What is a nebula? How does it form a protostar?
A nebula is a cloud of gas and dust which can be millions of light years in diameter
When gas and dust in a nebula begin to condense, their gravitational pull increases with mass, causing more and more condensation, which results in the formation of a pre main sequence star where nuclear fusion begins. This is how protostars are created.
After that, it develops into a main sequence star, with distinct consequences depending on the star's mass.
By signing up, you agree to our Terms of Service and Privacy Policy
An enormous cloud of gas and dust in space, a nebula eventually forms a protostar through a process known as gravitational collapse, in which the gas and dust particles within the nebula are drawn together by gravity, heat up as a result of the increasing pressure, and eventually reach a point where nuclear fusion ignites, forming a protostar.
By signing up, you agree to our Terms of Service and Privacy Policy
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.

- 98% accuracy study help
- Covers math, physics, chemistry, biology, and more
- Step-by-step, in-depth guides
- Readily available 24/7