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Nature Research, Nature, 7438(494), p. 452-454, 2013

DOI: 10.1038/nature11914

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A sub-Mercury-sized exoplanet

Journal article published in 2013 by Thomas Barclay, Jason F. Rowe, Jack J. Lissauer, Daniel Huber, Francois Fressin, Steve B. Howell, Stephen T. Bryson, William J. Chaplin, Jean-Michel Désert, Eric D. Lopez, Geoffrey W. Marcy, Fergal Mullally, Darin Ragozzine, Guillermo Torres, Elisabeth R. Adams and other authors.
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Abstract

Since the discovery of the first exoplanet we have known that other planetary systems can look quite unlike our own. However, until recently we have only been able to probe the upper range of the planet size distribution. The high precision of the Kepler space telescope has allowed us to detect planets that are the size of Earth and somewhat smaller, but no previous planets have been found that are smaller than those we see in our own Solar System. Here we report the discovery of a planet significantly smaller than Mercury. This tiny planet is the innermost of three planets that orbit the Sun-like host star, which we have designated Kepler-37. Owing to its extremely small size, similar to that of Earth's Moon, and highly irradiated surface, Kepler-37b is probably a rocky planet with no atmosphere or water, similar to Mercury. ; Comment: Accepted and published in Nature (2013 Feb 28). This is the submitted version of paper, merged with the Supplementary Information