<?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">AM</journal-id><journal-title-group><journal-title>Applied Mathematics</journal-title></journal-title-group><issn pub-type="epub">2152-7385</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/am.2016.716159</article-id><article-id pub-id-type="publisher-id">AM-71270</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Torque Free Axi-Symmetric Gyros with Changing Moments of Inertia
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>A.</surname><given-names>I. Ismail</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Fawaz</surname><given-names>D. El-Haiby</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Faculty of Science, Umm Al-Qura University, Makkah, Saudi Arabia</addr-line></aff><aff id="aff1"><addr-line>Department of Mechanics, Collage of Engineering and Islamic Architecture, Umm Al-Qura University, Makkah, Saudi Arabia</addr-line></aff><pub-date pub-type="epub"><day>14</day><month>10</month><year>2016</year></pub-date><volume>07</volume><issue>16</issue><fpage>1934</fpage><lpage>1942</lpage><history><date date-type="received"><day>July</day>	<month>13,</month>	<year>2016</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>October</month>	<year>15,</year>	</date><date date-type="accepted"><day>October</day>	<month>18,</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>
 
 
  The properties and characteristics of torque free gyros with rotational symmetry and changing moments of inertia are the subject of the subsequent discussion. It shall be understood that the symmetry can be expressed by the notation (A=B) which does not presuppose geometric symmetry, where A and B are the principle moments of inertia about x and y axes respectively. We study the case of a torque free gyro upon which no external torque is acting. The equations of motion are derived when the origin of the xyz-coordinate system coincides with the gyro’s mass center c. This study is useful for the satellites, which have rotational symmetry and changed inertia moments, the antennas and the solar power collector systems.
 
</p></abstract><kwd-group><kwd>The Gyroscopic Motions</kwd><kwd> Moments of Inertia</kwd><kwd> Satellites</kwd><kwd> Antennas</kwd><kwd> Solar Power  Collector Systems</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>A gyro is a body of rotation which is set spinning at a large angular velocity around its axis of symmetry. The most important practical applications of gyros are met in devices for measuring the orientation or maintaining the stability of airplanes, spacecrafts and submarine vehicles in general. Various gyros are used as sensors in inertial guidance systems. Most textbooks in introductory mechanics explain the mysterious behavior of a spinning gyro by using Lagrange equations and severe mathematics [<xref ref-type="bibr" rid="scirp.71270-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.71270-ref2">2</xref>] . Other textbooks [<xref ref-type="bibr" rid="scirp.71270-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.71270-ref4">4</xref>] treat the problem of torque-induced precession of a top based on Euler equations, which are referred to the non-inertial reference frame rotating together with the body. The problem of the torque free inertial rotation of a symmetrical top is discussed, in particular, in [<xref ref-type="bibr" rid="scirp.71270-ref5">5</xref>] and illustrated by a simulation computer program (free rotation of an axially symmetrical body) [<xref ref-type="bibr" rid="scirp.71270-ref6">6</xref>] . For our problem, we consider a gyro body with xyz-coordinate system fixed of it, such that the z-axis of the body is the axis of symmetry and the inertia tensor is assumed to take the form</p><disp-formula id="scirp.71270-formula241"><label>(1.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x3.png"  xlink:type="simple"/></disp-formula><p>Here A and C are the principal moments of inertia in the x and z directions.</p><p>The rate of change of the inertia tensor with respect to time takes the form</p><disp-formula id="scirp.71270-formula242"><label>(1.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x4.png"  xlink:type="simple"/></disp-formula><p>We note that the inertia products remain zeros.</p><p>Assume that the angular velocity of the satellite or the gyros is</p><disp-formula id="scirp.71270-formula243"><label>(1.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x5.png"  xlink:type="simple"/></disp-formula><p>and the angular momentum is</p><disp-formula id="scirp.71270-formula244"><label>(1.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x6.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x7.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x8.png" xlink:type="simple"/></inline-formula> are the unit vectors in the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x9.