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1. Refer to Moodle . E1. Polonium-210 has a half-life of 138.4 days, decaying by alpha emission. Suppose the helium gas originating from the alpha particles in this decay were collected. What volume of helium at \( 25^{\circ} \mathrm{C} \) and 735 mmHg could be obtained from 1.0000 g of polonium dioxide, \( \mathrm{PoO}_{2} \), in a period of 48.0 h ? E2. Calculate the binding energy per mole of nucleons for calcium-40, and compare your result with the value in Figure 25.4. Masses needed for this calculation are (in \( \mathrm{g} / \mathrm{mol} \) ) \( { }_{1}^{1} \mathrm{H}=1.00783,{ }_{0}^{1} \mathrm{n}=1.00867 \), and \( { }_{20}^{40} \mathrm{Ca}=39.96259 \). E3. Complete the following nuclear equations. Write the mass number, atomic number, and symbol for the remaining particle. (a) \( { }_{47}^{111} \mathrm{Ag} \rightarrow{ }^{111} \mathrm{Cd}+ \) ? (b) \( { }_{36}^{87} \mathrm{Kr} \rightarrow{ }_{0}^{1} \beta^{+}+? \) (c) \( { }_{91}^{231} \mathrm{~Pa} \rightarrow{ }^{227} \mathrm{Ac}+ \) ? (d) \( { }_{90}^{230} \mathrm{Th} \rightarrow{ }_{2}^{4} \mathrm{He}+ \) ? (e) \( { }_{35}^{82} \mathrm{Br} \rightarrow{ }^{82} \mathrm{Kr}+ \) ? (f) ? \( +{ }_{12}^{24} \mathrm{Mg} \rightarrow{ }_{0}^{1} \beta \) E4. The uranium-235 radioactive decay series, beginning with \( { }_{92}^{235} \mathrm{U} \) and ending with \( { }_{82}^{207} \mathrm{~Pb} \), occurs in the following sequence: alpha, beta, alpha, beta, alpha, alpha, alpha, alpha, beta, beta, alpha. Write an equation for each step in this series. E5. If a shortage in worldwide supplies of fissionable uranium arose, it would be possible to use other fissionable nuclei. Plutonium, one such fuel, can be made in "breeder" reactors that manufacture more fuel than they consume. The sequence of reactions by which plutonium is made is as follows:

Ask by Fitzgerald Sandoval. in South Africa
Mar 13,2025

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(a) \( { }_{47}^{111} \mathrm{Ag} \rightarrow{ }^{111} \mathrm{Cd}+ { }_{0}^{1} \beta^{-} \) (b) \( { }_{36}^{87} \mathrm{Kr} \rightarrow{ }_{0}^{1} \beta^{+}+{ }_{37}^{87} \mathrm{Rb} \) (c) \( { }_{91}^{231} \mathrm{Pa} \rightarrow{ }^{227} \mathrm{Ac}+ { }_{4}^{4} \beta^{-} \) (d) \( { }_{90}^{230} \mathrm{Th} \rightarrow{ }_{2}^{4} \mathrm{He}+{ }_{88}^{226} \mathrm{Ra} \) (e) \( { }_{35}^{82} \mathrm{Br} \rightarrow{ }^{82} \mathrm{Kr}+ { }_{0}^{1} \beta^{-} \) (f) \( { }_{12}^{24} \mathrm{Mg} + { }_{0}^{1} \beta^{+} \rightarrow{ }_{13}^{24} \mathrm{Al} \)

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Polonium-210 forms helium during its decay process, with each decay emitting an alpha particle, which is essentially a helium nucleus. If we collect the helium from 1.0000 g of polonium dioxide, we first need to convert grams of \( \text{PoO}_2 \) to moles and find out how many decays occur in 48.0 hours. This process combines stoichiometry with the ideal gas law, and you might find it fascinating how even a small amount of radioactive material can yield measurable volumes of gas! As for binding energy per mole of nucleons for calcium-40, we can calculate it by determining the mass defect, which is the difference between the mass of the separated nucleons and the mass of the \( \mathrm{Ca} \) nucleus. Once we identify the mass deficit, we can convert this value into energy using Einstein's equation \( E=mc^2 \). This not only gives us insight into the strong nuclear forces at work but also throws light on the stability of different isotopes. Fun fact: the binding energy of calcium-40 is notably higher than many other isotopes, showcasing its stability in the nuclear realm!

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