Unit 2 Exam Flashcards

1
Q

Daltons Atomic Theory

A
  1. All atoms of a given element are identical (except Isotopes)
  2. Atoms of different elements have different masses
  3. compounds are made of different elements combined in specific ratios
  4. in a chemcal reaction atoms are neither created or destroyed
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2
Q

Proton

A

Postively Charged particle

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3
Q

Neutron

A

nuetral particle

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4
Q

electron

A

negatively charged

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5
Q

Necleus Characteristics

A
  • contains protons and neutrons
  • positive charge
  • determines mass of atom
  • extremely small, but dense
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6
Q

Mass #

A

of protons plus # of neutrons

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7
Q

Atomic Number

A

Number of Protons

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8
Q

How to determine the # of neutrons

A

Mass # - atomic #

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9
Q

Determine the # of electrons

A

of protons for a neutral atom

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10
Q

Isotope

A

Something has the same # of protons but different # of neutrons

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11
Q

Ion

A

charged particle formed by gain or loss of electron

(+) ion loss of electron

(-) ion gain of electron

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12
Q

J.J. Thomson (1897)

A

Determined the charge to mass ratio of an electron

used the cathode ray tube (An electric field is set up between 2 plates, + and - charged and a magnetic field is applied perpendicular to the electric field and the electrons are fed between the the two plates)

Found that the charged particles (electrons) were the same regardless of the metal he used for the cathode.

Concluded that electrons are part of the makeup of all atoms

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13
Q

Milliken Oil Drop Exp (1909)

A

Determined the charge of electron then using thomsons value calculated mass of an electron

Observed tiny electrically charged oil droplets. From the strength of the electric field required to overcome the pull of gravity on the droplets, he determined the values of the charges on the particle.

Experiment Setup: oil is sprayed as a fine mist into a chamber containing a charged gas, and the location of an oil drop is monitored by using a microscope. Charged particles (ions) are generated in the gas by exposing it to x-rays. The fall of the charged droplet is balanced by the electric field.

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14
Q

Ernest Rutherford Exp (1908)

A

Determined nucleus (+) charge and very dense and atom is mostly empty space.

Experiment required shooting alpha particles toward a piece of platinum foil only a few atoms thick. Found almost all alpha particles passed through and were deflected only slightly (about 1 in 20,000 deflected more than 90 degrees). some bounced back straight in direction they had come.

When a positively charged alpa particle scored a direct hit on one of the minute but heavy platinum nuclei, the alpha particle was strongly repelled by the positive charge of the nucleus and deflected through a large angle.

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15
Q

mass spectrometer

A

can measure the mass of isotopes and % abundances

Deflection depends on:

  1. Magnitude of acclerating voltage
    1. higher voltage —-> beam moves more rapidly
      1. less deflection
  2. magnitude field strength-stronger field deflects beam more
  3. masses of particle-heavier particles deflected less
  4. charges on particles
    1. higher charges are deflected more
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16
Q

Steps for calculating average atomic mass

A
  1. change % to decimal
  2. multiply by mass
  3. Add
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17
Q

Wavelength

A

distance it takes for wave to repeat itself

C=λv

C=speed of light

v=frequency (given in Hz which is = to cycles/sec or s-1)

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18
Q

Energy Equation

A

E=hv

E=energy

h=planks constant

v=frequency

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19
Q

Neils Bohr (1930’s?)

A

Said electrons have a quantum value—can only have certain values

farther from the necleus—-higher the energy

there are places you expect to find atoms then gaps where you don’t

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20
Q

Balmer Series

A

visible spectrum

n1 = 2

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21
Q

Lyman Series

A

ultra-violet

n1 = 1

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22
Q

Bohr Frequency condition

A

V=Z2R( 1/n12 - 1/n22)

R = Ryberg constant

23
Q

Photoelectric Effect

A

shows the particle (photon) nature of electromagnetic radiation

When light of sufficient energy strikes the metal, an electron is knocked off, it travels to the positive electrode and current flows to the circuit. ( see image)

24
Q

Classical Theory

A

If low levels of light are emitted long enough then it should

EK = 1/2 mv2 = hν−ϕ

ϕ = energy needeed to remove electron work function

hv= energy supplied by photon

25
Q

deBroglie Relationship

A

moving particles have wave properties

λ=h/mv p=mv λ=h/p

m=mass

h=planks constant

p=momentum

26
Q

Heisenberg Uncertainty Principle

A

∆p ∆x = 1/2 ħ

ħ = h(planks constant)/ 2π = 1.054 x 10-34 J s

∆p= m∆v

27
Q

Schrodingers Equation

A

(-ћ2d2Ψ /2mdx2) + V(x) Ψ = EΨ

m= particle mass

V(x)= potential energy

probability of finding a particle is proportionate to Ψ 2

28
Q

Energies allowed for particle in the box

A
29
Q

Electron Shells

A

Main energy level; contains e- that are about same distance from nuclues and have about same energy

30
Q

Max number of e- in a shell

A

2n2

n= shell #

31
Q

subshells

A

contains e- that are same distance from the nucleus and have the same energy

of subshells is = to the shell #

labeled with shell # and a letter

32
Q

Orbitals

A

region of highest probability of finding an e-

33
Q

Max # of e- in any orbital

A

2e-

34
Q

radial nodes

A

1s—–0 radial nodes

2s——1 radial node

3s——-2 radial nodes

35
Q

Aufbau Principle

A

e- will usually occupy the lowest energy subshell available

36
Q

For (+) ion

A

e- are removed from the highest(outermost) shell

37
Q

Hund’s Rule

A

e- will fill orbitals singley before pairing

38
Q

Shell # for s and p elements

A

equals the row number

39
Q

shell # for d’s

A

= row#-1

40
Q

shell # for f’s

A

=row # - 2

41
Q

Electron config exceptions

A

Cu—s1d10

Ag—s1d10

Au—s1d10

Rg—s1d10

Cr—s1d5

Mo—s1d5

Ni—s2d8

Pd—d10

Pt—s1d9

42
Q

diamagnetic

A

all e- are paired

43
Q

paramagnetic

A

one or more unpaired e-

44
Q

Pauli Exclusion principle

A

no 2 e- in an atom can have the same set of quantum #’s

45
Q

Quantum numbers

A

n-shell

n,l - subshell

n,l,ml - orbital

n,l,ml,ms - an e- in an orbital

46
Q

Representative elements

A

s and p blocks

47
Q

Periodic Group Names

A
48
Q

Atomic Radii (how big is an atom) Trend

A
49
Q

Ionization Energy

A

amount of energy required to remove the outer most e- from an atom in the gaseous state

50
Q

2nd ionization energy

A

amount of energy to remove a 2nd e-

(lower ionization means want to form positive ions)

51
Q

Electron Affinity (EA)

A

amount of energy released when an atom in the gaseous state gains an e-

52
Q

electronegativity

A

the attraction an atom has for a shared pair of e-

53
Q

Ionic radii

A

positive ion is smaller than its neutral atom

54
Q

Isoelectronic Ions

A

ions w/ same number of e-

the ion w/ least # of protons will be the largest