spectral type

American  

noun

Astronomy.

1. a category for classifying a star, as A star or G star, according to features of its spectrum, as its shape as a function of temperature and wavelength and its absorption spectrum, that indicate the surface temperature of the star and the presence of particular atoms or molecules in its outer layers: principal types are spectral types O, B, A, F, G, K, and M.

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spectral type British  

noun

1. any of various groups into which stars are classified according to characteristic spectral lines and bands. The most important classification ( Harvard classification ) has a series of classes O, B, A, F, G, K, M, the series also being a scale of diminishing surface temperature

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spectral type Scientific  

1. A classification system for stars based on the strength of their spectral lines, using the letters O, B, A, F, G, K, M, L, and T to denote a range from blue (as in blue giant stars) to dim red (as in brown dwarfs). The spectrum of a star correlates with its surface temperature, ranging from over 60,000°K (O type) to less than 3,500°K (L and T types).

2. See also Hertzsprung-Russell diagram

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Etymology

Origin of spectral type

First recorded in 1920–25

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Example Sentences

See Examples For:

spectral type

Once astronomers take a spectrum of a nearby star for which we also know the parallax, we know the luminosity that corresponds to that spectral type.

From Textbooks ● Oct. 13, 2016

Look up the spectral type of Antares in Appendix J. Was your estimate of the temperature about right?

From Textbooks ● Oct. 13, 2016

Measure the spectrum and get the spectral type.

From Textbooks ● Oct. 13, 2016

To seek the Milky Way’s farthest-flung residents Bochanski's team started with nearly seven million stars, using near-infrared data to select those whose colors match spectral type M, which designates stars that are cool and red.

From Scientific American ● Aug. 11, 2014

We have already shown how the angular diameters subtended by many of the stars have been estimated, through the relation of surface brightness and spectral type.

From Astronomy: The Science of the Heavenly Bodies by David Peck Todd

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