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s restoration of the standard is not so easy a task as would be commonly supposed, for apart from the determination of the yard with mathematical accuracy, alternations of heat and cold have to be taken into account; for, as is well known, a strip of metal which measures thirty-six inches long in a temperature of 70 degrees, will not measure the same in 50 degrees. Connected with this subject, it was stated at one of the meetings of the society, that the ancient Saxon yard was nearly identical with the modern French _metre_; whence a suggestion of 'the possibility of the Saxon yard being actually derived from a former measure of the earth, made at a period beyond the range of history, the results of which have been preserved during many centuries of barbarism.' Be this as it may, we are now given to understand that the Egyptian Pyramids, whether originally erected for purposes of sepulture or not, are, at the same time, definite portions of a degree of the earth's surface in the meridian of Egypt; and it has been proposed, as these mighty structures are far more durable even now than anything which we could build in England, that when our standard shall be re-established, the length shall be cut on the side of one of the pyramids, together with such explanatory particulars as may he necessary, so as to preserve the record for all coming time. Modern science thus availing itself of the labours of the past, would be a remarkable incident in the history of philosophy. The appearance of extraordinary spots on the sun has attracted a more than ordinary degree of attention to that luminary, and to Mr J. Nasmyth's 'views respecting the source of light,' which, though published a few months since, are now again talked about. Mr Nasmyth, after several years' observation, comes to the conclusion, 'that whatever be the source of light, its production appears to result from an action induced on the _exterior surface_ of the solar sphere;' and he believes it reasonable to 'consider the true source of the latent element of light to reside, _not in the solar orb_, but in space itself; and that the grand function and duty of the sun is to act as an agent for the bringing forth into vivid existence its due portion of the illuminating or luciferous element; which element he supposes to be diffused throughout the boundless regions of space, and which in that case must be perfectly exhaustless. Further, assuming this luciferous element t
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