Table 3. Summary of carbonaceous chondrite characteristics. Bold type denotes critical criterion.
| Parameters | CI | CM | CO | CV | CK | CR | CH | C41 |
| Matrix Color2 | black | dark | med. gray | med. gray | light gray | light gray | light gray | light gray |
| Chondrule abundance (vol. %) | absent | 10-40 | 60-70 | 40-65 | 15 | 50-60 | 5-10 | 65 |
| Chondrule average size (mm) | - | < 0.5 | < 1.0 | > 0.7 | 0.7 | 0.4 | 0.05 | 0.6 |
| Coarse-grained chondrule rims | - | rare | rare | common | rare | common | none | rare |
| Ca-Al Inclusions (vol. %) | none | 5 | 8-15 | 7-20 | 4 | <1 | <1 | 1 |
|
Dominant matrix silicate |
clays3 |
clays3 |
olivine ~ 60% |
olivine ~ 60% |
olivine ~80% |
some clays |
pyroxene ~70 % |
olivine ~60% |
| Dominant martrix opaque4 | mag | mag > prh | mt with <1.0% Cr |
R = prh O = mag |
Cr-mag | mag ≥ prh | mt | tr |
| Ni-Fe metal (vol. %) | none | trace | 1-6 | 0-5 | none | 6 | 20-25 | 2 |
| Olivine composition (FeO & mol. %) |
- |
variable |
variable5 |
high (Fa 0-50) |
med/high (Fa 28-33) |
very low (Fa 3) |
low (Fa <10) |
low (Fa 10-14) |
| Pyroxene composition (FeO & mol. %) |
- |
variable |
variable |
variable |
med/high (Fs 22-29) |
very low (Fs 4) |
low (Fs <10) |
low |
| Opague darkening | no | no | no | no | yes | no | no | no |
| wt % Carbon | ~3.8 | ~2.5 | ~0.3 | <0.10 | <0.10 | <0.10 |
1 C4 is an old classification notation, given here for
convenience. The new scheme is "Coolidge grouplet."
2 Assuming low levels of terrestrial oxidation that colors the
rock interior light to red brown.
Dark to gray shades are consistent with total carbon content.
3 Clay is short lay-term for phyllosilicates.
4 mag
= magnetite; Cr-mag 1.5 to 14 wt. % Cr; prh = pyrrhotite; pt = pentlandite; tr =
troilite; mt = Ni-Fe metal.
R = reduced subgroup; O = oxidized subgroup.
5
Dependent on degree of equilibration (subtype), examples: CO3.0, Fa = 0-100;
CO3.4 = 48-60; CO3.6,
Fa = 36-46.
This chart courtesy of the
Northern Arizona University
It has been modified to meet ARN needs .
Notes from Phil Duton
[Carbonaceous chondrites; show alteration
due to aqueous action completely unlike the alteration seen in ordinary
chondrites. They are graded from "3" that indicates little alteration to "1"
that indicates the chondrules have been obliterated due to metamorphic
alteration. These primitive meteorites are rare with classifications named for
the specimen that originally had the type.
Thus, "CI" meteorites
are named for the Ivuna stone, which fell in Tanzania in 1938. It is a "CI 1"
stone with 3-5% carbon, 20% water in silicates, and magnetite. There are also
some amino acids present. The grade "1" indicates the chondrules have been
obliterated by the action of the water.
The type "CM" group is named for the Mighei stone
that fell in the Ukraine in 1889. It is a "CM 2" class stone with 0.6 to 2.9%
carbon and 13% water, visible chondrules and some amino acids.
The type "CO" group is named for the Ornans stone
that fell in Doubs, France in 1868. It is a class "CO 3.4" specimen with 0.2 to
1% carbon and 1% water. Chondrules, while present, are small.
The type "CV" group is named for the Vigarano stone
that fell in Italy in 1910. It is a class "CV 3.3" stone with less than 0.2%
carbon and less than 0.03% water. Chondrules are present. The Allende meteorite
that fell in Mexico is one of this type. It also contains mysterious "CAI"
inclusions, which are calcium, aluminum minerals not found on earth. These
white, irregular shaped inclusions do not derive from the same process as the
chondrules. Their origin is subject of current speculation.
Three recent additions have been added as new, rare, stones have been found.
These are "CK" from Karoonda, Australia that appear
to be similar to "CO" and "CV" meteorites.
"CR" for a stone from Renazzo, Italy formerly
classified as a "CM" but shown to have visible metal.
"CH" which is similar to "CR" but with a very high
metallic iron content.
NOTE: The carbonaceous meteorites are generally observed falls. This is because
they are extremely fragile in our earth's environment and rapidly weather beyond
recognition. Prompt recovery is essential to identification of these stony
meteorites.
O/I
