On the main sequence, red dwarfs and orange dwarfs are less bright than the sun. Our sun is a yellow dwarf.
Matar is a yellow bright giant star in the constellation Pegasus.
Theta Scorpii (Sargas) is a star in the southern zodiac constellation of Scorpius.It has a spectral type of F0, so it is a white (F-type) bright giant.
an o-type blue star has a less length life than a g-type sun like star, this is because a the larger, hotter star, (the o-type blue star) uses its fuel (converting hydrogen into oxygen) quicker, so the correct answer to your question is the o-type blue star.
The star Algenubi, or Epsilon Leonis, is a 162 million year old star, classified as a bright giant. The star is around four times the size of our sun.
Mu Sagittarii (Polis) is a multi star system. It's brightest component is a B-type star and thus appears as a bright blue-white star in the sky.
Matar is a yellow bright giant star in the constellation Pegasus.
If you mean after a supernova it could be a neutron star if it's less than 3 solar masses
A bright giant is a class of star that don't quite make it into the supergiant class but are much more luminous than giants.Eg. Epsilon Canis Majoris (Adhara): a blue-white (B-type) bright giant
Theta Scorpii (Sargas) is a star in the southern zodiac constellation of Scorpius.It has a spectral type of F0, so it is a white (F-type) bright giant.
Achernar is a bright, blue, B3-type star of six to eight solar masses lying
Algol (Demon Star) is a bright star in the constellation Perseus.Algol is actually a triple star system - Beta Persei A, B, and CBeta Persei A has a spectral type of B8 and is a blue-white giantBeta Persei B has a spectral type of K0 and is an orange subgiantSee related link for more information.
an o-type blue star has a less length life than a g-type sun like star, this is because a the larger, hotter star, (the o-type blue star) uses its fuel (converting hydrogen into oxygen) quicker, so the correct answer to your question is the o-type blue star.
It is the brightest type of star, Red Supergiant.
When a star begins to burn out, there are two things that can happen to it. If the star is equal or less than the mass of 3 times our Sun, it will collapse into a neutron star. Any larger, and it will become a black hole.
Sadatoni, also known as Zeta Aurigae, is a binary star . So, one star is a bright giant or a supergiant. It's companion is a main-sequence star.
The star Algenubi, or Epsilon Leonis, is a 162 million year old star, classified as a bright giant. The star is around four times the size of our sun.
They are very brittle and they can get up to a very bright temperature