| 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 |  |