February 17, 2016 Technical note Open Access

Modestino, Giuseppina

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  <identifier identifierType="DOI">10.15161/oar.it/76796</identifier>
  <creators>
    <creator>
      <creatorName>Modestino, Giuseppina</creatorName>
      <givenName>Giuseppina</givenName>
      <familyName>Modestino</familyName>
      <affiliation>INFN-Laboratori Nazionali di Frascati Via E. Fermi 40, Frascati, Italy</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Unconventional physical way for the orbital velocity evaluation</title>
  </titles>
  <publisher>INFN Open Access Repository</publisher>
  <publicationYear>2016</publicationYear>
  <subjects>
    <subject>Orbital velocity</subject>
    <subject>Solar system</subject>
    <subject>INFN-16-03-LNF</subject>
  </subjects>
  <dates>
    <date dateType="Issued">2016-02-17</date>
  </dates>
  <language>en</language>
  <resourceType resourceTypeGeneral="Text">Technical note</resourceType>
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    <rights rightsURI="https://creativecommons.org/licenses/by/4.0/">Creative Commons Attribution 4.0</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
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  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;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.&lt;/p&gt;</description>
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