Orbital velocity
Giuseppina Modestino
TL;DR
This paper derives the trajectory and orbital velocity of objects in gravitational systems, illustrating Keplerian laws and applying the analysis to solar system planets.
Contribution
It provides a fundamental derivation of orbital parameters based on independent variables, emphasizing the natural tracing of elliptical orbits.
Findings
Elliptical orbits naturally arise from the analysis
Verification of Keplerian laws
Application to solar system planets
Abstract
The trajectory and the orbital velocity are determined for an object moving in a gravitational system, in terms of fundamental and independent variables. In particular, considering a path on equipotential line, the elliptical orbit is naturally traced, verifying evidently the keplerian laws. The case of the planets of the solar system is presented.
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Taxonomy
TopicsRelativity and Gravitational Theory · Geophysics and Gravity Measurements · Astro and Planetary Science