Absolute magnitude.
Caution
If two stars have the same temperature, their luminosity is primarily determined by their size. According to the Stefan-Boltzmann law, luminosity increases with the fourth power of temperature and is also proportional to the surface area of the star. Therefore, if both stars have the same temperature but differ in size, the larger star will have a greater luminosity. If they are identical in size and temperature, they will have the same luminosity.
The star that is hotter will have a higher luminosity.
The star that is hotter will have a higher luminosity.
The luminosity depends on what stage of its life cycle the star is in. Also, the apparent luminosity depends on the distance from earth.
No. Apparent magnitude (or luminosity) means how bright a star (or other object) looks to us; absolute magnitude (or luminosity) refers to how bright it really is.
A star's luminosity is related to its radius and temperature through the Stefan-Boltzmann law, which states that luminosity (L) is proportional to the square of the radius (R) multiplied by the fourth power of its surface temperature (T): (L \propto R^2 T^4). This means that for two stars of the same temperature, a larger radius results in significantly greater luminosity. Conversely, for stars of similar size, a higher temperature will lead to increased luminosity. Thus, both radius and temperature are crucial in determining a star's luminosity.
The luminosity of the star would decrease by a factor of four. Luminosity is directly proportional to the inverse square of the distance from the star. So, if the distance is doubled, the luminosity decreases by a factor of 2^2 = 4.
It is a triple star system. Therefore every single star has different luminosity. However, as a whole the system is seen from earth at an appereant magnitude of 3.47, which means only %6 luminosity of the star vega.
Both the absorption and the luminosity of a blackbody in equilibrium increase in magnitude with increasing temperature, and the spectral distribution of the luminosity increases in frequency (decreases in wavelength).
Luminosity affects the habitable zone (CHZ) by determining the distance at which a planet would need to be from a star to have the right temperature for liquid water to exist on its surface. Stars with higher luminosity would have habitable zones farther out, while stars with lower luminosity would have habitable zones closer in. This means that the size and location of the CHZ around a star depend on its luminosity.
I was enthralled by the luminosity of the deep water jellyfish.