The Path Of A Total Solar Eclipse Is Modeled By F 00007 56 37743 The Aude In Degress Of The Stor Att Minces After The S 1 (6.72 KiB) Viewed 14 times
The Path Of A Total Solar Eclipse Is Modeled By F 00007 56 37743 The Aude In Degress Of The Stor Att Minces After The S 2 (20.83 KiB) Viewed 14 times
The Path Of A Total Solar Eclipse Is Modeled By F 00007 56 37743 The Aude In Degress Of The Stor Att Minces After The S 3 (20.83 KiB) Viewed 14 times
The path of a total solar eclipse is modeled by f-00007²-56-37743 the aude in degress of the stor att minces after the start of the sale What is the aude closest to the edges at which The uue to the equator in which the titleen wit be visie Round the final anewer to two decimal places as needed Round at intermediata vaas to four decimal places as needed) C
The path of a total solar eclipse is modeled by f(t)=0.0027512 -0.4611+37.743, 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.)
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