Odessa | has image
 |  |
has name Odessa |  |
is an instance of Og octahedrite  |  |
is an instance of type I iron meteorite |  |
has fall date Late Pleistocene about 50,000 years ago |  |
has find date 1920 |  |
has fall location Odessa, Texas, U.S.A  |  |
has fall coordinates Latitude 31 degrees 45 minutes 21 seconds North, Longitude 102 degrees 28 minutes 43 seconds West |  |
have composition 7.35% Ni, 0.48% Co, 0.25% P, 0.5% S, 0.2% C, 75 ppm Ga, 285 ppm Ge, 2 ppm Ir |  |
has crystal size 1.7 ±0.25 mm (coarse) |  |
Og octahedrite | has structural class Og |  |
type I iron meteorite | has composition kamacite, taenite, silicates, carbides |  |
has structural classe Om-Og octahedrite |  |
has total mass of finds 94688 kg |  |
has number of finds 69 |  |
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 |  |
structural iron meteorite | has distinguishing feature crystalline iron-nickel alloy |  |
metal-rich meteorite | has metal content higher than that of average solar system material |  |
has nickel content always greater than 4 % |  |
differentiated meteorite | has origin planet or asteroid much larger than 100 km in diameter |  |
meteorite | 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 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 |  |