We actually observe a flat rotation curve in our own Milky Way. (You will show this with a radio telescope in your second lab!) This means v(r) is nearly constant for a large range of distances.
(a) Lets call this constant rotational velocity Vc. If the mass distribution of the Milky Way is spherically symmetric, what must be the M(< r) as a function of r in this case, in terms of Vc, r, and G?
In question number three we found a formula for the Keplerian rotation curve, v(r) for a mass m if the central mass is concentrated in a single point at the center (with mass Menc). The formula we found for that problem ended up being \[ v^2 = \frac{G M_{enc} }{r} \] Rearranging this formula for this specific question leads us to: \[M(< r) = \frac{ V_c^2 r }{G} \]
(b) How does this compare with the picture of the galaxy you drew last week with most of the mass appearing to be in bulge?
This approximation assumes the mass of the galaxy is constant as you go out from the center. We know that is not true because there is a quite heavy bulge in the middle of the milky way.
In our first assignment we learned that the mass of the Milky Way is \(10^{10} M_{\odot} \). Lets see how our calculations compare: \[ M_{MW} = 10^{10} M_{\odot} = 10^{10} \times 2 \times 10^{33} = 2 \times 10^{43} \: grams \] \[M(< 100 \: kpc) = \frac{ V_c^2 r }{G} = \frac{ (240)^2 (2 \times 10^{43}) }{6.67 \times 10^{-8}} = 8.6 \times 10^{54} \: grams \]
That is a huge discrepancy between the two masses. Something suspicious is afoot...
Good job Danielle...that is quite the discrepancy in part c though. I think you should be very careful about units. In particular, what are the units of V_c that you plugged in? Are these the same units used for r and G? Additionally, your mass of the MW seems to be off due to math. Other than the algebraic mistakes, you logic is spot-on! 4/5
ReplyDeleteHi Ashley! I definitely typed something in funny. I fixed the algebra now, at least from what I wrote down, hopefully that gives the right answer.
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