Atomic Structure
Classical Model
Democritus Dalton
Democritus
Circa 400 BC
Greek philosopher
Dalton’s Atomic Theory (1808)
1. All matter is made of tiny indivisible particles called atoms.
2. Atoms of the same element are identical. The atoms of any one element are different from those of any other element.
3. Atoms of different elements can combine with one another in simple whole number ratios to form compounds.
J.J. Thomson (1897)
Determined the charge to mass ratio for electrons
Applied electric and magnetic fields to cathode rays
Rutherford’s Gold Foil
Experiment (1910)
Alpha particles (positively charged
helium ions) from a radioactive source was directed toward a very thin gold foil.
A fluorescent screen was placed behind the Au foil to detect the scattering of
Rutherford’s Gold Foil
Experiment (Observations)
Most of the -particles passed through
the foil.
Many of the -particles deflected at
various angles.
Rutherford’s Gold Foil
Experiment (Conclusions)
Rutherford concluded that most of the mass of an atom is concentrated in a core, called the atomic nucleus.
Shortfalls of Rutherford’s
Model
Did not explain where the atom’s negatively charged electrons are located in the space surrounding its positively charged nucleus.
We know oppositely charged particles attract each other
Bohr Model (1913)
Niels Bohr (1885-1962), Danish scientist working with Rutherford
Proposed that electrons must have enough energy to keep them in
constant motion around the nucleus
Planetary Model
The planets are attracted to the sun by gravitational force, they move with
enough energy to remain in stable orbits around the sun.
Electrons have energy of motion that enables them to overcome the
Think about satellites….
We launch a satellite into space with enough energy to orbit the earth
The amount of energy it is given, determines how high it will orbit
Electronic Structure of Atom
Waves-particle duality Photoelectric effect
Planck’s constant Bohr model
Radiant Energy
Radiation the emission of energy in
various forms
A.K.A. Electromagnetic Radiation
Electromagnetic Radiation radiation that consists of wave-like electric and
magnetic fields in space, including light, microwaves, radio signals, and x-rays
Electromagnetic waves can travel
through empty space, at the speed of
Waves
Waves transfer energy from one place to another
Think about the damage done by waves during strong hurricanes.
Think about placing a tennis ball in your bath tub, if you create waves at one it, that energy is transferred to the ball at the other = bobbing
Wave Characteristics
Wavelength, (lambda) distance between
successive points
Wave Characteristics
Frequency, (nu) the number of
complete wave cycles to pass a given point per unit of time; Cycles per
second
Units for Frequency
1/s s-1
hertz, Hz
Because all electromagnetic waves travel at the speed of light, wavelength is determined by frequency
Waves
Waves
Electromagnetic Spectrum
Radio & TV, microwaves, UV, infrared, visible light = all are examples of
electromagnetic radiation (and radiant energy)
Electromagnetic Spectrum
1024 1020 1018 1016 1014 1012 1010 108 106
Gamma Xrays UV Microwaves FM AM IR
Frequency Hz
Notes
Higher-frequency electromagnetic
waves have higher energy than lower-frequency electromagnetic waves
All forms of electromagnetic energy
interact with matter, and the ability of these different waves to penetrate
What is your favorite radio
station?
Radio stations are identified by their frequency in MHz.
We know all electromagnetic
radiation(which includes radio waves) travel at the speed of light.
Velocity of a Wave
Velocity of a wave (m/s) = wavelength (m) x frequency (1/s)
c =
c= speed of light = 3.00x108 m/s
My favorite radio station is 105.9 Jamming Oldies!!!
Wavelength of FM
c =
c= speed of light = 3.00x108 m/s
= 105.9MHz or 1.059x108Hz
= c/ =3.00x108 m/s = 2.83m
What does the electromagnetic
spectrum have to do with electrons?
It’s all related to energy – energy of
States of Electrons
When current is passed through a gas at a low pressure, the potential energy (energy due to position) of some of the gas atoms increases.
Ground State: the lowest energy state of an atom
Neon Signs
When an excited atom returns to its ground state it gives off the energy it gained in the form of electromagnetic radiation!
White Light
White light is composed of all of the colors of the spectrum = ROY G BIV When white light is passed through a prism, the light is separated into a
Line-emission Spectrum
When an electric current is passed
through a vacuum tube containing H2
gas at low pressure, and emission of a pinkish glow is observed.
