Luminosity.
Their distance away from you and their intrinsic luminosity.
It really depends on the type of star, but for certain star types, there is a relationship between the period and the absolute brightness, so if the period is observed, the absolute brightness can be deduced. Yes. It seems like this question is about the Cepheid variables.
Anything that is not the measure of intrinsic brightness of a celestial object.
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 HR diagram compares the luminosity (brightness) of stars against their surface temperature or spectral type. This plot helps astronomers classify stars based on their intrinsic characteristics and evolutionary stages.
Their distance away from you and their intrinsic luminosity.
The brightness of a star to an observer on Earth is called it's Apparent Magnitude. The intrinsic brightness of a star is known as it's Absolute Magnitude.
The real brightness of a star is called its absolute magnitude. This is a measure of the star's intrinsic luminosity, or how bright it would appear if it were located at a standard distance of 10 parsecs (32.6 light-years) from Earth.
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.
It really depends on the type of star, but for certain star types, there is a relationship between the period and the absolute brightness, so if the period is observed, the absolute brightness can be deduced. Yes. It seems like this question is about the Cepheid variables.
the moon can vary its brightness and the pink elephant called aphadophalis
Anything that is not the measure of intrinsic brightness of a celestial object.
Variable stars are stars whose brightness changes over time due to intrinsic or extrinsic factors. Intrinsic variables, like Cepheid and Mira variables, undergo changes in their own properties, such as pulsations or eruptions. Extrinsic variables, such as eclipsing binaries, have their brightness altered by external factors, like one star passing in front of another. These stars are important for studying stellar processes and measuring distances in the universe.
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 size of stars depends on their mass and the stage of their life cycle. Constellations are just stars which happen to lie in the same general direction from Earth, and have nothing really to do with each other. Apparent brightess of a star or galaxy is the result of its intrinsic brightness and its distance from us.
The apparent brightness of stars is called "apparent magnitude", and it is written with a lowercase "m" after the number.
The HR diagram compares the luminosity (brightness) of stars against their surface temperature or spectral type. This plot helps astronomers classify stars based on their intrinsic characteristics and evolutionary stages.