Planetary Systems from the Ancient Greeks to Kepler
Clasificación: | Libro Electrónico |
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Autor principal: | |
Formato: | Electrónico eBook |
Idioma: | Inglés |
Publicado: |
Seattle :
University of Washington Press,
2018.
|
Temas: | |
Acceso en línea: | Texto completo |
Tabla de Contenidos:
- Cover
- Planetary Systems from the Ancient Greeks to Kepler
- Title
- Copyright
- Contents
- List of Figures
- Foreword
- Introduction
- I. Astronomical Knowledge of the Ancient Greeks
- Knowledge of the Sun's, the Moon's, and the Planets' Apparent Motions
- The Aspects, Stations, and Retrograde Motions of the Planets
- The Periods of the Planets
- Apparent Planetary Loops and Zigzags
- The Elements of a Planetary Orbit
- Orbit Computation
- Concepts of Some Early Greek Philosophers
- Thales of Miletus (c. 624-546 B.C.)
- Anaximander (c. 611-545 B.C.)
- Anaximenes of Miletus (c. 585-528 B.C.)
- Anaxagoras of Clazomenae (c. 500-428 B.C.)
- Pythagoras of Samos (c. 580-500 B.C.)
- Philolaus, the Pythagorean (c. 470-400 B.C.)
- Hicetas of Syracuse (c. 350 B.C.)
- Ecphantus of Syracuse (c. 325 B.C.)
- Xenophanes of Colophon (c. 530 B.C.)
- Heraclitus of Ephesus (c. 500 B.C.)
- Empedocles of Agrigentum (c. 450 B.C.)
- Leukippus of Abdera (c. 450 B.C.)
- Democritus of Abdera (c. 400 B.C.)
- Metrodorus of Chios (c. 400 B.C.)
- Plato of Samos (427-347 B.C.)
- Aristotle of Stagira (384-322 B.C.)
- Heracleides of Pontus (c. 350 B.C.)
- Aristarchus of Samos (c. 310-230 B.C.)
- II. Eudoxus (408-355 B.C.)
- Eudoxus's Lunar Theory
- Eudoxus's Solar Theory
- Eudoxus's Planetary Theory
- The Systems of Spheres
- III. Hipparchus (fl. 146-126 B.C.)
- Hipparchus's Main Astronomical Contributions
- Hipparchus's Solar Theory
- The Apparent Nonuniform Motion of the Sun in the Ecliptic
- Hipparchus's Method of Finding the Line of Apsides and the Eccentricity of the Sun's Orbit (Considered as an Eccentric Circle)
- Hipparchus's Method of Predicting the Sun's Place at Any Instant
- Equivalence of Epicyclic and Eccentric Motion
- Hipparchus's Lunar Theory
- Hipparchus's Method of Finding the Line of Apsides and Eccentricity of the Moon's Orbit
- Hipparchus's Method of Predicting the Moon's Place at Any Time
- Hipparchus's (Abortive) Theory of Planetary Motion
- Hipparchus's Method of Finding the Stationary Points and Arcs of Retrogression of a Planet (a Method Originally Due to Apollonius)
- Hipparchus's Eclipse Method of Finding the Actual Distances and Diameters of the Sun and Moon
- Hipparchus's Discovery of the Precession of the Equinoxes
- Hipparchus's Discussion of Errors
- IV. Ptolemy (fl. 125-150)
- Ptolemy's Main Contributions to Astronomy
- Contents of the Almagest
- Ptolemy's Solar Theory
- Ptolemy's Work on the Lunar Orbit
- Ptolemy's View of the Regression of the Nodes and the Advance of the Apsides of the Lunar Orbit
- Ptolemy's Preliminary Derivation of the Elements of the Lunar Orbit
- The Motions in Ptolemy's Lunar Orbit
- The Effects of Evection
- Ptolemy's Explanation of the Evection
- Ptolemy's Determination of the Evection at the Quarters
- The Prosneusis
- Ptolemy's Computation of the Prosneusis and an Example of His Prediction of the Moon's True Longitude