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

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)

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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