Ch 9 Section 2 States of Matter Solids Particles packed closely together and constantly vibrating Fixed volume Fixed shape Ex: Rock Liquids Particles can slide past one another Definite volume No definite shape Ex: Liquid water Gas Particles are far apart and attractive forces are weak. No definite volume No definite shape Ex: Air you breath Plasma Matter consisting of positively and negatively charged particles No definite shape No definite volume Most common state of matter in the universe Ex: Sun Melting The temperature at which solids begin to melt is called the melting point Heat of fusion- energy required to change 1kg of a substance from a solid to a liquid. Freezing As a liquids temperature lowers the attractive forces of a liquid are strong enough to place the atoms in an ordered arrangement. The particles slow down enough so that the particles are able to come together and become a solid. Vaporization The energy of a liquid increases and some of the particles have enough energy to overcome the attractive forces between particles to change from a liquid to a gas. Vaporization that occurs at the surface is called evaporation. Boiling Occurs at certain temperature Boiling point is the temperature at which the pressure of the vapor in the liquid is equal to the external pressure acting on its surface. Heat of vaporization- the amount of energy required for 1 kg of the liquid at its boiling point to become a gas. Condensation When gas cools down to become a liquid. Ex: the water vapor in the air cooling and forming water droplets on a cold glass or soda can. Thermal expansion of solids As the temperature of a solid increases the molecules vibrate more and the attractive forces holding the solid together get weaker; this causes the material to expand. Thermal expansion in liquids As the temperature in a liquid increases the substance will expand. Thermal expansion of gases As the temperature of a gas increases it expands. As the gas expands it becomes less dense.
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