Gravitational Force: Difference between revisions
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===Middling=== | ===Middling=== | ||
''The mass of the Earth is <math>6 x 10^ {24}</math> kg, and the mass of the Moon is <math>7 x 10^ {22}</math> kg. At a particular instance the moon is at location <math><2.8 x 10^8,0,-2.8 x 10^8></math> m, in a coordinate system whose origin is at the center of the earth. '''(a)''' What is <math>\vec{\mathbf{r}}</math>, the relative position vector from the Earth to the Moon? '''(b)''' What is <math>|\vec{\mathbf{r}}|</math>? '''(c)''' What is the unit vector <math>\vec{\mathbf{r}}</math>? '''(d)''' What is the gravitation force exerted by the Earth on the Moon? Your answer should be in vector.'' | |||
The solution of the problem involves substituting known values of G (<math>6.673 x 10^{-11}</math>N m<sup>2</sup>/kg<sup>2</sup>), m<sub>1</sub> <math>6 x 10^ {24}</math> kg, m<sub>2</sub> <math>7 x 10^ {22}</math> kg and d <math><2.8 x 10^8,0,-2.8 x 10^8></math> m m into the universal gravitation equation and solving for F<sub>grav</sub>. The solution is as follows: | |||
: '''(a)''' The position vector of Moon relative to Earth is, | |||
:: <math>\vec{\mathbf{r}}</math> = <math><2.8 x 10^8,0,-2.8 x 10^8> - <0,0,0></math> | |||
:: <math>\vec{\mathbf{r}}</math> = <math><2.8 x 10^8,0,-2.8 x 10^8></math> m | |||
: '''(b)''' The magnitude of position vector of Moon relative to Earth is, | |||
:: <math>|\vec{\mathbf{r}}|</math> = <math>/sqrt((2.8 x 10^8)^2+0^2+(-2.8 x 10^8)^2)</math> | |||
:: <math>|\vec{\mathbf{r}}|</math> = <math> 4.0 x 10^8 </math> m | |||
: '''(c)''' The unit vector of Moon relative to Earth is, | |||
:: <math>{\mathbf{r}} = \frac {\vec{\mathbf{r}}}{|\vec{\mathbf{r}}|}</math> | |||
:: <math>{\mathbf{r}} = \frac{<2.8 x 10^8,0,-2.8 x 10^8>}{4.0 x 10^8} </math> | |||
:: <math>{\mathbf{r}} = <0.7,0,-0.7></math> | |||
: '''(d)''' The expression for the gravitational force on the Moon by the Earth is, | |||
::<math> |\mathbf{F_{g}}| = G \frac{m_E m_M}{r^2} </math> | |||
::<math> |\mathbf{F_{g}}| = 6.7x10^{-11} \frac{6 x 10^ {24} * 7 x 10^ {22}}{(4.0 x 10^8)^2 }</math> | |||
::<math> |\mathbf{F_{g}}| = 1.76x10^{20}N</math> | |||
::<math> \vec{\mathbf{F_{g}}}</math> = <math> -|\mathbf{F_{grav}}|*{\mathbf{r}}</math> | |||
::<math> \vec{\mathbf{F_{g}}}</math> = <math>-1.76x10^{20}*<0.7,0,-0.7></math> | |||
::<math> \vec{\mathbf{F_{g}}}</math> = <math><-1.232x10^{20},0,1.232x10^{20}></math> | |||
===Difficult=== | ===Difficult=== | ||
Revision as of 19:58, 27 November 2015
Main Idea
A Mathematical Model
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Units
In Si Unit, Gravitational Force F is measured in Newtons (N), the two masses, m1 and m2 are measures in kilograms (Kg), the distance is measured in meters (m), and the gravitational constant G is measured in N m2/ kg−2 and has a value of 6.674×10−11 N m2/ kg−2. The Gravitational Constant G have different values for different units. The value of constant G appeared in Newton's law of universal gravitation, but it was not measured until seventy two years after Newton's death by Henry Cavendish with his Cavendish experiment in 1798. The value of gravitational constant was also the first test of Newton's law between two masses in Laboratory.
