How Seasons Work on Flat Earth

In the Flat-Earth model, the Sun and Moon luminaries revolve around the Earth once every 24 hours illuminating like spotlights the areas over which they pass. The Sun’s annual journey from tropic to tropic, solstice to solstice, is what determines the length and character of days, nights and seasons. This is why equatorial regions experience almost year-round summer and heat while higher latitudes North and especially South experience more distinct seasons with harsh winters. The heliocentric model claims seasons change based on the ball-Earth’s alleged “axial tilt” and “elliptical orbit” around the Sun. Their flawed current model even places us closest to the Sun (91,400,000 miles) in January when its actually winter, and farthest from the Sun (94,500,000 miles) in July when its actually summer throughout much of the Earth. They say due to the ball-Earth’s tilt, different places receive different amounts of direct sunlight and that is what produces the seasonal and temperature changes. This makes little sense, however, because if the Sun’s heat travels over ninety million miles to reach the ball-Earth, how could a slight tilt, a mere few thousand miles maximum, negate the Sun’s ninety million mile journey, giving us simultaneous tropical summers and Antarctic winters?

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