The path of a total solar eclipse is modeled by f(t) = 0.003851 -0.583t +31.194, 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 total eclipse will be visible. The latitude closest to the equator at which the total eclipse will be visible is 's (Round the final answer to two decimal places as needed. Round all intermediate values to four decimal places as needed.)

The path of a total solar eclipse is modeled by f(t) = 0.003851 -0.583t +31.194, 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 total eclipse will be visible. The latitude closest to the equator at which the total eclipse will be visible is 's (Round the final answer to two decimal places as needed. Round all intermediate values to four decimal places as needed.)

College Algebra

10th Edition

ISBN:9781337282291

Author:Ron Larson

Publisher:Ron Larson

Chapter5: Exponential And Logarithmic Functions

Section: Chapter Questions

Problem 39CT: The population P (in millions) of Texas from 2001 through 2014 can be approximated by the model...

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