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Nuclear Stability Nuclear Changes

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Presentation on theme: "Nuclear Stability Nuclear Changes"— Presentation transcript:

1 Nuclear Stability Nuclear Changes
Nuclear Chemistry Nuclear Stability Nuclear Changes

2 Nuclear Forces Forces that hold the neutrons and protons together in the nucleus. Nucleons: Combined term to represent the protons and neutrons in the nucleus of the atom.

3 Nuclide expression

4 Quarks The particles that make up protons and neutrons
Described in 6 flavors Up Down top Bottom Charm strange Only the up and down quarks make up the protons and neutrons Protons: 2 up quarks 1 down quark Neutrons 1 up quark 2 down quarks

5 Predicting Nuclear Stability
Nuclear binding energy: Energy released when nucleons combine to form a nucleus separate nucleons  nucleus + energy The mass of any atom is less than the combined masses of its separated parts. This difference in mass is known as the also called mass deflect.

6 Mass Deflect The equation E = mc2 shows energy can be converted into mass, and mass can be converted into energy. A small quantity of mass is converted into an enormous quantity of energy when a nucleus forms.

7 Nuclear Change Radioactivity Types of Particles released
The release of particles, or waves during the change from an unstable nuclei to a stable one Types of Particles released Alpha Beta Gamma Video

8 Nuclear Particles

9 Beta decay A neutron in an unstable nucleus may emit a high-energy electron, called a beta particle ( particle), and change to a proton. The mass number does not change because the total number of nucleons does not change

10 Radioactive Decay Rules for radioactive decay
Gamma: Release of a gamma ray Alpha: Release of an alpha particle

11 Nuclear Fission The splitting of a very heavy nucleus into 2 smaller atoms Chain reaction The continuation of nuclei breaking down from the products of other fission A minimum quantity of radioactive material, called critical mass, is needed to keep a chain reaction going.

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13 Nuclear Fusion video when small nuclei combine, or fuse, to form a larger, more stable nucleus In the sun, hydrogen nuclei fuse to form a single nucleus

14 Assignment Complete the Isotopes Worksheet
Work on Nuclear reactions worksheet


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