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Electronic structure

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Two of them will be found in the 1s orbital close to the nucleus. ... Notice that the 2s orbital has a slightly lower energy than the 2p orbitals. ... – PowerPoint PPT presentation

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Title: Electronic structure


1
Electronic structure
2
Atomic structure
3
Atoms neutral
  • Protons have a positive charge and electrons have
    a negative charge.
  • Atoms are neutral so they have the same number
    of electrons as protons. 
  • The protons are in the nucleus and do not change
    or vary except in some nuclear reactions.
  • The electrons are in discrete pathways or shells
    around the nucleus.

4
Shells - Orbitals
5
ELECTRONIC STRUCTURE AND ATOMIC ORBITALS
  • In any introductory chemistry course you will
    have come across the electronic structures of
    hydrogen and carbon drawn as

6
Hydrogen's electron - the 1s orbital
7
Names of orbitals
  • Each orbital has a name.
  • The orbital occupied by the hydrogen electron is
    called a 1s orbital. The "1" represents the fact
    that the orbital is in the energy level closest
    to the nucleus.
  • The "s" tells you about the shape of the
    orbital. s orbitals are spherically symmetric
    around the nucleus - in each case, like a hollow
    ball with the nucleus at its centre.

8
2s orbitals
9
A p orbital is rather like 2 identical balloons
tied together at the nucleus. The diagram on the
right is a cross-section through that
3-dimensional region of space. Once again, the
orbital shows where there is a 95 chance of
finding a particular electron.
P orbitals
10
P orbitals
  • At any one energy level it is possible to have
    three absolutely equivalent p orbitals pointing
    mutually at right angles to each other. These are
    arbitrarily given the symbols px, py and pz. This
    is simply for convenience - what you might think
    of as the x, y or z direction changes constantly
    as the atom tumbles in space.

11
The electronic structure of hydrogen
  • Hydrogen has only one electron and that will go
    into the orbital with the lowest energy - the 1s
    orbital.
  • Hydrogen has an electronic structure of 1s1. We
    have already described this orbital earlier.
  • The electron of a hydrogen atom travels around
    the proton nucleus in a shell of a spherical
    shape

12
Helium
  • Helium, element number two, has two electrons in
    the same spherical shape around the nucleus.
  • The first shell only has one subshell, and that
    subshell has only one orbital, for electrons.
  • Each orbital has a place for two electrons. The
    spherical shape of the lone orbital in the first
    energy level has given it the name s orbital.

13
The electronic structure of carbon
  • Carbon has six electrons. Two of them will be
    found in the 1s orbital close to the nucleus. The
    next two will go into the 2s orbital.
  • The remaining ones will be in two separate 2p
    orbitals. This is because the p orbitals all have
    the same energy and the electrons prefer to be on
    their own if that's the case.
  • The electronic structure of carbon is normally
    written 1s22s22p2

14
Carbon
15
Carbon
  •  Name Carbon
  • Atomic Number 6
  • Chemical Symbol C
  • Electronic Configuration1s22s22p2
  • Atomic Mass 12.0
  • Atomic Ionization Energies
  • 2p 1086 kJ mol-1
  • 2s 1601 kJ mol-1
  • 1s 27788 kJ mol-1  

16
Orbitals, Shells
  • Physicists and chemists use a standard notation
    to describe the electron configurations of atoms
    and molecules. For atoms, we use atomic orbital
    labels (eg, 1s, 3d, 4f) with the number of
    electrons assigned to each orbital placed as a
    superscript. For example
  • hydrogen has one electron in the s-orbital of the
    first shell, so its configuration is written 1s1.
  • Lithium has two electrons in the 1s-subshell and
    one in the (higher-energy) 2s-subshell, so its
    configuration is written 1s2 2s1 (pronounced
    "one-ess-two, two-ess-one").
  • Phosphorus (atomic number 15), is as follows
    1s2 2s2 2p6 3s2 3p3.

