Mercury Database

http://arxiv.org/abs/1605.07603 The intriguing exoplanet candidate KIC 12557548b is believed to have a comet-like tail of dusty debris trailing a small rocky planet. The tail of debris scatters up to 1.3% of the stellar light in the Kepler observatory’s bandpass (0.42 um to 0.9 um). Observing the tail’s transit depth at multiple wavelengths can reveal the […]

via Reduced Activity And Large Particles From the Disintegrating Planet Candidate KIC 12557548b [EPA] — arXiver

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