Large mass starts are blue (when they are young) or Red (when they get old).
Stars can be considered count nouns when referring to individual celestial objects. However, when talking about the general concept of stars or a large group of stars collectively, it can be treated as a mass noun.
They produce light.
Stars come in different shapes, sizes, colors. This is due to the amount of spectra and temperature in each for classifying stars.Astronomers often use the Hertzsprung-Russell (H-R) Diagram plots stars color, temperature, luminosity, spectral type, and even evolutionary type.
High mass adult stars are classified as supergiants or giants, while low mass adult stars are classified as main sequence stars. This classification is based on the mass of the star and where it falls on the Hertzsprung-Russell diagram.
There are more low mass stars. this is for two reasons:- # the star forming process generates more low mass stars # High mass stars burn out very quickly and explode as supernovas and thus over time there are less and less of them.
Stars can range from blue to red depending on temperature and mass, with yellow stars in the middle and white stars on the back end of the spectrum.
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.
CARTER Payne
High-mass stars might become black holes, if the remaining matter (after the supernova explosion) is sufficiently large.
Neutron stars are so heavy because they are the compact core of a star that is 8 time the mass of our Sun. The most massive neutron stars possible are 3 times the mass of our Sun.
Gravitational pressure prevents stars of extremely large mass from forming as this pressure would likely initiate nuclear fusion earlier, preventing the star from accumulating enough mass to exceed the upper limit for star formation. This prevents the formation of supermassive stars and instead leads to the formation of smaller stars.
A star's "life cycle" depends mostly on its initial mass; everything is determined by mass. Small, low-mass stars may shine essentially forever, while very large high-mass stars may grow old and go supernova in only a few dozen million years.
Because there are many more small stars than large ones, our Sun turns out to be larger than about 60% of all other stars.
It's mass is not as large as some other stars, there was not as much hydrogen available in the local area when the solar system was formed. Stars with a higher mass have higher temperatures and pressures.
A star's color is determined by its surface temperature. This temperature is largely dependent on the star's initial mass.
A brown dwarf.
Kinetic energy is calculated as (1/2) x mass x speed squared, so to have a lot of kinetic energy, an object must have a large mass, a large speed, or both. Stars have tremendous amounts of kinetic energy, galaxies even more.Kinetic energy is calculated as (1/2) x mass x speed squared, so to have a lot of kinetic energy, an object must have a large mass, a large speed, or both. Stars have tremendous amounts of kinetic energy, galaxies even more.Kinetic energy is calculated as (1/2) x mass x speed squared, so to have a lot of kinetic energy, an object must have a large mass, a large speed, or both. Stars have tremendous amounts of kinetic energy, galaxies even more.Kinetic energy is calculated as (1/2) x mass x speed squared, so to have a lot of kinetic energy, an object must have a large mass, a large speed, or both. Stars have tremendous amounts of kinetic energy, galaxies even more.