DaG 609 | has image
 |  |
is an instance of Dar al Gani meteorite |  |
is an instance of S3 shock stage meteorite |  |
is an instance of eucrite |  |
has comment iron-rich, monomict, with chromite grains |  |
has mass 0.696 kg |  |
has find date 1998 |  |
has weathering stage W2 |  |
has pyroxene composition Fs% 27-63 |  |
classified by A. Sexton, Open University, UK. A. Sexton, Meteoritical Bulletin No 83  |  |
has number of fragments 2 |  |
has image
 |  |
has fall coordinates 26° 53.13' N. 16° 34.81' E.  |  |
Dar al Gani meteorite | has fall location Dar al Gani plateau, Libyan Sahara Desert |  |
has acronym DaG |  |
S3 shock stage meteorite | has shock stage S3 |  |
has shock pressure 15 to 20 GPa |  |
has degree of shock metamorphism weakly shocked |  |
eucrite | has letter designation AUEC |  |
has characteristic mineral anorthite-pigeonite Ca-rich |  |
has total mass of finds 231 kg |  |
has number of finds 23 |  |
shocked meteorite | has metamorphism mechanism shock metamorphism |  |
HED meteorite | is an acronym for Howardite, Eucrite, Diogenite |  |
has origin 4 Vesta |  |
has minerology orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica |  |
has petrology coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated |  |
has likely origin cumulates, crystallized melts, impact mixing |  |
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 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 |  |
has name based on the locale, region, or nearby town in which the fall occurred |  |
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 |  |
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 |  |
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 |  |
volcanic rock | has solidification mechanism extrusion onto the surface of the planet or asteroid via a volcanic eruption |  |
has solidification timescale very rapid |  |
rock | has part mineral |  |
has texture |  |
has genesis |  |
achondrite | has distinguishing feature no chondrules |  |