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Here, the peak is either at the edge of red or in the infrared, and clearly the star emits more red light than other colors) But if the spectrum also contains helium lines, then it is a b star, whereas if it contains lines of ionized iron and other metals, it must be a g star. Once again, we know from the colors of these stars that the blue star is hotter than the yellow star, because its apparent color indicates that the peak of its emission is in the blue, while the other star’s peak is in the yellow part of the spectrum.

The classification sequence included 7 categories named with letters Looking at the lines in our figure, you see that the star could be either a b star or a g star The sequence is solely based on the progression of line patterns in the spectra (a

Given an absorption line spectrum for a specific star, you can be asked to identify a star of similar chemical composition

It is important to pay attention to the spacing between the lines to be able to correctly identify the most similar star to the given one. From hottest to coolest these categories are o, b, a, f, g, k, and m These categories are each divided into 10 numbered subclasses, so an astronomer might speak of an a7 star or an m3 star. The peak emission of their thermal radiation (the continuum peak in the spectrum above) comes at a wavelength determined by the star’s surface temperature — the hotter the star, the bluer the continuum peak.

Continuum emission is the overall trend of the spectrum In panel six, for example, the spectrum rises at the left of the graph, peaks between 4000 and 5000 angstroms, and slowly declines again. Look at the graph of the stellar spectrum The curve in this plot shows the intensity of light (increasing upward) at different wavelengths (increasing to the right).

The absorption spectrum of hydrogen shows the results of this interaction

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