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Types of units
English/Imperial, metric, SI
SI units
Prefixes used in
SI system
Temperature
K=°C +273
SI derived Unit
a unit derived by combining SI base units that shows up often
1 dm^3=
1 cm^3=
1 L
1 mL
Density
- mass/volume
- physical and intensive property
- can be used to identify pure substances
- can be used as a conversion factor
particles
atoms, ions, molecules
Energy
the capacity to do work
E = force distance = kgm^2*s^-2
Work (W)
change in energy thatresults when a Force (F) is exerted over a distance (d)
W= F×d
Kinetic Energy (Ek)
energy due to motion
Potential Energy (V)
energy due to position in a force field
Radiant Energy (E photon)
energy due to radiation
E total
Ek + V + Ephoton
According to the law of conservation of energy E Total is
0
What is energy measured in?
Joules (J)
15=1 kg×m^2×s^-2
calories (cal)
1 cal=4.184J
kilowatt-hour(kWh)
1 kWh=3.60×10^6 J
electron Volts (eV)
1 eV= 1.6022×10^-19 J
What is force measured in?
Newtons [N]
1N= 1 kg×m×s^-2
Force formula
F= m×a
Pressure formula
p= F/I^2
Accuracy
how close a measurement is to the true value
Precision
a measure of how close a series of measurements are to one another
Exact numbers
have an infinite number of significant figures
Inexact Numbers
those whose values have some uncertainty
sig figs in multiplication and division
least number of sig figs
sig figs in addition and subtraction
least number of decimal places
Dimensional Analysis
a mathematical technique that allows you to use units to solve problems involving measurements
Chemistry definition
the study of matter, the changes it undergoes, and the energy associated with these changes
matter
Anything that has mass and takes up space
atoms
smallest unit of matter
Physical State
- solid, liquid, or gas
- based on the strength of interactions that occur between particles making up the substance at a given temperature
- stronger interaction = less space and vice versa
composition
pure substance or mixture
pure Substance
A form of matter that has definite (constant) composition and distinct properties
- includes elements (one type of atom) and compounds (more than I type of atom)
mixture
A combination of two or more substances that are not chemically combined
Allotropes
Different forms of the same element
Isomer
Compounds with the same formula but different structures.
Mixture types
homogenous (mixture has components that are uniform throughout & are also called solutions)
heterogenous (mixture is not
uniform throughout, as the
components are discernible by
the naked eye)
Quantitative
measured and expressed with a number
Qualitative
Do not require measurement and are usually based on Observation
Extensive
Depends on the amount of matter
Ex: mass, volume
Intensive
Does not depend on the amount of matter
Ex: temperature and density
Physical Property
can be observed and measured without changing the identity of the substance
Chemical Property
Cannot be observed without converting a substance into another substance
Law at Conservation of Mass
- Matter is not created nor destroyed in any chemical or physical change
- 1789, Antoine Lavoisier
Law of Definite Proportions
All samples of a given compound, regardless of their source or how they were prepared, have the same proportions of their constituent elements
- 1797, Joseph Proust
- Ex: water's O to H ratio is 8:1, so all samples of pure H2O must have O:H mass samples be 8:1
- elements in compounds should be in fixed and discrete amounts
Law of Multiple Proportions
when 2 elements form a different compounds, the masses of element B that combine with 1g of element A can be expressed as a ratio of small WHOLE numbers
- 1804, John Dalton
- Ex: carbon monoxide and carbon dioxide both are made up of only carbon and oxygen, but their C:O ratios differ from each other
velocity
distance/time
conversion factor
- ratio
- units on the top of the fraction are different from the units on the bottom of the fraction
- the top of the fraction is "equal" to the bottom
- created from an equality statement
John Dalton's Atomic Theory(1808)
1. Each element is composed of tiny, indestructible particles called atoms
2. All atoms of a given element have the same mass and other properties that distinguish them from atoms of other elements
3. Atoms combine in simple, whole-number ratios to form compounds
4. Atoms of one element can't change into atoms of another element. In a chemical reaction, atoms only change the way that they are bound together with other atoms
J.J. Thompson's Cathode Ray Experiment
- cathode rays are composed of negatively charged particles that travel in straight lines
- atoms are divisible and the electron was discovered
Robert Millikan's Oil Drop Experiment
- charges on oil drops are whole-number multiples of the charge of a single electron
- the charge of an electron was determined
- the charge of a single electron was calculated to be -1.60 * 10^19 Coulomb (C)
Ernest Rutherford's gold foil experiment
the discovery of the nucleus and the disproving of the plum-pudding model of an atom
Thompson's Plum Pudding Model
electrons held within a positive nucleus/charged sphere
Rutherford's Nuclear Theory of an Atom
- most of the atom's mass and all of its positive charge are contained in a small core called the nucleus
- most of the volume of the atom is empty space dispersed with tiny, negatively charged electrons
- there are positively charged particles called protons in the nucleus. The number of protons in the nucleus must equal the number of electrons so that the atom is electrically neutral
James Chadwick
the nucleus also contains uncharged particles called neutrons. The mass of a neutron is similar to the mass of a proton
atomic mass unit(amu or u)
- unit of mass well suited for dealing with individual protons, neutrons, atoms, molecules, etc.
