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Copyright of Canadian Journal of Earth Sciences is the property of Canadian Science Publishing and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)

Copyright of Canadian Journal of Earth Sciences is the property of Canadian Science Publishing and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)

Copyright of Canadian Journal of Earth Sciences is the property of Canadian Science Publishing and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)

Copyright of Canadian Journal of Earth Sciences is the property of Canadian Science Publishing and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)

Copyright of Canadian Journal of Earth Sciences is the property of Canadian Science Publishing and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)

Copyright of Canadian Journal of Earth Sciences is the property of Canadian Science Publishing and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)

Two newly discovered kimberlites from the Wawa area, Ontario, are Group-1 kimberlites in their petrographic, mineralogical, geochemical, and isotopic features. They contain mantle minerals and xenoliths of the Fe–Ti-association (magnesian ilmenite, iron-rich olivine, orange Ti-pyrope garnet, augite, and ferroan enstatite) and of the Cr-association (chromian spinel, forsteritic olivine, purple Cr-pyrope garnets, chromian diopside, and enstatite); minerals of Fe–Ti-association are much more abundant. Minerals of eclogitic association are absent. Both G-10 pyrope garnets and high Cr spinels typically associated with diamond are represented in the Cr-association. The average age of the kimberlites is 1097 ± 7 Ma; i.e., contemporaneous with other alkaline igneous rocks in the Wawa area. Equilibration pressures and temperatures of mantle xenoliths plot close to a 40–45 mW m[sup –2] geotherm. On the basis of the Ni-in-garnet geothermometer, garnets from the Wawa kimberlites equilibrated at 800–1350°C, and at least in part within the diamond stability field. It is likely that kimberlitic magma was derived from light rare earth-element-enriched asthenospheric mantle.Deux kimberlites découvertes récemment dans la région de Wawa, en Ontario, sont des kimberlites de Groupe 1 selon leurs caractéristiques pétrographiques, minéralogiques, géochimiques et isotopiques. Elles contiennent des minéraux du manteau et des xénolites d'association Fe–Ti (ilménite magnésienne, olivine riche en fer, grenat pyrope-Ti orange, augite et bronzite) et d'association Cr (diopside chromifère, olivine à fostérite, grenats pyrope-Cr pourprés, diopside chromifère et enstatite); les minéraux de l'association Fe–Ti sont beaucoup plus abondants. Il y a absence de minéraux d'association éclogite. Les grenats pyropes G-10 et les spinelles à haute teneur en Cr, typiquement associés au diamant, sont représentés dans l'association Cr. L'âge moyen des kimberlites et de 1097±7Ma, c.-à-d. elles sont contemporaines des autres roches ignées alcalines de la région de Wawa. Les pressions et les températures d'équilibre des xénolites du manteau se positionnent près du géotherme 40-45 mWm[sup –2] . En se basant sur le géothermomètre « Ni dans le grenat », les grenats provenant des kimberlites de Wawa auraient trouvé leur équilibre entre 800 et 1350 ºC et au moins en partie dans le champ de stabilité du diamant. Il est probable que le magma kimberlitique provenait du manteau asthénosphérique enrichi en éléments de terres rares légers.[Traduit par la Rédaction] [ABSTRACT FROM AUTHOR]

Numerous vertical to subvertical, cylindrical shafts occur in the rugged exposures of the Middle Silurian Amabel Formation bedrock along the Eramosa River, approximately 10 km northeast of Guelph. These shafts vary from < 1 m to 10 m in diameter, with depths as great as 12 m. They can occur as isolated depressions but more commonly are clustered closely together, and many coalesce to form sinuous bedrock walls. These depressions may contain soil, fine sediment, rubble from the surrounding dolomite bedrock, and rounded clasts of Precambrian basement lithologies. Till is conspicuously absent. These shafts occur in close proximity to cavernous pores that were formed during pre-Wisconsinan to Early Wisconsinan time, suggesting a possible karstic origin. The cylindrical shafts, however, with their greater midpoint diameters, sculpted interiors, and inclined axes, and their lack of vertical flutes and till, are more likely to have originated from glaciofluvial discharge at the end of the Late Wisconsinan. The development of these shafts may have been assisted by cavitation, which enhanced the erosional capacity of sediment-laden meltwaters.Plusieurs puits cylindriques, verticaux à sub-verticaux, se retrouvent dans les affleurements à relief accidenté de la Formation Amabel (Silurien moyen) le long de la rivière Eramosa, à environ 10 km au nord-est de Guelph. Le diamètre de ces puits varie de < 1 m à 10 m et les profondeurs atteignent 12 m. Ils se présentent sous forme de dépressions isolées mais sont généralement regroupés ensemble et forment des murs de roc sinueux. Ces dépressions peuvent contenir du sol, des sédiments fins, des débris de la roche dolomitique environnante et des roches clastiques arrondies de lithologies du socle précambrien. Le till est remarquablement absent. Ces puits se retrouvent tout près d'interstices caverneux qui ont été formés à l'époque du Pré-Wisconsinien au Wisconsinien précoce, suggérant une possible origine karstique. Cependant, les puits cylindriques, avec leurs plus grands diamètres au point milieu, des intérieurs sculptés et des axes inclinés ainsi que l'absence de flûtes verticales et de till, tirent probablement leur origine d'une décharge fluvio-glaciaire à la fin du Wisconsinien tardif. La cavitation a peut-être aidé au développement de ces puits, rehaussant la puissance d'érosion des eaux de fonte chargées de sédiments.[Traduit par la Rédaction] [ABSTRACT FROM AUTHOR]