LAP04840 is an unusual R chondrite that includes abundant hornblende amphibole. LAP04840 shows a texture of equilibrated chondrite composed of 59.3% olivine, 13.5% orthopyroxene, 13.3% hornblende, 6.2% plagioclase, 6.0% Fe-Ni sulfide, and 1.7% accessory minerals. Hornblende replaces olivine and pyroxene in both chondrules and matrices, suggesting its secondary origin. All major phases in LAP04840 are homogeneous: olivine (Fa
37), orthopyroxene (En
70Wo
1), and plagioclase (An
8Or
2). Hornblende is also nearly homogeneous, but the total sum by electron microprobe analysis is 96-98 wt%, suggesting the presence of Fe
3+ and a hydroxyl group. Synchrotron Fe-XANES analysis gives a Fe
3+/ΣFe ratio of ∼ 0.6 and micro-FT-IR analysis confirms the presence of a hydroxyl group. Thus, the structural formula is (Na
0.40K
0.04)(Ca
1.46Mn
0.02Fe
2+0.06Na
0.46)(Al
0.08Fe
2+0.43Fe
3+0.75Cr
0.08Mg
3.60)(Si
7.02Al
0.98)O
22(OH)
2. Single crystal X-ray diffraction of LAP04840 hornblende gives the following lattice constants:
a = 9.7957(9) Å,
b = 18.0788(12) Å,
c = 5.2949(5) Å,
β = 104.747(3)°. The relatively short distances of [M(1)-O = 2.069 Å], [M(2)-O = 2.081 Å], and [M(3)-O = 2.058 Å] suggest the feasible preference of small Fe
3+ at these sites. The mineralogy and petrology of LAP04840 are consistent with its classification as an R6 chondrite. However, the presence of hornblende and biotite is quite unique among not only R chondrites but also asteroidal meteorites in general. The presence of these hydrous minerals suggests metamorphism under high pressure and an aqueous environment probably at depth in the parent body. A thermometer using hornblende and plagioclase equilibria gives
T = 670-690 °C. Further, a barometer using Al content in hornblende gives
P = ∼ 0.1 GPa. Although these estimates bear some uncertainties, it is likely that the size of the R chondrite parent body was large enough to induce such metamorphism.
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