- avg atomic mass: f = natural abundance and m=mass;
- Average Mass(element) = fi(mi) + fi(mi)
Z(atomic number)
identity of an element determined by the number of protons
Atoms of an element must have the ______ amount of protons and ___________ amount of neutrons
same, different
ions
- they are not the same as atoms
- formed by a loss or gain of electrons to make cations(positive) and anions(negative)
isotopes
Atoms of the same element that have different numbers of neutrons, therefore having slightly different masses for each of the isotopes
mass number(A)
number of protons + number of neutrons
natural abundance
relative amount of an isotope in a naturally occurring sample of an element that is usually given in percentages
Mole(mol)
- unit of amount
- 1 mol = 6.022 * 10^23 entities
- that number above is Avogadro's number (NA)
Molar Mass (M)
- mass substance(g)/amount substance(mol)
- g/mol
- numerically equal to the atomic mass of the substance, but atomic mass units are amu/atom and molar mass is g/mol so don't mess it up
wave-particle duality of light
Sometimes light appears to behave like a wave, at other times like a particle depending on the specific scenario
wave nature of light
- the two-slit interference pattern can only be explained by a wave picture of light
Important characteristics:
- wavelength
- frequency
- amplitude
- energy
- speed
Wavelength
The distance between two corresponding parts of a wave
- measured in length units: nm, m, micrometers, mm
Frequency
the number of complete wave cycles that pass a point in a given time
- measure in cycles/s, s^-1, or Hz
- inversely proportional to wavelength
amplitude
the height of a wave's crest
- determines light intensity
Energy of a wave particle
- proportional to its amplitude and frequency
- greater energy means greater frequency and smaller wavelength
- lower energy means lower frequency and bigger wavelength
speed of light(c)
c=λ*v, c=3.00E8
- measured in m/s
order of Electromagnetic radiation energy
(least to greatest) radio waves, microwave, infrared, visible light, ultraviolet, x-ray, gamma ray
interference
separate light waves can interact by overlapping and either building up(constructive interference) or cancelling each other out(destructive interference)
diffraction
bending of light around an obstacle
Photoelectric effect
The emission of electrons from a metal when light shines on the metal
- Einstein's explanation: E photon = W + Ek
or hv = hv0 + 1/2mu^2
important observations of the photoelectric effect
- for a given metal, there is a minimum frequency(v0) of light needed for the photoelectric effect to occur; think of this as a threshold
- if the light is below the threshold frequency, increasing the light intensity or duration of irradiation has NO EFFECT, so electrons are still not ejected from the metal surface
- once the threshold frequency is met/exceeded, increasing the intensity will cause more photoelectrons to be emitted by the metal surface
- increasing the frequency past the threshold frequency increases the velocity of the ejected electrons, making them fast when they are emitted off the metal surface
- not explained by wave nature of light
How can the photoelectric effect be explained?
- Einstein(1905) explained that the photoelectric effect by treating light as being made up of packets of energy; light is quantized
the energy of the photon must be enough to overcome ________________________
the binding energy/ threshold energy/ work function of an electron or metal
- individual photons from the light source need to be absorbed by individual electrons to eject them
Energy of a photon equations
E = hv
E = hc/λ
v is frequency
Planck's constant(h)
h = 6.626 x 10^-34 J x s
Kinetic energy formula
KE = 1/2 x mass x velocity^2
relating kinetic energy to binding energy through the energy of a photon equation:
hv= hc/lambda = h(v0) + 1/2(mv^2)
electron-volt (eV)
1 eV = 1.60 x 10^-19 J
when atoms or molecules absorb energy, such as heat, light, and electricity, the energy is usually re-emitted as light
Ex: heating a metal until it glows, neon size, fireworks, etc.
- can be explained by the particle nature of light
What is an emission spectra?
- light emitted byy excited atoms can be separated by a prism into the different wavelengths present(pattern[emission spectrum] can be used to identify the atom/molecule)
- different sources of light emit different types of spectra
Rydberg Equation
1/wavelength = R (1/n1^2 - 1/n2^2)
Bohr Model of the (Hydrogen) Atom
- Niels Bohr expanded upon Rutherford's model of the atom to explain why hydrogen emits the specific line of spectra that it does
energy of electron in energy level, n
En = -2.179*10^-18J (1/n^2)
the energy difference between two energy levels (delta E)
Efinal - Einitial
- E photon = delta E = hv = hc/lambda
When delta E is positive
photon/energy is absorbed and electron went from a low energy level to a high energy level
When delta E is negative
photon/energy is released and electron went from a high energy level to a low energy level
Wave nature of matter
- Louis de broglie
- showed relation between mass and wavelength
- said matter should have wave properties
- lambda = h/mv
h = 6.626*10^-34 Js
m = mass of particle in kg
v = speed of the particle in m/s
1927 Double Slit Experiment performed using a beam of electrons
- interference pattern was formed
- conclusion: particles have wave properties and have a wave-particle duality just like light, so you can think of electrons using both a wave and particle image
Heisenberg uncertainty principle
- it is impossible to know exactly both the velocity and the position of a particle at the same time
- you can't observe both wave and particle properties of an electron at the same time
atomic orbitals
- the regions around the nucleus within which the electrons have the highest probability of being found
- described by 3 quantum numbers that designate energy, size, shape and orientation in space of the orbital
principal quantum number(n)
- indicates the relative size and energy of atomic orbitals
- possible values include n = 1, 2, 3... where n is a positive whole number
- the higher the value of n, the further away from the nucleus the electrons are and the higher the energy of the electrons in the energy level
angular momentum quantum number(l)
l = integer values and zero ranging from 0 to n-1
- designates a specific subshell within the principal energy level(n) and designates the shape of the orbitals within the subshell
magnetic quantum number (m sub l)
- an integer that specifies the orientation of an orbital
- possible values: positive and negative whole numbers and zero that range from -l to 0 to +l
magnetic spin number (m sub s)
only two possible values: +1/2 or -1/2
- designates the spin of electrons in the orbital(up or down/clockwise/counter-clockwise)
s orbitals
l = 0, m sub l = 0
- only one 3-D orientation in space
p orbital
l = 1, m sub l = +1, 0, -1
- 3 orientations in space
- lobes align parallel to an x-,y- or z-axis
- 2 lobes = 1 orbital