Starting from the mathematical expression for the Stefan-Boltzmann 6) law: L = 4TR²O$BT*, where ØSe is the Stefan-Boltzmann constant, R is the radius of the star and T is its temperature in Kelvin scale, verify that the isoradius lines in the HR Diagram must be parallel to each other.

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The isoradius lines are the green lines in the HR diagram

HR Diagram
106-
100 Ro
1000 Ro
105- 10 RO
104-
103- 1 RO
102.
101- 0.1 Ro
100.
10-1- 0.01 RO
10-2.
10-3 0.001 R©
10 -4+
40000
20000
10000
5000
2300
Temperature (K)
Luminosity (Lo)
Transcribed Image Text:HR Diagram 106- 100 Ro 1000 Ro 105- 10 RO 104- 103- 1 RO 102. 101- 0.1 Ro 100. 10-1- 0.01 RO 10-2. 10-3 0.001 R© 10 -4+ 40000 20000 10000 5000 2300 Temperature (K) Luminosity (Lo)
(1)
Starting from the mathematical expression for the Stefan-Boltzmann
law: L = 4tR?OSBT*, where gsR is the Stefan-Boltzmann constant, R is the
%3|
radius of the star and T is its temperature in Kelvin scale, verify that the
isoradius lines in the HR Diagram must be parallel to each other.
Transcribed Image Text:(1) Starting from the mathematical expression for the Stefan-Boltzmann law: L = 4tR?OSBT*, where gsR is the Stefan-Boltzmann constant, R is the %3| radius of the star and T is its temperature in Kelvin scale, verify that the isoradius lines in the HR Diagram must be parallel to each other.
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