Close the door on your way out - Life lit by a blue dwarf star
I'm seeking a hard science setting for a piece of xenofiction with a decidedly non-sciencey feel. That said, there is no magic or magic technology.
The idea is as follows:
- A red dwarf star has a rocky, icy planet well outside the habitable zone.
- After ~6 trillion years the red dwarf begins a transition into its blue dwarf stage for a further 400 billion years
- The massively increased stellar luminosity of the blue dwarf stage melts the icy planet turning it into a habitable planet, on which a civilisation develops. Since the planet is not too close to the star, it is not tidally locked, but is now in the habitable zone of a star with similar luminosity to the sun (according to article linked above).
- A timeline of 400 billion years is allowed for the creation of a habitable planet and for evolution.
This civilisation would be very alone in the universe at the end of the stellar phase of the universes evolution, with perhaps only a few other blue dwarf stars visible in the night sky, if any. All the other stars have turned into black dwarfs.
Obviously the timescales are immense so my question is this:
Is the notion of a planetary thawing of a truly ancient rocky ice planet some 6 trillion years after its formation is within the realms of plausibility.
This post was sourced from https://worldbuilding.stackexchange.com/q/23183. It is licensed under CC BY-SA 3.0.
1 answer
Yes, it can happen.
For this to be possible, you first have to put the planet far enough away that it can become totally icy. Then, after the temperature rises as the red dwarf transitions into a blue dwarf, the habitable zone must encompass the planet's orbit, melting the ice and making it a better place for life. We can easily calculate whether or not the final habitable zone can ever extend far enough for this to be possible.
Your initial goal is to place the planet "well outside the [initial] habitable zone". That's fine. We can find the initial inner and outer boundaries of the habitable zone using the formulae found here. The outer radius of the initial habitable zone is
You say you want to have an ice planet. We can estimate the inner radius at which it can form by calculating the distance of the initial frost line. If we use the model attributed to Hayashi (1981) by Ida & Lin (2005), then
For lack of more information, though, I'm going to have to stick to the original estimate.
Your article states that the initial surface temperature of the star is ~2230 K, prior to entering the blue dwarf phase. It then rises to ~5810 K, a change of a factor of about 2.5 The luminosity of a blackbody is proportional to its temperature to the fourth power (see the Stefan-Boltzmann law), so the inner and outer radii of the habitable zone are proportional to the temperature squared. This means that the final outer edge will be ~6 times as far out as it originally was - way beyond the initial frost line, about three times as far out.
This seems pretty good, but what about the inner edge of the final habitable zone. Where will that be? According to the same site that provided the formula for the outer edge, the inner edge will be
So, yes, from at least these estimates, the scenario is quite plausible.
1 Some results state that the habitable zone should be even smaller, although others disagree and say that it should be bigger.
2 Even more drastic changes are shown in Martin & Livio (2012).
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