HaH 193 Comparison Table

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Next Hammadah al Hamra meteorite: HaH 259 Up: Hammadah al Hamra meteorite, S1 shock stage meteorite, winonaite Previous Hammadah al Hamra meteorite: HaH 180

HaH 193 comparison table

Subject has sediment mechanism has weather resistance has minerology has degree of shock metamorphism has age has shock stage is an instance of has distinguishing feature has fragmentation probability has fall location has metamorphism mechanism has likely origin has name has weather has weathering stage has acronym has relative abundance has prototype has value has total mass of find has peak temperature has parent body has fall coordinate has composition is a kind of has find date has mass has image has number of find has ablative mass loss has inclusion minerology has shock pressure has petrology

Hammadah al Hamra meteorite which depends on its composition during meteor phase which depends on composition Hammadah al Hamra based on the locale, region, or nearby town in which the fall occurred can be severe due to long exposure time to environmental corrosion agents HaH lower because the fall was not witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude often minerals not found on Earth Sahara meteorite when the meteorite was found 1691 directly proportional to initial velocity

S1 shock stage meteorite which depends on its composition unshocked S1 during meteor phase which depends on composition strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity shock metamorphism 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 shocked meteorite 1691 directly proportional to initial velocity less than 5 GPa

winonaite agglomeration of particles, many of which record individual, diverse histories low olivine, orthopyroxene, clinopyroxene, metal with some troilite and some sodic plagioclase oldest and most primitive rock in solar system no chondrules high because it is more friable than iron meteorite strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity ultrametamorphism, partial melting with some melt migration based on the locale, region, or nearby town in which the fall occurred 7.1 % of meteorite falls Winona meteorite 1606 kg less than 950 degree Celsius during its entire history since solidification asteroid smaller than 100 km in diameter in degrees, minutes and seconds of lattitude and longitude IAB-silica related primitive achondrite 70 high because it is more friable than iron meteorite troilite, metal, daubreilite, schreibersite, graphite fine- to coarse-grained equigranular

HaH 193 agglomeration of particles, many of which record individual, diverse histories which depends on its composition olivine, orthopyroxene, clinopyroxene, metal with some troilite and some sodic plagioclase unshocked oldest and most primitive rock in solar system S1 S1 shock stage meteorite no chondrules during meteor phase which depends on composition Hammadah al Hamra shock metamorphism ultrametamorphism, partial melting with some melt migration HaH 193 can be severe due to long exposure time to environmental corrosion agents W3 HaH Winona meteorite lower because the fall was not witnessed 485755 kg less than 950 degree Celsius during its entire history since solidification asteroid smaller than 100 km in diameter 28° 39.28' N., 13° 27.52' E. IAB-silica related October 1996 0.259 kg
1691 directly proportional to initial velocity troilite, metal, daubreilite, schreibersite, graphite less than 5 GPa fine- to coarse-grained equigranular

Next Hammadah al Hamra meteorite: HaH 259 Up: Hammadah al Hamra meteorite, S1 shock stage meteorite, winonaite Previous Hammadah al Hamra meteorite: HaH 180

Subject	has sediment mechanism	has weather resistance	has minerology	has degree of shock metamorphism	has age	has shock stage	is an instance of	has distinguishing feature	has fragmentation probability	has fall location	has metamorphism mechanism	has likely origin	has name	has weather	has weathering stage	has acronym	has relative abundance	has prototype	has value	has total mass of find	has peak temperature	has parent body	has fall coordinate	has composition	is a kind of	has find date	has mass	has image	has number of find	has ablative mass loss	has inclusion minerology	has shock pressure	has petrology
Hammadah al Hamra meteorite		which depends on its composition							during meteor phase which depends on composition	Hammadah al Hamra			based on the locale, region, or nearby town in which the fall occurred	can be severe due to long exposure time to environmental corrosion agents		HaH			lower because the fall was not witnessed	485755 kg			in degrees, minutes and seconds of lattitude and longitude	often minerals not found on Earth	Sahara meteorite	when the meteorite was found			1691	directly proportional to initial velocity
S1 shock stage meteorite		which depends on its composition		unshocked		S1			during meteor phase which depends on composition	strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity	shock metamorphism		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	shocked meteorite				1691	directly proportional to initial velocity		less than 5 GPa
winonaite	agglomeration of particles, many of which record individual, diverse histories	low	olivine, orthopyroxene, clinopyroxene, metal with some troilite and some sodic plagioclase		oldest and most primitive rock in solar system			no chondrules	high because it is more friable than iron meteorite	strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity		ultrametamorphism, partial melting with some melt migration	based on the locale, region, or nearby town in which the fall occurred				7.1 % of meteorite falls	Winona meteorite		1606 kg	less than 950 degree Celsius during its entire history since solidification	asteroid smaller than 100 km in diameter	in degrees, minutes and seconds of lattitude and longitude	IAB-silica related	primitive achondrite				70	high because it is more friable than iron meteorite	troilite, metal, daubreilite, schreibersite, graphite		fine- to coarse-grained equigranular
HaH 193	agglomeration of particles, many of which record individual, diverse histories	which depends on its composition	olivine, orthopyroxene, clinopyroxene, metal with some troilite and some sodic plagioclase	unshocked	oldest and most primitive rock in solar system	S1	S1 shock stage meteorite	no chondrules	during meteor phase which depends on composition	Hammadah al Hamra	shock metamorphism	ultrametamorphism, partial melting with some melt migration	HaH 193	can be severe due to long exposure time to environmental corrosion agents	W3	HaH		Winona meteorite	lower because the fall was not witnessed	485755 kg	less than 950 degree Celsius during its entire history since solidification	asteroid smaller than 100 km in diameter	28° 39.28' N., 13° 27.52' E.	IAB-silica related		October 1996	0.259 kg		1691	directly proportional to initial velocity	troilite, metal, daubreilite, schreibersite, graphite	less than 5 GPa	fine- to coarse-grained equigranular