World Builders help

Isn't the '...on a roll of 12, DM+Law Level' ?
Oh, so it's just 2D+Law Level, no other DMs?

Was a bit unclear to me since it's still under the System of Justice section, so I thought it might be another roll (with DM+ for Law Level) on the table above it.
 
Apologies if this has already been covered, but wondered if there were any semi-automated tools to generate the superb detail of the World Builders, without having to create your own working sheet?

Something that takes input parameters, and outputs results to a standard format that can then be edited and manipulated for hand outs or a VTT journal?

I'm not a coder, so it is a bit beyond me. :)
 
Apologies if this has already been covered, but wondered if there were any semi-automated tools to generate the superb detail of the World Builders, without having to create your own working sheet?

Something that takes input parameters, and outputs results to a standard format that can then be edited and manipulated for hand outs or a VTT journal?

I'm not a coder, so it is a bit beyond me. :)
Not sure if this is what you're looking for, but if you can copy/paste a table into Excel, this might do the trick for you:

 
Not sure if this is what you're looking for, but if you can copy/paste a table into Excel, this might do the trick for you:

These are the sheets you are looking for.....

{deep James Earl Jones voice}
 
Yeah, I messed around with it and didn't come up with anything better. The first example you you mention is based on the problem with circumbinaries , and unless at least one star is bright, any Tatooine is going to be frozen.
Speaking of circumbinaries, when working out the innermost orbit slot, the equation uses MAO, If a primary has a companion, any orbits below .5 + ECC, are unavailable. Should I still be using MAO in the calculation, or the first allowable slot AFTER the companion's effect is added?
 
Speaking of circumbinaries, when working out the innermost orbit slot, the equation uses MAO, If a primary has a companion, any orbits below .5 + ECC, are unavailable. Should I still be using MAO in the calculation, or the first allowable slot AFTER the companion's effect is added?
It should be what's allowable after the companion's orbit is taken into account.
 
Another question popped up as I've been going through the generation procedure for a new sector.

So, to add a little flavor to my system generation, I've been rolling the standard age dice (D6x2 + D3-1 + d1000/1000 Gy) and, if it exceeds the MS lifespan for the Class V star, do a little jiggery-pokery to taste with the individual dice results to come up with a percentage of MS lifespan (which may end up >100%).

Now, that said, when said Class V star is turned into a Class IV by that procedure, I've been upping the Mass (like the moron that I now realize I am). But, some reading I've been doing shows that I shouldn't be increasing the star's mass at all, which makes me think I've been interpreting the chart on p.17 wrong.

For stellar mass, is it the intent of the chart on p.17 that the listed mass for each listed spectral type is the mass of the star through its entire life up to that point? If so, should I then change the spectral classification of said star based on its mass, instead of (as I've been ignorantly doing) increasing mass to fit the spectral classification? (Of course, as I'm typing this, my brain is going "Yes, that's exactly what you should be doing!")
 
Another question popped up as I've been going through the generation procedure for a new sector.

So, to add a little flavor to my system generation, I've been rolling the standard age dice (D6x2 + D3-1 + d1000/1000 Gy) and, if it exceeds the MS lifespan for the Class V star, do a little jiggery-pokery to taste with the individual dice results to come up with a percentage of MS lifespan (which may end up >100%).

Now, that said, when said Class V star is turned into a Class IV by that procedure, I've been upping the Mass (like the moron that I now realize I am). But, some reading I've been doing shows that I shouldn't be increasing the star's mass at all, which makes me think I've been interpreting the chart on p.17 wrong.

For stellar mass, is it the intent of the chart on p.17 that the listed mass for each listed spectral type is the mass of the star through its entire life up to that point? If so, should I then change the spectral classification of said star based on its mass, instead of (as I've been ignorantly doing) increasing mass to fit the spectral classification? (Of course, as I'm typing this, my brain is going "Yes, that's exactly what you should be doing!")
I would agree that you should not increase the mass, but rather increase the size. But to what?
I note that the sun (G2V) is predicted to become a red giant, but if size TBC.
I don’t have the book to hand but I would say that, in principle, if your main sequence star is too old to remain in the main sequence then you should increase its size to IV or beyond. Check the age limits given in the text and keep going as needed.
 
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