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Imagine a hypothetical star of radius R, whose mass density ρ is constant throughout the star. The star is composed of a clas

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Mian daetyP atan Corn pasad dinog cn conditt n pon cun @ Sungate prR).。 Lero-destan ce Total, no.of nucltonh↓ N6-1 A TotalMas and nadiu R enaron law cie i 8 152.31 1-1 I L3 t(te.hny.. Ele e [. %e6 θ)y3 | da a. Tun be at al har qual ton リー R 4 kR

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