Atomic Structure Flashcards

1
Q

What is a positive ion called?

A

Cation (this is right). The atom has lost electrons, whereas the anode in electrolysis would be gaining them which is why the positive electrode is called an an anode.

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2
Q

What is a negative ion called?

A

Anion

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3
Q

What are isotopes?

A

Isotopes are different atoms of the same element with different mass numbers i.e. different numbers of neutrons in the nucleus.

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4
Q

What is the same about 2 isotopes and what is different?

A

Isotopes have the same chemical properties (they react in the same way) but different physical properties (different melting points and boiling points).
This is because they have the same number of electrons but different numbers of neutrons and so move at different speeds because some are heavier than others.

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5
Q

What is the relative atomic mass of an element?

A

The relative atomic mass of an element is the average of the masses of the isotopes in a naturally occurring sample of the element relative to the mass of a 1/12 of an atom of carbon-12.

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6
Q

How do you calculate relative atomic mass from two isotopes?

A

You take their percentage and times it by their atomic mass and then add it to the other isotope times that isotopes atomic mass and put it over 100.

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7
Q

What does a mass spectrometer show?

A

It shows us how many of each isotope in a sample. The number of peaks shows how many isotopes we have, and the height (or more properly the area under each peak) is proportional to its abundance in the sample.

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8
Q

What is the K shell?

A

The lowest energy level or shell, the one closest to the nucleus.

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9
Q

What is a shorthand for how many electrons in an element?

A

2n^2 with n being the principle quantum number meaning the number of the outer shell.

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10
Q

How do electrons fill shells?

A

The general rule for filling these energy levels is that the electrons fill them from the lowest energy to the highest (from the nucleus out). The first two energy levels must be completely filled before an electron goes into the next energy level. The third main energy level is, however only filled to 8 before electrons are put into the fourth main energy level. This scheme works for elements with atomic number up to 20.

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11
Q

What is frequency?

A

v (frequency) = speed of light/wavelength

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12
Q

What are photons?

A

Photons are how we describe light or electromagnetic energy when it acts or displays the properties of a particle.

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13
Q

What is the evidence for energy levels in atoms?

A
  • Hydrogen atom spectrum

- Ionisation energies

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14
Q

What is the hydrogen atom spectrum and what does it show?

A

When hydrogen gas at low pressure is subjected to a very high voltage, the gas glows pink. The glowing gas can be looked at through a spectroscope, which contains a diffraction grating and separates the various wavelengths of light emitted from the gas. Because light is emitted by the gas, this is called an emission spectrum. In the visible region, the spectrum consists of a series of sharp, bright, lines on a dark background. This is a line spectrum as opposed to a continuous spectrum which consists of all the colours merging into each other.

The lines get closer together at higher/frequency. Passing an electric discharge through a gas causes an electron to be promoted to a higher energy level (shell). The electron in the higher state is excited and unstable at this higher level and therefore will fall to a lower level, as it does this it releases energy as a photon of light. So each line in the spectrum comes from the transition of an electron from a high energy level to a lower one. The fact that a line spectrum is produced provides evidence from electrons being in energy levels (shells): i.e. electrons in an atom are allowed to have only certain amounts of energy. Each line in the spectrum comes from the transition of an electron from a high energy level to a lower one.

It depends where the excited electrons are falling back down to, if they are falling all the way back to one they release lots of energy and that has a high frequency and is therefore ultraviolet. If they are falling to 2 then it produces visible and if they are falling back to 3 it produces infra red.

The lines in the emission spectrum get closer together at higher frequency/energy. Eventually they come together and converge. This is the convergence limit, the lines merge to form a continuum. Beyond this point the electron can have any energy and so must be free from the the influence of the nucleus. It is not normally observed in the spectrum but can be worked out.

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15
Q

What is the difference between a line spectrum and a continuous spectrum?

A

In the visible region, the spectrum consists of a series of sharp, bright, lines on a dark background. This is a line spectrum as opposed to a continuous spectrum which consists of all the colours merging into each other.

Line spectrum - only certain frequencies/wavelengths of light present.
Continuous spectrum - all frequencies/wavelengths of light present.

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16
Q

How is an emission spectrum formed?

A

Passing an electric discharge through a gas causes an electron to be promoted to a higher energy level (shell). The electron in the higher state is excited and unstable at this higher level and therefore will fall to a lower level, as it does this it releases energy as a photon of light. So each line in the spectrum comes from the transition of an electron from a high energy level to a lower one. The fact that a line spectrum is produced provides evidence from electrons being in energy levels (shells): i.e. electrons in an atom are allowed to have only certain amounts of energy. Each line in the spectrum comes from the transition of an electron from a high energy level to a lower one.

