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OnlineVanadium 50 said:Catanzar1 et al. ApJ 738 151 (2011)
That's based on the first four months of Kepler data, it's only looking at Sun-like stars, and only considering "Earth analog" planets. Kepler had no chance to observe three transits for habitable planets around Sun-like stars in that time so there is a huge amount of extrapolation involved as well.
Edit: Wikipedia's article explicitly references this as "older study" for historic context, it has a much larger more recent estimate in the previous paragraph.
It does make a difference because the references count planets in the habitable zone, not some much larger area. Venus-like planets and moons are not included in the numbers for planets in the habitable zone, so you shouldn't include them in your comparison either.Vanadium 50 said:But this won't make any difference - if I shrink the habitable zone, the fraction of habitable planets goes up, but the number of candidates goes down by the same factor.
There are published numbers and reliable estimates we can discuss.Vanadium 50 said:However, I question the entire premise of your post. I reported this as speculation untethered by science, and the Mentors elected to keep this thread going. Fine. Your call. But you can't then turn around and complain my speculations don't match your speculations.