Explorer
NVO HOME
EXPLORER HOME
TOOLS
HELP
PROJECTS
Projects
   Basic
   Advanced
     - H-R Diagram
   Teachers
   Other Projects


   H-R Diagram
   Making Diagrams
   Simple Diagram
   More Complete
   Nearest Stars
   Extending
   Parallaxes
   Distances
   Registry
   Interpreting
   Registry Results
   VizieR
   VizieR Results
   Final Diagram

Making a Final H-R Diagram

You now have enough data to make an H-R diagram for 3,803 stars. That's quite a few more than the 52 stars you used in Exercises 1 and 2!

Exercise 6. Use the graphing program to make an H-R diagram of the stars from the Gliese Catalogue. Remember to calculate the distance (in parsecs) from the parallax (in milliarcseconds). Create a new column in the spreadsheet with absolute magnitude using the equation

Mabsolute = mapparent - 5 log d + 5.

Then make a graph with b-v color on the x-axis and absolute magnitude on the y-axis. Don't forget to reverse the y-axis to put higher-luminosity stars toward the top. If you don't know how to do these tasks in your graphing program, see the virtualobservatory.org Graphing and Analyzing Data tutorial.

Question 14. Examine the diagram you just made. Compare it to the schematic H-R diagram you saw earlier. What groups do you see in the new diagram? Remember that the schematic diagram was just a theoretical guess, but the diagram you made in Exercise 4 comes from real data!

In this activity, you have learned what an H-R diagram is: a technique for studying the life cycles of stars by graphing their luminosities and temperatures. After making two simple diagrams, you used the NVO registry to search for data appropriate for making a diagram with many more stars. You used VizieR to get data from one survey, then created a graph of the data. So you have used real astronomical tools to download real data, which you used to make a real diagram! Congratulations!

Search Contact Us Feedback
Sponsored by the National Science Foundation under Cooperative Agreement AST0122449 with
The Johns Hopkins University. Developed in collaboration with the International Virtual Observatory Alliance.

Last Modified: Wednesday, June 21, 2006 at 5:22:47 PM by Jordan Raddick
Revision 1.4