Topic 2 + 12 Flashcards

1
Q

state one difference in physical properties of isotopes

A

(isotope with lower mass number) has lower boiling point/melting point/density than (isotope with higher mass number)

DIFFERENT MASS IS NOT ACCEPTED

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2
Q

explain why chemical properties of isotopes are the same

A

because they have the same (either one of these is accepted)
1. electron configuration
2. arrangement of electrons
3. same number of protons AND electrons

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3
Q

define the term “isotopes of an element”

A

atoms of same element with different numbers of neutrons
-> same chemical properties, different physical properties

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4
Q

define “empirical formula”

A

simplest (whole number) ratio of moles of each element present in a molecule

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5
Q

define “molecular formula”

A

actual numbers of moles of each element present in a molecule

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6
Q

define “first ionization energy”

A

energy needed to remove one mole of electron from the ground state of one mole of the gaseous atom

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7
Q

explain the large increase between nth and (n+1)th ionization energies

A

nth electron comes from pth energy level AND (n+1)th electron comes from (p-1)th energy level.
electron in (p-1)th energy level is closer to nucleus therefore is exposed to greater effective nuclear charge

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8
Q

explain the general increase in successive ionization energies of element

A

successive electrons are more difficult to remove because each is taken from more positively charged ion, therefore experiencing increased electrostatic attraction

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9
Q

valence electrons

A

electrons in the outermost shell/energy level of an atom

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10
Q

core electrons

A

electrons that are not valence electrons and do not participate in chemical bonding

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11
Q

percentage yield

A

actual yield / theoretical yield x 100

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12
Q

why experimental yield may be greater than theoretical yield

A

temperature greater than 273K / pressure less than 100kPa

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13
Q

line spectrum

A

shows discrete number of individual lines at specific points in the visible range

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14
Q

continuous spectrum

A

shows all colors/wavelengths/frequencies of visible light

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15
Q

atomic number

A

number of protons

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16
Q

mass number

A

number of protons + neutrons

17
Q

cations

A

lost electrons, positive charge

18
Q

anions

A

gained electrons, negative charge

19
Q

mass spectrometer

A

used to measure the mass of individual atoms,
basically incomprehensible therefore uses relative mass instead,
used to determine the relative atomic mass of an element from its isotopic composition

horizontal axis: mass/charge ratio of different ions on the carbon-12 scale
vertical axis: percentage abundance

20
Q

percent abundance

A

relative amounts of two isotopes

21
Q

electromagnetic (EM) radiation

A

comes in different forms of different energy, small portion can be seen as visible light

all EM radiation travels at same speed but have different wavelengths and frequency

22
Q

frequency

A

number of waves that pass a point in 1 second

23
Q

absorption spectrum

A

produced when EM radiation is passed through a collection of atoms and some of the radiation is absorbed and used to excite the electrons in the atoms from a low energy level to higher energy level.
transmitted radiation relative to incident radiation can be measured

24
Q

ground state

A

when electron is in the lowest unoccupied energy level

25
Q

excited state

A

when electron is in a higher energy level but is unstable

26
Q

photon

A

one packet of energy (quantum),
particle of light

27
Q

moving electrons

A
  • when an atom falls from excited state to ground state, light of specific frequency (v) is produced
  • when an atom moves from ground state to excited state, light of specific frequency is absorbed
28
Q

ionization energy

A

energy to remove an electron from the ground state of an atom in a mole of gaseous atoms

29
Q

emission spectra

A

produced when photons are emitted from atoms with excited electrons returning to a lower energy level

30
Q

line emission spectrum of hydrogen

A

provides evidence for existence of electrons in discrete energy levels which converge at higher energies

31
Q

orbital

A
  • each orbital has defined energy state for given electronic configuration and chemical environment
  • can hold two electrons of opposite spin
32
Q

Aufbau principle

A

states that electrons are placed into orbitals of lowest energy first

33
Q

Cu
(Copper)

A

exception to Aufbau principle:
[Ar] 4s^1 3d^10
because of full shell stability

34
Q

Cr
(Chromium)

A

exception to Aufbau principle:
[Ar] 4s^1 3d^5
because of half shell stability

35
Q

losing electrons

A
  • loses paired electrons in an orbital first
  • loses electrons in 4s first before 3d
36
Q

limit of convergence at higher frequency

A

corresponds to the first ionization energy in an emission spectrum

37
Q

hydrogen spectrum

A
  • absorption: lower level -> higher level
  • emission: higher level -> lower level
  • converges at higher energy level
  • UV radiation: absorption when n=1 -> higher level, emission when higher level -> n=1
  • visible light: absorption when n=2 -> higher level, emission when higher level -> n=2
  • IR: absorption when n=3 -> higher level, emission when higher level -> n=3
38
Q

exceptions to ionization energy trend

A
  1. First ionization energy of boron (B) is less than that of beryllium (Be) <group 2>
    -> for beryllium, first ionization potential electron comes from 2s orbital which is closer to nucleus and experiences higher electrostatic attraction than first electron of boron which comes from 2p orbital
  2. First ionization energy of oxygen is less than that of nitrogen <group 15>
    -> for both nitrogen and oxygen, the first electrons come from the 2p orbital, but all electrons of nitrogen in the 2p orbital are unpaired whereas for oxygen there is one set of paired electrons in one of the 2p orbitals. Due to the repulsion between electrons in that orbital, the first electron of oxygen would be easier to remove than that of nitrogen.