http://www.relativitybook.com/w/index.php?title=Einstein:Book_chapter_04_-_The_Galileian_System_of_Co-Ordinates&feed=atom&action=historyEinstein:Book chapter 04 - The Galileian System of Co-Ordinates - Revision history2024-03-29T08:24:25ZRevision history for this page on the wikiMediaWiki 1.26.3http://www.relativitybook.com/w/index.php?title=Einstein:Book_chapter_04_-_The_Galileian_System_of_Co-Ordinates&diff=537&oldid=prevEric Baird: Eric Baird moved page Einstein:Book chapter 04 to Einstein:Book chapter 04 - The Galileian System of Co-Ordinates2016-07-18T01:06:16Z<p>Eric Baird moved page <a href="/wiki/Einstein:Book_chapter_04" class="mw-redirect" title="Einstein:Book chapter 04">Einstein:Book chapter 04</a> to <a href="/wiki/Einstein:Book_chapter_04_-_The_Galileian_System_of_Co-Ordinates" title="Einstein:Book chapter 04 - The Galileian System of Co-Ordinates">Einstein:Book chapter 04 - The Galileian System of Co-Ordinates</a></p>
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</td></tr></table>Eric Bairdhttp://www.relativitybook.com/w/index.php?title=Einstein:Book_chapter_04_-_The_Galileian_System_of_Co-Ordinates&diff=452&oldid=prevEric Baird: Text replacement - "</person>" to "</span>"2016-07-08T20:23:27Z<p>Text replacement - "</person>" to "</span>"</p>
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<tr><td class='diff-marker'> </td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"><div><div id="PAGEBLOCK" ></div></td><td class='diff-marker'> </td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"><div><div id="PAGEBLOCK" ></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"><div>==4: The Galileian System of Co-Ordinates==</div></td><td class='diff-marker'> </td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"><div>==4: The Galileian System of Co-Ordinates==</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><p class="NOINDENT">{{Boldword|A|S}} is well known, the fundamental law of the mechanics of <span class="PERSON">Galilei</<del class="diffchange diffchange-inline">person</del>>-<span class="PERSON">Newton</<del class="diffchange diffchange-inline">person</del>>, which is known as the ''law of inertia'', can be stated thus:</p></div></td><td class='diff-marker'>+</td><td style="color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><p class="NOINDENT">{{Boldword|A|S}} is well known, the fundamental law of the mechanics of <span class="PERSON">Galilei</<ins class="diffchange diffchange-inline">span</ins>>-<span class="PERSON">Newton</<ins class="diffchange diffchange-inline">span</ins>>, which is known as the ''law of inertia'', can be stated thus:</p></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'>−</td><td style="color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>A body removed sufficiently far from other bodies continues in a state of rest or of uniform motion in a straight line. This law not only says something about the motion of the bodies, but it also indicates the reference-bodies or systems of co-ordinates, permissible in mechanics, which can be used in mechanical description. The visible fixed stars are bodies for which the law of inertia certainly holds for a high degree of approximation. Now if we use a system of co-ordinates which is rigidly attached to the earth, then, relative to this system, every fixed star describes a circle of immense radius in the course of an astronomical day, a result which is opposed to the statement of the law of inertia. So that if we adhere to this law we must refer these motions only to systems of co-ordinates relative to which the fixed stars do not move in a circle. A system of co-ordinates of which the state of motion is such that the law of inertia holds relative to it is called a "Galileian system of coordinates." The laws of the mechanics of <span class="PERSON">Galilei</<del class="diffchange diffchange-inline">person</del>>-<span class="PERSON">Newton</<del class="diffchange diffchange-inline">person</del>> can be regarded as valid only for a Galileian system of co-ordinates.</div></td><td class='diff-marker'>+</td><td style="color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>A body removed sufficiently far from other bodies continues in a state of rest or of uniform motion in a straight line. This law not only says something about the motion of the bodies, but it also indicates the reference-bodies or systems of co-ordinates, permissible in mechanics, which can be used in mechanical description. The visible fixed stars are bodies for which the law of inertia certainly holds for a high degree of approximation. Now if we use a system of co-ordinates which is rigidly attached to the earth, then, relative to this system, every fixed star describes a circle of immense radius in the course of an astronomical day, a result which is opposed to the statement of the law of inertia. So that if we adhere to this law we must refer these motions only to systems of co-ordinates relative to which the fixed stars do not move in a circle. A system of co-ordinates of which the state of motion is such that the law of inertia holds relative to it is called a "Galileian system of coordinates." The laws of the mechanics of <span class="PERSON">Galilei</<ins class="diffchange diffchange-inline">span</ins>>-<span class="PERSON">Newton</<ins class="diffchange diffchange-inline">span</ins>> can be regarded as valid only for a Galileian system of co-ordinates.</div></td></tr>
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</table>Eric Bairdhttp://www.relativitybook.com/w/index.php?title=Einstein:Book_chapter_04_-_The_Galileian_System_of_Co-Ordinates&diff=450&oldid=prevEric Baird: Text replacement - "<person>" to "<span class="PERSON">"2016-07-08T20:22:18Z<p>Text replacement - "<person>" to "<span class="PERSON">"</p>
