Understanding the Upper Mass Limit of Neutron Stars: A Quick Question

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SUMMARY

The upper mass limit of neutron stars is theorized to be approximately 2 solar masses. This figure is supported by various astrophysical studies and is distinct from the upper mass limit of white dwarfs, which is 1.4 solar masses, known as the Chandrasekhar limit. The discussion references a 9-year-old book that aligns with this understanding, confirming the established mass limit for neutron stars.

PREREQUISITES
  • Understanding of stellar evolution and types of stars
  • Familiarity with the Chandrasekhar limit
  • Basic knowledge of astrophysics terminology
  • Awareness of neutron star formation processes
NEXT STEPS
  • Research the implications of the 2 solar mass limit on neutron star stability
  • Explore recent studies on neutron star mass measurements
  • Learn about the differences between neutron stars and white dwarfs
  • Investigate the role of neutron degeneracy pressure in stellar structures
USEFUL FOR

Astronomy students, astrophysicists, and anyone interested in stellar physics and the characteristics of neutron stars.

kokain
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I am trying to figure something out and forgot the upper mas of a nuetron star. I remember (I think) that the upper mass of a white dwarf is 1.4suns but I can't remember the other.
 
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The book I referenced for this is 9 years old now, but it theorizes 2 solar masses for a neutron star.
 
Thank you, that sounds right.
 

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