Absolute magnitude 7 -6 5 4 3 2 7 0 Based on the figure, M = 0.3 & Cephel- kpc Type (classical) Cepheids Type II Cepheids RR Lyrae stars 1 3 10 Pulsation period (days) 30 104 103 10² 100 Luminosity, L/L Use the given average apparent magnitude to solve for the distance (in kpc). D = 10(m- (m-M+5)/5

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Hi! I just need help with the part circled in red. Thank you!

A globular cluster contains an RR Lyrae star with an observed pulsation period of 16 hours and an average apparent magnitude of 17.2.
What is the distance (in kpc) to the globular cluster?
If you measure the angular diameter to be 20 arc minutes, what is the linear diameter (in pc)?
Part 1 of 2
To determine the distance to the globular cluster, you need to use the magnitude-distance formula:
D = 10(m-M+5)/5
We can use the figure below to estimate the absolute magnitude of the RR Lyrae star.
Transcribed Image Text:A globular cluster contains an RR Lyrae star with an observed pulsation period of 16 hours and an average apparent magnitude of 17.2. What is the distance (in kpc) to the globular cluster? If you measure the angular diameter to be 20 arc minutes, what is the linear diameter (in pc)? Part 1 of 2 To determine the distance to the globular cluster, you need to use the magnitude-distance formula: D = 10(m-M+5)/5 We can use the figure below to estimate the absolute magnitude of the RR Lyrae star.
Absolute magnitude
-7
-6
50
4
3
2
-1
0
Based on the figure,
M =
0.3
& Cephel-
kpc
Type
(classical)
Cepheids
Type II
Cepheids
RR Lyrae stars
1 3
Pulsation period (days)
10 30
104
103
10²
100
Luminosity, L/L
Use the given average apparent magnitude to solve for the distance (in kpc).
D = 10(m- - M+5)/5
D =
Transcribed Image Text:Absolute magnitude -7 -6 50 4 3 2 -1 0 Based on the figure, M = 0.3 & Cephel- kpc Type (classical) Cepheids Type II Cepheids RR Lyrae stars 1 3 Pulsation period (days) 10 30 104 103 10² 100 Luminosity, L/L Use the given average apparent magnitude to solve for the distance (in kpc). D = 10(m- - M+5)/5 D =
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