Table of contents
- 0. Review of College Algebra4h 43m
- 1. Measuring Angles39m
- 2. Trigonometric Functions on Right Triangles2h 5m
- 3. Unit Circle1h 19m
- 4. Graphing Trigonometric Functions1h 19m
- 5. Inverse Trigonometric Functions and Basic Trigonometric Equations1h 41m
- 6. Trigonometric Identities and More Equations2h 34m
- 7. Non-Right Triangles1h 38m
- 8. Vectors2h 25m
- 9. Polar Equations2h 5m
- 10. Parametric Equations1h 6m
- 11. Graphing Complex Numbers1h 7m
3. Unit Circle
Defining the Unit Circle
Problem 3.45a
Textbook Question
Textbook QuestionFind the linear speed v for each of the following.
a point on the equator moving due to Earth's rotation, if the radius is 3960 mi
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Key Concepts
Here are the essential concepts you must grasp in order to answer the question correctly.
Linear Speed
Linear speed refers to the distance traveled per unit of time. In the context of circular motion, it can be calculated using the formula v = d/t, where d is the distance traveled along the circular path and t is the time taken. For a point on the equator, this speed is determined by the circumference of the Earth and the time it takes for one complete rotation.
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Circumference of a Circle
The circumference of a circle is the total distance around it, calculated using the formula C = 2πr, where r is the radius. For the Earth, with a radius of 3960 miles, the circumference provides the distance a point on the equator travels in one complete rotation. This value is essential for determining the linear speed of a point on the equator.
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Earth's Rotation Period
The Earth's rotation period is the time it takes for the Earth to complete one full rotation on its axis, approximately 24 hours. This period is crucial for calculating linear speed, as it serves as the time variable in the speed formula. Understanding this concept allows us to relate the distance traveled (circumference) to the time taken, yielding the linear speed of a point on the equator.
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