Celestial Mass Accretion Spectrum

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SUMMARY

The discussion centers on the development of a celestial mass accretion spectrum, which aims to categorize celestial objects based on mass, similar to the electromagnetic spectrum in physics. This spectrum would plot size (diameter) against a logarithmic mass scale, providing definitions for celestial bodies such as planets, stars, and black holes. The concept draws parallels to the Hertzsprung-Russell diagram and suggests that evolutionary trails could illustrate the mass changes of these objects over time. The idea also hints at the potential for calculating limits akin to the Chandrasekhar limit.

PREREQUISITES
  • Understanding of celestial object classification
  • Familiarity with logarithmic scales in scientific data
  • Knowledge of the Hertzsprung-Russell diagram
  • Basic concepts of mass accretion in astrophysics
NEXT STEPS
  • Research the Hertzsprung-Russell diagram and its applications in astronomy
  • Explore the concept of mass accretion in black holes and white dwarf interactions
  • Study the Chandrasekhar limit and its implications for stellar evolution
  • Investigate methods for visualizing complex astronomical data
USEFUL FOR

Astronomers, astrophysics students, and researchers interested in celestial object classification and mass accretion processes will benefit from this discussion.

Oriako
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Hello,
Over the past few weeks I've been interested in the idea of developing a celestial mass accretion spectrum, or in other words, a spectrum that places celestial objects of a given mass as being part of a band of that spectrum. This spectrum would help give definitions on what a planet is, what a star is, etc. and I'm sure could be a noticeable and useful landmark for astronomy just as the electromagnetic spectrum is in physics. The spectrum could plot the size (diameter) as a function of a logarithmic mass scale from left to right. Evolutionary trails could also be made to illustrate the lives of these objects as some will increase/decrease in mass in a certain way throughout their lives. It could be similar in fashion to the Hertzsprung-Russell diagram, except more expansive in its explanatory reach.

-Asteroids-Rocky Planets-Gas Planets-Brown Dwarfs-White Dwarfs-Star-Neutron Star-Galaxy-Black Holes, etc.

And there could be a general range that each of these fit into and possibly a limit to each could be calculated one day, just as the Chandrasekhar limit was calculated.

Thoughts, Comments?
 
Last edited:
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Nice idea but I always thought that significant mass accretes only in say : black holes,WD interaction in type1a supernovae and as suggested in the Accretion induced collapse.

I am not that much of an expert ,going to start my undergraduate at the end of this year.Correct me if I am mistaken.
I personally think that there is too much of data to be incorporated into a lone graph.
 

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