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Babylonian astronomy was the study or recording of celestial objects during early history Mesopotamia.
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The Greek philosopher Aristotle, established a geocentric universe in which the fixed, spherical Earth is at the centre, surrounded by concentric celestial spheres of planets and stars.
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He did this by noting the precise locations stars rose and set during equinoxes – the twice yearly dates when night length and day length are exactly 12 hours.
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The mathematical part of the Aryabhatiya covers arithmetic, algebra, plane trigonometry, and spherical trigonometry. It also contains continued fractions, quadratic equations, sums-of-power series, and a table of sines.
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Newton’s law of gravitation, any particle of matter in the universe attracts any other with a force varying directly as the product of the masses and inversely as the square of the distance between them.
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Swedenborg proposed that the sun had developed a dense surface layer that was forced outward by the centrifugal force of its rotation, into the equatorial plane of the solar rotation.
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Max Planck heuristically derived a formula for the observed spectrum by assuming that a hypothetical electrically charged oscillator in a cavity that contained black-body radiation could only change its energy in a minimal increment, E, that was proportional to the frequency of its associated electromagnetic wave.
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According to the Big Bang theory, the expansion of the observable universe began with the explosion of a single particle at a definite point in time.
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Edwin Hubble proved that there is a direct relationship between the speeds of distant galaxies and their distances from Earth.
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Black Hole Entropy is the amount of entropy that must be assigned to a black hole in order for it to comply with the laws of thermodynamics as they are interpreted by observers external to that black hole.
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Cosmological inflation, is a theory of exponential expansion of space in the early universe.