The Sun's stability depends on hydrostatic equilibrium and ener... | Filo
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1. (Phillips, 1.3) As the Sun evolved towards the main sequence, it contracted under gravity while remaining close to hydrostatic equilibrium, and its internal temperatures changed from about 30,000 K to about 6 × 10^6 K. Find the total energy radiated during this contraction. Assume that the luminosity during this contraction is comparable to the present luminosity of the Sun, and estimate the time the Sun took to reach the main sequence.
1. (Phillips, 1.3) As the Sun evolved towards the main sequence, it con…
5 months ago
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