I The Shape of Very Massive Stars: Spheres or Something Else?

  • I
  • Thread starter Thread starter windy miller
  • Start date Start date
  • Tags Tags
    Shape Stars
AI Thread Summary
The shape of very massive stars is primarily spherical unless they are rotating rapidly, in which case they become oblate spheroids. Surface irregularities exist on massive stars, influenced by their surface gravity; lower gravity allows for larger irregularities, while higher gravity results in smaller ones. For example, Betelgeuse, a supergiant with low surface gravity, is expected to have significant surface irregularities, while a smaller main sequence star like Theta Orionis A1 has much smaller irregularities due to its high surface gravity. Neutron stars, with extremely high surface gravity, exhibit minimal surface irregularities. Understanding these factors is crucial for studying the physical characteristics of massive stars.
windy miller
Messages
306
Reaction score
28
What is the shape of very massive stars? Are they simply spheres or something else?
 
Astronomy news on Phys.org
Why would you expect them to be anything other than spheres?
 
  • Like
Likes windy miller
If they are rotating rapidly, they will be oblate spheroids. Otherwise, they are spheres.
 
  • Like
Likes windy miller
phinds said:
Why would you expect them to be anything other than spheres?
I seem to recall someone saying they weren't , but I want to be clear I don't have any reference for that. Always best to ask i think if one has some doubts.
 
phyzguy said:
If they are rotating rapidly, they will be oblate spheroids. Otherwise, they are spheres.
thanks
 
Thanks for the help, could you clear up the surface deformrity issue though. When I think of a surface of a neutron star I thin of it being very smooth , but our sun has lots of bubbling convection flows I imagine. SO what about massive stars, will they have more surface irregularitites?
 
Last edited by a moderator:
windy miller said:
Thanks for the help, could you clear up the surface deformrity issue though. When I think of a surface of a neutron star I thin of it being very smooth , but ur sun has lots of bubbling convection flows I imagine. SO what about massive stars, will they have more surface irregularitites?

Of course they will have surface irregularities. The Earth is very close to a sphere, but it has mountains and canyons. The height of any surface irregularities will depend on the surface gravity. The higher the surface gravity, the more potential energy it will take to produce a "bump". A massive supergiant like Betelgeuse has a relatively low surface gravity because of its large radius (about 0.5 m/s^2 according to Wikipedia), so we would expect relatively large surface irregularities. A massive main sequence star like Theta Orionis A1 is much smaller, so has a much larger surface gravity (20,000 m/s^2 according to Wikipedia), so we would expect much smaller surface irregularities. A neutron star has an enormous surface gravity so any irregularities will be extremely small.
 
  • Like
Likes lomidrevo and windy miller
phyzguy said:
Of course they will have surface irregularities. The Earth is very close to a sphere, but it has mountains and canyons. The height of any surface irregularities will depend on the surface gravity. The higher the surface gravity, the more potential energy it will take to produce a "bump". A massive supergiant like Betelgeuse has a relatively low surface gravity because of its large radius (about 0.5 m/s^2 according to Wikipedia), so we would expect relatively large surface irregularities. A massive main sequence star like Theta Orionis A1 is much smaller, so has a much larger surface gravity (20,000 m/s^2 according to Wikipedia), so we would expect much smaller surface irregularities. A neutron star has an enormous surface gravity so any irregularities will be extremely small.
Thanks that makes a lot off sense.
 
  • #10
phyzguy said:
Of course they will have surface irregularities. The Earth is very close to a sphere, but it has mountains and canyons. The height of any surface irregularities will depend on the surface gravity. The higher the surface gravity, the more potential energy it will take to produce a "bump". A massive supergiant like Betelgeuse has a relatively low surface gravity because of its large radius (about 0.5 m/s^2 according to Wikipedia), so we would expect relatively large surface irregularities. A massive main sequence star like Theta Orionis A1 is much smaller, so has a much larger surface gravity (20,000 m/s^2 according to Wikipedia), so we would expect much smaller surface irregularities. A neutron star has an enormous surface gravity so any irregularities will be extremely small.

just to add, one should also realize that average density of supergiant stars like Betelgeuse, can be as low as ## 10^{-8} \rho_{sun} ##, where ##\rho_{sun} = 1410 \ kg \ m^{-3}## is the average solar density. That means that average density of Betelgeuse is approximately ##10^5## times less then the density of air we breathe at sea level. It might be quite difficult to define any surface in such conditions :)
 
  • Like
Likes windy miller
Back
Top