How do nebulas form stars and solar systems?

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Nebulae are primarily clouds of gas, mostly hydrogen, and play a crucial role in star and solar system formation. Stars form within these clouds when clumps of dust collapse under gravity, although stars can also originate in giant molecular clouds. Nebulae are composed of about 90% hydrogen and 10% helium, with some debate over the exact ratios depending on whether mass or number of atoms is considered. There are different types of nebulae, including diffuse and dark nebulae, each with distinct characteristics. Overall, nebulae are essential to understanding the origins of stars and the composition of the universe.
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What exactly are nebulas and do they form stars and even solar systems? Are they mostly iron?

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Nebula (as opposed to galaxies, which at one time were called nebula) are clouds of gas, mostly hydrogen. Whether or not stars can be born there depends on the size, density, etc.
 
Nebulae are made of dust and gas; in some parts of the nebula clumps of dust are formed and they collapse gravitationally to form stars. There are to classes of nebulae: diffusse nebulae and dark nebulae. Diffusse nebulae can be divided into emission nebulae and reflection nebulae
I will point also that stars don't form only in nebulae, they also form in giant molecular clouds
Are they mostly iron?
Not quite. Most nebulae are formed of about 90% hydrogen and 10% helium
 
meteor said:
... Most nebulae are formed of about 90% hydrogen and 10% helium
Well, I would say closer to 75-25, but it's just a fine point.
 
I believe the discrepancy has to do with what ratio we are talking about for H to He. The mass ratio is about 3-1, while the number ratio is 12.5-1. I hope this clears it up.
 
Once we convert to the same units, we will find agreement. about 90-10 is ratio by number of hydrogen v helium atoms, 75-25 is the ratio by mass. I had to check cause I pulled 75-25 off the top of my head [a sometimes risky practice]. Anyways, those are the textbook numbers [The New Solar System, Beatty & Chaikin]. No online version of that book but I have a link that includes the relevant table from the book.
http://www.genesismission.org/educate/scimodule/PlanetaryDiversity/plandiv_pdf/SupermarketST.pdf
 
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Interestingly, this implies that your average 'nebula gas' is close to primordial (in terms of composition). For the most part, that's quite reasonable (much of the non-primordial stuff in the dark nebulae, reflection nebulae, etc is in the form of dust, not gas), but not always ... for example, nebulae that are 'purely' supernova remnants will likely be deficient in H (and He).
 
Thanks Nereid
One of the links says that there are 5 types of nebulae: planetary nebulae,supernovae remnants, emission nebulae, reflection nebulae and dark nebulae. But, as there are supernovae remnants, there are also nova remnants. I wonder why these should be marginalized and not included as nebulae
 
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Good point meteor. I was thinking in terms of protosolar nebulae: the kind that birth stars. That was the spirit of the original question as I perceived it. Those of course can be expected to be very similar to the primordial gas clouds from which most stars are formed. Nebulae formed by events of a different nature are, as you note, horses of a different color.
 

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