A star who's brightness changes is called a variable star.
Examples are:
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A variable star is one whose brightness changes.
An apparent brightness is the brightness of a star as measured by an observer.
Its magnitude.
Theres `Absolute Magnitude` which is the brightness of a star at a set distance. Then there is `Apparent Magnitude` which is the apparent brightness from earth, regardless of distance.
Brightness of stars (apparent and absolute magnitude) is measured by convention, taking an another star as a standard.
The magnitude of a star refers to its brightness.
A variable star is a star whose brightness as seen from Earth that fluctuates.
A decrease in the star's temperature
A variable star is a star whose brightness as seen from Earth that fluctuates.
A variable star is a star whose brightness as seen from Earth that fluctuates.
the brightness of a star
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.
photographs use to measure the brightness of a star
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".
Absolute Brightness: How bright a star appears at a certain distance. Apparent Brightness: The brightness of a star as seen from Earth.
Well, I got a couple that I can think of off the top of my head Venus - Planet Virgo - Constellation Variable Star - A star whose brightness changes periodically Van Allen Belts - Radiation/Groups of charged particles that surround the Earth
There is no purpose of a star's brightness. They just exist and shine.
brightness and temperature are both related because brightness is actually tempature. However the system has become more refined. Instead of just looking at the star and determining magnitude one or magnitude two, an astronomer measures the brightness of the star using a device called a photometer. The photometer counts the number of photons coming from the star. This photon count is then compared to the photon count from a star whose magnitude is known. An accurate magnitude can then be calculated.