General Chemistry Intro Flashcards

(120 cards)

1
Q

Atoms

A

All mass consists of tiny particles called atoms

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2
Q

Composition of an atom

A

Nucleus surrounded by electrons

Necleons: protons and neutrons that make up the nucleus, approximately equal in size and mass

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3
Q

Strong nuclear force

A

Protons and neutrons are held together to form the nucleus by this force
Stability can be measured by binding energy: energy that would be required to break the nucleus into individual protons and neutrons

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4
Q

Angstrom

A

One angstrom is 10^-10 m

Radius of nucleus on order of 10^-14 Angstroms

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5
Q

What distance are electrons from the nucleus?

A

1 to 3 Angstroms

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6
Q

Mass of subatomic particles

A

Electron: 5.5 x 10^-4 amu
Proton: 1.0073 amu
Neutron: 1.0087 amu

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7
Q

Why is matter mostly empty space?

A

Matter is composed of atoms

Atom is composed of mostly empty space

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8
Q

Electron Charge

A

Symbol, e
Equal to 1.6 x 10^-19 Coulombs or C (SI unit for charge)
Charge of an electron or proton

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9
Q

Element

A

Building blocks of compounds and cannot be decomposed into simpler substances by chemical means

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10
Q

Atomic number, Z

A

Number of protons, provides identity of element

Each element has a unique number of protons

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11
Q

Mass Number, A

A

Number of protons plus neutrons
Varies depending on the number of neutrons
Mass number of element is approximately equal to atomic weight or molar mass of element

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12
Q

Isotope

A

Two or more atoms of the same element that contain different numbers of neutrons
Nucleus of specific isotope is called nuclide
Isotopes have similar chemical properties

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13
Q

Isotopes of Hydrogen

A

{1}^H, {2}^H, {3}^H
Protium, Deuterium, and Tritium
99.98% of naturally occurring hydrogen is protium

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14
Q

Isotopes of Carbon

A

{12}^C, {13}^C, {14}^C

6 neutrons, 7 neutrons, and 8 neutrons, respectively

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15
Q

Ion

A

Number of electrons and protons are not equal in atom
Atom carries a charge and is not electrically neutral
Cations: positively charged, have fewer electrons than protons
Anions: negatively charged, have more electrons than protons
Salt: neutral compound composed of positive and negative ion together

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16
Q

What does changing the number of neutrons, electrons, and protons do to an element?

A

Creates isotope, creates ion, and changes to another element, respectively

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17
Q

What happens to the atomic radius when a neutral atom loses an electron to become a cation? gains an electron to become an anion?

A

Atomic radius never changes, ionic radius does
Ionic radius gets smaller because positive charge of the nucleus exerts a greater attractive force on each valence electron, pulling them closer the nucleus
Loss of electron reduces repulsive forces between electrons further contributing to decrease in size
Loss of electron also increases Z_eff for each electron
Ionic radius gets larger

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18
Q

Periodic Table

A

Table that lists elements from left to right in order of their atomic numbers
Each horizontal row is called a period
Each vertical column is called a group or family
Elements in the same family share similar chemical and physical properties

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19
Q

What are the two methods commonly used to number groups in the periodic table?

A

Number 1 through 18 left to right is newer

Separate groups into A and B and then number with Roman numerals is older

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20
Q

What are three common groups for elements in the periodic table?

A

Nonmetals on right, metals in middle and left, metalloids along diagonal separating the metals and nonmetals

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21
Q

Metals

A

Large atoms that tend to lose electrons to form positive ions and oxidation states
Atoms in a sea of electrons, fluid-like nature of valence electrons
Metallic character: ductility (easily stretched), malleability (easily hammered into thin strips), thermal and electrical conductivity, and luster
Metal atoms easily slide past each other
Electrons move easily from one metal atom to the next, transferring energy or charge (heat or electricity)
All metals except mercury exist as solids at room temperature
Typically lose electrons to become cations (form ionic bonds)

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22
Q

Groups of periodic table that you should know

A
Group (1): alkali metals, IA
Group (2): alkaline earth metals, IIA
Group (16): oxygen group, VIA
Group (17): Halogens, VIIA
Group (18): Noble gases, VIIIA
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23
Q

What are the names of the periods of the bottom two rows of the periodic table?

