Chapter 2 Flashcards

1
Q
  1. State the major evidence for classifying light as a wave phenomenon. Use the de Broglie equation to show that matter has wavelike properties.
A

Lambda = h/mass*velocity

  • Young’s double slit experiment
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2
Q
  1. Describe the electromagnetic spectrum and calculate wavelength from frequency or frequency from wavelength. Also be able to calculate the energy of a photon from its frequency or wavelength.
A
  • Left to Right. Gamma rays, X - Rays, UV Light, Visible Light ( Blue - red) , Infrared, Microwave, Radio Waves
  • Gamma Rays are smallest wavelength, Radio waves are the largest wavelength
  • Gamma Rays are the highest frequency, Radio waves are the lowest frequency (Wavelength and frequency are inversely related)
  • Wavelength*Frequency = Speed of light Change in Energy = h*frequency => h*c/wavelength
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3
Q
  1. Given the energies of a set of energy levels, predict the wavelengths or frequencies of the lines in a line spectrum. Alternatively, calculate the energy level separations from the wavelength or frequency of the lines in a line spectrum.
A

Practice Problems

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4
Q
  1. State the major evidence for classifying light as a particle.
A
  • Photoelectric effect
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5
Q
  1. Explain the term “quantized” as it is applied to energy in this chapter.
A
  • Energy can be gained or lost only in integer multiples of h*frequency.
  • Each of these small “packets” of energy is called a quantum. A system can transfer energy only in whole quanta.
  • = atoms and molecules can’t accept just any amount of energy, but instead only the amount of energy that exactly matches the size of these quanta.
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6
Q
  1. Describe the photoelectric effect and discuss what was learned from a study of this effect.
A

Refers to the phenomenon in which electrons are emitted from the surface of a metal when light strikes it.

(a) Light with frequency less than the threshold frequency produces no electrons.
(b) Light with frequency higher than the threshold frequency causes electrons to be emitted from the metal.

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7
Q

Summarize the series of electromagnetic radiation for the names

A
  • Lyman: Emit to n = 1, Large transitions, Uv light
  • Balmer: Emit to n= 2, Medium transitions, Visible light
  • Paschen: Emit to n= 3, small transitions, Infrared “
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8
Q
  1. Explain what an atomic (line) spectrum is and describe the kind of information that it gives about the energy levels in an atom.
A
  • A spectrum in which spectral line can be distinguished.
  • Because each spectral line can be clearly distinguished, match each line to the transition between energy levels responsible for it.
  • Changes in energy between discrete energy levels in hydrogen will produce only certain wavelengths of emitted light,
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9
Q
  1. Distinguish between a continuous spectrum and a line spectrum.
A
  • Continuous spectrum results when white light is passed through a prism. This spectrum contains all the wavelengths of visible light.
  • Line spectrum: emission spectrum, only shows wavelengths for which the photons were emitted
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10
Q
  1. Distinguish between an emission and an absorption spectrum.
A
  • Absorption lines are where light has been absorbed by the atom thus you see a dip in the spectrum
  • Emission spectra have spikes in the spectra due to atoms releasing photons at those wavelengths.
  • EX: Hydrogen for example, indicates that only certain energies are allowed for the electron in the hydrogen atom.
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11
Q
  1. Explain how emission spectra and absorption spectra of the same element are related.
A

the lines in the emission spectrum of a substance are at the exact same wavelengths as the lines in the absorption spectrum of the same substance.

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12
Q
  1. State the Rydberg formula and explain its relationship to the spectrum of hydrogen atoms.
A
  • Use Rydberg equation to calculate the wavelength of light emitted when energy is emitted from n final to n initial
  • Look up formula - use exmple
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13
Q
  1. State the Bohr model of the hydrogen atom and explain its significance (work on this answer).
A

Key things to remember:

  • Energy levels are stationary states
  • Change in energy casues by electrons between stationary states
  • When electron move, absorbing electron (increase in energy), or emitting energy (decreasing energy)
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14
Q
  1. Explain the relationship of a line in a spectrum to the atom’s energy levels and photons emitted by that atom.
A

The lines on the atomic spectrum relate to electron transitions between energy levels, if the electron drops an energy level a photon is released resulting in an emission line and if the electron absorbs a photon and rises an energy level an absorption line is observed on the spectrum.

