Mass of Earth: Homework Solutions & Equations

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SUMMARY

The mass of the Sun was calculated to be approximately 2.0058 x 1030 kg using the gravitational force equation and the orbital velocity of Earth. The volume of the Sun was determined to be 1.41 x 1027 m3, allowing for the calculation of its density. However, the discussion highlighted a challenge in determining Earth's density due to insufficient information regarding its mass and radius, necessitating external resources for accurate values.

PREREQUISITES
  • Understanding of gravitational force equations (e.g., Fg = GMm / r2)
  • Knowledge of orbital mechanics (e.g., centripetal acceleration and velocity calculations)
  • Familiarity with density calculations (Density = mass / volume)
  • Basic geometry for volume of a sphere (Volume = 4/3πr3)
NEXT STEPS
  • Research the gravitational constant (G) and its applications in astrophysics
  • Learn how to calculate the mass and radius of celestial bodies using observational data
  • Explore the concept of density in astrophysics and its significance in understanding planetary composition
  • Investigate resources for obtaining accurate measurements of Earth's mass and radius
USEFUL FOR

Students studying physics, particularly those focusing on gravitational forces and celestial mechanics, as well as educators seeking to clarify concepts related to planetary mass and density calculations.

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Homework Statement



Earth is a satellite of the Sun with an orbit radius of approximately 1.5×1011 m.
a) What is the Sun’s mass?
b) If the Sun’s radius is 6.96×108 m, how does the Sun’s density compare with Earth’s density?

Homework Equations



v^2 / r = ac

GMm / r^2 = Fg

The Attempt at a Solution



For a) I know Fg has to = ac for the planet to orbit without crashing into it or moving away.

I set them equal to each other and simplified.

v^2 / r = GMm / r^2

Which simplified to

v^2 / G = M

I found the velocity of Earth using the v = d / t

d = the distance around one orbit
t = the number of seconds in 1 year

The using the expression

v^2 / G = M

I derived the sun's mass which was 2.0058 x 10^30

Part b)

I know Density = m / v

I have the mass of the sun

To find the volume I just used the formula for the volume of a sphere

which is = 4/3Pir^3

Volume of the sun was = 1.41 x 10^27

Since I have volume of the sun and the mass, I can also get the density

What's causing me trouble is finding the mass of the Earth.

I tried using this method.

ma = GMm / r^2

Where m = 1kg
a = 9.8m/s^2

But the problem was the radius of earth. Is there a way to finding the radius? I've tried everything I can possibly do. Any help would be appreciated. Thanks in advance. :)
 
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There's not enough information given in the question statement for you to find the density of the Earth. You'll have to refer to some resource that gives Earth's mass and radius.
 
gneill said:
There's not enough information given in the question statement for you to find the density of the Earth. You'll have to refer to some resource that gives Earth's mass and radius.

Thank you! I thought that might be the problem, but since I found an answer to a) without any outside source (except G which I knew), I thought I could solve this with my previous knowledge. Thank you. :)
 

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