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| Sample No.: | LAP 04757; LAP 04773 |
| Location: | LaPaz Ice Field |
| Field No.: | 17603; 17035 |
| Dimensions (cm): | 2.5x2.0x1.0; 2.25x1.25x1.5 |
| Weight (g): | 12.8; 8.298 |
| Meteorite Type: | Chondrite Ungrouped |
Macroscopic Description: Kathleen McBride
Exteriors of these meteorites have dull brown/black fusion crust with oxidation haloes. The interiors reveal a rusty brown/black matrix with high metal content.
Thin Section (,2) Description: Tim McCoy and Valerie Reynolds
These meteorites are so similar that a single description suffices. The sections consist of abundant chondrules set in a metal- and sulfide-bearing, weathered matrix. Shock effects are present, including metal-sulfide melting at grain boundaries. Olivine is homogeneous at Fa13 and pyroxene exhibits a small range at Fs13-16.
Links to the acapulcoites or low-FeO chondrites (Russell et al., 1998, MAPS 33, 853-856) should be considered, although LAP 04773/04757 are less metamorphosed than the former and more magnesian than is typical for the latter.
Oxygen Isotope Analysis: D. Rumble
Analysis for two subsamples of LAP 04757 give: A) δ18O = +3.67, δ17O = +2.68, and Δ17O = 0.746; B) δ18O = +3.75, δ17O = +2.94, and Δ17O = 0.97. These values plot above the terrestrial fractionation line, suggesting an unusual low FeO ordinary chondrite such as Burnwell.
| Cross-Polarized Light LAP 04757 |
Plane-Polarized Light LAP 04757 |
Reflected Light LAP 04757 |
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| Cross-Polarized Light LAP 04773 |
Plane-Polarized Light LAP 04773 |
Reflected Light LAP 04773 |
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