Estimating Mass Inside Galaxy Using Centrifugal Force

In summary, the conversation discusses using the constant velocity of a galaxy over a specific radius to estimate the mass within that radius. The individual is trying to use centrifugal force and gravitational force to derive the mass, but is unsure if the constant velocity will have an impact on the calculation. The other person in the conversation suggests using mechanics to solve the question.
  • #1
orange
28
0
I have another exam question, which I'm having some slight problems with...

"In a particular galaxy the velocity curve is constant over a large range of radii, and equal 300 km/sec at a particular radius of 10kpc in this range. Estimate the mass inside this radius."

Can I use centrifugal force equals gravitational force to derive M? This is what I'm trying to do. What I'm getting confused about, is if the constant velocity inside 10 kpc have any affect on M.

Very grateful for any help or suggestions!

Orange
 
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  • #2
well, the fact that the velocity is constant does say something about the mass of the galaxy as a whole, but in your case, since you're only dealing with mass in this radius, than you can use mechanics to solve your question.

Regards,

Nenad
 
  • #3
Jelly

Yes, you can use the equation for centrifugal force equaling gravitational force to estimate the mass inside the given radius. However, the constant velocity inside 10 kpc does not have any direct effect on the mass estimate. This is because the equation for centrifugal force is independent of velocity, and only depends on the mass and distance from the center of rotation. Therefore, the constant velocity at 10 kpc does not change the calculation for mass inside that radius. However, it is important to note that the velocity curve being constant over a large range of radii can indicate a more stable and evenly distributed mass distribution within the galaxy, which can affect the overall estimate of mass inside the given radius. It is also important to consider any other factors that may affect the velocity curve, such as the presence of dark matter. Overall, using the equation for centrifugal force can provide a good estimate of the mass inside the given radius, but it is important to consider all relevant factors and uncertainties in the calculation.
 

1. How is centrifugal force used to estimate mass inside a galaxy?

Centrifugal force is the outward force experienced by objects in circular motion due to their inertia. By measuring the speed and distance of stars and other objects within a galaxy, we can use the relationship between centrifugal force and gravitational force to estimate the mass of the galaxy.

2. What data is needed to estimate the mass inside a galaxy using centrifugal force?

To estimate the mass inside a galaxy using centrifugal force, we need to measure the orbital speed and distance of objects within the galaxy, such as stars or gas clouds. This data can be obtained through observations using telescopes or other instruments.

3. What assumptions are made when using centrifugal force to estimate galaxy mass?

One assumption is that the objects within the galaxy are in circular orbits. This may not always be the case, as some objects may have elliptical or irregular orbits. Additionally, we assume that the only force acting on these objects is gravity, neglecting other factors such as dark matter or interactions with other galaxies.

4. How accurate is the estimation of mass using centrifugal force?

The accuracy of the estimation depends on the quality of the data and the assumptions made. If the objects within the galaxy have mostly circular orbits and there is no significant presence of dark matter, the estimation can be quite accurate. However, if the galaxy has complex dynamics or significant amounts of dark matter, the estimation may be less accurate.

5. Can centrifugal force be used to estimate the mass of any type of galaxy?

Centrifugal force can be used to estimate the mass of any galaxy that has objects in circular motion. This includes spiral galaxies, elliptical galaxies, and irregular galaxies. However, the accuracy of the estimation may vary depending on the type of galaxy and its dynamics.

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