17
Electronic configuration
18
Electronic configuration
19
Electronic configuration
20
Shells
  • The shells or energy levels are numbered or
    lettered, beginning with K.
  • So K is one, L is two, M is three, N is four, O
    is five, P is six, and Q is seven.
  • As the s shells can only have two electrons and
    the p shells can only have six electrons, the d
    shells can have only ten electrons and the f
    shells can have only fourteen electrons.

21
Shells - Orbitals
22
Shells
  • The electron shells are labelled K, L, M, N, O,
    P, and Q or 1, 2, 3, 4, 5, 6, and 7 going from
    innermost shell outwards.
  • Electrons in outer shells have higher average
    energy and travel further from the nucleus than
    those in inner shells, making them more important
    in determining how the atom reacts chemically and
    behaves as a conductor, etc, because the pull of
    the atom's nucleus upon them is weaker and more
    easily broken.

23
Subshells
  • Each shell is composed of one or more subshells,
    which are themselves composed of atomic orbitals.
    For example, the first (K) shell has one
    subshell, called "1s" the second (L) shell has
    two subshells, called "2s" and "2p" the third
    shell has "3s", "3p", and "3d" and so on.3 The
    various possible subshells are shown in the
    following table

24
Orbitals, Shells,subshells
25
Orbitals, Shells, subshells
26
Shells and subshells
27
Shells and subshells
28
Number of electrons in each shell
  • Each s subshell holds no more than two electrons
  • Each p subshell holds no more than six electrons
  • Each d subshell holds no more than ten electrons
  • Each f subshell holds no more than fourteen
    electrons
  • Therefore, the K shell, which contains only an s
    subshell, can hold up to 2 electrons the L
    shell, which contains an s and a p, can hold up
    to 268 electrons and so forth. The general
    formula is that the nth shell can in principle
    hold up to 2n2 electrons.

29
Tin Sn
30
spdf notation
  • Electronic Configuration 1s22s22p63s23p64s23d104s
    1

31
Spdf notation
32
Electrons in boxes
33
The order of filling orbitals
34
Orbitals shellsEnergy levels
  • The circles show energy levels - representing
    increasing distances from the nucleus. You could
    straighten the circles out and draw the
    electronic structure as a simple energy diagram

35
Energy levels
36
Energy levels
37
Ground state
  • The electrons are housed in shells around the
    nucleus. There is a ranking or hierarchy of the
    shells, usually with the shells further from the
    nucleus having a higher energy.
  • As we consider the electron configuration of
    atoms, we will be describing the ground state
    position of the electrons.
  • Place electrons in lower energy shells.
  • Start from shell nearest to the nucleus, i.e 1s2

38
Order of filling atomic orbitals
39
Order of filling orbitals
40
Ground state
  • Electrons fill low energy orbitals (closer to the
    nucleus) before they fill higher energy ones.
    Where there is a choice between orbitals of equal
    energy, they fill the orbitals singly as far as
    possible.
  • The diagram (not to scale) summarises the
    energies of the various orbitals in the first and
    second levels.
  •  
  • Notice that the 2s orbital has a slightly lower
    energy than the 2p orbitals. That means that the
    2s orbital will fill with electrons before the 2p
    orbitals. All the 2p orbitals have exactly the
    same energy

41
Quantum
  • Electrons are able to move from one energy level
    to another by emission or absorption of a quantum
    of energy, in the form of a photon. Because of
    the Pauli exclusion principle, no more than two
    electrons may exist in a given atomic orbital
    therefore an electron may only leap to another
    orbital if there is a vacancy there. The word
    comes from the Latin "quantus," for "how much.

42
Principal quantum number
  • An electron shell is the set of atomic orbitals
    which share the same principal quantum number, n
    (the number before the letter in the orbital
    label) hence the 3s-orbital, the 3p-orbitals and
    the 3d-orbitals all form part of the third shell.
  • An electron shell can accommodate 2n2 electrons,
    ie the first shell can accommodate 2 electrons,
    the second shell 8 electrons, the third shell
    18 electrons, etc.

