RMK- atomic structure Flashcards

1
Q

Pure substances

A

elements and compounds are pure substances as they are made up of one type of substance and have a fixed composition

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2
Q

Impure substances

A

Mixtures are made by combining two or more pure substances together. they do not have a fixed composition

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3
Q

Elements

A

a chemical element is a neutral substance that cannot be broken down into simpler substances using chemical methods. it consists of only atoms that contain the same number of protons, although the atoms can contain a different number of neutrons. there are 118 known chemical elements

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3
Q

Compounds

A

a compound is a pure substance formed when two or more chemical elements are chemically bonded together in a fixed ratio. a compound has different properties from its component elements.

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4
Q

Mixtures

A

contain pure substances that aren’t chemically bonded so can be separated by physical means. Mixtures aren’t arranged in a fixed ratio. mixtures are categorised into two sections.

Homogenous: all elements are in the same phase e.g. salt and water

Heterogenous: all elements are in different phases e.g. oil and water

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5
Q

States of matter

A

solids: occupy a fixed space and fixed volume. particles are held closely together in a lattice. In the solid state particles are held closely together in a fixed position in a lattice. the particles can vibrate about a fixed point but possess no individual translational velocity

liquid: fixed volume that takes up the shape of its container. particles are close together but moving in random motion.

Gas: completely fills its container. widely spaced particles moving with rapid, random motion.

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6
Q

what is heat?

A

heat is a measure of the total amount of energy in a given amount of substance and therefore depends upon the amount of substance present. it is measured in joules

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7
Q

What is temperature?

A

measure of the hotness of a substance and therefore is independent on the amount of substance present. it is a measure of the average kinetic energy of the substance. absolute temperature is measured in Kelvin. 0 kelvin is when all motion has stopped.

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8
Q

Kelvin and Degrees

A

0 kelvin= -273 degrees celsius

273 kelvin= 0 degrees celsius

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9
Q

Explain the changes of state from solid to liquid to gas

A

In the solid state particles are held closely together in fixed position in a lattice. The particles can vibrate about a fixed point but possess no individual translational velocity.
As heat is supplied the vibration intensifies and eventually the particles will have sufficient energy for the lattice to break and the particles are free to move. This is the liquid state. There are still attractive forces between the particles.
As more heat is added the particles move faster, i.e. gain in kinetic energy.
Eventually they will have sufficient energy to overcome the attractive forces and escape as a vapour. When the vapour pressure is equal to the external pressure the liquid boils. Hence the boiling point depends upon the external pressure. At 100 kPa pressure water boils at 373 K (100 °C).

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10
Q

Changes of State (names)

A

Solid —> Gas = sublimation

Gas—>Solid = deposition

Solid—>Liquid =melting

Liquid—>Solid = freezing

Liquid—>Gas = vaporisation (evaporation)

Gas—>Liquid = condensation

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11
Q

Describe cooling and heating curves in graphs

A

in a graph that shows a change of state during the change of state there will be flat sections in the graph, this is because, when changing from a liquid to a solid, the temperature is dropping, but bonds are being made which is exothermic; the heat energy given out balances the decreasing temp leading to the flat line. When changing from a solid to a liquid the opposite is true, bonds are being broken which is endothermic, this results in heat being taken in; and so the energy taken in balances the increasing temp leading to a flat line.

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12
Q

Separation techniques (filtration)

A

to separate solid particles from a liquid. it may be carried out under gravity at atmospheric pressure or for finer particles under reduced pressure.

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13
Q

Separation techniques (solvation and evaporation)

A

where one component of a solid mixture is soluble the mixture can be warmed with the solvent, and filtered to remove insoluble particles then the solvent is removed by evaporation

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14
Q

Separation techniques (recrystallisation)

A

an impure solid can be dissolved in a suitable solvent by heating then allowed to cool slowly so that the solid separates out as crystals which can be washed to remove any lingering solvent and dried

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15
Q

Separation techniques (distillation)

A

used to separate a volatile liquid from dissolved components or less volatile liquids

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16
Q

Separation techniques (chromatography)

A

used to separate different components in a mixture. in paper chromatography a spot of the mixture is placed on the paper and the solvent allowed to rise up the paper. different components partition between the solvent and the paper by different amounts so rise at different rates. A developer can be used for colourless components. the retardation factor Rf= distance travelled by component divided by the distance travelled by the solvent from the original spot.

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17
Q

Key factors of a nucleus

A
  1. it is very small in comparison to the atom
  2. it has a highly dense structure containing virtually all the mass of the atom
  3. it has a positive charge
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18
Q

the Nucleus- relative charges, relative masses and location

A

proton: 1, +1, nucleus
neutron: 1, 0, nucleus
electron: negligible, -1, outside nucleus

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19
Q

Isotopes

A

isotopes are different atoms of the same element with a different number of neutrons. as a result, they have different mass numbers, A, but the same atomic number, Z.

Chlorine for example has two isotopes: one with mass number 35, and one with mass number 37. they have similar chemical properties, as they are both chlorine atoms, but different physical properties such as density, because atoms of one isotope are heavier than atoms of the other.

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20
Q

How is mass spectrometry done?

