User talk:EvenGreenerFish
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Re: Habitable zone diagram for solar system
[edit]Thanks for the question!
In the description of the HD 85512 diagram I link to the paper on arXiv [1] which gives the formulae, it also tabulates the value for a 5700K G2 star. The Sun at 5780 K is somewhat hotter.
The incident fluxes in units of the solar flux at the Earth's orbit of the six habitable zone boundaries (three inner, three outer) are given by:
Limit | Formula |
---|---|
Recent Venus | |
Runaway greenhouse | |
Water loss | |
CO2 cloud condensation | |
Maximum greenhouse | |
Early Mars |
Note the above expressions are based on interpolating points at 3700 K (M0 star), 5700 K (G2 star) and 7200 K (F0 star) so are not valid outside this range.
The flux can then be converted to distance using:
Where distance d is in AU, luminosity L is in solar luminosities and the incident flux S is in units of the solar flux at Earth.
The tabulated and interpolated values are as follows:
Limit | 5700 K (table) | 5780 K (interpolated) | ||
---|---|---|---|---|
Flux | Dist | Flux | Dist | |
Recent Venus | 1.76 | 0.75 | 1.77 | 0.75 |
Runaway greenhouse | 1.41 | 0.84 | 1.43 | 0.84 |
Water loss | 1.10 | 0.95 | 1.11 | 0.95 |
CO2 cloud condensation | 0.53 | 1.37 | 0.53 | 1.37 |
Maximum greenhouse | 0.36 | 1.67 | 0.36 | 1.66 |
Early Mars | 0.32 | 1.77 | 0.32 | 1.76 |
As you can see, moving from 5700 K to 5780 K does not make much difference!
Incidentally I would recommend you make the diagram as an SVG file rather than a PNG, this allows it to be scaled to any resolution and is ideal for diagrams. You can also put descriptive metadata into the files. Icalanise (talk) 21:00, 17 November 2012 (UTC)