Yes, No, O, Yus
above the main-sequence stars
The region of the Hertzsprung-Russell diagram with the most stars is the main sequence. This area, which stretches diagonally from the upper left (hot, luminous stars) to the lower right (cool, dim stars), contains about 90% of all stars, including our Sun. Main sequence stars primarily fuse hydrogen into helium in their cores, and this phase constitutes the longest stage in a star's life cycle.
Enjar Hertzsprung lived in 1873-1967 and Henry Russell lived in 1877-1957. They were scientists who worked separtely. They found the same answer about the temperature and color of stars. The diagram that they made is called the Hertzsprung-Russell diargram. It shows the connection between surface temperature and color.The discoverers of the famous Hertzsprung-Russel diagram (HR diagram), which turned out to be an important tool for the analysis of stars.
Mizar is a binary star system located in the constellation Ursa Major, primarily comprised of two stars: Mizar A and Mizar B. On the Hertzsprung-Russell diagram, Mizar A is classified as a spectral type A main-sequence star, specifically an A2V type, while Mizar B is a slightly smaller A-type star. Both stars fall into the category of the main sequence, where stars spend the majority of their lifetimes fusing hydrogen into helium. Their position on the diagram reflects their temperature, luminosity, and stage in stellar evolution.
The chart used to classify stars is called the Hertzsprung-Russell diagram (H-R diagram). This diagram plots stars based on their luminosity and temperature, helping to illustrate their evolutionary stages. It reveals relationships between different types of stars, including main-sequence stars, giants, and white dwarfs.
That's short for Hertzsprung-Russel diagram. It is a diagram in which the total luminosity versus color (and therefore temperature) of many stars is plotted.
above the main-sequence stars
Absolute magnitude and surface temperature
This may refer to the main sequence - stars that are on the main curve in the Hertzsprung-Russel diagram. Those are basically the stars that use fusion to convert protium into helium-4.
Hertzsprung-Russell diagrams are also referred to by the abbreviation H-R diagram or HRD. The diagram was created circa 1910 by Ejnar Hertzsprung and Henry Norris Russell and represents a major step towards an understanding of stellar evolution or "the lives of stars".
The Hertzsprung-Russell (HR) diagram is a graph that shows the relationship between a star's magnitude (luminosity) and temperature. It plots stars based on their color (temperature) and brightness (magnitude), allowing astronomers to classify stars and understand their evolutionary stage.
The region of the Hertzsprung-Russell diagram with the most stars is the main sequence. This area, which stretches diagonally from the upper left (hot, luminous stars) to the lower right (cool, dim stars), contains about 90% of all stars, including our Sun. Main sequence stars primarily fuse hydrogen into helium in their cores, and this phase constitutes the longest stage in a star's life cycle.
The main sequence phase means that, if you plot an H-R (Hertzsprung-Russel) diagram, it is in the so-called "main sequence", the area in the graph where you find the majority of stars. Those are the stars that currently fuse hydrogen into helium.
The Hertzsprung-Russel diagram shows brightness versus color (the color reflects the star's temperature).
see link below
The HR diagram contains only stars - so everywhere.
Austin is the first name of Chumlee in Pawn Stars.