Subject |
is an instance of |
has chromite content |
has distinguishing feature |
has olivine chromium content |
has olivine magnesium content |
has olivine SiO2 content |
has olivine grain shape |
has olivine content |
has fall location |
has olivine manganese content |
has olivine MgO content |
has metal content |
has formation cooling rate |
has name |
has olivine crystal distribution |
parent body radiu |
has olivine composition |
has weather |
has letter designation |
has relative abundance |
has value |
has olivine zinc content |
has olivine nickel content |
has olivine scandium content |
has total mass of find |
has phosphate content |
has fall coordinate |
has olivine CaO content |
has olivine cobalt content |
has composition |
is a kind of |
has olivine grain size |
has olivine MnO content |
has find date |
has nickel content |
has olivine Cr2O3 content |
has mass |
has olivine FeO content |
has image |
has number of find |
has origin |
has definition |
has olivine Fe/Mn ratio |
Eagle Station grouplet pallasite | | 1 % or less by volume | mixture of iron-nickel alloy and non-metallic minerals | | | | from angular fragments to rounded | 75 to 80 % by volume | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | | | higher than that of average solar system material | 2.5 to 4 degrees C per million years | based on the locale, region, or nearby town in which the fall occurred | from homogeneous to heterogeneous | 78 to 97 kilometers | more ferroan than main group pallasite | | PAL | 1.5 % of meteorite falls | | | | | 7207 kg | 1 % or less by volume | in degrees, minutes and seconds of lattitude and longitude | | | metallic iron plus olivine; core/mantle boundary samples | pallasite | typically one centimeter | | | always greater than 4 % | | | | | 33 | planet or asteroid much larger than 100 km in diameter | | |
meteorite find | | | | | | | | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | | | | | based on the locale, region, or nearby town in which the fall occurred | | | | can be severe due to long exposure time to environmental corrosion agents | | | lower because the fall was not witnessed | | | | 485755 kg | | in degrees, minutes and seconds of lattitude and longitude | | | often minerals not found on Earth | meteorite | | | when the meteorite was found | | | | | | 1691 | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | a meteorite whose fall was not witnessed | |
Eagle Station | meteorite find | 1 % or less by volume | mixture of iron-nickel alloy and non-metallic minerals | 404 microgram/gram using Instrumental Neutron Activation Analysis | 79.8 mg# or 100 * Mg/(Mg + Fe) | 38.7 % by weight | from angular fragments to rounded | 75 to 80 % by volume | 0.75 miles from Eagle Station, Carroll County, Kentucky | 1.34 milligram/gram using Instrumental Neutron Activation Analysis | 42.2 % by weight | higher than that of average solar system material | 2.5 to 4 degrees C per million years | Eagle Station | from homogeneous to heterogeneous | 78 to 97 kilometers | more ferroan than main group pallasite | can be severe due to long exposure time to environmental corrosion agents | PAL | | lower because the fall was not witnessed | 2.4 microgram/gram using Instrumental Neutron Activation Analysis | 45.1 microgram/gram using Instrumental Neutron Activation Analysis | 2.66 microgram/gram using Instrumental Neutron Activation Analysis | 485755 kg | 1 % or less by volume | 38° 37' N., 84° 58' W. | 0.070 % by weight | 26.0 microgram/gram using Instrumental Neutron Activation Analysis | often minerals not found on Earth | | typically one centimeter | 0.18 % by weight | 1880 | always greater than 4 % | 0.031 % by weight | 36.3 kg | 19.0 % by weight |
 | 1691 | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | | 104 |