MCAT General Chemistry - COMPLETE

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493 Terms

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Nucleus

centre of atom, holds most mass, protons and neutrons

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fundamental unit of charge (e)

magnitude of charge of a proton or electron (e = 1.6 × 10-19 C)

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atomic mass unit (amu)

mass of one proton or neutron, exactly 1/12 the mass of carbon-12

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Proton

subatomic particle with charge of +1 e, mass = 1 amu, found in the nucleus

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atomic number (Z)

identifies element, number of protons in one atom

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neutron

subatomic particle with no charge of , mass > 1 amu, found in the nucleus

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mass number (A)

sum of the protons and neutrons in one atom

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Isotopes

Atoms that have the same atomic number but different mass numbers; have the same number of protons but varying numbers of neutrons; referred to by the name of element followed by mass number; same atomic number means similar chemical properties

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Electrons

subatomic particle with charge of - 1 e, mass = 1/2000 amu (often considered 0), found outside the nucleus

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Electron shell

a given distance from the nucleus, corresponding to a particular level of electrical potential energy

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Valence electrons

Electrons furthest from the nucleus; strongest interactions from surrounding environment and weakest with nucleus; involved with bonding

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Ion

charged atom

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Cation

positively charged ion

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Anion

negatively charged ion

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Hydrogen Isotope Names

protium : Z=1, A=1

deuterium : Z=1, A=2

tritium : Z=1, A=3

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Atomic weight

weighted average of naturally-occurring isotopes of an element; represents mass of ‘average’ atom in amu and mass of one mol of element in g.

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Mole (mol)

number of things equal to Avogadro’s number

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Avogadro’s number (NA)

6.02 × 1023

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Ernest Futherford

1910 - proved atom has small, dense, positively charged nucleus - gold foil experiment

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Max Planck

1899 - first quantum theory, energy emitted as electromagnetic radiation comes in discrete bundles/quanta - blackbody experiments/ultraviolet catastrophe

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Quantum (pl. quanta)

discrete amount of energy

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Planck relation

relates the energy of a quantum to frequency via a proportionality constant; E=hf=hν=hc/λ

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Planck’s constant (h)

proportionality constant, 6.626 × 10−34 J · s

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frequency (f/ν)

wave frequency of radiation

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Niels Bohr

1913 - developed planetary model of atom; quantized angular momentum

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angular momentum (L)

a vector quantity that describes the rotary inertia of an object or system; L=mvr=nh/2π

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Rydberg equation

E= - RH/n2= RH[1/ni2-1/nf2]; negative = attractive force towards nucleus; energy of electron increases at increasing n

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Rydberg unit of energy

2.18 × 10−18 J/electron

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orbit

defined pathway of an electron at a discrete energy level

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ground state

state of lowest energy; all electrons are in lowest possible orbitals

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excited state

at least one electron is at a higher energy level

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Atomic Emission Spectrum

spectrum of frequencies of electromagnetic radiation emitted due to electrons making a transition from a high energy state to a lower energy state; each element has unique set of energy levels

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line spectrum

representation of atomic emission spectra, where each line represents light at a specific frequency

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Lyman series

hydrogen emission lines from n ≥ 2 to n = 1

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Balmer series

hydrogen emission lines from n ≥ 3 to n = 2

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Paschen series

hydrogen emission lines from n ≥ 4 to n = 3

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Atomic Absorption Spectrum

the fraction of incident radiation absorbed by the material over a range of frequencies of electromagnetic radiation; electrons absorb specific amounts of energy to get excited; equal to emission wavelengths

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orbitals

regions of space where electrons are often localised, holds two electrons of opposite spins

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Heisenberg Uncertainty Principle

It is impossible to simultaneously determine, with perfect accuracy, the momentum and the position of an electron.

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Quantum numbers

numbers that describe electrons in an atome

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Pauli Exclusion Principle

No two electrons in a given atom can possess the same set of four quantum numbers.

