(M-3) Formulas

  Unknown numbers are usually represented by letters of the alphabet. The letterx is the all-out favorite, with y used when a second unknown is needed and z for a third. By the way, the name used for the unknown number by early mathematicians (like Al-Khorezmi) was "the thing"--"shai" in Arabic, "res" in the Latin which scholars used in Europe.

  However, different letters are also used, often hinting at the quantity they represent--v for an unknown velocity, T for an unknown time,m or M for unknown masses and F for an unknown force. (These will be used later in the calculation of Lagrangian points).

  "Unknown" may be broadened to include "unspecified"--letters standing for numbers which may actually be known, but with whose exact values we do not want to bother, either because (#1) we want to save writing them out, or (#2) because we have not yet chosen them.

  An example of case (#1) is the ratio between the length of a circle and its diameter, a universal constant appearing in many equations (for example, Kepler's equation in section (12a)), whose value to 11 decimals is 3.14159265359... Although the number is known, it is universally represented in all equations by the letter p (Greek p, pronounced "pi"). It is only replaced with the actual number when the unknown quantity is derived.

  As an example of case (#2), consider the distance s which a dropped ball covers in a time of t seconds, starting from rest. It is

s = (1/2) gt2

(touching symbols--including the term (1/2)--get multiplied, remember?).
  Here g is the number giving the strength of the Earth's gravity pull: if s is in meters, g = 9.81, if in feet, g = 32.16 (9.81 meters = 32.16 feet). It is known, but (as in example #1 above), you don't bother with its actual value until the moment you actually use it. But the time t is not yet chosen! Whatever you choose for t, the formula will give you the appropriate distances.

  The above is a typical formula. It looks like an equation, but the game is a little different: you are not asked to "dig out the unknown number," because it is already in plain sight. All you do is choose the value of t and you get the corresponding value of s.

  Still, the "digging out" skills you learn with equations are also useful here. Suppose you seek the inverse relationship--given s, what is t? One now views t as the unknown and proceeds to isolate it. Multiply both sides by 2

2s = gt2

and divide by g

2s/g = t2

To go from t2 to t one must find the square root, an easy task for anyone with a calculator having a square root button (slower methods also exist, using pencil and paper). Mathematics has a sign for this, but since the web does not provide it, we write instead SQRT:

SQRT(2s/g) = t

Now, whatever the distance s is, one can put it in the equation and derive the appropriate time t, in seconds.


Substitution of Formulas

Continuing the discussion of substitutions from section (M-1), here is a situation which happens quite frequently. In one of the problems in "Stargazers", for instance, one arrives at two equations:

VT = 2 p R     (1)

VT1 = 2 p R1    (2)

where T1 and R1 are variables (known or unknown) different from T and R. If both sides of equation (2) are divided by the left side of (1)--that is, by VT--what remains is still equal, because we have treated both sides of (2) equally:

(VT1)/(VT)> = 2 p R1/(VT)

However, because of the = sign in (1), we could replace the denominator on the left by
2 p R, giving

(VT1)/(VT)> = 2 p R1/(2 p R)

Canceling equal multipliers ("factors") on top and on bottom leaves

T1/T = R1/R

which turns out to be useful in the rest of the calculation. This is a general rule: given two equations, we may divide each side of one by one of the sides of the other. "After dividing equals by equals, the results remain equal".


Next Stop:   #M-4    Identities



Back to Index

Author and curator: David P. Stern

Last updated 25 February 1999


RETURN TO SPACE EDUCATORS' HANDBOOK HOME PAGE