<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">OALibJ</journal-id><journal-title-group><journal-title>Open Access Library Journal</journal-title></journal-title-group><issn pub-type="epub">2333-9705</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/oalib.1102554</article-id><article-id pub-id-type="publisher-id">OALibJ-69127</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Biomedical&amp;Life Sciences</subject><subject> Business&amp;Economics</subject><subject> Chemistry&amp;Materials Science</subject><subject> Computer Science&amp;Communications</subject><subject> Earth&amp;Environmental Sciences</subject><subject> Engineering</subject><subject> Medicine&amp;Healthcare</subject><subject> Physics&amp;Mathematics</subject><subject> Social Sciences&amp;Humanities</subject></subj-group></article-categories><title-group><article-title>
 
 
  On the Intrinsic Precession of the Perihelion of Planets of the Solar System
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Barbaro</surname><given-names>Quintero-Leyva</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>119 SW 6th Ave., Miami, FL 33130, USA</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>doserate2002@yahoo.com</email></corresp></author-notes><pub-date pub-type="epub"><day>31</day><month>03</month><year>2016</year></pub-date><volume>03</volume><issue>03</issue><fpage>1</fpage><lpage>5</lpage><history><date date-type="received"><day>3</day>	<month>March</month>	<year>2016</year></date><date date-type="rev-recd"><day>accepted</day>	<month>20</month>	<year>March</year>	</date><date date-type="accepted"><day>25</day>	<month>March</month>	<year>2016</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
   
   By analytically solving a corrected balance between the force given by the Newton’s 2
   <sup style="line-height:1.5;">nd</sup>
    law and the Newton gravitational force in polar coordinates, an equation for the intrinsic (
   i.e.
    two-body problem) perihelion precession of the planets of the solar system was obtained that when the Kepler’s 3
   <sup style="line-height:1.5;">rd</sup>
    law is applied it coincides with the equation resulting from Einstein GTR. 
  
 
</p></abstract><kwd-group><kwd>Celestial Mechanics</kwd><kwd> Newtonian Gravitation</kwd><kwd> Newton’s 2nd Law</kwd><kwd> Theory of Relativity</kwd><kwd> Perihelion Precession</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The motivation of this paper was to find out if the modification to the balance between the force given by the Newton’s 2<sup>nd</sup> law and the Newton gravitational force introduced in [<xref ref-type="bibr" rid="scirp.69127-ref1">1</xref>] , to account for the perihelion precession of Mercury, is applicable to the rest of the planets of the solar system. One importance of this work is that the differential equations obtained for the law of motion are very simple (when compared, for example, to the GTR) which could have a positive impact on the computational efficiency when solving more complicated problems (e.g. the N-body problem for evolution calculations). Other importance is related with the fact that the modification of the ODEs involves only the use of a power of the ubiquitous Lorentz factor which could suggests that a kind of extension of the special theory of relativity and/or electron theory to gravitational problems could be made without assuming more-difficult-to-measure concepts (e.g. a curved space-time). Another importance related with this work could be its potential impact on, for example, current or future gravitational problems or projects.</p><p>The correction to the balance between the force given by Newton’s 2<sup>nd</sup> law and Newtonian gravitation, to account for the intrinsic perihelion precession of Mercury in 3D Cartesian geometry, introduced in [<xref ref-type="bibr" rid="scirp.69127-ref1">1</xref>] could be written, for the two-body problem with a static Sun, as</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x6.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x7.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x8.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x9.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x10.png" xlink:type="simple"/></inline-formula></p><p>where</p><p>G is the Newton universal gravitational constant</p><p>M is the mass of the Sun</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x11.png" xlink:type="simple"/></inline-formula>: The speed of the gravitational interaction (assumed to be equal to the speed of light in vacuum: c)</p><p>The equation of motion in the Heliocentric coordinate system [<xref ref-type="bibr" rid="scirp.69127-ref2">2</xref>] , considering that correction factor, is written as</p><disp-formula id="scirp.69127-formula1047"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/69127x12.png"  xlink:type="simple"/></disp-formula><p>Equation (1) was solved numerically in [<xref ref-type="bibr" rid="scirp.69127-ref1">1</xref>] , for n = +3, a rate of advance of the perihelion of Mercury was obtained in agreement with experiments. For n = −3 however the absolute value was also about 43&quot;/sec but of negative sign.