Understanding Newton's Law of Universal Gravitation

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Homework Help Overview

The discussion revolves around Newton's Law of Universal Gravitation, specifically calculating the gravitational force between the Earth and the Sun. Participants are working with the formula Fg=G(m1m2/r^2) and discussing the values of the masses and distance involved in the calculation.

Discussion Character

  • Exploratory, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • Participants are attempting to apply the gravitational force formula and are questioning which mass corresponds to m1 and m2. There is also confusion regarding the use of the gravitational constant G and how to incorporate it into their calculations.

Discussion Status

Some participants have provided guidance on the correct interpretation of the formula and the roles of the masses involved. There is an ongoing exploration of the calculations, with some expressing uncertainty about their progress.

Contextual Notes

Participants are working under the constraints of homework rules, which may limit the amount of direct assistance they can receive. There is also a noted confusion regarding the units and values used in the calculations.

Ecterine
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"Consider the Earth following its nearly circular orbit about the sun. The Earth has a mass mearth=5.98x10^24kg and the sun has mass msu=1.99x10^30kg. They are separated, center to center, by r=93 million miles = 150 million km."

What is the size of the gravitational force acting on the Earth due to the sun?

I'm still setting up the problem...

I think I use the equation Fg=G(m1m2 / r2).

r is the distance between the centers of the two objects.
G is the gravitational constant (so I just leave that as G, right?)

But, is the sun or the Earth m1?
 
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Wait... I just realized how stupid of a question that is. Why do I do this when I'm so tired?
 
K, so now for a better question!

Fg=G(5.98x10^24kg x 1.99x10^30kg / 150,000,000 km)
Fg=G(7.933 x 10^46)Am I on the right track? What do I do with the G?

I know that the gravitational constant G has a value G=6.67x10^-11 N x m2/kg2

If I plug the mass of the sun in as m2 it is...

G=6.67x10^-11 N x 1.99x10^30kg/kg2

but... now I'm lost. :(
 
Fg=(6.67x10^-11 N x 1.99x10^30kg / kg2) (7.933 x 10^46)

:(
 
Ecterine said:
"Consider the Earth following its nearly circular orbit about the sun. The Earth has a mass mearth=5.98x10^24kg and the sun has mass msu=1.99x10^30kg. They are separated, center to center, by r=93 million miles = 150 million km."

What is the size of the gravitational force acting on the Earth due to the sun?

I'm still setting up the problem...

I think I use the equation Fg=G(m1m2 / r2).

r is the distance between the centers of the two objects.
G is the gravitational constant (so I just leave that as G, right?)

But, is the sun or the Earth m1?


The formula for gravitation is F=GMm/R^2. Some people may prefer to rewrite it as F=GM1M2/R^2. Just need to take note that M1 or M is the primary mass and M2 or m is the secondary mass. In this question, the mass of Sun is taken to be M1 or M.

Data used:
Gravitational constant = 6.67x 10^-11 Nm^2kg^-2 = G
Mass of Sun = 1.99x 10^30 kg = M
Mass of Earth = 6.02x 10^24kg = m
Distance between Sun and Earth = 1.5x 10^11m = R

Force acting on Earth by Sun = GMm/R^2
= 3.39X 10^22 N
 
Thank you! :)
 

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