Hydrogen’s Emission
Spectrum
The pink light consisted of just a few specific frequencies, not the whole range of colors as with white light
Scientists had expected to see a continuous range of frequencies of electromagnetic
Bohr’s Model of Hydrogen
Atom
Hydrogen did not produce a continuous spectrum
New model was needed:
Electrons can circle the nucleus only in allowed
paths or orbits
When an e- is in one of these orbits, the atom has
a fixed, definite energy
e- and hydrogen atom are in its lowest energy
Bohr Model Continued…
Orbits are separated by empty space,where e- cannot exist
Energy of e- increases as it moves toorbits farther and farther from the nucleus
Bohr Model and Hydrogen
Spectrum
While in orbit, e- can neither gain or lose energy
But, e- can gain energy equal to the difference between higher and lower orbitals, and therefore move to the higher orbital (Absorption)
Bohr’s Calculations
Based on the wavelengths of
hydrogen’s line-emission spectrum,
Photoelectric Effect
An observed phenomenon, early 1900s
When light was shone on a metal, electrons were emitted from that metal
Light was known to be a form of energy,
capable of knocking loose an electron from a metal
Photoelectric Effect pg. 93
Light strikes the surface of a metal (cathode), and e- are ejected.
These ejected e- move from the cathode to the anode, and current flows in the cell.
A minimum frequency of light is used. If the frequency is above the minimum and the
Photoelectric Effect
Observed: For a given metal, no
electrons were emitted if the light’s frequency was below a certain
minimum, no matter how long the light was shone
Explanation….
Max Planck studied the emission of light by hot objects
Proposed: objects emit energy in small, specific amounts = quanta
(Differs from wave theory which would say objects emit electromagnetic radiation continuously)
Quantum: is the minimum quantity of
Planck’s Equation
E radiation = Planck’s constant x frequency of radiation
E = h
h = Planck’s constant = 6.626 x 10-34 J•s
Einstein Expands Planck’s
Theory
Theorized that electromagnetic
radiation had a dual wave-particle nature!
Behaves like waves and particles
Think of light as particles that each carry one quantum of energy =
Photons
Photons: a particle of electromagnetic radiation having zero mass and carrying a quantum of energy
Back to Photoelectric Effect
Einstein concluded:
Electromagnetic radiation is absorbed by
matter only in whole numbers of photons
In order for an e- to be ejected, the e-
Example of Planck’s Equation
CD players use lasers that emit red light
with a of 685 nm. Calculate the
energy of one photon.
Different metals require different minimum
Answer
Ephoton = h
h = Planck’s constant = 6.626 x 10-34 J•s
c =
c= speed of light = 3.00x108 m/s
= (3.00x108 m/s)/(6.85x10-7m)
=4.37x10141/s
Wave Nature of Electrons
de Broglie’s Equation
A free e- of mass (m) moving with a velocity (v) should have an associated
wavelength: = h/mv
Linked particle properties (m and v)
Example of de Broglie’s
Equation
Calculate the wavelength associated
with an e- of mass 9.109x10-28 g
traveling at 40.0% the speed of light.
Answer
C=(3.00x108m/s)(.40)=1.2x108m/s
= h/mv
= (6.626 x 10-34 J•s) =6.06x10-12m
(9.11x10-31kg)(1.2x108m/s)
Wave-Particle Duality
de Broglie’s experiments suggested that e- has wave-like properties.
Thomson’s experiments suggested that e- has particle-like properties
Quantum mechanical model
SchrÖdinger
Heisenberg Pauli
Where are the e- in the atom?
e- have a dual wave-particle nature
If e- act like waves and particles at the same time, where are they in the atom? First consider a theory by German
Heisenberg’s Idea
e- are detected by their interactions with photons
Photons have about the same energy as
e-Any attempt to locate a specific e- with a photon knocks the e- off its course
Heisenberg’s Uncertainty
Principle
Impossible to determine both the
position and the momentum of an e- in an atom simultaneously with great
Schr
Ö
dinger’s Wave Equation
An equation that treated electrons in atoms as waves
Only waves of specific energies, and therefore frequencies, provided
solutions to the equation
Schr
Ö
dinger’s Wave Equation
Solutions are known as wave functions Wave functions give ONLY the
probability of finding and e- at a given place around the nucleus
e- not in neat orbits, but exist in regions
Schr
Ö
dinger’s Wave Equation
Here is the equation
Don’t memorize this or write it down
It is a differential equation, and we need calculus to solve it
-h (ә2 Ψ )+ (ә2Ψ )+( ә2Ψ ) +Vψ =Eψ
Probability likelihood
Orbital wave function; region in space
where the probability of finding an electron is high
SchrÖdinger’s Wave Equation states
that orbitals have quantized energies But there are other characteristics to describe orbitals besides energy
Quantum Numbers
Definition: specify the properties of atomic orbitals and the properties of electrons in orbitals
There are four quantum numbers The first three are results from
Quantum Numbers (1)
Quantum Numbers
Principal Quantum Number, n
Values of n = 1,2,3,…
Positive integers only!
