Lifetimes of stars are ended when they run low on gas to burn. The star will expand exponentially and turn red (called a Red Giant). When the star runs out of gas completely, in explodes (called a Supernova) and will evntually transform into either a Black Hole or a Dwarf Star.
Yes, stars can exist outside of a galaxy. These stars are typically referred to as intergalactic stars, and they may have been ejected from their original galaxy due to interactions with other stars or galactic dynamics. Intergalactic stars are typically found in the space between galaxies.
Elements which exist in stars exist also in humans, the concentrations are very different. An exception is helium, an element without biological significance.
Two stars that are gravitationally bound to each other are sometimes called "binary stars".
No, when solids melt, the particles do not cease to exist; instead, they transition from a solid state to a liquid state. During melting, the particles gain energy and move more freely, breaking the rigid structure of the solid. However, the number of particles remains the same; they simply change their arrangement and behavior.
The stars are always there, it just doesnt seem like it when there are many city lights, or if its a cloudy night.
Certainly. There is a chance that the earth will cease to exist.
Only if you are a vampire or werewolf.
No. Matter cannot be creater nor destroyed. An object cannot simply cease to exist.
1990
yes without an identity you aren't reconized you cease to exist without dying while you are in the physical world you cease to exist in the mental world thus making you extinct while being here.
dead 'Vanish' which means cease to exist.
ECLIPSE
1937.
possibley
The cast of Cease to Exist No. 1 - 1975 includes: Cosey Fanni Tutti as herself
The concept that states objects do not cease to exist when they are out of reach or view is called object permanence.
The instant they are found they cease to exist. They are found and then they are identified. Once identified they cease to be UFOs.