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
Elephant Moraine 96226 2.1 g
Miller Range 090700 2.0 g
LaPaz Icefield 04527 2.0 g
MacKay Glacier 05242 2.0 g
Yamato 794082 1.9 g
Miller Range 07672 1.8 g
Queen Alexandra Range 97958 1.8 g
Miller Range 05086 1.7 g
Queen Alexandra Range 99342 1.7 g
Lewis Cliff 85307 1.7 g
Larkman Nunatak 04319 1.7 g
Lewis Cliff 88003 1.7 g
Yamato 86703 1.7 g
Yamato 75003 1.6 g
Yamato 86716 1.6 g
Lewis Cliff 86007 1.6 g
Meteorite Hills 001087 1.6 g
Elephant Moraine 92008 1.5 g
Elephant Moraine 92103 1.5 g
Allan Hills 84046 1.5 g
Yamato 86704 1.5 g
Yamato 794019 1.5 g
Grove Mountains 021536 1.5 g
Lewis Cliff 87008 1.4 g
Lewis Cliff 87167 1.4 g
Queen Alexandra Range 99752 1.4 g
Elephant Moraine 96005 1.4 g
Yamato 980071 1.4 g
Allan Hills 84041 1.3 g
Queen Alexandra Range 93018 1.3 g
Graves Nunataks 06158 1.3 g
MacKay Glacier 05245 1.3 g
Roberts Massif 04309 1.3 g
Yamato 81010 1.3 g
MacAlpine Hills 02658 1.3 g
Yamato 980092 1.2 g
Elephant Moraine 90986 1.2 g
Lewis Cliff 87028 1.2 g
LaPaz Icefield 04760 1.1 g
Elephant Moraine 92010 1.0 g
Allan Hills 82131 1.0 g
Yamato 86687 1.0 g
Yamato 980090 1.0 g
Lewis Cliff 87025 0.9 g
Miller Range 05119 0.9 g
Lewis Cliff 87271 0.9 g
Yamato 980098 0.9 g
Lewis Cliff 87027 0.8 g
Grove Mountains 050384 0.8 g
MacKay Glacier 92502 0.7 g

Related Classifications