unit 1 Flashcards
Electromagnetic radiation
A wave said to have dual nature (can behave as a wave and a particle)
waves with wavelength between 10 ^-14 and 10 ^4 m.
Speed of light
2x10 ^8 m/s
forms of electromagnetic radiation
Radio Waves, Microwaves, infrared, ultraviolet, x rays, gamma rays
What is the equation that links the speed of light, frequency and wavelength
c=fλ
EMR can exist as a stream of particles called
photons
equation which links energy and frequency of a photon
E=hf
equation used to calculate the energy of 1 mole of photons
E=Lhf
Combination of c=λf and E=Lhf
E= Lhc/λ
Lhc =
0.12
flame colours
when some metals burn they emit bright colours. This is because excited electrons are falling to lower energy levels and emitting light
Atomic Emission Spectra stage 1
The gaseous element is excited using high temperatures. This causes electrons to be promoted to higher energy levels. Electrons are said to be “excited”
Atomic Emission Spectra stage 2
Electrons fall down from these higher levels and in doing so emit energy in the form of light. (photon)
Atomic Emission Spectra stage 3
the electrons which make a big transition have high energy, high frequency and small wavelength.
Atomic Emission Spectra stage 4
the electrons which make a big transition have low energy, low frequency and large wavelength.
Atomic Emission Spectra stage 5
the different wavelengths of light given off pass into a prism where they are refracted. the light with the shortest wavelength are refracted most. A line spectrum is produced
Atomic Emission Spectra stage 6
each element has its own characteristic line spectrum. This line spectrum is concrete evidence for the existence of fixed energy levels in atoms.
Atomic Emission Spectra stage7
each line in the spectrum corresponds to the energy given out when an excited electron falls to a lower energy level.
what are the different transitions within an atom
Lyman : energy level which the electron falls=1
(high f, low λ) Part of the spectrum where lines are seen= UV
Balmer: energy level which the electron falls=2
Part of the spectrum where lines are seen= visible
Paschen :energy level which the electron falls=3
(low f, high λ) Part of the spectrum where lines are seen= IR
Atomic emission spectroscopy (AES)
Each element has its own characteristic emission spectrum, which can be matched to an unknown sample.
The position of spectral lines identify which element is present.
The Intensity tells you the concentration of the element
Atomic absorption spectroscopy (AAS)
Similar to AES however the wavelengths and intensity of the radiation are absorbed, which are measured during the promotion of electrons.
atomic orbital
a region of space where an electron is likely to be found
Principle quantum number, n
relates to the overall size/ energy or the orbitals.
for example sodium has electron arrangement 2,81, the value of n would be 1,2,3 respectively.
angular momentum quantum number, l
each electron shell is further divided into subshells.
values range form 0,1,2,3
magnetic quantum number, mℓ
tells us the multiplicity(how many) and orientation or the orbitals
values range from -3,…..,3
Values of n and corresponding letter
0 - s
1- p
2- d
3- f
shapes of orbitals: s orbitals
spherical,
-ℓ= 0
-mℓ = 0
-1 value = 1 orbital
shapes of orbitals: p orbitals
figure of 8,
- ℓ = 1
-mℓ = -1,0,1
3 values = 3 orbitals
shapes of orbitals: D orbital
ℓ =2
mℓ = -2,-1,0,1,2
5 values = 5 orbitals
spin quantum number
values of +1/2 or -1/2
Pauli exclusion principle
No two electrons can have the same set of 4 quantum numbers. meaning that the number of electrons in an given orbitals cannot exceed 2 and if there are two electrons in an orbital they must have opposite spin
Hund’s rule
electrons fill orbitals singly with parallel spins. before spin pairing.
Aufbau principle
electrons fill lowest energy orbitals first
1s, 2s, 2p, 3s, 3p, 4s, 3d
degenerate orbitals
orbitals with the same energy
Ionising energy
ionising energy increases across a period as more protons mean more pull
why ionising energy differs
if you are taking an electron form a full stable sunshell
if you are taking it from a half full subshell
the periodic table is split into 4 blocks
s d p
f
this is because the last letter/ orbital filled defines what black the element is in.
shapes of molecules
the shape of a molecule is determined by the number of bonding and nonbonding electron pairs.
given that a bond is a share of a pair of electrons, both being negatively charged they repel each other. the molecule adopts a shape which will minimise repulsion and maximise separation.