</p><p>When solving Equation (1) with n = −3 in polar coordinate it will be seen that the correct absolute value and sign of the perihelion precession of the planets is obtained.</p><p>The balance between the force given by Newton’s 2<sup>nd</sup> law and Newtonian gravitation in polar coordinates.</p><p>Equation (1) in polar coordinates (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x13.png" xlink:type="simple"/></inline-formula>) for a Newtonian (n = 0) balance, following [<xref ref-type="bibr" rid="scirp.69127-ref3">3</xref>] , is written as</p><disp-formula id="scirp.69127-formula1048"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/69127x14.png"  xlink:type="simple"/></disp-formula><p>From which the following differential equation is obtained [<xref ref-type="bibr" rid="scirp.69127-ref3">3</xref>] :</p><disp-formula id="scirp.69127-formula1049"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/69127x15.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x16.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x17.png" xlink:type="simple"/></inline-formula>: the angular momentum per unit mass, a constant.</p><p>The solution of an ODE of the type of Equation (3) is [<xref ref-type="bibr" rid="scirp.69127-ref4">4</xref>] :</p><disp-formula id="scirp.69127-formula1050"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/69127x18.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x19.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x20.png" xlink:type="simple"/></inline-formula> are the constants of integration. Equation (4) is the equation of a conic section which includes the ellipse (Kepler 1<sup>st</sup> law)</p><p>Equation (2) considering the correction factor of Equation (1) (using n = −3) can similarly be written as</p><disp-formula id="scirp.69127-formula1051"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/69127x21.png"  xlink:type="simple"/></disp-formula><p>Following the same approach used to obtain Equation (3) and considering that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x22.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.69127-ref5">5</xref>] , it is obtained:</p><disp-formula id="scirp.69127-formula1052"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/69127x23.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x24.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x25.png" xlink:type="simple"/></inline-formula></p><p>The solution of Equation (6), considering that the multiplier of b represents a small perturbation to a solution expressed by Equation (4), can be expanded into Fourier series as [<xref ref-type="bibr" rid="scirp.69127-ref4">4</xref>]</p><disp-formula id="scirp.69127-formula1053"><graphic  xlink:href="http://html.scirp.org/file/69127x26.png"  xlink:type="simple"/></disp-formula><p>Making use of trigonometric identities and neglecting terms containing 2<sup>nd</sup> and higher power of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x27.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.69127-formula1054"><graphic  xlink:href="http://html.scirp.org/file/69127x28.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69127-formula1055"><graphic  xlink:href="http://html.scirp.org/file/69127x29.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x30.png" xlink:type="simple"/></inline-formula>,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x31.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x32.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x33.png" xlink:type="simple"/></inline-formula></p><p>Neglecting terms containing 2<sup>nd</sup> and higher power of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x34.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.69127-formula1056"><graphic  xlink:href="http://html.scirp.org/file/69127x35.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.69127-formula1057"><graphic  xlink:href="http://html.scirp.org/file/69127x36.png"  xlink:type="simple"/></disp-formula><p>Substitute into Equation (6) and comparing coefficients of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x37.png" xlink:type="simple"/></inline-formula>: <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x38.png" xlink:type="simple"/></inline-formula>expanding into Taylor/ Maclaurin series up to the linear term:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x39.png" xlink:type="simple"/></inline-formula>.</p><p>The angle between two succeeding perihelion is [<xref ref-type="bibr" rid="scirp.69127-ref4">4</xref>] :</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x40.png" xlink:type="simple"/></inline-formula>so <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x41.png" xlink:type="simple"/></inline-formula></p><p>The precession of the perihelion per revolution is:</p><disp-formula id="scirp.69127-formula1058"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/69127x42.png"  xlink:type="simple"/></disp-formula><p>Considering that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x43.