CM2 Meteorites

carbonaceous group · 416 meteorites

CM2 carbonaceous chondrites are carbon-rich, hydrated meteorites. They contain up to 3% carbon, amino acids, and water-bearing minerals. Important for understanding organic chemistry in the early solar system.

Sort by: Mass Name Year Country
Name Mass
Yamato 981268 6.6 g
LaPaz Icefield 04675 6.6 g
Yamato 981945 6.6 g
Yamato 86700 6.6 g
Yamato 980088 6.5 g
Northwest Africa 6720 6.5 g
Miller Range 090994 6.5 g
Lewis Cliff 85306 6.5 g
Lewis Cliff 86009 6.5 g
Yamato 86699 6.5 g
Miller Range 090283 6.4 g
Scott Glacier 06042 6.4 g
Yamato 981290 6.4 g
Yamato 86697 6.4 g
Allan Hills 84030 6.2 g
Dominion Range 08016 6.2 g
Dhofar 1619 6.2 g
Yamato 86698 6.1 g
Meteorite Hills 00434 6.1 g
Yamato 980070 6.0 g
Elephant Moraine 99437 6.0 g
Meteorite Hills 00810 5.9 g
Elephant Moraine 96018 5.9 g
Miller Range 07701 5.7 g
Yamato 793500 5.7 g
Yamato 8412 5.6 g
Lewis Cliff 86008 5.6 g
Yamato 981632 5.5 g
Yamato 980036 5.5 g
Elephant Moraine 92005 5.4 g
Yamato 980091 5.4 g
Meteorite Hills 00781 5.4 g
Yamato 980399 5.3 g
Elephant Moraine 96011 5.3 g
Miller Range 07692 5.2 g
Allan Hills 84053 5.2 g
Pecora Escarpment 91327 5.2 g
Dominion Range 08009 5.2 g
Allan Hills A78261 5.1 g
Elephant Moraine 96007 5.1 g
Miller Range 07682 5.1 g
Grove Mountains 050179 5.0 g
Northwest Africa 4757 5.0 g
Yamato 82099 4.9 g
Yamato 86694 4.9 g
Queen Alexandra Range 94222 4.8 g
Lewis Cliff 86005 4.7 g
Allan Hills A81004 4.7 g
Yamato 86015 4.6 g
Yamato 74641 4.6 g

Related Classifications