Coordinated Stem and Nanosims Analysis of Enstatite Whiskers in Interplanetary Dust
نویسندگان
چکیده
Introduction: Enstatite whiskers (<10 µm length, <200 nm width) occur in chondritic-porous interplanetary dust particles (CP IDPs) [1], an Antarctic micrometeorite [2] and a comet 81P/Wild-2 sample [3]. The whiskers are typically elongated along the [100] axis and contain axial screw dislocations, while those in terrestrial rocks and meteorites are elongated along [001]. The unique crystal morphologies and microstructures are consistent with the enstatite whiskers condensing above ~1300 K in a low-pressure nebular or circumstellar gas [1]. To constrain the site of enstatite whisker formation, we carried out coordinated mineralogical, chemical and oxygen isotope measurements on enstatite whiskers in a CP IDP. Sample and Methods: The IDP sample, L2055N1 (8 µm in size) from cluster #7 of comet 26P/Grigg-Skjellerup dust stream collection was embedded in epoxy and 70 nm thick sections were obtained. Following the mineralogical and chemical identifications using a JEOL 2500SE field-emission scanning TEM (FE-STEM), the sample was analyzed for O isotopic compositions by isotopic imaging with the JSC NanoSIMS 50L ion microprobe. Results: L2055N1 is a typical anhydrous IDP dominated by very porous fine grained aggregates. No well-developed magnet-ite rims on mineral grains were observed, suggesting little heating during atmospheric entry. L2055N1 contains abundant GEMS (glass with embedded metal and sulfides) grains, and 20 – 200 nm sized enstatite and sulfide grains bound together by carbona-ceous material. An enstatite whisker occurs in two thin sections. In one section the whisker is 1.4 µm long and 0.1 µm wide and in the adjacent section it is 0.5 µm long. Both fragments are composed of En100 and display a fine-scale intergrowth of clino-and ortho-enstatite with stacking disorder along [100]. O isotopic images revealed that enstatite whiskers have δ 17 O =-75±101 ‰, δ 18 O =-117±37 ‰ (1σ), whereas the bulk IDP is very near the terrestrial value: δ
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