Lesson_5.3 - Lesson 5.3 Nuclear Energy Nuclear binding...

Info iconThis preview shows pages 1–3. Sign up to view the full content.

View Full Document Right Arrow Icon
Lesson 5.3 Nuclear Energy Nuclear binding energy and the mass defect A neutron has a slightly larger mass than the proton. These are often given in terms of an atomic mass unit, where one atomic mass unit (u) is defined as 1/12th of the mass of a carbon-12 atom. Is there something odd here? The carbon-12 atom has a mass of 12.000 u, and yet it contains 12 objects (6 protons and 6 neutrons) that each has a mass greater than 1.000 u. The fact is that these six protons and six neutrons have a larger mass when they're separated than when they're bound together into a carbon-12 nucleus. This is true for all nuclei, that the mass of the nucleus is a little less than the mass of the individual neutrons and protons. This missing mass is known as the mass defect , and is essentially the equivalent to the energy that binds the nuclear particles together called the binding energy. This is a measure of the energy that is needed to take the nucleus particles apart. Einstein's famous equation E = mc 2 establishes the equivalency of mass and energy. If you convert some mass to energy, Einstein's equation tells you how much energy you get. In any nucleus there is some binding energy, the energy you would need to put in to split the nucleus into individual protons and neutrons. To find the binding energy, then, all you need to do is to add up the mass of the individual protons and neutrons and subtract the mass of the nucleus. If m is the mass defect, then m = total mass of individual nucleon – the mass of the nuclesu The binding energy is then: Binding energy = m c 2 In a typical nucleus the binding energy is measured in MeV (million electron volts), considerably larger than the few eV associated with the binding energy of electrons in the atom. Nuclear reactions involve changes in the nuclear binding energy, which is why nuclear reactions give you much more energy than chemical reactions; those involve changes in electron binding energies. To judge the relative stability of nuclei, binding energy per nucleon is a better measure than absolute energy since large nuclei always have more binding energy than smaller ones. The following figure illustrates how binding energy per nucleon depends on the mass of a nucleus. The binding energy per nucleon varies widely from element to element. For hydrogen and helium it is very low, for iron it is at a maximum, and for elements beyond iron it decreases.
Background image of page 1

Info iconThis preview has intentionally blurred sections. Sign up to view the full version.

View Full DocumentRight Arrow Icon
The graph of binding energy per nucleon suggests that nuclides with a mass number larger than about 230 amu should spontaneously split apart to form lighter, more stable, nuclides. Such a process is called nuclear fission . Experimentally, we find that spontaneous fission reactions occur for only the very heaviest nuclides those with mass numbers of 230 or more. Even when they do occur, these reactions are often very slow. The half-life for the spontaneous fission of 238 U, for example, is 10 16 years, or about two million times longer than the age of our planet! We don't have to wait, however, for slow spontaneous fission reactions to occur. By irradiating
Background image of page 2
Image of page 3
This is the end of the preview. Sign up to access the rest of the document.

Page1 / 12

Lesson_5.3 - Lesson 5.3 Nuclear Energy Nuclear binding...

This preview shows document pages 1 - 3. Sign up to view the full document.

View Full Document Right Arrow Icon
Ask a homework question - tutors are online