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[personal profile] rfmcdonald
Will Baird at The Dragon's Tales, in his own linkage about Alpha Centauri Bb, pointed me to astronomer Greg Laughlin's analysis of the whole situation--planet, star, technology--at his blog systemic.

It's very thorough. For starters, Laughlin notes that it might be possible to see Bb eclipse its sun.

Alpha Cen B has a radius about 90% as large as the Sun. This means that transits, if they occur, would have a maximum photometric depth of ~0.01%, and would last up to three hours. These numbers make for a challenging, but by no means impossible, detection. HST (perhaps using the FGS instrument) should be able to reach a transit of this depth, and given that the phase, the depth, and the period are known in advance, I think that a purpose-engineered ground-based solution can be made to work as well. For example, see this post on orthogonal transfer arrays — Alpha Cen B delivers almost 5 megawatts to the Earth, and Alpha Cen A is a nice comparison star right next door.


He later goes into greater detail about the situation, covering everything from the stellar weather of Alpha Centauri B to the way B's changing velocity was measured to exacting detail. One thing Laughlin notes is worth sharing: if Venus, in its current orbit, circled the dimmer Alpha Centauri B, it would be squarely in the middle of B's habitable zone and could plausibly support an Earth-like climate. The current data certainly doesn't exclude this possibility.
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