How Do Stars Achieve Their Massive Sizes?

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SUMMARY

Stars achieve massive sizes through processes such as accretion and potential coalescence of lower mass stars. Hydrogen fusion initiates around 100 Jupiter Masses (MJup), but larger stars, exceeding 200 solar masses (Msun), form under specific environmental conditions that allow for continued accretion of matter. High core temperatures are essential for fusion to occur, and the formation of high mass stars remains a complex topic with ongoing research into the mechanisms involved, including the influence of density in their formation environments.

PREREQUISITES
  • Understanding of hydrogen fusion processes
  • Knowledge of stellar formation and evolution
  • Familiarity with concepts of accretion and hydrostatic equilibrium
  • Basic grasp of radiation pressure effects on stellar structures
NEXT STEPS
  • Research the role of environmental density in star formation
  • Study the mechanisms of stellar coalescence and mergers
  • Explore the implications of radiation pressure on massive stars
  • Investigate the lifecycle of high mass stars and their end stages
USEFUL FOR

Astronomers, astrophysics students, and anyone interested in the complexities of star formation and the characteristics of massive stars.

discord73
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If Hydrogen fusion starts around 100JM (Jupiter Masses) then how do the larger stars get so massive? I was watching The Universe and it said some stars are over 200 solar masses and higher. How can a star get so massive?
 
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discord73 said:
If Hydrogen fusion starts around 100JM (Jupiter Masses)

Well, what the start of hydrogen fusion really depends upon is temperature. If the core temperature is high enough, fusion will occur. I suppose it is possible that 100 MJup is the least massive object for which this can be the case, but I have to admit I am unsure.


discord73 said:
then how do the larger stars get so massive?

I'm not totally sure what you're asking here. You realize it is possible for matter to continue to accrete onto a protostar? If your question is, "what determines the masses with which stars will form?", then I think the answer might be "nobody knows for sure." People have ideas. There is the idea that there might be some dependence upon environment. For instance, in a dense environment, more matter can continue to accrete, causing the central temperature to get higher before hydrostatic equilibrium is achieved. In a less dense environment, maybe hydrostatic equilibrium is achieved at a lower mass. In any case, high mass star formation is particularly puzzling. People are not sure whether this accretion picture is accurate, or whether the highest masses of stars need to form by coalescence (i.e. by the merger of several lower mass stars that are in the process of formation).


discord73 said:
I was watching The Universe and it said some stars are over 200 solar masses and higher. How can a star get so massive?

I am pretty sure that around 100 Msun is the upper limit beyond which a star begins to blow itself apart (i.e. blow away its outer layers) due to radiation pressure (because the more massive a star is, the more luminous it is).
 

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