کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
1781318 1523952 2013 10 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
New evidence of meteoritic origin of the Tunguska cosmic body
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات فیزیک زمین (ژئو فیزیک)
پیش نمایش صفحه اول مقاله
New evidence of meteoritic origin of the Tunguska cosmic body
چکیده انگلیسی


• Diamond–lonsdaleite–graphite samples from peats of the Tunguska event were studied.
• Troilite, taenite, γ-Fe and schreibersite are established in the samples.
• The whole mineral association suggests that the samples are meteoritic remnants.
• Fe:Ni=22:1 ratio in the samples also indicates the meteoritic origin.
• We conclude that the microsamples are the remnants of the Tunguska meteoritic body.

Diamond–lonsdaleite–graphite micro-samples collected from peat after the 1908 catastrophic blast in the Tunguska area were studied with scanning (SEM) and transmission electron (TEM) microscopy, NanoSecondary Ion Mass Spectrometry (NanoSIMS) and Х-ray synchrotron technique. The high-pressure carbon allotropes in the Tunguska samples are being described for the first time and contain inclusions of FeS (troilite), Fe–Ni (taenite), γ-Fe and (FeNi)3P (schreibersite). The samples are nodule-like in shape and consist of 99.5% carbon minerals, e.g. diamond>lonsdaleite>graphite. Micro- and nanoinclusions of troilite (up to 0.5 vol%), taenite, γ-iron and schreibersite fill cracks, cleavages and pores in the carbon matrix. Carbon isotope studies from the two analyses of the Tunguska foil showed δ13C=−16.0±1.9‰ and δ13C=−15.2±2.1‰, suggesting δ13C=−15.6±2‰ as an average characteristic of the carbon reservoir. That value is close to δ13C of some extraterrestrial samples. A negligible concentration of Ir and Os in the carbonaceous matrix promotes some controversial interpretation of the origin of the studied materials. Attributing this fact to the primary inhomogeneity, and considering the micro-structural features such as cracks, deformation of the crystal lattices, etc. coupled with high-pressure carbon allotropes association with metals, sulfides and phosphides, and the high ratio of Fe:Ni=22:1 suggest that the studied samples are meteorite micro-remnants.

Figures a, b, c, d. SEM images of the Tunguska diamond–lonsdaleite–graphite micro-samples: a,b—the general form of the samples, c—lamellar structure of the sample, d—inclusion of troilite crystal in carbon matrix, indicated by arrow.Figure optionsDownload high-quality image (219 K)Download as PowerPoint slide

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Planetary and Space Science - Volume 84, August 2013, Pages 131–140
نویسندگان
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