Lecture 1: Atoms Flashcards

1
Q

What is each atom composed of?

A
  1. Made of a atomic nucleus(with protons and neutrons: together called nucleons) and electrons
    1a. Proton: 1amu
    1b. Neutron: 1amu (if atom has different neutrons: isotopes)
    1c. Electron: much smaller than protons and neutrons
  2. Charge: 1e=1.6x10^-19C
  3. Rutherford model says that atoms are mostly empty space with electrons orbiting a fixed, positive nucleus
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2
Q

Element notation

A
  1. Nuclide: When the number of protons and neutrons are specified for an atom
  2. X (A above) (Z below)
    2a. A: mass number =protons+ neutrons
    2b. Z: atomic number=protons
  3. Protons and neutrons have same mass, electrons are much smaller
  4. There are as many electrons as there are protons
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3
Q

Atomic mass vs atomic weight

A
  1. Atomic weight=(average of composition)/number of isotopes=((mass of 12C x percent composition) + (mass of 13C x percent composition))/number of isotopes (2)
    1a. Shown on periodic table with it being the average of the isotopes masses
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4
Q

Coulomb’s law

A
  1. Like charges repel, opposite charges attract
  2. Creates these equations:
    2a. Force: F=k(q1q2)/r^2
    2b. Energy: U=k(q1q2)/r
    2c. Potential: V=kq1/r
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5
Q

Plancks

A
  1. Planck said that energy (E) is transferred (emitted (low energy, n down) or absorbed (high energy, n up)) as photons according to E=hf where h=7x10^-34 Js
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6
Q

The Photoelectric effect

A
  1. Photon must have a minimum energy (work energy) in order to eject an electron (energy of ejected electron is the kinetic energy)
    1a. Kinetic energy=Energy of photon-Work energy
  2. intensity can increase by increasing number of photons or the frequency of each photon
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7
Q

Line spectra

A
  1. Continuous spectra: rainbow in visual spectra
    1a. Radiowaves-microwaves-infrared-(ROYGBIP)-ultraviolet-x rays-gamma rays
    1b. Gains energy as it goes to gamma rays
  2. Emission line spectrum: measures emitted
  3. Absorption line spectrum: measures all except absorbed
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8
Q

The Bohr Atom

A
  1. Says electrons are confined to a circular orbit around the nucleus which corresponds to energy levels of electrons
    1a. If energy/radiation is emitted, electron moves to lower energy
    1b. If energy is absorbed, electron moves to higher energy
  2. The Bohr model: Applies to any hydrogen like atom (atom with 1 electron)
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9
Q

Ground state vs excited states

A
  1. Ground: when n=1, electron is at lowest energy state
    1a. As n increases, the electron is in its excited states, photon is absorbed
    1b. As n decreases, photon is emitted
  2. Difference in energy between the energy states is: E=hc/wavelength
    2a. H=planck, c=speed of light (3x10^8)
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10
Q

Heinsenberg uncertainty principle

A
  1. There is a uncertainty in the position and momentum of a particle
  2. Momentum (p)=mv (mass*velocity)
  3. De broglies postulate: wavelength=h/p =h/mv
    3a. Planks constant=h
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11
Q

Quantum numbers

A
  1. Principle quantum number (n): (shell) # matches row of periodic table (except d, f)
    1a. Max # of electrons in a single energy level: 2n^2
  2. Azimuthals quantum number (l): gives 3D shape (sub shell) (l=0->(n-1))
    2a. 0=s, 1=p, 2=d, 3=f
    2b. Max # of electrons in a single sub shell: 4l +2
  3. Magnetic quantum number (ml): gives orbital subtype from (-l to l): values=2l +1
  4. Spin quantum number (Ms): gives electron spin in +1/2 or -1/2
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12
Q

Paulis exclusion principle

A
  1. Says 2 electrons occupying the same orbital have opposite spins so are paired
  2. No 2 electrons can share the same 4 identical quantum numbers
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13
Q

Aufbau/building up principle

A
  1. States that electrons will occupy lower energy orbitals before higher energy orbitals
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14
Q

Hunds rule

A
  1. All orbits must have one electron before any orbitals can obtain a second electron
  2. Fill spin one way in subshells before you do opposite spins
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15
Q

Magnetism

A
  1. Diamagnetic: spin paired electrons, opposing spins , weakly repelled by external magnetic field
  2. Paramagnetic: not spin paired, attracted to external magnetic field
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16
Q

Metals, nonmetals and metalloids

A
  1. Metals: lose electrons to form oxidation states (Easily oxidized), deductible, malleable , have thermal conductivity (heat transfer) and electrical conductivity (charge transfer) and luster (Shine)
  2. Nonmetals: lower melting/boiling points
  3. Metalloids: both
17
Q

Groups on periodic table (across)

A
  1. Hydrogen: unique nonmetal
  2. Group 1A: alkali metals: soft metals with low densities/melting points, reactive with nonmetals to form ionic compounds
  3. Group 2A: alkaline earth metals: pure, harder/denser/melt at higher temps than alkali,
  4. Group VIIA: halogens: want to gain one electron
  5. Group VIIIA: Nobel/inert gases: stable
  6. Transition metals: d block, formed by losing electrons from s subshell first
18
Q

Effective nuclear charge (Zeff)

A
  1. Effective nuclear charge: the charge an electron seems to experience from a nucleus (between 1 to Z(charge on nucleus))
    1a. Shielding effect: the more electrons an electron has around it, the less it feels the charge from the nucleus
  2. Zeff: Increases to the right/down
19
Q

Periodic trend: atomic radius

A
  1. Measure of size of atom
  2. Greatest bottom/ left (relates to Zeff)
20
Q

Periodic trend: ionization energy (IE)

A
  1. Energy to remove an electron from an atom
    1a. First ionization energy: energy to detach electron from neutral atom and form 1+ cation
    1b. Second ionization energy: energy to remove second electron from same atom and form 2+ cation / always greater than the first
  2. Trend: greatest top/right
21
Q

Periodic trend: electron affinity

A
  1. How much an atom wants to hold/accept the electron
  2. Trend: greatest top/right (except Nobel gases, 5A, and 2A)
    2a. Half filled/fully filled subshells are very stable and don’t want to chain electrons
22
Q

Periodic trend: electronegativity (X)

A
  1. Tendency for an atom in a compound to attract an electron to itself
  2. Trend: greatest right/top
  3. H(2), C(2.5), N(3), O(3.5), F(4)