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Nature of matter, Seperation methods, structure of an atom, isotopes, electron configuration, line spectra, hydrogen emission spectra, main energy levels and sublevels,
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What can a matter be divided into?
Pure substances (compounds, elements), mixtures
what is a compound
two or more elements chemically bonded, fixed ratio
what is a element
1 type of atom, simplest form of an element, cant be broken down into anything simpler
what is a mixture
two or more different elements or compounds, not fixed ratio, either heterogenous or homogenous
what is a heterogenous mixture
non-uniform composition, visible layers
what is a homogenous mixture
uniform composition, non-visible layers
what are the different states of matter
gas, liquid, solid
factors of a gas
far apart, random, move quick in all directions
factors of a liquid
close together, random arrangement, move around each other
factors of a solid
close together, vibrate, regular pattern
what are the different changes of state
chemical change, physical change
what is a chemical change
making a new substance
what is a physical change
rearranging of particles
example of a physical change
ice (solid) → water (liquid) → steam (gas)
solid → liquid
meliting
liquid → gas
vaporization
gas → liquid
condensation
liquid → solid
freezing
solid → gas
sublimation (adding heat (endothermic))
gas → solid
deposition (remove heat (exothermic))
different separation methods
filtration, distillation, paper chromatography, solvation
what is filtration
separating particles based on size using a porous material (the filter)
what is distillation
separating particles by different boiling points
what is paper chromatography
separating particles by their different affinities
what are the phases in paper chromatography
mobile phase (solvent moves up the paper), stationary phase (paper)
what is solvation
separating particles based on their solubility in different solvents
what is a solvent
water or alcohol
example of solvation
adding salt to water
what are radioisotopes
unstable radioactive isotopes due to the number of subatomic particles (protons or neutrons) in the nucleus
what are radioactive isotopes
substance that has an unstable nuclei, emits radiation as it decays
subatomic particles
electrons, neutrons, protones
factors of the nucleus
very dense, positively charged, contains almost the whole mass of the atom
how much does the nucleus weigh
= 2.3 × 10^17 kg m-3
electron symbol
e-
electron relative charge
-1
electron relative mass
1/2000
proton symbol
p+
neutron symbol
n0
proton relative charge
+1
neutron relative charge
0
proton relative mass
1
neutron relative mass
1
what are ions
an atom that has either lost or gained an electron
what are positive ions
when atoms lose electrons
what are negative ions
when atoms gain electrons
example of positive ion
sodium loses 1 electron to form a 1+ ion
example of negative ion
fluorine can gain one electron to form a 1- ion
what is a isotope
atom of same element with different number of neutrons
what changes do isotopes have
isotopes of same element behave similarly in chemical reactions, different physical properties cause if the masses
how to calculate relative atomic mass, Ar
from the percent abundance and masses of the isotopes of the atime
what is percent abundance
percent of an isotope in a naturally occurring sample of an elements
calculation of Ar with percent abundance
mass of each isotope is multiplied by its percent abundance, these values are added together and then divided by 100
hydrogen isotopes
hydrogen -1 (mass # 1), hydrogen -2 (deuterium (mass # 2)), hydrogen -3 (tritium (mass # 3))
how many regions is the electromagnetic spectrum divided into
1-7 regions, low energy → high energy (radio waves → gamma rays)
realtionship between energy, frequency and wavelength
high energy = high frequency = low wavelength (vice versa)
how is an emission line spectra formed
when electrons transition from high → low energy levels
what do electrons emit when transitioning from high → low energy levels
emit energy
what does ele. tran. to n=3 emit
infrared radiation
what does ele. tran. to n=2 emit
visible light
what does ele. tran. to n=1 emit
ultraviolet radiation
what does an emission line spectra show
specific wavelengths or frequencies of electromagnetic radiation (colours)
what is a continous spectrum
shows all wavelengths or frequencies of visible light
at what speed do the 7 regions travel at
speed of light → 3 × 108 m s -1
what is the continuous spectrum produced by
hot liquids
hot gas under pressure or plasma from sun
hot solids (glowing filament in an incandescent globe)
what happens to the lines on an emission spectra
converg (closer together) at high energy (high frequency, low wavelength)
how can electrons move between energy levels
absorbing energy
emitting energy
The form of energy absorbed or emitted is in photons
what happens if ele. absorb energy
transition from low energy → high energy
e.g. n=2 → n=3
what state do electrons go in when they transition to a higher energy level
‘excited state’
what is the ‘excited state’
unstable relative to ground state (n=1)
once ele. go to excited state they are unstable and go back to n=2
what does it mean if more energy is emitted (in terms of energy levels)
bigger jump in ‘n levels’
n=2 → n=5 more energy than n=2 → n=3
what is the absorption spectra
opposite of an emission spectra
what evidence does the hydrogen emission spectrum provide
provides evidence for energy levels in atom
what do the lines of an hydrogen emission spectrum represent
each line represents a discrete energy level in the hydrogen atom
electrons can only occupy these energy levels
what does n=∞ refer to
refers to point when ele. has been completely removed from attraction of nucleus
and atom has been ionised
where are electrons located
discrete energy levels:
main energy levels
principle energy levels
what are atomic orbitals
a region of space we assign because we never really know where ele. are located
what are main energy levels divided into
sublevels
different types of sublevels
s, p, d and f (based on shape of atomic orbitals they contain)
factors of an s atomic orbital
spherical
maximum 2 electrons
only has a single s atomic orbital
factors of p atomic orbitals
dumbbell shape
maximum 6 electrons
3 p atomic orbitals
factors of f atomic orbital
7 atomic orbitals
factors of d atomic orbital
5 d atomic orbitals
how many electrons can a single orbital hold
maximum 2 electrons
formula to find the # of orbital at each major energy level
n2 = # of orbital at each major energy level
what is the aufbau principle
when adding electrons to atom, lower energy orbitals must be filled first
what is the Pauli exclusion principle
atomic orbitals can only hold 2 electrons
must have opposite spins
what is Hund’s rule
when we have degenerate orbitals, each orbital gets 1 electron before being doubly occupied
what are degenerate orbitals
orbitals of same energy → e.g. three 3p orbitals
what are the core elements and their symbol
[He] = 1s2
[Ne] = 1s22s22p6
[Ar] = 1s22s22p63s23p6
Rules of electron configuration (subatomic particle blah blah)
overlap of energy between the 3d and 4s sublevels
ele. are removed from 4s sublevel first when forming ions
Aufbau principle exceptions
copper (Cu)
[Ar]4s1 3d10
chromium (Cr)
[Ar]4s1 3d5