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Questions and Answers
What is the Hertzsprung-Russell diagram?
What is the Hertzsprung-Russell diagram?
What is the Hertzsprung-Russell diagram (H-R diagram)?
What is the Hertzsprung-Russell diagram (H-R diagram)?
What is the Main Sequence?
What is the Main Sequence?
What are the three major groups of stars found on the H-R diagram?
What are the three major groups of stars found on the H-R diagram?
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What are the giants and supergiants?
What are the giants and supergiants?
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What can be inferred from the position of stars on the H-R diagram?
What can be inferred from the position of stars on the H-R diagram?
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What is the Stefan-Boltzmann relationship?
What is the Stefan-Boltzmann relationship?
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What is the Stefan-Boltzmann relationship?
What is the Stefan-Boltzmann relationship?
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What is the difference between supergiants and other stars?
What is the difference between supergiants and other stars?
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What are the three groups of M-class stars?
What are the three groups of M-class stars?
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What are white dwarfs?
What are white dwarfs?
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What are the characteristics of white dwarfs?
What are the characteristics of white dwarfs?
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Why does Procyon B have a smaller surface area than Barnard star?
Why does Procyon B have a smaller surface area than Barnard star?
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Which axis of the H-R diagram displays the luminosity of stars?
Which axis of the H-R diagram displays the luminosity of stars?
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What are colour-magnitude diagrams?
What are colour-magnitude diagrams?
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Study Notes
The Hertzsprung-Russell diagram (H-R diagram) is a useful and powerful plot in astrophysics that shows the relationship between temperature and luminosity of stars, and groups stars into distinct categories based on their position on the diagram.
The majority of stars, including our Sun, are found along a region called the Main Sequence, where hotter stars are more luminous.
Other major groups of stars found on the H-R diagram are the giants and supergiants, luminous stars that have evolved off the main sequence, and the white dwarfs.
The Stefan-Boltzmann relationship explains that the more luminous a star is, the bigger it is, and the difference between different groups of M-class stars is a difference in size.
Supergiants have the same effective temperature as other stars but have much higher luminosities due to their larger radii.
White dwarfs are very hot but have a very low surface area, meaning they are extremely small, roughly the size of Earth.
The scales on the axes of the H-R diagram can be confusing, with effective temperature decreasing from left to right, the highest temperature being on the left-hand side.
The vertical axis of the H-R diagram displays the luminosity of stars, either as a ratio compared to the Sun or as absolute magnitude.
When plotting stars in a specific open or globular cluster, apparent magnitude or V may be used instead of absolute magnitude.
Diagrams where V is plotted against colour index, B-V, are also known as colour-magnitude diagrams.
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Description
Test your knowledge of the Hertzsprung-Russell diagram with our quiz! Explore the different groups of stars found on the diagram and learn about the Stefan-Boltzmann relationship. See if you can navigate the confusing scales on the axes and understand the difference between absolute and apparent magnitude. Challenge yourself with questions about plotting stars in specific clusters and interpreting colour-magnitude diagrams. Sharpen your astrophysics skills and become an expert on the H-R diagram with our quiz.