The balance between pressure caused by heat and gravity caused by the star's mass.
At equilibrium, the rate of the forward reaction is equal to the rate of the reverse reaction. The concentrations of reactants and products remain constant, although they are still reacting. The equilibrium position can be affected by changes in temperature, pressure, or concentration.
Saline.
Sphere
To find the equilibrium concentration of NO, first calculate the equilibrium constant expression using the given concentrations of O2 and N2. Then, rearrange the equilibrium constant expression to solve for the concentration of NO. Finally, substitute the values of O2 and N2 concentrations into the rearranged expression to find the equilibrium concentration of NO.
Sublimation best describes the process in which a solid directly changes to a gas without passing through the liquid state.
Stellar equilibrium is the balance between the inward force of gravity and the outward force of gas pressure within a star. This balance allows the star to maintain its size and shape over time. Any disruptions to this equilibrium can result in changes to the star's structure and behavior.
Dust cloud
Stellar evolution is the collection of hypotheses that describes how stars develop as they age.
The balance between pressure caused by heat and gravity caused by the star's mass.
The main reactions that maintain stellar equilibrium are nuclear fusion reactions in the core, which produce energy that balances the gravitational force trying to collapse the star. The pressure generated by these reactions pushes outward, counteracting the gravitational force pulling inward, resulting in a stable balance known as hydrostatic equilibrium.
Homoeostasis. (Chemistry, biology) Equilibrium. (Physics, mechanics)
There is no surplus or shortage
There is no surplus or shortage
equilibrium
In the stellar equilibrium, the primary reaction is nuclear fusion, where hydrogen atoms are fused to form helium, releasing energy in the form of light and heat. This process is sustained by the star's gravitational pressure balancing the force of nuclear fusion. Helium fusion into heavier elements can also occur in more massive stars.
Equilibrium is not a force, it is a state in which all the forces acting on an object are balanced, resulting in no change in its motion. When an object is in equilibrium, the net force acting on it is zero.
Equilibrium describes any state where the acceleration and net force are zero. This means that the velocity will not change.