spectral line

Wavelength absorption signature

A spectral line is a distinct wavelength of light that appears as a bright or dark band in a spectrum.

When atoms emit or absorb energy, they do so at specific wavelengths characteristic of each element—hydrogen produces different lines than helium or sodium.

Bright emission lines indicate light being released; dark absorption lines show light being blocked.

Scientists use spectral lines to identify the chemical composition of stars, gases, and other materials from a distance.

atomic structure

energy level

Amount of vitality available

orbital · quantization · selection rules · energy gap · quantum jump · excitation · angular momentum · spin · hyperfine structure · degeneracy

emission

fluorescence

Light emitted after absorption

plasma · corona · radiance · atomic emission

astronomy

redshift

Wavelength stretch from recession

quasar · chromosphere

wavelength

nanometer

Metric unit, billion-fold smaller

ultraviolet

absorption

Fraunhofer lines

Dark spectral absorption features

absorbance · Beer-Lambert law · attenuation · molar absorptivity · analyte · concentration · filter

Opposites
spectral feature type

spectral linecontinuum

Uninterrupted, gradual sequence

white light

emission vs. absorption

spectral linebright line

Unambiguous legal boundary

Family

line, spectrum, linear, spectral, spectrometer, spectroscopy, spectrometry, spectrograph, spectroscopic

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