This would be the range of stars of a size range that maintains enough mass to bring a condensing contraction of the cooling star as it's nuclear fuel passes through the light elements until the fusion (sticking together as opposed to fission or splitting apart) is halted at the progression up the elemental chart at Fe or Iron and less energy is produced over a wider area as the Iron heart of the star builds providing less heat to keep the star expanded against its own mass... small stars with little mass tend to become brown dwarfs. Cinders almost. Stars with a bit more extra mass will fall in on themselves gaviticaly as their energy is expended until stopped by the physical forces that bind electrons (white dwarfs) and atomic nuclei (neutron stars) with the largest masses that don't go super nova massive are greater even than the electromagnetic forces binding atoms and the collapse is to a mathmatical singularity the famous black hole... but this picture is far to simple... for example the super massive black holes that seem to be associated with most galactic centers and there are timescale issues with large scale formations (apparent) but that's the idea in a nutshell
Gravitational collapse is a crucial step in the process of star formation. When a cloud of gas and dust in space collapses under its own gravity, it becomes denser and hotter, eventually leading to the formation of a protostar. This gravitational collapse is what initiates the fusion reactions in the core of the protostar, eventually leading to the birth of a new star.
A white dwarf's stability is maintained by electron degeneracy pressure, which prevents further collapse due to the immense gravitational pull.
The main force that causes a star to undergo gravitational collapse and transform into a black hole is the inward pull of gravity, which becomes stronger as the star's core runs out of fuel and can no longer support itself against its own gravity. This collapse results in a dense, compact object with a gravitational pull so strong that not even light can escape, creating a black hole.
When a black hole collapses, it shrinks in size and its gravitational pull becomes stronger. This process is called gravitational collapse. The consequences of this collapse include the black hole becoming denser and more massive, leading to an increase in its gravitational force. This can result in the black hole consuming nearby matter and energy, and potentially emitting powerful radiation and jets of particles.
An object needs to surpass the Chandrasekhar limit, approximately 2.0 × 10^17 kg/m^3, to develop a gravitational field. This limit represents the point at which electron degeneracy pressure can no longer support the object against gravitational collapse, leading to the formation of a neutron star or black hole.
a strong gravitational force which means that the star will collapse in on itself
Gravitational instability theory
Gravitational collapse is a crucial step in the process of star formation. When a cloud of gas and dust in space collapses under its own gravity, it becomes denser and hotter, eventually leading to the formation of a protostar. This gravitational collapse is what initiates the fusion reactions in the core of the protostar, eventually leading to the birth of a new star.
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Gravitational collapse of a protostellar nebula.
A white dwarf's stability is maintained by electron degeneracy pressure, which prevents further collapse due to the immense gravitational pull.
Black holes are the result of the gravitational collapse of a large star.
Several factors can cause pyroclastic flows. Fountain collapse of a volcano's eruption column structure, and gravitational collapse may cause pyroclastic flows.
The densest parts of a nebula collapse primarily due to gravitational forces. As regions within the nebula become denser, their gravitational pull increases, attracting surrounding gas and dust. When the pressure and density reach a critical threshold, the intense gravitational forces overpower the internal thermal pressure, leading to the collapse of these regions. This process can initiate star formation as the collapsing material forms a protostar.
By the gravitational collapse of massive stars - once they stop producing energy.
if they are massive enough and have sufficient gravitational force to overcome pressure forces and begin the process of nuclear fusion, which powers stars. This collapse is triggered by disturbances such as shock waves from supernovae or gravitational interactions with other clouds.
The main force that causes a star to undergo gravitational collapse and transform into a black hole is the inward pull of gravity, which becomes stronger as the star's core runs out of fuel and can no longer support itself against its own gravity. This collapse results in a dense, compact object with a gravitational pull so strong that not even light can escape, creating a black hole.