A sub-Mercury-sized exoplanet (Nature, 2013)

• Eric Agol
• Jonathon Fortney

Full Citation:
Barclay, T., Rowe, J., Lissauer, J. et al. A sub-Mercury-sized exoplanet. Nature 494, 452–454 (2013). https://doi.org/10.1038/nature11914

Abstract:
Since the discovery of the first exoplanets1,2, it has been known that other planetary systems can look quite unlike our own3. Until fairly recently, we have been able to probe only the upper range of the planet size distribution4,5, and, since last year, to detect planets that are the size of Earth6 or somewhat smaller7. Hitherto, no planets have been found that are smaller than those we see in the Solar System. Here we report a planet significantly smaller than Mercury8. This tiny planet is the innermost of three that orbit the Sun-like host star, which we have designated Kepler-37. Owing to its extremely small size, similar to that of the Moon, and highly irradiated surface, the planet, Kepler-37b, is probably rocky with no atmosphere or water, similar to Mercury.

URL:
https://www.nature.com/articles/nature11914

VPL Research Tasks:
Task E: The Observer