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Absorption of Light definitions
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Absorption
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Absorption
Process where energy is taken in, causing an electron or atom to move to a higher energy state, often resulting in black bands on a colored spectrum.
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Atomic Emission
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Terms in this set (15)
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Absorption
Process where energy is taken in, causing an electron or atom to move to a higher energy state, often resulting in black bands on a colored spectrum.
Emission
Release of previously absorbed energy as an electron or atom returns to a lower energy state, producing colored lines on a black spectrum.
Bohr Model
Atomic structure concept where electrons occupy discrete shells, with energy changes occurring during transitions between these shells.
Ground State
Lowest energy configuration of an electron or atom, from which excitation or emission transitions originate or terminate.
Excited State
Condition where an electron or atom possesses more energy than its lowest possible state, often after absorbing energy.
Emission Spectrum
Pattern of colored lines on a black background, unique to each element, resulting from energy released during electron transitions.
Absorption Spectrum
Pattern of black bands on a colored background, indicating specific frequencies absorbed as electrons move to higher energy states.
Lyman Series
Set of spectral lines in the ultraviolet region produced by electron transitions ending at the first shell.
Balmer Series
Set of visible light spectral lines resulting from electron transitions ending at the second shell.
Paschen Series
Group of infrared spectral lines produced by electron transitions ending at the third shell.
Brackett Series
Infrared spectral lines resulting from electron transitions ending at the fourth shell.
Humphrey Series
Spectral lines in the microwave region produced by electron transitions ending at the sixth shell.
Rydberg Constant
Physical constant used to calculate the potential energy of an electron in a shell, central to predicting spectral line positions.
Potential Energy
Energy associated with an electron's position in a shell, calculated using a formula involving the Rydberg constant and shell number.
Electromagnetic Spectrum
Range of all possible frequencies of electromagnetic radiation, including UV, visible, IR, and microwave regions relevant to atomic transitions.