Nicolaus Copernicus (1473-1543)
 
Latinized form of Niclas Kopernik, the name of the founder of the heliocentric planetary theory; born at Torun[Thorn], 19 february , 1473, died at Frankenburg, 24 May, 1543. Copernicus proposed that a rotating Earth revolving with the other planets about a stationary central Sun could account in a simpler way for the same observed phenomena of the daily rotation of the heavens, the annual movement of the Sun through the ecliptic, and the periodic retrograde motion of the planets. He was encouraged to publish his theories, but he was reluctant to do so. However, he relented and did publish them; they were handed to him the very day he died.

 

go to top


Johannes Kepler (1571-1630)


The German astronomer was the first strong supporter of the heliocentric theory of Copernicus; [refers to or measured from the Sun's center or appearing as if seen from it.Also, having or relating to the Sun as the center of the solar system.] Kepler was also the discoverer of the three laws of planetary motion. Kepler, always guided by the concept of beauty in the structure of the universe, and specifically by a theory of harmony in geometric figures, numbers, and music, especially in his Harmonices mundi [Harmomonies of the world, 1619], announced his third law--a relationship between the orbital periods and the distances of the planets from the Sun. His belief that the Sun regulates the velocity of the planets was a milestone in scietific thought, laying the foudation for Newton's theory of universal gravitation. The posthumous Somnium on which Kepler labored until shortly before his death, is indicative of his fertile mind. In this work, Kepler describes a journey to the Moon and discusses the existence of lunar inhabitants. A crucial link between the thought of Copernicus and that of Newton, Kepler was an important figure in thwe 17th-century scientific revolution.

go to top


Galileo Galilei (1564-1642)
In the summer of 1609, Galileo heard about a spyglass that a Dutchman had shown in Venice. From these reports, and using his pwn technical skills as a mathmetician and a workman, Galileo made a series of telescopes whose optical performance was much better than that of the Dutch intrument. The astronomical discoveries he made with his telescope were described in a short book called Message from the stars[Sidereus Nunicus] published in Venice in May 1610. It caused a sensation. Galileo claimed to have seen mountainson the Moon, to have proved the Milky Way was made up of tiny stars, and to have seen four small bodies orbiting Jupiter. These last, with an eye on getting a job in Florence, he promptly named 'the Medican stars'[Galileo Galilei]. There eventually followed some expression of interest by the Inquistion. According to the Holy Church, Copericanism was in contradiction with Scripture, and in 1616 Galileo was given some kind of secret, but official warning that he was not to defend Copernicanism. Just what was said on this occasion was to become a subject for dispute when Galileo was accused of departing from this undertaking in his Dialogue concerning the two greatest world systems, published in Florence in 1632. Galileo, who was not in the best of health, was summoned to Rome, found to be vehemently suspected of heresy, and eventually condemned to house arrest, for life, at his villa at Arcetri. He was also required to state an oath before the Holy Roman Church in which he was forced to renounce his belief that the Sun was at the center of  the solar system. 

Sir Isaac Newton (*1642-1727)

Isaac Newton{1643-1727}

Sir Isaac Newton was an English 
mathemetician and physcist. He is considered one of the greatest scietists in history, who made important contributions in many fields of science. His discoveries and theories laid the foundation for much of the progress in science since his time. Newton was one of the inventors of the btranch of mathematics called calculus. He also solved the mysteries of light and optics, formulated the three laws of motion, and derived from them the law of universal gravitation.Newton's laws of motion are the most fundamental natural laws of classical mechanics. Sir Isaac Newton stated them in his book Prinicipia Mathmatica[1686]. Taken together, Newton's three laws of motion underlie all interactions of force, matter, and motion except those of relativistic and quantum effects
  • The laws of Inertia-An object at rest tends to stay at rest unless acted upon by an outside force. Newton's second law of motion establishes a relationship between the unbalanced force applied to an object and the resultant acceleration of the object. [In other words, force equals mass times acceleration, or F=ma.

  • Newton's third law of motion, which is also known as the principle of action and reation, states for that every action, there is an equal but opposite reaction.