Neptunian exoplanets are a class of exoplanets that are similar in size to the ice giants Neptune and Uranus in the Solar System. Neptunian exoplanets may have a mixture of interiors though all would be rocky with heavier metals at their cores. Neptunian planets typically have hydrogen- and helium-dominated atmospheres. There are several recognized subtypes of Neptunian exoplanets:
Hot Neptune – orbiting close to its star Helium planet – a hypothetical type that can form from hot Neptune via hydrogen evaporation, leaving a helium-dominated atmosphere Mini-Neptune – considerably smaller than Neptune but still having a thick hydrogen-helium envelope, relatively common Super-puff – inflated planets with unusually low mean density Hycean planet – a hypothetical transitional type to ocean planets with a thin, hydrogen-helium-dominated atmosphere overlaying a liquid water ocean
List of Neptunian exoplanets
Kepler Kepler-56b Kepler-102e
GJ GJ 436b
TOI TOI-421c TOI-532b TOI-824b TOI-1231b TOI-2374b TOI-4010b TOI-4010c TOI-4010d
LTT LTT 9779b
HAT HAT-P-26b HAT-P-11b
OGLE OGLE-2005-BLG-169Lb OGLE-2005-BLG-390Lb
Other Mu Arae c- first hot Neptune discovered NGTS-4b NGTS-14Ab KMT-2017-BLG-0165Lb
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