Solve Obler's Paradox: Calculate Universe Size in Parsecs & Light Years

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SUMMARY

The discussion addresses Obler's Paradox by calculating the necessary size of the universe in parsecs and light years to prevent the paradox from occurring. It establishes that if stars are uniformly distributed with a density of approximately 1 star per cubic parsec, the universe must be sufficiently large for photons to collide with particles before reaching its edge. The equations provided, including κ = nσr/ρ, highlight the relationship between the total cross section per unit mass and the number of atoms per unit mass, which are critical in determining the universe's dimensions.

PREREQUISITES
  • Understanding of Obler's Paradox
  • Familiarity with photon-particle interactions
  • Knowledge of astrophysical density concepts
  • Basic grasp of mathematical equations related to cross sections
NEXT STEPS
  • Research the implications of Obler's Paradox in cosmology
  • Study the concept of photon mean free path in astrophysics
  • Learn about the distribution of stars in the universe
  • Explore the mathematical modeling of cosmic structures
USEFUL FOR

Astronomers, astrophysicists, students of cosmology, and anyone interested in the fundamental questions of universe size and structure.

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Homework Statement


Suppose all stars had the same radius as the Sun, and they were distributed throughout the universe with the same density as we have nearby- about 1 star per cubic parsec. Approximatly how bigh in parsecs and light years would the universe have to be in order to avoid Oblers Paradox?


Homework Equations


Think of light as a particle- how far does the photon have to go until it hits another particle?



The Attempt at a Solution


photon- particle relation xr= 1/an
tr= 1/anc
κ= nσr/ρ where (n/ρ) is the number of atoms per unit mass and κ= total cross section per unit mass
 
Physics news on Phys.org
The universe must be as large as necessary for the photon to hit another particle before it reaches the edge of the universe. Therefore, the size in parsecs and light years would depend on the total cross section per unit mass and the number of atoms per unit mass.
 

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