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Big Bang Theory

Throughout the ages, most people believed that the cosmos had existed for all eternity in an unchanging or static condition, neither expanding nor contracting. One reason individuals held this belief was an absence of scientific data, coupled with the inability to answer questions about the universe through measurement and observation. Another reason was that most individuals' beliefs tended toward parochialism and traditionalism. They preferred to believe in eternal, absolute truths, which supported their beliefs in an eternal, infinite cosmos created by God. With the arrival of the 20th century, both science and technology had developed to the point where scientists were able to formulate and then explore the empirical validity of what is called the “big bang theory.” According to this theory of the origin of the universe, at one time all space and time were packed into an incredibly small package or dimension. About 14 billion years ago, this package or dimension increased in size at an unimaginable speed, due to a massive explosion (called “singularity”). The primordial universe that was created consisted primarily of strong radiation, which led to the formation of matter and, eventually, to stars, galaxies, solar systems, planets, and moons. The evolution of the cosmos over billions and billions of years produced the right conditions for life to form on earth, leading to the development of thinking beings such as us. Although no one theory perfectly explains—or can explain—everything about the origin and structure of the universe, the big bang theory is convincing. No other theory comes as close in explaining what scientists think happened in the creation of the cosmos. The big bang theory fits both deductions from mathematical models and conclusions from observations of the cosmos.

The First Cosmologies

The Greek philosophers moved the study of the universe away from a strictly religious approach to a more naturalistic one. Aristotle's ideas influenced philosophers and scientists in the West for centuries. His observations of celestial events convinced him that the earth was spherical rather than flat like a pancake. During lunar eclipses, Aristotle noted that the shadow of the earth on the moon was always round, an impossibility if the earth were flat. A flat planet would have cast an elongated shadow, not a round one (unless he always made his observations when the sun was directly under the earth, an unlikely event). Aristotle made another observation that convinced him of the roundness of earth. He saw the sails of ships coming over the horizon before the rest of the vessel. (On a perfectly flat earth, Aristotle's first view would have been of the entire ship, not just its mast.)Although some of Aristotle's conclusions about the universe were accurate, others were not. For example, he remained steadfast in his conviction that the earth was stationary and the moon, sun, other planets, and stars moved in perfectly circular orbits around the earth.

The impact of both religion and philosophy on cosmology diminished with the growth of the physical sciences. Nicholas Copernicus, a Catholic priest, suggested in 1514 that the sun was stationary and the earth and other planets moved in circular orbits around it. Copernicus's heliocentric view was discounted for nearly a century until two astronomers, the Italian Galileo Galilei and the German Johannes Kepler, reaffirmed Copernicus's deductions. The invention of the telescope (in Holland) in the early 1600s allowed Galileo to observe stars, planets and their movements, meteors, and comets. It was during his observation of the movement of Venus that he realized Copernicus was right to believe that the earth moved around the sun. Kepler, like Copernicus and Galileo, concluded correctly that planets rotated elliptically around the sun, although he erred by thinking it was magnetic forces that were responsible.

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