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Reduced Mass Coordinates: Isolated Two-body Problem01:12

Reduced Mass Coordinates: Isolated Two-body Problem

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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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Dynamics of Circular Motion01:30

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An object undergoing circular motion, like a race car, is accelerating because it is changing the direction of its velocity. This centrally directed acceleration is called centripetal acceleration. This acceleration acts along the radius of the curved path (thus is also referred to as radial acceleration).
Any acceleration must be produced by some force. Therefore, any force or combination of forces can cause centripetal acceleration. A few examples include the tension in the rope on a...
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Principle of Angular Impulse and Momentum: Problem Solving01:19

Principle of Angular Impulse and Momentum: Problem Solving

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Consider a ball of mass m, attached to a massless rod of known length, subjected to a time-dependent torque. If the initial velocity of the mass is known, then the final velocity of the mass for time t can be determined using the principle of angular impulse and momentum.
Initially, a free-body diagram of the system is drawn to illustrate all the forces acting upon the system, providing a crucial understanding of the dynamics at play. Then, the principle of angular impulse and momentum is...
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First Law: Particles in Two-dimensional Equilibrium01:18

First Law: Particles in Two-dimensional Equilibrium

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Recall that a particle in equilibrium is one for which the external forces are balanced. Static equilibrium involves objects at rest, and dynamic equilibrium involves objects in motion without acceleration; but it is important to remember that these conditions are relative. For instance, an object may be at rest when viewed from one frame of reference, but that same object would appear to be in motion when viewed by someone moving at a constant velocity.
Newton's first law tells us about...
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Dynamics Of Circular Motion: Applications01:17

Dynamics Of Circular Motion: Applications

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Suppose a car moves on flat ground and turns to the left. The centripetal force causing the car to turn in a circular path is due to friction between the tires and the road. For this, a minimum coefficient of friction is needed, or the car will move in a larger-radius curve and leave the roadway. Let's now consider banked curves, where the slope of the road helps in negotiating the curve. The greater the angle of the curve, the faster one can take the curve. It is common for race tracks for...
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Euler Equations of Motion01:19

Euler Equations of Motion

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Imagine a rigid body that is rotating at an angular velocity of ω within an inertial frame of reference. Along with this, picture a second rotating frame that is attached to the body itself. This frame moves along with the body and possesses an angular velocity of Ω. The total moment about the center of mass is calculated by adding the rate of change of angular momentum about the center of mass in relation to the rotating frame and the cross-product of the body's angular velocity...
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Related Experiment Video

Updated: Sep 10, 2025

Impacts of Free-falling Spheres on a Deep Liquid Pool with Altered Fluid and Impactor Surface Conditions
08:49

Impacts of Free-falling Spheres on a Deep Liquid Pool with Altered Fluid and Impactor Surface Conditions

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Chaotic dynamics for the two-body problem on a sphere.

Sergey Bolotin1

  • 1Steklov Mathematical Institute of Russian Academy of Sciences, Moscow, Russia.

Chaos (Woodbury, N.Y.)
|August 25, 2025
PubMed
Summary

This study proves chaotic trajectories exist for the two-body problem on a sphere, featuring near-collisions similar to Poincaré

Area of Science:

  • Celestial Mechanics and Dynamical Astronomy
  • Mathematical Physics
  • Differential Geometry

Background:

  • The classical two-body problem typically exhibits regular, predictable motion.
  • Chaotic dynamics are well-established in the three-body problem, particularly Poincaré's second species solutions.
  • Investigating chaotic behavior in simplified systems like the spherical two-body problem offers insights into complex dynamics.

Purpose of the Study:

  • To demonstrate the existence of chaotic trajectories for the two-body problem specifically on a sphere.
  • To construct and characterize these chaotic trajectories, noting their similarity to known complex systems.
  • To apply advanced mathematical techniques to prove the existence of such phenomena.

Main Methods:

  • Utilizing a general result for Lagrangian systems with Newtonian potential singularities.

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Last Updated: Sep 10, 2025

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Experimental Measurement of Settling Velocity of Spherical Particles in Unconfined and Confined Surfactant-based Shear Thinning Viscoelastic Fluids
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  • Employing the anti-integrable limit method, pioneered by Serge Aubry.
  • Constructing specific trajectories that exhibit chaotic properties and near-collision behavior.
  • Main Results:

    • Existence of chaotic trajectories for the two-body problem on a sphere is rigorously proven.
    • The constructed trajectories exhibit characteristics of near-collisions.
    • These chaotic trajectories bear resemblance to Poincaré's second species solutions in the three-body problem.

    Conclusions:

    • Chaotic dynamics can arise in simplified gravitational systems like the spherical two-body problem.
    • The methods used provide a framework for studying chaos in systems with potential singularities.
    • This work extends our understanding of chaotic phenomena in celestial mechanics.