More Than Half of Kepler's Giant Exoplanets Were False Positives
StartsWithABang writes: By surveying an area of the sky containing over 150,000 stars visible to it, the Kepler satellite monitored each one over a multi-year period looking for periodic changes in brightness. Thousands of planetary candidates emerged via the transit method, where periodic dips of 3% or less were noted with regularity. However, a follow-up study has come out on the giant exoplanets, finding that over 50% of them aren't giant planets after all, but wound up being eclipsing binary stars. Perhaps our lone star Solar System is the oddity, after all.
"A fanatic is one who can't change his mind, and won't change the subject." -- Winston Churchill
We all live in a lone star state, even those of us who don't live in Texas.
They are "false positives" in the sense that the stellar companion may be a small star or a brown dwarf instead of a "planet". But the distinction between a "big hot gas giant" and a "brown dwarf" is fairly academic, in particular if you're concerned with things like habitability.
So someone comes up with a list of things that might be planets, then someone does further analysis and finds out that some aren't. Even (gasp) 52% of them! Science must therefore be useless.
No, that's how science works -- you do an experiment, examine the results, then refine your experiment. Or someone else does. Repeat ad nauseum.
I wouldn't really call it false positives since there's a sliding scale between giant planet and star.
It would have been a lot worse if it was revealed that there was no object at all.
If builders built buildings the way programmers wrote programs, then the first woodpecker would destroy civilization.
It's terribly incorrect, to say, as the summary says, "Perhaps our lone star Solar System is the oddity, after all" - to the point of blunt stupidity.
Kepler's transit method will find some exoplanets, or at least the signs that something is worth taking a closer look at, but it also relies on a system's elliptical plane being aligned just so such a large exoplanet can cross the path of the star - in other words, we have to be able to see that plan edge-on. This reduces the likelihood of practically using this method to actually find something around 100-to-1, if it even exists.