ap chem final study guide

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206 Terms

1

Lavoisier, Law of Conservation of Matter

in a chemical reaction, matter is neither created nor destroyed

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2

proust, law of constant composition

each pure chemical compound always has the same percentage composition of each element by mass

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3

atomic theory, 4 principles

- each element and all matter is composed of atoms
- atoms are identical to one another in mass, and unique against all other elements
- atoms of one element can't be changed into atoms of another element
- chemical reactions are just rearrangements of actions (different combos!)

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4

law of multiple proportions

if two or more different compounds are composed of the same two elements, then the ratio of the masses of the second element combined with a certain mass of the first element is always a ratio of small whole numbers

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5

cathode ray tube

Electrodes were stimulated to give off radiation -> these rays were consistent regardless of the cathode itself, and determined to be negatively charged; thus, the rays were concluded to be streams of negatively charged particles, aka electrons.

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6

electron's charge to mass ratio

- (1.76 x 10^8 coulombs) per gram

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7

millikan oil drop experiment

dropped oil drops which lost electrons as falling => gravity acted as downwards force, but the bottom plate repelled electron force; by determining when repulsion and gravity balanced, millikan discovers force and mass of an electron by applying charge to mass ratio

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8

charge of an electron

Charge of an Electron: -1.6 * 10^-19 Coulombs

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9

mass of an electron

9.11 * 10^-28 grams

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10

alpha radiation

fast moving particles with a positive charge

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11

beta radiation

fast moving high speed electrons with a negative charge

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12

gamma radiation

high energy radiation without particles of charge

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13

plum pudding model

electrons bathed like chocolate chips in a sea of positive charge

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14

gold foil experiment

shone alpha particles at a gold foil => deflection and bounceback proved the existence of a dense positive center (nucleus!)

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15

properties of a proton

Discovered by Rutherford, 1919

basic unit of positive charge

Magnitude: +1.6 * 10^-19 Coulombs

Mass of 1.67 * 10^-24 grams, 1836 times heavier than the electron

Relative Charge (+1)

Relative Mass in AMU: 1.0073

p

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16

neutrons

Magnitude: 0 Coulombs

Mass of 1.67 * 10^-24 grams, same as proton

Relative Charge 0

Relative Mass in AMU: 1.0087

n

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17

electrons

Magnitude: -1.6 * 10^-19 Coulombs

Mass of 9.109 * 10^-28 grams

Relative Charge (-1
)
Relative Mass in AMU: 5.486 * 10^-4
p

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18

line spectra

colors consist of discrete wavelengths of light, each element is unique!

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19

wave nature of light

all waves move thru a vacuum at the speed of light (3 x 10^ m/s)
- behave like sin/cosine functions; its periodic

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20

wavelength and frequency relationship

- inversely proportional; long wavelengths mean lower frequency n vice versa

wavelength x frequency = speed of light
WAVELENGTH NM VERSUS SPEED OF LIGHT M

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21

energy of light

energy is absorbed in quantum sizes

e = hv where v is the frequency.

h is planck's constant, 6.626 x 10^-34 joules per second

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22

strength of diff. wavelengths

longer wavelengths mean weaker, shorter means stronger; red is weakest, purple is strongest

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23

weakest to strongest wavelengths

radio, tv, microwave, infrared, uv, xray

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24

note for prefixes

nano = -9
micro = -6
milli = -3
yk the rest

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25

photoelectric effect

- when light hits a metal surface, the minimum amount of energy required to eject an electron differs
=> known as work function, the barrier to ejection

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26

postulates of the bohr model

- electrons can only circulate in orbits of specific radii
- in a permitted orbit, energy isn't released so electrons don't collapse into the nucleus
- energy is emitted or absorbed when electrons jump from one orbit to another

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27

ground vs excited state

ground state is when an electrion is in the lowest possible energy state, excited is when its in a higher energy state

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28

energies of specific orbits

always negative because if n is infinite, it has no attraction the nucleus, making the energy zero
- the closer/more stable it is, the more negative it is.

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29

principal energy levels

- big shells, hold max of n^2 orbitals and 2n^2 electrons
- starts at 1 starting from closest to the nucleus

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30

sublevels/subshells

number of subslevels possible is equal to the value of n
- there's an s sublevel, p sublevel, d sublevel, etc.

