Gibeon | has image
 |  |
has name Gibeon |  |
is an instance of Of octahedrite  |  |
is an instance of type IVA iron meteorite |  |
has find date 1838 |  |
has fall date pre-historic times |  |
has fall location Great Namaqualand, Namibia, Africa  |  |
has fall coordinates Latitude 25 degrees 20 minutes North, Longitude 18 degrees East |  |
has fall map
 |  |
has original mass greater than several tons |  |
have composition 90% iron, 7.93% Ni, 0.41% Co, 0.04% P, 2.0 ppm Ga, 0.12 ppm Ge, 2.3 ppm Ir |  |
has crystal size 0.3 ± 0.5 mm (fine) |  |
Of octahedrite | has structural class Of |  |
type IVA iron meteorite | has composition kamacite, taenite |  |
has formation cooling rate 11 to 500 degrees C per million years |  |
parent body radius 8 to 49 kilometers |  |
has total mass of finds 22254 kg |  |
has number of finds 39 |  |
has nickel content 8.0 % by weight |  |
has gallium content 2.15 microgram/gram |  |
has germanium content 0.124 microgram/gram |  |
has iridium content 1.9 microgram/gram |  |
has carbon content 200 microgram/gram |  |
has phosphor content 0.88 milligram/gram |  |
has sulfur content 0.8 % by weight |  |
has chromium content 140 microgram/gram |  |
has cobalt content 4.0 milligram/gram |  |
has copper content 150 microgram/gram |  |
has molydbenum content 5.9 microgram/gram |  |
has tungsten content 0.6 microgram/gram |  |
has palladium content 4.6 microgram/gram |  |
has gold content 1.5 microgram/gram |  |
has arsenic content 7.6 microgram/gram |  |
has antimony content 9 nanogram/gram |  |
structural iron meteorite | has distinguishing feature crystalline iron-nickel alloy |  |
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 | 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 |  |