Because of it's initial high temperature it is not even on the diagram, but far off to the left of the diagram.
On the main sequence.
The Hertzsprung-Russell (HR) diagram is based on plotting a star's luminosity against its temperature or spectral type. This diagram helps astronomers classify stars based on their evolutionary stage and enables them to study relationships between a star's properties such as temperature, luminosity, and size.
A supernova is a star saying "The End". The H-R diagram shows they different types of stars by spectral class, color, etc. It was never intended to show the ending of stars. On most H-R diagrams, you will find at the top, or occasionally top right, a place for "Supergiants". Some of those stars will eventually become supernovas. To be absolutely clear: A supernova isn't a type of star - it is the "end" of a type of star.
I don't know ok
Neutron stars are extremely dense remnants of massive stars that have undergone supernova explosions, and they typically possess strong magnetic fields and rapid rotation. The Hertzsprung-Russell (HR) diagram primarily charts stars based on their luminosity and temperature, focusing on the main sequence, giants, and white dwarfs. Neutron stars are not in thermal equilibrium like those stars, as they emit energy primarily through processes like thermal radiation and magnetic field interactions rather than nuclear fusion, which is why they do not appear on the HR diagram. Instead, they are often represented separately in discussions of stellar evolution and compact objects.
A neutron star is not typically shown on the Hertzsprung-Russell diagram because it is a remnant of a massive star that has undergone a supernova explosion. Neutron stars are extremely dense and have unique properties that do not fit neatly into the categories represented on the diagram.
HR diagram
On the main sequence.
You need to know the luminosity and temperature of star in order to plot it on the HR diagram.
evolving into a later stage. For example, a G2 star going into a red giant (M type)
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.
White dwarfs.
stars there called stars
White dwarfs.
stars there called stars
The Hertzsprung-Russell (HR) diagram is based on plotting a star's luminosity against its temperature or spectral type. This diagram helps astronomers classify stars based on their evolutionary stage and enables them to study relationships between a star's properties such as temperature, luminosity, and size.
The Hertzsprung-Russel diagram shows brightness versus color (the color reflects the star's temperature).