A star's Zero Age Main Sequence (ZAMS) radius R, luminosity L, and effective temperature Teff depend primarily on the star's mass. These parameters do evolve somewhat over time, however, while the star still remains on the main sequence. Discuss in what direction each of these parameters evolves, and explain why this occurs. By physical in your explanation. How did this evolution affect our own solar system, if at all?
A star's Zero Age Main Sequence (ZAMS) radius R, luminosity L, and effective temperature Teff depend primarily on the star's mass. These parameters do evolve somewhat over time, however, while the star still remains on the main sequence. Discuss in what direction each of these parameters evolves, and explain why this occurs. By physical in your explanation. How did this evolution affect our own solar system, if at all?
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Transcribed Image Text:A star's Zero Age Main Sequence (ZAMS) radius R, luminosity L, and effective temperature
Teff depend primarily on the star's mass. These parameters do evolve somewhat over
time, however, while the star still remains on the main sequence. Discuss in what direction
each of these parameters evolves, and explain why this occurs. By physical in your
explanation. How did this evolution affect our own solar system, if at all?
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