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What is the difference between fission and fusion?

Short Answer

Expert verified
Fission splits heavy nuclei; fusion combines light nuclei.

Step by step solution

01

Understanding Fission

Fission is a nuclear reaction in which a heavy atomic nucleus splits into two smaller nuclei along with a few neutrons and a large amount of energy. This process is usually initiated by the absorption of a neutron by the nucleus.
02

Features of Fission

In fission, the resultant nuclei (called fission fragments) are typically of intermediate mass. The process releases energy due to the conversion of mass into energy according to Einstein's equation, \(E = mc^2\). Nuclear fission is the principle behind atomic bombs and nuclear reactors.
03

Understanding Fusion

Fusion is a nuclear reaction in which two light atomic nuclei combine to form a heavier nucleus. This process releases a significant amount of energy and usually requires extremely high temperatures and pressures to overcome the electrostatic repulsion between the positively charged nuclei.
04

Features of Fusion

Fusion produces more energy per unit mass than fission and is the reaction that powers the sun and other stars. An example of a fusion reaction is the combining of two hydrogen isotopes, deuterium and tritium, to form helium and a free neutron, releasing energy.
05

Comparing Fission and Fusion

The main difference between fission and fusion is that fission splits a heavy nucleus into smaller nuclei, while fusion combines light nuclei to form a heavier nucleus. Fission is commonly used in nuclear reactors, while fusion powers stars and has potential for future clean energy sources.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Nuclear Fission
Nuclear fission occurs when a heavy atomic nucleus splits into two smaller ones. This often happens after the nucleus absorbs a neutron. As a result of this splitting, fission releases a significant amount of energy and a few neutrons. Each newly released neutron can trigger further fission reactions, creating a chain reaction which is fundamental to both nuclear reactors and atomic bombs. The energy release in fission occurs due to the conversion of mass into energy, as described by Einstein's equation.
Nuclear Fusion
Nuclear fusion involves the merging of two light atomic nuclei to form a heavier nucleus. For this process to occur, extremely high temperatures and pressures are needed to overcome the electrostatic repulsion between the positively charged nuclei. Fusion yields a large amount of energy and is the reaction that powers stars, including our sun. For example, when deuterium and tritium (two hydrogen isotopes) combine, they form helium and a neutron, releasing considerable energy. While not yet widely harnessed on Earth, nuclear fusion holds promise as a future energy source.
Energy Release
Both nuclear fission and fusion release substantial amounts of energy. This energy release stems from the conversion of a small amount of mass into energy. According to Einstein's equation, this relationship is given by: \(E = mc^2\). Here, \(E\) is energy, \(m\) is mass, and \(c\) is the speed of light. The conversion factor of \(c^2\) means even a tiny amount of mass can produce vast quantities of energy. This principle is what makes nuclear reactions so powerful.
Einstein's Equation
Einstein's equation, \(E = mc^2\), is crucial for understanding the energy release in both fission and fusion. This equation reveals that mass and energy are interchangeable. In nuclear reactions, a small amount of mass is converted into energy, leading to the tremendous energy outputs observed. For instance, in fission, the mass of the resulting fragments and neutrons is slightly less than the original nucleus. The 'lost' mass has been converted into energy. Similarly, in fusion, the mass of the fused nucleus is slightly less than the sum of the initial lighter nuclei, with the mass difference converted into energy.
Comparison of Fission and Fusion
While both fission and fusion are nuclear reactions that release energy, they operate in different ways. Fission splits a heavy nucleus into smaller nuclei, releasing energy and additional neutrons, which can lead to chain reactions. Fusion, on the other hand, combines light nuclei to form a heavier nucleus, demanding high temperatures and pressures.

Below are some key comparisons:
  • Fission is common in nuclear reactors, while fusion is the process powering stars.
  • Fusion releases more energy per unit mass compared to fission.
  • Fission produces radioactive waste, whereas fusion’s by-products are generally less harmful.

Understanding these differences helps in appreciating the potential applications and challenges of each process.

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Most popular questions from this chapter

A nuclear technician was accidentally exposed to potassium- 42 while doing some brain scans for possible tumors. The error was not discovered until \(36 \mathrm{~h}\) later when the activity of the potassium- 42 sample was \(2.0 \mu \mathrm{Ci}\). If potassium- 42 has a halflife of \(12 \mathrm{~h}\), what was the activity of the sample at the time the technician was exposed?

A vial contains radioactive iodine- 131 with an activity of \(2.0 \mathrm{mCi} / \mathrm{mL}\). If the thyroid test requires \(3.0 \mathrm{mCi}\) in an "atomic cocktail," how many milliliters are used to prepare the iodine-131 solution?

Fluorine- 18 , which has a half-life of \(110 \mathrm{~min}\), is used in PET scans. If \(100 . \mathrm{mg}\) of fluorine- 18 is shipped at \(8: 00\) A.M., how many milligrams of the radioisotope are still active if the sample arrives at the radiology laboratory at \(1: 30\) P.M.?

Naturally occurring iodine is iodine-127. The radioactive isotopes of iodine- 125 and iodine- 130 are used in nuclear medicine. a. Write the atomic symbol for each isotope. b. In what ways are the isotopes similar and in what ways do they differ?

Cesium-137, a beta emitter, has a half-life of \(30 \mathrm{y}\). a. Write the balanced nuclear equation for the beta decay of cesium-137. b. How many milligrams of a \(16-\mathrm{mg}\) sample of cesium- 137 would remain after \(90 \mathrm{y}\) ? c. How many years are required for \(28 \mathrm{mg}\) of cesium- 137 to decay to \(3.5 \mathrm{mg}\) of cesium- \(137 ?\)

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