Table of Contents
- 1 What are the two forces that balance out a star when it is in stellar equilibrium?
- 2 How is stellar equilibrium achieved?
- 3 What is stellar equilibrium?
- 4 Why is stellar equilibrium important?
- 5 Which of the following forces are balanced when a star is in equilibrium?
- 6 How is hydrostatic equilibrium in a star determined by mass?
- 7 What is the life cycle of a low-mass star?
- 8 What is the definition of stellar equilibrium?
What are the two forces that balance out a star when it is in stellar equilibrium?
Stars live out their lives in an exquisitely detailed equilibrium, or balance, between two powerful forces — outward pressure and the inward pull of gravity. The gravity force is a property of the mass of the star, and in order to support itself against gravity the star generates energy in its core.
How is stellar equilibrium achieved?
When gravity makes the core of a star so hot and dense that nuclear fusion commences, that pressure balances gravity and establishes equilibrium.
What forces are balanced when a star is in equilibrium?
You can imagine a star as a series of layers. The inward force of gravity is balanced out by the outward force of pressure to keep the star stable. This stable balance, the outward pressure of hot gases balancing the inward pull of gravity is called the hydrostatic equilibrium.
What are the two main forces that act on gases in a star?
Pressure and gravity. Pressure due to fusion reactions pushes outwards. Gravity pulls inwards to keep the star in equilibrium.
What is stellar equilibrium?
Stellar equilibrium is also known as hydrostatic equilibrium. A star is in equilibrium when the pressures inside the star balance out the force of gravity. The pressure is thermal pressure resulting from the fusion reactions taking place in the star’s core.
Why is stellar equilibrium important?
This shell helps move heat from the core of the star to the surface of the star where energy in the form of light and heat is released into space. The star’s main goal in life is to achieve stability, or equilibrium. The term equilibrium does not mean that there isn’t any change in the star.
What is it called when a star is in equilibrium?
Gravity constantly works to try and cause the star to collapse. The star’s core, however is very hot which creates pressure within the gas. This pressure counteracts the force of gravity, putting the star into what is called hydrostatic equilibrium. This phase of the star’s life is called the main sequence.
Which is the balance between gravity squeezing inward and pressure from?
For a star to be stable, it must have hydrostatic equilibrium,which is the balance between gravity squeezing inward and pressure from nuclear fusion and radiation pushing outward. This balance is governed by the mass of the star. The temperature inside a star determines the star’s energy output, or .
Which of the following forces are balanced when a star is in equilibrium?
The inward force of gravity is balanced out by the outward force of pressure to keep the star stable. This stable balance, the outward pressure of hot gases balancing the inward pull of gravity is called the hydrostatic equilibrium.
How is hydrostatic equilibrium in a star determined by mass?
Greater gravity compresses the gas, making it denser and hotter, so the outward pressure increases. In any given layer of a star, there is a balance between the thermal pressure (outward) and the weight of the material above pressing downward (inward). This balance is called hydrostatic equilibrium.
What is hydrostatic balance in atmosphere?
Gravity is pushing the atmosphere toward the Earth while the vertical pressure gradient force is pushing the air into space. These two forces when equally balanced is termed “hydrostatic balance”. Hydrostatic balance results in a stable striation of the atmosphere and no vertical motions.
What effect does stellar equilibrium have on stars?
A star is in equilibrium when the pressures inside the star balance out the force of gravity. The pressure is thermal pressure resulting from the fusion reactions taking place in the star’s core. A star stays in equilibrium until the supply of hydrogen in the core is depleted.
What is the life cycle of a low-mass star?
Low mass stars live out most of their lives as dim, small, and cool red dwarf stars. They last about 100 billion years, and in their last years they are a very hot, but dim white dwarf star.
What is the definition of stellar equilibrium?
Stellar equilibrium or also known as hydrostatic equilibrium is the balance between the pressure inside the star and the force of gravity.
What are the steps in star formation?
Describe the steps of star formation. 1. Gravity condenses a dense cloud (nebulae) of gas (there is nothing to fight gravity at this point) 2. As density increases, pressure increases, pushing against gravity. 3. As pressure rises, temp rises, and if temp gets hot enough ( if mass large enough) nuclear reactions wills start.