Astronomers have confirmed 104 planets beyond the solar system that were spotted by NASA's revamped Kepler space telescope.
Launched in March 2009, Kepler spent four years staring at small patch of the sky looking for slight dips in the amount of light coming from about 140,000 target stars. Scientists then used the information to determine which light dips are caused by planets passing across the face of their parent stars, relative to Kepler's line of sight, as opposed to, for example, stellar flares or eclipsing binary stars.
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For stability, the telescope needs to be oriented nearly parallel to its orbital path around the sun, which is slightly offset from Earth's orbital plane, known as the ecliptic.
Two of the planets, K2-72c and 72e, are properly distanced from the host star for liquid water, if it exists. Because the star is about half the size of the sun and much dimmer, its so-called "habitable zone" is closer than where Mercury's orbits the sun in our solar system.
Scientists believe all four of K2-72's planets are rocky. The star is located about 181 light-years away in the direction of the Aquarius constellation.
Telescopes used to confirm the K-2 planets include: the North Gemini telescope and the W. M. Keck Observatory in Hawaii: the University of California Observatories' Automated Planet Finder: and the University of Arizona's Large Binocular Telescope.
The research is published in this week's Astrophysical Journal Supplement Series.
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