The next question is in going around the ellipse, How does it go fast when it near the sun and slower when it further from the sun? and so on . If we take away the other focus we have the sun, and the planet going around. Kepler found the answer to this, too, He found this, that if you put this position of the planet down at two times separated by some definite time let's say three weeks. A nd then at another place in the orbit put the positions of the planets again separated by three weeks. A nd draw lines from the sun to the planet (technically called radius vector but anyway lines from the sun to the planet). Then the area that's enclosed in the orbit of the planet and the two lines that are separated by the planets' position three weeks apart is the same no matter what part of the orbit the thing is on. So that it has to g...