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Accurate knowledge of nEarth is necessary to plan future missions that will image and take spectra of Earthlike planets. Our result that Earths are relatively scarce means that a substantial effort will be needed to identify suitable target stars prior to these future missions.
Our result that Earths are relatively scarce means that a substantial effort will be needed to identify suitable target stars prior to these future missions.
This means there are a lot of Earth analogs out there — two billion in the Milky Way galaxy," researcher Joseph Catanzarite, an astronomer at NASA's Jet Propulsion Laboratory, told SPACE.com. "With that large a number, there's a good chance life and maybe even intelligent life might exist on some of those planets. And that's just our galaxy alone — there are 50 billion other galaxies."
Our result that Earths are relatively scarce means that a substantial effort will be needed to identify suitable target stars prior to these future missions.
When it comes to the 100 nearest sunlike stars within a few dozen light years, these findings suggest that only about two might have earth-like worlds
Nice trying to link documents and articles that are falsified. I said link a main stream source and you link a site that isn't even close to what i asked for.
So, Kepler can identify rocky planets with Earth-like masses that orbit at the right distance from their parent stars that liquid water can potentially exist on their surfaces*. However, what it can't do is tell us whether they have actually developed into life supporting worlds; and in our own solar system, Venus (about 25% closer to the sun than the Earth, about 80% of its mass, and yet a heat-sterilised volcanic hell-hole) provides a cautionary tale about getting too carried away if and when we start finding extra-solar 'Earths'. In reality, we'll have to wait for the likes of the Terrestrial Planet Finder or Darwin to directly identify possible signatures of life on any candidates that Kepler tracks down, by looking at the spectral characteristics of their atmospheres (although big Earth telescopes may also be able to contribute). However, this shouldn't be seen as a shortcoming. Kepler is designed to fill in a big gap in our present knowledge of solar systems outside our own: by the end of its mission, we'll have a much better idea of the average number of planets around a typical star, and the distribution of their sizes and orbits. We'll know whether our solar system, with its inner rocky planets and outer gas giants, is typical or unusual.
Our observations suggest that between 20% and 60% of Sun-like stars have evidence for the formation of rocky planets not unlike the processes we think led to planet Earth. That is very exciting.[22]
The discovery of Gliese 581 g, a Goldilocks planet only 20 light-years from Earth, has further called the Rare Earth hypothesis into question. With such proximity to Earth, exoplanetologists now estimate that the likelihood of finding an Earth-like planet in any given system in our galaxy is 10-20%,[36] bringing possible numbers close to Boss's guess
Originally posted by caf1550
reply to post by elevenaugust
i saw it on astronomy pic of the day a couple days ago but still very cool picture