Lab #6. The Hertzsprung-Russell Diagram And Stellar Evolution

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Skip to: [content ] [navigation] Lab #6. The Hertzsprung-Russell Diagram and Stellar Evolution

Students explore the basic phases of stellar evolution on and beyond the Main Sequence, and learn to utilize a Hertzsprung-Russell (color-magnitude) diagram to understand the relationship between fundamental parameters for stars such as mass, luminosity, temperature, and age. A detailed study of the M67 cluster enables students to fit radial profiles to individual stars, place them on the cluster color-magnitude diagram, and then derive an age estimate for the cluster based on the Main Sequence turn-off point.

Resources

  • PDF laboratory exercise
  • Video tutorial
  • Web application #1: H-R diagram (courtesy NAAP)
  • Web application #2: M67 cluster
  • Report template (Google Drive or Microsoft 365)
  • PDF instructor supplement

  • Home
  • Lab Exercises
    • 1. Scientific Experiments
    • 2. Observing the Sky
    • 3. Lunar Cratering
    • 4. The Martian Surface
    • 5. Parallax
    • 6. Stellar Evolution
    • 7. The Distance Scale
    • 8. Galaxy Properties
    • 9. Spectrum Analysis
  • Getting Started
    • Angular Extents
    • Correlation Coefficients
    • Common xy Relationships
    • Google Documents/Drive
    • Keywords
    • Logarithmic Plots
    • Lunar Phase Wheel
    • Mean Values
    • Measurement Techniques
    • Percent Differences
    • Slopes and y-intercepts
  • Web Applications
    • AGN Spectra
    • BCG Images
    • BCG Spectra
    • Galaxy Images
    • Galaxy Mosaic
    • Galaxy Spectra
    • Histograms
    • Martian Craters
    • M67 Cluster H-R Diagram
    • Plotting Tool (D vs. v)
    • Plotting Tool (Distances)
    • Plotting Tool (General)
    • Plotting Tool (Illumination)
    • Representing Numbers
    • Scientific Notation
    • Stellar Spectra
Copyright © 2011-2024 Nicole P. Vogt. All rights reserved.

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