
Index 9a. Earth orbits Sun? 9b. The Planets 9c. Copernicus to Galileo 10. Kepler's Laws Kepler's Laws (For teachers) 10a. Scale of Solar Sys. 11. Graphs & Ellipses 11a. Ellipses and First Law 12. Second Law 12a. More on 2nd Law 12b. Orbital Motion 12c. Venus transit (1) 12d. Venus transit (2) 12e. Venus transit (3) Newtonian Mechanics 13. Free Fall 14. Vectors 15. Energy 
The laws of orbital motion are mathematical, and one cannot explore them without some mathematics. The math used here is rather elementary; if you need a refresher click here. Otherwise, you can just skip the equations and follow the narrative. The Mathematical Description of a CurveAs already noted, the cartesian system labels any point in a plane (e. g. on a flat sheet of paper) by a pair of numbers (x,y), its distance from two perpendicular axes. These numbers are known as the "coordinates" of the point. A line in the planestraight or curvedcontains many points, each with its own (x,y) coordinates. Often there exists a formula ("equation") which connects x and y: for instance, straight lines have a relationship y = ax + b where any pair of numbers (a,b), positive, negative or zero, gives some straight line. The plot of a line given by one of such relationship (or indeed by any relationshipeven pure observation, e.g. temperature against timeis known as a graph. More complicated relationships give graphs that are curves: for instance y = ax^{2} gives a parabola, with a any number. Usually (though not always) y is isolated, so that the formula has the form y = f(x) where f(x) stands for "any expression involving x" or in mathematical terms, a "function of x." The curves drawn here are the straight line y = (2/3)x + 2 and the parabola y = x^{2}. A list of some of their points follows. 
Straight line: 
x  1  0  1  2  3  4 
y  8/3  2  4/3  2/3  0  2/3 
Parabola: 
x  2  1.5  1  0.5  0  0.5  1  1.5  2 
y  4  2.25  1  0.25  0  0.25  1  2.25  4 
The Equation of a CircleIn the vast majority of formulagenerated graphs, the formula is given in the form
Such a form makes it very easy to find points of the graph. All you have to do is choose x, calculate f(x) (= some given expression involving x) and out comes the corresponding value of y. However, any equation involving x and y can be used as the property shared by all points of the graph. The main difference is that with more complicated equations, after x is chosen, finding the corresponding y requires extra work, (and sometimes it is easier to choose y and find x). Perhaps the bestknown graph of this kind is a circle of radius R, whose equation is 
Draw a circle of radius R centered at the origin O of a system of (x,y) axes . Given any point P on the circle with specified values of (x,y), draw a perpendicular line from P to point A on the xaxis. Then 
Here x and/or y may be negative, if they are to the left of the yaxis or below the xaxis, but regardless of sign, x^{2} and y^{2} are both always positive. Since the triangle OAP has a 90° angle in it, by the theorem of Pythagoras, for any choice of P, the relation below always holds:
Since this can also be written The equation of the circle is satisfied by any point located on it. For instance, if the graph is defined by the equation:
this equation is satisfied by all the points listed below: 
x  5  4  3  0  3  4  5  4  3  0  3  4  ( 5 ) 
y  0  3  4  5  4  3  0  3  4  5  4  3  ( 0 ) 
The Equation of an EllipseThe equation of the circle still expresses the same relation if both its sides are divided by R^{2}:
The equation of an ellipse is a small modification of this:
where (a,b) are two given numbers, for example (8,4). What would such a graph look like? Near the x axis, y is very small and the equation comes close to
From which


The graph in that neighborhood therefore resembles the section of a circle of radius a, whose equation
also comes close to x^{2} = a^{2} in this region. In exactly the same way you can show that near the yaxis, where x is small, the graph cuts the axis at y=±b and its shape there resembles that of a circle of radius b.
An exampleLet us draw the ellipse
We already know that it cuts the axes at x=±8 and at y=±4. Let us now add a few points:

(1) Choose y = 2 .
Then from the equation

Substract 1/4 from both sides
Take roots (marked here by √) and retain only 34 figures:
from which x = 6.93 within resonable accuracy.

(2) Choose y = 3 . 
Substract 9/16 from both sides
Take square roots (to an accuracy of 34 figures):
from which, approximately, x = 5.29 Again, either sign can be attached to x and y. We get 12 points, enough for a crude graph: 
x  8  6.93  5.29  0  5.29  6.93  8  6.93  5.29  0  5.29  6.93  ( 8 ) 
y  0  2  3  4  3  3  0  2  3  4  3  2  ( 0 ) 
 The ellipse was already familiar to ancient Greek scientists (who fell under the term "philosophers", lovers of wisdom), but they defined it differently.
To them the ellipse was the collection of all points (in a flat plane) for which
the sum of the distances R_{1} + R_{2} from two given points was the same (see drawing). It was a natural extension of the definition of a circle, which is the collection of all points at the same distance (the radius R) from one given point (the center). One point and the distance R defines a circle, two points and the distance R_{1} + R_{2} define an ellipse. 
Next Stop, for those
familar with trigonometry #11a Ellipses and Kepler's First Law
Trigonometrywhat is it good for? and the sections that follow.) 
Timeline Glossary Back to the Master List
Author and Curator: Dr. David P. Stern
Mail to Dr.Stern: stargaze("at" symbol)phy6.org .
Last updated: 9182004
Curators: Robert Candey, Alex Young, Tamara Kovalick
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