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- Q2964430 abstract "The LL chondrites are a group of stony meteorites, the least abundant group of the ordinary chondrites, accounting for about 10–11% of observed ordinary-chondrite falls and 8–9% of all meteorite falls (see meteorite fall statistics). The ordinary chondrites are thought to have originated from three parent asteroids, with the fragments making up the H chondrite, L chondrite and LL chondrite groups respectively. The Chelyabinsk meteor is a LL chondrite meteor.".
- Q2964430 thumbnail Ragland_meteorite.jpg?width=300.
- Q2964430 wikiPageWikiLink Q107172.
- Q2964430 wikiPageWikiLink Q1195475.
- Q2964430 wikiPageWikiLink Q170258.
- Q2964430 wikiPageWikiLink Q177811.
- Q2964430 wikiPageWikiLink Q182120.
- Q2964430 wikiPageWikiLink Q191250.
- Q2964430 wikiPageWikiLink Q192880.
- Q2964430 wikiPageWikiLink Q22693.
- Q2964430 wikiPageWikiLink Q2964429.
- Q2964430 wikiPageWikiLink Q2964436.
- Q2964430 wikiPageWikiLink Q340587.
- Q2964430 wikiPageWikiLink Q411130.
- Q2964430 wikiPageWikiLink Q425316.
- Q2964430 wikiPageWikiLink Q429991.
- Q2964430 wikiPageWikiLink Q4661508.
- Q2964430 wikiPageWikiLink Q4748437.
- Q2964430 wikiPageWikiLink Q48361.
- Q2964430 wikiPageWikiLink Q5571836.
- Q2964430 wikiPageWikiLink Q60186.
- Q2964430 wikiPageWikiLink Q677.
- Q2964430 wikiPageWikiLink Q6823454.
- Q2964430 wikiPageWikiLink Q721849.
- Q2964430 wikiPageWikiLink Q78843.
- Q2964430 wikiPageWikiLink Q903965.
- Q2964430 comment "The LL chondrites are a group of stony meteorites, the least abundant group of the ordinary chondrites, accounting for about 10–11% of observed ordinary-chondrite falls and 8–9% of all meteorite falls (see meteorite fall statistics). The ordinary chondrites are thought to have originated from three parent asteroids, with the fragments making up the H chondrite, L chondrite and LL chondrite groups respectively. The Chelyabinsk meteor is a LL chondrite meteor.".
- Q2964430 label "LL chondrite".
- Q2964430 depiction Ragland_meteorite.jpg.