Star balance, often referred to in the context of astronomy, pertains to the equilibrium between the gravitational forces pulling inward on a star and the outward pressure generated by nuclear fusion in its core. This balance is crucial for a star's stability and longevity, allowing it to maintain its size and shape over time. If the balance is disrupted, either by the depletion of nuclear fuel or external forces, the star may undergo changes such as expansion into a red giant or collapse into a different stellar state.
Actual balance is the real balance while avialable balance is the physical balance
SYMMERTRICAL BALANCE
my balance sheet does not balance why?
Opening balance of cash in trail balance
firstily trial balance of total is the total balance of trial balance being show at the end of a year. trial balance of balance it is the balances being show doing the calcution of the trial balance.
Balance of Power - Star Trek - was created in 1994.
5 star defense 2 star attack 2 star balance 2 star stamina
hydrostatic
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.
The balance of forces that keep a star from collapsing is called hydrostatic equilibrium. This equilibrium is maintained between the inward force of gravity and the outward force generated by gas pressure within the star.
rock Scorpio is ok in stamina,great in defense,ok at attack,off in balance
Pressure and gravity
Dynamic equilibrium.
Star Trek - 1966 Balance of Terror 1-14 is rated/received certificates of: Argentina:Atp Canada:PG (video rating)
When the outward fusion and radiation pressure of a star balance with the inward force of gravity, the star reaches a state of hydrostatic equilibrium. In this state, the forces are in balance, preventing the star from collapsing under its own gravity or expanding uncontrollably. This equilibrium allows the star to maintain a stable size and temperature for an extended period, typically during its main sequence phase. It is a crucial aspect of stellar evolution, determining the star's lifecycle and eventual fate.