International Journal of Astronomy and Astrophysics

Volume 3, Issue 4 (December 2013)

ISSN Print: 2161-4717   ISSN Online: 2161-4725

Google-based Impact Factor: 0.78  Citations  h5-index & Ranking

Proposal of New Criteria for Celestial Mechanics

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DOI: 10.4236/ijaa.2013.34044    5,767 Downloads   9,195 Views  Citations
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ABSTRACT

Based on a new interpretation on the behavior of rigid bodies exposed to simultaneous non-coaxial rotations, we have developed a hypothesis: the Theory of Dynamics Interactions, which can be applied to understand celestial mechanics. We have analyzed the velocity and acceleration fields generated in a rigid body with intrinsic angular momentum, when exposed to successive torques, to assess new criteria for this speeds coupling. In this context, reactions and inertial fields take place, which cannot be justified by means of classical mechanics. We believe that the results obtained after the analysis of dynamics fields systems accelerated by rotation will allow us to conceive a new perspective in celestial dynamics, astrometry, stellar dynamics and galactic astronomy, unknown up to date. After carrying out ample research, we have come to the conclusion that there still exists an unstructured scientific area under the present general assumptions and, more specifically, in the area of dynamic systems submitted to rotational accelerations. The aim of this paper is to present information of the surprising results obtained, and to attract the interest towards the investigation of this new area of knowledge in rotational non-inertial dynamics, and its multiple and remarkable scientific applications.

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Barceló, G. (2013) Proposal of New Criteria for Celestial Mechanics. International Journal of Astronomy and Astrophysics, 3, 385-391. doi: 10.4236/ijaa.2013.34044.

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[5] The Dance of the Spinning Top
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[7] The Pendulum of Dynamic Interactions
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[8] Theory of Dynamic Interactions: The Flight of the Boomerang
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[9] Dynamic Interaction Confinement
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[10] On Motion, Its Relativity and the Equivalence Principle
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[11] Dynamic Interactions in the Atmosphere
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