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Physics Lesson 20.2.2 - Mass - Energy Equivalence

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Welcome to our Physics lesson on Mass - Energy Equivalence, this is the second lesson of our suite of physics lessons covering the topic of Nuclear Forces, Defect of Mass and Binding Energy, you can find links to the other lessons within this tutorial and access additional physics learning resources below this lesson.

Mass - Energy Equivalence

Consider an object of mass m moving linearly at a very high uniform speed, very close to the speed of light. Obviously, we denote this speed by c. Since the speed is uniform, there is a constant force F acting on the object during its motion. As a result, an energy E and momentum p are induced in the object, where

E = F ∙ d

and

p = m ∙ c

Here, d represents the distance travelled by the object during the process. We have used the scalar versions of formulae as we assumed the motion as linear.

Giving that the momentum gained during the process is equal to the impulse of object, we have

p = F ∙ t

where t is the duration of moving process. Thus, rearranging the last formula for F and substituting it in the first formula, we obtain

F = p/t ⇒ E = p ∙ d/t
= p ∙ c
= m ∙ c ∙ c

Thus, we obtain

E = m ∙ c2

This is the famous equation of mass-energy equivalence, introduced by Einstein. It implies that, despite the total mass of a system may change, the total energy and momentum remain constant. For example, if an electron and a proton collide with each other, this process destroys the mass of both particles but generates a large amount of energy in the form of photons. Now, you understand where does the m0 · c2 term discussed in article 18.6 when dealing with relativistic energy comes from. To avoid confusion we denoted this energy by ε instead of E and explained that it represents the stored energy in the object when it is at rest (we called it rest energy).

As you know, there are other forms of energy than just the rest energy and the kinetic energy. There is heat energy, chemical energy, binding energies of atoms and nuclei, etc. It turns out that all forms of energy are reflected in the total mass of the body. So although we have justified E = mc2 in terms of the kinetic energy, the mass-energy equivalence is quite a bit more general.

Example 1

How much energy a 200 g apple at rest would release if it was totally destroyed (not existed anymore)?

Solution 1

Clues:

m = 200 g = 0.2 kg
c = 300 000 km/s = 3 × 108 m/s
E = ?

The problem implies that the entire mass of the apple converts to energy. From the formula of mass-energy equivalence

E = m ∙ c2

we obtain after substitutions:

E = (0.2 kg) ∙ (3 × 108 m/s)2
= 1.8 × 1016 J

This value is enormous; it is 30 times greater than the energy released during the atomic bombing of Hiroshima (6 × 1014 J). However, it is not easy to convert mass into energy; this process requires very special appliances and the cost of this operation is extremely high.

You have reached the end of Physics lesson 20.2.2 Mass - Energy Equivalence. There are 3 lessons in this physics tutorial covering Nuclear Forces, Defect of Mass and Binding Energy, you can access all the lessons from this tutorial below.

More Nuclear Forces, Defect of Mass and Binding Energy Lessons and Learning Resources

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20.2Nuclear Forces, Defect of Mass and Binding Energy
Lesson IDPhysics Lesson TitleLessonVideo
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20.2.1Nuclear Force
20.2.2Mass - Energy Equivalence
20.2.3Binding Energy

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