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The seven fundamental stellar spectral types are O, B, A, F, G, K and M. Also, what are their relationships to the stellar temperatures?
Many people were involved in the current spectral classes.The person who first realised that the spectral sequence then categorised was in fact temperature, was Cecilia Payne.See related link for more information on her.
Astronomers use the patterns of lines observed in stellar spectra to sort stars into a spectral class. Because a star’s temperature determines which absorption lines are present in its spectrum, these spectral classes are a measure of its surface temperature. There are seven standard spectral classes.
Madalynne Braseltonstellar classification is the classification of stars based on their spectral characteristics
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The Hertzsprung-Russell diagram is a graphical representation of stars that plots their luminosity against their temperature or spectral class. It typically displays a broad range of stellar types, from hot, luminous stars in the upper left to cool, dim stars in the lower right. The diagram reveals important stellar relationships, such as the main sequence, where most stars, including the Sun, reside, as well as the positions of giants, supergiants, and white dwarfs. This tool is crucial for understanding stellar evolution and categorizing different types of stars in the universe.
Stellar classification is based on the analysis of light from stars. The temperature from the photosphere of the star effects the amount and types of ions and this is used classifying the star.
The most commonly used mnemonic for spectral classification is "Oh Be A Fine Girl/Guy, Kiss Me," which helps remember the sequence of spectral types: O, B, A, F, G, K, M. Each letter represents a class of stars, ordered by decreasing temperature and increasing wavelength. This mnemonic is particularly helpful for astronomy students and enthusiasts in recalling the order of stellar classifications.
The Russell diagram, also known as the Russell-Vogt diagram, is a graphical representation used in astrophysics to illustrate the relationship between a star's luminosity and its temperature (or spectral class). It typically features temperature on the horizontal axis and luminosity on the vertical axis, with stars plotted according to these characteristics. The diagram highlights different stellar groups, such as main-sequence stars, giants, and white dwarfs, providing insights into stellar evolution and classification.
The Sun is classified as a G-type main-sequence star (G dwarf) under the Harvard spectral classification system, specifically as G2V. This classification indicates that it has a surface temperature of approximately 5,500 degrees Celsius (about 5,800 Kelvin) and emits a yellowish light. The "G" signifies its color and temperature, while the "V" denotes its status as a main-sequence star, which is a stage in stellar evolution where it fuses hydrogen into helium in its core.
The purpose of stellar spectroscopy is to determine the chemical composition of stars, the temperature and some other characteristcs..
The four variables astronomers use to classify stars are temperature, luminosity, size or radius, and mass. By analyzing these properties, astronomers can determine a star's position on the Hertzsprung-Russell diagram and classify it into different spectral types and stages of stellar evolution.