Here are the essential concepts you must grasp in order to answer the question correctly.
Rotational Speed
Rotational speed refers to how fast an object rotates around an axis. For Earth, this speed varies with latitude; points on the equator move faster than those near the poles due to the Earth's spherical shape. The rotational speed can be calculated using the formula v = ωr, where v is linear speed, ω is angular velocity, and r is the radius of the circular path.
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Latitude and its Effect on Speed
Latitude is a geographic coordinate that specifies the north-south position of a point on the Earth's surface. As latitude increases from the equator to the poles, the circumference of the Earth decreases, resulting in a lower linear speed for objects at higher latitudes. For example, a student in Miami, located at 26 degrees latitude, will have a different rotational speed compared to someone at the equator.
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Centrifugal Force
Centrifugal force is an apparent force that acts outward on a body moving around a center, arising from the body's inertia. As the Earth rotates, this force affects objects on its surface, including a physics student in Miami. While this force is not directly responsible for the speed calculation, it is important to understand the dynamics of motion on a rotating body like Earth.
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