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In 1572 Tycho observed a star which suddenly
appeared in the heavens (we now recognize
this as an exploding star: a supernova). He noted that this ``new star''
did not change in position with respect to the other stars and should
therefore be in the outer sphere of Aristotle's universe. But this was
supposed to be an eternal, unchanging sphere! He published these
observations in The Nova Stella in 1574. The same type of problems
arose due to his observations of a comet which appeared in 1577, for he
could determine that this object was farther than Venus again
contradicting the Aristotelian idea that the universe beyond the Moon
was perfect, eternal and unchanging.
This is a case where better observations when pitted against
the best theory of the time produced discrepancies which, in time,
proved to be fatal to the current model
and would eventually give rise to a better, more
precise theory of the universe (see Sect. 1.2.1).
By this time also most of the Medieval approach to physics had been
shed, though not completely. For example, the motion of a projectile was
thought to be composed of an initial violent part (when thrown) and a
subsequent natural part (which returns it to the ground). Still it was
during this time that the importance of velocity and force in
determining the motion of objects was realized.
The birth of new theories is not easy, however. In this case
it was not until the late 17th century that a complete new view of the
universe was polished and could be used as a tool for investigating
Nature. By this time the Aristotelian doctrine was, finally, set aside.
The first step in this long road was taken by Copernicus, the next
by Johaness Kepler in his investigations of the motion of the planets
and then by Galielo through his investigations on the nature of motion
and his description of the solar system.
Next: Kepler
Up: The Copernican Revolution
Previous: The Copernican Revolution
Jose Wudka
9/24/1998