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Nebulae originate from clouds of gas and dust in space that are composed mostly of hydrogen and helium. These clouds can be found in various locations throughout galaxies, such as in the interstellar medium or surrounding newly formed stars. The different types of nebulae, such as reflection, emission, and planetary nebulae, each have their own unique origin stories.

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Q: Where did nebula originally come from?
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Related questions

Where did the cats eye nebula come from?

the sky


Why do they call a nebula a nebula?

"Nebula" comes from the Latin word for "cloud." Nebulae are large clouds of dust, hydrogen, helium, and other gases in space. The term was originally used to describe any celestial object with a hazy appearance.


Does the sun come close to nebula's while orbiting in the galaxy?

Which Nebula? Astronomically speaking, no it does not. In our lifetime, we will not come anywhere near to a nebula. If your thinking of the Andromeda Galaxy then - well expect galactic fireworks - but not for about 3 billion years. [See related question]


Do nebula's die?

Yes, Nebula's die. They die when they get to close to Black Holes.


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Musa comes from the Harmonic Nebula.


Why did the world come to be?

It condensed from the interstellar nebula form which our star, the Sun, was formed.


What is the difference between a nebula and a crab nebula?

The Crab Nebula is a nebula.


Where did pumpkins come from originally?

Pumpkin's are originally from America.


Where did the word fraction originally come from?

Latin, originally.


What is a mass of gases dust particle s and stars that are located in space?

nebula


What force is responsible for the nebula to come together?

Gravity is the force responsible for pulling particles within a nebula together. As particles within the nebula are attracted to each other by gravity, they gradually collapse and become more compact, eventually leading to the formation of stars and planets.


How does a nebula developes into a solar system?

A nebula develops into a solar system through the process of gravitational collapse. As the nebula contracts due to gravity, it starts to spin and flatten into a spinning disk. Within this disk, the material begins to clump together and form planetesimals, which eventually coalesce to form planets, moons, and other objects in the solar system.