- #1
onomatomanic
- 103
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Hi all,
I'd like to write a story whose setting is a planet that is, on the one hand, hospitable to earth-like flora and fauna, while on the other hand being as different as possible from Earth in as many respects as possible. In other words, which parameters can I fiddle with without greatly affecting surface conditions. Not exactly a novel idea, per se - one might say one has to look hard for sci-fi in which extrasolar planets don't have an extra sun or moon or two... but I'd like to go a bit deeper than that, while approaching the matter as scientifically as possible.
What I'm looking for are both new ideas and feedback on the ones I've come up with so far.
Okay, that's where I'm at, for now.
TIA for any constructive replies! :)
ETA: x-posted @ http://www.astronomyforum.net/gener...-how-design-weird-but-comfortable-planet.html, http://cs.astronomy.com/asycs/forums/t/45709.aspx
I'd like to write a story whose setting is a planet that is, on the one hand, hospitable to earth-like flora and fauna, while on the other hand being as different as possible from Earth in as many respects as possible. In other words, which parameters can I fiddle with without greatly affecting surface conditions. Not exactly a novel idea, per se - one might say one has to look hard for sci-fi in which extrasolar planets don't have an extra sun or moon or two... but I'd like to go a bit deeper than that, while approaching the matter as scientifically as possible.
What I'm looking for are both new ideas and feedback on the ones I've come up with so far.
- The basic physical characteristics (size and density) of the planet are more or less fixed, it seems to me, by the requirement that composition, gravity and atmosphere have to be earth-like.
- As concerns orbital and rotational dynamics, temperature (both average and variations) is of course the main concern as far as habitability is concerned. The following assumes that the sun is the dominant source of energy for the planet, which seems inevitable to me. In the case of Earth solar radiation contributes almost ten orders of magnitude more than internal effects like radioactive decay, and it seems unlikely that any non-negligible process that Earth is lacking could compete.
- Rotational period: The length of the day determines the temperature fluctuations between day and night. Assuming similar heat buffering and heat transfer processes as those on Earth, I'm thinking I can't make the day significantly longer than the terrestrial one. However, shortening it doesn't seem to present any immediate problems. What would be the limiting factor here? Coriolis storms? Tides (depending on satellites, obviously)?
- Axial tilt: Main driving force for seasonal change. Decreasing it from Earth's value towards zero makes things more and more boring. What are the effects of increasing it, in detail? If I've got this right, the extreme case of a 90-degree-inclination should mean that the annual average temperature at the poles and at the equator is more or less equal: The former still experience a single "day" and "night" each year, but the sun approaches the zenith during that day, which would make a radical difference. The latter experiences mild but definite winters during the polar days, as the sun doesn't climb far above the horizon. How about intermediate latitudes and inclinations?
- Orbital period: Fairly tightly bounded by the solar mass, which determines the solar luminosity, hence the habitable zone, and hence the orbital radius. Obvious limits here are imposed by standard stellar evolution - too heavy, and the sun is too short-lived for planet formation, too light, and nuclear fusion never ignites at all. Are there narrower limits? Is a Sun-like ("yellow") spectrum particularly suitable for earth-like life?
- Orbital eccentricity: This one seems quite interesting to me. A planet with small axial tilt and large orbital eccentricity would have a global summer during perihelion and a global winter during aphelion, accompanied by a visible change in solar size. I'm not quite sure how to figure this one out quantitatively, though. My back-of-the-envelope calculation went like this: Earth's temperate latitudes receive something like four times as much incident solar energy during summer as during winter (days twice as long and sun twice as high), which by the black body law predicts a 40% change in temperature (J ~ T^4). The actual change in temperature is at most 10% (30 K) for coastal and 20% for continental climates, so heat buffering and transfer processes must be taken into account. At least the latter of these would work very differently for eccentricity-driven seasons, though, so... non-trivial.
I found http://discovermagazine.com/2002/nov/featcircles" which gives some modelling results, at any rate.
- One of the more obvious considerations is to use a binary star system rather than a single sun. It can either be a distant binary in which the planet circles one of the two stars, but that option doesn't seem all that interesting: The second star has to be quite far away for the planetery orbit to remain stable, so it would primarily be a visual addition to the sky with little influence on the planetary conditions. Or, it can be a tight binary in which the planet circles the centre of mass of the system. Is it feasible for a planet to survive the death of one its suns? If so, the tight binary could consist of a normal star and a compact object, with mass transfer between the two via an accretion disk, etc. Though I suppose one would have to look at the radiative conditions in such a system, which might not be all that healthy... magnetic fields to the rescue, maybe? Other problems with this scenario?
Okay, that's where I'm at, for now.
TIA for any constructive replies! :)
ETA: x-posted @ http://www.astronomyforum.net/gener...-how-design-weird-but-comfortable-planet.html, http://cs.astronomy.com/asycs/forums/t/45709.aspx
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