Indicates the main energy level occupied
Quantum Numbers
Principal Quantum Number, n
Values of n = 1,2,3,…
Quantum Numbers
Principal Quantum Number, n
Values of n = 1,2,3,…
Describes the energy level, orbital size
Principle Quantum Number
n = 1 n=2
n=3 n=4 n=5 n=6
Principle Quantum Number
More than one e- can have the same n value
These e- are said to be in the same e- shell
The total number of orbitals that exist
Quantum Numbers (2)
Quantum Numbers
Angular momentum quantum number,
l
Quantum Numbers
Angular momentum quantum number,
l
Values of l = n-1, 0
Quantum Numbers
Angular momentum quantum number,
l
Values of l = n-1, 0
Describes the orbital shape
Indicates the number of sublevel
(subshells)
(except for the 1st main energy level,
Orbital Shapes
For a specific main energy level, the number of orbital shapes possible is equal to n.
Values of
l
= n-1, 0
Ex. Orbital which n=2, can have one of two
shapes corresponding to l = 0 or l=1
Depending on its value of l, an orbital is
Orbital Shapes
Angular magnetic quantum number, l
If l = 0, then the orbital is labeled s.
Orbital Shapes
If l = 1, then the orbital is labeled p.
Orbital Shapes
If l = 2, the orbital is labeled d.
Orbital Shapes
Energy Level and Orbitals
n=1, only s orbitals n=2, s and p orbitals
n=3, s, p, and d orbitals n=4, s,p,d and f orbitals
Atomic Orbitals
Atomic Orbitals are designated by the principal quantum number followed by letter of their subshell
Ex. 1s = s orbital in 1st main energy level
Quantum Numbers (3)
Quantum Numbers
Magnetic Quantum Number, ml
Quantum Numbers
Magnetic Quantum Number, ml
Values of ml = +l…0…-l
Describes the orientation of the
orbital
Atomic orbitals can have the same shape
Magnetic Quantum Number
s orbitals are spherical, only one orientation, so m=0
p orbitals, 3-D orientation, so m= -1, 0 or 1 (x, y, z)
Quantum Numbers (4)
Quantum Numbers
Electron Spin Quantum Number,ms
Values of ms = +1/2 or –1/2
e- spin in only 1 or 2 directions
A single orbital can hold a maximum of 2
Electron Configurations
Electron Configurations: arragenment of e- in an atom
There is a distinct electron configuration for each atom
Pauli Exclusion Principle
No 2 e- in an atom can have the same
set of four quantum numbers (n, l, ml,
ms ). Therefore, no atomic orbital can
Aufbau Principle
Aufbau Principle: an e- occupies the
Hund’s Rule
Hund’s Rule: orbitals of equal energy
Electron Configuration
The total of the superscripts must equal the atomic number (number of
electrons) of that atom.
Differentiating Electron
The differentiating electron is the electron that is added which makes the configuration different from that of the preceding element. The “last” electron.
H 1s1
He 1s2
Li 1s2, 2s1
Be 1s2, 2s2
Orbital Diagrams
These diagrams are based on the electron configuration.
In orbital diagrams:
Each orbital (the space in an atom that will
hold a pair of electrons) is shown.
The opposite spins of the electron pair is
Orbital Diagram Rules
1. Represent each electron by an arrow
2. The direction of the arrow represents the
electron spin
3. Draw an up arrow to show the first electron
in each orbital.
4. Hund’s Rule: Distribute the electrons among
the orbitals within sublevels so as to give the most unshared pairs.
Put one electron in each orbital of a sublevel before the second electron appears.
Orbital Diagram Examples
H _
1s
Li _
1s 2s
B __ __
1s 2s 2p
Dot Diagram of Valence
Electrons
When two atom collide, and a reaction takes place, only the outer electrons interact.
These outer electrons are referred to as the valence electrons.
Rules for Dot Diagrams
:Xy:
. .
. .
S sublevelelectrons Px orbital
Rules for Dot Diagrams
Remember: the maximum number of valence electrons is 8.
Only s and p sublevel electrons will ever be valence electrons.
Put the dots that represent the s and p electrons around the symbol.
Examples of Dot Diagrams
H
He
Examples of Dot Diagrams
C
N
O
Summary
Both dot diagrams and orbital diagrams will be use full to use when we begin our study of
atomic bonding.
We have been dealing with valence electrons since our initial studies of the ions.
The number of valence electrons can be determined by reading the column number.