Definition
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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© 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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