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7. Atomic structure and periodicity

Electromagnetic radiation

electromagnetic radiation: waves of energy that have magnetic
electricity + magnets + releasing
e.g. microwave, satellite, visible light (rainbow), ultraviolet, infrared, radio, television, gamma rays, X rays
wavelength (λ): distance from one peak to another peak (meters/m)
frequency (ν): the number of waves that pass a location in one second (hertz/Hz/s⁻¹)
image.png
visible light: 400 nm - 700 nm
c: speed of light (2.9979 × 10⁸ m/s)

Nature of matter

Max Planck:
E: energy (J)
h: Planck’s constant
ν: frequency (s⁻¹)
energy is quantized (little packets)
Albert Einstein: photoelectric effect (energy shot at metal → electrons fly out)
only certain wavelengths make electrons come off
visible/ultraviolet light: electrons change energy levels (think Bohr model)
microwaves: molecule rotates (think microwave plate)
infrared: molecules vibrate
E: energy
m: mass
c: speed of light
dual nature of matter: matter can be both a particle and a wave
de Broglie: all matter are waves

Atomic spectrum

if you put atoms in a prism, only certain colors appear
light spectrum

Bohr’s model of the atom

image.png
if you add energy to an orbital:
the electron will jump up an orbital/energy level
electron returns to original orbital
energy released (often visible light)
works for hydrogen (1 electron), but not with other elements
energy levels (n): orbitals according to Bohr model
n = 1: ground state

Quantum mechanical model

Ervin Schrödinger: equation for electron probability
image.png
Werner Heisenberg: we can know where an electron is or the momentum of the electron, never both

Quantum numbers and orbitals

quantum numbers: “address” of electron (big → small)
principal quantum number (n): 1 → ∞
energy level
angular momentum number (ℓ): 0 → n-1
0 = s
1 = p
2 = d
3 = f
4 = g
magnetic quantum number (m_ℓ): -ℓ → ℓ
1 orbital can hold two electrons
s: 2 electrons
p: 6 electrons
d: 10 electrons
f: 14 electrons
electronic spin (mₛ): 1/2 or -1/2
electron symbol: ⥮
Wolfgang Pauli: Pauli exclusion principle
every electron in an atom can only have one address
cannot have two electrons with the same address

Polyelectronic atoms

aufbau principle (“build up”): electron will always go to the lowest energy level first
examples
H
1 electron → 1 energy level
1 shape → s (orbital)
1 electron
1s¹ (electron configuration)
He
2 electrons → 1 energy level
1 shape → s
2 electrons
1s²
Li
3 electrons
1s²2s¹
Be
4 electrons
1s²2s²
B
5 electrons
1s²2s²2p¹
image.png
periodic table
image.png
look at row number
check orbital group

Periodic trends

atomic radius: distance from the nucleus to the valence electrons in an atom
down: increases (more shells)
right: decreases (more protons → more attraction)
ionization energy: amount of energy needed to remove one electron
down: decreases (electrons further from nucleus)
right: increases (want to lose on left but not on right)
electron affinity: amount of energy that is released when an electron is added
down: depends on column but generally decreases (electrons further away)
right: increases release of energy (more stable)
ionic radius: distance from the nucleus to the valence electrons in an ion
down: increases (more shells)
right
left: decreases (losing electrons)
goes up (more electrons)
right: decreases (adding electrons)
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