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Principal quantum number (n)

represents energy level/electron shell, any positive integer value, max # electrons in shell - 2n2

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azimuthal (angular momentum) quantum number (l)

shape and number of subshells within given shell; integers btwn 0 and n-1, max # electrons in subshell = 4l+2

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Spectroscopic notation

shorthand representation of the principal and azimuthal quantum numbers; l=0=s, l=1=p, l=2=d, l=3=f

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magnetic quantum number (ml)

specifies orbital; integers from -l to l, including 0; 2 electrons per orbital

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spin quantum number (ms)

specifies spin orientation, ±½

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paired electrons

two electrons that occupy the same orbital and have opposite spins

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parallel spin

electrons in different orbitals but same spin number

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Electron Configuration

the pattern by which subshells are filled, as well as the number of electrons within each principal energy level and subshell; can be abbreviated by placing the noble gas that precedes the element of interest in brackets

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Aufbau (building-up) principle

Electrons fill from lower- to higher-energy subshells

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n + l rule

the lower the sum of the values of the first and second quantum numbers, n + l, the lower the energy of the subshell.

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Hund’s Rule

within a given subshell, orbitals are filled such that there are a maximum number of half-filled orbitals with parallel spins; due to electron repulsion; half-filled and fully filled orbitals have lower energies (higher stability) than other states

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paramagnetic

Materials composed of atoms with unpaired electrons will orient their spins in alignment with a magnetic field, and the material will thus be weakly attracted to the magnetic field

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diamagnetic

Materials consisting of atoms that have only paired electrons will be slightly repelled by a magnetic field

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Periodic Table of the Elements (PT)

ordering of the known elements by atomic weights/number; reveals a pattern of periodically recurring physical/chemical properties

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periodic law

the chemical and physical properties of the elements are dependent, in a periodic way, upon their atomic numbers

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periods

rows of PT; 7 representing the first 7 principal quantum numbers; each element in a given period has one more proton and one more electron than the element to its left

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groups/families

columns of PT; Groups contain elements that have the same electronic configuration in their valence shell and share similar chemical properties

may be named by Roman numeral of valence electrons and split into A/B classes OR 1-18 (modern IUPAC stanadard)

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valence shell

outermost shell of electrons

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valence electrons

The electrons in the valence shell, farthest from the nucleus and having the greatest amount of potential energy; can form bonds with valence electrons of other atoms

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A/representative elements

valence electrons in s or p subshells

IA - VIIIA

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B/nonrepresentative elements

include both the transition elements and the lanthanide and actinide series; may have unexpected electron configurations

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transition elements

have valence electrons in the s and d subshells; can have multiple oxidation states due to losing different numbers of s and d electrons

(Groups IB-VIIIB/3-12)

some (Cu, Ni, Ag, Au, Pd, Pt) are particularly nonreactive

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lanthanide and actinide series

have valence electrons in the s and f subshells

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metals

lustrous solids* with high melting points, high densities^; can be deformed without making; good conductors

low effective nuclear charge, low electronegativity (high electropositivity), large atomic radius, small ionic radius, low ionisation energy, low electron affinity

left and middle of PT

*except mercury (liquid @ RT)
^excpet lithium (half that of water)

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lustrous

shiny

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malleability

ability of metal to be hammered into shapes

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ductility

ability to be pulled or drawn into wires

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oxidation states

charges when forming bonds with other atoms

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conductor

can transmit heat and electricity

i.e. metals are good conductors because of their loose, free-moving valence electrons

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active metals

valence electrons found in s subshell

do not exist naturally in neutral forms; always found in ionic compounds/minerals/ores

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nonmetals

brittle and dull when solid; poor conductors; less unified in chemical and physical properties than metals

high electronegativity (low electropositivity), small atomic radius, large ionic radius, high ionisation energy, high electron affinity

upper right of PT

*except mercury (liquid @ RT)
^excpet lithium (half that of water)

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metalloids/semimetals

physical properties vary widely

chemical properties between metals and nonmetals; reactivities depend on elements with which they are reacting

staircase btwn metals and non-metals (B, Si, Ge, As, Sb, Te, Po, At)

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effective nuclear charge (Zeff)

electrostatic attraction between the valence shell electrons and the nucleus

increases along period; largely stable along group

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noble (inert) gases

have a full octet; minimal chemical reactivity; high ionisation energies and no measurable electronegativities

Group VIIIA/18

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atomic radius

equal to one-half of the distance between the centers of two atoms of an element that are briefly in contact with each other

decreases along period; increases along group

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ionic radii

  1. metals lose electrons and become positive, while nonmetals gain electrons and become negative

