EETA 79001 | is an instance of depleted basalt shergottite |  |
is an instance of Antarctic meteorite |  |
has name EETA 79001 |  |
has fall location Elephant Moraine, Antarctica |  |
has find date 1979 |  |
has identification date 1980 |  |
has mass 7.90 kg |  |
has curatorial location MWG (JSC), SI |  |
has SiO2 content 48.5 % by mass |  |
has TiO2 content 0.63 % by mass |  |
has Al2O3 content 5.69 % by mass |  |
has Cr2O3 content 0.61 % by mass |  |
has FeO content 18.6 % by mass |  |
has MnO content 0.48 % by mass |  |
has MgO content 16.4 % by mass |  |
has CaO content 7.22 % by mass |  |
has Na2O content 0.84 % by mass |  |
has K2O content 0.04 % by mass |  |
has P2O5 content 0.60 % by mass |  |
has sulfur content 0.20 % by mass |  |
shergottite | has letter designation AEUC |  |
depleted basalt | has composition depleted by gravitational separation |  |
meteorite | has fall date recorded by eyewitness or inferred from dating methods |  |
has fall coordinates in degrees, minutes and seconds of lattitude and longitude |  |
has fall map which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity |  |
can have crater image |  |
has original mass which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site |  |
has composition often minerals not found on Earth |  |
has relative abundance |  |
has total mass of finds 485755 kg |  |
has number of finds 1691 |  |
has impact velocity when it hits the ground which is smaller than its velocity before it enters the atmosphere |  |
has impact angle |  |
has weather resistance which depends on its composition |  |
has monetary value large if the fall was witnessed |  |
often produce power outages and failures in electrical equipment due to EMP (electromagnetic pulse) |  |
can be associated with crater |  |
has origin meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal |  |
vaporizes completely if size is between 3 micrometers and 3 millimeters |  |
can survive fall if size is larger than 3 mm and velocity is less than 24 km per second |  |
can survive fall if it fragments because smaller pieces with less mass are more easily slowed by the atmosphere |  |
has ablative mass loss depending on composition, more friable stony meteoroids loses more mass than iron meteoroid |  |
has ablative mass loss directly proportional to initial velocity |  |
can shatter during impact phase |  |
can fragment during meteor phase |  |
has fragmentation probability during meteor phase which depends on composition |  |
SNC meteorite | is an acronym for Shergottite, Nakhilite, Chassignite |  |
volcanic rock | has solidification mechanism extrusion onto the surface of the planet or asteroid via a volcanic eruption |  |
has solidification timescale very rapid |  |
gravitationally separated rock | has property formed by separation of molten rock in a gravity field |  |
rock | has part mineral |  |
has texture |  |
has genesis |  |
achondrite | has distinguishing feature no chondrules |  |