A

Lanthanides on top

Actinides on bottom

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24
Q

Nonmetals

A

Diverse appearances and chemical behaviors
Molecular substances generally made with nonmetals, because tend to covalently bond
Lower melting points than metals
Tend to form anions, reacting with cations to form ionic compounds

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25
Metalloids
Some metallic and some non-metallic characteristics
26
Representative elements
Section A groups: 1, 2, 13, 14, 15, 16 17, 18 Main-group elements Make ions by forming closest noble gas electron configuration Metals tend to form cations and nonmetals tend to form anions to form noble gas config.
27
Transition Metals
Section B groups (3, 4, 5, 6, 7, 8, 9, 10, 11, 12) | When transition metals form ions, lose electrons from highest s-subshell and then from d-subshell
28
Common ions formed by transition metals
Group 11 makes +1 ions: Cu+, Ag+, Au+, but also Cu2+, Au3+ Group 6: Cr3+, Group 7: Mn2+, Group 8: Fe2+, Fe3+, Group 9: Co2+, Group 10: Ni2+, Pt2+, Group 12: Zn2+, Cd2+, Hg_2 2+, Hg2+ Group 13: Al3+ Group 14: Sn2+, Pb2+ Group 15: Bi3+
29
What types of orbitals will an ion have, if possible?
Half-filled or completely filled orbitals Group 1: half-filled s orbital Group 2: completely filled s orbital Group 7: (VIIB) half-filled d orbital Group 12: (IIB) completely filled d orbital Group 15: half-filled p orbital Group 18: completely filled p orbital
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Valence electron
Electrons in the outermost shell Elements in the same group have same number of valence electrons - Tend to make same number of bonds and exist as similarly charged ions - Contribute most to an element’s chemical properties - Located in outermost shell of an atom - Usually only e-‘s from s and p are considered valence e-‘s
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Group 1
Alkali Metals: soft metallic solids with low densities and low melting points Form 1+ cations (Na+), highly reactive (reacting with most nonmetals to form ionic compounds and hydrogen to form hydrides) React exothermically (explosively) with water to produce respective metal hydroxide and hydrogen gas Exist only in compounds in nature Hydrogen is nonmetal and not like other elements, forms covalent bonds
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Hydrogen
Unique and unlike other elements, does not conform to own family Nonmetal, can form covalent bonds, or ionic bonds with metal cations Hydrogen is usually colorless, odorless diatomic gas Acid-base chemistry and intermolecular forces
33
Group 2
Alkali earth metals: harder, more dense, and melt at higher temperatures than alkali metals Form 2+ cations (Mg2+) Less reactive than alkali metals because highest energy electron completes s orbital Heavier alkaline earth metals are more reactive than lighter ones Only exist as compounds in nature
34
Group 14 elements
Form four covalent bonds with nonmetals, but not all are nonmetals 1 nonmetal, 2 metalloids, and 2 metals All beyond second period form two additional bonds with Lewis bases using d orbitals Carbon is only element to form strong pi-bonds making double or triple bonds
35
Group 15 elements
Can form 3 covalent bonds All beyond second period can form two additional covalent bonds by using d orbitals, and can further bond with Lewis base to form sixth covalent bond Nitrogen: fourth covalent bond by donating lone pair of electrons to form a bond, forms strong pi-bonds to make double and triple bonds Phosphorous: can form weak pi-bonds to make double bonds
36
Group 16 elements
Chalcogens, or oxygen group Oxygen second most electronegative element, divalent and can form strong pi-bonds to make double bonds and exists as O2 (dioxygen) or O3 (ozone) Oxygen reacts with metals to form metal oxides and with alkali metals to form peroxides (Na2O2) and super oxides (KO2) Sulfur: most common form of pure sulfur is yellow solid S8. Metal sulfides (Na2S) are most common in nature. Can form 2, 3, 4, 5, or 6 bonds due to 3d orbital, can form strong double pi-bonds also
37
Group 17 elements
Halogens Radioactively stable elements are Fluorine (F2 gas at room temp), chlorine (Cl2 gas at room temp), bromine (Br2 liquid at room temp), and iodine (I2 solid at room temp) Highly reactive, like to gain electron to attain a noble gas config In compounds: - Oxidation states as high as 7+ (except F) when bonding to high electronegative elements - Hydrogen halides: gaseous hydrogen halides soluble in water (hydrohalic acids) - Ionic halides: React with metals to form (NaCl) - F always has oxidation state of -1 in compounds (can only make one bond)
