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Physics Lesson 22.2.7 - Planetary Rotation around Own Axis

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Welcome to our Physics lesson on Planetary Rotation around Own Axis, this is the seventh lesson of our suite of physics lessons covering the topic of Sun and Planetary Motion, you can find links to the other lessons within this tutorial and access additional physics learning resources below this lesson.

Planetary Rotation around Own Axis

In addition to orbital motion (revolution) around the Sun, planets rotate around themselves as well. This rotation occurs according an axis passing through the centre of planet, known as planetary axis. This self-rotation derives from the fact that planets are objects with large dimensions; they are not merely material points as assumed in Kepler's Laws.

Planetary axis forms a certain angle to the Solar System axis (they are not parallel). The last column of planets table in the previous tutorial gives the values in degree of this inclination angle for all planets of our Solar System. Thus, for Mercury the angle is 0°. This means Mercury equator plane is in the same direction to the plane of its orbit around the Sun. on the other hand, Earth has an inclination of 23.45°. (Recall the deflection of Earth geographic poles in respect to the corresponding magnetic poles explained in Section 16, which is exactly 23.45°. This is because magnets point towards north-south direction of our galaxy). The figure below that gives a view taken from behind the Earth clarifies this point. The dashed line represents the North-South direction of our galaxy.

Physics Tutorials: This image provides visual information for the physics tutorial Sun and Planetary Motion

From the aforementioned table we have the following values for the angle of inclination: Mercury 0°, Venus 177.3°, Earth 23.45°, Mars 25.19°, Jupiter 3.12°, Saturn 26.73°, Uranus 97.86° and Neptune 120°. Planets that have an angle less than 90° rotate in the same direction while those with angle of inclination greater than 90° rotate in the same direction with each other but in opposite direction to planets with inclination angle less than 90°.

The period of self-rotation is known as a "day" in popular terminology. The longest day is that of Mercury (which is more than 253 Earth days) and the shortest one is that of Jupiter (less than 10 hours).

You have reached the end of Physics lesson 22.2.7 Planetary Rotation around Own Axis. There are 10 lessons in this physics tutorial covering Sun and Planetary Motion, you can access all the lessons from this tutorial below.

More Sun and Planetary Motion Lessons and Learning Resources

Cosmology Learning Material
Tutorial IDPhysics Tutorial TitleTutorialVideo
Tutorial
Revision
Notes
Revision
Questions
22.2Sun and Planetary Motion
Lesson IDPhysics Lesson TitleLessonVideo
Lesson
22.2.1Basic Features
22.2.2The Source of Solar Energy
22.2.3Energy Transmission from Core to Surface of the Sun
22.2.4Structure of the Sun
22.2.5Planetary Motion around the Sun
22.2.6Observation of Planetary Motion from Earth
22.2.7Planetary Rotation around Own Axis
22.2.8Earth Rotation around its Own Axis
22.2.9Seasons
22.2.10Day and Night

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