history of the atom leading up to the current model
TRANSCRIPT
![Page 1: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/1.jpg)
History of the Atom
Leading up to the current model
![Page 2: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/2.jpg)
History of the Atom
Leading up to the current model
Assessment statement Obj Teacher’s notes
2.1.1 State the position of protons, neutrons and electrons in the atom.
1 TOK: None of these particles can be (or will be) directly observed. Which ways of knowing do we use to interpret indirect evidence gained through the use of technology? Do we believe or know of their existence?
2.1.2 State the relative masses and relative charges of protons, neutrons and electrons.
1 The accepted values are:
2.1.3 Define the terms mass number (A), atomic number (Z) and isotopes of an element.
1
2.1.4 Deduce the symbol for an isotope given its mass number and atomic number.
3 The following notation should be used: , for example,
2.1.5 Calculate the number of protons, neutrons and electrons in atoms and ions from the mass number, atomic number and charge.
2
2.1.6 Compare the properties of the isotopes of an element. 3
2.1.7 Discuss the uses of radioisotopes 3 Examples should include 14C in radiocarbon dating, 60Co in radiotherapy, and 131I and 125I as medical tracers.Aim 8: Students should be aware of the dangers to living things of radioisotopes but also justify their usefulness with the examples above.
2.1 The atom 1 hourTOK: What is the significance of the model of the atom in the different areas of knowledge? Are the models and theories that scientists create accurate descriptions of the natural world, or are they primarily useful interpretations for prediction, explanation and control of the natural world?
![Page 3: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/3.jpg)
Models of the Atom
Earliest Models:Dalton (and contemporaries)
“Billiard Ball” Solid sphereCannot be divided up into smaller particles or pieces.Atom neutral and no chargeAtoms of same element are made of the same types of atoms.
FaradaySuggested that structure of atom is somehow
related to electricity. Long series of experiments:
Atoms contain particles that have electrical charge.
*
![Page 4: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/4.jpg)
Models of the Atom (cont.)Faraday (cont.)
Greeks knew that if you rubbed amber with a cloth, it attracted dust or other particles.
Static electricity
FranklinStudied Static Electricity
Famous Kite Flying experimentFindings:
Object could have one of two electrical charges
Called them positive and negative (+, -)
Alike charges repel (+ +) and (- -)
Lightning was static electricity on a larger scale.
![Page 5: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/5.jpg)
Models of the Atom (cont.)Others (mid-1800s)
Scientists investigated electric currents
Cathode Ray Tube (CRT)
J.J. Thompson (1896)Systematic studies on cathode rays Movieconcluded that:
Through experiments, cathode rays were composed of negative particles and these negative particles could be manipulated with magnet & electric currents.
Atoms were not indivisible, solid sphere. But had substructure(s).
Eventually, addition of “pinwheel” to the tube showed that particles in beam had mass.
Uses of this Technology
*
![Page 6: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/6.jpg)
Models of the Atom (cont.)J.J. Thompson (cont.)
called negative particles “Electrons”Was able to determine ratio of electron’s electrical
charge to mass (1.76 x 108 coulombs per gram)
Millikan (1909)Oil Drop Experiment (Movie)
Measured the charge of an electron charged droplets with x-rays (negative charge)Varied rate of falling by changing charge in two charged plates. Calculated that the charge on each oil drop was a multiple of 1.60 x 10-19 C (coulombs)
Figured the charge for an electron must be 1.60 x 10-19
From this and Thompson’s ratio, calculated the mass of e-.
*
![Page 7: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/7.jpg)
Models of the Atom (cont.)What did this do to the idea of the Model?
This new research/data showed that the atom was NOT a solid sphere. But had “parts” that had a negative charge.However, the overall atom was neutral in charge.Therefore, there must be positive “parts” to balance the negative “parts”.Gave rise to the “Plum Pudding” Model.
Electrons (-) spread randomly throughout the atom. And surrounded by randomly spread out positive (+) parts.
*
![Page 8: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/8.jpg)
Models of the Atom (cont.)
RadioactivityBecquerel (1896)
Accidentally discovered uranium sample was radioactive (placed on photography film).
Radioactivity: Spontaneous emission from atom
Curie (Marie and hubby Pierre)Becquerel’s colleagues
Isolated 2 other radioactive materialsRadium and Polonium
![Page 9: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/9.jpg)
Models of the Atom (cont.)Radioactivity
Scientists soon after discovered several things:Radioactivity accompanies fundamental changes in
an atom.A chemical change happens as radiation is given off!!!
