Gravitational Force Near Earth: Difference between revisions
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==Main Idea== | ==Main Idea== | ||
Near Earth's surface, the magnitude of acceleration due gravity is approximately constant. Newton's Law of Universal Gravitation states that any two bodies attract each other with a force directly proportional to the product of the masses and inversely proportional to the square of the distance between the objects. If we approximate the Earth as a point mass, we find that the distance to the surface is simply the radius of the Earth. We now want to apply Newton's Law of Universal Gravitation to our approximation and see if we can calculate the acceleration due to gravity near Earth's surface. Generally this is only acceptable because the distance between the object of interest and Earth's surface is <math> << </math> the distance from the center of the Earth to Earth's surface. Thus the difference in distances is so small that the result is well-approximated using only Earth's radius. | Near Earth's surface, the magnitude of acceleration due gravity is approximately constant. Newton's Law of Universal Gravitation states that any two bodies attract each other with a force directly proportional to the product of the masses and inversely proportional to the square of the distance between the objects. If we approximate the Earth as a point mass, we find that the distance to the surface is simply the radius of the Earth. We now want to apply Newton's Law of Universal Gravitation to our approximation and see if we can calculate the acceleration due to gravity near Earth's surface. Generally this is only acceptable because the distance between the object of interest and Earth's surface is <math> << </math> the distance from the center of the Earth to Earth's surface. Thus the difference in distances is so small that the result is well-approximated using only Earth's radius. | ||
===A Mathematical Model=== | ===A Mathematical Model=== | ||
From Newton's Law of Universal Gravitation we know: | From Newton's Law of Universal Gravitation we know: | ||
::<math> {F}_{grav}=G \frac{m_1 m_2}{r^2}\ </math> | ::<math> {F}_{grav}=G \frac{m_1 m_2}{r^2}\ </math> | ||
Where | |||
::* ''F'' is the gravitational force between the masses; | ::* ''F'' is the gravitational force between the masses; | ||
::* ''G'' is the [https://en.wikipedia.org/wiki/Gravitational_constant gravitational constant], <math>6.674×10^{−11} \frac{N m^2}{kg^2}\ </math>; | ::* ''G'' is the [https://en.wikipedia.org/wiki/Gravitational_constant gravitational constant], <math>6.674×10^{−11} \frac{N m^2}{kg^2}\ </math>; | ||
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::* ''r'' is the distance between the objects. | ::* ''r'' is the distance between the objects. | ||
Since the only forces acting on a object in free fall near earth's surface are it's weight, (mass and gravity), we can set <math> {F}_{grav} = {mg} </math> ,and then plug that into Newton's Law of Universal Gravitation. After canceling out the constants, we arrive at the gravitational constant for a free falling object near earth. | |||
::<math> | ::<math> {g} = \frac{GM_{Earth}}{R_{Earth}^2}</math> | ||
Near Earth's surface ''g'' is unchanging. As such, we define it as the gravitational constant near Earth's surface, ''g'', which is approximately <math>9.8 \frac{m}{s^2} </math>. This calculation is shown below: | |||
::<math>C= \frac{(6.67*10^{-11} \frac{m^3}{kgs})(5.972*10^{24} kg)}{(6.378*10^{6} m)^2} = 9.8 \frac{m}{s^2}</math> | |||
This then puts the force near Earth due to gravity into a much simpler form: | This then puts the force near Earth due to gravity into a much simpler form: | ||
:: <math>|\vec{\mathbf{F}}_{grav}|= mg </math> | :: <math>|\vec{\mathbf{F}}_{grav}|= mg </math> | ||
Where | |||
::* ''g'' is the near-Earth gravitational constant, as defined above to be <math>9.8 \frac{m}{s^2} </math> | ::* ''g'' is the near-Earth gravitational constant, as defined above to be <math>9.8 \frac{m}{s^2} </math> | ||
::* ''m'' is the mass of the object whose behavior we are interested in | ::* ''m'' is the mass of the object whose behavior we are interested in | ||
The gravitation constant ''g'' applies to all masses ''significantly'' smaller than Earth's mass. These masses will all fall at the same acceleration. | |||
===The Gravitational Field=== | |||
[[File:Newtons2LawImage344.png|thumb|left|Distance between the centers of mass of Earth and an object on its surface to be the radius of Earth.]] | |||
