3.4 - Thermochemical Principles And Properties Of Particles And Substances Flashcards

1
Q

Isotopes

A

Various numbers of neutrons in an atom

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2
Q

Atomic number determined by..?

A

Number of protons.

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3
Q

Ionisation energy definition

A

Energy needed in kJ mol-1 to remove one electron from each atom in 1 mole at its gaseous state

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4
Q

Going down/across groups in Ionisation Energy

A

Across:
Number of protons will increase so more electrons are added in the same shell therefore the effective nuclear charge acting on the outermost electron is stronger.

Down:
Ionisation energy decreases as electron being lost is further away from the nucleus and has more shielding from inner electrons therefore electron is not held as strongly.

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5
Q

S subshell

A

Filling this gives extra stability to elements He, Be, Mg, Ca so first ionisation energy os above the trend

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6
Q

P subshell

A

Filling this gives N and P extra stability due to a higher value.

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7
Q

Ionic Radii

metals, non-metals, transition metals

A

Metals:
Groups 1-3 lose electrons forming +ve ions. Less shielding occurs so greater ENC. Ions are smaller than corresponding atom due to increased attraction.

Non-metals:
Gain electrons to form -ve ions. Therefore more electrons are in the same space creating more repulsion. Larger ionic radius.

Transition:
Groups 4-15 lose some outer electrons. They decrease their radii because there are fewer outer electrons (decreased repulsion). First electrons lost are from the valence shell therefore decreased size.

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8
Q

Atomic Radii definition

A

Calculated from the average distance between 2 atoms. Dependant on EDSeR.

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9
Q

EDSeR stand for?

A

Effective Nuclear charge - # protons in nucleus.
Distance of valence electrons from the nucleus.
Shielding - how many electrons between nucleus and valence shell.
Repulsion - of electrons (negative ions)

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10
Q

Atomic Radii

Down/Across

A

Down:
Electrons go into different energy levels (more shells), each shell is further away from the nucleus and increased shielding occurs due to more inner electrons. Radii gets bigger. Attraction between nucleus and valence electrons decreases.

Across:
Decreases due to increased ENC (more protons). Outside electrons are pulled closer to the nucleus. Similiar shielding effect due to same amount of energy shells between the nucleus and valence electrons. Radii gets smaller.

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11
Q

Electronegativity

A

Measure of attraction of an atom for a bonded pair of electrons.
Greater the Electronegativity, greater the pull on the electrons.

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12
Q

Polarity.
PEAS
EBELSDSO

A

Polarity
Electronegativity
Atoms
Symmetry

Electronegativity
Bond type 
Electron clouds
Lone pairs
Shape
Dipoles
Symmetry
Overall
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13
Q

Polar Covalent Bond Dipoles

A

Intermolecular forces - weak forces between molecules.
Temporary dipoles - temporary uneven distribution of electrons around an atom which repel electrons in nearby molecules inducing a small dipole. (Electrons move randomly)
Permanent dipoles - occurs between opposite ends of molecules. More polar a molecule, stronger the attraction.
Hydrogen bonds - strongest attraction force. Molecule must contain a H atom bonded to a F, O or N atom.

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14
Q

SHIP - Intermolecular Bonding

A

Shape
Hydrogen bonds
Instantaneous (temporary) dipoles
Permanent dipoles

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15
Q

Periodic table

A
  • Atomic number increases across a period - protons increase.
  • Atoms get smaller across a period - ENC increases, pulling electrons closer.
  • Atoms become larger going down a group - # of electron shells increase. ENC decreases from shielding.
  • Ions formed by elements on the left are smaller than their atoms as they lose electrons to have an empty shell.
  • Ions formed by elements on the right are bigger as they have gained electrons increasing the repulsion between valence electrons.
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16
Q

Transition Metals

A
  • Elements in d block always lose the 4s electrons first when forming ions.
  • Chromium (Cr) and Copper (Cu) are exceptions with greater stability with half-filled 4s and 3d orbitals.
  • Coloured ions are formed due to incomplete d orbitals. Colours are wave lengths not absorbed.
17
Q

SPEAR - Periodic Trends

A
Shielding 
# of Protons (EFN)
Energy levels/ electrons repelling 
Attraction of nucleus for valence electrons 
Relate to question
18
Q

How do you get Mass number?

A

Sum of protons + neutrons