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Related Concept Videos

Kepler's First Law of Planetary Motion01:10

Kepler's First Law of Planetary Motion

In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. He formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe.
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
What is Evolutionary History?02:35

What is Evolutionary History?

Scientists record evolutionary history by analyzing fossil, morphological, and genetic data. The fossil record documents the history of life on Earth and provides evidence for evolution. However, both fossil and living organisms offer evidence that outlines Earth’s evolutionary history.Phylogenetic trees illustrate the evolutionary relationships among these organisms. Scientists infer organisms’ common ancestry by evaluating shared morphological and genetic characteristics. Together, the fossil...
Kepler's Second Law of Planetary Motion01:29

Kepler's Second Law of Planetary Motion

In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. His first law states that all planets orbit the Sun in an elliptical orbit, with the Sun at one of the ellipse's foci. Therefore, the distance of a planet from the Sun varies throughout its revolution around the Sun.
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Conservation of Angular Momentum: Application01:18

Conservation of Angular Momentum: Application

A system's total angular momentum remains constant if the net external torque acting on the system is zero. Examples of such systems include a freely spinning bicycle tire that slows over time due to torque arising from friction, or the slowing of Earth's rotation over millions of years due to frictional forces exerted on tidal deformations. However in the absence of a net external torque, the angular momentum remains conserved. The conservation of angular momentum principle requires a change...
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Related Experiment Video

Updated: Jul 12, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
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Published on: June 5, 2014

Chaotic evolution of the solar system.

G J Sussman, J Wisdom

    Science (New York, N.Y.)
    |July 3, 1992
    PubMed
    Summary

    The solar system

    Area of Science:

    • Planetary Science
    • Astrodynamics
    • Celestial Mechanics

    Background:

    • Understanding the long-term dynamical evolution of planetary systems is crucial for assessing their stability.
    • Previous studies suggested potential chaotic behavior in the solar system, but lacked comprehensive long-term numerical validation.

    Purpose of the Study:

    • To numerically integrate the evolution of the entire planetary system over 100 million years.
    • To confirm the chaotic nature of the solar system's evolution and quantify its timescale.
    • To investigate the dynamical behavior of the Jovian subsystem and Pluto.

    Main Methods:

    • Numerical integration of the gravitational interactions of all planets in the solar system.
    • Long-term simulation spanning approximately 100 million years.

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    Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
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    Published on: June 5, 2014

    Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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    Scattering And Absorption of Light in Planetary Regoliths
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  • Analysis of dynamical stability and divergence timescales.
  • Main Results:

    • The long-term evolution of the entire solar system is confirmed to be chaotic.
    • The calculated timescale for exponential divergence is approximately 4 million years.
    • The Jovian planet subsystem exhibits chaotic dynamics, with potential for quasiperiodic motion under specific model variations.
    • Pluto's orbital motion is robustly and independently chaotic.

    Conclusions:

    • The solar system's long-term evolution is inherently chaotic, underscoring the unpredictability of planetary positions over extended timescales.
    • The chaotic nature extends to the Jovian subsystem and Pluto, highlighting the complex gravitational interactions at play.
    • These findings have implications for understanding planetary system stability and the long-term fate of our solar system.