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  2. File:PIA02863 - Jupiter surface motion animation 10fps.ogv

    en.wikipedia.org/wiki/File:PIA02863_-_Jupiter...

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  3. Jupiter - Wikipedia

    en.wikipedia.org/wiki/Jupiter

    Jupiter radiates more heat than it receives through solar radiation, due to the Kelvin–Helmholtz mechanism within its contracting interior. [70]: 30 [71] This process causes Jupiter to shrink by about 1 mm (0.039 in) per year. [72] [73] At the time of its formation, Jupiter was hotter and was about twice its current diameter. [74]

  4. File:PIA02863 - Jupiter surface motion animation thumbnail ...

    en.wikipedia.org/wiki/File:PIA02863_-_Jupiter...

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  5. Comoving and proper distances - Wikipedia

    en.wikipedia.org/wiki/Comoving_and_proper_distances

    Comoving distance factors out the expansion of the universe, giving a distance that does not change in time except due to local factors, such as the motion of a galaxy within a cluster. [1] Proper distance roughly corresponds to where a distant object would be at a specific moment of cosmological time , which can change over time due to the ...

  6. Precession - Wikipedia

    en.wikipedia.org/wiki/Precession

    In other words, if the axis of rotation of a body is itself rotating about a second axis, that body is said to be precessing about the second axis. A motion in which the second Euler angle changes is called nutation. In physics, there are two types of precession: torque-free and torque-induced.

  7. Rotation period (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Rotation_period_(astronomy)

    In astronomy, the rotation period or spin period [1] of a celestial object (e.g., star, planet, moon, asteroid) has two definitions. The first one corresponds to the sidereal rotation period (or sidereal day), i.e., the time that the object takes to complete a full rotation around its axis relative to the background stars (inertial space).

  8. Dynamo theory - Wikipedia

    en.wikipedia.org/wiki/Dynamo_theory

    It is theorized that the Moon once had a magnetic field, based on evidence from magnetized lunar rocks, due to its short-lived closer distance to Earth creating tidal heating. [15] An orbit and rotation of a planet helps provide a liquid core, and supplements kinetic energy that supports a dynamo action.

  9. Differential rotation - Wikipedia

    en.wikipedia.org/wiki/Differential_rotation

    Stars and planets rotate in the first place because conservation of angular momentum turns random drifting of parts of the molecular cloud that they form from into rotating motion as they coalesce. Given this average rotation of the whole body, internal differential rotation is caused by convection in stars which is a movement of mass, due to ...