giant
When compared to the other stars, the Red Giant Star are very minute. There are other stars that are very large by far as compared to the Red giant stars.
Giant stars are commonly referred to as "giant" stars because of their large size compared to main sequence stars like the Sun. These stars are in a later stage of their evolution and have expanded in size due to the depletion of their core's hydrogen fuel.
Stars in their giant and supergiant stages are located in the top right portion of the Hertzsprung-Russell diagram, also known as the "red giant branch." These stars are characterized by being large and cool compared to main sequence stars, and they represent later stages in stellar evolution.
Red giants. By the way, what if it was a white star.
The red giant galaxies are large non-main sequence star of stellar classification. These are classified K or M because of the reddish appearance of the cooler giant stars.
Giant Dwarves are old stars.
Those may be stars, or giant planets (like Jupiter, Saturn, Uranus, Neptune).Those may be stars, or giant planets (like Jupiter, Saturn, Uranus, Neptune).Those may be stars, or giant planets (like Jupiter, Saturn, Uranus, Neptune).Those may be stars, or giant planets (like Jupiter, Saturn, Uranus, Neptune).
An average giant galaxy contains a trillion or more stars.
The two types of stars that do not fall into the main sequence of an H-R diagram are white dwarfs and giant stars. White dwarfs are small, hot stars that have exhausted their nuclear fuel, while giant stars are large, luminous stars that have evolved off the main sequence due to changes in their internal structure.
The fate of an old star depends on its mass. Small stars will burn, essentially, forever. Medium mass stars like our Sun will eventually expand into a red giant, and collapse into a white dwarf. Very large stars will explode as supernova stars; these end up as neutron stars or if their initial mass is large enough, as black holes.
The five main groups of stars are main sequence stars, giant stars, supergiant stars, white dwarf stars, and neutron stars. These groups are classified based on their size, temperature, and stage in their life cycle.
A giant cluster refers to a large grouping of stars, typically containing thousands to millions of stars tightly bound together by gravity. These clusters are often found in galaxies and can be classified as globular clusters or open clusters based on their age, size, and distribution of stars. Giant clusters can provide valuable information about the formation and evolution of galaxies.