Follow this link to skip to the main content

White Dwarfs - Try This!

White Dwarfs

Try this!

Using the H-R diagram below, compare the following properties of a white dwarf to those of a main sequence star such as our Sun. You must choose one value for each question.

An H-R Diagram, also know as the Hertzsprung-Russell diagram, is of great importance in the study of stellar evolution. It is a two-dimensional graph that demonstrates the correlation between the spectral type, temperature and luminosity of stars. It shows that 90% of stars lie along a diagonal band known as the main sequence. Remaining stars also form their own individual bands in different spectral type areas of the graph.

HR Diagram

  1. Would a white dwarf have a larger or smaller proportion of hydrogen then a main sequence star?

  2. Would a white dwarf be larger or smaller in size than main sequence stars?

  3. Would the density of a white dwarf be lower or higher than a main sequence star?

  4. Would the luminosity of a white dwarf be lower or higher than a main sequence star of the same temperature?

This activity was developed by Jacqueline Slay, Largo High School, Largo, MD



 

A service of the High Energy Astrophysics Science Archive Research Center (HEASARC), Dr. Alan Smale (Director), within the Astrophysics Science Division (ASD) at NASA/GSFC

NASA Logo, National Aeronautics and Space Administration
Goddard