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Unconventional physical way for the orbital velocity evaluation

Modestino, Giuseppina


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  "@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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