Brother Moses_Young,
All I am saying is that the sun rises on Jerusalem, in the east, to an altitude of around 28.65 statute miles above sea level when it gets due south of Jerusalem. Then from there it starts going down, all the way until it sets in the west, on Jerusalem, at an altitude of around 7.83 statute miles above sea level. From there it continues over the north at that altitude until it gets to the east again, where it rises on Jerusalem again. The moon and the stars that run their courses near the sun also have similar altitudes.
And the math for the altitude of the sun comes from reverse engineering the heliocentric model. The line of light from the edge of the sun to the Geographical North Pole, on the equinox, is the hypotenuse side of the right triangle. The perpendicular line - to the line going through the center of a sphere world from the Geographical North Pole to the Geographical South Pole - from the Geographical North Pole to where it intersects the sun, on the equinox, is the adjacent side of the right triangle. Then since the world is flat, the length of the adjacent side of the right triangle is 6,214.209 statute miles - the distance from the Geographical North Pole to the equator - and since you know the angle of elevation to the top of the seen sun from the horizon, you just solve for the opposite side of the right triangle, that is the height of the sun above the world, on the equinox, on the Longitude 035.23474576724° E line, when it is due south of Jerusalem.
The formula is:
opposite = tan(angle) × adjacent
You then just multiply that answer, 28.6467 statute miles by 0.2732395447, the percent the distance from the Geographical North Pole to the north Geographical South Pole is of the distance from the Geographical North Pole to the south Geographical South Pole, to get 7.8274 statute miles.
Glory to God.
All I am saying is that the sun rises on Jerusalem, in the east, to an altitude of around 28.65 statute miles above sea level when it gets due south of Jerusalem. Then from there it starts going down, all the way until it sets in the west, on Jerusalem, at an altitude of around 7.83 statute miles above sea level. From there it continues over the north at that altitude until it gets to the east again, where it rises on Jerusalem again. The moon and the stars that run their courses near the sun also have similar altitudes.
And the math for the altitude of the sun comes from reverse engineering the heliocentric model. The line of light from the edge of the sun to the Geographical North Pole, on the equinox, is the hypotenuse side of the right triangle. The perpendicular line - to the line going through the center of a sphere world from the Geographical North Pole to the Geographical South Pole - from the Geographical North Pole to where it intersects the sun, on the equinox, is the adjacent side of the right triangle. Then since the world is flat, the length of the adjacent side of the right triangle is 6,214.209 statute miles - the distance from the Geographical North Pole to the equator - and since you know the angle of elevation to the top of the seen sun from the horizon, you just solve for the opposite side of the right triangle, that is the height of the sun above the world, on the equinox, on the Longitude 035.23474576724° E line, when it is due south of Jerusalem.
The formula is:
opposite = tan(angle) × adjacent
You then just multiply that answer, 28.6467 statute miles by 0.2732395447, the percent the distance from the Geographical North Pole to the north Geographical South Pole is of the distance from the Geographical North Pole to the south Geographical South Pole, to get 7.8274 statute miles.
Glory to God.
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