A

the sample is injected into the instrument and vaporised. the atoms within the sample are then bombarded with high energy electrons. As a result, the atoms lose some of their electrons to form positively charged ions, known as cations.

the resulting ions are then accelerated by an electric field and deflected by a magnetic field. the degree of deflection depends on the mass to charge ratio. particles with no charge are not affected by the magnetic field and will therefore never reach the detector. the species with the lowest mass and highest charge will be deflected the most.

21
Q

Emission spectra and absorption spectrum.

A

a pure gaseous element subjected to a high voltage under the reduced pressure will glow- in other words, it will emit light. when this light passes through a prism, it produces a series of lines against a dark background. this is known as an emission spectrum. in contrast when a cold gas is placed between the prism and a source of visible light of all wavelengths, a series of dark lines within a continuous spectrum will appear. this is known as the absorption spectrum.

22
Q

how do you carry out a flame test?

A
  • clean the end of the potassium or nichrome wire by dipping it into a small sample of dilute hydrochloric acid and placing it in a non luminous bunsen burner flame. repeat until no flame colour is observed
  • dip the end of the flame test wire into one of the salt samples , and place it in the edgre of the non luminous bunsen burner flame, noting down the identity of the metal in the salt and the colour observed.
23
Q

Flame test colours (zinc, potassium, strontium, sodium and copper)

A

Zinc- Yellow

Potassium- Lilac

Strontium- Red

Sodium- Orange

Copper- Blue/green

24
Q

what is the EM spectrum in order of decreasing wavelength, increasing frequency and increasing energy

A

R–>M–>I–>V–>U–>X–>G

25
Q

what Is the speed of light

A

3.00x10^8

26
Q

how do you calculate ionisation energy?

A

E=hf

where E is the specific energy possessed by the photon, expressed in joules, J

h= plancks constant, 6.63x10^-34 Js

f= frequency of the radiation, expressed in hertz, Hz, or inverse seconds, s^-1

27
Q

What postulations did the Bohr model lead to in regard to electron position?

A
  1. the electron can only exist in certain stationary orbits around the nucleus. these orbits are associated with discrete energy levels.
  2. when an electron in the orbit with the lowest energy level absorbs a photon of the right amount of energy, it moves to a higher energy level and remains at that level for a short time (excited state)
  3. when the electron returns to a lower energy level it emits a photon of light. this photon represents the energy difference between the two levels.
28
Q

where is the most stable states of hydrogen?

A

state at n=1 (n is the principle quantum number), where the electron has the lowest possible energy. this energy level is known as the ground state of the atom. In contrast, the energy levels with n=2,3… are called excited states. atoms in excited states are unstable and spontaneously return to the ground state by emitting photons of specific wavelengths.

29
Q

what energy is released at n=1?

A

Electron transitions to the ground state, n=1, release higher energy, shorter wavelength ultraviolet light

30
Q

What energy is released at n=2

A

visible light

31
Q

what energy is released at n=3

A

while electrons returning to n=3 produce lines in the infrared region of the electromagnetic spectrum.

32
Q

Limitations of the Bohr model

A
  1. the model could not predict the emission spectra of elements containing more than one electron. it was only successful with the hydrogen atom.
  2. it assumed the electron was a subatomic particle in a fixed orbit around the nucleus
  3. it could not account for the effect of electric and magnetic fields on the spectral lines of atoms and ions
  4. it could not explain molecular bonding and geometry
33
Q

what is Heisenbergs uncertainty principle?

A

it is impossible to precisely know the location and momentum of an electron simultaneously. as opposed to bohrs model which stated that electrons exhibited fixed momentum in specific circular orbits

34
Q

what are schrodingers wave functions?

A

electrons in atoms in terms of their probability density, using heisenbergs idea that the momentum and position of electrons are uncertain. instead of saying that electrons will follow a defined travel path, this theory gives the probability that an electron will be found at a specific region of space where there is a high probability of finding an electron.

35
Q

what are atomic orbitals?

A

there are several types of atomic orbitals, and each orbital can hold a maximum of two electrons. each orbital has a characteristic shape and energy. the first four atomic orbitals, in order of increasing energy are labelled s,p (x,y,z) ,d and f. subsequent orbitals are theoretical, and these are labelled alphabetically (g,h,i,k and so on)

36
Q

What are the main energy levels in an atom (as opposed to sublevels).

A

the principle quantum number (n), introduced by the bohr model represents the main energy levels. these energy levels are split into sublevels comprised of atomic orbitals. for example, for n=1,2 and 3, the s atomic orbitals are 1s, 2s, 3s… As n increases, the s orbitals are further distanced from the nucleus

37
Q

Orbital diagrams

A

the electrons are shown in pairs or singular, and shown by arrows, one up and one down (in a paired electron) the arrows represent the direction of the spin

38
Q

What are Atomic Orbitals?

A

Atomic orbitals are regions of space where there is a high probability of finding electrons. electrons are charged negatively, and like charges repel each other, so two electrons should not be able to occupy the same region of space. a pair of electrons with opposite spins behave like magnets facing in opposite directions.

39
Q

what is the Pauli exclusion principle?