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15
Q
  1. State the Heisenberg Uncertainty Principle and explain its meaning.
A
  • The exact position of the electron is never known, which is consistent with the Heisenberg uncertainty principle:
  • it is impossible to know accurately both the position and the momentum of a particle simultaneously.
  • Think about how small the mass of an electron is - this helps to explain it’s uncertainty
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16
Q
  1. Describe wave‐particle duality.
A

Electromagnetic radiation, which was previously thought to exhibit only wave properties, seems to show certain characteristics of particulate matter as well.

17
Q
  1. Discuss the probability interpretation of an atomic orbital.
A
  • The square of the wave function indicates the probability of finding an electron near a particular point in space.
  • The maximum in the curve occurs because of two opposing effects.
    • The probability of finding an electron at a particular position is greatest near the nucleus, but the volume of the spherical shell increases with distance from the nucleus.
  • Therefore, as we move away from the nucleus, the probability of finding the electron at a given position decreases, but we are summing more positions.
  • Thus the total probability increases to a certain radius and then decreases as the electron probability at each position becomes very small. “
18
Q
  1. Give the allowed values and names of the quantum numbers n, l, and ml and relate how each affects the energy, shape, orientation, and average radius of the orbital.
A

Make the table and make the filling in electron shell oribitals

19
Q
  1. Sketch the shapes and orientations of s, p, and d orbitals.
A

Sketch the shapes

20
Q
  1. Describe the Pauli Exclusion Principle.
A

no two electrons in a given atom can have the same set of quantum numbers

21
Q
  1. Use the Aufbau principle and Hund’s rule to diagram an atom’s or ion’s electron configurations.
A
  • Aufbau: As protons are added one by one to the nucleus to build up the elements, electrons are similarly added to these hydrogenlike orbitals.
  • Hund: For an atom with unfilled subshells, the lowest energy is achieved by electrons occupying separate orbitals with parallel spins, as far as allowed by the Pauli exclusion principle. “
22
Q

Exceptions to Aufbau

A

Cr and Cu - both valence shell configurations move one from the 4s into the 4p - making them stable as half full

23
Q

Atomic radius (nuclear charge are the same thing)

A
  • Down a group - radius increases, the size gets bigger, and the electrons further away = less effective nuclear charge
  • Left to right on a period - radius decreases, adding electrons to the same shell, but also adding protons, the protons are better able to pull on the the eletrons
24
Q

Atomic radius (nuclear charge) - Ions

A
  • An ion has the same number of protons
  • Nuetral atom < Anion anions have more electrons - aka a fuller electron cloud
  • Nuetral atom > Cation B/C cations got rid of their valence shell, made the entire atom smaller, made electron cloud smaller
25
Q

Ionization energy

A
  • X => X- How tightly an atom is holding its electrons
  • Left to right, inoization energy increases
  • Going down a group ionization energy decreases
26
Q

Successive Ionization Energy

A

Overall trend - successive ionization energy increases, but BIG jump at core electrons

27
Q

Exceptions to Ionization Energy Trends

A

Phosphorus and sulfur are neighboring elements in Period 3 of the periodic table and have the following valence electron configurations: Phosphorus is 3s^2 3p^3 , and sulfur is 3s^2 3p^4 . Ordinarily, the first ionization energy increases as we go across a period, so we might expect sulfur to have a greater ionization energy than phosphorus. However, in this case the fourth p electron in sulfur must be placed in an already occupied orbital. The electron–electron repulsions that result cause this electron to be more easily removed than might be expected.

28
Q

Electron affinity

A

is the energy change associated with the addition of an electron to a gaseous atom

29
Q

What is group 1 on the periodic table?

A

“Alkali metals - *1s in valence shell *likely to form+1 cations “

30
Q

What is group 2 on the PT?

A

“Alkaline Earth Metals *s^2 valence shell electrons *likely to form +2 cation”

31
Q

What is group 17 on the PT?

A

“Halogens *7 valence electrons s^2,p^5 *likely to become -1 anion “

32
Q

What is group 18 on the PT?

A

“Nobel gases *Full outershell”

33
Q

What are groups 3-12 on the PT?

A

“Transition Metals *d block “

34
Q

Why are the values for emission negative?

A

Energy at infinity corresponds to the electron being infinitely far away from the nucleus. When it is bound to the nucleus at lower values of n, the atom is more stable, thus lower energy, which must then be negative.

35
Q

What is the periodic table mostly made of?

A

Metals!