In an ellipse, the ratio of the distancebetweenthefocitothemajoraxis
Ellipse
Aclosedcurve for which the sum of the distances from any point on the ellipse to two points inside (called the foci) is alwaysthesame
Focus
(Plural: foci) Oneoftwofixedpointsinsideanellipse from which the sum of the distances to any point on the ellipse isconstant
Kepler'sfirstlaw
Each planet moves around the Sun in an orbit that is an ellipse, with the Sun at one focus of the ellipse
Kepler's second law
The straight line joining a planet and the Sun sweeps out equal areas in space in equal intervals of time
Kepler's third law
The square of a planet's orbital period is directly proportional to the cube of the semimajor axis of its orbit
Major axis
The maximum diameter of an ellipse
Orbit
The path of an object that is in revolution about another object or point
Orbital period (P)
The time it takes an object to travel once around the Sun
Orbital speed
The speed at which an object (usually a planet) orbits around the mass of another object; in the case of a planet, the speed at which each planet moves along its ellipse
Semimajor axis
Half of the major axis of a conic section, such as an ellipse
Tycho Brahe
Danish astronomer and nobleman
Made accurate observations of the movement of celestial bodies
Invented different astronomical instruments
Made an extensive study of the solar system
Determined the position of777 fixed stars accurately
Johannes Kepler
Born to a poor German family
Studied as a scholar at the University of Tübingen in 1589
Worked as an assistant to Tycho Brahe
Interpreted Brahe's observations of Mars
Formulated the three laws of planetary motion
When King Frederick II died
Brahe moved to Prague where he was supported by Emperor Rudolf II
Emperor Rudolf II
Recommended Johannes Kepler to work for him as an assistant
Brahe and Kepler had an unsteady working relationship
Brahe mistrusted Kepler with his astronomical data in fear of being shadowed by his assistant
Brahe's work with Kepler
1. Brahe assigned to Kepler the interpretation of his observations of Mars
2. Kepler was tasked to figure out what pattern the movement of Mars did not match Brahe's calculations
Tycho Brahe
Danish astronomer and nobleman who made accurate observations of the movement of celestial bodies
Johannes Kepler
German astronomer and mathematician who worked as an assistant to Brahe and formulated the three laws of planetary motion based on Brahe's extensive astronomical data
Kepler's First Law
Planets follow an elliptical orbit
Kepler's Second Law
When an imaginary line is drawn from the center of a planet to the center of the Sun, an equal amount of space is swept in equal amount of time
Kepler's Third Law
The ratio of the squares of the period of two planets is equal to the ratio of the cubes of the planets' average distance from the Sun
Brahe was able to determine the position of 777 fixed stars accurately
When King Frederick II died, and the successor did not fully support Brahe's work, he moved to Prague in 1599 where he was supported by Emperor Rudolf II and worked as an imperial mathematician
Emperor Rudolf II recommended Johannes Kepler to work for him as an assistant
Kepler was born to a poor German family and studied as a scholar at the University of Tübingen in 1589
Brahe and Kepler had an unsteady working relationship. Kepler was Brahe's assistant. However, Brahe mistrusted Kepler with his astronomical data in fear of being shadowed by his assistant
Brahe assigned to Kepler the interpretation of his observations of Mars, whose movement did not match Brahe's calculations. Kepler was tasked to figure out what path Mars followed as it revolved around the Sun
Kepler postulated that there must be a force from the Sun that moves the planets. He was able to conclude that this force would explain the orbit of Mars and the Earth, including all the other planets, moved fastest when it is nearest from the Sun and moved slowest when it is farthest from the Sun
Brahe decided to give all his data to Kepler hoping that he would be able to prove his Tychonic system and put together new tables of astronomical data. This table was known as Rudolphine Tables, named after the Roman emperor and was useful in determining the positions of the planets for the past 1000 years and the future 1000 years
After Brahe died in 1601, Emperor Rudolf II assigned Kepler as the new imperial mathematician, and all of Brahe's writings, instruments, and the Rudolphine tables were passed on to him
From Brahe's data, Kepler was able to formulate his laws of planetary motion: the law of ellipses, the law of equal areas, and the law of harmonies