| Vermillion | has image
 |  |
| is an instance of pyroxene grouplet pallasite |  |
| is an instance of meteorite find |  |
| has name Vermillion |  |
| has find date May, 1991 |  |
| has fall coordinates 39° 44.18' N., 96° 21.68' W. |  |
| has fall location grain field in Marshall County, Kansas |  |
| has mass 34.36 kg |  |
| has olivine content 14 % by volume |  |
| has olivine grain shape rounded to subrounded 1.5 cm |  |
| has olivine grain size 1.5 cm |  |
| has pyroxene content 0.7 % by volume (orthopyroxene) |  |
| has chromite content 0.2 % by volume |  |
| pyroxene grouplet pallasite | has distinguishing feature large mm sized pyroxene crystals poikilitically containing small olivine grains |  |
| meteorite find | has value lower because the fall was not witnessed |  |
| has weathering can be severe due to long exposure time to environmental corrosion agents |  |
| pallasite | has composition metallic iron plus olivine; core/mantle boundary samples |  |
| has letter designation PAL |  |
| has phosphate content 1 % or less by volume |  |
| has olivine crystal distribution from homogeneous to heterogeneous |  |
| has formation cooling rate 2.5 to 4 degrees C per million years |  |
| parent body radius 78 to 97 kilometers |  |
| has total mass of finds 7207 kg |  |
| has number of finds 33 |  |
| 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 original mass which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site |  |
| has composition often minerals not found on Earth |  |
| has relative abundance |  |
| has total mass of finds 485755 kg |  |
| has number of finds 1691 |  |
| has impact velocity when it hits the ground which is smaller than its velocity before it enters the atmosphere |  |
| has impact angle |  |
| has weather resistance which depends on its composition |  |
| 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 |  |
| has origin meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal |  |
| 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 |  |
| has ablative mass loss depending on composition, more friable stony meteoroids loses more mass than iron meteoroid |  |
| has ablative mass loss directly proportional to initial velocity |  |
| can shatter during impact phase |  |
| can fragment during meteor phase |  |
| has fragmentation probability during meteor phase which depends on composition |  |
| rock | has part mineral |  |
| has texture |  |
| has genesis |  |
| metal-rich meteorite | has metal content higher than that of average solar system material |  |
| has nickel content always greater than 4 % |  |
| igneous rock | has solidification mechanism |  |
| has solidification timescale |  |