Rutherford (early 1900s)Studied Radioactivity
Used 2 electrically charged plates (Movie)Found that some radiation deflected towards negative
plate. Called it an ALPHA RADIATION.Other radiation deflected towards positive plate. Called
it BETA RADIATION.Later scientists found another radiation which was
undeflected by electrical charge. GAMMA RADIATION.Both Alpha and Beta radiations were shown to be particles.
![Page 10: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/10.jpg)
Models of the Atom (cont.)Rutherford (cont.)
Concluded that atoms contain electrons, but were electronically neutral
Alpha-scattering experiment (Gold Foil Experiment)
Movie
*
![Page 11: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/11.jpg)
Models of the Atom (cont.)Gold Foil Experiment (results)
A few particles were deflected off their path.Some particles “bounced back”
Think of playing pool. Glancing hits vs. more direct hits.Findings.
Most of the mass was concentrated in the core. The positive charge was concentrated in the core. Most of the area around an atom was “empty”.Nucleus is small compared to the atom, but very
large compared to electrons.Rutherford called this core, the nucleus. Lead to new model:
Nuclear Model
*
![Page 12: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/12.jpg)
MoseleyStudent of Rutherford’s
Found that atoms of each element contained unique positive charge in their nucleus.
Helped solve the mystery of what makes atoms of one element different from another element.
Atomic Number = # of PROTONSProton is the positive charge within an atom’s nucleus.
Atoms are electronically neutral.# of Protons (atomic #) = # of Electrons
*
![Page 13: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/13.jpg)
Bohr (1913):Niels Bohr came to work in Rutherford’s laboratory
Bohr asked to work on model because there were some problems with the nuclear model
According to Bohr's model only certain orbits were allowedVisualized the atom like the solar system. (Electrons in distinct “orbits” around the atom’s nucleus).
![Page 14: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/14.jpg)
Bohr's model of the atom is important introduced the concept of the quantum (levels) Started to explain atomic properties. However, Bohr's model needed revision
failed to explain the nature of atoms more complicated than hydrogen.
It took roughly another decade before a new more complete atomic theory was developed
the modern atomic theory.
*
![Page 15: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/15.jpg)
Louis de Broglie introduces the wave/particle duality of matter (1921) Traditional (classical) physics had assumed that particles were particles
and waves were waves
However, de Broglie suggested that particles could sometimes behave as waves and waves could sometimes behave as particles - the wave/particle duality of nature.
He suggested a simple equation that would relate the two: Particles have momentum (p), waves have wavelengths (l) and the two are related by the equation
l=h/p
h=Planck's constant = 6.634x10-34 Js
p=(mass)x(velocity)
This wave/particle duality of nature turned out to be a key to the new atomic theory.
![Page 16: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/16.jpg)
Werner Heisenberg elucidated the Uncertainty Principle (1923)
Classical physics had always assumed that precise location and velocity of objects was always possible.
Heisenberg, however discovered that this was not necessarily the case at the atomic level.
In particular, he stated that the act of observation interfered with the location and velocity of small particles such as electrons.
This is the case because observation requires light and light has momentum.
When light bounces off an electron, momentum exchange can occur between light and the electron which means the electrons location and velocity have been altered by the act of measurement.
This scenario has important implications to what we can measure at the atomic level.
![Page 17: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/17.jpg)
Erwin Schrodinger took the ideas developed by de Broglie, Heisenberg and others and put them together in a single equation that is named after him.
Schrodinger Equation
Hamiltonian represents the total energy of the system.
Solving this equation can, in principle, predict the properties and reactivities of all atoms and molecules.
Unfortunately, it is extremely difficult to solve for any but the most simple atoms and molecules. some essential conclusions:
I) Energies are quantized: Atoms and molecules cannot have any energy but only certain energies. This means that energies are "quantized".
II) The orbitals, associated with each energy, determine where the electrons are located.
![Page 18: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/18.jpg)
•These orbitals can be seen as the "rooms" in which the electrons in an atom "live". •The quantum energies together with the orbitals can be used to explain chemical properties and reactivities.
Electron Cloud Model
Electrons are located within
certain 3-D regions around the nucleus called clouds.
