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
Meteorite Hills 01071 4.5 g
Yamato 86701 4.5 g
Allan Hills 84047 4.4 g
LaPaz Icefield 031022 4.2 g
Miller Range 07674 4.2 g
Pecora Escarpment 91203 4.2 g
Yamato 980095 4.1 g
Allan Hills 83016 4.1 g
Miller Range 07497 4.1 g
Lewis Cliff 87001 4.0 g
Allan Hills 85012 3.9 g
Yamato 981946 3.7 g
Yamato 794079 3.7 g
Yamato 980087 3.7 g
Grove Mountains 020025 3.6 g
MacAlpine Hills 02755 3.5 g
Queen Alexandra Range 97657 3.5 g
Queen Alexandra Range 93004 3.5 g
Yamato 981975 3.5 g
Yamato 793530 3.3 g
Yamato 82090 3.3 g
Yamato 8452 3.3 g
Allan Hills 84035 3.2 g
Yamato 86702 3.2 g
Allan Hills 84050 3.2 g
Allan Hills 85010 3.2 g
Lewis Cliff 87249 3.1 g
Yamato 86736 3.1 g
Yamato 982070 3.0 g
Miller Range 07668 3.0 g
Queen Alexandra Range 97621 2.8 g
Allan Hills 84036 2.8 g
Miller Range 05112 2.8 g
Pecora Escarpment 91147 2.8 g
Allan Hills 85106 2.7 g
Queen Alexandra Range 93006 2.7 g
Pecora Escarpment 02011 2.6 g
Miller Range 05124 2.6 g
Queen Alexandra Range 94220 2.6 g
Yamato 980097 2.5 g
Yamato 8403 2.5 g
Miller Range 07680 2.5 g
Queen Alexandra Range 97676 2.4 g
Meteorite Hills 00435 2.4 g
Elephant Moraine 96014 2.3 g
Meteorite Hills 00635 2.3 g
Grove Mountains 020017 2.2 g
Elephant Moraine 96013 2.1 g
Lewis Cliff 87003 2.1 g
Lewis Cliff 86004 2.1 g

Related Classifications