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Last updated 3:36 AM on 10/10/23
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142 Terms

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atom

smallest unit of matter that possesses the properties of an element – building blocks of matter

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element

substance containing only one type of atom – its properties are determined by the number of protons in the atom

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molecule

unit made up of two or more atoms

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diatomic

molecule made up of two of the same type of atom

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compound

substance made up of two or more elements

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determines the element

number of protons in an atom

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isotopes

atoms with the same number of protons but different number of neutrons

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electrons are

negative

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protons are

positive

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neutrons are

have no charge

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determines the mass of an element

neutrons and protons

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1 mol (Avogrado’s number)

6.022×10²3

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molar mass

average isotopic atomic weight in grams

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mass-mol-atom conversion

<p></p>
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atomic oxygen

O

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molecular oxygen

O2

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measured mass

m=V(p)

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solution

a homogeneous mixture of substance composed of at least one
solute and one solven

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homogenous mixture

uniform mixture of only one phase (one substance)

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solute

substance that is dissolved in a solvent

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solvent (aq)

refers to water – usually present in much larger quantities than the solutes (Note: solvents need not be liquid

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aqueous

refers to types of solutions that have water as the solvent. Water is the most common solvent, with even blood plasma as an “aqueous solution”.

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types of aqueous solutions

Electrolytic Solutions and Non-electrolytic solutions

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Electrolytic Solutions

solutions that can conduct electricity – usually due to a dissociation reaction during dissolution resulting in individual charged cations and anions

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non-electrolytic solutions

solutions that do not conduct electricity – in such solutions, the dissolved molecules are electrically neutral and remain intact

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example of electrolytic solution

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stoichiometric reactant

is a reactant that is consumed in a reaction

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representation of a dissociation reaction

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example of non-electrolytic solution

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concentration

amount of a solute dissolved in a given volume of solvent (expressed as mass/volume or moles/volume).

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Concentrated vs. dilute solutions (aq)

concentrated solutions have a large amount of solute dissolved in a volume of water, while dilute solutions have a small amount of solute. a vendor)

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dilution (aq)

process of making a solution of lower concentration from a solution of higher concentration, by adding more solvent (water)

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standard solution

prepared solutions of known concentration

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how are standard solutions prepared

prepared by diluting more concentrated solutions, called stock solutions.

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stock solutions

will be of sufficient concentration to be able to make several
volumes of more dilute standard solutions and will also be of known concentration.

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<p>moles as concentrations</p>

moles as concentrations

concentration is moles/L

<p>concentration is moles/L</p>
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dilution

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stoichiometry

the relationship between the relative quantities of substances taking part in a reaction or forming a compound, typically a ratio of whole integers (i.e., the mole ratios from a balanced equation

<p><span style="font-family: sans-serif">the relationship between the relative quantities of substances taking part in a reaction or forming a compound, typically a ratio of whole integers (i.e., the mole ratios from a balanced equation</span></p>
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stoichiometric ratios help determine

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convert the mass of one substance to the mass of another

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example: how many grams of hydrogen are need to produce 68 g of ammonia?

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Some racing cars use methanol, CH3OH, as their fuel. What mass of water results from every Liter used (density = 0.8 g/mL)

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percent yields

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main reasons for incomplete reactions

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theoretical yield

the amount of product we would get if all reactants were converted entirely to products completely with nothing leftover (maximum amount in a perfect world)

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actual amount

the quantity of product actually obtained from a chemical
reaction in the lab

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Imagine a synthesis with two steps needed to make the desired product. We’re told the first step has an 85% yield, and the 2nd has a 90% yield. Calculate the final yield:

After 1st Step: Ideal x 85% = 0.85 of Ideal yield
After 2nd Step: 0.85 Ideal x 90% = 0.69 of Ideal yield
* You can see how fast the yield is dropping with each successive step

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yield reduction is

cumulative

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limiting reactant

The “leftover” reactants are said to be excess. The limiting reagent directly affects the potential yield for a reaction.

