(c) Explain why convective instability occurs in hydrogen ionization zones within stars. (d) Estimate the main sequence

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(c) Explain why convective instability occurs in hydrogen ionization zones within stars. (d) Estimate the main sequence

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C Explain Why Convective Instability Occurs In Hydrogen Ionization Zones Within Stars D Estimate The Main Sequence 1
C Explain Why Convective Instability Occurs In Hydrogen Ionization Zones Within Stars D Estimate The Main Sequence 1 (52.13 KiB) Viewed 14 times
(c) Explain why convective instability occurs in hydrogen ionization zones within stars. (d) Estimate the main sequence lifetime of a 5 Mo star. Explain carefully all the assump- tions you have made in the calculation. The effective temperature of such a star is approximately 17000 K and its radius 2.7 times that of the Sun. The mass of a He nucleus is 6.6465 x 10-27 kg.
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