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
The apparent brightness of stars is called "apparent magnitude", and it is written with a lowercase "m" after the number.
The apparent brightness of stars is called "apparent magnitude", and it is written with a lowercase "m" after the number.
Apparent magnitude is the brightness as observed from earth, while absolute magnitude is the brightness of a star at a set distance. The apparent magnitude considers the stars actual brightness as well as it's distance from us, but absolute magnitude takes the distance factor out so that star brightnesses can be directly compared.
A star's brightness at a standard distance is referred to as its apparent magnitude. This standard distance is 10 parsecs (32.6 light-years) from Earth. Apparent magnitude allows astronomers to compare the brightness of stars as seen from Earth, regardless of their actual distance from us.
The measure of a star's brightness is its magnitude. A star's brightness as it appears from Earth is called its Apparent Magnitude.Star's brightness is measured by there magnitude.
Apparent magnitude.
Apparent magnitude.
Apparent magnitude.
An astrometer is a device designed to measure the brightness, relation, or apparent magnitude of stars.
Brightness of stars (apparent and absolute magnitude) is measured by convention, taking an another star as a standard.
Both relate to brightness; both are measured in the same units; both are used for astronomical objects such as stars or galaxies.
The apparent magnitude of the Sun is listed as -26.74. I want to know what is the formula used to compute this? How is this figure of -26.74 arrived at? Can this formula be employed for calculating the apparent magnitudes of stars of different spectral types too?