Sirius (brightest star in the night sky, 6th closest star to the sun, also a binary star)
Canis Majoris VY (largest star known to man)
Stars a yellow-ish orange for the majority of their lifetimes.
The majority of stars in our galaxy are red dwarfs, which are smaller and cooler than our sun. They make up about 70-80% of the stars in the Milky Way.
The majority of visible stars in the sky are main sequence stars, like our own Sun. These stars are in the stable phase of their life cycle where they are fusing hydrogen into helium in their cores.
Outside our (Milky Way) galaxy.
Correct. M-type stars on the main sequence are called red dwarfs.
Stars spend the majority of their life span in the main sequence phase, which is a stable period of nuclear fusion where they convert hydrogen into helium. This phase can last for billions of years for stars like the sun.
The great majority of stars are plotted along a diagonal band called the main sequence on an H-R diagram. This band represents stars that are fusing hydrogen into helium in their cores, where the varying luminosities and temperatures of stars are displayed.
You can fill that out with lots of verbs, for example, "the majority of stars shine". Here are some others:* The majority of stars are smaller than our Sun. * The majority of stars are main-sequence stars. That means that they fuse hydrogen-1, converting it into helium-4.
White dwarfs are the remnants of dead low to medium mass stars, which is the mass range of the majority of stars.
Rated 4 and a half stars
Most stars are plotted along the main sequence in the Hertzsprung-Russell (HR) diagram, which extends diagonally from the upper left (hot and luminous stars) to the lower right (cool and less luminous stars). This is because the majority of stars, including our Sun, spend the majority of their lives in the main sequence phase where they are fusing hydrogen into helium.
Actually, not all of them are white, but the vast majority of them are.