Using the rotation curve above, fill in the rotational velocity for each indicated radius. Then, use this equation to calculate gravitational mass (in solar masses) at each radius. M = R where G = 4.31. 10-6 kpc km² Mos² Your values for M should be quite large, since we are talking about the mass of a galaxy! So, please express these large numbers in scientific notation. A Radius (kpc) 2 + 6 8 10 B Rotational Velocity (km/s) C Gravitational Mass (Mo) Sanity check: The mass should increase with larger radii, since you are calculating the total mass enclosed within each widening orbit.

College Physics
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Chapter1: Units, Trigonometry. And Vectors
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Radial velocity vs Radius from center
Using Newton's gravity equation, we will be able to determine the gravitational mass profile of the
galaxy. This is a plot that shows the redshifted portion of the galaxy (which is spinning away from
us) with the velocities corrected for inclination angle. So, the velocities in this graph represent the
true orbital velocities of the stars and gas at each point in the galaxy's disk.
Radial velocity, v (km s-¹)
175
150
125
100
75
50
25
O
0
Best-fit line
NGC 2742 data
8
1
2
3
Rotation curve for NGC 2742
Power law best-fit: v=aRb
where a 94 km s-¹ and b=0.28
4
5
6
Radius from center, R (kpc)
7
8
9
10
Transcribed Image Text:Radial velocity vs Radius from center Using Newton's gravity equation, we will be able to determine the gravitational mass profile of the galaxy. This is a plot that shows the redshifted portion of the galaxy (which is spinning away from us) with the velocities corrected for inclination angle. So, the velocities in this graph represent the true orbital velocities of the stars and gas at each point in the galaxy's disk. Radial velocity, v (km s-¹) 175 150 125 100 75 50 25 O 0 Best-fit line NGC 2742 data 8 1 2 3 Rotation curve for NGC 2742 Power law best-fit: v=aRb where a 94 km s-¹ and b=0.28 4 5 6 Radius from center, R (kpc) 7 8 9 10
Using the rotation curve above, fill in the rotational velocity for each indicated radius. Then, use
this equation to calculate gravitational mass (in solar masses) at each radius.
M = R where G = 4.31 10-6 kpc km²
Mos²
Your values for M should be quite large, since we are talking about the mass of a galaxy! So, please
express these large numbers in scientific notation.
A
Radius (kpc)
2
+
6
8
10
B
Rotational Velocity (km/s)
C
Gravitational Mass (Mo)
Sanity check: The mass should increase with larger radii, since you are calculating the total mass
enclosed within each widening orbit.
Transcribed Image Text:Using the rotation curve above, fill in the rotational velocity for each indicated radius. Then, use this equation to calculate gravitational mass (in solar masses) at each radius. M = R where G = 4.31 10-6 kpc km² Mos² Your values for M should be quite large, since we are talking about the mass of a galaxy! So, please express these large numbers in scientific notation. A Radius (kpc) 2 + 6 8 10 B Rotational Velocity (km/s) C Gravitational Mass (Mo) Sanity check: The mass should increase with larger radii, since you are calculating the total mass enclosed within each widening orbit.
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