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Physics 20 Online
OpenStudy (anonymous):

The sun’s mass is about 2.7 x 107 times greater than the moon’s mass. The sun is about 400 times farther from Earth than the moon. How does the gravitational force exerted on Earth by the sun compare with the gravitational force exerted on Earth by the moon?

OpenStudy (anonymous):

@radar

OpenStudy (theeric):

Hello! We're looking for a comparison, so do you think that it would be okay to find a ratio? That's what my guess is.

OpenStudy (anonymous):

yes it is

OpenStudy (theeric):

Alright! So, the first step is to identify what we're given, because that and some general knowledge is what we have to start with. We're given a couple numbers, can you identify what one of them is?

OpenStudy (anonymous):

give me a seccond im in class connect ill be out in five

OpenStudy (theeric):

Okay!

OpenStudy (anonymous):

2.7 x 107 and 400

OpenStudy (anonymous):

@theEric

OpenStudy (theeric):

Okay, so those are the numbers (where the first number is probably \(22\times 10^7\). We are told that "The sun’s mass is about 2.7 x 107 times greater than the moon’s mass." So, \(sun's\ mass = 2.7\times10^7\ moon's\ mass\). So, to make the algebra easier to work with lets rename the variables. \(m_s\equiv sun's\ mass\) \(m_m\equiv moon's\ mass\) So now we can write \(m_s=2.7\times10^7\ m_m\)

OpenStudy (theeric):

With some algebra, we can now say what \(2.7\times 10^7\) means to physics:\[\frac {m_s}{ m_m} = 2.7\times10^7\]

OpenStudy (theeric):

Is that okay with you?

OpenStudy (anonymous):

perfectly fine

OpenStudy (theeric):

Alright! Now, it's your turn. The next number is about distance (a good variable would be \(d\) or \(r\)). So given that "the sun is about 400 times farther from Earth than the moon," use the same process that I did (or any other, really) to find what the "400" means to us.

OpenStudy (theeric):

Actually, don't even go that far.

OpenStudy (anonymous):

Fgs/Fgm = 2.7E7/400² = 169

OpenStudy (theeric):

If you just write that statement, you have the information that you need.

OpenStudy (anonymous):

so was that right

OpenStudy (theeric):

Yep! I didn't pull out the calculator, but that looks correct!

OpenStudy (theeric):

Looks good. Congrats! Take care!

OpenStudy (theeric):

Did you have any questions?

OpenStudy (anonymous):

could ya help me with like five more questions and thank you so much

OpenStudy (theeric):

Yep! Just ask them separately for the sake of other people who find each post. And, if you have already worked stuff out, let me know so I'm not tempted to drag you through the setup again! :)

OpenStudy (anonymous):

haha dont mind draggin me it might teach me a thing or two im all about learning seya on the next post

OpenStudy (theeric):

For anyone who looks up this answer after the fact, there are at least two simple algebraic ways to solve it, and I'll go through one. From the second piece of information, \(distance\ from\ sun = 400 \times distance\ from\ moon\) so \(r_s = 400\ r_m\) That's the given. Now we use our general knowledge. We want to compare gravitational force, so let's look at the ratio \[\frac{F_{g,s}}{F_{g,m}}\] Well, for any gravitational force between two masses,\[F_g=G\frac{m_1\ m_2}{r^2}\]That's the universal law of gravitation (so look that up if your unsure what it all means). For the gravitational force between the sun and the Earth, one mass is \(m_s\) and the other is \(m_E\) (for Earth's mass). For the gravitational force between the moon and the Earth, one mass is \(m_m\) and the other is still \(m_E\). So,\[F_{g,s} = G\dfrac{m_s\ m_E}{r_{s,E}^2}\]and\[\dfrac{1}{F_{g,m}} = \dfrac1G\dfrac{r_{m,E}^2}{m_m\ m_E}\] Put those together, some variables cancel, and your left with... \[\frac{F_{g,s}}{F_{g,m}}=\frac{m_s}{r_{s,E}^2}\frac{r_{m,E}^2}{m_m}=\left(\frac{m_s}{m_m}\right)\left(\frac{r_{m,E}}{r_{s,E}}\right)\left(\frac{r_{m,E}}{r_{s,E}}\right)\] Each factor in parenthesis can be derived from the information that is given in the problem.

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