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Evolution and resonances in the rotational motion of a viscoelastic planet in an elliptical orbit - MaRDI portal

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Evolution and resonances in the rotational motion of a viscoelastic planet in an elliptical orbit (Q1314032)

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scientific article; zbMATH DE number 500801
Language Label Description Also known as
English
Evolution and resonances in the rotational motion of a viscoelastic planet in an elliptical orbit
scientific article; zbMATH DE number 500801

    Statements

    title
    Evolution and resonances in the rotational motion of a viscoelastic planet in an elliptical orbit (English)
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    author
    E. V. Sinitsyn
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    publication date
    2 March 1994
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    review text
    The rotational motion of a viscoelastic planet in the solar system is studied using the many-parameter model of the linear theory of viscoelasticity. The method of averaging is used to obtain the equations describing the evolution of plane rotational motion in the non-resonant and resonant cases. The limiting angular velocity and conditions for the existence of a stable resonant rotation are obtained as functions of the eccentricity and of the parameters characterizing the properties of the material of the planet.
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    zbMATH Keywords
    Kelvin-Voigt model
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    many-parameter model
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    method of averaging
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    stable resonant rotation
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    eccentricity
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    Identifiers

    zbMATH DE Number
    500801
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    OpenAlex ID
    W2040543065
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