Liste des Groupes | Revenir à p relativity |
Paul.B.Andersen <relativity@paulba.no> wrote://///////////////////////////////////////////////////////////////////
>Den 28.09.2024 04:34, skrev rhertz:>This link illustrates a bit:>
>
https://en.wikipedia.org/wiki/Gravitational_redshift
>
Using the most common formula from that link: "To first approximation,
gravitational redshift is proportional to the difference in
gravitational potential divided by the speed of light squared"
>
?f/f = ??/? = z = GM/c? (1/R - 1/r) = ?(R)/c? - ?(r)/c?
??/? = GM/Rc? observed at infinity (r -> ∞)
>
https://www.space.com/41290-biggest-star.html>>
G = 6.6743E?11 m^3 kg^?1 s^?2
M = 5E+09 x 1.989E+30 Kg = 9.945E+39 Kg
R = 1,700 x 634,000 Km = 1,077,800,000,000 m
>
>
?(R)/c? = 6,842,736.59
From whence did you get the idiotic idea that the mass
of UY Scuti was 5 billion solar masses? :-D
>
M = 30 solar masses = 5.967e31 kg
R = 696340e3?1700 m = 57868e6 m
c = 299792458 m/s
>
??/? = GM/Rc? = 7.65e-7
>
Which is less than the red shift from the Sun.
>>>
In comparison, ?(RSun)/c? = 0.000002327
M = 1.989E+30 kg
R = 696340e3 m
>
??/? = GM/Rc? = 2.12e-6
>
>
>>>
WHAT IS WRONG WITH MY CALCULATIONS, BASED ON THE WIKI LINK?
Now you know.
He is looking for trouble where none exists.
Even for neutron stars you get a nice finite gravitational redshift,
which is 'easily' observable. For example:
<https://pubmed.ncbi.nlm.nih.gov/12422210/>
>
They find a redshift value of z = 0.35 ,
which is consistent with standard neutron star models,
(but not with some exotic ones)
>
Jan
>
(such a large gravitational redshift dwarfs any possible Doppler shift)
Les messages affichés proviennent d'usenet.