When the mass exceeds the Chandrasekhar limit.
It becomes a white dwarf.
a few tons.
WHITE DWARF ;p
in lamen's terms probably.A supernova Type Ia occurs between two companion stars usually a large star and small companion white dwarf. What happens is that the dwarf star accretes (takes away) stellar material from the larger star. After this happens for a long time the amount of material becomes more and more dense (the star will actually become smaller in radius) and hotter and hotter until the conditions are correct for a fusion reaction to occur. The process is much more complicated than my explanation, but basically after fusion occurs...boom.
A white dwarf is what stars like the Sun become after they have exhausted their nuclear fuel. Near the end of its nuclear burning stage, this type of star expels most of its outer material, creating a planetary nebula. Only the hot core of the star remains. This core becomes a very hot white dwarf, with a temperature exceeding 100,000 kelvin.
white dwarf
white dwarf/nova
white dwarf
It becomes a white dwarf.
a red giant
A brown dwarf.A brown dwarf.A brown dwarf.A brown dwarf.
a few tons.
WHITE DWARF ;p
in lamen's terms probably.A supernova Type Ia occurs between two companion stars usually a large star and small companion white dwarf. What happens is that the dwarf star accretes (takes away) stellar material from the larger star. After this happens for a long time the amount of material becomes more and more dense (the star will actually become smaller in radius) and hotter and hotter until the conditions are correct for a fusion reaction to occur. The process is much more complicated than my explanation, but basically after fusion occurs...boom.
millions of times grater
A teaspoon (5ml) of white dwarf material would weigh about 6,500,000 grams or just over 7 metric tons.
About 907 Kilograms