The sun is a low mass sequence star. It is classified as a G-type main-sequence star, which means it is in the middle of its stellar evolution and will remain stable for billions of years.
Eltanin, also known as Gamma Draconis, is classified as a giant star with a spectral type of M3 III. It is considered a low to intermediate mass star, having evolved off the main sequence after exhausting the hydrogen in its core. Its mass is estimated to be around 2-3 times that of the Sun, placing it in the low to intermediate mass range for stars.
High mass.
A low mass star will become a white dwarf star, eventually this will cool to become a black dwarf. A high mass star (at least 8 times the mass of our Sun) will form a neutron star or a black hole, after a supernova event.
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.
The sun is a low mass sequence star. It is classified as a G-type main-sequence star, which means it is in the middle of its stellar evolution and will remain stable for billions of years.
Eltanin, also known as Gamma Draconis, is classified as a giant star with a spectral type of M3 III. It is considered a low to intermediate mass star, having evolved off the main sequence after exhausting the hydrogen in its core. Its mass is estimated to be around 2-3 times that of the Sun, placing it in the low to intermediate mass range for stars.
High mass.
High mass.
A red gaint star is a luminous star of low or intermediate mass(0.5ms to 10ms). its
white dwarf
The Sun is a medium mass star in main sequence.
A low mass star will become a white dwarf star, eventually this will cool to become a black dwarf. A high mass star (at least 8 times the mass of our Sun) will form a neutron star or a black hole, after a supernova event.
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.
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.
Juvenile star is typically classified as a low mass star, as it is in the early stage of its life cycle. These stars have a mass similar to that of the Sun or less. They are characterized by their long lifespan and relatively stable nature.
a low mass protostar is the begining formation of a low mass star. a low mass protostar is formed by a nebula (stellar nursery), like a cloud in space, where all stares come from. the definition of protostar is: a collection of gas, and dust who`s gravitational pull is causing it to collapse on itself & form a star. a LOW MASS protostar just has a LOWER MASS then a HIGH MASS protostar. Your Welcome:)