The seven fundamental stellar spectral types are O, B, A, F, G, K and M.
Also, what are their relationships to the stellar temperatures?
The most common spectral type of stars in the universe is M, which includes red dwarfs and red giants. These stars are relatively cool and dim compared to other spectral types like O, B, or A.
The fundamental paticles are Quarks , they are of 6 types.
A spectral signature is a unique pattern of electromagnetic energy emitted or reflected by a particular object. It is used in remote sensing to identify and distinguish different types of features on Earth's surface based on their characteristic spectral responses across different wavelengths of light.
Simple Prisms A hexagonal prism is the most basic snow crystal geometry (see the Snowflake Primer). Depending on how fast the different facets grow, snow crystal prisms can appear as thin hexagonal plates, slender hexagonal columns (shaped a lot like wooden pencils), or anything in between. Simple prisms are usually so small they can barely be seen with the naked eye.
Spectral lines tell us how many different energy levels an atom has, and how far apart those energy levels are spaced. This is possible because spectral lines are the result of an excess (emission lines) or deficiency (absorption lines) of observed photons emitted from certain types of matter. The lines are caused by electrons moving between energy levels within individual atoms. Since each element emits it's own unique spectrum, this means that different types of atoms must have a distinct number of electrons in very particular energy levels.
not enough info
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 seven classifications of snowflakes are plate, stellar dendrite, column, needle, capped column, spatial dendrite, and irregular snowflakes. Each classification is based on the shape and structure of the snowflake as it forms.
stellar, supermassive, miniature
Stars can be classified into different spectral types based on their color, which is related to their surface temperature. The classification system uses the letters O, B, A, F, G, K, and M to represent the range of temperatures from hottest (blue/white) to coolest (red). This sequence is known as the spectral sequence or spectral types.
The most common spectral type of stars in the universe is M, which includes red dwarfs and red giants. These stars are relatively cool and dim compared to other spectral types like O, B, or A.
The fundamental paticles are Quarks , they are of 6 types.
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.
The spectral type of a star measures its temperature and determines its color, luminosity, and size. It is determined by the characteristics of the star's spectrum, such as the absorption lines caused by elements in its atmosphere. Astronomers use spectral types to classify stars based on their physical properties.
Assuming by "fundamental" you mean the primitive data types: boolean, byte, char, short, int, long, float, and double
When different spectral colors are mixed together, it is called color mixing. This can result in intermediate colors being produced, depending on the proportions and types of colors being combined.
Three types of snowflake shapes are stellar dendrites, sectored plates, and hollow columns. While stellar dendrites appear tree-like, hollow columns are hexagonal tube-like structures. There can be other shapes like needles and spatial dendrites.