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rock > igneous rock |
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igneous rock comparison table |
Subject | has name | fragment | has impact velocity | has origin | shatter | has number of find | has shade | be associated with | has fall date | has genesi | is a kind of | has fall map | has property | has weather resistance | has fall coordinate | has color index | has fragmentation probability | produce | has monetary value | has solidification mechanism | has total mass of find | has texture | have crater image | has fall location | survive fall if | has impact angle | has solidification timescale | has definition | vaporize completely if | has original mass | has relative abundance | has ablative mass loss |
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allotriomorphic rock | igneous rock | approximately equant anhedral grains | a rock with texture characterized by approximately equant anhedral grains | |||||||||||||||||||||||||||||
differentiated meteorite | based on the locale, region, or nearby town in which the fall occurred | during meteor phase | when it hits the ground which is smaller than its velocity before it enters the atmosphere | planet or asteroid much larger than 100 km in diameter | during impact phase | 1691 | crater | recorded by eyewitness or inferred from dating methods | igneous rock | which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity | which depends on its composition | in degrees, minutes and seconds of lattitude and longitude | during meteor phase which depends on composition | power outages and failures in electrical equipment due to EMP (electromagnetic pulse) | large if the fall was witnessed | 485755 kg | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | it fragments because smaller pieces with less mass are more easily slowed by the atmosphere | size is between 3 micrometers and 3 millimeters | which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site | directly proportional to initial velocity | |||||||||||
fractional crystallized rock | fractional crystallization | gravitationally separated rock | formed by separation of molten rock in a gravity field | a rock produced by differentiation in which part of the magma is crystallized and separated from further reaction with remaining liquid | ||||||||||||||||||||||||||||
hypabyssal rock | igneous rock | extrusion into an undeground dike or sill near the surface | rapid | |||||||||||||||||||||||||||||
hyperleucocratic rock | very light | igneous rock | 10 or less | very light colored rock with color index of 10 or less | ||||||||||||||||||||||||||||
hypermelanocratic rock | very dark | igneous rock | 90 or greater | very dark colored rock with color index greater than 90 | ||||||||||||||||||||||||||||
leucocratic rock | light | igneous rock | 11 to 50 | light-colored rock with color index between 11 and 50 | ||||||||||||||||||||||||||||
melanocratic rock | dark | igneous rock | 50 to 89 | dark-colored rock with color index between 50 and 89 | ||||||||||||||||||||||||||||
plutonic rock | igneous rock | cooling in deep underground chambers | very slow | cooling of magma in the interior of a planet or asteroid | ||||||||||||||||||||||||||||
volcanic rock | igneous rock | extrusion onto the surface of the planet or asteroid via a volcanic eruption | very rapid |
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