Line of sight and star density question.

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Discussion Overview

The discussion revolves around calculating the average distance one could see in an infinitely large universe before encountering a star, given specific parameters such as star density and stellar radius. The context includes aspects of theoretical physics and mathematical reasoning related to the concept of mean free path.

Discussion Character

  • Homework-related, Mathematical reasoning, Exploratory

Main Points Raised

  • One participant seeks assistance with a homework problem regarding the average distance to a star in a universe with a specified star density and radius.
  • Another participant suggests looking up the concept of "mean free path" as a potential approach to the problem.
  • A different participant emphasizes the importance of unit consistency, noting that the cross-sectional area of the Sun should be converted to Mpc2 to match the density units of Mpc-3.
  • There is a mention of a calculated cross-sectional area for the Sun and a query about how to combine this with the given density to determine the mean free path.
  • One participant proposes using dimensional analysis to derive a relationship between the given quantities, although they note that this method may not yield constants or dimensionless results.

Areas of Agreement / Disagreement

Participants have not reached a consensus on the approach to solving the problem, and multiple viewpoints on how to tackle the calculations remain present.

Contextual Notes

Participants express uncertainty regarding the implications of the universe's size and age in relation to the problem, with one suggesting that a significantly larger universe would be required to encounter a star.

Who May Find This Useful

This discussion may be of interest to students or individuals exploring concepts related to astrophysics, particularly those dealing with star density and observational limits in cosmology.

Illuminati
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This is blatant homework help that I don't know how to approach. Any hints would be appreciated.

Suppose you are in an infinitely large old universe in which the average density of stars is n = 109 Mpc-3 and the average stellar radius is equal to the sun's radius is R = 7*108. How far, on average, could you see in any direction before your line of sight strikes a star?
 
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Look up "mean free path".
 
Also, be careful of the units here-- if the density is in terms of Mpc-3, then you want the cross sectional area of the Sun in units of Mpc2 to avoid having to convert units during your calculation. wolframalpha.com tells me that the answer for the Sun is 2 times 10-38 Mpc2. How can you combine that with the density to get a distance, which will be the mean free path you want? (It would require a pretty darn big universe to hit a star-- for one thing, the universe would need to be almost 1019 times older than it actually is, right?)
 
You can use dimensional analysis to get something out of this, and then see if it makes sense to you. 1/L^3 and L^2 can be combined how to get L?

This won't get you any constants or other unit-less things though, but maybe it will help you see the problem more clearly.
 

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