By Richard L. Myers
Scholars may be brought to the technological know-how of physics, and its functions to daily life, during this quantity. Tracing its improvement from antiquity to the current, the writer examines all features of physics together with movement, paintings, power, warmth, subject, mild, and electrical energy. Quantum & Nuclear physics also are integrated. The bankruptcy with directions for experiments in physics will support scholars in initiatives for technology festivals, and the bankruptcy on physics as a occupation may also help scholars to discover a few of the innovations for operating during this box of technological know-how. A word list, conversion desk, and record of the Nobel Prize Winners in Physics will give you the extra instruments valuable for college students.
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Additional resources for The Basics of Physics (Basics of the Hard Sciences)
Sample text
Copernicus' model of the universe put the Sun near the center of the solar system, with the Earth and the other planets revolving about the Sun. He imposed several motions on the Earth: a daily rotation, an annual revolution around the Sun, and the precession of the axis. After introducing his ideas in the Commentariolus, Copernicus continued to work on his ideas for the remainder of his life. When he was 66, with the help of Georg Joachim Rheticus (1514-1574), a German scholar from Wittenberg, Copernicus assembled his life's work on astronomy into a treatise that was eventually published in Germany.
The publication of De Revolutionibus produced little controversy during the immediate 75 years following its publication. Copernicus had died the same year it was published, and its preface presented the work as a hypothetical model. There were strong scientific and philosophical arguments that precluded its acceptance. One serious flaw was that parallax of the stars was not observed. If the Earth revolved around The Development of Classical Physics ii • xt-S r««3 X \ \ i ! / J / the Sun, then its position would change by approximately 200 million miles (twice the mean distance between the Earth and the Sun of 93 million miles) over six months.
The publication of De Revolutionibus produced little controversy during the immediate 75 years following its publication. Copernicus had died the same year it was published, and its preface presented the work as a hypothetical model. There were strong scientific and philosophical arguments that precluded its acceptance. One serious flaw was that parallax of the stars was not observed. If the Earth revolved around The Development of Classical Physics ii • xt-S r««3 X \ \ i ! / J / the Sun, then its position would change by approximately 200 million miles (twice the mean distance between the Earth and the Sun of 93 million miles) over six months.