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"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."
In actual stars, all four fundamental forces (strong, weak, electromagnetic, gravity) are at work.
It allows the sun to be relatively stable for the last 4.5 billion years. (and hopefully for the next 5 billion.)
gravity. (gravitational force.)
When your body explodes outward from your center of gravity in space. There is no pressure in space. Your body's inner pressure is about the same as the earth's, preventing the earth's pressure from crushing you. In space, your body's pressure, as it has nothing pressing against it, expands outward in all directions until you are ripped apart.
"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."
"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."
In actual stars, all four fundamental forces (strong, weak, electromagnetic, gravity) are at work.
No an nebula is held together by the balance of the inward force of gravity and outward pressure.
Radiation
The inward force of gravity is counteracted by two outward forces: gas pressure, and radiation pressure. Once the star runs out of fuel, the radiation pressure stops, the gas pressure is no longer enough to counteract gravity, and the star collapses - into a white dwarf, a neutron star, or a black hole, depending on its mass.
It allows the sun to be relatively stable for the last 4.5 billion years. (and hopefully for the next 5 billion.)
Radiation. Mostly sunshine in, infrared radiation outward.
Radiation.
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.
Yes, a stable star is in equilibrium, called hydrostatic equilibrium, when the outward pressure from heat caused by core fusion processes balances the inward pull of gravity. There are other factors which alter the form of stars such as their rotation or gravity from external sources such as a nearby mass.
No, the Earth's gravity pulls the moon in towards Earth.