Describe scientific method
Apply the COAST approach to problem solving
Collect and Organize
Identify key concepts and skills required to solve a problem; assemble the information needed.
Analyze
Evaluate information and relationships or connections; sometimes units will help identify steps needed to solve the problem.
Solve
Perform calculations, check units, etc.
Think About It
Is the answer reasonable? Are the units correct?
Distinguish between the classes of matter between the physical and chemical properties of pure substances
Physical Properties:
Intensive property:
independent of amount of substance
Example: color, melting point, density
Extensive property:
dependent with quantity of substance present
Example: volume, mass
Chemical Property:
property of substance only observed by reacting it with another substance
Example: H2 and O2 reacting to create compound water
States of Matter
Pure substance or mixture
Law of conservation
states that energy cannot be created nor destroyed, but it can be converted from one form to another
Prefixes
Tera = 12
Giga = 9
Mega = 6
Kilo = 3
Hecto = 2
Deka = 1
Deci = -1
Centi = -2
Mili = -3
Micro = -6
Nano = -9
Pica = -12
Convert C to K
K = C + 273.15
Sig Figs
34.023 = 5
0.068 = 2
0.0680 = 3
*zeros at the end of the number with a decimal point are significant
110 = 2
= 3
1.234 x 10^-5 = 4
1.234 x 10^5 = 4
1.2340 x 10^5 = 5
Precision in Calculation
When adding or subtracting
least precise determines the answer
When multiplying or dividing
Precision is based on experimental values
Quantum theory
Energy = hv
energy = proton energy
h = plancks contant 6.626 X 10 -34 J
v = frequncy
Quantized States
Quantized states: Discrete energy levels (e.g., steps)
Unquantized states: smooth transition between levels (e.g., ramp)
Black Body Radiation
Objects heated > emits radiation
Key Idea: Wavelength distribution of the radiation depends on temperature
Planck introduced concept that energy is released or absorbed in discrete “chunks”
Quantization of energy required for theory to match
E = hv
E= energy
V = frequency
h= Planck’s constant
the key overall point is energy is emitted or absorbed in chunks and that is related to temperature
Line Spectrum
Dark lines = Bright lines
Emitted light (bright line) at the same “energy” as absorbed light (dark line)
SO… there must be certain characteristic energy states in a gas that are reversible (can take in or give off energy)
Atomic Emission Spectra
bright line emission spectra are unique for different elements and therefore a key way to identify unknown elements
more complex the elements the more lines
The Photoelectric Effect
Key Idea: When a photon hits a metal surface it ejects an electron
*einstein
Experimental Observations:
No electrons are ejected unless the light exceeds a threshold frequency ( if not enough or below freq then no ejection of electrons)
The kinetic energy of the electrons increases linearly with the frequency of the light
But the kinetic energy of the electrons is independent of the light intensity
Even at a low light intensity, electrons are ejected immediately
Experimental Results: If you triple the number of photons then it triples the electrons
-higher freq of light increases then velcity increaese
Photoelectric Effect Overall
Observation
Electons are emitted by metal only if light has frequnwcy greater than certain minimum value, no mater how intese the light
When electons are emitted, the number emitted is proportional to tlight intenisty