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x10.png" xlink:type="simple"/></inline-formula> directions.</p><p>Thus the gyro’s kinetic energy of rotation becomes</p><disp-formula id="scirp.71270-formula245"><label>(1.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x11.png"  xlink:type="simple"/></disp-formula></sec><sec id="s2"><title>2. Equations of Motion</title><p>Applying Euler’s equations of motion and putting the applied torque equal zero, we get</p><disp-formula id="scirp.71270-formula246"><label>(2.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x12.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71270-formula247"><label>(2.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x13.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71270-formula248"><label>(2.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x14.png"  xlink:type="simple"/></disp-formula><p>For the considered problem (mentioned above) we apply the angular momentum principle to get</p><disp-formula id="scirp.71270-formula249"><label>, (2.4a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x15.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71270-formula250"><label>, (2.4b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x16.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71270-formula251"><label>. (2.4c)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x17.png"  xlink:type="simple"/></disp-formula></sec><sec id="s3"><title>3. Components of Angular Momentum</title><p>The Equation (2.4c) can be integrated to give</p><disp-formula id="scirp.71270-formula252"><graphic  xlink:href="http://html.scirp.org/file/4-7403280x18.png"  xlink:type="simple"/></disp-formula><p>We can conclude that the z-component of the angular moment is constant, that is</p><disp-formula id="scirp.71270-formula253"><label>(3.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x19.png"  xlink:type="simple"/></disp-formula><p>The angular velocity is obtained by multiplying the Equations (2.4a) by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x20.png" xlink:type="simple"/></inline-formula> and (2.4b) by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x21.png" xlink:type="simple"/></inline-formula> and adding the resulted equations, we get</p><disp-formula id="scirp.71270-formula254"><label>, (3.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x22.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71270-formula255"><label>(3.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x23.png"  xlink:type="simple"/></disp-formula><p>that is <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x24.png" xlink:type="simple"/></inline-formula> or<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x25.png" xlink:type="simple"/></inline-formula> (3.4)</p><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x26.png" xlink:type="simple"/></inline-formula>.</p><p>Thus the<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x27.png" xlink:type="simple"/></inline-formula>―component of angular momentum is constant</p><disp-formula id="scirp.71270-formula256"><label>(3.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x28.png"  xlink:type="simple"/></disp-formula><p>The <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x29.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x30.png" xlink:type="simple"/></inline-formula> can be shown, see <xref ref-type="fig" rid="fig1">Figure 1</xref>.</p><p>For torque free axi-symmetric gyro, angular velocity<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x31.png" xlink:type="simple"/></inline-formula>, angular momentum<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x32.png" xlink:type="simple"/></inline-formula>,</p><fig-group id="fig1"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> The angular momentum components.</title></caption><fig id ="fig1_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-7403280x33.png"/></fig></fig-group><p>and the gyro’s symmetry axis lie in one plane [<xref ref-type="bibr" rid="scirp.71270-ref7">7</xref>] .</p><p>Since the Equations (3.1) and (3.5) represent the angular momentum components, it can be deduced that the nutation angle remains constant when the inertia moments change as it when the inertia moments does not change.</p><p>For the components of angular velocity (3.4), we introduce the auxiliary frequency <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x34.png" xlink:type="simple"/></inline-formula> defined by</p><disp-formula id="scirp.71270-formula257"><label>, (3.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x35.png"  xlink:type="simple"/></disp-formula><p>then</p><disp-formula id="scirp.71270-formula258"><label>. (3.