[mesa-users] A common stellar-structure myth
RICHARD H D TOWNSEND
townsend at astro.wisc.edu
Tue Aug 30 18:26:42 EDT 2016
Ideal gas, hydrostatic equilibrium plus radiative diffusion for a constant opacity — combine together, and one finds that L ~ M^3. This scaling fits the main sequence reasonably well.
cheers,
Rich
> On Aug 30, 2016, at 5:20 PM, Brian Jackson <bjackson at boisestate.edu> wrote:
>
> Since we're reviewing basic stellar evolution, can I ask why L ~ M^3?
> That just comes from the equation of state?
>
> Thanks,
> Brian
>
> On Tue, Aug 30, 2016 at 4:17 PM, RICHARD H D TOWNSEND
> <townsend at astro.wisc.edu> wrote:
>> That’s as maybe, but the gravity is not stronger.
>>
>> In any case, what really drives the large energy generation rate in massive stars is the energy loss rate through the stellar surface, which scale as L ~ M^3 (independent of nuclear reactions). The pre-MS star continues to contract until the core energy generation rate matches this loss rate.
>>
>> cheers,
>>
>> Rich
>>
>>> On Aug 30, 2016, at 5:05 PM, Tomasz Plewa <tomekplewa at gmail.com> wrote:
>>>
>>> It's a deeper potential well.
>>>
>>> Tomek
>>> --
>>>
>>>
>>>> On Aug 30, 2016, at 5:52 PM, RICHARD H D TOWNSEND <townsend at astro.wisc.edu> wrote:
>>>>
>>>> Hi folks —
>>>>
>>>> While reading the textbook I’m going to be teaching from this semester (“Pathways to Astronomy”, by Schneider & Arny), I came across this common myth about stellar structure:
>>>>
>>>> “The stronger gravity of a more massive star drives up the rate of nuclear fusion dramatically, while smaller stars consume their fuel at a more leisurely pace”.
>>>>
>>>> The attached figure, courtesy of MESA, shows the internal gravity for 1Msun and 10Msun stars at the ZAMS — and nicely busts the myth.
>>>>
>>>> cheers,
>>>>
>>>> Rich
>>>>
>>>> <gravity.pdf>
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