38
Group 18
Noble Gases (inert gases) Nonreactive and very stable Noble gases are normally found in nature as isolated atoms Gases at room temperature
39
Common Diatomic Molecules
Hydrogen, Oxygen, Nitrogen, and Halogens Safe to assume these are in diatomic form unless otherwise stated Statement “Nitrogen is nonreactive” refers to N2
40
Four periodic trends
1: atomic radius- increases going down and to left 2: ionization energy- increases going up and to the right 3: electronegativity- increases going up and to the right 4: electron affinity- increases going up and to the right
41
Atomic radius
Distance from center of nucleus to outermost electron Corresponds to size of atom Radius decreases across period, each subsequent element has additional proton which pulls more strongly on surrounding electrons Moving down, more shells are added, outer electrons are shielded from attraction of protons, so atomic radius decreases going down group
42
Electrostatic force
Force between charged objects | Attractive between opposite charges, repulsive between like charges
43
Coulomb’s law
F = k q1 q2 / r^2 F: electrostatic force, q1 and q2, two charges of particles considered, r: distance between two objects Negative means an attractive force When calculating for an electron, should use Z_eff and not Z
44
Effective nuclear charge
Z_eff Amount of charge felt by most recently added electron Perfect Shielding: each electron added to atom would be completed shielded from attractive force of all protons in nucleus except for the last proton added, Z_eff would be 1eV for each electron then Without shielding, Z_eff would equal Z for each electron
45
How does Z_eff change in periodic table?
Generally increases going left to right and top to bottom Although energy level of outermost electrons increases down a group, attractive pull of growing positively charged nucleus outweighs additional shielding effects of higher electron shells Drops from Neon to Sodium because new shell and only one more proton added to outweigh shielding
46
How can we understand atomic radius trend using Z_eff?
Effective nuclear charge increases from left to right on periodic table, so each additional electron is pulled more strongly toward nuclease Result is that atoms tend to get smaller when adding electrons across the periodic table When moving down a group, each drop represents addition of new electron shell, so atoms tend to increase in size moving down a group even though Z_eff increases
47
Isoelectric Ions
Ions with the same number of electrons, but different elemental identities E.g. O2-, F-, neutral Ne, Na+, and Mg2+ all have same number of electrons Electrons feel different Z_eff with diff. # protons Largest is O2-, and smallest is Mg2+
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Ionization energy
Energy needed to detach an electron from an atom Generally increases from left to right and bottom to top First ionization energy: energy necessary to remove an e- from a neutral atom in its gaseous state (largest for noble gases) Second ionization energy: energy required to remove second e- from same atom to form +2 cation (always greater than first bc Z_eff increases after 1 e- is removed) Remember that as move to right, Z_eff increases, so pulling e- away is harder, however down a trend, distance is more important
49
Electronegativity
Tendency of atom to attract electrons shared in a covalent bond When two atoms have diff. Electronegativities, share e- unequally causing polarity Relative electronegativity determines direction of polarity w/in bond and w/in molecule Increases across period and up a group Pauling Scale: ranges from value of 0.79 for Cesium to 4.0 for fluorine
50
Which 3 E period trends increase going to the right and up?
Energy of Ionization, Electron Affinity, and Electronegativity
51
What is the electronegativity of a Noble Gas?
Undefined, they tend not to make bonds | Electronegativity provides useful system for predicting which type of bond will form between two atoms
52
How can electronegativity be used to predict bond type?
Difference of >= 1.6 on Pauling scale form ionic bonds (metals and non-metals) Moderate differences between 0.5-1.5 on Pauling scale form polar covalent bonds Small differences (<= 0.4) form nonpolar covalent bonds
53
Electron Affinity
Willingness of atom to accept an additional electron Energy released when electron is added to an isolated atom Tends to increase from left to right and bottom to top, more exothermic Sign can be diff.- Some require energy to receive e- and some release energy Electron affinity for noble gases, however, is endothermic, bc they are stable
