High mass stars have a faster rate of burning compared to low mass stars. This is because high mass stars have more gravitational pressure in their cores, leading to faster nuclear reactions and higher energy output. This results in a shorter lifespan for high mass stars compared to low mass stars.
A low-mass protostar is a young star in the early stages of formation that has a relatively low mass compared to other stars. It is in the process of accumulating material from a surrounding gas and dust cloud and undergoing gravitational collapse to eventually ignite nuclear fusion in its core. These stars typically have lower luminosity and longer formation times compared to high-mass protostars.
High compared to hydrogen and helium, low compared to lead, gold and uranium.
High-mass stars might become black holes, if the remaining matter (after the supernova explosion) is sufficiently large.
The similarities of high-end low-mass stars include their ability to fuse hydrogen and helium at the same time, very short lifetimes, and being incredibly luminous.
High mass stars have a faster rate of burning compared to low mass stars. This is because high mass stars have more gravitational pressure in their cores, leading to faster nuclear reactions and higher energy output. This results in a shorter lifespan for high mass stars compared to low mass stars.
Low and high mass stars are indirectly related; high mass stars evolve faster and have shorter lifespans compared to low mass stars. This is because high mass stars burn through their fuel at a faster rate due to their higher core temperature and pressure.
They produce light.
In a newly formed star cluster stars with low masses must greaty out number stars with high masses. High mass stars are rare and low mass stars are extremely common.
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.
A low-mass protostar is a young star in the early stages of formation that has a relatively low mass compared to other stars. It is in the process of accumulating material from a surrounding gas and dust cloud and undergoing gravitational collapse to eventually ignite nuclear fusion in its core. These stars typically have lower luminosity and longer formation times compared to high-mass protostars.
High compared to hydrogen and helium, low compared to lead, gold and uranium.
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.
Altair is classified as an A-type main-sequence star, which means it is relatively high-mass compared to other stars like the Sun. Its mass is estimated to be about 1.8 times that of the Sun.
high mass has shortest life (stars right?)
There are three types of stellar remnants. Low to medium mass stars will become white dwarfs. High mass stars will become neutron stars. Very high mass stars will become black holes.
High volume and low mass result in low density because density is calculated by dividing mass by volume. When the mass is low compared to the volume, the density will also be low because there is less mass per unit of volume.