A protosun is an early-stage version of a star before it has fully formed and ignited nuclear fusion in its core. It is composed mainly of gas and dust, undergoing gravitational collapse as it accumulates mass from its surrounding nebula. Over time, the protosun will eventually reach a critical mass and temperature to initiate nuclear fusion, becoming a fully functional star.
The name given to the concentration of mass at the center of the solar nebula that eventually formed the Sun is the protosun or solar protostar. This dense core accumulated gas and dust, triggering nuclear fusion to ignite as a star.
The nebular hypothesis proposes that protoplanets formed around the protosun in a protoplanetary disk through collisions and aggregations of gas and dust. This process, known as accretion, led to the formation of larger bodies from smaller ones over time.
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Mean solar time on the prime meridian is known as Greenwich Mean Time (GMT).
what do the largest clumps surrounding the protosun to begin to form
A protosun is a young star in the early stages of formation, where nuclear fusion has not yet started in its core. Once nuclear fusion begins in the core, the protosun transitions into a sun and starts emitting light and heat.
Protosun
The protosun has not fully "ignited" meaning nuclear fusion is not stably providing the energy output of the star. Once ignition takes place, the central core of the sun will produce energy almost exclusively through fusion, creating enough energy and radiation to slowly wash away the nebulous gas surrounding the protosun revealing the sun itself.
No our Sun is a fully formed Star. A Protostar is gas that is still acreeting matter (still collecting via gravtaional rotation) to form a star. And as a result they are not very bright as they have not condensed enough to start Nuclear Fusion.
Heat, derived from gravitational energy. The gravitational collapse of the original nebula of gas and dust produced very high temperatures and a "protosun". Eventually the protosun became a star (our Sun) when the nuclear fusion reactions began at temperatures of millions of degrees Celsius.
The name given to the concentration of mass at the center of the solar nebula that eventually formed the Sun is the protosun or solar protostar. This dense core accumulated gas and dust, triggering nuclear fusion to ignite as a star.
The nebular hypothesis proposes that protoplanets formed around the protosun in a protoplanetary disk through collisions and aggregations of gas and dust. This process, known as accretion, led to the formation of larger bodies from smaller ones over time.
The nebular hypothesis suggests that protoplanets began to form around the protosun from the collisions and combinations of gas and matter in the protoplanetary disk. This theory explains how the solar system's planets, including Earth, formed from the rotating disk of gas and dust around the young Sun about 4.6 billion years ago.
AnswerA proto star hasn't accumulated enough mass for the thermo-nuclear reacton to start, which would make it a star.To add to the above answer, most of the light that a protostar produces is due to the pressure from gravity. -Phil
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you mean what you mean