States of matter
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Chemistry I · original Chapter 1 · combined Chapter 1
Section 2
States of matter
Temperature and pressure both affect state changes. At high temperatures, molecules have more energy and thus more freedom to move around. At high pressures, molecules are more constrained.
For example, the conditions for these changes in water are well known. When water reaches its melting point, 0°C, it changes from solid to liquid. When it reaches its boiling point of 100°C, it changes from liquid to gas.
Some characteristics of each state include:
Solid: is rigid and does not take either the shape or volume of container it is in.
Liquid: flows and takes up the shape, but not the volume, of that container it is in.
Gas: expands and takes up both the shape and the volume of the container it is in.
Example Problem 1.2.1
Water vapor is a gas, that means it takes the shape and volume of its container. If the flask measured 100 mL, then the volume of the gas would also be 100 mL.
As mentioned before, temperature and pressure greatly influence phase transitions, or the change from one phase (physical state) to another.
It should become clearer through the images that: lowering energy moves matter to a more ordered state (i.e. solid). Adding heat is giving energy to a system, whereas cooling a system takes away energy. A highly pressurized system is usually more ordered than a low pressurized system because the molecules are held more tightly together. These concepts are reinforced in Chapter 8 (Thermodynamics) but it is good to have a conceptual understanding.
How could you change molten steel into a solid steel bar?
Molten steel is a liquid, so to change it into a solid, it must be cooled down. This is a well-known process for many metals called metal casting.
The Fourth State of Matter
A fourth state of matter that was understood only recently is known as plasma. It is the most common fundamental state of matter found in the universe (though not on Earth). A gas becomes a plasma when it is heated so much that its electrons stop being restricted to a specific electron cloud and just start flying around everywhere!
This gives plasmas a property that regular gases don’t have: the ability to carry and conduct charge. Plasma is found in stars, lightning, and many other structures in the universe, such as nebulas (where stars are born).


