1/17
Looks like no tags are added yet.
Name | Mastery | Learn | Test | Matching | Spaced |
---|
No study sessions yet.
nuclear charge
number of protons
Zeff
harder to lose electrons
S has a greater zeff →greater coulumbic attractive force between its nuc and valence e- shell
Across a periodic table
Zeff increases from left to right, n stays the same
Down periodic table
nuclear charge increases, n increases as you go down
Explaining trends
Same
difference
CAF
trend
Atomic radius Row comparion
decreases going from left to right
the e- cloud is pulled in closer resulting in a smaller atomic force
Atomic radius column comparison
increases going down periodic table
n = 2 vs n = 6
n=6 has a greater distance between its nuc and valence e- shell
the e cloud expands resulting in a larger atomic radius
CAF
high zeff = larger CAF bc increases going left to right \
high n = lower CAF bc greater distance between nuc and valence e- shell
Ionic radius
protons vs. neutrons → e-/e- repulsion, nuclear charge, energy levels
high nuc charge (protons) → small ionic radius
high e-/e- repulsion (e-)→ high ionic radius
electronegativity
row comparison: Atoms that have a larger zeff will have greater EN
Coulomb comparison: smaller n will have greater EN
Ionization Energy
p+ to e- ration
Row: Zeff increases left to right → high ionization energy
Coulomb: ionization decreases going down → bigger n = less ionization
harder to remove e- from a positively charged ion Ni+
nm
high nm →less energy
Transition metals configs
remove e- from the highest energy level 4s 5s S first
Diamagnetic
NO UNPAIRED electrons/spins PAIRED Di = 2
Paramagnetism
contains UNPAIRED spins
1 or more e- unpaired
aufbau principal
electrons fill lower energy levels first then fill higher ones
1s then 2s then 3s
Hunds rule
when e- occupy orbitals of equal energy, one e- enters each orbital until all orbitals contain e- before doubling up
Pauli exclusion principal
an individual orbital may only hold 2 e- max