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StudentWiki:StatesOfMatter

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States of Matter


General Principles

S.I. Units

These basic quantities are vital within physical chemistry (and obviously just in general).
It is also important to automatically understand the magitudes of various quantities. A chemist in general needs to know from mega- to femto- (or even atto-), i.e. the very small scale. A dirty physicist ( :P ) on the other hand needs to be aware of the macro scale of objects.

File:Time scale of molecular interactions.png
Time scale of molecular interactions.
Quantity Unit S.I. Unit Symbol
Mass Kilogram YES kg
Time Seconds YES s
Length Meter YES m
Electrical Potential Volt YES V
Temperature Kelvin YES K
Degrees Celcius NO °C
Moles Mole
(6.02 x 1023 molecules)
YES mol
Energy Joules YES J
Velocity Meters/second YES ms-1
Force Newton YES kgms-2 (N)
Pressure Pascal YES kgm-1s-2 (Nm-2 = Pa)
Bar NO 1 bar = 105 Pa
Atmosphere NO 1 atm = 1.01325 bar
Torr NO 1 atm = 760 Torr (1 Torr = 1 mmHg)
Magnitude (prefix) Mathematical Description
Mega 106
Kilo 103
Centi 10-2
Milli 10-3
Micro 10-6
Nano 10-9
Pico 10-12
Femto 10-15
Atto 10-18

Physical States

State Description
GAS Distance travelled between “collisions” is large compared to the size of the particle. Particles are free to move past each other - they have unimpeded movement.
LIQUID Distance travelled between “collisions” is comparable to the size of the particle. Particles are able to move past each other - “jostling with movement”.
SOLID Distance travelled between “collisions” is less than the size of the particle - continuous collisions. Particles are unable to move past each other - "jostling" but no movement.

Properties of Gases

A gas, as described previously, is a substance whose molecules are free too move without hindrance. Like liquids, they are capable of filling any container they're in.
The difference between a gas ana a liquid is simply that gas particles have a lot of space and time separating molecule collisions.
This has led scientists to question what the properties of a perfect gas are.


The Ideal Gas Law

A perfect (or ideal) gas is in fact a hypothetical substance, for it does not take into account molecular interactions that real gases experience.
The ideal gas law is one of the most important equations to know. It is given below:


PV=nRT


where:

  • P = pressure (Pa)
  • V = volume (m3)
  • n = number of moles (mol)
  • R = Universal Gas Constant (J mol-1 K-1)
  • T = temperature (Kelvin)


Its derivation can be summarised by the combination of three important observations:

Physical Law Observation Symbolic Description
Charles' Law At a constant pressure, the volume of a gas varies linearly with temperature. V=constant×T
at constant n, T
Boyle's Law' At a constant temperature, the pressure of a fixed amount of gas is inversely proportional to its volume. P×V=constant
at constant n, V
Avogadro's Principle At a given pressure and temperature, equal volumes of gas contain the same number of molecules.
This introduces the concept of molar volume, i.e. the volume occupies by 1 mol of gas (Vm).
V=constant×n
at constant P, T
Vm=V÷n

Boyle's Law and Charles' Law are examples of limiting laws, in other words they can only be applies to a certain range - in this case from p0