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Construct Your Own Problem

Consider the decay of radioactive substances in the Earth's interior. The energy emitted is converted to thermal energy that reaches the earth's surface and is radiated away into cold dark space. Construct a problem in which you estimate the activity in a cubic meter of earth rock? And then calculate the power generated. Calculate how much power must cross each square meter of the Earth's surface if the power is dissipated at the same rate as it is generated. Among the things to consider are the activity per cubic meter, the energy per decay, and the size of the Earth.

Short Answer

Expert verified

a) The activity of the earth rock in cubic meter is\(R = \frac{E}{{{E_\alpha }}}\).

b) Calculated power generate is\(P\)is\(\left( {1.6 \times {{10}^{ - 13}}} \right)q\;W\).

c) The power crosses per unit cubic meter is \(\left( {1.48 \times {{10}^{ - 33}}} \right)q\frac{{\rm{W}}}{{{{\rm{m}}^3}}}\).

Step by step solution

01

Definition of thermal energy

The energy contained within a system that is accountable for its temperature is referred to as thermal energy. The transfer of thermal energy is referred to as heat.

02

Activity of the earth rock in cubic meter

Consider the given problem.

The energy, the heat radiated and the volume of earth is related by the formula given by:

\(\begin{align}{}E & = \frac{Q}{{{V_e}}}\\E & = \frac{{q\,{\rm{MeV}}}}{{\frac{4}{3}\pi {{\rm{R}}^3}}}\end{align}\)

Where\(Q\) is the heat radiated,\(E\) is energy and the\({V_e}\) is the volume of earth

Now substitute the value of\(R & = 6380\;{\rm{km}}\) as the radius of earth is\(6380\;{\rm{km}}\)in the above equation

\(\begin{align}{}E & = \frac{{q\,{\rm{MeV}}/{\rm{s}}}}{{\frac{4}{3}\pi {{(6380\,{\rm{Km}})}^3}}}\\ & = \frac{{q\,{\rm{MeV}}/{\rm{s}}}}{{\frac{4}{3} \times 3.14{{\left( {6380 \times {{10}^3}\;\,{\rm{m}}} \right)}^3}}}\\ & = \frac{{q\,{\rm{MeV}}/{\rm{s}}}}{{1.09 \times {{10}^{21}}\;\,{{\rm{m}}^3}}}\end{align}\)

Thus, the activity of earth's rock is given by:

\(R & = \frac{{\rm{E}}}{{{{\rm{E}}_\alpha }}}\)

Therefore, the value of \(R\) is \(\frac{{\rm{E}}}{{{{\rm{E}}_\alpha }}}\).

03

Calculate the power generated

b)

Find the power generated.

The power generating is the energy per unit time\(P = E\).

so after plug in the value we get,

\(\begin{array}{c}P = q\,{\rm{MeV}}/{\rm{s}}\\ = \left( {1.6 \times {{10}^{ - 13}}} \right)\,q\;{\rm{J}}/{\rm{s}}\\ = \left( {1.6 \times {{10}^{ - 13}}} \right)\,q\;{\rm{W}}\\P = \left( {1.6 \times {{10}^{ - 13}}} \right)\,q\;{\rm{W}}\end{array}\)

Therefore, the value of \(P\) is\(\left( {1.6 \times {{10}^{ - 13}}} \right)q\;{\rm{W}}\).

04

The power crosses per unit cubic meter

c)

Let us solve the given problem.

The power crosses per unit cubic meter is\(p = \frac{{\rm{P}}}{{{{\rm{V}}_e}}}\).

Plug in the value we get ,

\(\begin{array}{c}p = \frac{{\left( {1.6 \times {{10}^{ - 13}}} \right)q\;{\rm{W}}}}{{1.09 \times {{10}^{21}}\;{{\rm{m}}^3}}}\\ = \left( {1.48 \times {{10}^{ - 33}}} \right)q\,\frac{{\rm{W}}}{{{{\rm{m}}^3}}}p\\ = \left( {1.48 \times {{10}^{ - 33}}} \right)q\,\frac{{\rm{W}}}{{{{\rm{m}}^3}}}\end{array}\)

Therefore, the value of \(t\) is \(\left( {1.48 \times {{10}^{ - 33}}} \right)q\frac{{\rm{W}}}{{{{\rm{m}}^3}}}\).

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Most popular questions from this chapter

Verify that a\(2.3 \times {10^{17}}\,{\rm{km}}\)mass of water at normal density would make a cube\(60\,{\rm{km}}\)on a side, as claimed in Example\({\rm{31}}{\rm{.1}}\). (This mass at nuclear density would make a cube\(1.0\,{\rm{m}}\)on a side.)

The Galileo space probe was launched on its long journey past several planets in 1989, with an ultimate goal of Jupiter. Its power source is\(11.0{\rm{\;}}\,{\rm{kg}}\)of \(^{{\rm{238}}}{\rm{Pu}}\), a by-product of nuclear weapons plutonium production. Electrical energy is generated thermoelectrically from the heat produced when the\({\rm{5}}{\rm{.59}}\,{\rm{MeV\alpha }}\)particles emitted in each decay crash to a halt inside the plutonium and its shielding. The half-life of\(^{{\rm{238}}}{\rm{Pu}}\)is\(87.7\)years.

  1. What was the original activity of the\(^{{\rm{238}}}{\rm{Pu}}\)in Becquerel?
  2. What power was emitted in kilowatts?
  3. What power was emitted\(12.0\)y after launch? You may neglect any extra energy from daughter nuclides and any losses from escaping \({\rm{\gamma }}\).
  1. What is the kinetic energy in MeV of a\({\rm{\beta }}\)ray that is traveling at\(0.998\,{\rm{c}}\)? This gives some idea of how energetic a\({\rm{\beta }}\)ray must be to travel at nearly the same speed as a\({\rm{\gamma }}\)ray.
  2. What is the velocity of the\({\rm{\gamma }}\)ray relative to the\({\rm{\beta }}\)ray?

There is more than one isotope of natural uranium. If a researcher isolates \(1.00\,{\rm{mg}}\) of the relatively scarce\({}^{{\rm{235}}}{\rm{U}}\) and finds this mass to have an activity of \(80.0\,{\rm{Bq}}\), what is its half-life in years?

The relatively scarce naturally occurring calcium isotope \(^{48}{\rm{Ca}}\) has a half-life of about \(2 \times {10^{16}}{\rm{y}}\). (a) A small sample of this isotope is labeled as having an activity of \(1.0\)Ci. What is the mass of the \(^{48}{\rm{Ca}}\)in the sample?

(b) What is unreasonable about this result?

(c) What assumption is responsible?

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