How much stuff will neutralise the sun's pull on the earth

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Discussion Overview

The discussion revolves around the theoretical question of how much mass, specifically in the form of protons, would be required to neutralize the gravitational pull of the Sun on the Earth through electromagnetic repulsion. Participants explore the interplay between gravitational and electromagnetic forces, using Coulomb's law and Newton's law of universal gravitation to frame their calculations.

Discussion Character

  • Exploratory
  • Technical explanation
  • Mathematical reasoning

Main Points Raised

  • One participant suggests starting with Coulomb's law to calculate the electromagnetic force and emphasizes the need to determine the distance between the Earth and the Sun.
  • Another participant mentions the importance of converting between Coulombs and kilograms of protons, noting that 1 mole of protons is equivalent to 1 gram.
  • It is proposed that the gravitational force can be calculated using the period and radius of the Earth's orbit, factoring in the mass of the Earth.
  • A participant points out that the radius cancels out in the equations, which may simplify the calculations.
  • Newton's law of universal gravitation and Coulomb's law are presented as equations that can be set equal to find the charge needed to balance the forces.
  • One participant hypothesizes that if both the Earth and Sun were composed entirely of protons, the electric repulsion would need to be reduced significantly to equal the gravitational attraction, suggesting specific masses of protons to be added to both bodies.
  • Another participant expresses interest in whether similar calculations have been done by others, indicating a desire for further exploration of the topic.

Areas of Agreement / Disagreement

Participants express various approaches to the problem, with no consensus on the exact calculations or methods. Some agree on the use of Coulomb's law and gravitational equations, while others raise questions about the assumptions and values used in the calculations.

Contextual Notes

There are limitations regarding the assumptions made about the nature of the forces and the simplifications in the calculations. The discussion does not resolve the complexities involved in accurately determining the required mass of protons.

bland
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I tried to make the title as descriptive as I could without being overly long.

Anyway, I've been trying to work this out but I'm having some difficulty. We all know the strength of the electromagnetic force is very much greater than the gravitational force. I'm not sure what it is as it's a number that seems to vary between 10^35 and 10^40 times depending on the source. And the mass of the Earth is 6 x 10^24kg.

For the sake of the argument, let's call the gravitational force 10^36 times weaker than the EM force and the mass of the Earth as 10^25kg

I was trying to work out given the above numbers, how many kg's of protons would need to be evenly spread through the sun and also evenly spread through the earth, such that the electromagnetic repulsion would be enough to overcome the pull of the gravitational attraction between the two objects (sun and earth) So that the Earth would float away.

At first I thought it would be simple to work out but after thinking about it for a while I realize that I don't really know how to do this.

I hope this makes sense.
 
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One place to start would be Coulomb's law. That gives you force in terms of charges and distance.

You'd need to figure out the distance between Earth and Sun.

You'd need to get a conversion factor between Coulombs and kilograms of protons. There are several ways to get that conversion factor. One way is to look up how many elementary charges per Coulomb, and how many elementary charges per mole. Then, a bit of background knowledge in chemistry is that 1 mole of protons (aka 1 mole of hydrogen nuclei) is 1 gram.

Then you'd need to repeat the exercise for the force of gravity between Earth and Sun. You could use the period and radius of the Earths orbit to arrive at the acceleration of the Earth in its orbit around the sun and factor in the mass of the Earth to get the force of gravity on the Earth by the sun.
 
jbriggs444 said:
One place to start would be Coulomb's law. That gives you force in terms of charges and distance.

You'd need to figure out the distance between Earth and Sun.

You'd need to get a conversion factor between Coulombs and kilograms of protons. There are several ways to get that conversion factor. One way is to look up how many elementary charges per Coulomb, and how many elementary charges per mole. Then, a bit of background knowledge in chemistry is that 1 mole of protons (aka 1 mole of hydrogen nuclei) is 1 gram.

Then you'd need to repeat the exercise for the force of gravity between Earth and Sun. You could use the period and radius of the Earths orbit to arrive at the acceleration of the Earth in its orbit around the sun and factor in the mass of the Earth to get the force of gravity on the Earth by the sun.

The radius of the orbit cancels out of the equations. No need to waste time figuring that factor.
 
dauto said:
The radius of the orbit cancels out of the equations. No need to waste time figuring that factor.

Good point, thanks. Though it depends on which known values and you Googled up to work from when computing the gravitational force and which equations you used with them.

If you calculated the gravitational force using the approach that I mentioned then would do not have a factor of 1/radius2 in the gravitational force to cancel against the factor of 1/radius2 in the electrostatic force.
 
Newton's law of universal gravitation says:

$$F_g=\frac{Gm_1m_2}{d^2}$$

Coulomb's law says:

$$F_e=\frac{kq_1q_2}{d^2}$$

Setting the two forces equal, you will get very simply:

$$k q_1 q_2=Gm_1m_2$$

If you assume ##q_1=q_2=q## you can solve that equation very easily to find q. From q, you need to use jbrigg's suggestion to find the mass of the protons involved.
 
Imagine the Earth and the sun both consisted completely of protons and had therefore a rediculous amount of charge. In that case the electric repulsion should be 10^36 times stronger than the attraction. That means the electric repulsion has to be reduced by a factor of 10^36 to make both forces equal.

That could for example be achieved by reducing the charge of both bodies by a factor of 10^18.
The sun's mass is 2 * 10^30 kg. Divided by 10^18 is 2 * 10^12 kg
Earth's mass is 6 * 10^24 kg. Divided by 10^18 = 6 * 10^6 kg

That means you'd have to add 2 * 10^12 kg of protons to the sun and 6 * 10^6 kg of protons to the earth.
 
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DrZoidberg said:
That means the electric repulsion has to be reduced by a factor of 10^36 to make both forces equal.

That could for example be achieved by reducing the charge of both bodies by a factor of 10^18.
The sun's mass is 2 * 10^30 kg. Divided by 10^18 is 2 * 10^12 kg
Earth's mass is 6 * 10^24 kg. Divided by 10^18 = 6 * 10^6 kg

That means you'd have to add 2 * 10^12 kg of protons to the sun and 6 * 10^6 kg of protons to the earth.

Interesting approach here. Has anyone worked it out the other way and gotten similar numbers?
 

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