Magnitude of net Gravitational Force

In summary, the magnitude of the net gravitational force on the m2=10kg mass is 5.0867 Newtons and the direction of the net gravitational force is positive towards the x-axis.
  • #1
Jonwolf5400
1
0

Homework Statement


a) What is the magnitude of the net gravitational force on the m2=10kg mass? Assume m1=20kg and m3=15kg.
b) What is the direction of the net gravitational force on the m2=10kg mass? Assume m1=20kg and m3=15kg.

Homework Equations


F = G*m2*m3/R^2

The Attempt at a Solution


M2 x vector force
sin(26.565)*G*m2*m3/(0.223)^2
M2 y vector force
cos(26.565)*G*m2*m3/(0.223)^2

Total force
x vector
sin(26.565)*G*m2*m3/(0.223)^2 = 9.03796*10^-8
y vector
G*m2*m1/0.2^2 + cos(26.565)*G*m2*m3/(0.223)^2
= 5.0058*10^-7

magnitude
sqrt((9.03796*10^-8)^2+(5.0058*10^-7)^2) =
5.0867

angle
Don't know
 

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  • #2
Jonwolf5400 said:

Homework Statement


a) What is the magnitude of the net gravitational force on the m2=10kg mass? Assume m1=20kg and m3=15kg.
b) What is the direction of the net gravitational force on the m2=10kg mass? Assume m1=20kg and m3=15kg.

Homework Equations


F = G*m2*m3/R^2

The Attempt at a Solution


M2 x vector force
sin(26.565)*G*m2*m3/(0.223)^2
M2 y vector force
cos(26.565)*G*m2*m3/(0.223)^2

Total force
x vector
sin(26.565)*G*m2*m3/(0.223)^2 = 9.03796*10^-8
y vector
G*m2*m1/0.2^2 + cos(26.565)*G*m2*m3/(0.223)^2
= 5.0058*10^-7

magnitude
sqrt((9.03796*10^-8)^2+(5.0058*10^-7)^2) =
5.0867
You seem to be on the right track, but before we go any further, in what units is that answer? Your instructor may very well ding your answer for not specifying units. A simple number means little to nothing without units.

Beyond that, your answer may have some significant rounding errors. Try to work the problem symbolically before plugging the numbers in. This not only makes the problem simpler and easier to work with, but it also reduces rounding errors by reducing the number of numerical calculations.

Some useful identities are:

[itex] \sin \theta = \frac{\mathrm{opposite}}{\mathrm{hypotenuse}} [/itex]

[itex] \cos \theta = \frac{\mathrm{adjacent}}{\mathrm{hypotenuse}} [/itex]

[itex] \tan \theta = \frac{\mathrm{opposite}}{\mathrm{adjacent}} [/itex]

angle
Don't know

For the angle, you'll usually use an inverse trigonometric function such as [itex] \mathrm{arctan} \left( \frac{y}{x} \right) [/itex]. But it's up to you to draw out the triangle and specify the correct angle in the triangle for which you are looking. You'll need to specify what the angle is relative to ("relative to the positive x-axis," for example).

[Edit: It's also possible to specify directions with unit vectors. I'm not sure what your instructor wants, angles or unit vectors. I'm guessing an angle.]
 
Last edited:

1. What is the magnitude of net gravitational force?

The magnitude of net gravitational force refers to the strength of the attractive force between two objects due to their masses and the distance between them.

2. How is the magnitude of net gravitational force calculated?

The magnitude of net gravitational force can be calculated using the equation F = G(m1m2)/r^2, where F is the force, G is the universal gravitational constant, m1 and m2 are the masses of the two objects, and r is the distance between them.

3. What factors affect the magnitude of net gravitational force?

The magnitude of net gravitational force is affected by the masses of the two objects and the distance between them. The larger the masses, the stronger the force, and the greater the distance, the weaker the force.

4. How does the magnitude of net gravitational force change with distance?

The magnitude of net gravitational force decreases as the distance between two objects increases. This is known as the inverse-square law, where the force is inversely proportional to the square of the distance between the objects.

5. Why is the magnitude of net gravitational force important?

The magnitude of net gravitational force is important because it helps us understand the interactions between objects in the universe. It is also essential in explaining phenomena such as planetary motion and the formation of galaxies.

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