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17
Q

How are different lines produced in the hydrogen emission spectrum?

A

A hydrogen spectrum looks like a series of coloured lines across a black background, however there are parts of the emission spectrum that we cannot see, there are infrared and ultraviolet sections. These sections have their own convergence, and then start agains spaced out at the next part of the electromagnetic spectrum. So in the ultraviolet region the lines get closer and closer together and then they return to being spaced out much further to the right in the visible part.
The different series of lines occur when electrons fall back down to different energy levels. Falling down to shell 3 produces infra red, falling down to 2 produces visible and falling down to 1 produces ultraviolet.

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18
Q

Why are different electromagnetic waves produced by the hydrogen emission spectrum?

A

It depends where the excited electrons are falling back down to, if they are falling all the way back to one they release lots of energy and that has a high frequency and is therefore ultraviolet. If they are falling to 2 then it produces visible and if they are falling back to 3 it produces infra red.

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19
Q

Why do we use the hydrogen emission spectrum?

A

It provides evidence for electrons being in energy levels but we particularly use hydrogen because it is simple as it only has one electron.

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20
Q

What is the convergence limit and what does it show?

A

The lines in the emission spectrum get closer together at higher frequency/energy. Eventually they come together and converge. This is the convergence limit, the lines merge to form a continuum. Beyond this point the electron can have any energy and so must be free from the the influence of the nucleus. It is not normally observed in the spectrum but can be worked out.

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21
Q

What is the order of energy of the orbitals?

A

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22
Q

What is the Aufbau principle?

A

The Aufbau principle is the name given to the process of working out the electron configuration of an atom. Electrons fill sub-levels from the lowest energy upwards - this gives the lowest possible (potential) energy.

23
Q

What is the order of energy of ALL the orbitals?

A

1s 2s 2p 3s 3p 4s 3d 4p. 4s is at a lower energy than 3d, and therefore fills first, but it also empties first.

24
Q

What is an orbital?

A

An orbital is a region of space in which there is a high probability of finding an electron. It represents a discrete energy level.

25
Q

How many electrons can an orbital contain?

A

A single orbital can contain a maximum of 2 electrons.

26
Q

What is the s orbital?

A

The s orbital is centred on the nucleus. The electron is moving all the time and the intensity of colour here represents the probability of finding the electron at a certain distance from the nucleus. The darker colour the greater the probability of the electron being found at that point. This represents the electron density.

27
Q

What is the first energy level made up of?

A

The first energy level is just an s orbital, and so can only hold 2 electrons.

28
Q

What is the second energy level made up of?

A

The second energy level is made up of the 2s sub level and then the p sub level is made up of 3 p orbitals, and therefore the second energy level can hold 8 electrons.

29
Q

How does the 2s orbital differ from the 1s orbital?

A

The 2s orbital is at a higher energy and is also larger.

30
Q

What is the p orbital?

A

The p orbitals have a ‘dumb-bell’ shape and there are 3 of them making up the sub-level. They lie at 90 degrees to one another and are named px py and pz. The px orbital is along the x axis and so on. They all have the same energy and are therefore described as degenerate.

31
Q

What does degenerate mean?

A

Degenerate orbitals are orbitals with the same energy. Within any sub-shell all the orbitals are degenerate, for example in the third energy level the 3p sub-shell contains 3 p orbitals all at the same energy.

32
Q

What is the third energy level made up of?

A

The third energy level is made up of an s orbitals, 3 p orbitals and 5 d orbitals. As each orbital contains 2 electrons it can hold up to 18.

33
Q

What is the fourth energy level made up of?

A

One 4s, three 4p, 5 4d and seven 4f orbitals.

34
Q

How many orbitals are there with d?

A

5 d orbitals are together

35
Q

How many orbitals are there with f?

A

7 f orbitals are together

36
Q

What is the second part of the Aufbau principle?

A

As well as moving around in space within an orbital, electrons also have another property called spin. There are two rules that must be considered before electrons are put into orbitals.

1) The Pauli exclusion principle: the maximum number of electrons in an orbital is two. If there are two electrons in an orbital, they must have opposite spin.
2) Hund’s rule: Electrons fill orbitals of the same energy (degenerate orbitals) so as to give the maximum number of electrons with the same spin. This is because they repulse each other. So for example when filling the 3p sub-shell, each p orbital will fill with one clockwise electron so there will be 3 electrons one in each before any of the opposite spin are added.

37
Q

What is ionisation energy?

A

The ionisation energy is the minimum amount of energy required to remove an electron from a gaseous atom.
M(g) = M+(g) - e-

38
Q

How do we know the ionisation energy of hydrogen?

