What is the equation of state explain?
In physics and thermodynamics, an equation of state is a thermodynamic equation relating state variables which describe the state of matter under a given set of physical conditions, such as pressure, volume, temperature (PVT), or internal energy.
What is the PVT equation of state?
The equation called the thermic equation of state allows the expression of pressure in terms of volume and temperature p = p(V, T) and the definition of an elementary work δA = pδV at an infinitesimal change of system volume δV.
What is an equation of state write the equation of state for an ideal gas?
In the limit of low pressures and high temperatures, where the molecules of the gas move almost independently of one another, all gases obey an equation of state known as the ideal gas law: PV = nRT, where n is the number of moles of the gas and R is the universal gas constant, 8.3145 joules per K.
How stars are formed?
Stars form from an accumulation of gas and dust, which collapses due to gravity and starts to form stars. The process of star formation takes around a million years from the time the initial gas cloud starts to collapse until the star is created and shines like the Sun.
How many stars are there?
There are an estimated one hundred billion (100,000,000,000) stars in our own Milky Way galaxy, although some estimates range up to four times that many, much depending on the number of brown dwarfs and other very dim stars. A typical galaxy may contain anywhere between about ten million and one trillion stars.
What is the lifespan of a star?
about 10 billion years
Which star has the shortest life expectancy?
red dwarfs
What are 3 ways a star dies?
Black holes, neutron stars and red dwarfs – it all depends on the mass. Stars die because they exhaust their nuclear fuel. The events at the end of a star’s life depend on its mass.
How do start die?
Most stars take millions of years to die. When a star like the Sun has burned all of its hydrogen fuel, it expands to become a red giant. After puffing off its outer layers, the star collapses to form a very dense white dwarf. …