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x36.png"  xlink:type="simple"/></disp-formula><p>The two Equations (2.4a) and (2.4b) can be combined to yield</p><disp-formula id="scirp.71270-formula259"><label>. (3.8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x37.png"  xlink:type="simple"/></disp-formula><p>The solution of this differential equation can be obtained as</p><disp-formula id="scirp.71270-formula260"><label>. (3.9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x38.png"  xlink:type="simple"/></disp-formula><p>If the constant<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x39.png" xlink:type="simple"/></inline-formula>, and in order to find the value of constant <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x40.png" xlink:type="simple"/></inline-formula> we employ the Equation (3.5) to get <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x41.png" xlink:type="simple"/></inline-formula> and then</p><disp-formula id="scirp.71270-formula261"><label>, (3.10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x42.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71270-formula262"><label>, (3.11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x43.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71270-formula263"><label>, (3.12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x44.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x45.png" xlink:type="simple"/></inline-formula>.</p><p>We can get the<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x46.png" xlink:type="simple"/></inline-formula>―component of the angular velocity at any instant by using</p><disp-formula id="scirp.71270-formula264"><label>(3.13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x47.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71270-formula265"><label>(3.14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x48.png"  xlink:type="simple"/></disp-formula><p>where the subscript (0) refers to values of time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x49.png" xlink:type="simple"/></inline-formula></p><p>The components of angular velocity can be shown, see <xref ref-type="fig" rid="fig2">Figure 2</xref>.</p><p>The angular velocity component <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x50.png" xlink:type="simple"/></inline-formula> has a relative angular velocity <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x51.png" xlink:type="simple"/></inline-formula> in the xy- plane.</p><p>Introducing a floating <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x52.png" xlink:type="simple"/></inline-formula> coordinate system, we can express the angular velocity (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x53.png" xlink:type="simple"/></inline-formula>) by using the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x54.png" xlink:type="simple"/></inline-formula> or the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x55.png" xlink:type="simple"/></inline-formula> coordinate system.</p><p>The Equations (3.11) and (3.12) show that the component <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x56.png" xlink:type="simple"/></inline-formula> and consequently v-axis and u-axis are perpendicular, such that u-axis rotates with a relative angular velocity <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x57.png" xlink:type="simple"/></inline-formula> where</p><disp-formula id="scirp.71270-formula266"><graphic  xlink:href="http://html.scirp.org/file/4-7403280x58.png"  xlink:type="simple"/></disp-formula><p>In the xy-plane, the z-component of the absolute angular velocity of v-axis is</p><fig-group id="fig2"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> The components of angular velocity.</title></caption><fig id ="fig2_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-7403280x59.png"/></fig></fig-group><disp-formula id="scirp.71270-formula267"><label>(3.15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x60.png"  xlink:type="simple"/></disp-formula><p>We can find that, for a flattened gyro<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x61.png" xlink:type="simple"/></inline-formula>, the v-axis rotates faster than the x-axis, and for elongated gyro <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x62.png" xlink:type="simple"/></inline-formula> the v-axis rotates more slowly than the x-axis.</p><p>Thus, the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x63.png" xlink:type="simple"/></inline-formula> coordinate system moves with an angular velocity</p><disp-formula id="scirp.71270-formula268"><label>(3.16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x64.png"  xlink:type="simple"/></disp-formula><p>The angular velocity <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x65.png" xlink:type="simple"/></inline-formula> of the gyro body and the angular velocity <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x66.png" xlink:type="simple"/></inline-formula> of the floating <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x66.