has solidification timescale very slow |  |
sedimentary rock | has sediment mechanism |  |
achondrite | has distinguishing feature no chondrules |  |