*
![Page 19: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/19.jpg)
Atoms
The practical “stuff”
![Page 20: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/20.jpg)
Atoms Made up of:Electrons
Negative charge
Around the nucleus
VERY small massProtons
Positive charge
In the nucleus
Accounts for large part of mass of an atomNeutrons
No charge
In the nucleus
Accounts for large part of mass of an atom.
“Glue” of an atomA force called the strong force opposes and overcomes
the force of repulsion between the protons and holds the nucleus together. (Binding Energy.)
*
![Page 21: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/21.jpg)
Atoms (cont.)Ions Atoms can gain or lose electrons Become Ions (more or less electrons than the # of
protons) Can be either POSITIVE or NEGATIVE Charge of ion = # of Protons - # of Electrons e.g. Magnesium (Mg) atomic # 12. Loses 2 e-
# of Protons 12
-# of electrons -10
+2
Mg2+
Try a few:
a) Ca loses 2 e- b) F gains 1 e- c) As gains 3 e-
Ca2+ F1- As3-
*
![Page 22: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/22.jpg)
Atoms (cont.)Isotopes All about Neutrons
“Glue”
Mass is 1 a.m.u. (Atomic Mass Unit)
(Mass of Proton are each 1 a.m.u.)
Think about the charges in the nucleus
(Repelling + charges)
More “glue” is needed as the # of protons climbs Same # of protons (why?) and different # of neutrons e.g. Hydrogen
Hydrogen (1H) has 1 proton, 0 neutrons. Mass is 1 a.m.u.
Deuterium (2H) has 1 proton, 1 neutron. Mass is 2 a.m.u.
Tritium (3H) has 1 proton, 2 neutron. Mass is 3 a.m.u. Mass Number:
Sum of isotope’s protons and neutrons.
*
![Page 23: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/23.jpg)
Isotopes (cont.)
Mass # 37Cl
Atomic # 17
What is that number (decimal) at the bottom under the symbol?
WHY?
Average of the isotope’s mass
e.g.12C 98.90% (of mass # 12) 0.9890 x 12 = 11.868 13C 1.10 % (of mass # 13) 0.0110 x 13 = 0.143
Average atomic mass: 12.011 amu
*
![Page 24: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/24.jpg)
Radioactivity
![Page 25: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/25.jpg)
Changes in the NucleusRadioactivity
Nuclear stability (instability)
Recall:Protons (? Charge)
Therefore: REPEL each otherNeutron (? Charge)
“Glue” to hold Protons togetherStrong Nuclear Force (the glue)
![Page 26: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/26.jpg)
Nuclear stability (cont.)From 1-20, approximate 1:1 Protons: Neutrons.
Beyond 20, more Neutrons.
83 and beyond, spontaneous emissions Can’t hold together indefinitelyFalls apart
Called “Decay”
As a radioisotope tries to stabilize, it may transform into a new element in a process called transmutation.
Not only too little “glue”, but also too much.
As a general rule, lighter & heavier isotopes (vs. common isotope) are likely radioactive.
*
![Page 27: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/27.jpg)
Nuclear stability (cont.)The basic unit of measure for radioactivity is the curie,
named after Marie Curie.
A quantity of 1 curie (or 1 C) is 37 billion atoms decay (disintegrate) in one second.
1C = 3.7 X 1010 disintegrations/sec. If the rate of decay is greater than 37 billion atoms in one second, then the source would have an activity greater than one curie if that source had fewer than 37 billion atoms decaying in one second, its activity would be less than one curie.
![Page 28: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/28.jpg)
Types of Radioactive Decay (basics)AlphaBetaGammaSpecials
Positron EmissionElectron Capture
Alpha Consists of 2 protons & 2 neutrons
What is that? 4
2He or 42a
Helium Nucleus (no electrons)Penetration power:
Stopped by paperCharge/Mass:
2+ / 4 amuWith Alpha, think LOSS
*
![Page 29: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/29.jpg)
Types of Radioactive Decay (cont.)Beta
Consists of high speed electronsWhat is that?
e- or 0-1b
Where do they come from????
Neutron changing into a proton (flip of a quark), ejects e-
Penetration power:
Stopped by heavy clothing
Charge/Mass:
1- / ~0 amu
With Beta, think CHANGE
*
![Page 30: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/30.jpg)
Types of Radioactive Decay (cont.)Gamma
Consists of high energy photons
What is that? gSimilar to X-rays
Penetration power:
Stopped by lead, concrete
Charge/Mass:
0 / 0
With Gamma,
Think ENERGY•See Radiation Movie
*
![Page 31: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/31.jpg)
Types of Radioactive Decay (cont.)Specials
Positron Emission (also called Beta positive decay)
A positron is exactly like an electron in mass and charge force except with a positive charge.
Charge/Mass: 1+ / 0 amu
It is formed when a proton breaks into a neutron with mass and no charge
= positron (no mass and the positive charge)
Positron emission is most common in lighter elements with a low neutron to proton ratio.
![Page 32: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/32.jpg)
Specials (cont)Electron Capture
A captured electron joins with a proton in the nucleus to form (change to) a neutron.
= one less proton, turned into a neutron.
Charge/Mass: changes from + 0 / same
Electron capture is common in larger elements with a low neutron to proton ratio.
![Page 33: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/33.jpg)
Decay of Uranium
![Page 34: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/34.jpg)
Uranium
![Page 35: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/35.jpg)
Reminder:
Nuclear Equations Equation that keeps track of the reaction’s components.
Alpha decay of Gold185
79Au 18177Ir + 4
2a
Decay of Iodine131
53I 13154Xe + 0
-1b
Try a few (solve):238
92U 23490Th + ______
2411Na ______ + 0
-1b
*
![Page 36: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/36.jpg)
Uranium:
Enriched Uranium: U-235Low: 3-4% U-235 (remaining is U-238)
Reactor GradeHigh: 90% U-235 (remaining is U-238)
Weapons GradeSlightly (0.9%-2%) (replaces natural U in some reactorsRecovered: less U-235 than in natural occurring Uranium
Depleted Uranium: U-238Remnants after enrichment
Less radioactive then natural Uranium
VERY Dense
-Useful for armor and penetrating weapons
NOTE: Depleted U-238 is still radioactive. Just LESS.
![Page 37: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/37.jpg)
Uses for Radioactive materials:
Weapons:Nuclear weapons
“Little Boy”
-Uranium, gun-type
-City of Hiroshima on
August 6, 1945
“Fat Man”
-Plutonium, Implosion
-City of Nagasaki on
August 9, 1945
![Page 38: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/38.jpg)
Uses for Radioactive materials:
Smoke Detectors: Am-241Gives off a particles
Ionizing energy (makes Ions)Ionize smoke particles
Allows completion of a circuit (allows electricity to flow)With a complete circuit, alarm sounds.
Cancer Treatment (BNCT)Boron Neutron Capture TherapyPatient is given Boron-10 (10B)Using a neutron beam, doctors create thermal neutrons which changes Boron-10 into excited Boron-11Boron-11 decays, given off an a particle
a particle penetrated one-two cells deep,
Kills the cell(s)
![Page 39: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/39.jpg)
Uses for Radioactive materials:
Carbon-14 datingThe radioactive C-14 method of dating is used to determine the age of organic matter that is several hundred years to approximately 50,000 yrs old.
C-14 is continually formed in nature by the interaction of neutrons with N-14 in the Earth’s atmosphere.
The neutrons required for this reaction are produced by cosmic rays interacting with the atmosphere.
C-14, along with non-radioactive C-13 and C-12, is converted into CO2 and assimilated by plants and organisms.
When plant or animal dies, it no longer acquires carbon.
C-14 begins to decay.
![Page 40: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/40.jpg)
Nucleosynthesis:
How were/are elements formed?
![Page 41: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/41.jpg)
Nucleosynthesis (cont.):
How were/are heavier elements formed?
Fusion with increasingly larger and larger elements4
2He + 42He 8
4Be + g
42He + 8
4Be 126C + g
Elements present in stars (depends on its size)H, He, C, O, Ne, Mg + other heavier elements
Larger stars (greater gravitational energies), heavier elements
Each “layer” acts to fuel the next “layer”.H He; He C; C O; O Ne; Ne Mg; Mg Si; Si Fe
Heavier elements are created in supernovas (exploding stars).
![Page 42: History of the Atom Leading up to the current model](https://reader036.vdocument.in/reader036/viewer/2022062516/56649dea5503460f94ae5d46/html5/thumbnails/42.jpg)