54
Quantum Mechanics
Elementary particles can only gain or lose energy in discrete units Each energy unit is very small, and is only significant when dealing with elementary particles
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Bohr Atom
Represents the atom as a nucleus surrounded by electrons in discrete electron shells Proposed by Niels Bohr Orbital structure of H atom: single e- orbits H nucleus in electron shell
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Four quantum numbers
N, l, m_l, and m_s Principal quantum number: n, designates the shell level of e- Azimuthal quantum number: l, designates e-‘s subshell with a distinct shape Magnetic quantum number: m_l, designates precise orbital within subshell which holds a max of 2 e- Electron spin quantum number: m_s, -1/2 or +1/2 denotes the spin of the e- in the same orbital
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Pauli Exclusion Principle
No two electrons in same atom can have same four quantum numbers
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Principal Quantum Number
Designates shell level of electron Symbol: n Value: 1, 2, 3, ...
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Azimuthal Quantum Number
Designates the electron’s subshell, each with a distinct shape, 2nd number Subshells include s (spherical), p (dumbbell-shaped), d, or f Symbol: l Values: 0 (s), 1 (p), ..., n-1
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Magnetic Quantum Number
3rd Quantum number Designates precise orbital within a given subshell, 3D orientation Each orbital holds two electrons Symbol: m_l Values: -l to +l So s subshell is 0, p subshell is -1, 0, or 1
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Electron Spin Quantum Number
Fourth quantum number Designates the spin value of an electron in the exact orbital and subshell Symbol: m_s Values: -1/2 or +1/2
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Heisenberg Uncertainty Principle
There is an inherent uncertainty in the product of the position of a particle and its momentum Uncertainty arises from dual nature (wave-particle) of matter On order of Planck’s constant (6.6 x 10^-34 Js = h) \delta x \delta p >= h/2
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Aufbau principle
“Building up principle” States that with each new proton added to create a new element, new electron that is added to maintain neutrality will occupy the lowest energy level available Lower energy state of system, more stable the system
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How can you tell the shell level of the most recently added electron?
Representative elements: shell level is given by period Transition elements: Shell of most recently added electron lags one behind the period Lanthanides and Actinides: shell of most recently added e- lags two behind period
65
Orbital shapes
Subshells of s, p, d, and f are orbital shapes Not true paths that electrons follow, but rather represent probability functions for position of e- 90% chance of finding e- inside given shape
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Why are electrons in higher shells at a higher energy level?
Because force is attractive between the proton and electron, work is required to separate them Force must be applied over a distance Work is transfer of energy into or out of system (electron and nucleus) Energy being added to the system by adding e-, increased electrostatic potential eenergy
67
Electron Conifguration
Lists the shells and subshells of an element’s e-‘s from lowest to highest energy level Do not have to be written from lowest to highest energy subshells, but usually are E.g. Na: 1s^2, 2s^2, 2p^6, 3s^1 Fe: 1s^2, 2s^2, 2p^6, 3s^2, 3p^6, 4s^2, 3d^6
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What is different about ions formed by transition metals?
Ions are formed by losing electrons from the subshell with the highest principal quantum number first Generally this is the s subshell Few exceptions to configurations: Group 6 and 11 have nearly half-filled d subshells Borrow one e- from highest s subshell so they und with two half-filled subshell Most likely appears with Cr and Cu Cr: [Ar] 4s^1 3d^5, Cu: [Ar] 4s^1 3d^10
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Hund’s Rule
Electrons will not fill any orbital in the same subshell until all orbitals in that subshell contain at least one electron and that the unpaired electrons will have parallel spins
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Paramagnetic Elements
Elements with unpaired electrons A subshell is not completely filled (e.g. Li) Spin of each unpaired electron is parallel to the others Electrons will align with external magnetic field
