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3 votes
1 answer
3k views

How long does it take a star to transition from main sequence to red giant?

I have read that it takes billions of years for stars of approximately the size of the Sun to get through the main sequence, after which it will enter the red giant phase. When that happens, how long ...
Johnny Dollard's user avatar
4 votes
1 answer
2k views

What is the largest hydrogen-burning star?

I am wondering what is the largest known core hydrogen-burning star? A look at the list of largest known stars on Wikipedia seems to indicate VV Cephei B (at the bottom of the list), but I would like ...
NeutronStar's user avatar
  • 2,673
15 votes
2 answers
5k views

Does a star fuse helium to beryllium on the main sequence?

When a star has finished fusing all its hydrogen into helium, it will then start fusing helium into beryllium and so on and so forth up until iron. When the star is fusing to beryllium, will the ...
MiscellaneousUser's user avatar
12 votes
1 answer
434 views

Is there a relation between mass, radius, and luminosity in deuterium-burning brown dwarfs?

I'm a worldbuilder and my setting has a lot of brown dwarfs. While I'm trying to keep my setting as science-compliant as possible, I can't seem to find any resources for brown dwarfs like there are ...
TerranAmbassador's user avatar
4 votes
4 answers
4k views

Why is the main sequence often called 'zero age' main sequence?

The main sequence stage for a star begins after it stars burning hydrogen into helium. This is often referred to as the zero age main sequence. This is confusing since stars have already lived ...
Gabriel's user avatar
  • 822
3 votes
0 answers
48 views

Strength of core-envelope coupling in stars (again)

I asked this on the physics SE but it received little attention: Consider a high-mass zero-age main-sequence (ZAMS) (e.g., $m_{\rm ZAMS} \gtrsim 30\,$M$_{\odot}$) star. I understand that the core-...
Daddy Kropotkin's user avatar