| 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 |  |