Quantum Numbers and Atomic Orbitals

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Vocabulary practice flashcards covering quantum numbers, orbital shapes and capacities, atomic models, and electron energy level transitions.

16 Terms

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Heisenberg Uncertainty Principle

The quantum mechanical principle stating that one can never simultaneously know both the exact position and velocity (or energy) of an electron.

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Orbital

A probability distribution map that represents the best guess of both the position and energy of an electron, indicating where it is most likely to be found.

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Principal Quantum Number (nn)

The quantum number that designates the principal energy level (PEL), describing the overall size and energy of any given orbital.

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Angular Momentum Quantum Number (ll)

The quantum number that describes the shape of an orbital, with allowed integer values ranging from 00 up to n−1n - 1.

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Magnetic Quantum Number (mlm_l)

The quantum number specifying the 3D spatial orientation of an orbital, with integer values ranging from −l-l to +l+l, including 00.

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Spin Quantum Number (msm_s)

A fundamental property of an electron designating its magnetic spin state, which can strictly take the value of either +12+\frac{1}{2} (spin up) or −12-\frac{1}{2} (spin down).

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Stern-Gerlach Experiment

A classic experiment that demonstrated the discrete magnetic spin of electrons by firing them between magnetic poles and observing deflection exclusively to the top (+12+\frac{1}{2}) or bottom (−12-\frac{1}{2}) with nothing in between.

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ss Orbital

A largely spherical orbital defined by l=0l = 0, having only 11 spatial orientation (ml=0m_l = 0) and accommodating a maximum of 22 electrons.

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pp Orbital

A dumbbell-shaped orbital defined by l=1l = 1, possessing 33 distinct orientations (pxp_x, pyp_y, and pzp_z) and capable of holding up to 66 electrons.

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dd Orbital

A largely four-leaf clover-shaped orbital defined by l=2l = 2, possessing 55 distinct spatial orientations and capable of holding up to 1010 electrons.

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ff Orbital

A multi-lobed orbital defined by l=3l = 3, possessing 77 distinct orientations and capable of accommodating up to 1414 electrons (represented by the lanthanide and actinide blocks).

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PEL

An acronym used in lecture referring to the Principal Energy Level, directly designated by the quantum number nn.

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Electron Mass

A physical constant and property of an electron, given as 9.11×10−31 kg9.11 \times 10^{-31}\,\text{kg}.

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Rydberg's Constant (in Atomic Transitions)

The proportionality constant given as −2.18×10−18 J-2.18 \times 10^{-18}\,\text{J}, used to calculate energy changes during atomic electron transitions via ΔE=−2.18×10−18 J(1nf2−1ni2)\Delta E = -2.18 \times 10^{-18}\,\text{J} \left(\frac{1}{n_f^2} - \frac{1}{n_i^2}\right).

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Photon Energy Equation

The relationship used to calculate the energy of an emitted photon from its wavelength: E=hcλE = \frac{h c}{\lambda}, where energy gained by the photon equals the energy lost by the relaxing atom.

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Hydrogen Emission Line (n=3→n=2n = 3 \rightarrow n = 2)

The electronic transition in hydrogen where an electron falls from the third to the second principal energy level, emitting a photon with a wavelength of 656 nm656\,\text{nm}.