Sun and Earth Mass, Distance, and Center-of-Mass Problem: Exam Sample

  • Thread starter quickclick330
  • Start date
  • Tags
    Earth Sun
In summary, the conversation discusses a sample exam problem involving the mass and distance between the sun and a planet. The second equation mentioned is the third law of Johannes Kepler, which relates to the period and distance of a planet's orbit. The solution involves using the equations for centripetal force and gravitational force, and finding the distance between the center of mass of the sun and the center of mass of the Sun-Earth system.
  • #1
quickclick330
83
0
More sample exam problems...

2) The mass of our sun is ~ 2 x 10^30 kg. The mass of a planet is 6 x 10^24 kg. If the
distance between the center-of-mass of each is 100 x 10^11 m, what is the distance
in meters from the center-of-mass of the sun to the center-of-mass of the Sun-
Earth system?

What should I use to go about this problem? Thanks!
 
Physics news on Phys.org
  • #2
Well, you could start by writing down some relevant formulas, such as:

[tex]F_{g} = \frac{Gm_{1}m_{2}}{r^{2}}[/tex]

[tex]\frac{T_{A}^{2}}{r_{A}^{3}} = \frac{T_{B}^{2}}{r_{B}^{3}}[/tex]
 
  • #3
What is the second equation? I'm not familiar with that one.
 
  • #4
That is the third law of Johannes Kepler. ;-)
r: sun-planet distance
T: period
 
  • #5
That one would help. So how would you relate them together? Energy Principle?
 
  • #6
The second equation is what happens as a result of some fancy manipulation of centripetal force and gravitational force of attraction.
 
  • #7
ooh okay. I went to a help center and we had the centripetal force and gravitational force set equal to each other but the grad TA couldn't figure out how to get rid of velocity. So that second equation is really all i need right?
 
  • #8
Use the centripetal force as [itex]m\omega^2r[/itex] where [itex]\omega=\frac{2\pi}{T}[/itex] to not have v and have the period of revolution
 
  • #9
will r be the distance from planet to center of mass?
 
  • #10
Yes.
 
  • #11
I realize this is too late, but the help here has been quite bad. There is no need to invoke any of Kepler's laws to solve this problem. This is a simple problem. Quickclick, what is the equation of the center of mass for a group of particles?
 

FAQ: Sun and Earth Mass, Distance, and Center-of-Mass Problem: Exam Sample

What is the "Sun and Earth Problem"?

The "Sun and Earth Problem" refers to the scientific puzzle of how the Earth has been able to maintain a stable climate and habitable conditions for life despite receiving a relatively constant amount of energy from the Sun over millions of years.

Why is the "Sun and Earth Problem" important?

The "Sun and Earth Problem" is important because understanding the factors that influence Earth's climate and habitability can help us predict and mitigate the effects of climate change. It also allows us to better understand the potential for life on other planets with different solar energy input.

What are some proposed solutions to the "Sun and Earth Problem"?

Some proposed solutions include the greenhouse effect, which is the trapping of heat by Earth's atmosphere, and the role of the carbon cycle, which regulates the amount of carbon dioxide in the atmosphere and influences the planet's temperature. Other factors such as Earth's orbit, tilt, and geological processes also play a role.

How do scientists study the "Sun and Earth Problem"?

Scientists use a variety of methods, including computer simulations, laboratory experiments, and data analysis from sources such as ice cores and satellite observations. They also study other planets in our solar system and beyond to gain a broader understanding of the relationship between a planet's distance from its star and its habitability.

Is the "Sun and Earth Problem" solved?

While there is still much to learn about the complex interactions between the Sun and Earth, scientists have made significant progress in understanding the factors that contribute to Earth's stable climate. However, ongoing research and monitoring of our changing climate are necessary to continue improving our understanding and potentially find solutions to any future challenges that may arise.

Back
Top