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.69127-ref6">6</xref>] , Equation (7) becomes:</p><disp-formula id="scirp.69127-formula1059"><graphic  xlink:href="http://html.scirp.org/file/69127x44.png"  xlink:type="simple"/></disp-formula><p>The precession of the perihelion per orbital period is</p><disp-formula id="scirp.69127-formula1060"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/69127x45.png"  xlink:type="simple"/></disp-formula><p>Neglecting the mass of the planets in comparison to the mass of the Sun:</p><disp-formula id="scirp.69127-formula1061"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/69127x46.png"  xlink:type="simple"/></disp-formula><p>See the ratio of the mass of the planets to the mass of the Sun in the next section.</p></sec><sec id="s2"><title>2. Computational Results and Analysis</title><p>The application of the Equation (9) to the planets of the solar system is given in <xref ref-type="table" rid="table1">Table 1</xref> along with the results of the Einstein GTR (Equation (10)).</p><p>The Einstein GTR result of the precession per revolution is given by [<xref ref-type="bibr" rid="scirp.69127-ref7">7</xref>]</p><disp-formula id="scirp.69127-formula1062"><graphic  xlink:href="http://html.scirp.org/file/69127x47.png"  xlink:type="simple"/></disp-formula><p>which when expressed per orbital period is,</p><disp-formula id="scirp.69127-formula1063"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/69127x48.png"  xlink:type="simple"/></disp-formula><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Perihelion precession of planets (S: Corrected Newtonian gravitation, Sε: Einstein GTR, Sk: S = Sε through Kepler’s 3<sup>rd</sup> law)</title></caption><table><tbody><thead><tr><th align="center" valign="middle"  rowspan="2"  >Planet</th><th align="center" valign="middle" >a</th><th align="center" valign="middle" >e</th><th align="center" valign="middle" >T</th><th align="center" valign="middle" >S</th><th align="center" valign="middle" >Sε</th><th align="center" valign="middle" >Sk</th></tr></thead><tr><td align="center" valign="middle" >(AU)</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >(days)</td><td align="center" valign="middle" >(&quot;/cy)</td><td align="center" valign="middle" >(&quot;/cy)</td><td align="center" valign="middle" >(&quot;/cy)</td></tr><tr><td align="center" valign="middle" >Mercury</td><td align="center" valign="middle" >0.38709893</td><td align="center" valign="middle" >0.20564</td><td align="center" valign="middle" >87.968435</td><td align="center" valign="middle" >42.98184</td><td align="center" valign="middle" >42.98273</td><td align="center" valign="middle" >42.98139</td></tr><tr><td align="center" valign="middle" >Venus</td><td align="center" valign="middle" >0.72333199</td><td align="center" valign="middle" >0.00676</td><td align="center" valign="middle" >224.695434</td><td align="center" valign="middle" >8.62495</td><td align="center" valign="middle" >8.62538</td><td align="center" valign="middle" >8.62474</td></tr><tr><td align="center" valign="middle" >Earth</td><td align="center" valign="middle" >1.00000011</td><td align="center" valign="middle" >0.01673</td><td align="center" valign="middle" >365.256363051</td><td align="center" valign="middle" >3.83877</td><td align="center" valign="middle" >3.83879</td><td align="center" valign="middle" >3.83877</td></tr><tr><td align="center" valign="middle" >Mars</td><td align="center" valign="middle" >1.52366231</td><td align="center" valign="middle" >0.09337</td><td align="center" valign="middle" >686.980</td><td align="center" valign="middle" >1.35095</td><td align="center" valign="middle" >1.35087</td><td align="center" valign="middle" >1.35099</td></tr><tr><td align="center" valign="middle" >Jupiter</td><td align="center" valign="middle" >5.20336301</td><td align="center" valign="middle" >0.04854</td><td align="center" valign="middle" >4330.595</td><td align="center" valign="middle" >0.06235</td><td align="center" valign="middle" >0.06249</td><td align="center" valign="middle" >0.06229</td></tr><tr><td align="center" valign="middle" >Saturn</td><td align="center" valign="middle" >9.53707032</td><td align="center" valign="middle" >0.05551</td><td align="center" valign="middle" >10746.94</td><td align="center" valign="middle" >0.01372</td><td align="center" valign="middle" >0.01375</td><td align="center" valign="middle" >0.01370</td></tr><tr><td align="center" valign="middle" >Uranus</td><td align="center" valign="middle" >19.19126393</td><td align="center" valign="middle" >0.04686</td><td align="center" valign="middle" >30685.4</td><td align="center" valign="middle" >0.00239</td><td align="center" valign="middle" >0.00239</td><td align="center" valign="middle" >0.00238</td></tr><tr><td align="center" valign="middle" >Neptune</td><td align="center" valign="middle" >30.06896348</td><td align="center" valign="middle" >0.00895</td><td align="center" valign="middle" >60189</td><td align="center" valign="middle" >0.00077</td><td align="center" valign="middle" >0.00078</td><td align="center" valign="middle" >0.00077</td></tr><tr><td align="center" valign="middle" >Pluto</td><td align="center" valign="middle" >39.48168677</td><td align="center" valign="middle" >0.24440</td><td align="center" valign="middle" >90465</td><td align="center" valign="middle" >0.00042</td><td align="center" valign="middle" >0.00042</td><td align="center" valign="middle" >0.00042</td></tr></tbody></table></table-wrap><p>The semi-major axis and the orbital period are taken from [<xref ref-type="bibr" rid="scirp.69127-ref8">8</xref>] . The eccentricity is taken from [<xref ref-type="bibr" rid="scirp.69127-ref3">3</xref>] except for Pluto that was taken from [<xref ref-type="bibr" rid="scirp.69127-ref6">6</xref>] .