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rock > gravitationally separated rock > fractional crystallized rock > plutonic cumulate > diogenite > Tatahouine
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Tatahouine
subjectfact 
Tatahouinehas image
  
2000-12-14 14:19:38.0
is an instance of diogenite    2000-12-14 14:19:38.0
is an instance of meteorite fall2000-12-14 14:19:39.0
has name Tatahouine2000-12-14 14:19:39.0
has fall date 1:30 am June 27, 19312000-12-14 14:19:39.0
has fall coordinates 32° 57' N., 10° 25' E.2000-12-14 14:19:39.0
has fall location Foum Tatahouine, 4 km NE of a small village in Tunisia2000-12-14 14:19:39.0
has mass 13.5 kg2000-12-14 14:19:39.0
has image
  
2000-12-14 14:19:39.0
diogenitehas letter designation ADIO2000-12-14 14:18:46.0
has characteristic mineral hyperstene2000-12-14 14:18:46.0
has total mass of finds 68 kg2000-12-14 14:18:46.0
has number of finds 82000-12-14 14:18:46.0
meteorite fallhas value higher because the fall was witnessed2000-12-14 14:18:32.0
has fall description what witnesses saw or what was recorded by instruments2000-12-14 14:18:32.0
has weathering negligible due to quick recovery of meteorite before corrosion begins2000-12-14 14:18:32.0
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
meteoritehas 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 composition often minerals not found on Earth2000-12-14 14:18:31.0
has relative abundance2000-12-14 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 weather resistance which depends on its composition2000-12-14 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
has origin meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal2000-12-14 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
has ablative mass loss depending on composition, more friable stony meteoroids loses more mass than iron meteoroid2000-12-14 14:18:31.0
has ablative mass loss directly proportional to initial velocity2000-12-14 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
has fragmentation probability during meteor phase which depends on composition2000-12-14 14:18:32.0
plutonic rockhas solidification mechanism cooling in deep underground chambers2000-12-14 14:18:22.0
has solidification timescale very slow2000-12-14 14:18:22.0
fractional crystallized rockhas genesis fractional crystallization2000-12-14 14:18:21.0
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
gravitationally separated rockhas property formed by separation of molten rock in a gravity field2000-12-14 14:18:20.0
achondritehas distinguishing feature no chondrules2000-12-14 14:18:42.0

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