"She still has her dress that she was wearing the night of the abduction. Each time I see the dress, there is a little less of it to see as samples are taken and sent off to be analyzed in labs around the world."— Avis Ruffu, Rense.com

"NASA's Kepler Mission has discovered the first super-Earth orbiting in the habitable zone of a star similar to the Sun. A team of researchers, including Carnegie's Alan Boss, has discovered what could be a large, rocky planet with a surface temperature of about 22 degrees Celsius (72 degrees Fahrenheit), comparable to a comfortable spring day on Earth. [...]
     'This discovery supports the growing belief that we live in a universe crowded with life,' Boss said. 'Kepler is on the verge of determining the actual abundance of habitable, Earth-like planets in our galaxy.'"
— Science Daily
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"Scientists doing their first exploring of deep-sea vents in the Antarctic have uncovered a world unlike anything found around other hydrothermal vents, one populated by new species of anemones, predatory sea stars, and piles of hairy-chested yeti crabs.
     It was 'almost like a sight from another planet,' said expedition leader Alex Rogers, a professor of zoology at Oxford University."
—Stephanie Pappas, Live Science
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"The Drake equation is closely related to the Fermi paradox in that Drake suggested that a large number of extraterrestrial civilizations would form, but that the lack of evidence of such civilizations (the Fermi paradox) suggests that technological civilizations tend to disappear rather quickly. This theory often stimulates an interest in identifying and publicizing ways in which humanity could destroy itself, and then counters with hopes of avoiding such destruction and eventually becoming a space-faring species. A similar argument is the Great Filter, which notes that since there are no observed extraterrestrial civilizations, despite the vast number of stars, then some step in the process must be acting as a filter to reduce the final value. According to this view, either it is very hard for intelligent life to arise, or the lifetime of such civilizations must be relatively short.
     The Drake equation states that:

where:
N = the number of civilizations in our galaxy with which communication might be possible;
and
R* = the average rate of star formation per year in our galaxy
fp = the fraction of those stars that have planets
ne = the average number of planets that can potentially support life per star that has planets
fℓ = the fraction of the above that actually go on to develop life at some point
fi = the fraction of the above that actually go on to develop intelligent life
fc = the fraction of civilizations that develop a technology that releases detectable signs of their existence into space
L = the length of time for which such civilizations release detectable signals into space [...]"
— Wikipedia
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