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The path of a total solar eclipse is modeled by f(t) = 0.00393t2 - 0.528t + 30.206. where f(t) is the latitude in degrees south of the equator at t minutes after the start of the total eclipse. What is the latitude closest to the equator, in degrees, at which the tolal eclipse will be visible. \"-CE)~~ Thelatitude closest to the equator at which the total eclipse will be visible is E]S. (Round the nal answer to two decimal places as needed. Round all intermediate values to four decimal places as needed.)