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A spectral line is choose a fingerprint that deserve to be supplied to identify the atoms, elements or molecules current in a star, galaxy or cloud the interstellar gas. If we different the incoming irradiate from a celestial resource using a prism, we will frequently see a spectrum of colours crossed v discrete lines. Note that spectral currently can also occur in various other regions the the electromagnetic spectrum, return we can no longer use a prism to aid identify them.

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There room two species of spectral currently in the visible component of the electromagnetic spectrum:


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Emission lines are seen as coloured present on a black color background.
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Absorption present are viewed as black lines on a coloured background.

The existence of spectral currently is defined by quantum mechanics in terms of the energy levels of atoms, ions and molecules. These energy levels rely on the number of protons, electrons and also neutrons in an atom, and also the restricted set of construction in which these elemental particles have the right to exist (the set of quantum numbers). Atoms like to it is in in your ground state, where all of the electrons are situated as close come the nucleus together possible. Absorption lines take place when an atom, aspect or molecule absorbs a photon through an energy equal to the difference between two energy levels. This causes an electron to be advocated into a greater energy level, and the atom, facet or molecule is claimed to it is in in an excited state. Emission lines happen when the electron of one excited atom, facet or molecule move between energy levels, returning in the direction of the soil state.

The spectral currently of a certain element or molecule at remainder in a laboratory constantly occur in ~ the exact same wavelengths. Because that this reason, we room able to recognize which element or molecule is bring about the spectral lines. If the emitter or absorber is in motion, however, the place of the spectral lines will be Doppler shifted follow me the spectrum. A redshift (spectral lines move to longer wavelengths) occurs for an emitter/absorber relocating away from the observer, when a blueshift (spectral lines relocate to shorter wavelengths) corresponds to movement towards the observer.

Spectral present may additionally be broadended by:

Collisional Broadening: due to interactions with adjoining atoms, ion or moleculesZeeman Splitting: where energy levels are separation into sub-levels by a magnetic field.

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The apprehension Principle additionally provides a natural broadening of every spectral lines, v a organic width that Δν = ΔE/h ≈ 1/Δt whereby h is Planck’s constant, Δν is the broad of the line, ΔE is the corresponding spread in energy, and also t is the lifetime of the power state (typically ~10-8 seconds).