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Unification of Sciences: Astronomy, Physics, and Chemistry I
Takeshi Oka Department of Astronomy and Astrophysics and Department of Chemistry, the Enrico Fermi Institute, the University of Chicago Tokyo Institute of Technology, 10:40 – 12:10, October 16, 2007
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Experiments, Observations
Empirical rule Fundamental theory
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PV PV = nRT = nR T The Ideal Gas Law Thermo Dynamics 273 K 1662 Boyle
Charles Gay-Lussac 273 K Avogadro Cannizzaro Boltzmann Thermo Dynamics
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Battery Luigi Galvani Alessandro Volta
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Unification of Concepts
Michael Faraday James Clerk Maxwell Electricity Magnetism Electricity Chemistry Electrochemistry Electromagnetism Light Ion, cation, anion, cathode, anode, electrode, electrolysis,… Electricity Gravity ×
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Molecule, Ion, Gas. Liquid. Salt, Solution, Colloid,
I have long held an opinion, almost amounting to conviction, in common I believe with many other lovers of natural knowledge, that the various forms under which the forces of matter are made manifest have one common origin; or, in other words, are so directly related and mutually dependent, that they are convertible, as it were, one into another, and possess equivalents of power in their action. Action of magnets on light Michael Faraday Philosophical Transactions, 1846, p. 1 Molecule, Ion, Gas. Liquid. Salt, Solution, Colloid, Crystal, Steel, Glass, Force, Motion, Electricity, Magnetism, Electrolysis, Light, Field, Discharge.
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A P C B Unification of Fields Synthesis of urea, 1828 Johannes Kepler
Galileo Galilei Friedrich Wöhler Synthesis of urea, 1828 Isaac Newton 1666
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PV PV = nRT = nR T A P C B Physics and Chemistry
Boyle PV PV = nRT = nR T Gay-Lussac Avogadro Thermo Dynamics Chemistry Statistical thermodynamics Quantum mechanics Willard Gibbs
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Astronomy, Physics, and Chemistry
X-ray Crystallography,…… A P C B Spectroscopy 1814 Approximavit Sidera "The most remarkable discovery in all of astronomy is that the stars are made of atoms of the same kind as those on the earth." Feynman Lectures on Physics I, 3-6 (1963) Joseph von Fraunhofer 1787 – 1826
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A P C B P P A B B A C C
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Who discovered H3+ ? 1766 Henry Cavendish Discovery of Hydrogen
Anders Ångstrom Spectrum of H J. J. Thomson Discovery of H3+ Niels Bohr Theory of H 堀 健夫 Analysis of H2 spectrum Charles Coulson Theory of H3+ Gerhard Herzberg Search for H3+ 岡 武史 Spectrum of H3+
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H3+ Astronomy Chemistry Nuclear fusion
Star, Galaxy, Universe Atom, Molecule, Matter Nuclear fusion H → He → C, N, O, Ne, Mg, Si, S,…..Fe… Star ← Molecular cloud Interstellar chemistry HCO+ Ion – neutral reactions H3+ William Klemperer
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H3+ Star formation Formation of molecules Star Diffuse cloud
Dense cloud Formation of molecules Star H3+ Spontaneous emission Collision
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Astronomers’ Periodic Table
H He C N O Ne Mg Si S Ar Fe Ben McCall
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Molecules everywhere CO HC5N HC7N HC9N ●
Ungerechts & Thaddeus, ApJS 63, 645 (1987)
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H2 → H2+ + e- [H2] ~ 10-17s-1 Plasmas everywhere
Cosmic Ray primary particles cm-2s-1 H2 → H2+ + e [H2] ~ 10-17s-1 H2+ + H2 → H + H kL[H2][H2+] H3+ + O → OH+ + H kL[H3+][O] kL~ 10-9 cm3 s-1 H2 H2 e OH+ → H2O+ → H3O+ → H2O -H -H O + H2 → OH + H
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