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If a solar eclipse is visible near the equatorial region on the Earth, does it move from West to East at about 1000 miles/hr?
The velocity of the shadow of a solar eclipse at the equator is definitively 1000 miles per hour. This speed is consistent across solar eclipses visible near the equatorial region of the Earth. The discussion references a specific resource that provides further explanation of this phenomenon. For those interested in the mathematical calculations behind this speed, additional details are requested.
PREREQUISITESAstronomy enthusiasts, educators teaching about solar eclipses, and students studying the physics of celestial events will benefit from this discussion.