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how to find the limiting reactant

use the stoichiometric ratios and compare the number of moles of each starting material available against the number of moles required to make the desired product

<p>use the stoichiometric ratios and  compare the number of moles of each starting material available against the number of moles required to make the desired product</p>
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<p>limiting reactant example</p>

limiting reactant example

<p></p>
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limiting reactant table example

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law of conservation of mass

atoms cant be subdivided, created nor destroyed

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law of constant composition

atoms are combined, separated ir rearranged i constant ratios in chemical reactions

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j.j thompson

plum pudding atom - identified negatively and positively charged pieces of an atom → subatomic particles (electron, proton)

  • first evidence of isotopes (same element, different
    number of neutrons)

  • he theorized that electrons were embedded in the atom like chocolate chips in a cookie

<p>plum pudding atom - <span style="font-family: sans-serif">identified negatively and positively charged pieces of an atom → subatomic particles (electron, proton)</span></p><ul><li><p><span style="font-family: sans-serif">first evidence of isotopes (same element, different</span><span><br></span><span style="font-family: sans-serif">number of neutrons)</span></p></li><li><p><span style="font-family: sans-serif">he theorized that electrons were embedded in the atom like chocolate chips in a cookie</span></p></li></ul>
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rutherford gold foil experiment

He arranged a Sn detector around a piece of gold foil. He directed a beam of alpha particles (protons) at the gold fold.
particles were deflected at wide angles, and some were reflected back towards the detector.

<p><span style="font-family: sans-serif">He arranged a Sn de</span><span style="font-family: sans-serif">tector around a piece of gold foil. He directed a beam of alpha particles (protons) at the gold fold. </span><span><br></span><span style="font-family: sans-serif">particles were deflected at wide angles, and some were reflected back towards the detector.</span></p>
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atomic model

the nucleus is surrounded by the electrons
with mostly empty space in between

<p>the nucleus is <span style="font-family: sans-serif">surrounded by the electrons</span><br><span style="font-family: sans-serif">with mostly empty space in between </span></p>
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modern atomic orbital theory

diffuse electron cloud around nucleus (if we consider the relative size of the nucleus to the electron cloud, we see that if the electron cloud were the size of a football stadium, the nucleus would be the size of a pea.
- specific shapes and probability of locations for different levels.
- uses Heisenberg Uncertainty Principle to define states of electrons.

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characteristics of atoms

have

  • mass and volume

  • positive nuclei, charge Z

  • electrons (determine properties of an element)

  • unique physical and chemical properties

  • atoms attract one another and can combine

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atomic values example

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light - EM radiation in 400-700 nm range

  • is a form of electromagnetic radiation

  • behaves as a wave

  • composed of photons (particles)

  • interacts with atoms in a predictable and diagnostic way

  • Waves: repeating oscillations

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wavelength

the distance between two successive crests (units: meters or nanometers)

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frequency

the number of waves passing a certain point over a unit of time (units: s−1 = Hz)

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amplitude

height of the wave measured from the axis of propagation, a measure of intensity

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amplitude and intensity

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light is a

wave and has energy measured in J

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photoelecric effect

  • Below a certain frequency, no electrons were
    observed, no matter what the intensity.

  • The energy of the ejected electrons increased
    linearly with the frequency of light.

  • The number of emitted electrons increased with
    light intensity.

  • All metals show the same pattern, but each
    metal has a different threshold frequency.

<ul><li><p><span style="font-family: sans-serif">Below a certain frequency, no electrons were</span><span><br></span><span style="font-family: sans-serif">observed, no matter what the intensity.</span></p></li><li><p><span style="font-family: sans-serif">The energy of the ejected electrons increased</span><span><br></span><span style="font-family: sans-serif">linearly with the frequency of light.</span></p></li><li><p><span style="font-family: sans-serif">The number of emitted electrons increased with</span><span><br></span><span style="font-family: sans-serif">light intensity.</span></p></li><li><p><span style="font-family: sans-serif">All metals show the same pattern, but each</span><span><br></span><span style="font-family: sans-serif">metal has a different threshold frequency.</span><span style="font-family: Arial"><br></span></p></li></ul>
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Electrons are only ejected if

the frequency of light is high enough.

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the greater the intensity of light

the more photons, but if no individual photon has enough
energy (a high enough frequency) to remove an electron, then none are ejected

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planck equation

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When a metal surface absorbs a photon

the energy is transferred to an electron.

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binding and kinetic energy

Electron kinetic energy = Photon energy – Binding energy

  • Some of the energy must be used to cover the forces that bind the electron to the metal.

  • The remainder shows up as the kinetic energy of the ejected electron.

