The Sun is located on the main sequence of the H-R diagram, which is where stars like the Sun reside for most of their lifetime. It falls in the middle of the main sequence, representing a stable phase of hydrogen fusion in its core.
Of course they are on the HR diagram. They are simply not on the main sequence.
The red dwarves.
The sun is closer to Earth than any of the other stars. Light from the sun takes 8 minutes to reach Earth, but light from others stars take years to reach Earth. They both are giant balls of hot gas.
The colors of the HR Diagram are:BlueBlue-WhiteYellowOrangeRed-OrangeRed
The Sun is located on the main sequence of the H-R diagram, which is where stars like the Sun reside for most of their lifetime. It falls in the middle of the main sequence, representing a stable phase of hydrogen fusion in its core.
On the HR diagram the Sun's spectrum is of type G2 which makes it yellow.
Slightly to the right of centre on the main sequence. If you look on the Australian Telescope National facility website, their HR diagram shows the position of the sun.
The Sun is classified as a G-type main-sequence star (G dwarf) on the Hertzsprung-Russell (HR) diagram. It has a surface temperature of about 5,500 degrees Celsius and an absolute magnitude of approximately +4.83. On the HR diagram, the Sun is located in the middle of the main sequence, where it occupies a position indicative of its mass and luminosity relative to other stars.
Of course they are on the HR diagram. They are simply not on the main sequence.
The HR diagram contains only stars - so everywhere.
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.
Nebulae themselves are not directly plotted on the Hertzsprung-Russell (HR) diagram, which is a graphical representation of stars based on their luminosity and temperature. However, nebulae are often the regions where stars form, and the stars that emerge from these nebulae can be represented on the HR diagram. The HR diagram primarily focuses on the evolutionary stages of individual stars rather than the nebulae from which they originate.
HR diagram
The red dwarves.
Up at the top right. If you look on the Australian Telescope National facility website, their HR diagram shows this clearly.
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.