A Map of Future Exoplanetary Discovery

Most of the alien worlds closest to our own are found around the smallest, dimmest nearby stars

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Astronomers know of more than 3,500 exoplanets—worlds orbiting stars other than our sun—and will probably find thousands more in the next few years. Some of these newfound worlds will resemble our own planet in size, composition and temperature. Yet many of these potential “mirror Earths” will be alien in one respect: they will orbit red dwarfs, also known as M dwarfs, rather than sunlike stars. M dwarfs are the universe's smallest, coolest stars, but they are also the hottest sites for exoplanet discovery, largely because of their sheer abundance. Although none are visible to the naked eye, they make up more than half of the 140 known stars within 20 light-years of the sun and harbor two thirds of the known exoplanets in that region (graphic). Even though M dwarfs are cool stars, planets orbiting close to them would be warm. Earth-like or not, these alien worlds are destined to become the ones we know best.

Credit: Nadieh Bremer; Sources: Jessie Christiansen and Eric Mamajek (consultants); NASA Exoplanet Archive and NASA Exoplanet Exploration Program (data)

Lee Billings is a science journalist specializing in astronomy, physics, planetary science, and spaceflight and is senior desk editor for physical science at Scientific American. He is author of a critically acclaimed book, Five Billion Years of Solitude: The Search for Life Among the Stars, which in 2014 won a Science Communication Award from the American Institute of Physics. In addition to his work for Scientific American, Billings’s writing has appeared in the New York Times, the Wall Street Journal, the Boston Globe, Wired, New Scientist, Popular Science and many other publications. Billings joined Scientific American in 2014 and previously worked as a staff editor at SEED magazine. He holds a B.A. in journalism from the University of Minnesota.

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Scientific American Magazine Vol 317 Issue 6This article was published with the title “Meet the Neighbors” in Scientific American Magazine Vol. 317 No. 6 (), p. 94
doi:10.1038/scientificamerican1217-94

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