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		<title>2. Introduction to force and gravity - Versionshistorik</title>
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		<title>Taifun: Created page with &quot;__NOTOC__ {| border=&quot;0&quot; cellspacing=&quot;0&quot; cellpadding=&quot;0&quot; height=&quot;30&quot; width=&quot;100%&quot; | style=&quot;border-bottom:1px solid #797979&quot; width=&quot;5px&quot; | &amp;nbsp; {{Selected tab|[[2. Introduction t...&quot;</title>
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		<summary type="html">&lt;p&gt;Created page with &amp;quot;__NOTOC__ {| border=&amp;quot;0&amp;quot; cellspacing=&amp;quot;0&amp;quot; cellpadding=&amp;quot;0&amp;quot; height=&amp;quot;30&amp;quot; width=&amp;quot;100%&amp;quot; | style=&amp;quot;border-bottom:1px solid #797979&amp;quot; width=&amp;quot;5px&amp;quot; |   {{Selected tab|[[2. Introduction t...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;Ny sida&lt;/b&gt;&lt;/p&gt;&lt;div&gt;__NOTOC__&lt;br /&gt;
{| border=&amp;quot;0&amp;quot; cellspacing=&amp;quot;0&amp;quot; cellpadding=&amp;quot;0&amp;quot; height=&amp;quot;30&amp;quot; width=&amp;quot;100%&amp;quot;&lt;br /&gt;
| style=&amp;quot;border-bottom:1px solid #797979&amp;quot; width=&amp;quot;5px&amp;quot; | &amp;amp;nbsp;&lt;br /&gt;
{{Selected tab|[[2. Introduction to force and gravity|Theory]]}}&lt;br /&gt;
{{Not selected tab|[[2. Exercises|Exercises]]}}&lt;br /&gt;
{{Not selected tab|[[2. Video|Video]]}}&lt;br /&gt;
| style=&amp;quot;border-bottom:1px solid #797979&amp;quot;  width=&amp;quot;100%&amp;quot;| &amp;amp;nbsp;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== '''Key Points''' ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Newton's First Law'''&lt;br /&gt;
&lt;br /&gt;
A particle will move with a constant velocity or remain at rest if the resultant force on the particle is zero.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Equilibrium'''&lt;br /&gt;
&lt;br /&gt;
If the resultant force on a particle is zero, then the forces acting on the particle are said to be in equilibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''The Universal Law of Gravitation'''&lt;br /&gt;
&lt;br /&gt;
{| width=&amp;quot;500px&amp;quot; cellspacing=&amp;quot;10px&amp;quot; &lt;br /&gt;
| &amp;lt;math&amp;gt;F=\frac{Gm_{1}m_{2}}{{d}^{\ 2}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;G=6\textrm{.}67\times 10^{-11}\text{ kg}^{\text{-1}}\text{m}^{\text{3}}\text{s}^{\text{-2}}&amp;lt;/math&amp;gt;&lt;br /&gt;
| valign=&amp;quot;top&amp;quot;|[[Image:Gravitation.gif]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Gravitational force from an heavenly body'''&lt;br /&gt;
{| width=&amp;quot;500px&amp;quot; cellspacing=&amp;quot;10px&amp;quot; &lt;br /&gt;
| For a particle in the neighbourhood of a planet, moon or star the distance &amp;lt;math&amp;gt;d&amp;lt;/math&amp;gt; is measured from the centre to the particle.  &lt;br /&gt;
&lt;br /&gt;
Thus &lt;br /&gt;
&amp;lt;math&amp;gt;d=R+h&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;h&amp;lt;/math&amp;gt; is distance to the surface.&lt;br /&gt;
&lt;br /&gt;
| valign=&amp;quot;top&amp;quot;|[[Image:fig2gif.gif]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Gravity on Earth'''&lt;br /&gt;
&lt;br /&gt;
The force of gravity is often called the weight.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
&amp;amp; F=mg \\ &lt;br /&gt;
&amp;amp; g=9\textrm{.}8\text{ ms}^{\text{-2}} \\ &lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''Data'''&lt;br /&gt;
&lt;br /&gt;
Radius of Earth is &lt;br /&gt;
&amp;lt;math&amp;gt;\text{6}\textrm{.}\text{37}\times \text{1}0^{\text{6}}\text{ }&amp;lt;/math&amp;gt;&lt;br /&gt;
metres&lt;br /&gt;
	&lt;br /&gt;
Mass of Earth is &lt;br /&gt;
&amp;lt;math&amp;gt;\text{5}\textrm{.}\text{98}\times \text{1}0^{\text{24}}\text{ }&amp;lt;/math&amp;gt;&lt;br /&gt;
kg&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''[[Example 2.1]]'''&lt;br /&gt;
&lt;br /&gt;
Describe whether or not the forces acting on the following objects are in equilibrium:&lt;br /&gt;
&lt;br /&gt;
a) A passenger in a train that travels at a constant speed.&lt;br /&gt;
&lt;br /&gt;
b) A hot air balloon rising at a constant rate.&lt;br /&gt;
&lt;br /&gt;
c) A stone dropped into a very deep well full of water.&lt;br /&gt;
&lt;br /&gt;