The gravitational field describes the area that is created by a mass. The field exerts a force on the objects inside the field depending on the magnitude of the field and the mass of the object inside the field. The lines in the image below represent the field lines. The magnitude of the field is inversely proportional the the spacing of the lines. The direction of vector ''g'' will always be parallel to the field lines, which will always be equally spaced and distributed. Objects inside of Earth's gravitational field, feel the force called ''weight'' and in the case of Earth's gravitational field, the center of gravity is equal to its center of mass. As a result, we have the gravitational constant ''g''. | |||
[[File:Gravitational field Earth lines equipotentials.svg|thumb|Gravitational field lines]] | |||
To get the force of gravity in vector form, we can use the equation below. | |||
:: <math> \vec g = \frac{GM}{r^2} \hat r\ </math> | |||
'''Conceptual Question''': Say you are standing in the basement of a building and weigh yourself. Then you immediately go to the 10th floor of the same building and weigh yourself again. Is your weight the same? | |||
::Your weight is ''not'' the same, however the significance that it changes is negligible if you are just traveling to the top of a building. Although you are further from the Earth's center of mass, the difference in distance from the Earth's center of mass is too small to significantly change your weight. Although your weight may change in varying levels due to your distance from Earth's surface, your mass will always stay the same. This is because <math> {F} = {ma} </math> | |||
===A Computational Model=== | ===A Computational Model=== | ||
Using the approximation derived above, we can create a computational model for the force of gravity near Earth's surface by applying Newton's second law in an iterative fashion to update acceleration, velocity, and finally position. This allows us to simulate the motion of an object near Earth's surface using only its mass. Seen below is a GlowScript code snippet accomplishing this iterative update technique. | Using the approximation derived above, we can create a computational model for the force of gravity near Earth's surface by applying Newton's second law in an iterative fashion to update acceleration, velocity, and finally position. This allows us to simulate the motion of an object near Earth's surface using only its mass. Seen below is a GlowScript code snippet accomplishing this iterative update technique. | ||
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==History== | ==History== | ||
Prior to the age of Newton, gravity as a force was a totally foreign concept. During the 17th century, Galileo realized that all objects, regardless of mass, fall with the same acceleration towards Earth. It was in 1687 when Newton published his ''Principia'' that he hypothesized that gravity acts as a force whose magnitude is inversely proportional to the square of distance between objects. This description was incomplete, however, and remained unfinished until Cavendish determined the value of ''G'', the universal gravitational constant. | Prior to the age of Newton, gravity as a force was a totally foreign concept. During the 17th century, Galileo realized that all objects, regardless of mass, fall with the same acceleration towards Earth. It was in 1687 when Newton published his ''Principia'' that he hypothesized that gravity acts as a force whose magnitude is inversely proportional to the square of distance between objects. This description was incomplete, however, and remained unfinished until Cavendish determined the value of ''G'', the universal gravitational constant. The purpose of this venture was to eventually determine the mass of Earth, which one he found the value of ''G'', he could determine. | ||
==Connectedness== | |||
1.How is this topic connected to something that you are interested in? | |||
:: I am personally interested in our solar system, and how the planets have orbited each other. The gravitational fields of each planet and their moons control how how solar system orbits. | |||
2. How is it connected to your major? | |||
::As a civil engineering major, in general understanding the laws of physics ensures that the tools and construction we create are safe and realistic. Research on gravitational fields has allowed civil engineers to test the bounds of construction, and also know when gravitational fields need not be considered. | |||
3. Is there an interesting industrial application? | |||
The leaning tower of Pisa is an example of civil and structural engineers using gravitational fields to their advantage. They calculated the center of mass of the tower, and the center of mass is not outside of the base, allowing it to tilt without ever falling. | |||
==See Also== | ==See Also== | ||
Latest revision as of 18:58, 4 December 2022
[Nahli Jinks Fall 2022] This section describes gravitational force near Earth's surface, including applications and relevant derivations.
