Reactivity & Structure 1: Models Of The Particulate Nature Of Matter Flashcards

1
Q

Democritus’ Model

A

Theorized that matter could be continually split until a size where it could not be split any further. He called these tiny pieces atomos, meaning “indestructible” in Greek.

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2
Q

Dalton’s Model

A

All matter is made up of atoms, which are tiny, indivisible particles. All the atoms of an element have the same size, mass, and properties but the atoms of different elements have different sizes and masses. Atoms cannot be created, destroyed, or divided into smaller particles.

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3
Q

J. J. Thompson’s Model

A

The Plum Pudding Model, in which electrons were embedded in a sphere of positive charge.

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4
Q

The Cathode Ray Experiment

A

J. J. Thompson’s experiment showed that all atoms contain tiny negatively charged subatomic particles or electrons.

He placed two oppositely-charged plates around the cathode ray, and the ray was deflected from the negative plate but attracted to the positive one.

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5
Q

Rutherford’s Model

A

Described the atom as having a tiny, dense, and positively charged core called the nucleus. It was established that the mass of the atom was concentrated in its nucleus. The light, negatively charged, electrons circulated around this nucleus. It was the first dynamic/planetary model.

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6
Q

The Gold Foil Experiment

A

Rutherford fired a beam of alpha particles at a thin sheet of gold that was surrounded by a censor that would flash when hit. It was predicted that the particles would pass straight through, as the Plum Pudding Model stated that the positive charges were spread out and subsequently too weak to impact the particles. However, some particles were deflected, resulting in the conclusion that the positive charge must be localized over a very tiny volume of the atom and that the atom must be made up of mostly empty space.

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7
Q

Bohr’s Model

A

Electrons can only exist in stationary orbits around the nucleus, which are associated with discrete energy levels that converge at higher energy.

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8
Q

Emission Line Spectrum

A

Produced by hot gas. Shows the release of a photon of a specific energy as electrons return to a lower level, related to a specific frequency of light.

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9
Q

Absorption Line Spectrum

A

Produced by cold gas, shows the absorption of a photon of specific energy as they are excited to a higher level, related to a specific frequency of light.

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10
Q

The Electromagnetic Spectrum

A

*Left to right

Gamma rays, X-rays, ultraviolet, visible light, infrared, microwaves, radio waves.

(Raging Martians Invaded Venus Using X-ray Guns)

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11
Q

Allotropes

A

Alternative forms of an elemental substance. For example, diamond and graphite are allotropes of carbon.

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12
Q

The Kinetic Molecular Theory

A
  1. All matter is made up of particles/molecules/atoms
  2. All particles have kinetic energy that causes them to constantly move
  3. No intermolecular forces
  4. Completely elastic collisions, no loss in kinetic energy
  5. The amount of energy is proportional to the temperature
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13
Q

Density

A

The density of a substance is its mass per unit volume (mass ÷ volume). Substances with higher densities will feel ‘heavier’ compared to substances with lower densities (of the same volume).

d = m ÷ v

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14
Q

Sublimation

A

Solid to gas with no liquid state. Heat is absorbed.

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15
Q

Deposition

A

Gas to solid with no liquid state. Heat is released.

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16
Q

The Atomic Number

A

The atomic number (symbol Z) is the number of protons in the nucleus of an atom.

17
Q

The Mass Number (Nucleon Number)

A

The mass number (symbol A), also called the nucleon number , is the number of protons and the number of neutrons in the nucleus of an atom.

18
Q

Relative Atomic Mass

A

The weighted average mass of an atom compared to 1/12 the mass of an atom of carbon-12.

Can be calculated by multiplying the percent abundance with the masses of the isotopes then dividing by 100.

[(Percent abundance • mass of isotope) ÷ 100]

19
Q

Mass Spectrometer

A

An instrument that is used to determine the abundance of the various isotopes of an element, based on a measurement of the mass-to-charge (m/z) ratio of ions within a sample of the element.

20
Q

Five Stages of a Mass Spectrometer

A
  1. Vaporization: substance is vaporised to produce gaseous molecules.
  2. Ionization: high-energy electrons are fired at gaseous molecules, causing them to be ionised, forming gaseous ions (known as molecular ions).
  3. Acceleration: the gaseous ions are accelerated in an electric field.
  4. Deflection: the gaseous ions are deflected by an electromagnet. The degree of deflection they undergo depends on their m/z ratio. Ions with lower m/z ratios are deflected the most and ions with higher m/z ratios are deflected the least.
  5. Detection: the gaseous ions are detected and a mass spectrum is produced.
21
Q

Emission Spectra

A

The range of frequencies or wavelengths of electromagnetic radiation emitted during an electron transition from a higher to a lower energy level.

22
Q

Principal Quantum Number

A

The main energy levels occupied by electrons, assigned the letter “n”.

23
Q

Degenerate Orbitals

A

Atomic orbitals that have equal energy levels. For example, the three 3p orbitals are degenerate orbitals.

24
Q

Aufbau Principle

A

States that when adding electrons to an atom, the lower energy orbitals must be filled first.

25
Q

Pauli Exclusion Principle

A

States that an atomic orbital can only hold two electrons and they must have opposite spins.

26
Q

Hund’s Rule

A

States that when we have degenerate orbitals (orbitals of the same energy) then each orbital is filled with a single electron before being doubly occupied.

27
Q

First Ionization Energy

A

The energy required with remove one mole of electrons from one mole of gaseous atoms to form one mole of gaseous 1+ ions.

28
Q

First Ionization Energy: Beryllium and Boron

A

First ionization energy decreases from beryllium to boron because:

beryllium: 1s² 2s²
boron: 1s² 2s² 2p¹

Electrons in p orbitals are of higher energy and further from the nucleus than electrons in s orbitals, therefore they require less energy to remove.

29
Q

First Ionization Energy: Nitrogen and Oxygen

A

First ionization energy decreases from beryllium to boron because:

nitrogen has the electron configuration 1s² 2s² 2p³
oxygen has the electron configuration 1s² 2s² 2p⁴

An electron in a doubly occupied orbital is repelled by the second electron and requires less energy to remove than an electron in a half-filled orbital.

30
Q

Exothermic Reactions

A

Describes a reaction in which energy is transferred or released to the surroundings.

31
Q

Endothermic Reactions

A

Describes a reaction in which energy is transferred or absorbed from the surroundings.

32
Q

Enthalpy

A

Measurement of heat energy within a system. It is symbolised in expressions by H.

33
Q

Standard Enthalpy Change

A

The heat energy transferred within a reaction under standard conditions with all substances present in their standard states.

34
Q

Specific Heat Capacity

A

The quantity of energy needed to raise 1 g of a substance by 1 K.

35
Q

Change in Enthalpy

A

ΔH (change in enthalpy) = -Q (thermal energy) ÷ n (number of moles)

36
Q

Bond Enthalpy

A

The energy required to break one mole of chemical bonds in the gaseous state.

  • Bond enthalpy values are always positive because they refer to bonds being broken (bond breaking is endothermic).