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Diamagnetic Elements
Elements with no unpaired electrons (e.g. He), so subshells are completely filled Unresponsive to external magnetic field
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Emission line Spectrum
Energy emitted when excited electrons of an element fall to lower energy state Characteristic of a given element
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Absorption Line Spectrum
Radiation absorbed when electrons absorb energy to move to a higher energy state Characteristic of a particular element
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How did Max Planck explain absorption and emission spectra?
Electromagnetic energy is quantized and comes only in discrete units related to wave frequency Energy can only change in discrete increments given by: \delta E = h f H is Planck’s constant Energy of a single photon is given by same equation (according to Einstein) Electrons can only jump or fall to specific energy levels in atom
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Photoelectric Effect
(Einstein) Light is made up of particles called photons Shining light on metal emits photoelectrons corresponding to intensity and frequency of light If frequency of light shining on metal is less than necessary quanta of energy, no electrons will be emitted Intensity above required frequency increases number of emitted photoelectrons, but not KE Electrons must be ejected by one-to-one photon to electron collisions rather than by combined energies of two or more photons Minimum energy required to eject e- is work function, Phi KE = hf - Phi
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Covalent Bonds
Nuclei share a pair of electrons, forms a molecule Known as intramolecular bonds (bonds within molecules) Formed only between nonmetal elements, predominant in organic chemistry Attractive and repulsive forces balance each other
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Bond length
Distance between nuclei of two atoms in a bond when they are at their lowest possible energy state If atoms are separated by an infinite distance, forces between them and so energy of bond goes to zero Atoms closer than bond length (internuclear distance) have a great spike in energy Energy necessary for complete separation of bond is given by vertical distance on graph between energy at bond length and zero (internuclear distance v potential energy)
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Bond Dissociation Energy
Bond energy Energy necessary for complete separation of bond Can be seen by plotting potential energy and internuclear distance for two atoms Vertical distance on graph between lowest stable energy and x axis
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Partial Ionic Character
Difference in electronegativity between two atoms in bond is significant, but not large enough to be ionic (polar covalent)
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Ionic Bonds
Electronegativities differ vastly between two atoms in a bond Electron was actually transferred to other atom and oppositely charged ions are held together by electrostatic forces Ionic compound, separate distinct unit cannot be separated Lattice structure within a compound
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Intermolecular Forces
Molecules interact with each other through intermolecular forces Much weaker than intramolecular forces of bonds, similarly influenced by charge and electronegativity
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Dipole Moment
Center of positive charge in bond does not coincide with center of negative charge, partial positive / partial negative character Analogous to center of mass Vector pointing from center of positive charge to center of negative charge Measured in units of debye, D, given by equation: /mu = q d Where q is magnitude of charge, d is distance between centers of charge
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Polar Bond
Bond that has a dipole moment is polar, but molecule with polar bonds may not have net dipole moment, and therefore may not be polar (symmetry) Bond without dipole moment is nonpolar
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Intermolecular Attractions
Attractions between separate molecules occur due to dipole moments Weak electrostatic bonds, about 1% as strong as covalent bonds Attraction roughly proportional to their dipole moments; stronger the dipole, stronger the attraction
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Hydrogen Bond
