un:galileo
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- | ====== Galileo Galilei ====== | ||
- | Galileo (1564--1642, | ||
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- | Galileo' | ||
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- | Galileo' | ||
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- | $$ \frac{t_1}{t_2} = \frac{s_1}{s_2} $$ | ||
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- | or the ratio of the times is equal to the ratio of the distances if the velocity is constant. If the velocity is different for two different motions, then it can be shown that | ||
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- | $$ \frac{t_1}{t_2} = \frac{s_1}{s_2} \frac{v_2}{v_1} $$ | ||
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- | or the ratio of the times is equal to the product of the direct ratio of the distances and the inverse ratio of the velocities. | ||
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- | What if the velocity is not just different for different sets of motions, but changes continually during a movement, that is if the velocity is subjected to a constant acceleration $a$? Galileo understood that in this case, $v=at$ and | ||
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- | $$ s = \frac{1}{2} at^2 $$ | ||
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- | if an object is accelerated from rest for a certain period of time. If an object is falling freely under gravity on the surface of the Earth, it is subjected to a constant acceleration $g$ and the equations become $v=gt$ and $s=gt^2/2$. Galileo did not use this notation, but he did discover the ' | ||
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- | $$ \frac{s_1}{s_2} = \frac{t_1^2}{t_2^2}. $$ | ||
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- | Galileo combined the concepts of motion at //constant [[velocity]]// | ||
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- | His mathematical methods looked back to Euclid, but his experimental and observational methods looked forward to our modern age. His system of units was as modern as us. His unit of length was called //punto// where 1 punto = 0.094 cm. And for time he used 1 tempo = 0.01 s. For weighing he used 1 grain = 0.065 g. His units were so small that his experiments always yielded large numbers, therefore he could get many significant figures without resorting to decimals. | ||
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- | His celestial observations set the standard for astronomical observations once and for all. | ||
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- | Galileo' | ||
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