The sun isn't an ordinary fire, but an ordinary fire can answer your question:
A fire keeps burning as long as it has fuel to burn. When the fuel runs out and
there's nothing left to burn, the fire goes out.
The sun is a nucleasr fusion reactor, pressing the nuclei of hydrogen atoms
together so hard that they 'fuse', which creates nuclei of helium and releases
energy in the process. The sun has been doing that for something like 3 or 4
billion years, and has fused something like 1/2 of the hydrogen it started with.
When the rest of the hydrogen is used up, in something like another 4 billion
years, the sun will either swell up, blow up, or go out.
No, the size of the sun remains relatively stable over short periods of time. The sun does go through changes over long periods, but these changes occur gradually over millions of years.
No, the sun is not breaking apart. It is a stable star that is undergoing nuclear fusion in its core, converting hydrogen into helium and releasing energy in the process. The sun is expected to remain stable for billions of years to come.
The sun remains stable over time through a delicate balance between the force of gravity pulling it inward and the pressure from nuclear fusion pushing outward. This balance allows the sun to maintain its shape and energy output for billions of years.
Planets orbit around the sun due to the gravitational force between the sun and the planet. The planet's velocity and distance from the sun are balanced in such a way that it follows a stable orbit path. This balance allows the planet to remain in a relatively stable position around the sun without drifting off into space.
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.
The sun is expect to remain stable for another three billion years.
The sun is expect to remain stable for another three billion years.
roughly 6 billion years
No, the size of the sun remains relatively stable over short periods of time. The sun does go through changes over long periods, but these changes occur gradually over millions of years.
No, the sun is not breaking apart. It is a stable star that is undergoing nuclear fusion in its core, converting hydrogen into helium and releasing energy in the process. The sun is expected to remain stable for billions of years to come.
gravity is what keeps the earth in orbit around the sun the gravitational pull exerted by the sun causes the earth to remain at a relatively stable distancefrom the sun
The sun remains stable over time through a delicate balance between the force of gravity pulling it inward and the pressure from nuclear fusion pushing outward. This balance allows the sun to maintain its shape and energy output for billions of years.
The mass of the sun is decreasing over time.
Planets orbit around the sun due to the gravitational force between the sun and the planet. The planet's velocity and distance from the sun are balanced in such a way that it follows a stable orbit path. This balance allows the planet to remain in a relatively stable position around the sun without drifting off into space.
"Inertia" plus gravity (of the sun). Note that the orbits do change over time, but that in the last few billion years they have been quite stable.
Hydrostatic equilibrium in the Sun refers to the balance between the inward gravitational force and the outward pressure force generated by nuclear fusion. This balance maintains the Sun's stable structure and allows it to maintain its size and shape over time.
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.