Topic 2.2: Electron configuration Flashcards

1
Q

Electromagnetic spectrum

A

Spectrum of wavelengths that comprise the various types of electromagnetic radiation

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2
Q

Relation of energy, wavelength, and frequency

A

a) Energy is inversely proportional to wavelength

b) Energy is proportional to frequency

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3
Q

Electromagnetic radiation

A

A form of energy that propagates through space at the speed of light as photons

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4
Q

Continuous spectrum

A

Radiation that spreads all frequencies / wavelengths of light present

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5
Q

Line spectrum

A

Radiation that emits only certain frequencies/wavelengths of light present

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6
Q

Line spectrum and element

A

Each element has its own characteristic line spectrum which can be used to identify the element

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7
Q

Quantization

A

Electromagnetic radiation comes in discrete parcels.

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8
Q

Energy equation

A

E = hv = hc / A

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9
Q

Electron transition in energy levels

A

a) Electron can move to a higher energy level by absorption of a photon
b) Electron can move from an excited state to a lower energy level by emitting a photon

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10
Q

Hydrogen line spectrum

A

Discrete lines which converge at higher energies and form a continuum

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11
Q

Ionization in line spectrum

A

Beyond the convergence limit the electron can have any energy and is not longer in the atom.

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12
Q

Series of lines in the hydrogen line emission spectrum

A

a) Balmer series
b) Lyman series
c) Paschen series

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13
Q

Balmer series

A

a) Visible region

b) Electronic transitions from upper energy levels back down to the n = 2 energy level.

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14
Q

Lyman series

A

a) UV region

b) Electronic transitions from upper energy levels back down to the n = 1 energy level.

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15
Q

Paschen series

A

a) IR region

b) Electronic transitions from upper energy levels back down to the n = 3 energy level.

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16
Q

Emission spectrum

A

Spectrum of frequencies of ER emitted due to an atom making a transition from a high energy to a lower energy state.

17
Q

How is an emission spectrum formed?

A

a) Passing an electric discharge through a gas causes an electron to be promoted to a higher energy level (shell).
b) The electron is unstable in this higher level and will fall to a lower energy level, giving out extra energy in the form of a photon light

18
Q

Electron shell (n = 1,2,3)

A

a) Main energy level

b) Can hold a maximum number of 2n^2 e-

19
Q

Subshells (s < p < d < f)

A

Each subshell has a particular number of orbitals

20
Q

Atomic orbital

A

a) Region in space where there is a high probability of finding an electrom
b) Can hold a maximum of two electrons of opposite sign

21
Q

Electron arrangement

A

Shows the number of electrons in each shell or orbit

22
Q

Aurfbau principle

A

Electrons fill sub-levels from the lowest energy level upwards

23
Q

Reasons for removing electron from 4s before 3d levels of 3d-block elements

A

3d orbitals are more compact than the 4s orbitals and hence electrons entering the 3d orbitals will experience a much greater mutual repulsion.

24
Q

Pauli exclusion principle

A

Any orbital can hold a maximum of two electrons, having opposite spin

25
Q

Hund’s rule of maximum multiplicity

A

When filling degenerate orbitals, electrons fill all the orbitals singly before occupying them in pairs to minimize repulsion

26
Q

Reason for exceptions in Cr and Cu

A

Having the maximum number of electron spins the same within a set of degenerate orbitals gives a lower energy (more stable) situation