It may be just about anything. The apparent magnitude tells us how bright the star looks to us, not how bright it really is. The apparent magnitude (or brightness) depends both on the absolute magnitude (real brightness), but also depends on the star's distance.
Gamma Hydrae is a third magnitude star in the constellation Hydra.It has a spectral type of G8 which means it is a yellow giant falling off the main sequence.
Main sequence stars are located on the H-R diagram based on their luminosity or absolute magnitude verses their spectral class and effective temperature.
Gamma Leonis (Algieba) is a binary star system in the constellation Leo.The brightest star has a spectral type of K0 and it is a orange giant star with an apparent colour of orange-yellow.The secondary star has a spectral type of G7, so it is a yellow giant star with an apparent colour of yellow-orange.Both stars are no longer on the main sequence.
Our sun is a yellow main sequence star of spectral type G2 V
G2V; can be interpreted as yellow two tenths towards orange main sequence star
The apparent magnitude depends on distance, and without that information, it's literally impossible to tell what it might be.
The apparent magnitude od the main star in the Polaris system is 1.98
Gamma Hydrae is a third magnitude star in the constellation Hydra.It has a spectral type of G8 which means it is a yellow giant falling off the main sequence.
Main sequence stars are located on the H-R diagram based on their luminosity or absolute magnitude verses their spectral class and effective temperature.
If they are converting hydrogen to helium, then they are on the main sequence. This can be confirmed with a spectral analysis
Gamma Leonis (Algieba) is a binary star system in the constellation Leo.The brightest star has a spectral type of K0 and it is a orange giant star with an apparent colour of orange-yellow.The secondary star has a spectral type of G7, so it is a yellow giant star with an apparent colour of yellow-orange.Both stars are no longer on the main sequence.
Gamma Leonis (Algieba) is a binary star system in the constellation Leo.The brightest star has a spectral type of K0 and it is a orange giant star with an apparent colour of orange-yellow.The secondary star has a spectral type of G7, so it is a yellow giant star with an apparent colour of yellow-orange.Both stars are no longer on the main sequence.
The Sun is a yellow main sequence star of type G2 V.
Our sun is a yellow main sequence star of spectral type G2 V
G2V; can be interpreted as yellow two tenths towards orange main sequence star
A main sequence star with a spectral calss of G2V or yellow dwarf.
The three brightest stars in Leo the Lion are : Alpha Leonis or Regulus (the Lion's heart) with an apparent magnitude of 1.35, Beta Leonis or Denebola (the Lion's tail) with an apparent magnitude of 2.14 and Gamma Leonis or Algieba (where the Lion's mane meets his body) with an apparent magnitude of 1.98 Hope that helps!