A

Look at where, on the hydrogen emission spectrum, the lines converge this is when the electron has so much energy, any energy, it is free from the influence of the nucleus.
The ionisation energy for hydrogen represents the minimum energy for the removal of an electron (from level 1 to infinity) and the frequency of the convergence limit in the Lyman series represents the amount of energy given out when an electron falls from outside the atom to level 1. These are the same amount of energy.

39
Q

How do you calculate how much energy a photon of a particular type of radiation has?

A
Light and other forms of electromagnetic radiation, exhibit the properties of both waves and particles - this is known as wave - particle duality. The energy (E) of a photon is related to the frequency of the electromagnetic radiation:
E=hv
where:
v is the frequency of the light
h is Plank's constant (6.63x10^-34)

This equation can be used to work out the differences in energy between various levels in the hydrogen atom.

40
Q

How are wavelength and frequency related?

A

The wavelength is the speed of light over frequency.

41
Q

What is the speed of light?

A

c=3x10^8 metres per second

42
Q

Calculate the ionisation energy given the frequency of the convergence limit?

A

You would calculate the energy of the photon released by multiplying the frequency by Planks constant.
E=hv
Then this is just for one electron, and ionisation energy is for a mole of gaseous ions. Therefore you need to times the energy by Avogadro’s constant, because that is the number of atoms in a mole.

43
Q

What is the first ionisation energy?

A

The energy required for the process:
M(g) = M+(g) + e-
The energy required to remove one electron from each atom in one mole of gaseous atoms under standard conditions.

44
Q

What is the second ionisation energy?

A

The energy required for the process:

M+ = M2+ + e-

45
Q

Which is higher the first ionisation energy or the second? And why?

A

The second ionisation energy is always higher than the first. This is explained in two ways:

1) Once an electron has been removed from an atom, a positive ion is created. A positive ion attracts a negatively charged electron more strongly than a neutral atom does. More energy is therefore required to overcome this attraction and remove an electron from a positive ion.
2) Once an electron has been removed from an atom there is less repulsion between the remaining electrons. They are therefore pulled in closer to the nucleus. If they are closer to the nucleus they are more strongly attracted and more difficult to remove.

46
Q

Why do you log the energies on a ionisation energy of one element graph?

A

Plotting log10 of these numbers reduces the range. The first ionisation energy of potassium is 418 kj per mole whereas the 19th is 475000kj. It would be very difficult to plot these values on a single graph.

47
Q

Why is there such a jump in the ionisation energies between shells?

A

Complete shells of electrons between the nucleus and a particular electron reduce the attractive force of the nucleus for that electron. In potassium for example there are three full shells of electrons between the outermost electron and the nucleus, and if this shielding were perfect the effective nuclear charge felt by the outer electron would be +1 (19+ in nucleus, -18 shielding electrons). This shielding is not perfect, however, and the effective nuclear charge felt by the outermost electron is higher than +1.

48
Q

How does ionisation energy vary across a period?

A

The general trend is that ionisation energy increases from left to right across a period. This is because as protons are added to the nucleus the electrons are more strongly attracted and therefore harder to remove.
There are however 2 exceptions to the general increase in ionisation energy across a period.

1) Beryllium (2) has a higher ionisation energy than Boron (3). You would expect Boron to be higher as it has the same shielding and a higher nuclear charge, however it is not. The electron configurations of the elements are:
Be - 1s2 2s2
B - 1s2 2s2 2p1
The major difference is that the electron to be removed from the boron atom is in a 2p sub-shell, whereas it is in a 2s sub-level in beryllium. The 2p sub-level in B is higher in energy than the 2s sub-level and therefore less energy is required to remove it.

2) The second is that the ionisation energy of oxygen (6) is lower than that of nitrogen (5).
The electron configurations for nitrogen and oxygen are:
N - 1s2 2s2 2p3
O - 1s2 2s2 2p4

The major difference is that oxygen has 2 electrons in one of the p orbitals, but nitrogen does not. An electron in the same p orbital as another electron is easier to remove than one in an orbital by itself because of the repulsion from the other electron.
When two electrons are in the same p orbital they are closer together than if there is one in each p orbital. If the electrons are closer together they repel each other more strongly. If there is greater repulsion, an electron is easier to remove.

49
Q

What is the trend down a group in ionisation energy?

A

Ionisation energy decreases as the shells increase and the distance between the nucleus and the electron being removed increases.

50
Q

Which are filled first 3d and 4s, and which are removed first?

A

Although the sub-levels are filled in the order 4s and then 3d, because 4s are at a lower energy level, the 4s electrons are always removed before the 3d electrons.