Unit 1: Atomic Structure & Periodicity Test Flashcards

1
Q

matter

A

anything that has mass and takes up space

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2
Q

element

A

simplest form of matter. Composed of only one type of atom. Elements cannot be broken down into simpler substances

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3
Q

pure substance

A

made up of one type of particle, thus they include elements. Pure substances have specific and consistent properties

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4
Q

compounds

A

occur when 2 or more elements chemically bond together

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5
Q

mixture

A

when 2 or more pure substances are physically mixed together, thus no chemical reaction/change has taken place and no new substances have been formed

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6
Q

heterogenous mixture

A

when 2 or more substances are mixed and the composition is not uniform throughout the mixture. You can visibly see that there are different substances mixed together

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7
Q

homogenous mixture

A

when 2 or more substances mix with a uniform composition at the particle level. A homogenous mixture appears as one substance

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8
Q

atom

A

A single particle of an element

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9
Q

molecules

A

particles composed of two or more atoms chemically bonded

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10
Q

ions

A

particles with an overall charge due to an imbalance of protons and electrons. Negative ions or anions have more electrons than protons. Positive ions or cations have less electrons than protons

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11
Q

isotopes

A

atoms with the same number of protons (atomic no.) but a different number of neutrons (mass no.)

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12
Q

frequency

A

the number of waves that pass in one second

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13
Q

wavelength

A

distance between two peaks

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14
Q

relationship between properties of a wave

A

inverse relationship where a shorter wavelength produce higher frequency, and a longer wavelength produce a lower frequency

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15
Q

rank types of electromagnetic radiation in terms of increasing wavelength and decreasing energy (frequency)

A

(infrared) ROY G BIV (ultra violet)

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16
Q

spectrum

A

a band of colours, as seen in a rainbow, produced by separation of the components of light by their different degrees of refraction according to wavelength.

17
Q

continuous spectrum

A

a spectrum that consists of light at all wavelengths without interruption. Hot dense objects produce a continuous spectra

18
Q

emission spectrum

A

a spectrum that only emits light at specific wavelengths, producing only a fe lines of colour. hot gases produce emission spectra

19
Q

absorption spectrum

A

a spectrum that looks like a rainbow with black lines removed at specific wavelengths. they are created when the light of an object that produces a continuous spectrum passes through a cloud of cool gas

20
Q

spectrograph

A

instrument that uses a prism or diffraction grating to split light into its component wavelengths.

21
Q

ionisation energy

A

energy to remove (1 mol) an electron from (1 mol of) a GASEOUS atom
equation: H(g) –> H+ (g) + e-

22
Q

electron affinity

A

energy change when a gaseous atom gains an electron
equation: H(g) + e- –> H(g)-

23
Q

first ionisation energy

A

the energy required to remove 1 mole of electrons from 1 mole of gaseous atoms

24
Q

successive ionisation energies

A

the energy required (per mole) to remove more than one electron from an atom. e.g. oxygen can have up to 8 successive ionisation energies, removing all 8 of its electrons

25
Q

limit of convergence

A

theoretical value for ionisation energy; where the energy levels converge (on an energy level diagram) represents ionisation energy

26
Q

effective nuclear charge (Z/Zeff)

A

the net electrostatic attraction experienced by valence electrons for the nucleus of an atom. (the overall pull that the nucleus of an atom has on its outermost (valence) electrons)

27
Q

effects of atomic structure on Zeff

A

1) number of principle energy levels
* the higher the energy level the farther away the electron is from the nucleus + the more inner shell electrons which result in a greater shielding effect of the nucleus’ positive charge
* more energy levels = lower Zeff
2) number of protons
* more protons = more positive charge in the nucleus, causing electrons to experience more attraction
* when the atoms’ shielding effect is equal (in the same period (row)): more protons = higher Zeff
3) number of electrons
* when atoms have the same number of energy levels and protons, the only thing left to compare is their electrons. With this, more electrons = lower Zeff
* more electrons = more electron repulsion, resulting in a reduction of the attraction felt by each valence electron

28
Q

atomic radius

A

the size of an atom of a given element (half the distance between two neighbouring nuclei) - usually listed in picometers (pm)

29
Q

ionic radius

A

the size of an ion of a given element (based on the distance between two neighbouring nuclei) - usually listed in picometers (pm)

30
Q

electronegativity

A

the relative ability of an atom to attract an electron pair when bonding

31
Q

types of electron orbitals and their shapes

A

1) s orbitals: sphere. comes in 1s, 2s, 3s
2) p orbitals: propeller. comes in 2px, 2py, 2pz
3) d orbitals: clover. comes in dyz, dxz, dxy, dy^2x^2, dz^2 (weird shape)

32
Q

oxidation state (or oxidation number)

A

a number assigned to an atom to show the number of electrons transferred in forming a bond. The term s used interchangeably with “charge.” e.g.
oxidation state: +1, +2, -2
ion symbol with charge: Na1+, Ca2+, O2-

33
Q

absorption on an energy level diagram

A

arrow between energy levels pointing UP

34
Q

emission on an energy level diagram

A

arrow between energy levels pointing DOWN

35
Q

UV region on an energy level diagram

A

transitions down to n=1

36
Q

Visible region on an energy level diagram

A

transitions down to n=2

37
Q

infrared region on an energy level diagram

A

transitions down to n=3

38
Q

ionisation energy on an energy level diagram

A

n=1 to n= infinity

39
Q

relative atomic mass

A

weighted average of the masses of all the isotopes of an element based on their abundance. All other atomic masses are relative to the mass of carbon-12. 1 atom of carbon-12 weighs exactly 12 amu, hence being the standard for atomic mass.