OBAFGKM
The Sun is a as a G2V type star, a yellow dwarf and a main sequence star. Stars are classified by their spectra(the elements that they absorb) and their temperature. There are seven main types of stars. In order of decreasing temperature, O, B, A, F, G, K, and M
The spectral sequence of stars is not alphabetical because it is based on the temperature of the star, with O-type stars being the hottest and M-type stars being the coolest. The sequence was originally arranged in this manner by Annie Jump Cannon, a pioneering astronomer, in order to classify stars based on their spectral features.
To plot a star on the H-R diagram, you need the star's luminosity (or absolute magnitude) and its surface temperature (or spectral type). These two properties allow you to place the star accurately on the diagram based on its position relative to other stars.
The correct order of these stellar evolutionary stages is main sequence, red giant, white dwarf. A star begins its life on the main sequence where it fuses hydrogen into helium. As it runs out of fuel, it expands into a red giant before shedding its outer layers and collapsing into a white dwarf.
That's the sequence of the colors of light in order from longest to shortest wavelengths.
The Sun is a as a G2V type star, a yellow dwarf and a main sequence star. Stars are classified by their spectra(the elements that they absorb) and their temperature. There are seven main types of stars. In order of decreasing temperature, O, B, A, F, G, K, and M
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 spectral sequence of stars is not alphabetical because it is based on the temperature of the star, with O-type stars being the hottest and M-type stars being the coolest. The sequence was originally arranged in this manner by Annie Jump Cannon, a pioneering astronomer, in order to classify stars based on their spectral features.
If the temperature of the gas is decreasing, then in order to maintain constant pressure, you would have to compress it in volume.
The colors of visible light, in order of decreasing frequency, are violet, indigo, blue, green, yellow, orange, and red. Violet has the highest frequency, while red has the lowest. This sequence represents the visible spectrum, which is part of the electromagnetic spectrum.
Spectral class is the categorization of stars by temperature and size, mostly the former. Spectral class B is very hot. In descending order (hottest to coolest) the spectral classes are O,B,A,F,G,K,M. You can see that B is very near the top.
The HR diagram has the star's temperature along the horizontal axis and the absolute magnitude (brightness) along the vertical axis. Each star is represented by a single dot. Higher temperature is usually associated with more brightness so many stars lie on or near a line on the diagram called the Main Sequence. Red giant stars are found on the upper right hand quarter because they are relatively cool but still very bright.
The ranking of radicals in order of decreasing stability is as follows: benzyl allyl tertiary secondary primary methyl.
ORDER BY
the denotation of sequence is put in order
The reason main sequence has a limit at the lower end is because of temperature and pressure. The lower limit exists in order to exclude stellar objects that are not able to sustain hydrogen fusion.
Sequence of Events.