What is Today’s Model?
Dense, Positively Charged Nucleus Mostly Empty Space Negatively Charged Electron Cloud Most Probable Location of theElectrons Composed of Protons,
Democritus proposes the 1st atomic
theory
460 – 370 BC
History of the Atom - Timeline
Antoine Lavoisier makes a substantial number of contributions
to the field of Chemistry
1766 – 1844
John Dalton proposes his atomic theory in
1803
1743 – 1794
0
1856 – 1940
J.J. Thomson discovers the electron and proposes the Plum Pudding Model in 18971871 – 1937
Ernest Rutherford performs the Gold Foil
Experiment in 1909
1885 – 1962
Niels Bohr proposes the Bohr Model in
1913
1887 – 1961
Erwin Schrodinger
describes the electron cloud in 1926
1891 – 1974
James Chadwick discovered the neutron
in in 1932
1700s 1800s 1900s
Early Greeks
Matter is made of indestructible
particles called “atomos”
Summary for Dalton’s
Atomic Theory
(Father of the Modern Atomic Theory)
All atoms of a single element have the same mass
Atoms of different elements are different.
Atoms can’t be divided, created or destroyed.
Atoms of different elements combine in simple
Discovery of the Electron
In 1897, J.J. Thomson used a cathode ray tube to deduce the presence of a negatively charged particle.
Cathode ray tubes pass electricity through a gas that is contained at a very low pressure.
J.J. Thomson
• ALL atoms must contain
these negative particles.
• atoms did not have a net
negative charge
• there must be something
Ernest Rutherford’s (1871-1937)
electrons embedded in a positive pudding.
Where exactly are those electrons?
Thomson’s Theory: “Plum Pudding”
Shoot something at them to see where they are.
Rutherford’s Conclusion (1911)…
Small, dense, positive nucleus.
Equal amounts of (-) electrons at large distances
Neils Bohr’s Atomic model (1913)
Small, dense, positive nucleus.
Equal amounts of (-) electrons at specific orbits
around the nucleus.
This incorrect version of the atom is often used to represented atoms
Bohr’s Calculations
• Bohr calculated the
energies that an e-would have in the
allowed energy levels for the hydrogen
Chadwick
** James Chadwick
discovered neutrons in 1932.
---- n0 have no charge
and are hard to detect
V.Montgomery & R.Smith 14
V.Montgomery & R.Smith 15
Where are the e- in the atom?
• e- have a dual wave-particle nature (Recall deBroglie)
V.Montgomery & R.Smith 16
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
• ALWAYS a basic uncertainty in trying to locate
e-V.Montgomery & R.Smith 17
Heisenberg’s Uncertainty Principle
• Impossible to determine both the position and
ErwinS Schrodinger
(1887-1961)
• 1926
• the exact location of an electron
cannot be stated
• more accurate to view the
electrons in regions called
electron clouds
• electron clouds are places where
the electrons are likely to be found
• Did extensive work on the Wave
formula Schrodinger equation • Won a Nobel Prize
Image taken from: nobelprize.org/.../1933/schrodinger
V.Montgomery & R.Smith 19
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
• Quantization of e- energies was a natural
Quantum Model
Major points
1. Electrons do not follow fixed paths
2. They move randomly in areas of probability (orbitals)
3. There are specific energies associated with each orbital
New Model =
According to quantum mechanics, each electron is described by four quantum numbers:
•1. Principal quantum number (n)
•2. Angular momentum quantum number (l)
•3. Magnetic quantum number (ml)
•4. Spin quantum number (ms)
•The first three define the wave function for a
The Shapes of Atomic Orbitals
• the l quantum number primarily determines
the shape of the orbital
• l can have integer values from 0 to (n – 1)
• each value of l is called by a particular letter
that designates the shape of the orbital
– s orbitals are spherical
– p orbitals are like two balloons tied at the knots
l
= 0, the
s
orbital
• each principal energy
state has 1 s orbital
• lowest energy orbital in a
principal energy state
• spherical
25
2
s
and 3
s
2sn = 2, l = 0
3s n = 3,
l
= 1
, p
orbitals
• each principal energy state above n = 1 has 3 p orbitals
– ml = -1, 0, +1
• each of the 3 orbitals point along a different axis
– px, py, pz
l
= 2
, d
orbitals
• each principal energy state above n = 2 has 5 d orbitals
Atomic Models-
Simulation
• The question now is what is a fundamental
particle?
• Radioactive decay shows that protons and
neutrons are not fundamental