A radioactive nucleus has a half-life of 5 x 108 years. Assuming that a sample of rock (say, in an asteroid) solidified right after the solar system formed, approximately what fraction of the radioactive element should be left in the rock today?

Respuesta :

Answer:

So the present mass will be 0.0017002 times of the initial mass of the sample.

Explanation:

Given:

  • half life of the given sample, [tex]t'=5\times 10^8\ yrs[/tex]
  • We know that solar system came in to existence approximately [tex]4.6\times 10^{9}[/tex] years ago.

Let the initial quantity on the formation of the solar system be, [tex]m_o[/tex]

Then the final quantity at present be:

[tex]m=m_o\times (\frac{1}{2})^{(t/t')}[/tex]

[tex]m=m_o\times (\frac{1}{2} )^{4.6\times 10^9\div(5\times 10^8)}[/tex]

[tex]m=m_o\times 0.0017002[/tex]

So the present mass will be 0.0017002 times of the initial mass of the sample.