Analysis of Kepler data has yielded the smallest known mass for an exoplanet orbiting a normal star. Its mass and size are similar to those of Mars, setting a benchmark for the properties of exoplanets smaller than Earth. See Letter p.321
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Jontof-Hutter, D., Rowe, J. F., Lissauer, J. J., Fabrycky, D. C. & Ford, E. B. Nature 522, 321–323 (2015).
Borucki, W. et al. Science 327, 977–980 (2010).
Marcy, G. W. et al. Astrophys. J. Suppl. Ser. 210, 20 (2014).
Gautier, T. N. III et al. Preprint at http://arxiv.org/abs/1001.0352 (2010).
Fischer, D. A. et al. in Protostars and Planets VI (eds Beuther, H. et al.) 715–737 (Univ. Arizona Press, 2014).
Grant, R. History of Physical Astronomy (Bohn, 1852).
Ricker, G. et al. J. Astron. Telesc. Instrum. Syst. 1, 014003 (2014).
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Laughlin, G. A Mars-sized exoplanet. Nature 522, 290–291 (2015). https://doi.org/10.1038/522290a
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DOI: https://doi.org/10.1038/522290a