Main Idea
Near Earth's surface, the magnitude of acceleration due gravity is approximately constant. Newton's Law of Universal Gravitation states that any two bodies attract each other with a force directly proportional to the product of the masses and inversely proportional to the square of the distance between the objects. If we approximate the Earth as a point mass, we find that the distance to the surface is simply the radius of the Earth. We now want to apply Newton's Law of Universal Gravitation to our approximation and see if we can calculate the acceleration due to gravity near Earth's surface. Generally this is only acceptable because the distance between the object of interest and Earth's surface is [math]\displaystyle{ \lt \lt }[/math] the distance from the center of the Earth to Earth's surface. Thus the difference in distances is so small that the result is well-approximated using only Earth's radius.
A Mathematical Model
From Newton's Law of Universal Gravitation we know:
- [math]\displaystyle{ {F}_{grav}=G \frac{m_1 m_2}{r^2}\ }[/math]
Where
- F is the gravitational force between the masses;
- G is the gravitational constant, [math]\displaystyle{ 6.674×10^{−11} \frac{N m^2}{kg^2}\ }[/math];
- m1 is the mass of the first object;
- m2 is the mass of the second object;
- r is the distance between the objects.
Since the only forces acting on a object in free fall near earth's surface are it's weight, (mass and gravity), we can set [math]\displaystyle{ {F}_{grav} = {mg} }[/math] ,and then plug that into Newton's Law of Universal Gravitation. After canceling out the constants, we arrive at the gravitational constant for a free falling object near earth.
- [math]\displaystyle{ {g} = \frac{GM_{Earth}}{R_{Earth}^2} }[/math]
Near Earth's surface g is unchanging. As such, we define it as the gravitational constant near Earth's surface, g, which is approximately [math]\displaystyle{ 9.8 \frac{m}{s^2} }[/math]. This calculation is shown below:
- [math]\displaystyle{ C= \frac{(6.67*10^{-11} \frac{m^3}{kgs})(5.972*10^{24} kg)}{(6.378*10^{6} m)^2} = 9.8 \frac{m}{s^2} }[/math]
This then puts the force near Earth due to gravity into a much simpler form:
- [math]\displaystyle{ |\vec{\mathbf{F}}_{grav}|= mg }[/math]
Where
- g is the near-Earth gravitational constant, as defined above to be [math]\displaystyle{ 9.8 \frac{m}{s^2} }[/math]
- m is the mass of the object whose behavior we are interested in
The gravitation constant g applies to all masses significantly smaller than Earth's mass. These masses will all fall at the same acceleration.
The Gravitational Field
The gravitational field describes the area that is created by a mass. The field exerts a force on the objects inside the field depending on the magnitude of the field and the mass of the object inside the field. The lines in the image below represent the field lines. The magnitude of the field is inversely proportional the the spacing of the lines. The direction of vector g will always be parallel to the field lines, which will always be equally spaced and distributed. Objects inside of Earth's gravitational field, feel the force called weight and in the case of Earth's gravitational field, the center of gravity is equal to its center of mass. As a result, we have the gravitational constant g.
To get the force of gravity in vector form, we can use the equation below.
- [math]\displaystyle{ \vec g = \frac{GM}{r^2} \hat r\ }[/math]
Conceptual Question: Say you are standing in the basement of a building and weigh yourself. Then you immediately go to the 10th floor of the same building and weigh yourself again. Is your weight the same?
- Your weight is not the same, however the significance that it changes is negligible if you are just traveling to the top of a building. Although you are further from the Earth's center of mass, the difference in distance from the Earth's center of mass is too small to significantly change your weight. Although your weight may change in varying levels due to your distance from Earth's surface, your mass will always stay the same. This is because [math]\displaystyle{ {F} = {ma} }[/math]
A Computational Model
Using the approximation derived above, we can create a computational model for the force of gravity near Earth's surface by applying Newton's second law in an iterative fashion to update acceleration, velocity, and finally position. This allows us to simulate the motion of an object near Earth's surface using only its mass. Seen below is a GlowScript code snippet accomplishing this iterative update technique.
- Fnet = vector(0, -g, 0)
- ball.vel = ball.vel + Fnet / ball.m * deltat
- ball.pos = ball.pos + ball.vel * deltat
Examples
Introductory
Suppose a 50 kg man stands on the Earth's surface. What is the magnitude of the gravitational force experienced by the man?
