The altitude h to the directly overhead sun midline, with r factored out, is given by:
h = r_earth * ( SQRT(1 + sin^2 theta) -1) Given time after sunset t we have:theta = (t/(8.64x10^4 s))*(2*Pi) radians = (t/(1440 min))*(2*Pi) radians
Earth radius, r_earth, at Hawaii is about 3951 mi. Here are some numbers:
t (min) theta (radians) h (miles)
1 0.00436331944 0.03760073165
5 0.02181659722 0.93976780755
10 0.04363319444 3.75594358
20 0.08726638889 14.973936498
30 0.13089958333 33.506081478
60 0.26179916667 130.1553394
90 0.39269875 279.3533269
Since the above is time after total sunset, you don't have to correct
for the angular width of the sun. However, even total sunset is not
good enough to black out an object though, due to light
diffraction. Clearly not enough time, i.e. "shortly after sunset",
passed to rule out an airplane.
<<inline: Umbra.jpg>>
Best regards, Horace Heffner http://www.mtaonline.net/~hheffner/

