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Four rocky planets around one star? Kepler's new finds intrigue scientists

Four rocky planets around one star? Kepler's new finds intrigue scientists
Under the K2 mission, NASA's Kepler space telescope has found 104 confirmed exoplanets -- including several worlds that could be small and rocky, like Earth. (NASA/JPL-Caltech)

NASA's Kepler spacecraft has pulled in the largest crop of confirmed exoplanets ever found by the K2 mission – a triple-digit trove that includes a star system with four small planets that may be rocky, like Earth.

The 104 worlds, described in the Astrophysical Journal Supplement Series, bolster the idea that there may be plenty of rocky, Earth-sized planets circling the Milky Way's many stars.

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"K2 is significantly increasing the fraction of fairly small planets orbiting fairly bright stars," said lead author Ian Crossfield, an astronomer at the University of Arizona's Lunar and Planetary Laboratory in Tucson.

Among those interesting star systems is the M dwarf star K2-72, which lies about 181 light-years away in the direction of the constellation Aquarius. K2-72 hosts four planets with diameters that are each between 20% and 50% larger than Earth's, and so have a very good chance of being rocky planets like our own. All four planets lie really close to their star – closer than Mercury lies to the sun, in fact – but their temperatures are probably relatively cool because M dwarfs are relatively cool and dim.

NASA's Kepler spacecraft was sent into space in 2009 to stare at a single patch of sky and pick out planets crossing in front of their host stars. The spacecraft discovered loads of distant worlds but lost the first of its four reaction wheels in 2012 and the second in 2013, leaving the spacecraft crippled. Without at least three reaction wheels, the spacecraft was unable to point with the exquisite precision needed to spot the tiny dips in starlight caused by passing planets.

Kepler was down, but not out. Eventually, engineers came up with a clever solution: They could use the pressure of photons from the sun to act as a third reaction wheel, giving Kepler a second shot at life. Now, as part of the K2 mission, the spacecraft would no longer stare at a single patch of stars but scan wide swaths of sky in roughly 80-day periods. This allows Kepler to study a host of different phenomena, including black holes, supernovae and binary stars, all on top of its exoplanet work.

Because the K2 mission takes its cues from the scientific community, "we're able to target systems that we think are especially interesting," Crossfield said.

There's a slight downside: Because the spacecraft's can no longer point at the same area for more than 80 days, Kepler can no longer spot planets that are as far out from their host stars as Earth is from the sun. In fact, Crossfield said, the planets K2 has found basically have orbital periods that are 40 days or less – so that the spacecraft can detect them transiting across the planet twice during those roughly 80-day campaigns. (A single dip in the amount of light across the face of a star could be caused by a number of different phenomena, but seeing a repeated transit is what tells Kepler scientists that it's a planet.)

Kepler showed strong signs that there are plenty of planets, especially smallish planets around these smaller, cooler, so-called red dwarf stars.


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But even that downside has a silver lining: With such short observation campaigns, scientists can focus on the planets around M dwarfs, or red dwarf-type stars, which are significantly cooler and dimmer than stars like our sun. That means planets can circle really close to the star's surface and yet still have what Crossfield called "moderately cool" temperatures.

That's actually a pretty big plus in the search for potentially habitable exoplanets, because M dwarfs are thought to be the most common stars in our galaxy. They may well end up hosting many of the most promising targets for rocky, Earth-sized, habitable-zone planets.

"Kepler showed strong signs that there are plenty of planets, especially smallish planets around these smaller, cooler, so-called red dwarf stars," Crossfield said. "That's very exciting because these cool red dwarf stars dramatically outnumber stars like the sun."

To confirm that these planets were not false positives, the scientists followed up on Kepler's detections using a variety of ground telescopes, including the North Gemini Telescope, the W. M. Keck Observatory in Hawaii, the Automated Planet Finder at the University of California Observatories as well as the University of Arizona's Large Binocular Telescope.

In some ways, K2 is serving as the preamble to TESS, the Transiting Exoplanet Survey Satellite, set to launch in late 2017. And it's living on limited fuel reserves, which will probably only allow for two or so more years of operation. Even so, Kepler is already helping to identify some of the most promising targets for future missions like the James Webb Space Telescope, which will be able to probe these planet's atmospheres, to see if they've got the right ingredients to form a protective, life-friendly barrier above the planet's surface.

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