Examples
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Simple
Middling
The mass of the Earth is [math]\displaystyle{ 6 x 10^ {24} }[/math] kg, and the mass of the Moon is [math]\displaystyle{ 7 x 10^ {22} }[/math] kg. At a particular instance the moon is at location [math]\displaystyle{ \lt 2.8 x 10^8,0,-2.8 x 10^8\gt }[/math] m, in a coordinate system whose origin is at the center of the earth. (a) What is [math]\displaystyle{ \vec{\mathbf{r}} }[/math], the relative position vector from the Earth to the Moon? (b) What is [math]\displaystyle{ |\vec{\mathbf{r}}| }[/math]? (c) What is the unit vector [math]\displaystyle{ \vec{\mathbf{r}} }[/math]? (d) What is the gravitation force exerted by the Earth on the Moon? Your answer should be in vector.
The solution of the problem involves substituting known values of G ([math]\displaystyle{ 6.673 x 10^{-11} }[/math]N m2/kg2), m1 [math]\displaystyle{ 6 x 10^ {24} }[/math] kg, m2 [math]\displaystyle{ 7 x 10^ {22} }[/math] kg and d [math]\displaystyle{ \lt 2.8 x 10^8,0,-2.8 x 10^8\gt }[/math] m m into the universal gravitation equation and solving for Fgrav. The solution is as follows:
- (a) The position vector of Moon relative to Earth is,
- [math]\displaystyle{ \vec{\mathbf{r}} }[/math] = [math]\displaystyle{ \lt 2.8 x 10^8,0,-2.8 x 10^8\gt - \lt 0,0,0\gt }[/math]
- [math]\displaystyle{ \vec{\mathbf{r}} }[/math] = [math]\displaystyle{ \lt 2.8 x 10^8,0,-2.8 x 10^8\gt }[/math] m
- (b) The magnitude of position vector of Moon relative to Earth is,
- [math]\displaystyle{ |\vec{\mathbf{r}}| }[/math] = [math]\displaystyle{ /sqrt((2.8 x 10^8)^2+0^2+(-2.8 x 10^8)^2) }[/math]
- [math]\displaystyle{ |\vec{\mathbf{r}}| }[/math] = [math]\displaystyle{ 4.0 x 10^8 }[/math] m
- (c) The unit vector of Moon relative to Earth is,
- [math]\displaystyle{ {\mathbf{r}} = \frac {\vec{\mathbf{r}}}{|\vec{\mathbf{r}}|} }[/math]
- [math]\displaystyle{ {\mathbf{r}} = \frac{\lt 2.8 x 10^8,0,-2.8 x 10^8\gt }{4.0 x 10^8} }[/math]
- [math]\displaystyle{ {\mathbf{r}} = \lt 0.7,0,-0.7\gt }[/math]
- (d) The expression for the gravitational force on the Moon by the Earth is,
- [math]\displaystyle{ |\mathbf{F_{g}}| = G \frac{m_E m_M}{r^2} }[/math]
- [math]\displaystyle{ |\mathbf{F_{g}}| = 6.7x10^{-11} \frac{6 x 10^ {24} * 7 x 10^ {22}}{(4.0 x 10^8)^2 } }[/math]
- [math]\displaystyle{ |\mathbf{F_{g}}| = 1.76x10^{20}N }[/math]
- [math]\displaystyle{ \vec{\mathbf{F_{g}}} }[/math] = [math]\displaystyle{ -|\mathbf{F_{grav}}|*{\mathbf{r}} }[/math]
- [math]\displaystyle{ \vec{\mathbf{F_{g}}} }[/math] = [math]\displaystyle{ -1.76x10^{20}*\lt 0.7,0,-0.7\gt }[/math]
- [math]\displaystyle{ \vec{\mathbf{F_{g}}} }[/math] = [math]\displaystyle{ \lt -1.232x10^{20},0,1.232x10^{20}\gt }[/math]
Difficult
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