[Space] Gliese 581
Anyone interested in seeing and/or writing up the Gliest 581 system to campaign-ready stats?
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Re: [Space] Gliese 581
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Rather than an unusually dynamic atmosphere with perpetual winds sweeping from a too hot perpetual dayside to a too cold eternal nightside, I suspect you would actually see some sort of static Venusian atmosphere. Some future astronomical project might be able to confirm this by getting a too strong Co2 spectrum from the the planet. So just personally I would not rush to write this place up as the target for Man's first extra-solar colonization effort or similar rpg scenario. To the best of my understanding the habitable zone of any M-class dwarf is going to be filled with tidally locked worlds. You'd need some sort of exotic scenario such as a double planet system tidally locked to each other but still spinning relative to the star or something like that. |
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As for exotic double-planet scenarios, it's very likely that the same tidal forces that result in an individual planet becoming tide-locked would split up a binary pair of planets in short order; it's the same reason why we can reasonably assume that a tidally locked world won't have any moons to speak of. A gas giant might get away with keeping some satellites; but I doubt that anything smaller would. |
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I believe the exact mechanism of Mercury's resonance isn't perfectly understood, though, and without a Jupiter-scale gas giant it might not happen. |
Re: [Space] Gliese 581
Plus Gliese 581 d is also around 3 earth masses, in the goldilocks zone, and not tidelocked.
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Re: [Space] Gliese 581
Mercury's resonance depends on it having a highly elliptical orbit; Gliese 581 g appears to have no ellipticity to speak of. And as far as we can tell, it probably is tidally locked, unless something strange is happening.
Really though, I was wondering what we could come up with by taking the solar and planetary data that we know about (the latter essentially being estimates of each planet's mass, distance from primary, and ellipticity) and plugging them into GURPS Space's planetary design system. Can the book handle them? If so, how interesting can we reasonably make the resulting system? In terms of g in particular, can it be made habitable without unduly stretching the existing numbers? The fact that it's nominally in the biozone is a step in that direction; but is it enough? |
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Do you have a source for your variant data? |
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Fred, assuming that it is possible that the atmosphere of the newly discovered planet isn't like that of Venus, what sort of life do you think might develop there? Or is any talk of life on the planet just wishful thinking, IYO? |
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