February 17, 2016 Technical note Open Access

Modestino, Giuseppina

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  <dc:creator>Modestino, Giuseppina</dc:creator>
  <dc:date>2016-02-17</dc:date>
  <dc:description>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.</dc:description>
  <dc:identifier>https://www.openaccessrepository.it/record/76796</dc:identifier>
  <dc:identifier>10.15161/oar.it/76796</dc:identifier>
  <dc:language>eng</dc:language>
  <dc:relation>doi:10.15161/oar.it/76795</dc:relation>
  <dc:relation>url:https://www.openaccessrepository.it/communities/infn</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by/4.0/</dc:rights>
  <dc:subject>Orbital velocity</dc:subject>
  <dc:subject>Solar system</dc:subject>
  <dc:subject>INFN-16-03-LNF</dc:subject>
  <dc:title>Unconventional physical way for the orbital velocity evaluation</dc:title>
  <dc:type>info:eu-repo/semantics/technicalDocumentation</dc:type>
  <dc:type>publication-technicalnote</dc:type>
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