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静水圧平衡

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The planetary-mass moons to scale, compared with Mercury, Venus, Earth, Mars, and Pluto (the other planetary-mass objects beyond Neptune have never been imaged up close). Borderline Proteus and Nereid (about the same size as round Mimas) have been included. Unimaged Dysnomia (intermediate in size between Tethys and Enceladus) is not shown; it is in any case probably not a solid body.[1]

惑星質量天体（PMO）とは？定義から多様な分類までを解説

惑星質量天体PMO静水圧平衡準褐色矮星
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Under geophysical definitions of a planet, there are more satellite and dwarf planets in the Solar System than classical planets.

惑星の定義を再考する天文学的視点と地球物理学的アプローチの違い

惑星の定義IAU地球物理学的定義静水圧平衡
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Diagram of a newly formed planet in a state of hydrostatic equilibrium

静水圧平衡のメカニズム天体の形状と大気を決定づける物理法則

静水圧平衡流体力学惑星科学重力
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Planetary-mass moons larger than Pluto, the largest Solar dwarf planet

惑星質量衛星天文学における「衛星惑星」の定義と正体

惑星質量衛星衛星惑星静水圧平衡ガニメデ
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気圧傾度力と流体力学の基礎圧力差がもたらす加速と現象

気圧傾度力流体力学静水圧平衡マグヌス効果
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