Structure 1 Flashcards

1
Q

Homogeneous Mixture.

A
  • Components in same phase
  • Even distribution of particles
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2
Q

Heterogeneous Mixture

A
  • Components in different phases
  • Uneven distribution of particles
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3
Q

Pure Substance

A
  • Elements
  • Compounds

(Chemically bonded)

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4
Q

Mixtures

A
  • Homo/hetero-geneous

(Physically bonded)

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5
Q

Kinetic Molecular Theory

A
  • All matter made up of constantly moving particles
  • Energy of particles proportional to temperature
  • Change in energy can drive change in state
  • Empty space between particles increase from solid —> gas
  • Attractive forces between particles increase as particles move closer
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6
Q

Relative Atomic Mass

A

Weighted average mass of an atom compared to 1/12th the mass of Carbon-12

—> ∑(%abundance x isotopic mass)/100

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7
Q

Mass Spectrometry (HL)

A

Measuring the individual masses of atoms in an element.

1) Vaporization
2) Ionization - electrons fired at sample, particles made into +1 charge
3) Acceleration - electric field
4) Deflection - magnetic field (effect by mass, results in change in velocity)
5) Detection - can detect the number of isotopes depending on the speeds of particles

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8
Q

Aufbau Principle

A

Lowest energy levels filled first.

—> Exceptions: |Cr| & |Cu|
—> Half filled (Cr)/full (Cu) sublevels are more stable than partially filled ones.
—> Exception occurs due to very small energy diff. Between 3d & 4s sub-levels.

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9
Q

Hydrogen Emission Spectra (HL)

A

1) …—> n=1 (Lyman Series - UV)
2)…—> n=2 (Balmer Series - Visible Light)
3)…—> n=3 (Paschen Series - Infrared)

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10
Q

Convergence Limit

A

Energy levels move closer together as they are further away from the nucleus. Eventually they converge and no extra energy is needed to promote an electron so it becomes ionized.

—> You can calculate the First IE using the frequency of the convergence limit (E = hf)

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11
Q

Hund’s Rule

A

Orbitals within same level filled first/no empty space.

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12
Q

Pauli’s Exclusion Principle

A

Positive & negative spin of electrons in orbitals.

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13
Q

Ionization Energy

A

The energy required to remove one mole of electrons from one mole of gaseous atoms.

—> General trend: increase across period, decrease down group
—> Exceptions: Slight drop between sublevels (eg. p having slightly higher energy which counteracts increase in Zeff)

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14
Q

Ground State

A

The lowest energy level occupied by an electron in an atom.

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15
Q

Empirical Formula

A

Simplest whole number ratio of atoms in a compound.

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16
Q

Mole

A

Set number of particles in a certain element/substance

—> 6.02 x 10^23 /mol (Avogadro’s constant)

17
Q

Ideal Gas Model

A

(Assumptions)

1) Collisions between particles are purely random (no IMF) & elastic (total KE/momentum conserved)
2) Particles have negligible volume
3) Particles have no potential energy (Internal energy only proportional to avg. kinetic energy)

(Deviations)

  • (Deviate) significantly at (low temperatures and high pressures) because (particles grow closer) together - making (IMF more significant).
18
Q

Ideal Gas Laws

A

Combined gas law: PV = nRT (main)

Additional: PV = NkT

Avogadro’s law: (P1V1)/T1 = (P2V2)/T2

  • P & V (Boyle)
  • V & T (Charles)
  • P & T (Gay-Lussac)
19
Q

Volume of ideal gases

A

V = (n)(Vm)

n —> moles
Vm —> molar volume = 22.7 dm^3/mol