3.2 Quantum Numbers Flashcards

1
Q

What is the Principal Quantam Number, n? Describe its characteristics.

A

a positive whole number that indicates the energy level and relative size of an atomic orbital
~ aka “shell”

n can have values from 1 to infinity, however 1 to 7 practically
~ as n values increase, so does size and energy level

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2
Q

What is the Orbital Shape Quantam number, l? Describe its characteristics.

A

an integer that describes the shape of atomic orbitals within each principal energy level
~ aka “sublevel” or “subshell”

l can have values from 0 to n-1
(ex. if n=3, l = 0 or 1 or 2)

each value of l can be identified by a letter
~ l = 0 (s)
~ l = 1 (p)
~ l = 2 (d)
~ l = 3 (f)

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3
Q

What is the Magnetic Quantam Number, ml? Describe its characteristics.

A

an integer that indicates the orientation of an orbital in the space around a nucleus
~ can have values from -l to +l
(ex. if l = 2 then ml = -2, -1, 0, 1, or 2 )

  • an atomic orbital can contain a max of 2 electrons
  • # of orbitals at an energy level n is n^2
  • max # of electrons at an energy level n is 2n^2
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4
Q

What is the Spin Quantam Number, ms? Describe its characteristics.

A

The quantam number that specifies the orientation of the axis on which the electron is spinning
~ ms can have values of +1/2 (spin up) or -1/2 (spin down)

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5
Q

What is the pauli exclusion principle

A
  • a max number of 2 electrons can occupy an orbital
  • electrons in an orbital must have OPPOSITE spins
  • each electron in an atom has a unique set of 4 quantam numbers
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6
Q

What is the exception for Cr?

A

[Ar] 4s1 3d5

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7
Q

What is the exception for Mo?

A

[Kr] 5s1 4d5

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8
Q

What is the exception for Cu?

A

[Ar] 4s1 3d10

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9
Q

What is the exception for Ag?

A

[Kr] 5s1 4d10

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10
Q

What is the exception for Au?

A

[Xe] 6s1 4f14 5d10

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11
Q

What did Heisenberg propose?

A

an uncertainty principle that says that it is not possible to exactly define both the position and momentum (speed); the more you define one value, the less you know about the other

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