Strongest type of dipole-dipole interaction Occurs between hydrogen covalently bonded to fluorine, oxygen, or nitrogen (highly electronegative) and a fluorine, oxygen, or nitrogen from another molecule Large dipole moments cause positive H to attract to negative electronegative elements Responsible for high boiling point of water Still much weaker than covalent bond
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Induced Dipole
Dipole moment is momentarily induced in otherwise nonpolar molecule or bond by polar molecule, ion, or electric field Partial or full charge of polar molecule or ion attracts or repels electrons of nonpolar molecule, separating centers of positive and negative charge Weaker than permanent dipoles
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Instantaneous Dipole
Can arise spontaneously in an otherwise nonpolar molecule Occur due to movement of electrons and at any given moment may not be distributed exactly between two bonding atoms Can create induced dipole in neighboring molecule Weakest and short-lived Known as London dispersion forces or Van der Waals’ forces All molecules exhibit London dispersion forces
88
Do molecular crystals and ice experience intermolecular forces?
Yes, all dipole and intermolecular forces apply, especially when atoms are in such close contact Generally insignificant in gases because molecules are spread far apart
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Naming of Ionic Compounds
Named after cation or anion Transition metals with different oxidative states: roman numeral Copper(I): Cu+1, Copper(II): Cu+2 or cuprous and cupric, respectively Nonmetal: cation ends in -ium, NH4+ is ammonium Monatomic anions and simple polyatomic have suffix ‘ide’, Hydride for H- Polyatomic anions w/ multiple Oxygens have suffix ‘ite’ or ‘ate’ relative # O’s Nitrite: NO2-, Nitrate: NO3- Hypo and per used for more O’s, hypo-ite, ite, ate, per-ate Oxyanions with hydrogen have hydrogen in front For compounds: Put cation in front of anion and for two atoms begin with element to left down and for second element add suffix ‘ide’, Number prefix used for element with more than one atom, dinitrogen tetroxide (N2O4)
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Naming Acids / Bases
Named for anions If anion ends in ‘ide’, acid name starts with ‘hydro’ and ends in ‘ic’, e.g. hydrosulfuric acid (H2S) For oxyacid: ending ‘ic’ used for multiple O’s, ‘ous’ for fewer O’s, e.g. sulfuric acid H2SO4 and sulfurous acid H2SO3
91
What are the seven base SI units you should know?
``` Mass: Kilogram (Kg) Length: Meter (m) Time: Second (s) Electric current: Ampere (A) Temperature: Kelvin (K) Luminous intensity: Candela (cd) Amount of substance: Mole (mol) ```
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What is the derived units for the Newton?
1 N = 1 kg m / s^2
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Compound
Substance made from two or more elements in fixed proportions
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Empirical Formula
Smallest ratio of whole numbers that can be used to represent proportions of elements in a compound Ionic compounds are represented by empirical formula
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Molecular Formula
Commonly used for molecular compounds, represents the exact number of elemental atoms in each molecule Glucose: C6H12O6 is molecular formula, CH2O is empirical formula
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Percent Composition by Mass
Multiple an element’s atomic weight by number of atoms it contributes to empirical formula and divide by total weight of all atoms yields mass fraction of that element in the compound (multiple by 100% to get percentage)
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Physical Reactions
Reactions of compounds that maintain their molecular structure (and identity) Examples are melting, evaporation, dissolution, rotating of polarized light
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Chemical Reaction
Compound undergoes a reaction and changes its bonding or structure to form a new compound Examples are combustion, metathesis, and redox reactions
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Combination (Synthesis) Reaction
A + B -> C | E.g. Fe(s) + S(s) -> FeS(s)
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Decomposition Reaction
C -> A + B | E.g. 2Ag2O(s) -> 4Ag(s) + O2(g)
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Single Displacement Reaction
A + BC -> B + AC | Mg(s) + 2HCl(aq) -> MgCl2(aq) + H2(g)
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Double Displacement Reaction
