Saratov | has image
 |  |
has name Saratov |  |
is an instance of L4 chondrite  |  |
has fall date September 6, 1918, 1800 hrs |  |
has fall location Near Donguz, Penza, Russia |  |
has original mass greater than 328 kg |  |
L4 chondrite | has total mass of finds 1197 kg |  |
has number of finds 21 |  |
L chondrite | has synonym hypersthene chondrite |  |
has chondrule abundance 60 to 80 % by volume |  |
has matrix abundance 10 to 15 % by volume |  |
has refractory inclusion abundance 0.1 to 1 % by volume |  |
has metal abundance 5 % by volume |  |
has chondrule mean diameter 0.7 millimeters |  |
has total iron content low |  |
has metal iron content 5 to 10 % |  |
has iron metal and iron sulfide 50 % of total iron |  |
type 4 chondrite | has petrologic type 4 |  |
has degree of thermal metamorphism weak |  |
has olivine and low Ca pyroxene homogeneity less than 5 % mean deviations |  |
has structural state of low Ca pyroxene greater than 20 % monoclinic |  |
has chondrule glass type devitrified, absent |  |
has part feldspar secondary, grains than 2 microns |  |
has part maximum bulk Ni in metal greater than 20 % by weight, kamacite and taenite in exsolution relationship |  |
has part sulfide Ni content less than 0.5 % by weight |  |
has part matrix transparent, recrystallized, small crystals |  |
has part chondrule chondrules well defined |  |
has part carbon less than 0.2 % by weight |  |
has part water less than 1.5 % by weight |  |
ordinary chondrite | has abundance most common chondrite observed from falls |  |
thermally altered chondrite | has metamorphism mechanism thermal metamorphism |  |
has alteration temperature range the range over at which the alteration took place |  |
altered chondrite | has degree of secondary processing providing insight into geological evolution of parent asteroid |  |
chondrite | has petrologic type range which depends on degree of aqueous alteration and thermal metamorphism |  |
has relative abundance 85.7 % of meteorite falls |  |
has homogeneity of olivine and low Ca pyroxene definition goes here |  |
has part metal maximum bulk in weight % |  |
has part mean Ni content of sulfides in weight % |  |
stony meteorite | has weather resistance low |  |
has fragmentation probability high because it is more friable than iron meteorite |  |
has ablative mass loss high because it is more friable than iron meteorite |  |
undifferentiated meteorite | has peak temperature less than 950 degree Celsius during its entire history since solidification |  |
has parent body asteroid smaller than 100 km in diameter |  |
has age oldest and most primitive rock in solar system |  |
rock | has part mineral |  |
has texture |  |
has genesis |  |
meteorite | 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 composition often minerals not found on Earth |  |
has impact velocity when it hits the ground which is smaller than its velocity before it enters the atmosphere |  |
has impact angle |  |
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 |  |
can shatter during impact phase |  |
can fragment during meteor phase |  |
conglomerate | has sediment mechanism agglomeration of particles, many of which record individual, diverse histories |  |