43
The periodic table
  • The form of the periodic table is closely related
    to the electron configuration of the atoms of the
    elements. For example, all the elements of group
    2 have an electron configuration of E ns2
    (where E is an inert gas configuration), and
    have notable similarities in their chemical
    properties.
  • The outermost electron shell is often referred to
    as the "valence shell" and determines the
    chemical properties. It should be remembered that
    the similarities in the chemical properties were
    remarked more than a century before the idea of
    electron configuration.

44
History
  • The existence of electron shells was first
    observed experimentally in X-ray absorption
    studies. Shells were first labeled with the
    letters K, L, M, N, O, P, and Q.
  • The origin of this terminology was alphabetic.
  • Later experiments indicated that the K absorption
    lines are produced by the innermost electrons.
  • These letters were later found to correspond to
    the n-values 1, 2, 3, etc.
  • K1 ,L 2 , M 3, N 4, etc.

45
Quantum theory
  • The "quantum" theory was proposed more than 90
    years ago, and has been confirmed by thousands of
    experiments. Science and education has failed to
    clearly describe the energy level concept to
    almost four generations of citizens. This
    experiment is an exercise aimed at throwing a
    little more light on the subject.
  • Atoms have two kinds of states a ground state
    and an excited state. The ground state is the
    state in which the electrons in the atom are in
    their lowest energy levels possible (atoms
    naturally are in the ground state). This means
    the electrons have the lowest possible values for
    "n" the principal quantum number.

46
Spectrum, spectra
47
Wavelength and frequency
48
The visible spectrum with respect to infrared and
ultraviolet radiation. 
49
UV and visible light
  • Ultraviolet (200-400 nm) and visible (400-800 nm)
    radiation are found towards the short wavelength,
    high frequency end of the electromagnetic
    spectrum. Figure 1 shows the portion of the
    electromagnetic spectrum where UV-Vis radiation
    exists.

50
White light
  • You need to know that white light is the
    combination of all colors of the spectrum. 

51
Separation of white light spectrum
52
Continuous,emission ,absorption
53
Different kinds of spectra
  • Thus, emission spectra are produced by thin
    gases in which the atoms do not experience many
    collisions (because of the low density). The
    emission lines correspond to photons of discrete
    energies that are emitted when excited atomic
    states in the gas make transitions back to
    lower-lying levels.
  • A continuum spectrum results when the gas
    pressures are higher. Generally, solids, liquids,
    or dense gases emit light at all wavelengths when
    heated.
  • An absorption spectrum occurs when light passes
    through a cold, dilute gas and atoms in the gas
    absorb at characteristic frequencies since the
    re-emitted light is unlikely to be emitted in the
    same direction as the absorbed photon, this gives
    rise to dark lines (absence of light) in the
    spectrum.
  •  

54
Emission spectrum
  • An element's 'emission spectrum' is the relative
    intensity of electromagnetic radiation of each
    frequency it emits when it is heated (or more
    generally when it is excited).
  • When the electrons in the element are excited,
    they jump to higher energy orbits. As the
    electrons fall back down, and leave the excited
    state, energy is re-emitted, the wavelength of
    which refers to the discrete lines of the
    emission spectrum. Note, however, that the
    emission extends over an area of frequencies, an
    effect called spectral line broadening. This
    spectrum is caused by hydrogen.

55
Emission spectrum...
  • The emission spectrum can be used to determine
    the composition of a material, since it is
    different for each element of the periodic table.
    One example is identifying the composition of
    stars by analysing the received light

56
Electronic configuration of Na
57
Emission spectrum for Na
58
Absorption spectra
59
Flame test
  • A flame test is a procedure used in chemistry to
    detect the presence of certain metal ions, based
    on each element's characteristic emission
    spectrum. The color of flames in general also
    depends on temperature see flame color.
  • The test involves introducing a sample of the
    element or compound to a hot, non-luminous flame,
    and observing the color that results. Samples are
    usually held on a platinum wire cleaned
    repeatedly with hydrochloric acid to remove
    traces of previous analytes

60
Flame test
61
Flame test
62
Shells - Orbitals
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