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rock > igneous rock > differentiated meteorite > differentiated achondrite > asteroidal achondrite > HED meteorite |
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HED meteorite (Howardite, Eucrite, Diogenite) | ||||
subject | fact |
HED meteorite | is a kind of asteroidal achondrite | ![]() |
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 | ![]() | |
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 | ![]() | |
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 composition often minerals not found on Earth | ![]() | |
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 | ![]() | |
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 | ![]() | |
igneous rock | has composition silicates (with very few exceptions) | ![]() |
has solidification mechanism | ![]() | |
has solidification timescale | ![]() | |
rock | has part mineral | ![]() |
has texture | ![]() | |
has genesis | ![]() |
Kinds of HED meteorite :
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