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super-puff
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super-puff

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Also known as super-puff planet

thumb|Artistic representation of a super-puff planet A super-puff is a type of exoplanet with a mass only a few times larger than Earth's but with a radius larger than that of Neptune, giving it a very low mean density. They are cooler and less massive than the inflated low-density hot-Jupiters.

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Vinony's link graph records 254 inbound references to super-puff, and connects out to list of planet types, outer space and cosmic dust.

It sits within the topics Giant planets and Types of planet.

Vinony links it to 15 Wikipedia language editions.

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Subclass of
gas giant

via Wikidata · CC0

~2 min read

Encyclopedic overview

2 sections
Contents
  • Formation hypotheses
  • References

thumb|Artistic representation of a super-puff planet A super-puff is a type of exoplanet with a mass only a few times larger than Earth's but with a radius larger than that of Neptune, giving it a very low mean density. They are cooler and less massive than the inflated low-density hot-Jupiters.

The most extreme examples known are the three planets around Kepler-51 which are all Jupiter-sized but with densities below 0.1 g/cm3. These planets were discovered in 2012 but their low densities were not discovered until 2014. Another example is Kepler-87c.

Excerpted from Wikipedia’s “super-puff” article, available under the CC BY-SA 4.0 licence.

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