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Systematic error
error due to the equipment accuracy or set up, ‘consistent’, cannot be averaged out
Random error
caused by human ability, different each time, can be averaged out, given by half the smallest division.
Accuracy
How close results are to the true value
Precision
a measure of how consistent you can be with your measurements
Tables should:
Plan the correct number of columns and rows to avoid adjustments later.
Use a ruler to create neat, straight lines.
Label columns and rows clearly with quantities and units (e.g., Temperature / °C) using slash notation to keep table values unitless.
Maintain consistency in significant figures.
For calculated differences, include initial, final, and difference values.
Add columns for simple conversions, like inverting or scaling.
no. of moles
m/M
Enthalpy change
-Energy/no. of moles
Unified atomic mass
the mass of one-twelth of the mass of a carbon 12 atom
Mole
the amount of a sumstance that contains the same number of stated elemtary units as there are atoms in 12g of Carbon-12
Relative molecular mass
the weighted average mass of a molecule in a given sample of that molecule compared to the vlue of the unified atomic mass
Relative formula mass
the weighted average mass of one formula unit compared to the value of the unified atomic mass
Relative atomic mass
the weighted average mass of atoms in a given sample of an element, compared to the value of the unified atomic mass
Relative isotopic mass
the mass of a particular atom of an isotope compared to the value of the unified atomic mass
Isotope
atoms of the same element which have the same atomic number nut different mass number
Heisenberg Uncertainty model
Everything we do affects the electrons so we cannot know both the speed and position at the same time
Relative abundance
different isotopes weigh differently - when one isotope is is more abundant, the relative atomic mass will be closer to that isotopic weight
mass spectometre
ionizes atoms and then sends them through an electromagnetic field where they are deflected on the basis of their mass and charge
Volatility
how easily a substance vaporizes
Ionization energies
the energy needed to remove 1mol of electrons from 1mol of atoms
Factors that affect ionization energy
less electrons in outer shell = less ionization energy (Nuclear Attraction)
more shells = less ionization energy (electron shielding)
bigger atomic radius = less ionization energy
Elastic collision
all energy is transfered
Inelastic collision
energy is lost (e.g through heat) during a collision
Ideal gas Law
a gas whose volume varies exactly in proportion to the temperature an exactly in inverse proportion to the pressure
R
Gas constant (8.31JK-1mol-1)
To convert to Kelvin
+237.15o
avagadros constant
6.02 × 1023
principle quantam number
number of shells
free radical
a species with one or more unpaired electron
Paul’s eulsion principle
No orbital may contain more than 2 electrons, the elctrons may not have the same spin.
Hund’s rule of ‘maximum mutiplicity’
when in orbitals of equal energy, electrons will try to remain unpaired
Aufbau (buildup principle)
electrons enter the lowest available energy level
molar second ionization energy
the nergy needed to remove one mole of electrons from one mole of gaseous plus 1 ions.
emperical formula
the simplest whole number ratio of atoms present in a compound
molecular formula
shows the exact number of molecules present
Atomic radius
As the Atoms get bigger, the valence electrons are further away and require less energy to be taken off.
Electron shielding
As atoms gain shells the inner electrons repel the outer electrons and the ionization energy decreases
Nuclear Attraction
the greater the number of protons in the nucleus, the greater the attractive forces on the outer electrons and therefore the greater the ionization energy.
fragmentation
the process in which a molecular ion breaks into smaller ions, radicals and/or neutral molecules.
free radical
a species with one or more unpaired elctrons
gas constant
8.31JK-1mol-1
To convert from degrees celsius to Kelvin
+273.15
Combustion formula
HxCy + (x+y/4)O2 → xCO2 + y/2H2O
Ideal gas Law formula
PV = nRT
electronegativity
The ability of an atom in a molecule to attrcat bonding electrons in a covalent bond to itself
Ionic bond
metal & non-metal - Electron transferred. Full charges on atoms
Nonpolar Covalent bond
Bonding lectrons shared equally between two atoms. No charges
Polar covalent bond
Bonding electrons shared unequally between two atoms. Partial charges on atoms
The pauling scale
measure electronegativity
Trend in Elctronegativity
Increases from bottom left to top right
avogadros constant value
6.02×1023
electronegativity difference of less than 0.5
bond type: pure Covalent
Electronegativity difference between 0.5 and 1.6
Bond type: polar covalent
Electronegativity difference 1.6 - 2.0 ( + a metal)
bond type: ionic
avogadros constant
the amount of particles in a mole
NO3-
Nitrate
CO32-
carbonate
SO42-
sulfate
OH-
Hydroxide
NH4+
ammonium
Zn2+
Zinc
Ag+
Silver ion
HCO3-
bicarbonate ion
PO43-
Phosphate
covalent bond
Non-metals react together, share electrons to gain full outer shells, there is electrostatic attraction between their nuclei
electron deficient
a compound in which the central atom’s octet is stable without complete octet. Boron, Beryllium, aluminium.
Expanded octet
Atoms from periods 3 or above expand their octet by moving s or p electrons into the d orbital
Dative covalent vond
one species donates a lone pair f electrons to another atom or ion.
Dimer
a molecule or molecular complex consisting of two identical molecules linked together.