A protostar is a massive object that forms from the contraction of gas from a giant molecular cloud. This protostellar phase is the early stage of star formation. For a protostar with the mass of the Sun it will last about 100,000 years. It starts with a core of increased density in a molecular cloud and ends with the formation of a T Tauri star, which then develops into a main sequence star. This is heralded by the T Tauri wind, a type of super solar wind that marks the change from the star accreting mass into radiating energy. A T Tauri star is similar to those of main sequence stars of the same mass, but they're significantly more luminous because their radii are larger. See related links for more information.
we scientist really have no idea how it get its power but we are getting there....
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A protostar is a large mass of gas and dust that is collapsing under gravity. It is an early stage of stellar formation. It is also a very short stage. For a star of 1 solar mass it only last about 100,000 years
Using Boyle's Law
(P*V)/T=K
where
P= Pressure,
V= Volume,
T= Temperature &
K= a Constant
Therefore T=(P*V)/K
we can calculate that as pressure inside the ball of gas increases so does the temperature. Eventually the temperature of the interior of the the star reaches a point where that nuclear fusion can take place.
Primarily hydrogen, the most common element in the universe. When a cloud of hydrogen starts collapsing under its own gravity, it can (if nothing disturbs it) collapse into a proto-star, or "pre-star". If there's enough mass, the central pressure and temperature will increase as everything falls together, and eventually hydrogen fusion will begin. This is when the star is born, when the hydrogen begins fusing into helium.
Hydrogen, mostly. Some helium, and traces of heavier elements.
NGC 7538S is one of the most massive protostars known.
A protostar is a star that is still is still in the process of forming and has not yet driven away the surrounding envelope of gasses from its parent nebula.
the elements are hydrogen and helium cloud
See related link for a pictorial
Mostly hydrogen & helium
Helium, Hydrogen, and Lithium
the color of the protostar is red
As gravity pulls more material toward the center of the protostar, the pressure inside the protostar builds.
A protostar will live as long as 100,000 years. After material stops falling on the protostar it will enter then T Tauri star phase.
No, a protostar is basically the BEGINNING of a star's life cycle.
A protostar isÊthe beginning or birth of a star. Before a protostar can glow it must go thru a period of contraction in order to allow nuclear reactions at its core.
Mostly hydrogen (with some helium, deuterium, and lithium). Other elements (all other elements) are added as the date of formation of the protostar comes closer to the current date.
the color of the protostar is red
A Protostar.
As gravity pulls more material toward the center of the protostar, the pressure inside the protostar builds.
A protostar will live as long as 100,000 years. After material stops falling on the protostar it will enter then T Tauri star phase.
A protostar is more like a stage previous to a star - before it ignites.
A protostar takes about 100,000 years to reach the main sequence.
No. The sun was a protostar about 4.6 billion years ago.
The term is "protostar", not "prostar". Yes. A protostar is an early stage of a star.
A protostar has 100% Hydrogen. A young star has a Helium core.
"Binary" means there are two stars. And "protostar" means the stars are in an early, or preliminary, stage.
Apparently someone not paying ATTENTION.