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| rock > igneous rock > differentiated meteorite > differentiated achondrite > asteroidal achondrite > HED meteorite |
| 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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