A supernova.
supernova
A nova is a star that suddenly increases in brightness.
A star the size of our Sun or smaller is too small to become a "Nova", so we can expect that the original brightness of a "nova" star is probably brighter than the Sun; possibly a lot brighter.
The star that suddenly flares and then fades away is known as a "flaring star" or a "flare star". These stars experience temporary increases in brightness due to magnetic activity on their surfaces, before returning to their normal luminosity. This phenomenon is common in red dwarfs and other types of variable stars.
A star that temporarily increases its brightness by about 100,000 times is known as a nova. This phenomenon occurs when a white dwarf star in a binary system accumulates material from its companion star, leading to a thermonuclear explosion on its surface. This explosion causes a dramatic increase in brightness, which can last for days to weeks before gradually fading. Novae are distinct from supernovae, which involve the complete destruction of a star.
If the star is larger than about 5 times the size of our Sun, a black hole can form from the core of the exploded star
A nova is a star that suddenly increases in brightness.
A star the size of our Sun or smaller is too small to become a "Nova", so we can expect that the original brightness of a "nova" star is probably brighter than the Sun; possibly a lot brighter.
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.
The star that suddenly flares and then fades away is known as a "flaring star" or a "flare star". These stars experience temporary increases in brightness due to magnetic activity on their surfaces, before returning to their normal luminosity. This phenomenon is common in red dwarfs and other types of variable stars.
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".
A star that temporarily increases its brightness by about 100,000 times is known as a nova. This phenomenon occurs when a white dwarf star in a binary system accumulates material from its companion star, leading to a thermonuclear explosion on its surface. This explosion causes a dramatic increase in brightness, which can last for days to weeks before gradually fading. Novae are distinct from supernovae, which involve the complete destruction of a star.
There is no purpose of a star's brightness. They just exist and shine.
An apparent brightness is the brightness of a star as measured by an observer.
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.
If the star is larger than about 5 times the size of our Sun, a black hole can form from the core of the exploded star