2 atomic structure Flashcards

1
Q

structure of an atom

A

positively charged nucleus
‘cloud’ of negative charge

electrostatic attraction betw pos nucleus and neg charged electrons – holds it tgt

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2
Q

define isotope

A

different atoms of the same element
same protons
but diff number of neutrons

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3
Q

speed of light? (in section 2 of data booklet)

A

3.00 x 10^8 m/s

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4
Q

excited state electrons are further / closer to the nucleus

A

further (higher energy level)

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5
Q

in a line emission spectrum of hydrogen, describe the lines

A

they get closer toegther towards the blue end of the spectrum (convergence towards the higher energy end)

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6
Q

what does it mean when lines converge towards the higher energy end in an emission spectrum

A

the electron is reaching its maximum amt of energy = ionisation energy of the electron

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7
Q

who observed line emission spectra

A

Johannes Balmer

(the balmer series is in the visible spectrum)

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8
Q

lines in an emission spectrum correspond w the electron jumping from _____ levels to the ______ energy level

A

higher

second

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9
Q

when an electron jumps to n3, what is the region and energy level?

A

infrared

low

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10
Q

when an electron jumps to n2, what is the region

A

visible

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11
Q

when an electron jumps to n1, what is the region and energy

A

ultraviolet

high

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12
Q

how to calculate the number of electrons each principal quantum number can hold?

A

2n^2

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13
Q

how many electrons can the principal quantum number 3 and 4 hold?

A

well yknow n=1 can have 2 and n=2 can have 8 BUT as it turns out
3 = 18
4 = 32

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14
Q

what is the sequence of letters for the subshells! + how many electrons can each have

A

s p d
2 6 10

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15
Q

s and p orbital shapes

A

s is just a sphere around the centre

p is a dumbell shape? along the axes so like an hourglass

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16
Q

what is the ground state of an atom

A

most stable electronic configuration with lowest amount of energy

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17
Q

what is the Aufbau principle

A

ground state is acheived by filling subshells with lowest energy first
(does not follow pattern above n=2)

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18
Q

exception to subshell increase in energy as follows: s < p < d < f

A

3d subshell has slightly higher energy level than 4s = 4s filled first

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19
Q

what does it mean when orbitals are ‘degenerate’?

A

orbitals in the SAME subshell have the same ENERGY (1s=2s=3s=4s)

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20
Q

subshells can be further divided into orbitals, which each can hold ___ electrons

A

2

so if theyre like ooh 2p subshell how many orbitals?? well it can hold 6 electrons so 3 orbitals

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21
Q

the size of s orbitals increases with _______ shell number

A

increasing

so like n=3 is gonna be a bigger sphere than n=1

22
Q

p subshell has ____ orbitals and they are oriented?

A

3 orbitals

occupy x,y,z axes perpendicular to each other in a dumbell shape

23
Q

shape change of p orbitals with increasing principal quantum number?

A

longer and larger lobes

24
Q

what is spin-pair repulsion?

A

when 2 electrons spinning in the same direction (same spin) repel each other

25
Q

what is Hunds rule?

A

due to spin-pair repulsion, electrons occupy seperate orbitals before pairing up with another with opposite spin

(basically in the square thing, you fill in ^ ^ ^ before going ^v ^v ^v)

26
Q

what is the Pauli Exclusion principle?

A

an orbital can hold 2 electrons and they must have opposite spin

27
Q

how does shorthand electron configuration work

A

use the nearest preceding noble gas + rest of the config

[Ar]3d^54s^1

28
Q

transition metals fill the 4s/3d subshell first and lose electrons from the 4s/3d subshell first

A

4s !!!

29
Q

according to electronic configuration, how is the periodic table split up?

A

left grp: s block
mid (transmetals): d block
right (nm): p block
below: f block

30
Q

name the 2 exceptions to Aufbau principle

A

Cr (Chromium)
Cu (copper)

31
Q

Cr is NOT 3d4 4s2 it is?

A

3d5 4s1

32
Q

why are Cr and Cu exceptions to Aufbau principle

A

its more energetically favourable to have a full/half 3D SUBSHELL than a full 4s

33
Q

when energy is released when electron goes from n=2 to n=1, what series does it correpsond with?

A

ultraviolet

Lyman series

34
Q

what is Bohr’s model?

A

idea that electrons exist in discrete energy levels SO an EXACT amt of energy is needed to ‘jump’ an energy level

35
Q

3 limitations of Bohr’s model

A
  1. assumes positions of electrons are FIXED
  2. assumes energy levels are SPHERICAL in nature
  3. only applicable to HYDROGEN
36
Q

what is the limit of convergence?

A

the frequency at which the spectral lines appear to meet // converge

= first ionisation energy

37
Q

frequency of radiation in emission spectrum at the limit of convergence can be used to determine the ?

A

first ionisation energy

38
Q

what is the first ionisation energy from the Lyman series?

A

UV region! limit of convergence = energy given out when electron falls from n=infinite to n=1

39
Q

what data booklet constant will you need to calculate first ionisation energy using convergence limit?

A

plancks constant!

40
Q

in the conversion between wavelength and frequency whats the unit for wavelength

A

m!

so if its nm then you gotta x10^-9

41
Q

convert J to kJ

A

divide by 1000

42
Q

2 things to rmb when calucating first ionisation energy from convergence limit

A

convert to per mole using AVOGARDOS CONSTANT

convert final units to kJ/mol (if asked for)

  • all eqns in formula booklet
43
Q

4 factors affecting first ionisation energy

A
  1. size of nuclear charge
  2. distance of outer electrons from nucleus
  3. shielding effect (inner electrons)
  4. spin pair repulsion
44
Q

first ionisation energy ______ across a period and _______ decreases down a group

A

increases

decreases

(top right corner highest)

45
Q

explain the increase in ionisation energy across a period 4

A

nuclear charge incr

atomic radius decr = decr dist

shielding constant

harder to move electron = more energy needed

46
Q

dips in the trend of first ionisation energy increasing across the period name 2

A

between beryllium and boron

between nitrogen and oxygen (spin-pair repulsion)

47
Q

why is there a dip in the ioniastion energy trend between beryllium and boron

A

distance

5th beryllium electron is in 2s
BUT
5th in boron is in 2p (further) = lower

48
Q

why is there a dip in the ioniastion energy trend between nitrogen and oxygen

A

spin-pair repulsion in 2p orbital of oxygen

nitrogen has
p orbital ^ ^ ^

oxygen has
p orbital
^v ^ ^

= repulsion = easier to remove = decr first ionisation energy

49
Q

how does first ionisation energy change one period to the next + why? (dist, shielding, charge)

A

it has a LARGE DECREASE

  • incr dist
  • incr shielding bc new shell
  • outweighing the incr nuclear charge
50
Q

why do successive ionisation energies increase

A

remove first electron = ion

more difficult to remove electron

attractive forces incr with electron decr
- decr shielding
- incr charge

also depends on electronic configuration

51
Q

big jumps in successive ionisation energies = ?

A

change of shell
(so if 2nd is hard to remove, there is 1 valence electrion)

(smaller jumps = change of subshell)