Read e-book online 40 Days and 40 Nights: Darwin, Intelligent Design, God, PDF

By Matthew Chapman

ISBN-10: 0061337765

ISBN-13: 9780061337765

During this attention-grabbing tale of evolution, faith, politics, and personalities, Matthew Chapman captures the tale at the back of the headlines within the debate over God and technology in America.

Kitzmiller v. Dover Board of schooling, made up our minds in overdue 2005, pitted the educating of clever layout (sometimes referred to as "creationism in a lab coat") opposed to the instructing of evolution. Matthew Chapman, the great-great-grandson of Charles Darwin, spent numerous months overlaying the trial from starting to finish. via his in-depth encounters with the participants—creationists, preachers, lecturers, scientists on either side of the problem, legal professionals, theologians, the pass judgement on, and the 11 mom and dad who resisted the fundamentalist proponents of clever design—Chapman tells a occasionally terrifying, usually hilarious, and notably relocating tale of normal humans doing conflict in the United States over where of faith and technology in sleek lifestyles.

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Extra info for 40 Days and 40 Nights: Darwin, Intelligent Design, God, Oxycontin®, and Other Oddities on Trial in Pennsylvania

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Attempts to characterize the composition of interstellar dust in both the dense and diffuse ISM have led to observations of bright background sources observed through great quantities of interstellar dust. These features are not intrinsically related to the sources which illuminate the column of dust, but rather are carried by the intervening dust along our line-of-sight. A multitude of absorption and emission features have been observed in this manner (see Whittet & Tielens 1997). Among the many spectroscopic signatures observed in the near infrared are two absorption bands that may be the strongest representatives of the processed organic component of interstellar dust.

Sauval, A. , and Blomme, R 1992, in Infrared Solar Physics, eds. D. Rabin and J. T. Jefffries [Dordrecht: Kluwer]' p. 539 Holweger, H. and Mueller, E. A. , 39, 19 Hong, S. S. and Greenberg, J. M. 1980, Astron. , 88, 194 Jenkins, E. B. 1986, Astrophys. , 304, 739 Jenkins, E. , Savage, B. , and Spitzer, 1. 1986, Astrophys. , 301, 355 Joseph, C. 1. 1988, Astrophys. , 335, 157 Joseph, C. , Snow, T. , and Seab, C. G. 1989, Astrophys. , 340, 314 Joseph, C. , Snow, T. , Seab, C. , and Crutcher, R M.

Thus far, none of the dense cloud detections have shown subfeatures like those in the diffuse ISM spectra. Smith et al. (1993) discussed the most likely scenarios for the absence of the aliphatic substructure in the dense cloud spectra. Among the possibilities that were ruled out was the idea that the aliphatic hydrocarbons are part of the grain core which becomes mantled with ice in the dense cloud. 4 J-lm in the laboratory spectra. 4 J-lm wing in dense cloud spectra arises from material in the grain mantle, rather than the core, comes from correlation studies comparing the optical depth of the "long-wavelength wing" with other dense cloud absorption features.

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40 Days and 40 Nights: Darwin, Intelligent Design, God, Oxycontin®, and Other Oddities on Trial in Pennsylvania by Matthew Chapman


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