In accordance with their mass.
More massive stars by default are bluer and burn more quickly, go supernovae and can become a black hole or neutron star, depending on it's mass. Less massive stars are redder, last longer because they don't burn their fuel as furiously and don't go supernovae and don't become really dense stars after their "shed" their outer layer like the bigger ones do.
There is even a category of 'failed stars', which is when a gas giant didn't get big enough to to activate nuclear fusion in its core. Jupiter is in this category. If it had been a bit bigger, it would have been another sun.
Stars can be described by their temperature, size (diameter), brightness (luminosity), color, composition, and age. These characteristics help scientists classify and study stars in the universe.
Hertzsprung-Russell diagram. This diagram plots a star's luminosity against its temperature (or color), allowing scientists to classify stars by size, brightness, and lifecycle stage.
Scientists classify stars based on several key characteristics, including their temperature, luminosity, size, and spectral type, which is determined by the absorption lines in their spectrum. The Hertzsprung-Russell diagram is a common tool used to visualize the relationship between a star's luminosity and temperature, allowing for further categorization into groups such as main sequence stars, giants, and white dwarfs. Additionally, the chemical composition of a star can also influence its classification.
Stars are classified by four different characteristics. Apparent magnitude (brightness) and absolute magnitude (how bright it would appear at 10 parsecs from the earth). Luminosity, another measure of brightness, compares the star to the sun's brightness. Spectral classifications are measured by the star's temperatures. Finally stars are signed a number by scientists through the Morgan-Keenan System.
In Astronomy stars can be classified by theircolor (temperature)composition (as found by their spectrum)agelocation in a galaxymassproximity to other stars
Scientists use color, size, brightness, and temperature to classify stars.
Scientists classify stars by size based on their mass. Stars can be categorized as dwarf stars (like our Sun), giant stars, or supergiant stars, with the size increasing as the mass of the star increases. The classification can also include specific categories such as red dwarfs, white dwarfs, or blue giants, depending on additional characteristics.
Stars can be described by their temperature, size (diameter), brightness (luminosity), color, composition, and age. These characteristics help scientists classify and study stars in the universe.
scientists classify Mount Kilauea as a shield volcano
Astronomers classify stars.
Hertzsprung-Russell diagram. This diagram plots a star's luminosity against its temperature (or color), allowing scientists to classify stars by size, brightness, and lifecycle stage.
Scientists classify vertebrate into different groups by the way the animal looks or how big or small it is
Scientists classify silicon as a metalloid, which is an element that exhibits properties of both metals and non-metals.
Scientists classify stars based on several key characteristics, including their temperature, luminosity, size, and spectral type, which is determined by the absorption lines in their spectrum. The Hertzsprung-Russell diagram is a common tool used to visualize the relationship between a star's luminosity and temperature, allowing for further categorization into groups such as main sequence stars, giants, and white dwarfs. Additionally, the chemical composition of a star can also influence its classification.
By looking at the water to find the classify
conragationistsories
Yes