## FANDOM

8 Pages

The geometric probability was calculated with the following formula:

$P = \frac{R_* + R_p}{a(1-e^2)}\frac{1}{1-e \cos(\pi - \omega)}$

If the parameters were unknown, the following values were used:

$R_* = R_{sun}$

$R_p = R_{jup}$

$e = 0$

$\omega = 0$

If a was unknown, the geometric transit probability was left blank.