Gravity is constantly pulling the matter of a star together, while the nuclear fission reaction that makes the star shine and put off heat is trying to make it explode. The two are very precariously balanced.
Stars are held together only by the force of gravity. The other 3 fundamental forces have no influence on that.
gravity and fusion
stuff
Pressure and gravity
No an nebula is held together by the balance of the inward force of gravity and outward pressure.
The balance between pressure caused by heat and gravity caused by the star's mass.
Any satellite is in a careful balance between gravity and inertia.
While the star can produce energy, that keeps the star in balance - it keeps the star from collapsing. By the way, another outward force is the gas pressure, but that, by itself, is not enough to counteract the force of gravity in the case of a star.
You used the term nebular. I take it you mean a galaxy. There would not be a balance between gravity and pressure. There would be a balance between gravity and centrifugal force.
The balance between gravity and pressure can be upset if two nebulas collide. It can also be upset if a nearby star explodes.
The balance between gravity and pressure can be upset if two nebulas collide. It can also be upset if a nearby star explodes.
Two events that can upset the balance between gravity and pressure in a nebula are a supernova explosion or the collision of two nebulae. A supernova explosion releases an enormous amount of energy and can disrupt the delicate equilibrium between gravity and pressure. The collision of two nebulae can also disturb the balance by introducing additional gravitational forces and increasing the overall pressure within the system.
Pressure and gravity
Pressure and gravity
Hydrostatic equilibrium occurs when compression due to gravity is balanced by a pressure gradient which creates a pressure gradient force in the opposite direction. The balance of these two forces is known as the hydrostatic balance.
Pressure and gravity
No an nebula is held together by the balance of the inward force of gravity and outward pressure.
To start with, the star's gravitational attraction is not sufficient to offset the outward radiation pressure. As a result, the star increases in size until the two are in balance.
When hydrogen in the core of the star is depleted, a balance no longer exists between pressure and gravity, with that the core contracts and temperature rises. This cause outer layers to cool and expand. In this late stage of the star's life cycle, it is called a giant. The sun will continue to be a main sequence for about 5 billion years, then the sun will become a giant.
The balance between pressure caused by heat and gravity caused by the star's mass.