First notice that since we are near Earth's surface, it is appropriate to use our approximation of gravitational force rather than Newton's Law of Universal Gravitation. As such, recall [math]\displaystyle{ |\vec{\mathbf{F}}_{grav}|= mg }[/math]. Here, m is equal to 50 kg, and g is equal to [math]\displaystyle{ 9.8 \frac{m}{s^2} }[/math]. This means that:
- [math]\displaystyle{ |\vec{\mathbf{F}}_{grav}|= mg = (50 kg)(9.8 \frac{m}{s^2}) = 490 N }[/math]
Intermediate
A person is laying on their back and pushing a 20 kg weight straight up (they're bench pressing the weight). What is the magnitude of the force they must be exerting on the weight if the weight is moving straight up without any acceleration?
We know from Newton's Second Law that force is directly proportional to acceleration. Thus if acceleration is zero, net force must also be zero and the weight will move at a constant velocity. This means that the force exerted by the person must be equal in magnitude to the force of gravity on the object (since they act in exactly opposite directions).
- [math]\displaystyle{ F_{g}=F_{person}=mg }[/math]
- [math]\displaystyle{ F_{person}=(20 kg)(9.8 \frac{m}{s^2})=196 N }[/math]
Advanced
Suppose a 60 kg person is standing in an elevator that is accelerating upwards at [math]\displaystyle{ 1 \frac{m}{s^2} }[/math]. If they are standing on a scale, what does that scale read while the elevator accelerates upwards? A picture illustrating the situation is attached.
Here, the net acceleration is the same as that of the elevator, which is [math]\displaystyle{ 1 \frac{m}{s^2} }[/math]. The mass is 60 kg. In order to determine the weight that the scale reads, we must look at the normal force exerted by the scale.
The above means that the net force is in the upwards direction.
- [math]\displaystyle{ |\vec{\mathbf{F}}_{net}|=F_{N}-mg=ma }[/math]
- [math]\displaystyle{ F_{N}=m(a+g) }[/math]
- [math]\displaystyle{ F_{N}=(60 kg)(1 \frac{m}{s^2} +9.8 \frac{m}{s^2}) = 648 N }[/math]
Importance
Understanding gravity and its applications is fundamental to building intuition for our universe. On a small scale, we can use our knowledge of Earth's intrinsic qualities to simplify many basic physics problems and better understand the world around us, but the approximation scheme described here can be used for any (relatively uniform) bodies, including other planets in our solar system, extending its usefulness to beyond just Earth's surface. In particular, the ideas in this article help to show why a scale would show different values depending upon the planet on which it's placed (try calculating your weight on the moon, for instance).
From an industrial perspective, understanding gravitational force near Earth's surface is important because it may affect the design process for various products. When designing a bridge, for instance, one must verify that the force on the bridge due to gravity will not be strong enough to undermine the bridge's stability. Even when making a lamp it's important to check that a joint is powerful enough to withstand the torque experienced by the object due to the force of gravity near Earth's surface.
History
Prior to the age of Newton, gravity as a force was a totally foreign concept. During the 17th century, Galileo realized that all objects, regardless of mass, fall with the same acceleration towards Earth. It was in 1687 when Newton published his Principia that he hypothesized that gravity acts as a force whose magnitude is inversely proportional to the square of distance between objects. This description was incomplete, however, and remained unfinished until Cavendish determined the value of G, the universal gravitational constant. The purpose of this venture was to eventually determine the mass of Earth, which one he found the value of G, he could determine.
Connectedness
1.How is this topic connected to something that you are interested in?
- I am personally interested in our solar system, and how the planets have orbited each other. The gravitational fields of each planet and their moons control how how solar system orbits.
2. How is it connected to your major?
- As a civil engineering major, in general understanding the laws of physics ensures that the tools and construction we create are safe and realistic. Research on gravitational fields has allowed civil engineers to test the bounds of construction, and also know when gravitational fields need not be considered.
3. Is there an interesting industrial application? The leaning tower of Pisa is an example of civil and structural engineers using gravitational fields to their advantage. They calculated the center of mass of the tower, and the center of mass is not outside of the base, allowing it to tilt without ever falling.