Bilanga Comparison Table

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rock > gravitationally separated rock > fractional crystallized rock > plutonic cumulate > diogenite > Bilanga

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Bilanga comparison table

Subject has weather resistance has probability of occurence has minerology has shape is an instance of has distinguishing feature has fragmentation probability has fall location has fall date has likely origin has solidification mechanism has name has genesi 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 property has mass has image has number of find has origin has ablative mass loss has solidification timescale has definition be an acronym for has petrology

diogenite 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 cooling in deep underground chambers based on the locale, region, or nearby town in which the fall occurred fractional crystallization ADIO 7.1 % of meteorite falls 68 kg in degrees, minutes and seconds of lattitude and longitude hyperstene silicates (with very few exceptions) plutonic cumulate formed by separation of molten rock in a gravity field 8 4 Vesta high because it is more friable than iron meteorite very slow 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

oriented meteorite which depends on its composition higher for non-spherical, flattened or angular meteoroids conical from preferential ablation during atmospheric passage during meteor phase which depends on composition strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity recorded by eyewitness or inferred from dating methods based on the locale, region, or nearby town in which the fall occurred 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 conical meteorite shape resulting from preferential ablation during atmospheric passage

Bilanga which depends on its composition higher for non-spherical, flattened or angular meteoroids orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica conical from preferential ablation during atmospheric passage oriented meteorite no chondrules during meteor phase which depends on composition Bilanga Yanga and Gomponsago, Burkina Faso, Africa 10:30 am October 27, 1999 cumulates, crystallized melts, impact mixing cooling in deep underground chambers Bilanga negligible due to quick recovery of meteorite before corrosion begins what witnesses saw or what was recorded by instruments ADIO higher because the fall was witnessed 68 kg 12° 27' N., 0° 05' W. hyperstene often minerals not found on Earth formed by separation of molten rock in a gravity field 25 kg
8 meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal directly proportional to initial velocity very slow Howardite, Eucrite, Diogenite coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated

Next diogenite: Johnstown Up: diogenite, meteorite fall, oriented meteorite Previous diogenite: Tatahouine

Subject	has weather resistance	has probability of occurence	has minerology	has shape	is an instance of	has distinguishing feature	has fragmentation probability	has fall location	has fall date	has likely origin	has solidification mechanism	has name	has genesi	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 property	has mass	has image	has number of find	has origin	has ablative mass loss	has solidification timescale	has definition	be an acronym for	has petrology
diogenite	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	cooling in deep underground chambers	based on the locale, region, or nearby town in which the fall occurred	fractional crystallization			ADIO	7.1 % of meteorite falls		68 kg	in degrees, minutes and seconds of lattitude and longitude	hyperstene	silicates (with very few exceptions)	plutonic cumulate	formed by separation of molten rock in a gravity field			8	4 Vesta	high because it is more friable than iron meteorite	very slow		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
oriented meteorite	which depends on its composition	higher for non-spherical, flattened or angular meteoroids		conical from preferential ablation during atmospheric passage			during meteor phase which depends on composition	strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity	recorded by eyewitness or inferred from dating methods			based on the locale, region, or nearby town in which the fall occurred							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		conical meteorite shape resulting from preferential ablation during atmospheric passage
Bilanga	which depends on its composition	higher for non-spherical, flattened or angular meteoroids	orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica	conical from preferential ablation during atmospheric passage	oriented meteorite	no chondrules	during meteor phase which depends on composition	Bilanga Yanga and Gomponsago, Burkina Faso, Africa	10:30 am October 27, 1999	cumulates, crystallized melts, impact mixing	cooling in deep underground chambers	Bilanga		negligible due to quick recovery of meteorite before corrosion begins	what witnesses saw or what was recorded by instruments	ADIO		higher because the fall was witnessed	68 kg	12° 27' N., 0° 05' W.	hyperstene	often minerals not found on Earth		formed by separation of molten rock in a gravity field	25 kg		8	meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	directly proportional to initial velocity	very slow		Howardite, Eucrite, Diogenite	coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated