Chapter 1 - Atomic Theory Flashcards

1
Q

Democritus

  • Greek philosopher
  • 2400 years ago
  • ‘Could matter be divided into smaller and smaller pieces forever or was there a limit?
A

Atomos

  • Matter could not be divided into smaller and smaller pieces forever, eventually we would come to the smallest piece at the end.
  • The piece would be indivisible
  • Atomos means ‘indivisible’ in Greek
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2
Q

Democritus’ Atomic Model

  • Atoms: small, hard particles made of the same material but were different shapes and sizes
  • Atoms were infinite in number and capable of joining together
A

This theory was ignored for 2000 years because of two eminent philosophers named Aristotle and Plato.
They believed that the 4 main elements were made of Earth, Water, Fire, Air.

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3
Q

Dalton’s Atomic Theory

1) All element contain indivisible particles named atoms
2) Atoms cannot be created or destroyed
3) Atoms of the same element are exactly alike, they have the same masses
4) Atoms of different elements have different masses

A

Law of Constant Compositions
- A compound always contains atoms of two or more elements combined in definite proportions by mass.

Law of Multiple Compositions
- Atoms of two or more elements may combine in different ratios to produce more than one compound.

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4
Q

Modern Objections to Dalton’s Theory

1) Atoms are not indivisible, they contain subatomic particles
2) Not all atoms of an element have exactly the same mass
3) Some nuclear transformations alter (destroy) atoms

A

Crooke’s Experiment

  • Put a magnet next to a light beam caused it to be deflected
  • Experiment: passing an electrical current through a gas at very low pressure caused the gas to glow.
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5
Q

Lavoisier

  • Proposed the law of conservation of matter
  • Matter cannot be destroyed or created
A

Proust

  • Law of Definite proportions
  • Law of Multiple proportions
  • Dalton used these to develop his theory
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6
Q

J.J. Thompson

  • Discovered the electron
  • Proposed that negative charges came from within the atom
  • From this he reasoned that there must be positive charged subatomic particles as well to keep a neutral charge.
  • E/m= 1.76 * 10^8
A

Protons were first discovered by E. Goldstein in 1896
- Mass of Proton = 1.673*10^-24 grams
Then was officially proven by Rutherford.
- This lead to the discovery of neutrons
His experiment required a gold foil and noticed that once atoms were shot directly at the sheet some bounced off.
- Protons bounced off of the gold sheet as the sheet had protons as well (positive charges repel positive charges)

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7
Q

Neutrons were officially discovered by Chadwick

A

The Bohr Model

  • Electrons move in definite orbits around the nucleus like planets moving around the sun
  • Each electron moves in a specific energy level
  • Electrons that are further away from the nucleus have higher energy levels
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8
Q
  • When electrons jump from a higher energy level to a lower energy level, atoms radiate energy
  • When electrons jump from a lower energy level to a higher energy level, atoms absorb energy
A

Planck

  • Suggested that energy consists of small paricles known as photons
  • photons can only have discreet energies
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9
Q

Einstein

  • Matter and Energy are not different things but different expressions of the same thing
  • E (energy)= m (mass) c (speed of light)^2
A

De Broglie

  • If energy could be thought of as having particle properties along with wave like properties
  • Then matter can be thought of as having wave like properties along with particle properties
  • mc^2 = h (planck’s constant) v (frequency)
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10
Q

Heisenberg Uncertainty Principle

  • It is impossible to know the location and the momentum of a high speed particle such as an electron
  • .by finding out one, the other os changed
A

Wave Mechanical Model

  • Atom is more like a cloud
  • Atom orbitals around the nucleus define the places where electrons are most likely to be found
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11
Q

Compound

A

Elements chemically bonded together to produce different properties that its original elements
- E.g. Hydrogen (flammable)+ Oxygen (flammable) –> Water ( a substance that puts out fire)

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12
Q

Mixture

A

Elements not chemically bonded together to retain properties of its original elements.

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13
Q

The Functions:

  • Protons –> The identity of the element
  • Neutrons –> Stability, changing amount of neutrons make elements unstable and radioactive
  • Electrons–>Chemical radioactivity, electrons are on the outside of the atom.
A

Isotopes

  • Isotopes of an element have the same chemical properties because they have the same number of electrons.
  • Isotopes of an element however have different physical properties
  • Isotopes with fewer neutrons will have:
    a) lower masses and densities
    b) faster rate of diffusion
    c) lower melting and boiling points
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14
Q

Used to determine the Average Atomic Mass of an Element

A

m (mass in a.m.u.) * r (relative abundance in decimals) + m2*r2 = average atomic mass

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15
Q

The Mass Spectrometer

A

Used to:

  • measure the relative masses of isotopes
  • find the relative abundance of the isotopes in a sample of an element
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16
Q

Vaporization

A

the sample is heated to form a gas.

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17
Q

Ionisation

A
  • sample is bombarded by a stream of high energy electrons from an electron gun.
  • an electron is knocked from an atom
  • a positive ion forms
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18
Q

Acceleration

A

accelerates postiveions and creates a narrow beam of ions

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19
Q

Deflection

A

the accelerated ions are deflected (bent) by the magnetic field

  • Deflection is greater when:
    a) mass of ion is smaller
    b) charge of ion is greater
    c) strength of magnetic field is greater
20
Q

Detection

A

amount of ions hitting detector in one spot

21
Q

Radioactive Nuclei

A
  • Radionuclides are unstable

- some isotopes are stable however the others are radioactive e.g. C12 is stable but C14 is radioactive.

22
Q

Stability Factors

A

1) the mass number (which is the total number of nucleons in the nucleus)
2) the neutron to proton ratio

23
Q

Alpha Emitters

A
  • Radionuclide has a lower neutron to proton ratio (too many protons) than for a stable nucleus.
  • To increase the neutron to proton ratio back to a stable ratio, it releases an ‘alpha’ particle
  • Can be stopped by paper, low energy
24
Q

Beta Emitters

A
  • Radionuclide has a higher neutron to proton ratio (too many neutrons) than for a stable nucleus.
  • A neutron is changed into a proton by releasing a beta particle (electron)
  • Raises the number of protons by one and reduces the number of neutrons by one
  • Can be stopped by a large wall or lead vest, higher energy
25
Q

Gamma Radiation

A
  • A type of electromagnetic radiation
  • When a positron (e+) and electron (e-) combine
  • Has no mass and no charge but a lot of energy
26
Q

Uses of Radioisotopes

A

1) Generate electricity
2) Preserve food
3) Sterilise surgical equipments
4) Detect cracks in structural materials
5) Archeology (dating of objects) through half-life

27
Q

Treating electromagnetic radiation (light as a wave)

A
  • Waves have a frequency
  • Waves have a wavelength
  • Speed of light (3.00*10^8)
    so. ..
  • c (speed of light) = v (frequency) * (wavelength)
  • > short wavelength = high frequency
  • > high wavelength = low frequency
28
Q

Treating electromagnetic radiation (light as a particle)

A
  • Photons: packets of energy released when electrons drop to lower energy level
  • Quantised (can only have certain values)
  • change in energy (electron) = change in energy (photon)

/Particles have a frequency
/Particles have energy
/E (energy) = h (Planck’s constant = 6.63*10^-34) * v (frequency)

29
Q

Which frequencies can be observed?

- From n=x to n=1

A
  • These electron transitions emit the most energy (highest frequency or shortest wavelength)
30
Q

Which frequencies can be observed?

- UV range

A
  • n=3 -> n=1 emits a higher frequency than n=2 to n=1
31
Q

From n=x to n=2

A
  • These electron transitions emit less energy

- This is the visible range

32
Q

From n=x to n=3

A
  • These electron transitions emit the least energy (lowest frequency or longest wavelength)
  • IR range
33
Q

Note

A

an electron at n=infinity is no longer in the atom, an ion has formed

34
Q

Quantum Numbers

  • Define the shape, size, and energy of each electron
  • forth quantum number defines spin
  • these numbers give each electron its own identity.
A

1) n –> principle
- the energy level
2)l –> orbital
- shape of orbital
a-)if l=0 then its s orbital
b-)if l=1 then its p orbital
c-)if l=2 then its d orbital
d-)if l=3 then its f orbital

35
Q

m1 = magnetic

  • l=0 then one orientation
  • l=1 then 3 orientations
  • l=2 then 5 orientations
  • l=3 then seven orientations

number is in between -3 and 3

A

mS = spin

-This is either -1/2 or 1/2

36
Q

Pauli Exclusion Principle

A

This principle discusses that an orbital must have an electron with a positive spin (up arrow) and are with a negative spin (down arrow)

37
Q

Aufbau Principle

A
  • States that electrons are placed into orbitals with lowest energy first.
38
Q

Hund’s Rule

A
  • States that within a sub-level, the electrons occupy orbitals as unpaired electrons first then as paired electrons to reduces as much repulsion as possible.
39
Q

Orbital Notation

A
  • Use boxes or line to represent orbitals

- The direction of arrows (electrons) indicate the spin of the electron

40
Q

Valence Electrons

A
  • Are the electrons on the outer shell
  • Electrons are divided between cone and valence electrons
  • E.g. B -> 1s2 2s2 2p1
  • > Core = [He], Valence = 2s2 2p1
41
Q

Ions
-The electrons that are lost or gained should be added/removed from the highest energy level (not the highest orbital in energy)

A

Positive:

  • formed by the loss of electrons
  • 1s2 2s2 2p6 3s1 (Na atom)
  • > 1s2 2s2 2p6 (Na+ atom)

Negative:

  • formed by the gain of electrons
  • 1s2 2s2 2p4 (O atom)
  • 1s2 2s2 2p6 (O- ion)
42
Q

First Ionisation Energy:

A

This is the energy required to remove one mole of electrons from one mole of gaseous neutral atoms.

43
Q

Second Ionisation Energy:

A

This is the energy required to remove second electron from a 1+ ion. Requires more than first ionisation energy, since the protons are pulling on less electrons.

44
Q

Third Ionisation Energy:

A

Energy required to remove third electron from a 2+ ion. Requires more than second ionisation energy. Electrons feel the pull of two more protons.

45
Q

Energy needed to remove electron related to stability

  • Full energy level (n)
  • Full sub-level (s,p,d,f)
  • Half full sub-level
A

Scanning Tunnelling Microscope

  • STM
  • Physical technique to manipulate individual atoms
  • Not “see” not “feel” atoms using computer
46
Q

Trends in 1st ionisation energy (left to right along the period)

A
  • same shielding
  • stronger attraction between nucleus and outer electrons (increased effective nuclear charge/ increased electrostatic attraction)
  • outer electrons harder to pull off increased first ionisation energy
47
Q

Trends in ionisation energy (Metals)

A
  • More energy levels are added
  • atomic radii increases
  • more shielding form inner electrons
  • outer electrons further from the nucleus
  • decreased attraction of protons for outer electrons
  • decreased first ionisation energy