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31

orbitals

think of it more as subshell orientations
- s sublevel has 1 s orbital, p sublevel has 3 p orbitals, etc..

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32

quantum numbers

n = prinicpal quantum number

l = angular momentum number, represents sublevel starting from 0 to n-1
-- 0 is the s orbital, n so on

ml = orientations of a specific orbital (-l to l)
-- -1 represents the first p orbital, 0 the second, etc...

spin quantum number, either + or - 0.5
-- positive is counterclockwise, negative is clockwise

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33

pauli exclusion

no two electrons have the same 4 quantum numbers (you can't put a person in a person)

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34

heisenberg uncertaintiy

position and momentum can't be known at the same time; the more you know about one the less you know about the other

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35

hund's

electrons of the same energy go indiv. in each orbital before doubling up - like how u sit on the subway

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36

aufbau

sideways christmas tree

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37

exceptions to aufbau

- completely filled d for cu ag and au by unfilling s sublevel
- half filled d level for cr and mo is done by unfilling s sublevel

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38

reading periodic table

d block starts on thrid shell
f block starts on fourth shell

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39

spectroscopy

- microwave radiation represents molecular rotational disturbance
- infrared is molecular vibrational levels
- ultraviolet represent change in energy levels

electronic energy, vibration, and rotation << order from most energy to least energy required

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40

beer lambert

lower concentration = lower absorbance, IE DILUTION = LESS ABSORBANCE

- if fingerprints are left, they cause light to scatter, making the light measurer think there's less light passing thru the sample and greater absorbance!

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41

PERIOD VS GROUPS

PERIOD IS A ROW, GROUP IS A COLUMN

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42

what are isotopes

Atoms of the same element with different numbers of neutrons

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43

numbers of particles in atoms

- proton and electrons are always equal to the atomic number, but number of neutrons depend on the isotope mass minus the atomic number
-- i.e. uranium 235 has 143 (235 - 95) neutrons

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44

radioactive decay

- unstable nucleus emits small particles to achieve stability
- emits electrons, neutrons, helium nucleus n positrons
- changes nuclear mass and charge!
- released in the form of xrays/gamma rays

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45

mass spectrometry

molar mass is weighted avg of masses of all naturally occuring isotopes

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46

groups of periodic table

- alkali metals, alkaline earth metals, transition metals, halogens, n noble gases respectively from left to right

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47

elements liquid at STP

mercury and bromine

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48

gases at STP

all noble gases

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49

diatomic molecules

H, N, O, F, Cl, Br, I

BRINCLHOF

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50

Polyatomic elements

sulfur and phosphorus

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51

allotropes

elemet that has two or more distinct sets of chemical n phsyical properties like ozone and oxygen

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52

effective nuclear charge

- core electrons shield valence electrons from getting full nuclear charge

effective charge = nuclear charge - screening constant, abides by coulomb's

trend: increases left to right, top to bottom

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53

coulomb's

charge increases as nuclear charge increases n distance decreases

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54

ionization energy

energy needed to remove an electron

trends = increases bottom to top, left to right

EXCEPT
- beryllium higher than boron because you're removing from full subshell
- same thing with nitrogen n oxygen

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55

atomic radii

van der waals - shortest distance separating two nuclei during a colission is twice the radii of the atoms

trend: increases top to bottom, right to left

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56

electron affinity

how much an atom wants an electron
- halogen has the most negative affinities meaning they WANT electrons
- noble gases have the most positive = DONT want electrons
- doesn't change much moving down a group

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57

electronegativity

how much an atom can pull shared electrons toward itself, diagonal rule!

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58

ionic radii

cations always smaller than neutral atoms of the same element, anions always larger due to increase in electrons and repulsion

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59

boiling points

decreases top to bottom for metals, but increases top to bottom for nonmetals

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60

PES

measures binding energy
- peak size proportional to number of electrons in a subshell
- electrons closer to core have higher energy, PAY ATTENTION TO THE AXIS.

