U1: trends + bonding Flashcards

1
Q

prefixes

A

mono, di, tri, tetra, penta, hexa, hepta, octa, nona, deca

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2
Q

roman numerals?

A

I, II, III, IV, V, VI, VII, VIII, IX, X

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3
Q

annhydruous

A

hydrate removed

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4
Q

boron, carbon, & silicon charge?

A

boron: 3+
carbon: 4+
silicon: 4+

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5
Q

which periods (rows) can have 8-18 valence electrons?

A

period 3 and below

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6
Q

EN values mean which bonds?

A

0-0.5 is non-polar covalent
0.5-1.7 is polar covalent
1.7-3.3 is ionic

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7
Q

melting and boiling points for each intramolecular bond?

A

ionic: high
polar-covalent: medium
non-polar covalent: low

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8
Q

water solubility for each intramolecular bond?

A

ionic: water-soluble
polar-covalent: water-soluble
non-polar covalent: non-water-soluble

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9
Q

electrical conductivity for each intramolecular bond?

A

ionic: yes, electrolyte
polar-covalent: no, non-electrolyte
non-polar covalent: no, non-electrolyte

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10
Q

electrolyte

A

substances that conduct electricity in the molten state or in solution

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11
Q

when are imfs broken/formed?

A

broken during boiling/melting, formed during freezing/condensing

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12
Q

which properties do imfs impact?

A

physical. i.e. changes of state, solubility

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13
Q

which states are imfs strong in?

A

liquids + solids. almost non-existent in gases except extreme conditions. (tht’s why there r gas laws)

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14
Q

relationship between imf and state at room temp?

A

strong imf = solid at room temp
weak imf = gas at room temp

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15
Q

order from strong-weak of imfs

A
  1. ionic/covalent bonds
  2. ion-dipole (ion+dipole)
  3. hydrogen bonds (H w/ NOF)
  4. dipole-dipole (polar molecules)
  5. london dispersion (non-polar, but exist in all molecules)
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16
Q

polarizability + what impacts it

A

“ease with which an electron cloud can be deformed.” larger (more electrons) = more polarizable

17
Q

PEN rule

A

protons = atomic number
electrons = atomic number - charge
neutrons = atomic mass - atomic number

18
Q

atomic mass unit

A
  • calculated w/ magnetic field
  • approx. mass of 1 proton
  • 1/12 mass of C-12 atom
19
Q

isotope

A
  • same atom have diff. amnts of neutrons/protons
  • each occur in abundance, e.g. 12% means 12% will be that isotope in a sample
20
Q

radioisotope

A
  • has unstable nucleus
  • has radioactive decay
21
Q

radioactive decay

A
  • process by which an unstable nucleus rearranges itself
  • nucleus can throw out protons/neutrons that are imbalanced
22
Q

electron configuation + wht it’s based off of

A
  • an atoms arrangement of electrons around the nucleus to have the lowest possible energy bc thats the most stable state
  • stability based on atomic radii, ionization energy, electron affinities, and electronegativity
23
Q

atomic radii

A
  • size of atom
  • measured in picometres (pm) or angstroms (A w/ degree) from centre of nucleus to outermost electron
24
Q

wht’s atomic radii influenced by?

A
  1. energy level: high energy levels are further from nucleus
  2. charge on nucleus: more protons=more pull on electrons
  3. shielding effect
25
Q

shielding effect

A

electrons in inner shells (kernel electrons) shield the valence electrons from the positive charge of nucleus, so the valence electrons can move further out = bigger atom. +like charges repel, so kernel electrons repel the valence

26
Q

ions

A

charged atoms, happen when there’s more or less electrons than protons (imbalance)

27
Q

cation

A
  • positively charged ions formed as a result of loss of electron(s)
  • metals usually form cations
    -smaller than neutral atom bc. less electrons mean the positive nucleus is more potent
28
Q

anion

A
  • negatively charged ions formed as a result of gain of electron(s)
  • non-metals usually form anions
    -larger than neutral atom bc. extra electrons repel each other
29
Q

ionization energy

(wht does a low IE mean)

A
  • amount of energy required to completely remove an electron from a gaseous atom
  • low IE = easy to take electron = more reactive
30
Q

what impacts ionization energy

(wht causes big/small IE)

A
  • bigger IE w/ bigger charge of nucleus
  • smaller IE if valence electrons are far away from nucleus
  • exception: filled and half-filled (4 & 8) valence shells have high IE
  • shielding effect
31
Q

electron affinity

A
  • energy change associated with adding an electron to a gaseous atom: typically negative due to release of energy
  • easiest to add to halogens
32
Q

wht does a negative electron affinity cause

A

atom becomes more stable and thus releases a great deal of energy when it gains an electron
- decrease in potential energy

33
Q

wht does a positive electron affinity cause

A

atom becomes less stable and thus gains energy when it gains an electron
- increase in potential energy

34
Q

which group has the highest electron affinity?

A

halogens: release the most energy when they gain an electron, meaning they become very stable

35
Q

electronegativity

A

tendency for an atom to attract electrons to itself when it is chemically combined with another element

36
Q

relationship between electronegativity and electron affinity?

A

atoms with large negative electron affinity have large electronegativity: large electronegativity means it pulls the electron toward it

37
Q

trends of each periodic trend?

A

electron affinity, ionization energy, electronegativity: increase right and up
atomic radius: increase left and down