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typical results when light interacts with electrons

  • Photoionization: energy high enough to eject an
    electron

  • No ionization: atoms can gain energy, but do not
    ionize (light has lower energy than threshold)

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excited state of an electron

  • are unstable

  • will re-emit the excitation energy as light, heat, or
    motion (kinetic energy)

  • re-emitting the excitation energy returns the atom to ground state

  • ground state is an atom’s most stable state

<ul><li><p><span style="font-family: sans-serif">are unstable</span></p></li><li><p><span style="font-family: sans-serif">will re-emit the excitation energy as light, heat, or</span><span><br></span><span style="font-family: sans-serif">motion (kinetic energy)</span></p></li><li><p><span style="font-family: sans-serif">re-emitting the excitation energy returns the atom to ground state</span></p></li><li><p><span style="font-family: sans-serif">ground state is an atom’s most stable state</span></p></li></ul>
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absorption and emission spectra

  • Need a way to represent the energy of the bound electron to the energy of the excited electron.

  • Convention is to compare it to a hypothetical “free” electron at rest, whose energy is deemed to be 0.

  • Bound electron will have negative energy compared to this.

  • Excited electron will have positive
    energy compared to “free” electron.


<ul><li><p><span style="font-family: sans-serif">Need a way to represent the energy of the bound electron to the energy of the excited electron.</span></p></li><li><p><span style="font-family: sans-serif">Convention is to compare it to a hypothetical “free” electron at rest, whose energy is deemed to be 0.</span></p></li><li><p><span style="font-family: sans-serif">Bound electron will have negative energy compared to this.</span></p></li><li><p><span style="font-family: sans-serif">Excited electron will have positive</span><span><br></span><span style="font-family: sans-serif">energy compared to “free” electron.</span></p></li></ul><p><span><br></span></p>
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ground state

lowest energy state of an atom

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excited state

when an atom absorbs a photon

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energy level diagram

depicts the changed in energy of a atom

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When an atom emits a photon (or radiates heat)

it returns to the ground state

<p><span style="font-family: sans-serif">it returns to the ground state</span></p>
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absorption

Usually, a source of white light passes through a
sample, and the atoms absorb specific
frequencies of light.

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An absorption spectrum measures

the frequencies of photons that an atom absorbs

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emission

  • When excited atoms emit photons, the frequencies of the photon are specific.

  • An emission spectrum plots the intensity of light as a function of frequency.


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niels bohr

  • used planet model - electrons orbiting around the
    nucleus.

  • electrons can only occupy certain energy levels;
    quantized levels.


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energy state potential energy model

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absorption/emission

  • If the atom absorbs a photon = energy of atom increases.

    ΔE is positive : final energy is higher than initial energy

  • If the atom emits a photon = energy of atom
    decreases.
    ΔE is negative : final energy is lower than initial energy


<ul><li><p><span style="font-family: sans-serif">If the atom absorbs a photon = energy of atom increases.</span></p><p><span style="font-family: sans-serif">ΔE is positive : final energy is higher than initial energy</span></p></li><li><p><span style="font-family: sans-serif">If the atom emits a photon = energy of atom</span><span><br></span><span style="font-family: sans-serif">decreases.</span><span><br></span><span style="font-family: sans-serif">ΔE is negative : final energy is lower than initial energy</span></p><p><span><br></span></p></li></ul>
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electron “cloud”

Not an amorphous cloud, but actually is described by the probability of where an electron could be at any given point in time. These areas of probability are discrete and “quantized” - That is, an electron cannot exist in between these regions.


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properties of light

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properties of electrons

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orbital names

The names of orbitals from early
spectroscopic measurements.
s = “sharp”
p = “principle”
d = “diffuse”
f = “fundamental”

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orbital

A region of probability where an electron will exist at a specific
energy level. Its shape can be represented with an Electron Density Plot

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shell

A group of atomic orbitals with the same value of Principal
Quantum Number, n

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subshell =

orbital – denoted by letters s, p, d, f, etc. Each subshell has a
predictable 3D shape, a quantized energy level, and can accommodate a specific number of electrons

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valence electrons

those electrons that occupy the highest shell of an atom and are the electrons that form chemical bonds with other atoms

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quantum numbers

a unique group of 4 numbers assigned to describe the state of an individual electron in an atom. Can be considered the “address” of the electron on the atom

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principal quantum number (n)

a number specifying the theoretical energy level of and electron in an atom – refers to the “shell” the electron inhabits
(n= 1, 2, 3, 4 etc)

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azimuthal Quantum Number (l)

the number referring to the orbital in which an electron resides (s=0, p=1, d=2, f=3, etc.)

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Magnetic Quantum Number (ml))

is the quantum number that denotes the orientation of an orbital in space on the x-y-z 3D axis (between +l and –l)

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Spin Quantum Number (ms)

the quantum number that denotes the spin of an electron. The values can only be + ½ or - ½ .


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restrictions on quantum numbers for atoms

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