Kepler's Laws and Planetary Movement

By the 1600's, the way the solar system and the entire universe started to observe have changed. In the controversial conclusions of Copernicus, scientists began to adopt the concept of the solar system in the solar center. Further development of astronomy was achieved through the work of Tycho Brahe and his assistant Johannes Kepler. The three planetary laws developed by Kepler and the data collected by Brahe form a way for science to closely observe the structure and movement of planets in the solar system and continue to this day.

German astronomer Johannes Kepler of the 17th century accepted the claim of Nicola Copernicus (which can be traced back to Samos Alistar Kos) that the planet goes around the sun instead of the earth. Using an improved measurement of planetary motion by the 16th century Danish astronomer Tycho Brahe, Kepler depicted the orbit of the planet with simple geometric and mathematical relationships. At the same time, Italian astronomers and natural philosopher Galileo Galilei made progress on understanding the "natural" movements of the Earth's celestial body and simply accelerating its movement. This force is necessary to change the movement and it is not necessary to maintain the same movement. When studying how an object falls to the earth, Galileo discovered that motion is a constant acceleration.

Johannes Kepler (1571 - 1630) was in charge of developing the Keplerian law of planetary motion. These laws include sweeping across equal areas at equal time intervals where the planet's orbit is elliptical, the sun is at one of the two focal points, and the line connecting the planet and the sun is equal Yes. The long axis cube is proportional. Kepler was one of the first people to integrate in the fields of physics and astronomy. This caused some controversy, but his idea was widely read and accepted after his death. When Newton derives Kepler's law from the universal gravity theory, they become part of the classic of scientific revolution.