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Avanesov G Zhukov B Ziman YA Kostenko V Kuzmin A Murav'ev V Fedotov V Bonev B Mishev D Petkov D Krumov A Simeonov S Boycheva V Uzunov YU Weide GG Halmann D Pössel W Head J Murchie S Schkuratov YuG Berghänel R Danz M Mangoldt T Pihan U Smith B 《Planetary and Space Science》1991,39(1-2):281-295
From February to March 1989 the Phobos 2 spacecraft took 37 TV images of Phobos at a distance of 190-1100 km. These images complement Mariner-9 and Viking data by providing higher-resolution coverage of a large region West of the crater Stickney (40-160 degrees W) and by providing disk-resolved measurements of surface brightness at a greater range of wavelengths and additional phase angles. These images have supported updated mapping and characterization of large craters and grooves, and have provided additional observations of craters' and grooves' bright rims. Variations in surface visible/near-infrared color ratio of almost a factor of 2 have been recognized; these variations appear to be associated with the ejecta of specific large impact craters. Updated determinations of satellite mass and volume allow calculation of a more accurate value of bulk density, 1.90 +/- 0.1 g cm-3. This is significantly lower than the density of meteoritic analogs to Phobos' surface, suggesting a porous interior perhaps containing interstitial ice. 相似文献
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V. I. Vinogradov M. I. Bujakaite V. I. Murav'ev M. B. Burzin A. F. Veis 《Lithology and Mineral Resources》2002,37(5):454-461
The Rb–Sr characteristics of whole-rock samples of Upper Vendian clayey rocks recovered by Gavrilov-Yam boreholes are studied. The Rb–Sr age versus sampling depth relationship has been revealed. Three sample assemblages are identified. The errorchron relationship of samples in the first interval (1760–2400 m) fits the age of 390 ± 40 Ma corresponding to the initial Hercynian history characterized by the transformation of platformal sediments. The other two assemblages (2410–2525 and 2528–2560 m) make up isochrons with slopes corresponding to 590 ± 50 and 690 ± 10 Ma, respectively. Their geochronological meaning is unclear. 相似文献
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Vinogradov V. I. Murav'ev V. I. Bujakaite M. I. Golovin D. I. Gorozhanin V. M. Veis A. F. 《Lithology and Mineral Resources》2000,35(6):571-582
The Rb–Sr and K–Ar characteristics of whole-rock argillite samples from the Middle Riphean Yurmatinian Group have been studied. The timing of final rock alteration was estimated at 525 ± 30 Ma by the Rb–Sr geochronometer. In the section near the Bol'shoi Avzhyan Settlement, the rocks experienced alteration up to the stage of deep epigenesis. The K–Ar data indicate that rock alterations continued after the Rb–Sr system conservation and was accompanied by a gradual gain of K. The great temporal gap between alterations of Middle and Lower Riphean rocks was established in the southern Urals. This gap may be explained either by the affiliation of sampled rocks to different tectonic units or by principal errors in stratigraphic correlations. 相似文献
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Egorov V. A. Vinogradov V. I. Kolesnikov E. M. Murav'ev V. I. Bujakaite M. I. 《Lithology and Mineral Resources》2003,38(5):394-402
Riphean carbonate rocks of the Baikit Anteclise with hydrocarbon raw material reserves exhibit a complicated block structure. Therefore, correlation of sections of even adjacent wells and general understanding of the geological structure of the territory are extremely hampered. The problem becomes more complicated because of multiple epigenetic reworking of Riphean rocks. Study of Rb–Sr and K–Ar systems based on materials from three boreholes drilled on the Baikit Anteclise reveal at least three stages of such reworking dated at about 1400, 1000, and 700 Ma, respectively. Rocks of the whole penetrated pre-Vendian section are assumed to be Early Riphean or even pre-Riphean. Brines saturating them are likely to be related to Vendian–Cambrian saliferous rocks. 相似文献
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