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Uniform Circular Motion01:14

Uniform Circular Motion

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Uniform circular motion is a specific type of motion in which an object travels in a circle with a constant speed. For example, any point on a propeller spinning at a constant rate is undergoing uniform circular motion. The second, minute, and hour hands of a watch also undergo uniform circular motion. It is hard to believe that points on these rotating objects are actually accelerating, even though the rotation rate is constant. To understand this, we must analyze the motion in terms of...
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Apparent Weight and the Earth's Rotation01:28

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Since all objects on the Earth's surface move through a circle every 24 hours, there must be a net centripetal force on each object, directed towards the center of that circle. The points of the north and south poles are the only exception to this rule.
For an object on the Earth's equator, the net centripetal force that accounts for its rotation is the Earth's pull towards its center, or the weight minus the normal force that prevents it from piercing into the Earth's surface....
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Inertial Frames of Reference01:03

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Newton’s first law is usually considered to be a statement about reference frames. It provides a method for identifying a special type of reference frame: the inertial reference frame. In principle, we can make the net force on a body zero. If its velocity relative to a given frame is constant, then that frame is said to be inertial. So, by definition, an inertial reference frame is a reference frame where Newton's first law holds valid. Newton's first law applies to objects with...
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Variation in Acceleration due to Gravity near the Earth's Surface01:20

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An object's apparent weight is its weight measured by a spring balance at its location. It is different from its true weight, the force with which the Earth pulls it, because of the Earth's rotation. Mathematically, an object's apparent weight equals its true weight minus the centripetal force that keeps it in a circular motion along with the Earth's surface every 24 hours.
The difference between the true and apparent weights is proportional to the square of the Earth's...
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Reduced Mass Coordinates: Isolated Two-body Problem01:12

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In classical mechanics, the two-body problem is one of the fundamental problems describing the motion of two interacting bodies under gravity or any other central force. When considering the motion of two bodies, one of the most important concepts is the reduced mass coordinates, a quantity that allows the two-body problem to be solved like a single-body problem. In these circumstances, it is assumed that a single body with reduced mass revolves around another body fixed in a position with an...
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Gyroscope: Precession01:24

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Precession can be demonstrated effectively through a spinning top. If a spinning top is placed on a flat surface near the surface of the Earth at a vertical angle and is not spinning, it will fall over due to the force of gravity producing a torque acting on its center of mass. However, if the top is spinning on its axis, it precesses about the vertical direction, rather than topple over due to this torque. Precessional motion is a combination of a steady circular motion of the axis and the...
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Inertial motion on the earth's spheroidal surface.

Boyd F Edwards1, Cade Pankey1, John M Edwards2

  • 1Department of Physics, Utah State University, Logan, Utah 84322, USA.

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|December 1, 2022
PubMed
Summary

Earth's spheroidal shape neutralizes centrifugal force, leaving the Coriolis force to govern inertial motion. This study classifies all inertial motion types, including new circumpolar waves, and provides approximations for their behavior.

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Area of Science:

  • Geophysics
  • Classical Mechanics
  • Fluid Dynamics

Background:

  • Earth's rotation influences motion via Coriolis and centrifugal forces.
  • Previous models often simplified Earth as a sphere, neglecting its spheroidal shape's impact.
  • Latitude-dependent equations of motion can become highly nonlinear.

Purpose of the Study:

  • To derive and justify equations of motion for objects on a rotating spheroid.
  • To identify, classify, and describe all classes of inertial motion.
  • To introduce and illustrate a new class of motion: circumpolar waves.

Main Methods:

  • Derivation of weakly spheroidal equations of motion.
  • Analysis of rotational/time-reversal symmetry.
  • Development and validation of closed-form small-amplitude approximations.
  • Utilizing Coriolis visualization software (CorioVis).

Main Results:

  • Identification of five classes of inertial motion, including circumpolar waves.
  • Classification and description of each motion class.
  • Calculation of frequencies, zonal drifts, and latitude ranges for validated approximations.
  • Demonstration of circumpolar waves encircling both poles.

Conclusions:

  • Earth's spheroidal deformations are crucial for accurately modeling inertial motion.
  • The study provides a comprehensive framework for understanding inertial motion on Earth.
  • New insights into circumpolar waves and validated approximations offer predictive capabilities for geophysical phenomena.