Technical note Open Access
Modestino, Giuseppina
{ "@context": "https://schema.org/", "@id": "https://doi.org/10.15161/oar.it/76796", "@type": "ScholarlyArticle", "creator": [ { "@type": "Person", "affiliation": "INFN-Laboratori Nazionali di Frascati Via E. Fermi 40, Frascati, Italy", "name": "Modestino, Giuseppina" } ], "datePublished": "2016-02-17", "description": "<p>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.</p>", "headline": "Unconventional physical way for the orbital velocity evaluation", "identifier": "https://doi.org/10.15161/oar.it/76796", "image": "https://zenodo.org/static/img/logos/zenodo-gradient-round.svg", "inLanguage": { "@type": "Language", "alternateName": "eng", "name": "English" }, "keywords": [ "Orbital velocity", "Solar system", "INFN-16-03-LNF" ], "license": "https://creativecommons.org/licenses/by/4.0/", "name": "Unconventional physical way for the orbital velocity evaluation", "url": "https://www.openaccessrepository.it/record/76796" }
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