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Unformatted text preview: composition? 3. When H burning ends what else appears to happen? Five solar Mass Star 0.25 0.5 0.75 1.0 Stars Lifetime ________________ Notes: Using the information above, work with your group to construct a comprehensive graph showing changes over time in the stars central density, temperature, pressure, surface temperature, luminosity, etc. Use a key, the notes section above or other means to clarify what the graph means for a reader.Prepare the graph to turn in as a group. Individual Conclusion post in submission box on Blackboard: A. Compare a one solar mass star to the 5 solar mass star, looking at what is different and what is the same. Pay particular attention to the places where things changewhere H runs out in the core for example, or where radius changes abruptly. B. Do the same for a 25 solar mass star, again compare changes and similarities....
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- Spring '08