Newsletter |
41,2 |
Location |
Miller Range |
Field Number |
23335 |
Dimensions (cm) |
3.1 x 2.7 x 1.6 |
Weight (g) |
21.47 |
Original Classification |
CV3 Chondrite |
Updated Classification |
CV 3.6 Chondrite Reduced |
Pairing |
MIL 07277;
MIL 090646;
MIL 090677;
MIL 15123;
MIL 15148;
MIL 15192;
MIL 15227;
MIL 15229;
MIL 15240;
MIL 15247;
MIL 15254;
MIL 15255;
MIL 15257;
MIL 15264;
MIL 15265;
MIL 15268;
MIL 15363;
MIL 15472;
MIL 15480;
MIL 15511;
MIL 15516;
MIL 15524;
MIL 15555;
MIL 15565;
|
Fayalite (mol%): 1-44;Ferrosilite (mol%): 1 |
B |
A |
Exterior has 60% black fusion crust with brown weathered areas. Oxidation is heavy in areas. The interior is a dark gray to black matrix with some oxidation scattered. Tiny white and weathered specks are visible. |
The sections exhibit large chondrules (up to 3 mm) and CAIs in a dark matrix. Olivines range from Fa0-52, and pyroxenes from Fs1-15. The paired meteorites are moderately weathered, unequilibrated, CV3 carbonaceous chondrites. |
Reclassification and pairing based on Raman spectroscopy (petrologic type 3.6), and on Ni content of metal and sulfide and magnetic susceptibility (Reduced). Details are reported in Righter et al. (2022); doi: 10.1111/maps.13932. |