Kapoeta Comparison Table

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rock > igneous rock > differentiated meteorite > differentiated achondrite > asteroidal achondrite > HED meteorite > howardite > Kapoeta

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Kapoeta comparison table

Subject has weather resistance has minerology is an instance of has distinguishing feature has fragmentation probability has fall location has fall date has likely origin has name has weather has fall description has letter designation has relative abundance has value has total mass of find has fall coordinate has characteristic mineral has composition is a kind of has mass has image has number of find has origin has ablative mass loss has definition be an acronym for has petrology

howardite low orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica no chondrules high because it is more friable than iron meteorite strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity recorded by eyewitness or inferred from dating methods cumulates, crystallized melts, impact mixing based on the locale, region, or nearby town in which the fall occurred AHOW 7.1 % of meteorite falls 41 kg in degrees, minutes and seconds of lattitude and longitude eucrite-diogenite mixture silicates (with very few exceptions) HED meteorite 19 4 Vesta high because it is more friable than iron meteorite Howardite, Eucrite, Diogenite coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated

meteorite fall which depends on its composition during meteor phase which depends on composition strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity recorded by eyewitness or instruments based on the locale, region, or nearby town in which the fall occurred negligible due to quick recovery of meteorite before corrosion begins what witnesses saw or what was recorded by instruments higher because the fall was witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude often minerals not found on Earth meteorite 1691 meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal directly proportional to initial velocity a meteorite whose fall was witnessed by human or electronic means

Kapoeta which depends on its composition orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica meteorite fall no chondrules during meteor phase which depends on composition Kapoeta-Nathalani Road, Equatoria, Sudan 7:00 pm April 22, 1942 cumulates, crystallized melts, impact mixing Kapoeta negligible due to quick recovery of meteorite before corrosion begins what witnesses saw or what was recorded by instruments AHOW higher because the fall was witnessed 41 kg 31° 10' S., 127° 45' E. eucrite-diogenite mixture often minerals not found on Earth 11.355 kg
19 meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal directly proportional to initial velocity Howardite, Eucrite, Diogenite coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated

Next howardite: Old Homestead 001 Up: howardite, meteorite fall

Subject	has weather resistance	has minerology	is an instance of	has distinguishing feature	has fragmentation probability	has fall location	has fall date	has likely origin	has name	has weather	has fall description	has letter designation	has relative abundance	has value	has total mass of find	has fall coordinate	has characteristic mineral	has composition	is a kind of	has mass	has image	has number of find	has origin	has ablative mass loss	has definition	be an acronym for	has petrology
howardite	low	orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica		no chondrules	high because it is more friable than iron meteorite	strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity	recorded by eyewitness or inferred from dating methods	cumulates, crystallized melts, impact mixing	based on the locale, region, or nearby town in which the fall occurred			AHOW	7.1 % of meteorite falls		41 kg	in degrees, minutes and seconds of lattitude and longitude	eucrite-diogenite mixture	silicates (with very few exceptions)	HED meteorite			19	4 Vesta	high because it is more friable than iron meteorite		Howardite, Eucrite, Diogenite	coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated
meteorite fall	which depends on its composition				during meteor phase which depends on composition	strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity	recorded by eyewitness or instruments		based on the locale, region, or nearby town in which the fall occurred	negligible due to quick recovery of meteorite before corrosion begins	what witnesses saw or what was recorded by instruments			higher because the fall was witnessed	485755 kg	in degrees, minutes and seconds of lattitude and longitude		often minerals not found on Earth	meteorite			1691	meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	directly proportional to initial velocity	a meteorite whose fall was witnessed by human or electronic means
Kapoeta	which depends on its composition	orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica	meteorite fall	no chondrules	during meteor phase which depends on composition	Kapoeta-Nathalani Road, Equatoria, Sudan	7:00 pm April 22, 1942	cumulates, crystallized melts, impact mixing	Kapoeta	negligible due to quick recovery of meteorite before corrosion begins	what witnesses saw or what was recorded by instruments	AHOW		higher because the fall was witnessed	41 kg	31° 10' S., 127° 45' E.	eucrite-diogenite mixture	often minerals not found on Earth		11.355 kg		19	meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	directly proportional to initial velocity		Howardite, Eucrite, Diogenite	coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated