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  2. Mini-Neptune - Wikipedia

    en.wikipedia.org/wiki/Mini-Neptune

    Smaller gas planets and planets closer to their star will lose atmospheric mass more quickly via hydrodynamic escape than larger planets and planets farther out. [13] [14] [15] A low-mass gas planet can still have a radius resembling that of a gas giant if it has the right temperature. [16]

  3. Gas giant - Wikipedia

    en.wikipedia.org/wiki/Gas_giant

    The smallest known extrasolar planet that is likely a "gas planet" is Kepler-138d, which has the same mass as Earth but is 60% larger and therefore has a density that indicates a thick gas envelope. [16] A low-mass gas planet can still have a radius resembling that of a gas giant if it has the right temperature. [17]

  4. List of Solar System objects by size - Wikipedia

    en.wikipedia.org/wiki/List_of_Solar_System...

    For the giant planets, the "radius" is defined as the distance from the center at which the atmosphere reaches 1 bar of atmospheric pressure. [ 11 ] Because Sedna and 2002 MS 4 have no known moons, directly determining their mass is impossible without sending a probe (estimated to be from 1.7x10 21 to 6.1×10 21 kg for Sedna [ 12 ] ).

  5. Jupiter - Wikipedia

    en.wikipedia.org/wiki/Jupiter

    It is a gas giant with a mass more than 2.5 times that of all the other planets in the Solar System combined and slightly less than one-thousandth the mass of the Sun. Its diameter is eleven times that of Earth , and a tenth that of the Sun. Jupiter orbits the Sun at a distance of 5.20 AU (778.5 Gm ), with an orbital period of 11.86 years .

  6. Sudarsky's gas giant classification - Wikipedia

    en.wikipedia.org/wiki/Sudarsky's_gas_giant...

    Sudarsky's classification of gas giants for the purpose of predicting their appearance based on their temperature was outlined by David Sudarsky and colleagues in the paper Albedo and Reflection Spectra of Extrasolar Giant Planets [1] and expanded on in Theoretical Spectra and Atmospheres of Extrasolar Giant Planets, [2] published before any successful direct or indirect observation of an ...

  7. Kepler-37b - Wikipedia

    en.wikipedia.org/wiki/Kepler-37b

    Because of its small size, it is not expected to have an atmosphere. [6] Its radius is approximately 0.31 R 🜨 (about 1,980 kilometres (1,230 mi)), [2] slightly larger than the Moon [7] (0.27 R 🜨), but a little smaller than Mercury (0.38 R 🜨). Due to its small size, it is very likely Kepler-37b is a rocky planet with a solid surface. [6]

  8. Dwarf planet - Wikipedia

    en.wikipedia.org/wiki/Dwarf_planet

    A dwarf planet is a small planetary-mass object ... as are all the rounded satellites of the gas giants. ... Two known moons and one known ring. Makemake (2005 FY 9 ...

  9. 55 Cancri e - Wikipedia

    en.wikipedia.org/wiki/55_Cancri_e

    It was initially unknown whether 55 Cancri e was a small gas giant like Neptune or a large rocky terrestrial planet. In 2011, a transit of the planet was confirmed, allowing scientists to calculate its density. At first it was suspected to be a water planet.