Gravitational Force (Earth and Sun)

In summary, the conversation discusses determining the thickness of a steel cable that would replace the gravitational force between the Earth and the Sun. The equation F = m(4)(pi^2)(r)/t^2 is used, but the correct solution is found by simplifying the equation to find the cross-sectional area of the cable. This is done by dividing the maximum tensional force by the tensile strength of steel cable.
  • #1
jgens
Gold Member
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Homework Statement



To better comprehend the gravitational force between the Earth and the Sun, pretend gravity is turned off and the pull replaced by the tension in a steel cable joining them. How thick would such a cable need to be? You can estimate the diameter by knowing the tensile strength of steel cable is about 5.1 * 10^8 N/m^2.



Homework Equations



Any equations concerning gravitation/cirular motion.

The Attempt at a Solution



This is my attempt at a solution, the answer key says it's wrong.

F = m(4)(pi^2)(r)/t^2

d^2 = m(4)(pi^2)(r)/(t^2)(tensile strength)

thickness = m(4)(pi^2)/(t^2)(tensile strength)

thinkness = 465.45 m or 0.465 km

Where have I gone wrong in my calculations? Can someone please steer me in the right direction. Thanks.
 
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  • #2
jgens said:
F = m(4)(pi^2)(r)/t^2

OK.

d^2 = m(4)(pi^2)(r)/(t^2)(tensile strength)

Didn't understand.

Try to think simply.

Max tensional force/cross-sectional area of cable = tensile strength =>
Centripetal force/area = tensile strength.
 
  • #3




Your calculations are on the right track, but there are a few things to consider. First, the tensile strength of the steel cable is given in units of force per area (N/m^2), so it cannot be used directly in the calculation of thickness. Instead, you would need to use the cross-sectional area of the cable (which can be calculated from its diameter) to determine the force it can withstand.

Secondly, the equation you have used is for centripetal force in circular motion, which is not directly applicable to this scenario. Instead, you would need to use Newton's law of universal gravitation, which states that the gravitational force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.

So, the equation you would need to use is F = G(m1m2)/r^2, where G is the universal gravitational constant (6.67 * 10^-11 Nm^2/kg^2), m1 and m2 are the masses of the Earth and Sun respectively, and r is the distance between them.

Once you have calculated the force, you can use the cross-sectional area of the cable (based on its diameter) and the given tensile strength to determine the required thickness.

Hope this helps!
 

1. What is the gravitational force between the Earth and the Sun?

The gravitational force between the Earth and the Sun is approximately 3.54 x 1022 Newtons. This force is what keeps the Earth in its orbit around the Sun, and is responsible for the tides and the seasons on Earth.

2. How does the distance between the Earth and the Sun affect the gravitational force?

The gravitational force between two objects decreases as the distance between them increases. This means that the farther the Earth is from the Sun, the weaker the gravitational force between them will be.

3. What is the formula for calculating the gravitational force between the Earth and the Sun?

The formula for calculating the gravitational force between two objects is F = G(m1m2)/d2, where F is the force, G is the gravitational constant, m1 and m2 are the masses of the two objects, and d is the distance between them.

4. How does the mass of the Earth and the Sun affect the gravitational force between them?

The mass of the two objects directly affects the gravitational force between them. The greater the mass of an object, the stronger its gravitational pull will be. This means that the larger mass of the Sun is what allows it to exert a stronger gravitational force on the Earth.

5. Is the gravitational force between the Earth and the Sun constant?

No, the gravitational force between the Earth and the Sun is not constant. It can vary slightly due to factors such as the changing distance between the two objects, the gravitational pull of other planets, and the movement of the Earth's tectonic plates. However, these variations are relatively small and do not significantly affect the overall gravitational force between the two objects.

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