Difference between revisions of "Structure of the Sun"
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| − | Questions in this category have been asked by MT, PJ, DC, EB | + | Questions in this category have been asked by MT, PJ, DC, EB, SR |
*Where are the convection & radiative zones? | *Where are the convection & radiative zones? | ||
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*What are the line-broadening mechanisms and where do they occur? | *What are the line-broadening mechanisms and where do they occur? | ||
| + | *What is the surface temp. of the sun? What is the core temp? | ||
Revision as of 16:23, 30 November 2007
Questions in this category have been asked by MT, PJ, DC, EB, SR
- 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?
- What is the surface temp. of the sun? What is the core temp?
