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Comet Bennett 1970 II.

Z Sekanina, F D Miller

    Science (New York, N.Y.)
    |February 9, 1973
    PubMed
    Summary
    This summary is machine-generated.

    The Finson and Probstein dust comet model was successfully applied to Comet Bennett, providing new insights into dust particle characteristics. This study details the size distribution, emission rate, and initial velocities of dust from the comet

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    Area of Science:

    • Cometary Science
    • Dust Dynamics
    • Astrophysics

    Background:

    • The Finson and Probstein model is a key tool for understanding dust comets.
    • Previous validation was limited to Comet Arend-Roland (1957 III).
    • Comet Bennett provides a new subject for model application.

    Purpose of the Study:

    • To apply the Finson and Probstein dust comet model to Comet Bennett.
    • To determine the physical characteristics of dust particles emitted from Comet Bennett.
    • To validate the model's applicability to a new cometary body.

    Main Methods:

    • Utilized three calibrated photographic plates of Comet Bennett.
    • Applied the Finson and Probstein dust comet model.
    • Analyzed dust particle size distribution, emission rate, and initial velocities.

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    Main Results:

    • Successfully applied the Finson and Probstein model to Comet Bennett data.
    • Determined the size distribution of dust particles.
    • Quantified the emission rate and initial velocities of dust particles from the nucleus.

    Conclusions:

    • The Finson and Probstein model is effective for analyzing dust comets.
    • Comet Bennett's dust characteristics have been quantified.
    • The study expands the validation of the dust comet model.