A

only two electrons can occupy the same atomic orbital and those electrons must have opposite spins.

40
Q

what is Hunds rule?

A

every degenerate orbital in a sublevel is singly occupied before any orbital is doubly occupied and that all electrons in singly occupied orbitals have the same spin. this means that the three p orbitals must have one electron with the same spin in each of them before any orbital can become doubly occupied with an electron of opposite spin.

41
Q

What are exceptions to the Aufbau principle?

A

The Aufbau principle correctly predicts the order of filling atomic orbitals for most elements. However, when atoms loose electrons to form ions the electrons in the sublevel with the highest principle quantum number (n) are lost first.
The ground state for copper and chromium are also different for those predicted by the Aufbau principle. The predicted electron configuration of copper is [Ar] 4s^2 3d^9, as the Aufbau principle suggests that the lower energy 4s orbital should be filled first. However the observed ground state electron configuration for copper is [Ar] 4s^1 3d^10. For chromium the predicted configuration is [Ar] 4s^2 3d^4 and the observed is [Ar] 4s^1 3d^5. In each case, promoting a 4s electron to a 3d level leads to a more stable electron configuration. In the case of copper, this gives a full 3d sublevel, and in the case of chromium, there are no paired electrons but rather six half occupied orbitals, each containing an electron with the same spin

41
Q

What is the Aufbau principle?

A

as electrons are added to atoms, the lowest available energy orbitals fill before higher energy orbitals do.
when electron shells fill, generally the following order is observed.
1s<2s<2p<3s<3p<4s<3d<4p<5s<4d<5p<6s<4f<5d<6p

42
Q

Condensed electron configurations.

A

as the atomic number of an element increases, the full electron configuration gets longer and it can be time consuming to write. the chemistry of atoms and ions is mostly determined by their valence electrons, that is, the outermost electrons, rather than the inner core electrons. a more convenient way to write the electron configurations is to highlight the valence electrons and represent the inner core electrons as the previous group 18 (noble gases) element in the period table.

43
Q

what is ionisation energy?

A

the minimum energy required to eject an electron out of a neutral atom or molecule in its ground state.

44
Q

how does ionisation energy vary going down the groups and across the periods?

A

First ionisation energy generally decreases going down the groups of the periodic table and increases across the periods.

Going down a group, the number of sublevels increases. the outermost electrons are shielded from the pull of the nucleus by the electrons in the lower energy sublevels. the more sublevels the greater the shielding and therefore less energy is required to remove electrons from the outermost sublevel.

Going across a period, the number of protons in the nucleus increases, so the outermost electrons are held closer to the nucleus by the increased nuclear charge. At the same time, the shielding effect remains nearly constant because the number of inner electrons does not change. therefore more energy is required to remove the outermost electron, so IE increases along the period

45
Q

what is the discontinuity of ionisation energy across the period of group 2 and group 3 elements? (dip in the graph)

A

The valence electron configuration of beryllium is 2s^2 while for boron it is 2s^2 2p^1. the paired 2s^2 electrons shield the single 2p electron in boron from the nucleus, making the electron slightly easier to remove.

The same trend can be observed in comparing group 2 to group 3 elements in any period. For example, the 3s62 electrons shield the lone 3p^1 electron in aluminium, so the first ionisation of aluminium is lower than that of magnesium.

Electrons are always removed from the highest occupied energy level, and from the highest energy sublevel within that level.

46
Q

what is the discontinuity of ionisation energy across the period between the group 15 and 16 elements? (dip in the graph)

A

From group 15 to 16 there is also a drop in ionisation energy. The electron configuration of nitrogen is 1s^2 2s^2 2p^3 while for oxygen it is 1s^2 2s^2 2p^4.

Nitrogen has a more stable electron configuration than oxygen as it has a half filled p sublevel and therefore more energy is required to remove an electron from nitrogen. This is because the paired electrons in oxygen occupy the same region of space and have increased repulsion. However, in nitrogen the three electrons in the 2p orbitals do not come into close proximity.

47
Q

How do you calculate ionisation energy from spectral data?

A

As the principle quantum number of energy levels increases, the distance between the levels converges to a continuum. This can be observed by the convergence of spectral lines in the hydrogen emission spectrum.

E= hc/λ

ionisation energy in kJ mol^-1= ((energy needed to remove one electron from an atom)*6.022x10^23)/λ

48
Q

Why is it harder to remove electrons in successive ionisation energies/

A

It requires more energy to remove the second and successive electrons from an atom because the number of protons exceeds the number of remaining electrons while the electron-electron repulsion decreases (removing from an increasingly positive ion) As a result electron clouds are pulled closer to the nucleus and held tighter by increased electrostatic attraction. Once all the valence electrons are removed so that only the stable noble gas configuration remains, the energy required to remove the next electron increases sharply.

49
Q

Why do certain gaseous vapours only emit certain frequencies of visible light?

A
  • Electrons can only occupy energy levels
  • Which are fixed characteristic energies/ distances from the nucleus
  • So when an excited electron falls to a lower energy level it emits a known, discrete energy corresponding to the energy groups
  • E= hv, so only frequency observed