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61

properties of metals

- shiny luster, malleable, ductile, good heat and electricity conductors
- metallic character increases top to bottom, right to left

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62

nonmetal properties

no luster, brittle, bad conductors of everything

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63

metalloids

if metals n nonmetals had a mixed child, good for semiconductors

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64

avogadro's

number of things in a mole => 6.02 * 10^23 particles/atoms/etc

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65

amu

grams/mole

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66

molecular vs empirical formula

actual number of compounds versus greatest common factor

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67

chemical bonds

attraction between nucleus of one atom and electron of another

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68

intramolecular - ionic

complete transfer of valence electrons
- en is greater than 2.0

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69

intramolecular - covalent

similar electronegativites
- nonpolar covalent when less than 0.5, very equal sharing
- polar covalent when between 0.5 and 2; slightly more unequal sharing

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70

intramolecular - metallic

when electrons free to move throughout a metallic lattice; attraction is the attraction between mobile electrons moving in a sea

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71

strongest to weakest intramolecular forces

metallic, ionic, polar covalent, nonpolar covalent

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72

intermolecular - dipdip

dipole-dipole; dipole of one molecule attractions to oppositely charged dipole of another; STRONGEST IMF

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73

intermolecular - hydrogen

H and NOF
- positive end of hydrogen attracts to oxygen, nitrogen, or fluroine

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74

london dispersion or van der waals

weakest forces, exist in all types of molcules
- momentarily induced dipole attraction due to uneven distribution

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75

strongest to weakest imfs

hydrogen, dipole dipole, london dispersion attraction

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76

boiling points by imfs

ionic compounds w ion to ion attraction, covalent compounds w hydrogen, polar covalent, and then nonpolar covalent

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77

potential energy curves

if less than 0, its stable, if greater than 0 its unstable, and if there's no attraction, its zero.

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78

bond energy

emergy required to break a bond, ENDOTHERMIC because you have to absorb energy

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79

bond length

distance btwn atoms

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80

single, double, triple bond

single is the weakest and longest, triple is strongest and shortest

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81

lattice energy

energy require dto separate ions in an ionic bond

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82

requirements for conductivity

charged particles that are MOBILE

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83

substitutional vs interstitial

substituional = similar sizing, changes properties a lil

interstitial = smaller fits inside interstices of bigger, strengthens.

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84

formal charge

valence electrons - number of assigned electrons

MINIMIZE for best lewis diagram

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85

VSEPR Theory

- negative electrons repel each other
- bonds n lone pairs arrange themselves as far as possible to minimize repulsion

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86

molecular versus electron geometry

- molecular geometry depends on number of lone pairs, electron just depends on total electron regions.

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87

BOND polarity

electrons shared equally only when its a covalent bond between two identical atoms

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88

free radicals

odd number of electrons

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89

bond order

number of bonds divided by number of atoms bonded to

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90

MOLECULAR polarity

- symmetrical means nonpolar
- nonsymmetrical are polar if the bonds are polar
- if central atom has more than one type of atom or nonbonding, its polar.

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91

valence bond theory

covalent bonds are overlapping orbitals,

= sigma bonds are single bonds, overlap of two s orbitals
- pi bonds are overlaps of p orbitals
- doule bonds are one sigma one pi
- triple bonds are one sigma two pi

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92

ELECTRON GEOMETRIES

two regions = linear
three regions = trigonal planar
four regions = tetrahedral
five regions = trigonal bipyramidal
six regions = octahedral

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93

molecular shapes n angles - for two electron regions

always linear, 180 degree

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94

molecular shapes n angles - for three electron regions

if there's no nonbonding, it's trigonal planar, 120
if there's one nonbonding, it's bent, 120

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95

molecular shapes n angles - for four electron regions

if there's no nonbonding, its tetrahedral, 109.5

one nonbonding = trigonal pyramidal, 107

two nonbonding = bent, 104.5

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96

molecular shapes - for five electron regions

no nonbonding = trigonal bypyramidal, 120 in plane and 90 in perpendicular to plane

one nonbonding is a seesaw, complex no one really knows ig

two nonbonding is a t, about 90

three nonbonding is linear, 180

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97

molecular shapes - for six electron regions

zero nonbonding is octahedral, 90

one nonbonding is square pyramidal, 90

two nonbonding is square planar, 90

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98

hybdrization (BY ELECTRON GEOMETRY)

sp for two regions, sp2 for three regions, sp3 for four regions, sp3d for five regions, sp3d2 for six regions

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99

polar geometries

3 regions
- bent

4 regions
- trigonal pyramidal
- bent

5 regions
- seesaw
- t

6 regions
- square pyramidal

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100

bond length pe graph

lowest point on graph represents length!

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