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protostar is a very young star that is still gathering mass from its parent molecular cloud.The protostellar phase is the earliest one in the process of stellar evolution. For a low mass star (i.e. that of the Sun or lower), it lasts about 500,000 years The phase begins when a molecular cloud fragment first collapses under the force of self-gravity and an opaque, pressure supported core ...
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cTsOiFIYpq emezFPItQ A protostar acquiring two condensations will become a binary and be stable thereafter [..] Whether a binary or a single star results depends largely on the total angular momentum of the protostar
Deuterium fusion, also called deuterium burning, is a nuclear fusion reaction that occurs in stars and some substellar objects, in which a deuterium nucleus and a proton combine to form a helium-3 nucleus. It occurs as the second stage of the proton–proton chain reaction, in which a deuterium nucleus formed from two protons fuses with another proton, but can also proceed from primordial ...
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Protostars and the Nebula. This animation shows how a star begins to form out of a nebula.. A nebula is a cloud of dust and gas, composed primarily of hydrogen (97%) and helium (3%). Within a nebula, there are varying regions when gravity causes this dust and gas
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cSDPncfrMLt Protostars:. Once a clump has broken free from the other parts of the cloud core, it has its own unique gravity and identity and we call it a protostar. buy Protostars
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