Main Sequence blue giants such as Rigel are located on the left-hand side of the H-R diagram. The order is O B A F G K M, and these are spectral classes based on color and temperature. The hottest stars burn blue/white because blue light has the shortest wavelengths and the highest temperatures. Moderate stars like our sun, a type G star, are found in the center of the Main Sequence, and red dwarf stars are found on the right-hand end, in the K and M classes.
Hot blue stars are found in younger parts of galaxies.
There are no blue stars in our Solar System, only one yellow star - the Sun
There are lots of bluish stars. We don't know which one you mean. One guess would be Rigel.
i don't know about the hr diagram but the brightest star known is r136a1
Our Sun is a G2V star and will thus appear in the centre of the HR diagram.
You need to know the luminosity and temperature of star in order to plot it on the HR diagram.
As the HR diagram shows, the hottest stars on the main sequence range from 30,000K as blue-white stars to about 3,000K as redish stars.
stars there called stars
i don't know about the hr diagram but the brightest star known is r136a1
The main reason that the HR Diagram is so useful and important to scientists is, you can tell the size of the star by plotting it on the HR Diagram. The different sizes of stars form a pattern on the HR diagram.
HR diagram
The most massive type of main sequence star on the HR diagram would be indicated by the main sequence area at the top left of the HR diagram, which would be blue or violet in color. Zeta Puppis is an example of such a star. It comes in at 40 solar masses. It is classified as a type "O" star.
On the main sequence.
As the HR diagram shows, the hottest stars on the main sequence range from 30,000K as blue-white stars to about 3,000K as redish stars.
You need to know the luminosity and temperature of star in order to plot it on the HR diagram.
You need to know the luminosity and temperature of star in order to plot it on the HR diagram.
Our Sun is a G2V star and will thus appear in the centre of the HR diagram.
its located somewhere
As the HR diagram shows, the hottest stars on the main sequence range from 30,000K as blue-white stars to about 3,000K as redish stars.
Based on initial size and chemical composition a star will enter a band on the HR diagram as a mains sequence star. Stars on the main sequence are in equilibrium from thermal pressure trying to enlarge the star and gravitational pressure trying to collapse the star. Stars on the main sequence range from massive hot blue-white stars to much less massive red stars.