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 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">Russian Journal of Earth Sciences</journal-id>
   <journal-title-group>
    <journal-title xml:lang="en">Russian Journal of Earth Sciences</journal-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Russian Journal of Earth Sciences</trans-title>
    </trans-title-group>
   </journal-title-group>
   <issn publication-format="online">1681-1208</issn>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="publisher-id">46600</article-id>
   <article-categories>
    <subj-group subj-group-type="toc-heading" xml:lang="ru">
     <subject>ОРИГИНАЛЬНЫЕ СТАТЬИ</subject>
    </subj-group>
    <subj-group subj-group-type="toc-heading" xml:lang="en">
     <subject>ORIGINAL ARTICLES</subject>
    </subj-group>
    <subj-group>
     <subject>ОРИГИНАЛЬНЫЕ СТАТЬИ</subject>
    </subj-group>
   </article-categories>
   <title-group>
    <article-title xml:lang="en">Re-distribution of the planetary material between the Sun and giant planets at the process of the terrestrial planets formation</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Re-distribution of the planetary material between the Sun and giant planets at the process of the terrestrial planets formation</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Anfilogov</surname>
       <given-names>V N</given-names>
      </name>
      <name xml:lang="en">
       <surname>Anfilogov</surname>
       <given-names>V N</given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Institute of Mineralogy of the Ural Division of RAS</institution>
     <country>ru</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Mineralogy of the Ural Division of RAS</institution>
     <country>ru</country>
    </aff>
   </aff-alternatives>
   <volume>16</volume>
   <issue>1</issue>
   <fpage>1</fpage>
   <lpage>5</lpage>
   <history>
    <date date-type="received" iso-8601-date="2021-10-29T12:52:40+03:00">
     <day>29</day>
     <month>10</month>
     <year>2021</year>
    </date>
   </history>
   <self-uri xlink:href="https://rjes.ru/en/nauka/article/46600/view">https://rjes.ru/en/nauka/article/46600/view</self-uri>
   <abstract xml:lang="ru">
    <p>The mathematical approximation of the relation for the distances of planets from the Sun and distribution of the planet masses in the Solar system are represented. It is shown that the planetary distances from the Sun can be accurately described by the logarithmic spiral equation. The same relation is established for the four biggest satellites of the Jupiter. The relationship between the masses of the terrestrial planets and their distance from the Sun. is described by the parabola equation. This relationship for the outer planets of the Solar system is described by hyperbola equation. These data allow us to conclude, that the big gaseous planets were formed on the terrestrial planets position on the beginning stage. The gaseous components of these planets were redistributed between the Sun and the Jupiter on the next stage and the terrestrial planets were formed from residual material. There are three hypotheses, which can be used for the new models of formation of the planetary systems. Hypothesis 1. Besides molecular clouds there is another source of material, from which stars and planet systems forms. Hypothesis 2. Protosolar cloud can have form high temperature plasma jet. Hypothesis 3. The jet of plasma can roll up in the spiral whirl in which a material moves towards the pole of the spiral where the central star forms.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>The mathematical approximation of the relation for the distances of planets from the Sun and distribution of the planet masses in the Solar system are represented. It is shown that the planetary distances from the Sun can be accurately described by the logarithmic spiral equation. The same relation is established for the four biggest satellites of the Jupiter. The relationship between the masses of the terrestrial planets and their distance from the Sun. is described by the parabola equation. This relationship for the outer planets of the Solar system is described by hyperbola equation. These data allow us to conclude, that the big gaseous planets were formed on the terrestrial planets position on the beginning stage. The gaseous components of these planets were redistributed between the Sun and the Jupiter on the next stage and the terrestrial planets were formed from residual material. There are three hypotheses, which can be used for the new models of formation of the planetary systems. Hypothesis 1. Besides molecular clouds there is another source of material, from which stars and planet systems forms. Hypothesis 2. Protosolar cloud can have form high temperature plasma jet. Hypothesis 3. The jet of plasma can roll up in the spiral whirl in which a material moves towards the pole of the spiral where the central star forms.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>Planetary system</kwd>
    <kwd>terrestrial planets</kwd>
    <kwd>distances of the planet from the Sun</kwd>
    <kwd>distribution of mass in the Solar system</kwd>
    <kwd>planet formation</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>Planetary system</kwd>
    <kwd>terrestrial planets</kwd>
    <kwd>distances of the planet from the Sun</kwd>
    <kwd>distribution of mass in the Solar system</kwd>
    <kwd>planet formation</kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <p></p>
 </body>
 <back>
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