Oh, the beauty of nature unfolding before our eyes! When a star with the same mass as our Sun reaches the end of its life, it will gracefully transform into a planetary nebula and leave behind a hot core called a white dwarf, glimmering softly amidst the cosmic symphony. Just like each happy little tree we paint, even in its final moments, it continues to...shine brightly in the vast universe.
When a supergiant star exhausts its nuclear fuel and dies, it may explode in a supernova event. Depending on its mass, the remnants can either collapse into a neutron star or form a black hole. The outcome is determined by the star's initial mass and the processes occurring during the supernova explosion.
Saturn has a mass roughly equal to 95 times the mass of Earth, so 318 Earths would be about 3.35 times the mass of Saturn.
It is true that a white dwarf above about 1.4 solar masses cannot exist. When a star dies, most of the mass does not become part of the remnant. A star 5 times the mass of the sun will shed most of its mass during the red giant phase. Only the innermost portion will collapse to form a white dwarf.
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 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.
No. The sun does not have enough mass to become a black hole. When the sun dies it will become a white dwarf.
Well, to put it shortly, the crane's wing mass is equal on both sides.
Because it takes a large amount of mass for the star to end up that way. Most stars will become white dwarfs. A small fraction will become neutron stars. And even smaller fraction will become black holes.
Different kinds of stars become different different stuffs......
The gas has molecules that are single atoms, as do the noble gases.
You will know what a star becomes when it dies based off of its mass. If the mass of the star is less than, around, or slightly greater than the sun's mass, it will become a white dwarf. If the mass of the star is a few solar masses, a supernova will happen and a neutron star will be created. If the mass of the star is many times that of the sun, it will explode in a giant supernova called a hypernova and create a black hole.
They are measured in amu (atomic mass units). However if you're taking Chemistry as a course, they are also measured in g/mol (grams per mol) which is equivalent.
The mass of a proton is equal to a neutron.
It probably won't ever become a black hole, unless for some reason a lot of additional matter falls on the Sun. Stars the mass of our Sun become white dwarves after they run out of fuel.
atomic mass unit is equal to one-twelfth of the mass of a carbon-12 atomic mass is equal to one-twelfth of the mass of a carbon-12Atomic Mass is equal to the number of protons and neutrons.
I believe if its over a certain mass it becomes 2 forms of super giant, then usually becomes supernova and cause a black hole. If under a certain mass it may expand slightly but then become a black or white dwarf star.
An avoirdupois ounce is equal to 437.5 grains, while an international troy ounce is equal to 480 grains. It is based upon the mass of a single grain of cereal.