EETA 79001 Comparison Table

Meteorites View all facts Glossary Help

rock > gravitationally separated rock > depleted basalt > depleted basalt shergottite > EETA 79001

Next Antarctic meteorite: Isna Up: Antarctic meteorite, depleted basalt shergottite Previous Antarctic meteorite: EET 87720

EETA 79001 comparison table

Subject has CaO content has weather resistance has MnO content is an instance of has distinguishing feature has TiO2 content has FeO content has fragmentation probability has fall location has P2O5 content has solidification mechanism has name has sulfur content has Al2O3 content has identification date has letter designation has relative abundance has curatorial location has total mass of find has SiO2 content has MgO content has composition is a kind of has find date has K2O content has Na2O content has property has mass has number of find has origin has ablative mass loss has solidification timescale has Cr2O3 content be an acronym for

Antarctic meteorite which depends on its composition during meteor phase which depends on composition indicated by letters in the beginning of name 3 or 4 letter contracted from find location then last two digits of year then id number 485755 kg often minerals not found on Earth meteorite recovery year is first 2 numbers in name 1691 meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal directly proportional to initial velocity

depleted basalt shergottite low no chondrules high because it is more friable than iron meteorite strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity extrusion onto the surface of the planet or asteroid via a volcanic eruption based on the locale, region, or nearby town in which the fall occurred AEUC 7.1 % of meteorite falls 1606 kg depleted by gravitational separation depleted basalt formed by separation of molten rock in a gravity field 70 Mars high because it is more friable than iron meteorite very rapid Shergottite, Nakhilite, Chassignite

EETA 79001 7.22 % by mass which depends on its composition 0.48 % by mass Antarctic meteorite no chondrules 0.63 % by mass 18.6 % by mass during meteor phase which depends on composition Elephant Moraine, Antarctica 0.60 % by mass extrusion onto the surface of the planet or asteroid via a volcanic eruption EETA 79001 0.20 % by mass 5.69 % by mass 1980 AEUC MWG (JSC), SI 485755 kg 48.5 % by mass 16.4 % by mass often minerals not found on Earth 1979 0.04 % by mass 0.84 % by mass formed by separation of molten rock in a gravity field 7.90 kg 1691 meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal directly proportional to initial velocity very rapid 0.61 % by mass Shergottite, Nakhilite, Chassignite

Next Antarctic meteorite: Isna Up: Antarctic meteorite, depleted basalt shergottite Previous Antarctic meteorite: EET 87720

Subject	has CaO content	has weather resistance	has MnO content	is an instance of	has distinguishing feature	has TiO2 content	has FeO content	has fragmentation probability	has fall location	has P2O5 content	has solidification mechanism	has name	has sulfur content	has Al2O3 content	has identification date	has letter designation	has relative abundance	has curatorial location	has total mass of find	has SiO2 content	has MgO content	has composition	is a kind of	has find date	has K2O content	has Na2O content	has property	has mass	has number of find	has origin	has ablative mass loss	has solidification timescale	has Cr2O3 content	be an acronym for
Antarctic meteorite		which depends on its composition						during meteor phase which depends on composition	indicated by letters in the beginning of name			3 or 4 letter contracted from find location then last two digits of year then id number							485755 kg			often minerals not found on Earth	meteorite	recovery year is first 2 numbers in name					1691	meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	directly proportional to initial velocity
depleted basalt shergottite		low			no chondrules			high because it is more friable than iron meteorite	strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity		extrusion onto the surface of the planet or asteroid via a volcanic eruption	based on the locale, region, or nearby town in which the fall occurred				AEUC	7.1 % of meteorite falls		1606 kg			depleted by gravitational separation	depleted basalt				formed by separation of molten rock in a gravity field		70	Mars	high because it is more friable than iron meteorite	very rapid		Shergottite, Nakhilite, Chassignite
EETA 79001	7.22 % by mass	which depends on its composition	0.48 % by mass	Antarctic meteorite	no chondrules	0.63 % by mass	18.6 % by mass	during meteor phase which depends on composition	Elephant Moraine, Antarctica	0.60 % by mass	extrusion onto the surface of the planet or asteroid via a volcanic eruption	EETA 79001	0.20 % by mass	5.69 % by mass	1980	AEUC		MWG (JSC), SI	485755 kg	48.5 % by mass	16.4 % by mass	often minerals not found on Earth		1979	0.04 % by mass	0.84 % by mass	formed by separation of molten rock in a gravity field	7.90 kg	1691	meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	directly proportional to initial velocity	very rapid	0.61 % by mass	Shergottite, Nakhilite, Chassignite