Difference between revisions of "Structure of the Sun"
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| − | Questions in this category have been asked by MT, PJ, DC | + | Questions in this category have been asked by MT, PJ, DC, EB |
*Where are the convection & radiative zones? | *Where are the convection & radiative zones? | ||
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**How has this been confirmed experimentally? | **How has this been confirmed experimentally? | ||
| − | + | * What is the energy produced for the reaction involving neutrino? | |
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| − | * What is the energy produced for the reaction involving neutrino? | + | |
** What are the experiments to detect the neutrinos and the reactions involve. | ** What are the experiments to detect the neutrinos and the reactions involve. | ||
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| + | *What are the line-broadening mechanisms and where do they occur? | ||
Revision as of 20:28, 10 March 2007
Questions in this category have been asked by MT, PJ, DC, EB
- Where are the convection & radiative zones?
- What causes the transition?
- How does opacity vary throughout the convective layer?
- What causes the opacity?
- How does the picture change for a 5 Solar Mass Star?
- What about at 0.2 Solar Mass Star? Why?
- Does the Sun rotate & how do we know?
- Where does it rotate fastest?
- Is it solid body rotation?
- How has this been confirmed experimentally?
- What is the energy produced for the reaction involving neutrino?
- What are the experiments to detect the neutrinos and the reactions involve.
- What are the line-broadening mechanisms and where do they occur?
