Object Cards for the 13 Officially Listed Targets
In astronomy, stellar classification is the classification of stars based on their spectral characteristics. Electromagnetic radiation from the star is analyzed by splitting it with a prism or diffraction grating into a spectrum exhibiting the rainbow of colors interspersed with spectral lines. Each line indicates a particular chemical element or molecule, with the line strength indicating the abundance of that element. The strengths of the different spectral lines vary mainly due to the temperature of the photosphere, although in some cases there are true abundance differences. The spectral class of a star is a short code primarily summarizing the ionization state, giving an objective measure of the photosphere's temperature.
Figures (7)
Key Points
- Other modern stellar classification systems, such as the UBV system, are based on color indices—the measured differences in three or more color magnitudes.
- In the MK system, a luminosity class is added to the spectral class using Roman numerals.
- Spectroscopy is also used to study the physical properties of many other types of celestial objects such as planets, nebulae, galaxies, and active galactic nuclei.
- The Hertzsprung–Russell diagram, which the MK system is based on, is observational in nature so these remnants cannot easily be plotted on the diagram, or cannot be placed at all.
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Sources & licensing(4)
- Wikipedia contributors — en.wikipedia.org/wiki/Stellar_classification (Creative Commons Attribution-ShareAlike 4.0)
- Wikipedia contributors — en.wikipedia.org/wiki/Hertzsprung%E2%80%93Russell_diagram (Creative Commons Attribution-ShareAlike 4.0)
- Wikipedia contributors — en.wikipedia.org/wiki/Astronomical_spectroscopy (Creative Commons Attribution-ShareAlike 4.0)
- Wikipedia contributors — en.wikipedia.org/wiki/Distance_modulus (Creative Commons Attribution-ShareAlike 4.0)