For the same real brightness, at a larger distance it would look less bright. On the other hand, you may have two stars that look like they are the same brightness, but one might be million times brighter (in real brightness) than the other - which would be compensated by the fact that the brighter star is a thousand times farther away.
The actual brightness of stars, known as their intrinsic luminosity, depends primarily on their temperature, size, and energy output. Hotter and larger stars emit more energy and therefore appear brighter. Additionally, the composition of a star, including its age and the presence of elements, can also influence its luminosity. Ultimately, a star's brightness is a combination of these factors, along with its distance from Earth, which affects how we perceive its brightness from our vantage point.
The brightness of a star as observed from Earth decreases with distance due to the inverse square law, meaning that as the distance doubles, the observed brightness is reduced to a quarter. Additionally, a star's apparent size, or angular diameter, diminishes with increased distance, making it appear smaller even though its actual size remains unchanged. Thus, a distant star can be much larger than a nearby star, but it may appear fainter and smaller due to the vast distance separating them.
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.
The distance on maps and actual distance on the ground depend on the scale of the maps if you chose 1 cm for one kilometer than it will be 9 kilometer on the ground.This is the simple understanding and dont be confuse with the calculation of cm. M.Saleem
Absolute magnitude is based on the distance at which a star would appear if it were located at a standard distance of 10 parsecs (32.6 light-years) from Earth. This standardized distance allows astronomers to compare the true brightness of stars regardless of their actual distance from Earth.
It's distance from Earth and the star's actual brightness
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.
Distance from Earth.
The brightness as seen from Earth is called the "apparent magnitude".The real brightness (defined as the apparent brightness, as seen from a standard distance) is called the "absolute magnitude".
Scientists use the brightness of the object to determine its distance in space. By measuring how bright an object appears from Earth and comparing it to its actual brightness, they can calculate its distance based on the inverse square law of light.
Actual Mech. Advantage
No. Brighter distant stars can have the same apparent magnitude as fainter stars that are closer.(Absolute magnitude does not refer to actual brightness, but rather to what the brightness of a star would likely be at an arbitrary distance of 10 parsecs, rather than its actual distance.)
That refers to its actual brightness, not to how we see it. The apparent brightness depends on the real ("absolute") brightness, but also on the distance.
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.
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
A standard candle is an object in space with a known brightness. By comparing the actual brightness of a standard candle to how bright it appears from Earth, astronomers can calculate the distance to that object. This method helps measure distances in astronomy by providing a consistent reference point for determining how far away celestial objects are.
The scale.