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<tr><td class='diff-marker'> </td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"><div>==4: The Galileian System of Co-Ordinates==</div></td><td class='diff-marker'> </td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"><div>==4: The Galileian System of Co-Ordinates==</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><p class="NOINDENT">{{Boldword|A|S}} is well known, the fundamental law of the mechanics of <<del class="diffchange diffchange-inline">person</del>>Galilei</person>-<<del class="diffchange diffchange-inline">person</del>>Newton</person>, which is known as the ''law of inertia'', can be stated thus:</p></div></td><td class='diff-marker'>+</td><td style="color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><p class="NOINDENT">{{Boldword|A|S}} is well known, the fundamental law of the mechanics of <<ins class="diffchange diffchange-inline">span class="PERSON"</ins>>Galilei</person>-<<ins class="diffchange diffchange-inline">span class="PERSON"</ins>>Newton</person>, which is known as the ''law of inertia'', can be stated thus:</p></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f9f9f9; color: #333333; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #e6e6e6; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'>−</td><td style="color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>A body removed sufficiently far from other bodies continues in a state of rest or of uniform motion in a straight line. This law not only says something about the motion of the bodies, but it also indicates the reference-bodies or systems of co-ordinates, permissible in mechanics, which can be used in mechanical description. The visible fixed stars are bodies for which the law of inertia certainly holds for a high degree of approximation. Now if we use a system of co-ordinates which is rigidly attached to the earth, then, relative to this system, every fixed star describes a circle of immense radius in the course of an astronomical day, a result which is opposed to the statement of the law of inertia. So that if we adhere to this law we must refer these motions only to systems of co-ordinates relative to which the fixed stars do not move in a circle. A system of co-ordinates of which the state of motion is such that the law of inertia holds relative to it is called a "Galileian system of coordinates." The laws of the mechanics of <<del class="diffchange diffchange-inline">person</del>>Galilei</person>-<<del class="diffchange diffchange-inline">person</del>>Newton</person> can be regarded as valid only for a Galileian system of co-ordinates.</div></td><td class='diff-marker'>+</td><td style="color:black; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>A body removed sufficiently far from other bodies continues in a state of rest or of uniform motion in a straight line. This law not only says something about the motion of the bodies, but it also indicates the reference-bodies or systems of co-ordinates, permissible in mechanics, which can be used in mechanical description. The visible fixed stars are bodies for which the law of inertia certainly holds for a high degree of approximation. Now if we use a system of co-ordinates which is rigidly attached to the earth, then, relative to this system, every fixed star describes a circle of immense radius in the course of an astronomical day, a result which is opposed to the statement of the law of inertia. So that if we adhere to this law we must refer these motions only to systems of co-ordinates relative to which the fixed stars do not move in a circle. A system of co-ordinates of which the state of motion is such that the law of inertia holds relative to it is called a "Galileian system of coordinates." The laws of the mechanics of <<ins class="diffchange diffchange-inline">span class="PERSON"</ins>>Galilei</person>-<<ins class="diffchange diffchange-inline">span class="PERSON"</ins>>Newton</person> can be regarded as valid only for a Galileian system of co-ordinates.</div></td></tr>
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</table>Eric Bairdhttp://www.relativitybook.com/w/index.php?title=Einstein:Book_chapter_04_-_The_Galileian_System_of_Co-Ordinates&diff=219&oldid=prevEric Baird: 1 revision imported2016-07-04T21:39:49Z<p>1 revision imported</p>
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</td></tr></table>Eric Bairdhttp://www.relativitybook.com/w/index.php?title=Einstein:Book_chapter_04_-_The_Galileian_System_of_Co-Ordinates&diff=218&oldid=prevErkDemon: ErkDemon moved page Einstein:Book chapter04 to Einstein:Book chapter 04 without leaving a redirect: Text replacement - "chapter0" to "chapter 0"2016-06-30T02:01:56Z<p>ErkDemon moved page <a href="/w/index.php?title=Einstein:Book_chapter04&action=edit&redlink=1" class="new" title="Einstein:Book chapter04 (page does not exist)">Einstein:Book chapter04</a> to <a href="/wiki/Einstein:Book_chapter_04" class="mw-redirect" title="Einstein:Book chapter 04">Einstein:Book chapter 04</a> without leaving a redirect: Text replacement - "chapter0" to "chapter 0"</p>
<p><b>New page</b></p><div>{{Bookblock|04}}<br />
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==4: The Galileian System of Co-Ordinates==<br />
<p class="NOINDENT">{{Boldword|A|S}} is well known, the fundamental law of the mechanics of <person>Galilei</person>-<person>Newton</person>, which is known as the ''law of inertia'', can be stated thus:</p><br />
<br />
A body removed sufficiently far from other bodies continues in a state of rest or of uniform motion in a straight line. This law not only says something about the motion of the bodies, but it also indicates the reference-bodies or systems of co-ordinates, permissible in mechanics, which can be used in mechanical description. The visible fixed stars are bodies for which the law of inertia certainly holds for a high degree of approximation. Now if we use a system of co-ordinates which is rigidly attached to the earth, then, relative to this system, every fixed star describes a circle of immense radius in the course of an astronomical day, a result which is opposed to the statement of the law of inertia. So that if we adhere to this law we must refer these motions only to systems of co-ordinates relative to which the fixed stars do not move in a circle. A system of co-ordinates of which the state of motion is such that the law of inertia holds relative to it is called a "Galileian system of coordinates." The laws of the mechanics of <person>Galilei</person>-<person>Newton</person> can be regarded as valid only for a Galileian system of co-ordinates.<br />
</div></div>ErkDemon