Meteorites created in the early solar system contaned aluminum-26, which is a
radioactive isotope of aluminum with a half-life of \(7.2 \times 10^5
\mathrm{yrs}\). Aluminum-26 decays first into an excited state of magnesium-26
via the reaction \({ }_{13}^{26} \mathrm{Al} \rightarrow{ }_{12}^{26}
\mathrm{Mg}^*+\mathrm{e}^{+}\), where the \(e^{+}\)has energy \(2.99
\mathrm{MeV}\). (The \(e^{+}\)is a positron; see previous problem. The asterisk
(*) indicates "excited.") The \({ }_{12}^{26} \mathrm{Mg}^*\) then decays into
the stable isotope magnesium- 26 via the reaction \({ }_{12}^{26} \mathrm{Mg}^*
\rightarrow{ }_{12}^{26} \mathrm{Mg}+\gamma\). The \(\gamma\) has energy \(1.8
\mathrm{MeV}\).
a) If you were asked to calculate the de Broglie wavelength of the positron,
would it be permissible to use Newtonian physics? Justify your answer.
b) What is the wavelength of the photon emitted when the excited magnesium-26
decays into its ground state? What is its momentum?
c) \({ }_{12}^{26} \mathrm{Mg}\) has an atomic mass of \(25.9826 \mathrm{u}\).
What is the speed of the recoiling nucleus when the photon is emitted?
d) What is the nucleus' kinetic energy in electron volts?
e) Precise measurements indicate that for a certain meteorite \(A\) the present
ratio \({ }^{26} \mathrm{Mg} /{ }^{27} \mathrm{Al}=5 \times 10^{-5}\), where \({
}^{27} \mathrm{Al}\) is the common, stable isotope of aluminum. For a meteorite
\(B\) the ratio is \({ }^{26} \mathrm{Mg} /{ }^{27} \mathrm{Al}=1.55 \times
10^{-7}\). Assuming that the different ratios are due to the difference in the
meteorites' times of creation, how much older is meteorite \(B\) than \(A\) ?