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.
A star's brightness as viewed by the unaided eye is measured using its apparent magnitude, which quantifies how bright a star appears from Earth. The scale is logarithmic, meaning a difference of 5 magnitudes corresponds to a brightness factor of 100. Stars with an apparent magnitude of around 6 or lower can typically be seen without telescopes, while brighter stars have lower magnitude values. For example, the brightest stars in the night sky, like Sirius, have apparent magnitudes of around -1.46.
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.