'''Solution'''&lt;br /&gt;
&lt;br /&gt;
a) Yes, if it is travelling in a straight line.&lt;br /&gt;
&lt;br /&gt;
b) Yes, if it is travelling in a straight line.&lt;br /&gt;
&lt;br /&gt;
c) Yes, if it reaches a terminal velocity, so that it is travelling in a straight line at a constant speed.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''[[Example 2.2]]'''&lt;br /&gt;
&lt;br /&gt;
Find the magnitude of the force of gravity (weight) acting on a lorry of mass 22 tonnes.&lt;br /&gt;
&lt;br /&gt;
'''Solution'''&lt;br /&gt;
&lt;br /&gt;
This is calculated using the fact that the weight is given by &amp;lt;math&amp;gt;mg&amp;lt;/math&amp;gt;.&lt;br /&gt;
	&lt;br /&gt;
&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
&amp;amp; mg=22000\times 9\textrm{.}8 \\ &lt;br /&gt;
&amp;amp; =215600\text{ N}  &lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The diagram shows the lorry and its weight.&lt;br /&gt;
&lt;br /&gt;
[[Image:truck.gif||center]]&lt;br /&gt;
&lt;br /&gt;
Note that reaction forces also act upwards on each wheel.&lt;br /&gt;
	&lt;br /&gt;
&amp;lt;math&amp;gt;{{R}_{1}}+{{R}_{2}}+{{R}_{3}}+{{R}_{4}}=215600\ \text{N}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''[[Example 2.3]]'''&lt;br /&gt;
&lt;br /&gt;
A box of mass 30 kg is at rest on a table. &lt;br /&gt;
&lt;br /&gt;
a) Calculate the weight of the box.&lt;br /&gt;
&lt;br /&gt;
b) State the magnitude of the upward force that the table exerts on the box.&lt;br /&gt;
&lt;br /&gt;
'''Solution'''&lt;br /&gt;
&lt;br /&gt;
a) &lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
&amp;amp; W=30\times 9\textrm{.}8 \\ &lt;br /&gt;
&amp;amp; =294\text{ N}  &lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
b) An upward force of 294 N must act for the box to remain in equilibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''[[Example 2.4]]''' &lt;br /&gt;
&lt;br /&gt;
A satellite, of mass 400 kg, is at a height of 12 km above the surface of the earth. Find the magnitude of the gravitational attraction on the satellite.&lt;br /&gt;
&lt;br /&gt;
Data:	&lt;br /&gt;
&amp;lt;math&amp;gt;G=6\textrm{.}67\times {{10}^{-11}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&amp;lt;math&amp;gt;\text{k}{{\text{g}}^{-\text{1}}}{{\text{m}}^{\text{3}}}{{\text{s}}^{-\text{2}}}&amp;lt;/math&amp;gt;&lt;br /&gt;
		&lt;br /&gt;
Radius of earth  &amp;lt;math&amp;gt;=6\textrm{.}37\times {{10}^{6}} \text{m} &amp;lt;/math&amp;gt; &lt;br /&gt;
		&lt;br /&gt;
Mass of earth  &amp;lt;math&amp;gt;=5\textrm{.}98\times {{10}^{24}} \text{kg}&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
'''Solution'''&lt;br /&gt;
	&lt;br /&gt;
&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
&amp;amp; \frac{G{{m}_{1}}{{m}_{2}}}{{{d}^{\ {2}}}}=\frac{6\textrm{.}67\times {{10}^{-11}}\times 400\times 5\textrm{.}98\times {{10}^{24}}}{{{\left( 6\textrm{.}37\times {{10}^{6}}+12000 \right)}^{2}}} \\ &lt;br /&gt;
&amp;amp; =3917\text{ N}  &lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
'''[[Example 2.5]]'''&lt;br /&gt;
&lt;br /&gt;
The sun has mass &lt;br /&gt;
&amp;lt;math&amp;gt;1\textrm{.}99\times {{10}^{30}} \text{kg}&amp;lt;/math&amp;gt;&lt;br /&gt;
. The mean distance of the earth from the sun is approximately &lt;br /&gt;
&amp;lt;math&amp;gt;1\textrm{.}5\times {{10}^{11}} \text{m}&amp;lt;/math&amp;gt;&lt;br /&gt;
.&lt;br /&gt;
&lt;br /&gt;
(a) Calculate the force that the sun exerts on the earth.&lt;br /&gt;
&lt;br /&gt;
(b) State the force that the earth exerts on the sun.&lt;br /&gt;
&lt;br /&gt;
(c) Explain why this force varies.&lt;br /&gt;
&lt;br /&gt;
'''Solution'''&lt;br /&gt;
&lt;br /&gt;
(a) &lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
&amp;amp; \frac{G{{m}_{1}}{{m}_{2}}}{{{d}^{\ 2}}}=\frac{6\textrm{.}67\times {{10}^{-11}}\times 1\textrm{.}99\times {{10}^{30}}\times 5\textrm{.}98\times {{10}^{24}}}{{{\left( 1\textrm{.}5\times {{10}^{11}} \right)}^{2}}} \\ &lt;br /&gt;
&amp;amp; =3\textrm{.}53\times {{10}^{22}}\text{ N}  &lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
(b) &lt;br /&gt;
&amp;lt;math&amp;gt;3\textrm{.}53\times {{10}^{22}}\text{ N}  &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
(c) The distance between the earth and the sun varies.&lt;/div&gt;</summary>
		<author><name>Taifun</name></author>	</entry>

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