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We present the detection of five planets—Kepler-62b, c, d, e, and f—of size 1.31, 0.54, 1.95, 1.61 and 1.41 Earth radii (R ⊕ ), orbiting a K2V star at periods of 5.7, 12.4, 18.2, 122.4, and 267.3 days, respectively. The outermost planets, Kepler-62e and -62f, are super-Earth-size (1.25 R ⊕ < planet radius < 2.0 R ⊕ ) planets in the habitable zone of their host star, respectively receiving 1.2 ± 0.2 times and 0.41 ± 0.05 times the solar flux at Earth's orbit. Theoretical models of Kepler-62e and -62f for a stellar age of ~7 billion years suggest that both planets could be solid, either with a rocky composition or composed of mostly solid water in their bulk.

The solar eclipse coming August 21 offers students the opportunity not only to explore the geometry of the solar system but also to learn about exoplanets transiting distant stars. Students can glimpse a great frontier of science: the search for other worlds and life. This article presents information on exoplanets, discovering planets around distant stars, and an activity to incorporate into the classroom.

Humans have long wondered about life in the universe. Are we alone? Is Earth unique? What is it that makes our planet a habitable one, and are there others like Earth? NASA's Kepler Mission seeks the answers to these questions. Kepler is a space-based, specially designed 0.95 m aperture telescope. Launching in 2009, Kepler is NASA's first mission capable of finding Earth-size and smaller planets in the habitable zone of other stars in our galaxy. Therefore, the Kepler Mission provides an opportunity for interdisciplinary science teaching, as it combines Earth and space science with life sciences. Teachers and students can bring this mission down to Earth by using the accompanying poster, partaking in classroom activities, and visiting the mission's website.

Koch et al discuss the Kepler Mission, NASA's 10th Discovery mission, which seeks to answer questions about life in the universe. A space-based, specially designed 0.95 m aperture telescope, Kepler is NASA's first mission capable of finding Earth-size and smaller planets in the habitable zone of other stars in the galaxy. Koch et al also explain how the mission helps in interdisciplinary science teaching.

The Kepler mission has discovered over 2500 exoplanet candidates in the first two years of spacecraft data, with approximately 40% of them in candidate multi-planet systems. The high rate of multiplicity combined with the low rate of identified false-positives indicates that the multiplanet systems contain very few false-positive signals due to other systems not gravitationally bound to the target star (Lissauer, J. J., et al., 2012, ApJ 750, 131). False positives in the multi- planet systems are identified and removed, leaving behind a residual population of candidate multi-planet transiting systems expected to have a false-positive rate less than 1%. We present a sample of 340 planetary systems that contain 851 planets that are validated to substantially better than the 99% confidence level; the vast majority of these have not been previously verified as planets. We expect ~2 unidentified false-positives making our sample of planet very reliable. We present fundamental planetary properties of our sample based on a comprehensive analysis of Kepler light curves and ground-based spectroscopy and high-resolution imaging. Since we do not require spectroscopy or high-resolution imaging for validation, some of our derived parameters for a planetary system may be systematically incorrect due to dilution from light due to additional stars in the photometric aperture. None the less, our result nearly doubles the number of verified exoplanets.