Main sequence stars.
The main sequence.
In terms of absolute magnitude, a larger hotter star will necessarily be more luminous than a smaller cooler star. However, if a smaller cooler star is much closer to us than a larger hotter star, it may appear to be brighter. None of this has anything to do with the HR diagram.
main sequence
Each planets has a different length of time it takes to make a full rotation. The approximate lengths are: Mercury: 58 days, Venus: 243 days, Earth: 24 hours, Mars: 24 hours, Jupiter: 10 hours, Saturn: 11 hours, Uranus: 17 hours and Neptune: 16 hours.
You cannot convert kilograms per hour (kg/hr) into nanometers cubed per hour (nm3/hr). The kilogram is a measure of mass or weight while the cubic nanometer is a measure of volume. There is no direct conversion, unless you specify the density of the material involved.
110 mph is equal 177.028 km/hr.
The HR diagram contains only stars - so everywhere.
Of course they are on the HR diagram. They are simply not on the main sequence.
All stars.
main-sequence stars
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.
stars there called stars
stars there called stars
The red dwarves.
Main sequence
They are very hot stars.
The HR diagram does not reference stars on their way to the main sequence, only during or after.
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.