A red dwarf.
A decrease in a star's absolute brightness could be caused by the star moving farther away from Earth, interstellar dust blocking some of its light, or a decrease in the star's temperature. All of these factors would result in less light reaching Earth, causing a decrease in the star's apparent brightness.
No, the color of a star does not directly indicate its absolute distance. Star color is related to its surface temperature, and stars of different temperatures can be located at varying distances from Earth. The brightness of a star, as measured by its apparent magnitude, is more indicative of its distance.
Eta Carinae, with a mass 180 times that of the sun has a surface temperature of around 40,000 K. It is the hottest known star.
The luminosity of a star gives the most information about its physical nature. Luminosity is a measure of how much energy a star emits per unit of time and is directly related to its size, temperature, and distance. By knowing a star's luminosity, scientists can determine its mass, age, and evolutionary stage.
The absolute magnitude of a star depends on the size and temperature; a large cooler star can generate as much light as a small very hot star.
The absolute magnitude of a start will increase both:* If its surface temperature increases, and * If its diameter increases.
This star would be a white dwarf, as it has a high surface temperature of 20000 K but a low absolute magnitude of 10. White dwarfs are small, dense remnants of low to medium mass stars that have exhausted their nuclear fuel and collapsed.
the larger the mass of the star, the more luminous it is.
The star's mass determines the temperature in its core. A stars mass will also determined it size and the amount of gravitational pull it will have.
A star's color is determined by its surface temperature. This temperature is largely dependent on the star's initial mass.
The absolute magnitude of a main sequence star with a temperature of 25,000K would depend on its luminosity, which is not provided in the question. However, at this temperature range, the star would appear blue-white in color, as it falls within the blue-white region of the stellar temperature-color relationship.
A decrease in a star's absolute brightness could be caused by the star moving farther away from Earth, interstellar dust blocking some of its light, or a decrease in the star's temperature. All of these factors would result in less light reaching Earth, causing a decrease in the star's apparent brightness.
30,000-52,000 degrees, Kelvin
You can find the luminosity of a main sequence star by measuring its apparent brightness and distance from Earth. Knowing the distance allows you to calculate the star's absolute brightness. Luminosity is then determined by comparing the absolute brightness of the star to that of the Sun, which has a known luminosity.
The Hertzsprung-Russell diagram (H-R diagram) shows the relationship between absolute magnitude, luminosity, classification, and effective temperature of stars. The diagram as originally conceived displayed the spectral type (effectively the surface temperature) of stars on the horizontal axis and the absolute magnitude (their intrinsic brightness) on the vertical axis.
No, the color of a star does not directly indicate its absolute distance. Star color is related to its surface temperature, and stars of different temperatures can be located at varying distances from Earth. The brightness of a star, as measured by its apparent magnitude, is more indicative of its distance.
The color of a star is mainly related to the star's surface temperature. This is only remotely related to the star's mass; for example, high-mass stars can either be very hot (blue) or not-so-hot (red), depending on the phase in the star's life.