  2. metalloids can go in either direction, but tend to follow the trend based on which side of the metalloid line they fall on. (Si behaves more like a nonmetal, while (Ge) tends to act more like a metal)

non-metal ions closest to metalloid staircase are largest
metal ions closest to metalloid staircase are smallest

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Ionization energy (IE)/ionization potential

energy required to remove an electron from a gaseous species

subsequent removals will require increasing amounts of energy

increases along a period, decreases along a group

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Electron affinity

to the energy dissipated by a gaseous species when it gains an electron (reported as a positive number)

increases along a period; decreases along group

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Electronegativity

measure of the attractive force that an atom will exert on an electron in a chemical bond

increases along a period; decreases along group

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Alkali metals

possess most of the classic physical properties of metals, except that their densities are lower than those of other metals; only one loosely bound electron in their outermost shells - form monovalent cations

Group IA/1

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Alkaline earth metals

possess most of the classic physical properties of metals; two electrons in their outermost shells - form divalent cations

Group IIA/2

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Chalcogens

eclectic group of nonmetals and metalloids; some are crucial for normal biological functions, the rest are metallic and toxic, and all are toxic in high doses

Group VIA/16

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Halogens

highly reactive nonmetals with seven valence electrons; multiple states of matter; so reactive only found as ions or diatomic molecules

Group VIIA/17

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halide

anion of halogens

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hydration complexes

complex ions interactions with water

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compex ions

Any ion in which a central metal atom (normally a transition element) is surrounded by a group of ions or molecules (ligands)

known for varied bright colors; absorbs certain frequencies of light

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subtraction frequencies

light reflected or not absorbed by an object that gives the object its color

complementary color to the frequency that was absorbed

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complementary color

‘opposite’ colour, as in a colour wheel

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Maillard reaction

a nucleophilic reaction between the amino terminus of the peptide chain of a protein and the carbonyl functionality of a sugar to form an N-substituted glycosylamine; a complex series of rearrangements and other reactions to produce a set of compounds that gives cooked food its pleasing color and delectable flavor

ex. browning meat, crisping cookies

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molecules

combinations of bonded atoms

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chemical bonds

strong attractive forces between atoms in a molecule formed via the interaction of the valence electrons of the combining atoms

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octet rule

an atom tends to bond with other atoms so that it has eight electrons in its outermost shell, thereby forming a stable electron configuration similar to that of the noble gases

<p>an atom tends to bond with other atoms so that it has eight electrons in its outermost shell, thereby forming a stable electron configuration similar to that of the noble gases</p>
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Incomplete octet

stable with fewer than 8 electrons in their valence shell

  • hydrogen (2 electrons)

  • helium (2)

  • lithium (2)

  • beryllium (4)

  • boron (6)

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Expanded octet

Any element in period 3 and greater can hold more than 8 electrons

  • phosphorus (10)

  • sulfur (12)

  • chlorine (14)

<p>Any element in period 3 and greater can hold more than 8 electrons</p><ul><li><p>phosphorus (10)</p></li><li><p>sulfur (12)</p></li><li><p>chlorine (14)</p></li></ul><p></p>
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Odd numbers of electrons

Any molecule with an odd number of valence electrons cannot distribute those electrons to give eight to each atom

ex. nitric oxide (NO) has eleven valence electrons

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common elements that almost always abide by the octet rule

carbon, nitrogen, oxygen, fluorine, sodium, magnesium

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ionic bonding

one or more electrons from an atom with a low ionization energy, typically a metal, are transferred to an atom with a high electron affinity, typically a nonmetal; difference in electronegativity must be greater than 1.7 on the Pauling scale

<p>one or more electrons from an atom with a low ionization energy, typically a metal, are transferred to an atom with a high electron affinity, typically a nonmetal; difference in electronegativity must be greater than 1.7 on the Pauling scale</p>
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ionic crsytalline lattice

repeating rows of cations and anions; attractive forces between oppositely charged ions are maximized, and the repulsive forces between ions of like charge are minimized

<p>repeating rows of cations and anions; attractive forces between oppositely charged ions are maximized, and the repulsive forces between ions of like charge are minimized</p>
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covalent bonding

an electron pair is shared between two atoms, typically nonmetals, that have relatively similar values of electronegativity

<p>an electron pair is shared between two atoms, typically nonmetals, that have relatively similar values of electronegativity</p>