The star, EPIC 201367065, is a cool red M dwarf about half the size and mass of our Sun. At a distance of 150 light-years, the star ranks among the top 10 nearest stars known to have transiting planets. The star’s proximity means it’s bright enough for astronomers to study the planets’ atmospheres to determine whether they are like Earth’s atmosphere and possibly conducive to life.
“A thin atmosphere made of nitrogen and oxygen has allowed life to thrive on Earth. But nature is full of surprises. Many exoplanets discovered by the Kepler mission are enveloped by thick, hydrogen-rich atmospheres that are probably incompatible with life as we know it,” said Ian Crossfield from the University of Arizona in Tucson.
The three planets are 2.1, 1.7, and 1.5 times the size of Earth. The outermost planet, at 1.5 Earth radii, is the smallest and orbits far enough from its host star that it receives levels of light from its star similar to those received by Earth from the Sun, said Erik Petiguar from University of California, Berkeley, who discovered the planets January 6 while conducting a computer analysis of the Kepler data NASA has made available to astronomers. He calculated that the three planets receive 10.5, 3.2, and 1.4 times the light intensity of Earth, respectively.
“Most planets we have found to date are scorched. This system is the closest star with lukewarm transiting planets,” Petigura said. “There is a very real possibility that the outermost planet is rocky like Earth, which means this planet could have the right temperature to support liquid water oceans.”
Andrew Howard from the University of Hawaii noted that extrasolar planets are discovered by the hundreds these days, though many astronomers are left wondering if any of the newfound worlds are really like Earth. The newly discovered planetary system will help resolve this question, he said.
“We’ve learned in the past year that planets the size and temperature of Earth are common in our Milky Way Galaxy,” Howard said. “We also discovered some Earth-sized planets that appear to be made of the same materials as our Earth, mostly rock and iron.”
Kepler’s K2 mission
After Petigura found the planets in the Kepler light curves, the team quickly employed telescopes in Chile, Hawaii, and California to characterize the star’s mass, radius, temperature, and age. Two of the telescopes involved, the Automated Planet Finder on Mount Hamilton near San Jose, California, and the Keck Telescope on Mauna Kea, Hawaii, are University of California facilities.
The next step will be observations with other telescopes, including the Hubble Space Telescope, to take the spectroscopic fingerprint of the molecules in the planetary atmospheres. If these warm, nearly Earth-sized planets have puffy hydrogen-rich atmospheres, Hubble will see the telltale signal, Petigura said.
The discovery is all the more remarkable, he said, because the Kepler telescope lost two reaction wheels that kept it pointing at a fixed spot in space. Kepler was reborn in 2014 as “K2” with a clever strategy of pointing the telescope in the plane of Earth’s orbit, the ecliptic, to stabilize the spacecraft. Kepler is now back to mining the cosmos for planets by searching for eclipses, or “transits,” as planets pass in front of their host stars and periodically block some of the starlight.
“This discovery proves that K2, despite being somewhat compromised, can still find exciting and scientifically compelling planets,” said Petigura. “This ingenious new use of Kepler is a testament to the ingenuity of the scientists and engineers at NASA. This discovery shows that Kepler can still do great science.”
Kepler sees only a small fraction of the planetary systems in its gaze: those with orbital planes aligned edge-on to our view from Earth. Planets with large orbital tilts are missed by Kepler. A census of Kepler planets that the team conducted in 2013 corrected statistically for these random orbital orientations and concluded that one in five Sun-like stars in the Milky Way Galaxy have Earth-sized planets in the habitable zone. Accounting for other types of stars as well, there may be 40 billion such planets galaxy- wide.
The original Kepler mission found thousands of small planets, but most of them were too faint and far away to assess their density and composition and thus determine whether they are high-density rocky planets like Earth or puffy low-density planets like Uranus and Neptune. Because the star EPIC 201 is nearby, these mass measurements are possible. The host star, an M dwarf, is less intrinsically bright than the Sun, which means that its planets can reside close to the host star and still enjoy lukewarm temperatures.
According to Howard, the system most like EPIC 201 is Kepler 138, an M dwarf star with three planets of similar size, though none are in the habitable zone.
