The nature of olfaction; its importance for understanding perennial issues of philosophy of mind, perception, and consciousness; and its implications for cognitive neuroscience. What are smells? Despite the best efforts of philosophy and the chemosciences, the question remains vexing—but no more perplexing than the historical lapse of the past centuries to seriously consider a sense that has a key place in philosophy of mind and perception. Stinking Philosophy! is Benjamin Young’s answer to this critical lapse. Drawing together more than a decade's research on olfactory philosophy, the book offers a clear, comprehensive look at the nature of odors—how we perceive smells, how we cognitively represent odors, how we communicate about them as categories, and what they can tell us about consciousness. In Stinking Philosophy! Young presents a methodology for addressing the philosophical and conceptual issues raised by the sense of smell. Then, in an exacting and coherent fashion, he explores how the philosophy of smell contributes to—and advances—a wide range of debates within philosophy of mind, perception, and cognitive neuroscience. Ultimately, his work demonstrates how empirically informed philosophy can have a significant impact on interdisciplinary research on smell across philosophy, the chemosciences, and neuroscience.
In this widely acclaimed literary debut, Benjamin Cavell stalks the male ego, unleashing a ferocious volley of nine sharply written and deeply penetrating stories. In Balls, Balls, Balls, we are introduced to Logan Bryant, the star member of the “fourth best paintball team in the tristate area.” Despite his knowledge of napalm recipes and his skill during Military Simulations—MilSim, for short—Logan’s armor shows fractures with every move he makes. In The Death of Cool, an insurance adjuster has come to realize much too clearly the range of threats that surround him. “Tired of trusting in the other guy’s morality,” he embraces his paranoia and leaves as little to chance as possible. The Ropes opens in a hospital room after Alex Folsom has sustained a devastating concussion. With both college and his boxing career behind him, he reunites with his father on Martha’s Vineyard to assess the damage--both physical and emotional. Rumble, Young Man, Rumble is a ground-shaking announcement of the next heavy hitter in American letters.
This historic book may have numerous typos and missing text. Purchasers can download a free scanned copy of the original book (without typos) from the publisher. Not indexed. Not illustrated. 1902 Excerpt: ...earth. r' = radius of moon, or other body. P = moon's horizontal parallax = earth's angular semidiameter as seen from the moon. f = moon's angular semidiameter. Now = P (in circular measure), r'-r = r (in circular measure);.'. r: r':: P: P', or (radius of earth): (radios of moon):: (moon's parallax): (moon's semidiameter). Examples. 1. Taking the moon's horizontal parallax as 57', and its angular diameter as 32', find its radius in miles, assuming the earth's radius to be 4000 miles. Here moon's semidiameter = 16';.-. 4000::: 57': 16';.-. r = 400 16 = 1123 miles. 2. The sun's horizontal parallax being 8"8, and his angular diameter 32V find his diameter in miles. ' Am. 872,727 miles. 3. The synodic period of Venus being 584 days, find the angle gained in each minute of time on the earth round the sun as centre. Am. l"-54 per minute. 4. Find the angular velocity with which Venus crosses the sun's disc, assuming the distances of Venus and the earth from the sun are as 7 to 10, as given by Bode's Law. Since (fig. 50) S V: VA:: 7: 3. But Srhas a relative angular velocity round the sun of l"-54 per minute (see Example 3); therefore, the relative angular velocity of A V round A is greater than this in the ratio of 7: 3, which gives an approximate result of 3"-6 per minute, the true rate being about 4" per minute. Annual ParaUax. 95. We have already seen that no displacement of the observer due to a change of position on the earth's surface could apparently affect the direction of a fixed star. However, as the earth in its annual motion describes an orbit of about 92 million miles radius round the sun, the different positions in space from which an observer views the fixed stars from time to time throughout the year must be separated ...
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