Comet 81P/Wild 2 dust impactors of Stardust turnip-like tracks analogous to cluster IDPs

被引:3
|
作者
Zhang, Mingming [1 ]
Chaumard, Noel [1 ,5 ]
Defouilloy, Celine [1 ,6 ]
Nachlas, William O. [2 ]
Brownlee, Donald E. [3 ]
Joswiak, David J. [3 ]
Westphal, Andrew J. [4 ]
Gainsforth, Zack [4 ]
Kitajima, Kouki [1 ]
Kita, Noriko T. [1 ]
机构
[1] Univ Wisconsin Madison, Dept Geosci, WiscSIMS, Madison, WI 53706 USA
[2] Univ Wisconsin Madison, Dept Geosci, Eugene Cameron Electron Microprobe Lab, Madison, WI 53706 USA
[3] Univ Washington, Dept Astron, Seattle, WA 98195 USA
[4] Univ Calif v, Space Sci Lab, Berkeley, CA 94720 USA
[5] Fi Grp, Direct Sci, 14 Terrasse Bellini, F-92800 Puteaux La Defense, France
[6] Cameca SA, 29 Quai Gresillons, F-92622 Gennevilliers, France
关键词
Silicate fragments; comet Wild 2; Inner solar system materials; CR chondrite chondrules; Aerogel tracks; OXYGEN-ISOTOPE SYSTEMATICS; FINE-GRAINED MATERIAL; INTERPLANETARY DUST; SOLAR-SYSTEM; CHONDRULE FORMATION; CRYSTALLINE SILICATES; II CHONDRULES; PARTICLES; CONSTRAINTS; FRAGMENTS;
D O I
10.1016/j.gca.2024.02.013
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
We measured oxygen isotope ratios of 16 silicate fragments from seven aerogel tracks (turnip -like type B tracks 77, 149, 172, 191, and 220; carrot -like type A tracks 22 and 175) of the comet 81P/Wild 2 collector from NASA's Stardust mission using secondary ion mass spectrometry. Thirteen were prepared by ultramicrotomy; three from track 220 were prepared by sputtering resin blocks using a SIMS Kohler beam, a new procedure aiming to mine as many cometary particles encased in aerogel/resin as possible. Combining new and literature results, we recognized that most silicate fragments of individual type B tracks have diverse mineralogy but consistent massindependent fractionation of oxygen isotopes ( Delta 17 O = delta 17 O - 0.52 x delta 18 O). These observations suggest that their impactors are loosely bound aggregates of unequilibrated materials originating mainly from similar protoplanetary disk regions, resembling the cluster IDP U2-20-GCA. Furthermore, silicate fragments from type A track 22 have almost identical mineralogy and Delta 17 O values, confirming that its impactor is a single chondrule-like fragment. The terminal particle of type A track 175 is pure forsterite with Delta 17 O of - -23 %o. Six iron -rich fragments of this study have positive oxygen isotope ratios ( Delta 17 O- +2 %o) and ordinary chondrite chondrule-like olivine compositions. Together with five similar fragments in the literature, a unique population (Mg# <= 86) of Wild 2 fragments that resemble chondrules from the inner solar system (O -E -R) chondrites or the outer solar system CH -CB chondrites was identified. The remaining 16 O -poor Wild 2 fragments are Mg# >= 79 silicates with Delta 17 O - -2 %o and a small amount of Mg# <= 79 silicates with Delta 17 O - 0 %o, which are most consistent with CR chondrite chondrules. Thus, we conclude that in addition to the possible major source of CR chondrite chondrule-like materials, the inner solar system or CH -CB chondrule-like materials are a minor component of comet Wild 2, like the cluster IDP U2-20-GCA.
引用
收藏
页码:214 / 227
页数:14
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