Calculate the total force on the Earth

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SUMMARY

The discussion focuses on calculating the total gravitational force on Earth due to Venus, Jupiter, and Saturn, using the formula F = Gm1 m2/r^2. The masses of the planets are given as MV=0.815ME, MJ=318ME, and MSat=95.1ME, where ME is the mass of Earth. Participants suggest starting with a normalized mass for Earth and then substituting the actual mass into the final equation after researching it online. The importance of identifying relevant equations from textbooks rather than relying on provided information is emphasized.

PREREQUISITES
  • Understanding of gravitational force calculations
  • Familiarity with the formula F = Gm1 m2/r^2
  • Knowledge of planetary masses relative to Earth
  • Ability to interpret astronomical distances in millions of kilometers
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  • Research the gravitational constant G and its application in force calculations
  • Learn how to calculate gravitational forces between multiple bodies
  • Study the mass of Earth (ME) and its significance in gravitational equations
  • Explore the concept of ratios in physics problems for simplification
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Students studying physics, particularly those focusing on gravitational forces and celestial mechanics, as well as educators seeking to enhance their teaching methods in these topics.

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Homework Statement
Calculate the total force on the Earth due to Venus, Jupiter, and Saturn, assuming all four planets are in a line, as shown in the figure. The masses are MV=0.815ME, MJ=318ME, MSat=95.1ME, and the mean distances of the four planets from the Sun are 108, 150, 778, and 1430 million km
Relevant Equations
I was not given relevant equations, but I am assuming it is F = Gm1 m2/r^2
I am confused how I am supposed to figure out the answer if I do not know the mass of the earth? Do I just set it to 1 and use m1 and m2 as ratios?
 
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anajonicholson said:
Homework Statement:: Calculate the total force on the Earth due to Venus, Jupiter, and Saturn, assuming all four planets are in a line, as shown in the figure. The masses are MV=0.815ME, MJ=318ME, MSat=95.1ME, and the mean distances of the four planets from the Sun are 108, 150, 778, and 1430 million km
Relevant Equations:: I was not given relevant equations, but I am assuming it is F = Gm1 m2/r^2

I am confused how I am supposed to figure out the answer if I do not know the mass of the earth? Do I just set it to 1 and use m1 and m2 as ratios?
Welcome to PF.

Yeah, I would start by doing that, then look up ME online and plug that into the final equation to get the total force. Can you show us that work?
 
Are all the planets on the same side of the Sun? You did not post the picture that goes with this. Also, don't expect a physics problem to give you the relevant equations for each problem separately. You are supposed to find which equation(s) is (are) relevant by reading the book. Nevertheless, you are supposed to post what you think is appropriate to make sure that you have thought about the problem and have done some background work. It seems that you have done that.
 
It is the weakest force in nature. The strength of the gravitational force is proportional to the product of the masses and inversely proportional to the square of the distance between them. so you can simply put values and add them all together.
 

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