Additional Topic!
Gas Laws
The main distinguishing property of gases is their uncanny ability to be compressed into smaller and smaller spaces. Gases are also the least complex state of matter. Don't get it wrong, just because they are the simplest doesn't mean that they are not one of the most interesting and useful states of matter.
Boyle's Law
Mathematically Boyle's law can be expressed as P1V1 = P2V2
- V1 is the original volume
- V2 is the new volume
- P1 is original pressure
- P2 is the new pressure
Charles's Law
V / T =constant
- V is the volume
- T is the absolute temperature (measured in Kelvin)
Charles's Law can be rearranged into two other useful equations.
V1 / T1 = V2 / T2
- V1 is the initial volume
- T1 is the initial temperature
- V2 is the final volume
- T2 is the final temperature
V2 = V1 (T2 / T1)
- V2 is the final volume
- T2 is the final temperature
- V1 is the initial volume
- T1 is the initial temperature
Important: Charles's Law only works when the pressure is constant.
Note: Charles's Law is fairly accurate but gases tend to deviate from it at very high and low pressures.
Combined Law
This can be written as PV / T = constant. Since for a given amount of gas there is a constant then we can write P1V1 / T1 = P2V2 / T2.
- P1 is the initial pressure
- V1 is the initial volume
- T1 is the initial temperature (in Kelvin)
- P2 is the final pressure
- V2 is the final volume
- T2 is the final temperature (in Kelvin)
This equation is useful if you have the current volume, temperature, and pressure of a gas, and if you have two of the three final values of the gas.
Ideal Gas Law
- P is the pressure in atm
- V is the volume in liters
- n is the number of moles
- R is a constant
- T is the temperature in Kelvin
The constant R is calculated from a theroretical gas called the ideal gas. The most commonly used form of R is .0821 L * atm / (K * mol). This R will allow the units to cancel so the equation will work out.
Dalton's Law of Partial Pressure:
The pressure of a mixture of gases is equal to the sum of the pressures of all of the constituent gases alone.
Mathematically, this can be represented as:
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