Chinga | has image
 |  |
has name Chinga |  |
is an instance of ataxite  |  |
is an instance of type IVB iron meteorite |  |
has find date 1913 |  |
has fall location Tanna Tuva, Tuvinskaya, Russia |  |
has fall coordinates Latitude 51 degrees 3 minutes 30 seconds North, Longitude 94 degrees 0 degrees 24 seconds East |  |
has original mass greater than 80 kg |  |
have composition 16.38% Ni, 0.181 ppm Ga, 0.082 ppm Ge, 3.6 ppm Ir |  |
ataxite | has structural class D |  |
type IVB iron meteorite | has composition kamacite, taenite |  |
has formation cooling rate 30 to 260 degrees C per million years |  |
parent body radius 11 to 30 kilometers |  |
has total mass of finds 60487 kg |  |
has number of finds 11 |  |
has nickel content 7.1 % by weight |  |
has gallium content 0.221 microgram/gram |  |
has germanium content 0.0526 microgram/gram |  |
has iridium content 22 microgram/gram |  |
has carbon content 40 microgram/gram |  |
has phosphor content 1 milligram/gram |  |
has sulfur content 0.03 % by weight |  |
has chromium content 87.7 microgram/gram |  |
has cobalt content 7.4 milligram/gram |  |
has copper content 12 microgram/gram |  |
has molydbenum content 27 microgram/gram |  |
has tungsten content 3 microgram/gram |  |
has palladium content 12 microgram/gram |  |
has gold content 0.15 microgram/gram |  |
has arsenic content 1.1 microgram/gram |  |
has antimony content 1.5 nanogram/gram |  |
structural iron meteorite | has distinguishing feature crystalline iron-nickel alloy |  |
has crystal size also called Widmanstatten bandwidth |  |
iron meteorite | has relative abundance 5.7 % of meteorite falls |  |
has weather resistance high |  |
has fragmentation probability low because it is tougher than stony meteorite |  |
has ablative mass loss low because it has higher tensile strength than stony meteorite |  |
metal-rich meteorite | has metal content higher than that of average solar system material |  |
differentiated meteorite | has origin planet or asteroid much larger than 100 km in diameter |  |
meteorite | has fall date recorded by eyewitness or inferred from dating methods |  |
has fall map which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity |  |
can have crater image |  |
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 |  |
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 |  |
igneous rock | has solidification mechanism |  |
has solidification timescale |  |
rock | has part mineral |  |
has texture |  |
has genesis |  |