HR Diagram Read Your Textbook: Foundations of Astronomy –Chapter 9, 10 Homework Problems Chapter 9...
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Transcript of HR Diagram Read Your Textbook: Foundations of Astronomy –Chapter 9, 10 Homework Problems Chapter 9...
HR Diagram• Read Your Textbook: Foundations of Astronomy
– Chapter 9, 10
• Homework Problems Chapter 9– Review Questions: 1, 4, 5, 7– Review Problems: 1-5– Web Inquiries: 1
• Homework Problems Chapter 10– Review Questions: 1, 2, 4, 6-8– Review Problems: 1-4, 8– Web Inquiries: 2
Intrinsic Brightness vs Spectral TypeA.K.A. Luminosity vs Temperature
• HR diagram
Stars within 5 parsecs
• HR diagram
100 Brightest Stars
• HR diagram
Luminosity Function
Spectral Frequency
Luminosity Classes CLASS DESCRIPTION
I Supergiants
II Bright giants
III Giants
IV Subgiants
V Main-sequence stars/dwarfs
Luminosity Classes
Spectral Luminosity Class SURFACE TEMPERATURE (K) LUMINOSITY (Lsun) RADIUS (Rsun) OBJECT
4000 0.1 0.7 K7 V MS
4000 20 10 K7 III giant
4000 3000 100 K7 I supergiant
Main Sequence Masses
Using The HR Diagram• Example 1: Spectroscopic Parallax
• Same Spectral Type– means same temperature
• Same Luminosity Class– means same size
• m-M = 5 log d - 5
• Determine Distance by observing (m ), and utilizing the HR diagram to assume (M ).
L/Lsun
O B A F G K M
Using The HR Diagram• Example 2: Size Determination
• Same Spectral Type– means same temperature
• Different Luminosity Class– means different size
L = 4R2T4 M = 0, Msun = 5
L/Lsun
O B A F G K M
Using The HR Diagram• Example 2: Size Determination
• Same Spectral Type– means same temperature
• Different Luminosity Class– means different size
L = 4R2T4 M = 0, Msun = 5
A difference in 5 magnitudes is 100x in brightness
4R2T4 = 100 4Rsun2T4
R2 = 100 Rsun2
L/Lsun
O B A F G K M
Using The HR Diagram• Example 2: Size Determination
• Same Spectral Type– means same temperature
• Different Luminosity Class– means different size
L = 4R2T4 M = 0, Msun = 5
A difference in 5 magnitudes is 100x in brightness
4R2T4 = 100 4Rsun2T4
R2 = 100 Rsun2 Therefore, R/Rsun = (100)1/2
L/Lsun
O B A F G K M
Fundamental Stellar Parameters