Stars form in molecular clouds and nebulae, consisting mostly of hydrogen, with some helium and lithium. When enough mass (along with a few other factors) accumulates, such clouds begin to collapse under their own weight, forming dense pockets of dust and gas called Bok Globules. As Bok Globules increase in mass, their cores undergo more and more pressure, and when the cloud reaches hydrostatic equilibrium, a protostar forms at the center.
The obvious reason is that the specific star has bigger density compared with the Sun. For example, that star could be a "white dwarf star". A white dwarf mostly contains "electron degenerate matter", which is very dense. A white dwarf is a small dense star.
gravity
A supernova is a highly energetic and explosive event that occurs when a star reaches the end of its life cycle. It involves a rapid and violent collapse of the star's core, resulting in a burst of energy and matter being expelled into space. During a supernova, the matter is in a highly energetic and dense state, transitioning from a combination of different states of matter including plasma.
As matter from a nebula condenses, it begins to form into clumps due to gravity. These clumps eventually evolve into protostars, as heat and pressure increase at their cores, initiating the process of nuclear fusion. This marks the beginning of a star's life cycle.
Theoretically, an infinitely dense point of matter produced when a major star collapsed; the gravity shift and the huge amount of mass imploding creates a vaccuum which draws surrounding matter into it continuously, increasing the amount of matter but not necessarily the space it takes up; matter is crushed and compated into ridiculously small pieces.
The beginning stage in the formation of a star is called a protostar. This is when a dense core within a molecular cloud begins to accumulate gas and dust, causing it to heat up and eventually become a star.
"Small but very dense" sounds like the description of a neutron star or "collapsed matter star". Theoretically, a black hole (the only thing more dense) has no physical size at all. So, "neutron star". If the neutron star is spinning rapidly, they are called "pulsars" for the radio-wave pulses that they generate.
The description matches that of a neutron star, which is formed after a supernova explosion of a massive star. Neutron stars are incredibly dense, with matter packed tightly together. Due to their high gravitational pull, a small amount of neutron star material would have an extremely high mass.
The obvious reason is that the specific star has bigger density compared with the Sun. For example, that star could be a "white dwarf star". A white dwarf mostly contains "electron degenerate matter", which is very dense. A white dwarf is a small dense star.
Gravity plays an important role in the birth of a star. It concentrates matter in the interstellar medium to the point where fusion occurs.
Gravity plays an important role in the birth of a star. It concentrates matter in the interstellar medium to the point where fusion occurs.
gravity
As gravity increases so the pressure within the star increases, the matter becomes more dense and hotter, more matter is fused. The star decreases in volume initially. The thermal pressure increases to maintain equilibrium.Depending on the total mass the star may then expand to a giant or 'explode' catastrophically as a nova.
Studying star and star types can be fun, but it can be challenging to remember each type. A Neuron star is a dense, rapidly spinning star.
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White dwarf
A pulsar.