Kapoeta | has image
 |  |
is an instance of howardite |  |
is an instance of meteorite fall |  |
has name Kapoeta |  |
has fall date 7:00 pm April 22, 1942 |  |
has fall coordinates 31° 10' S., 127° 45' E. |  |
has fall location Kapoeta-Nathalani Road, Equatoria, Sudan |  |
has mass 11.355 kg |  |
howardite | has letter designation AHOW |  |
has characteristic mineral eucrite-diogenite mixture |  |
has total mass of finds 41 kg |  |
has number of finds 19 |  |
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 |  |
HED meteorite | is an acronym for Howardite, Eucrite, Diogenite |  |
has origin 4 Vesta |  |
has minerology orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica |  |
has petrology coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated |  |
has likely origin cumulates, crystallized melts, impact mixing |  |
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 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 |  |
rock | has part mineral |  |
has texture |  |
has genesis |  |
achondrite | has distinguishing feature no chondrules |  |
igneous rock | has solidification mechanism |  |
has solidification timescale |  |