Chapter 9.2 Nuclear Radiation.

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Presentation transcript:

Chapter 9.2 Nuclear Radiation

An atom consists of a nucleus surrounded by electrons. The electrons are negatively charged.                                                                                                                               

The atom is held in place by an electric force of attraction between the positively charged protons and negatively charged electrons. The nucleus contains two types of particles: protons and neutrons.

A proton is positive and has a charge that is equal and opposite of the electron. A neutron has no charge and is neutral.

The atomic number of an atom is the number of protons in the nucleus of the atom. The mass number is the number of protons plus the number of neutrons is the nucleus.

An atom that has more or less protons than normal or found in nature is called an isotope. The force of attraction between the protons and neutrons is called the strong force.

To remove a proton or neutron from the nucleus of an atom, we must have a force that is greater than the strong force and therefore, work is required. The amount of work required to remove a proton or neutron is called the binding force.

There are 3 types of radiation: Alpha Radiation Beta Radiation Gamma Radiation

UV Light and Radiation

Geiger Counter Demo

Unstable protons and neutrons that emit radiation are called radioactive. Alpha and Beta are made up of particles while gamma is made up of energy.

A positively charged electron is called a positron and can be found in beta radiation. A positron is also known as an antiparticle or a particle of antimatter.

When neutrons split into smaller particles it is called fission. When one neutron splits it bumps into other neutrons and causes them to split. This is called a Nuclear Chain Reaction.

Theses nuclear chain reactions are self sustained which means they do not need additional energy once the reaction is started. These nuclear chain reactions is what makes nuclear reactors and bombs.

In fusion, two small nucleus are combined to form a larger nucleus.

Nuclear fusion is the source of energy for the stars, like our sun. To achieve fusion, nucleus must be heated to millions of degrees.