Subject |
is an instance of |
has chromite content |
has distinguishing feature |
has olivine grain shape |
has olivine content |
has fall location |
has metal content |
has formation cooling rate |
has name |
has olivine crystal distribution |
parent body radiu |
has weather |
has letter designation |
has relative abundance |
has value |
has total mass of find |
has phosphate content |
has fall coordinate |
has composition |
is a kind of |
has olivine grain size |
has nickel content |
has find date |
has mass |
has image |
has number of find |
has origin |
has definition |
has pyroxene content |
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 | |
pyroxene grouplet pallasite | | 1 % or less by volume | large mm sized pyroxene crystals poikilitically containing small olivine grains | from angular fragments to rounded | 35 to 85 % 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 | | 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 | | |
Vermillion | meteorite find | 0.2 % by volume | large mm sized pyroxene crystals poikilitically containing small olivine grains | rounded to subrounded 1.5 cm | 14 % by volume | grain field in Marshall County, Kansas | higher than that of average solar system material | 2.5 to 4 degrees C per million years | Vermillion | from homogeneous to heterogeneous | 78 to 97 kilometers | can be severe due to long exposure time to environmental corrosion agents | PAL | | lower because the fall was not witnessed | 485755 kg | 1 % or less by volume | 39° 44.18' N., 96° 21.68' W. | often minerals not found on Earth | | 1.5 cm | always greater than 4 % | May, 1991 | 34.36 kg |
 | 1691 | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | | 0.7 % by volume (orthopyroxene) |