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x67.png" xlink:type="simple"/></inline-formula> coordinate system are related by</p><disp-formula id="scirp.71270-formula269"><label>. (3.17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x68.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x69.png" xlink:type="simple"/></inline-formula> is the spin of the gyro.</p></sec><sec id="s4"><title>4. Euler Frequencies</title><p>The frequency of the angular momentum remains constant since there is no external torque applied to the gyro [<xref ref-type="bibr" rid="scirp.71270-ref8">8</xref>] , the direction of the angular momentum vector may be used to define as space-fixed coordinate axis L which assigned to Z-axis and is called the precession axis [<xref ref-type="bibr" rid="scirp.71270-ref9">9</xref>] .</p><p>If the z-axis of the rotating <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x70.png" xlink:type="simple"/></inline-formula> coordinate system is the symmetry axis of the gyro, the v-axis lies in a plane formed by the Z- and z- axes, and we write</p><disp-formula id="scirp.71270-formula270"><label>. (4.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x71.png"  xlink:type="simple"/></disp-formula><p>The nutation angle <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x72.png" xlink:type="simple"/></inline-formula> is the angle between the z-axis and Z-axis where Z-axis and L are coincide, see <xref ref-type="fig" rid="fig3">Figure 3</xref>.</p><p>The components of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x73.png" xlink:type="simple"/></inline-formula> for elongated axis symmetric gyro are obtained from the shape, so</p><disp-formula id="scirp.71270-formula271"><label>(4.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x74.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71270-formula272"><label>(4.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x75.png"  xlink:type="simple"/></disp-formula><p>The nutation angle remains a constant and the gyro is carry out a steady precession about the angular momentum vector, since</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x76.png" xlink:type="simple"/></inline-formula> (4.4) we obtain</p><disp-formula id="scirp.71270-formula273"><label>(4.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x77.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.71270-formula274"><label>. (4.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x78.png"  xlink:type="simple"/></disp-formula><p>Also from the figure</p><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Euler’s angles</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-7403280x79.png"/></fig><disp-formula id="scirp.71270-formula275"><label>(4.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x80.png"  xlink:type="simple"/></disp-formula><p>Also for the angle <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x81.png" xlink:type="simple"/></inline-formula> between the z-axis and the angular velocity <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x82.png" xlink:type="simple"/></inline-formula> axis, we have</p><disp-formula id="scirp.71270-formula276"><label>. (4.8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x83.png"  xlink:type="simple"/></disp-formula><p>The motion of a torque free gyro with rotational symmetry and changing moment of inertia can be visualized by imaging a space cone and body cone as shown see <xref ref-type="fig" rid="fig4">Figure 4</xref> and <xref ref-type="fig" rid="fig5">Figure 5</xref>.</p><p>We can obtain the relation between the precession and the spin as follows</p><disp-formula id="scirp.71270-formula277"><label>. (4.9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-7403280x84.png"  xlink:type="simple"/></disp-formula><p>For the elongated gyro <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x85.png" xlink:type="simple"/></inline-formula> we find that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x85.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x86.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x85.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x87.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x85.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x88.png" xlink:type="simple"/></inline-formula> have the same sign then the precession is direct.</p><p>For the flattened gyro <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x89.png" xlink:type="simple"/></inline-formula> we find that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x90.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x90.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x91.png" xlink:type="simple"/></inline-formula> have the opposite signs, then the precession is retrograde.