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Flat Earth Theory / Re: The moon
« on: February 14, 2018, 08:32:25 PM »
Tom, I think you missed you the part of this thread where I provided empirical observational evidence that Euclid's ideas of geometry and perspective are functional at a distance of 3000 miles.
The observable fact that the percentage of totality of a solar eclipse is proportional to the distance from the path totality it is observed from, fully supports Euclid geometry and perspective. It shows that angle the eclipse being observed from is not the same for all observers. It looks like this:
The moon appears to be observed from basically the same angle, that is the same side is presented, to all observers regardless of the distance of separation between them.
If the angle the eclipse is observed at is NOT the same for all observers, how can the angle the moon is observed at BE the same for all observers???
Please review the diagram and explain if geometry and perspective doesn't work for points thousands of miles distant from each other:
How is it that distant observers can all look up and observe the moon surfaces at the same angle but at the same exact moment in time observe that moon occlude the sun at different angles proportional to their distance from a median line extended from the center of the solar object, through the center of the lunar object and terminating on the ground?
The observable fact that the percentage of totality of a solar eclipse is proportional to the distance from the path totality it is observed from, fully supports Euclid geometry and perspective. It shows that angle the eclipse being observed from is not the same for all observers. It looks like this:
The moon appears to be observed from basically the same angle, that is the same side is presented, to all observers regardless of the distance of separation between them.
If the angle the eclipse is observed at is NOT the same for all observers, how can the angle the moon is observed at BE the same for all observers???
Please review the diagram and explain if geometry and perspective doesn't work for points thousands of miles distant from each other:
How is it that distant observers can all look up and observe the moon surfaces at the same angle but at the same exact moment in time observe that moon occlude the sun at different angles proportional to their distance from a median line extended from the center of the solar object, through the center of the lunar object and terminating on the ground?