Physics Tutorial 22.3 - The Moon's Movement. Eclipses. Calendars

There are 5 lessons in this physics tutorial covering The Moon's Movement. Eclipses. Calendars. The tutorial starts with an introduction to The Moon's Movement. Eclipses. Calendars and is then followed with a list of the separate lessons, the tutorial is designed to be read in order but you can skip to a specific lesson or return to recover a specific physics lesson as required to build your physics knowledge of The Moon's Movement. Eclipses. Calendars. you can access all the lessons from this tutorial below.

In this Physics tutorial, you will learn:

How does the Moon move?
What is tropical and synodic month? How do they differ from each other?
What are the Moon phases? When do they occur?
What are eclipses? How many eclipses are there?
How calendars are designed? How many calendars are there?
What factors are considered when designing a calendar?
How to calculate the alignment period between two planets?

Introduction

It is a matter of fact that the Moon is the only natural satellite of Earth and its closest celestial body. It is a rocky celestial body with many craters on its surface formed by the strike from asteroids experienced in time. Moon was formed about 4.5 billion years ago, about 30-50 million years after the origin of the Solar System, out of debris thrown into orbit by a massive collision between a smaller proto-Earth and another planetoid, about the size of Mars.

Physics Tutorials: This image provides visual information for the physics tutorial The Moon's Movement. Eclipses. Calendars

Gravitational forces, like in all the other celestial bodies, are the main factors that determine the movement of Moon. However, unlike in planets where only the Sun is considered when dealing with gravitational forces, as the effect of other celestial bodies in this force is negligible, there are two different gravitational forces that determine the trajectory of Moon: the gravitational force exerted by the Sun and that exerted by Earth on the Moon. The sum of these two forces (net gravitational force) makes the Moon deflect too much from the pure circular (or elliptic if you want) motion (discussed in tutorial 8.2) as shown in the figure below. (Actually Earth makes the same kind of rotation around the centre of our galaxy when revolving around the Sun but for now, we are not interested on this).

Please select a specific "The Moon's Movement. Eclipses. Calendars" lesson from the table below, review the video tutorial, print the revision notes or use the practice question to improve your knowledge of this physics topic.

Cosmology Learning Material
Tutorial ID	Physics Tutorial Title	Revision Notes	Revision Questions
22.3	The Moon's Movement. Eclipses. Calendars
Lesson ID	Physics Lesson Title	Lesson	Video Lesson
22.3.1	Main Features of the Moon's Movement
22.3.2	Moon Phases
22.3.3	Eclipses
22.3.4	Calendars
22.3.5	Calculating the Time Needed for the Earth and Another Planet to Realign Again

Whats next?

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Cosmology Revision Notes: The Moon's Movement. Eclipses. Calendars. Print the notes so you can revise the key points covered in the physics tutorial for The Moon's Movement. Eclipses. Calendars
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Continuing learning cosmology - read our next physics tutorial: Stars

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