By Steve Dinh, a.k.a. Võ Đức Diên
I am taking the opportunity to write a phenomenon about the moon as I have been asked by many readers on why the moon appears to be round at full-moon and at other times it does not.
So the question is that whether the moon is ever perfectly round? The roundness I am talking about here is its illumination at the “full” moon and not its physical shape as we have already known or assumed that it shape is already round. The perfect roundness, by mathematical and geometrical definition, is 100% perfectly round. The general understanding thus far by humans is that the moon is perfectly round at full moon and not at 0.098… % percent round as it is about to be proven mathematically. While proving the illumination is not 100% round at full-moon we assume that its shape is already 100% round. Astronomically speaking, the moon illumination is never round because its shape is never perfectly round physically.
The calculations below are based on the assumption that the moon is 100% round physically and that there are no craters or rough areas on its surface.
The moon, as we have known, gets the sunlight from the Sun and, assuming that it’s 100% physically round, half of its surface is always illuminated. Basically, its illumination is always round unless when the earth blocks the sunlight from getting to it.
But humans on earth are never in a perfect position to see the total sunlight on the moon. Even on a full-moon, our eyes see the illumination almost perfectly whereas our calculations suggest otherwise. As a matter of fact, in order to see the moon light being 100% round, one has to position himself on the line connecting the centers of the sun and the moon. If a human is able to be in this position, the moon will be totally eclipsed by the earth, and thus there is no light on the moon to be seen instead of the round moon illumination.
We are looking at a scenario above when the there is a single ray of sun light which tangents both the earth and the moon. This can happen in real life although it is extremely rare. In such a situation if there is a person at position J which is at a time when the sun is setting down or rising up, that person will see the moon at an angle which is largest and with the highest illumination. Indeed, you will see the illumination of the moon at a smaller angle and less illumination if you are somewhere else. Basically, the best scenario is for a person to position at J.
The area colored green on the moon is the area where the illumination can not be seen by the person even positioning at J on earth. That person can only see the illumination on arc from C to B. Now we can find the angle α, phase angle β and distance from C to B in this case.
Let r be the radius of the moon, R the radius of the earth, d is the shortest distance from the surface of the earth to that of the moon, we have:
Two triangles OBI and O’JI are similar, hence
= = (1)
EF = d is the distance from the earth to the moon, we have
OO’ = OI + IO’ = r + d + R (2)
From (1) and (2), we have OI (1 + ) = r + d + R
Or OI =
From there BI =
BI =
Also from (1) JI = ; therefore,
BJ = BI + JI = BI (1 + ) = (1 + )
We also have OJ orthogonal to CB and BJ orthogonal to AB, and therefore the two triangles OBJ and ACB also similar, and we have
=
Therefore, CB = (3)
But OJ² = r² + BJ²
Or OJ² = r² + (1 + )²[]
AB = 2r, from (3) we have
CB = 2r(1 + )/
Substituting in their values to get
r = 1737 km
R = 6371 km
d = 384000 km
into the equation of CB we have CB = 3473.97 km.
And we have found the distance CB of the area of illumination which a person at position J can see. The remaining illuminated area colored green is the area we can not see has the distance AC.
Now let’s find the phase angle β.
OJ is the bisector of angle CJB and the phase angle β on triangle ABC equals angle OJB and equals half angle α,
β = α
sinβ =
From there we find angle β = arcsine
β = arcsine{r/}
Again substituting in their values and we get β = 0.28°.
The area we can not see k has the distance equals the diameter of the moon subtracted from CB, or
k = 2r – 2r(1 + )/
or k = 34.10 m.
Therefore, we can conclude that the illumination we can see on a full-moon is not perfectly round, and its phase angle is 0.28°. Its percentage compared to the diameter of the moon is = 0.098 %
Attention: Wikipedia.com also gives data about the phase angle of the moon but did not offer a calculation or an explanation.