There are two factors in "apparent magnitude", or, how bright a star appears to be. These are absolute magnitude, how bright the star really is, and distance. Very bright stars will seem to be bright even when they are a long distance away.
On the other hand, the closest star to the Sun is the red dwarf Proxima Centauri, which is invisibly dim, EVEN THOUGH it is the nearest star. It's a tiny red dwarf.
The apparent brightness of a star is determined by its luminosity (true brightness), distance from Earth, and any intervening dust or gas that may absorb or scatter its light. These factors affect how bright a star appears in the night sky to an observer on Earth.
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.
A nova is a star that suddenly increases in brightness.
Stellar brightness refers to the amount of light emitted by a star as perceived from Earth, often quantified in terms of apparent magnitude and absolute magnitude. Apparent magnitude measures how bright a star appears from our viewpoint, while absolute magnitude represents its intrinsic brightness at a standard distance of 10 parsecs. Factors such as distance, size, temperature, and composition influence a star's brightness. Understanding stellar brightness helps astronomers categorize stars and study their properties and distances.
The brightness of a star as observed from Earth is known as its apparent magnitude. This measurement reflects how bright the star appears in the sky, which can be influenced by factors such as distance, size, and luminosity. In contrast, a star's intrinsic brightness, or true luminosity, is referred to as its absolute magnitude. These two concepts help astronomers understand both the distance to stars and their actual energy output.
Composition and distance.
distance from the sun and the age of the star
The apparent brightness of a star is determined by its luminosity (true brightness), distance from Earth, and any intervening dust or gas that may absorb or scatter its light. These factors affect how bright a star appears in the night sky to an observer on Earth.
How dense it is, and how far away it is.
Two factors that affect a star's apparent brightness are: 1.) The distance between the Earth and the star 2.) The absolute magnitude (the actual brightness) of the star Hope that helps :P
Distance from Earth, size of star, and temperature of star.
Distance from Earth, size of star, and temperature of star.
Distance and intervenng or close celestial bodies
Distance and intervenng or close celestial bodies
Distance and intervenng or close celestial bodies
Distance and intervenng or close celestial bodies
Three physical factors that determine a star's brightness are its temperature (hotter stars are brighter), size (larger stars are generally brighter), and distance from Earth (the closer a star is, the brighter it appears).