2006-06-22 17:43:38 · 6 answers · asked by Christopher P 1 in Science & Mathematics ➔ Astronomy & Space
The Chandrasekhar limit, is the maximum mass possible for a white dwarf (one of the end stages of stars when they cool down) and is approximately 3 × 1030 kg, around 1.44 times the mass of the Sun. This number is different in various articles, from 1.2 to 1.46 times the mass of the Sun and depends on the chemical composition of the star.
2006-06-22 17:49:03 · answer #1 · answered by alooo... 4 · 1⤊ 0⤋
The Chandrasekhar limit, is the maximum mass possible for a white dwarf (one of the end stages of stars when they cool down) and is approximately 3 Ã 1030 kg, around 1.44 times the mass of the Sun. This number is different in various articles, from 1.2 to 1.46 times the mass of the Sun and depends on the chemical composition of the star.
2006-06-23 02:36:57 · answer #2 · answered by Anonymous · 0⤊ 0⤋
The Chandrasekhar Limit designates the amount of mass of a star at which it will ultimately evolve into a white dwarf. If the mass is greater, it will evolve into a neutron star or if great enough possibly a singularity (black hole).
2006-06-28 07:45:06 · answer #3 · answered by quntmphys238 6 · 0⤊ 0⤋
Its the place in space where all the prayers of sports betters accumulate.
2006-06-23 00:50:49 · answer #4 · answered by mitchskram 3 · 0⤊ 0⤋
star
2006-06-23 11:49:05 · answer #5 · answered by Anonymous · 0⤊ 0⤋
you dont know even this much-shame on you
2006-06-23 03:30:29 · answer #6 · answered by the_zombie 2 · 0⤊ 0⤋