<egg> !wpn UmbralRaptor
* Qboid gives UmbralRaptor a spectral 555 timer
<UmbralRaptor> !wpn egg
* Qboid gives egg an analytic blurglecruncheon
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<Greys> I think what I'd like is a graph corelating sight horizon factors to an estimated minimum star by range
<Greys> this might need to be a 3D graph
<UmbralRaptor> hrm
<Greys> at the very least it's going to need multiple lines to represent different kinds of stars
<Greys> small stars will need to be brighter faster than big stars, etc
<Greys> btw I am ignoring nebula and galaxies entirely
<Greys> so the main sequence is determined by luminosity and color temperature; but it also relates to diameter (indirectly?)
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<Greys> are there any other factors I'm missing for whether a star would be visible? so then we could project the main sequence on a range axis with a ribbon to represent visibility factor
<Greys> then this would inform the density of representitive star points in the emulation
<UmbralRaptor> For medium mass stars, there's a rough scaling of mass with everything (temp, diameter, luminosity)
<UmbralRaptor> I'll need to check my notes on exact mass range, but something like L~M^3.5 between 0.5 and 5 solar masses.
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<UmbralRaptor> Okay, from notes: there's a rough empirical scaling of L = M^3.7, with L and M in solar luminosities and masses.
<UmbralRaptor> It holds over 0.3 to 12 solar masses(!)
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