For a long times, it was considered to be VY Canis Majoris, but new studies have reduced its size. The present record is held by UY Scuti at 1708 times the diameter of the Sun. That works out to about 2,250,000,000km.
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
A stable star in the Hertzsprung-Russell (HR) diagram is one that is in hydrostatic equilibrium, where the gravitational forces pulling inward are balanced by the pressure from nuclear fusion reactions pushing outward. These stars typically reside in the main sequence region of the HR diagram, where they effectively fuse hydrogen into helium in their cores. Stability is characterized by a predictable luminosity and temperature, allowing for a steady lifecycle until they exhaust their nuclear fuel. As stars evolve, their position on the HR diagram changes, reflecting different stages of stability and energy production.
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
stars there called stars
White dwarfs.
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.
The Hertzsprung-Russel diagram shows brightness versus color (the color reflects the star's temperature).