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Mini-Neptunes

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Mini-Neptune is the suggested term for a diverse class of exoplanets with masses in the upper range of Super-Earths (e.g., 7–10 Earth-masses, see the entry on Super-Earths). Unlike low-mass super-Earths, mini-Neptunes can have more massive and thicker atmospheres, and as a result, a small mean density. An example of a mini-Neptune could be Kepler-11f. With a radius of ~2.5 Earth-radii and mass of ~2 Earth-masses, this planet has a density of ~0.7 g/cc, similar to that of the gas-giant planet, Saturn.

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Correspondence to Nader Haghighipour .

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© 2014 Springer-Verlag Berlin Heidelberg

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Haghighipour, N., Kaltenegger, L. (2014). Mini-Neptunes. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1001-3

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  • DOI: https://doi.org/10.1007/978-3-642-27833-4_1001-3

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Online ISBN: 978-3-642-27833-4

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