# NavList:

## A Community Devoted to the Preservation and Practice of Celestial Navigation and Other Methods of Traditional Wayfinding

**Re: First sine table (Ptolemy)**

**From:**Frank Reed

**Date:**2009 Jan 23, 23:23 -0800

Jim, you asked: "Were infinite series used in the initial creation of tables?" No, not the early tables. One way to generate tables is to use the trigonometric identities for sums and differences of angles. Consider this: we know some exact values, e.g. sine and cosine of 0�, 30�, 45�, 60�, 90�. If you have arbitrarily good values for the square root of two and the square root of three, then you have arbitrarily good values for the trig functions of those angles. Now we can also calculate the sine of one degree to fairly good accuracy using a variety of methods (see below). That's our anchor. And the cosine of one degree is sqrt(1-sin^2(1)) so we calculate that one by hand as accurately as possible. Then how do we get the sine and cosine of 2 degrees? Use the identities: sin(a+b) = sin(a)*cos(b) + sin(b)*cos(a), cos(a+b) = cos(a)*cos(b) - sin(a)*sin(b), which in this case would be sin(2�) = sin(1�)*cos(1�) + sin(1�)*cos(1�), cos(2�) = cos(1�)*cos(1�) - sin(1�)*sin(1�). And then the sine and cosine of 3 degrees? Just build on the previous result: sin(3�) = sin(2�)*cos(1�) + sin(1�)*cos(2�), cos(3�) = cos(2�)*cos(1�) - sin(2�)*sin(1�). And so on... And note that you really only need to calculate from 0 to 45 degrees. After that, you just re-label the table using sin(x) = cos(90-x) etc. Next we look up all of these values in our table of logarithms (let's assume someone has already provided us with that) and then we can get a table of tangents rather quickly from tan(a) = inverselog[logsin(a)-logcos(a)]. These are the general sorts of calculations that were used. There are lots of tricks for speeding things up and reducing error. For example, we can get exact values for the sine and cosine of 15 degrees using half-angle identities. And from there, the sine/cosine of 7.5 degrees. Then going back to the sum identities, we get "exact" values for any angle that is a multiple of 7.5 degrees. Finally, up at the top I mentioned that we need the sine of 1 degree. At some level of accuracy the sine of a small angle is equal to the arc. That is, sin(x degrees) = x*pi/180, for a small angle. For a low accuracy table, you could assume that this holds for x=1�. For a higher accuracy table, you would assume that this holds for x=1'. Then you build up arcminute by arcminute until you get a better value for the sine of 1 degree and proceed again as above. -FER --~--~---------~--~----~------------~-------~--~----~ Navigation List archive: www.fer3.com/arc To post, email NavList@googlegroups.com To unsubscribe, email NavList-unsubscribe@googlegroups.com -~----------~----~----~----~------~----~------~--~---