</p></sec><sec id="s5"><title>5. Conclusions</title><p>The system (2.4) is integrated to obtain the angular velocities and the angular momentum,</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Space cone and body cone for an elongated gyro</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-7403280x92.png"/></fig><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Space cone and body cone for a flattened gyro</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-7403280x93.png"/></fig><p>then Euler’s angles are deduced. The motions are classified into two cases:</p><p>1) the elongated gyro<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x94.png" xlink:type="simple"/></inline-formula>.</p><p>2) the flattened gyro<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-7403280x95.png" xlink:type="simple"/></inline-formula>.</p><p>For each case, we investigate the equations of motions, the precession, the nutation and the spin for these motions in detailed by using the analytical techniques and the illustrated shapes. The obtained results can be applied on the satellites [<xref ref-type="bibr" rid="scirp.71270-ref10">10</xref>] with rotational symmetry and changed inertia moments, the antennas [<xref ref-type="bibr" rid="scirp.71270-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.71270-ref12">12</xref>] and the solar power collector systems [<xref ref-type="bibr" rid="scirp.71270-ref13">13</xref>] .</p></sec><sec id="s6"><title>Acknowledgements</title><p>This project is supported by Institute of Scientific Research and Islamic Heritage Revival, Umm Al-Qura University, Saudi Arabia.</p></sec><sec id="s7"><title>Cite this paper</title><p>Ismail, A.I. and El-Haiby, F.D. (2016) Torque Free Axi- Symmetric Gyros with Changing Moments of Inertia. Applied Mathematics, 7, 1934- 1942. http://dx.doi.org/10.4236/am.2016.716159</p></sec></body><back><ref-list><title>References</title><ref id="scirp.71270-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Goldstein, H. (1980) Classical Mechanics. 2nd Edition, Addison-Wesley, Reading.</mixed-citation></ref><ref id="scirp.71270-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Goldstein, H., Poole, Ch.P. and Safko, J.L. (2002) Classical Mechanics. 3rd Edition, Addison-Wesley, Reading.</mixed-citation></ref><ref id="scirp.71270-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Kittel, Ch., Knight, W.D. and Ruderman, M.A. (1965-1971) Mechanics. Berkeley Physics Course. McGraw-Hill, New York.</mixed-citation></ref><ref id="scirp.71270-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">Landau, L.D. and Lifschitz, E.M. (1976) Mechanics. Pergamon, New York.</mixed-citation></ref><ref id="scirp.71270-ref5"><label>5</label><mixed-citation publication-type="journal" xlink:type="simple"><name name-style="western"><surname>Butikov</surname><given-names> E. </given-names></name>,<etal>et al</etal>. (<year>2006</year>)<article-title>Inertial Rotation of a Rigid Body</article-title><source> European Journal of Physics</source><volume> 27</volume>,<fpage> 913</fpage>-<lpage>922</lpage>.<pub-id pub-id-type="doi"></pub-id></mixed-citation></ref><ref id="scirp.71270-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">Butikov, E. (2006) Free Rotation of an Axially Symmetrical Body.  
http://www.ifmo.ru/butikov/Applets/Precession.html</mixed-citation></ref><ref id="scirp.71270-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">Bruno, A.D. (2007) Analysis of the Euler-Poisson Equations by Methods of Power Geometry and Normal Form. Journal of Applied Mathematics and Mechanics, 71, 168-199. 
http://dx.doi.org/10.1016/j.jappmathmech.2007.06.002</mixed-citation></ref><ref id="scirp.71270-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">Amer, T.S. (2004) Motion of a Rigid Body Analogous to the Case of Euler and Poinsot. Analysis, 24, 305-315. http://dx.doi.org/10.1524/anly.2004.24.14.305</mixed-citation></ref><ref id="scirp.71270-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">Udwadia, F.E. and Kalaba, R.E. (2007) Analytical Dynamics: A New Approach.</mixed-citation></ref><ref id="scirp.71270-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">Eshagh, M. and Najafi Alamdari, M. (2007) Perturbations in Orbital Elements of a Low Earth Orbiting Satellite. Journal of the Earth &amp; Space Physics, 33, 1-12.</mixed-citation></ref><ref id="scirp.71270-ref11"><label>11</label><mixed-citation publication-type="other" xlink:type="simple">Kraus, J.D. and Marhefka, R.J. (2002) Antennas for all Applications. McGraw-Hill, New York.</mixed-citation></ref><ref id="scirp.71270-ref12"><label>12</label><mixed-citation publication-type="other" xlink:type="simple">Balanis, C. (1997) Antenna Theory. John Wiley &amp; Sons, New Jersey, Published simultaneously in Canada, 450-458.</mixed-citation></ref><ref id="scirp.71270-ref13"><label>13</label><mixed-citation publication-type="other" xlink:type="simple">Price, H., Lupfert, E., Kearney, D., Zarza, E., Cohen, G., Gee, R. and Mahoney, R. (2002) Advances in Parabolic Trough Solar Power Technology. Journal of Solar Energy Engineering, 124, 109-125.</mixed-citation></ref></ref-list></back></article>