Chapter 1 Atomic Structure Flashcards

1
Q

protons

A
  • found in the nucleus of an atom
  • e= 1.6 x 10^-19 C
  • 1 amu
  • equal to the atomic number
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2
Q

neutrons

A
  • no charge
  • make up nucleus with protons
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3
Q

mass number

A

sum of protons and neutrons

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4
Q

isotopes

A
  • same atomic number, different masses
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5
Q

electrons

A
  • move through space around nucleus
  • negative charge
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6
Q

electron shells

A
  • lower electron shell, closer to nucleus, lower energy levels
  • higher electron shell, farther from nucleus, higher energy levels
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7
Q

Valence electrons

A
  • electrons farthest from nucleus
  • strong interaction with environment, weak interactions with nucleus
  • more likely to become involved in bonds with other atoms
  • determine reactivity of the atom
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8
Q

describe sharing of valence electrons

A
  • allows elements to fill their highest energy levels to increase stability
  • neutral… = numbers of proton and electrons
  • gain electrons, atom gains negative charge
  • lose electrons, atom gains positive charge
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9
Q

cation

A

positively charged atom

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10
Q

anion

A

negatively charged atom

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11
Q

Avogadro’s number

A
  • 6.02 x 10^23 = one mole
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12
Q

Planck relation

A
  • energy of a quantum
  • E = hf
    h = plancks constant (6.626 X 10^-34 J*s)
    f = frequency of radiation
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13
Q

Angular momentum

A
  • L = mvr
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14
Q

Kinetic energy

A

K = 1/2 mv^2

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15
Q

Bohr model of angular momentum

A
  • L = (nh)/(2pi)
    n = principal quantum number
    h = planks constant (6.626 x 10^-34 J*s)
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16
Q

Energy of the electron

A
  • E = - ( R_H) / (n^2)
  • R_H is rydberg unit of energy (2.18 X 10^-18 J/electron)
  • energy of an electron increases (less negative) the further from the nucleus (increasing n)
17
Q

ground state

A
  • lowest energy radius n = 1
  • all electrons in the lowest possible orbital
18
Q

excited state

A
  • electrons moved to an orbit with a larger radius
  • at least one electron has moved to a subshell of higher than normal energy
  • often as a result of heat or other energy forms to cause excited state
19
Q

Electromagnetic energy emitted from photon when returning to ground state

A
  • E = hc / gamma
    h = plancks constant (6.626 x 10^-34)
    c = speed of light (3.00 X 10^8 m/s)
    gamma = wavelength
20
Q

line spectrum

A
  • each line on the emission spectrum corresponds to a specific electron transition
21
Q

atomic emission spectrum

A

due to each element having electrons that can be excited to a different set of distinct energy levels

22
Q

difference in energy between higher and lower energy states

A

E = hc / gamma = R_H [ (1/n1^2) - (1/n2^2)]

23
Q

principal quantum number

A
  • n
  • first quantum number…
  • larger the integer value of n, the higher the energy level and radius of the electron’s shell
24
Q

maximum number of electrons within a shell:

25
azimuthal quantum number
- letter l - second quantum number, shape and number of subshells within a given principal energy level - value of n limits value or l - only possible values are 0 or (n-1)
26
spectroscopic notation
- l = 0 subshell is s - l = 1 subshell is p - l = 2 subshell is d - l = 3 subshell is f ex: n=4, 4d
27
maximum number of electrons within a shell
4l + 2 l = azimuthal quantum number
28
magnetic quantum number
- third quantum number - ml - specifies particular orbital within a subshell - possible values of ml are the integers between -l and +l, including 0
29
spin quantum number
- fourth quantum number - ms - two spin orientations (+1/2) and (-1/2) - two electrons in same orbital = opposite spin
30
Aufbau principle
- electrons fill from lower to higher energy subshells (building up principle)
31
Hunds rule
- within a given subshell, orbitals are filled such that there are a meximum number of half-filled orbitals with parallel spins