AB + CD -> AD + CB E.g. HCl(aq) + NaOH(aq) -> NaCl(aq) + H2O(l) Often occur between ionized salts dissolved in water Helpful to know the charges of common ions to predict new compound’s molecular formula Ions will often combine to form a new compound with net charge of 0
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Redox Reaction
E.g. 2Au3+ 3Zn -> 2Au + 3Zn2+ | Transfer of electrons, oxidation or reduction
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Combustion Reaction
E.g. C6H12 + 9O2 -> 6CO2 + 6H2O | Usually involves input heat (burning)
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Bronsted-Lowry acid-base
HI + ROH -> I- + ROH2+
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Lewis acid-base
Ni2+ + 6NH3 -> Ni(NH3)6 2+
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What does the delta symbol above reaction arrows indicate?
Heat was added
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Theoretical Yield
Amount of product that should be created when a reaction runs to completion, based on stoichiometry Amount of product created by real experiment is actual yield Percent Yield = 100 x (Actual yield / Theoretical yield)
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Stoichiometry
Determining quantities of products and reactants in chemical equation Use grams, amu, moles
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Mole
6.011 x 10^23 of something This is Avogadro’s number 12^C serves as standard for this, Avogadro’s number is equal to the number of Carbon atoms in 12 grams of 12^C 6.022 x 10^23 amu = 1 gram Moles = grams / atomic or molecular weight
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Radioactive decay
Process in which atoms spontaneously break apart All atoms other than hydrogen are subject to some type of spontaneous decay Atoms with relatively high decay are said to be radioactive, rate at which decay occurs varies dramatically Atomic nuclei are held together by strong nuclear force, without which they would repel one another
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Half-life
Length of time necessary for one half of a given amount of a substance to decay Radioactive decay follows first order kinetics Amount of atoms that remain after decay can be expressed as follows: At = A0 e^(-kt) OR ln(At/A0) = -kt At is amount at time t, A0 is original amount, k is rate constant, t is time
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Exponential Decay
The relationship governing radioactive decay are described in terms of an exponential relationship Plotting logarithm of amount of atoms as a function of time would produce a straight line semi-log plot
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Three types of radioactive decay on MCAT
Alpha decay, Beta decay, and gamma decay | Positron emission and electron capture are both types of beta decay
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Alpha Decay
Loss of an alpha particle Alpha particle is a helium nucleus (contains 2 protons and 2 neutrons) E.g. {238}^ {92}_ U -> {4}^ {2}_alpha + {234}^ {90}_ Th
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Beta Decay
Breakdown of a neutron into a proton and electron, and expulsion of newly created electron Since a neutron is destroyed, but a proton is created, mass number stays the same, but atomic number increases by one E.g. {234}^ {90}_Th -> {234}^ {91}_ Pa + {0}^ {-1}_ e + neutrino Neutrino is virtually massless particle, typically represented by greek letter nu (v)
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Positron Emission
Emission of a positron when a proton becomes a neutron Type of beta decay Positron can be thought of as electron with positive charge, where both electrons and positrons are considered beta particles E.g. {22}^ {11}_ Na -> {0}^ {1}_ e + {22}^ {10}_ Ne + neutrino
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Electron Capture
Capture of electron and merging of electron with proton to create a neutron Proton destroyed and a neutron created E.g. {201}^ {80}_ Hg + {0}^ {-1}_ e -> {201}^ {79}_ Au + {0}^ {0}_ gamma Where gamma is gamma ray
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Gamma ray
High frequency photon | Has no mass or charge, does not change identity of atom from which it is given off
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Gamma decay
AKA gamma ray emission Often accompanies other types of radioactive decay Can occur when an electron and positron collide: {0}^ {-1}_ e + {0}^ {1}_ e -> {0}^ {0}_ gamma + {0}^ {0}_ gamma Matter-antimatter collision called annihilation where mass is destroyed and converted to energy in the form of gamma rays