</p><p>From <xref ref-type="table" rid="table1">Table 1</xref> it can be seen a remarkable agreement between <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x49.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x50.png" xlink:type="simple"/></inline-formula>, which suggests a strong connection between them.</p><p>To find out that connection, the 3<sup>rd</sup> law of Kepler expressed as <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x51.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.69127-ref3">3</xref>] is substituted into Equation 9, it results in:</p><disp-formula id="scirp.69127-formula1064"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/69127x52.png"  xlink:type="simple"/></disp-formula><p>This is the equation used in the calculation of the precession shown in the last column of <xref ref-type="table" rid="table1">Table 1</xref>. When the Kepler’s 3<sup>rd</sup> law is also substituted into Equation (10) (Einstein GTR), the Equation (11) is also obtained. So Equations (9) and (10) are equivalent when the orbital period is expressed in term of the semi-major axis.</p><p>If the mass of the planets is considered in S, h and in T, then Equations (9)-(11) become:</p><disp-formula id="scirp.69127-formula1065"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/69127x53.png"  xlink:type="simple"/></disp-formula><p>which results in a very small impact on Jupiter.</p><p>Note that the ratio of the mass of the planets to the mass of the Sun based on [<xref ref-type="bibr" rid="scirp.69127-ref9">9</xref>] is 1.660137E−7, 2.447840E−6, 3.040433E−6, 3.227149E−7, 9.547907E−4, 2.858776E−4, 4.355401E−5, 5.177591E−5, 7.692308E−9 for Mercury, Venus, Earth, …, Pluto respectively.</p><p>It is noted that if the number “3” in Equation (12) is replaced with L/2 where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x54.png" xlink:type="simple"/></inline-formula>, the results are in close agreement with the values reported for Mercury in <xref ref-type="table" rid="table1">Table 1</xref> of reference [<xref ref-type="bibr" rid="scirp.69127-ref1">1</xref>] for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x55.png" xlink:type="simple"/></inline-formula>.</p><p>Equation (1) was solved numerically using n = 3 as in reference [<xref ref-type="bibr" rid="scirp.69127-ref1">1</xref>] . The results of the rate of the advance of the longitude of the perihelion (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x56.png" xlink:type="simple"/></inline-formula>) for Venus and Earth were 8.65&quot;/cy and 3.83&quot;/cy respectively which were determined from the slope of a linear fit of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x57.png" xlink:type="simple"/></inline-formula> with time which had correlation coefficients (R<sup>2</sup>) greater than</p><p>0.95 (for Mercury R<sup>2</sup> was &gt;0.9998). The simulation time was about 909 years forward and the integration step was 10<sup>−4</sup> days. The set of points used for the orbital-elements calculation and for the fit were the set containing the calculated (from r(t) data) closest point to the Sun in each consecutive time interval of an orbital period. The mass of the planets and the initial conditions were taken from reference [<xref ref-type="bibr" rid="scirp.69127-ref9">9</xref>] .</p><p>Using the numerical approach just described, the solution of Einstein GTR equation of motion neglecting the mass of the planets [<xref ref-type="bibr" rid="scirp.69127-ref2">2</xref>] resulted in 8.58&quot;/cy and 3.84&quot;/cy for Venus and Earth respectively.</p><p>It could be worthy to perform experiments to find the value of n in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/69127x58.png" xlink:type="simple"/></inline-formula> for gravitational bound systems involving motions at very high speed and to find a fundament for this correction.</p></sec><sec id="s3"><title>3. Concluding Remarks</title><p>An equation for the intrinsic (i.e. two-body problem) perihelion precession of the planets of the solar system was obtained based on the Fourier series solution of a corrected balance between the force given by the Newton’s 2<sup>nd</sup> law and the Newton gravitational force in polar coordinates. When the Kepler’s 3<sup>rd</sup> law is used to express the orbital period in term of the semi-major axis the perihelion precession equation coincides with the equation resulting from Einstein GTR.</p></sec><sec id="s4"><title>Cite this paper</title><p>Barbaro Quintero-Leyva, (2016) On the Intrinsic Precession of the Perihelion of Planets of the Solar System. Open Access Library Journal,03,1-5. doi: 10.4236/oalib.1102554</p></sec></body><back><ref-list><title>References</title><ref id="scirp.69127-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Quintero-Leyva, B. (2015) On the Intrinsic Precession of the Perihelion of Mercury. 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