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The Moon. Motion and phases of the Moon

09/04/2026

The online simulations of motion of the Moon on this page will help us to learn more about the rotation and translation movements of the Moon and the four phases of the Moon that are generated as a consequence of these lunar movements.

What is the Moon

The Moon, the Earth’s only natural satellite, has been the object of fascination and study for thousands of years. With a diameter of approximately 3,474 kilometers, the Moon is about one-fourth the size of the Earth. Its surface is covered with craters, mountains, valleys, and lunar seas, which are flat, dark areas formed by ancient lava flows. The Moon has a significant influence on our planet. Its gravitational forces interact with the Earth and cause tides in the oceans.

Exploration of the Moon

The Moon has been the subject of human exploration. In 1969, the Apollo 11 mission brought the first astronauts to walk on the lunar surface, with Neil Armstrong and Buzz Aldrin becoming the first humans to set foot on the Moon. Over the years, several space missions have conducted scientific investigations on the Moon, collecting samples of lunar rocks and conducting studies on their composition and origin.

Motion of the Moon. Rotation and translation of the Moon

Motion of the Moon is the result, as in the case of the Earth, of the two main motions of rotation and translation of the Moon.

Rotation of the Moon. The Moon rotates on its own axis approximately once every 27.3 days. This is its period of rotation.

Translation of the Moon. At the same time, the Moon orbits the Earth in a similar period of about 27.3 days (sidereal month).

Because the Moon’s rotation and translation periods are nearly equal (a motion called synchronous rotation), the Moon always shows the same side to the Earth, while its opposite side, known as the “hidden side of the Moon,” remains invisible from our perspective.

In addition to the Moon’s rotational and translational motions, the Moon is gradually moving away from the Earth at a rate of about 3.8 centimeters per year due to tidal energy transfer.

Explore the exciting STEM world with our free, online, simulations and accompanying companion courses! With them you’ll be able to experience and learn hands-on. Take this opportunity to immerse yourself in virtual experiences while advancing your education – awaken your scientific curiosity and discover all that the STEM world has to offer!

Simulations of motion of the Moon

Four phases of the Moon I


Only the Sun produces light by itself. The Earth and Moon only reflect the light they receive from the Sun. Because the Earth and Moon are round, areas that receive sunlight appear bright and areas that do not receive sunlight appear dark. Notice in this simulation of motion of the Moon how the illuminated area of the Moon changes as the lunar cycle progresses and the four phases of the moon are generated
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Four phases of the Moon II


Only the Sun produces light by itself. The Earth and Moon only reflect the light they receive from the Sun. Because the Earth and Moon are round, areas that receive sunlight appear bright and areas that do not receive sunlight appear dark. Observe in this online simulation of motion of the Moon how the four phases of the Moon are generated by changing its position with respect to the source of the light.






Far side of the Moon


Why do we only see one side of the Moon? This is because the rotation speed of the Moon and its translation speed with respect to the Earth is the same and that makes that, from the Earth, we always see the same face of the Moon.






Actual sizes of the Earth, the Moon and its orbit


The last of these online Moon simulations, allows us to see to scale what is the size of the Earth, the Moon and the Moon’s orbit around the Earth..






“If I have seen further, it is by standing on the shoulders of giants”

Isaac Newton

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The Moon is Earth’s only natural satellite and stands out because of its relatively large size compared to the planet it orbits, which gives it a strong influence on several key terrestrial phenomena. Its presence is fundamental because it stabilizes Earth’s axial tilt, helping maintain regular seasons over long periods of time. Its gravitational pull generates tides, a crucial process for coastal ecosystems and ocean dynamics. The Moon also reflects sunlight, illuminating the night sky and allowing us to observe its phases, which result from the changing positions of the Earth, Moon and Sun. Its surface, covered with craters and dark plains known as lunar maria, preserves ancient geological evidence because it lacks an atmosphere that could erode or alter it. For all these reasons, the Moon is essential for understanding both Earth’s behavior and the history of the solar system.
The Moon’s phases occur because, as it orbits Earth, we see different portions of its sunlit side. This cycle lasts about 29.5 days and includes eight main phases: new moon, waxing crescent, first quarter, waxing gibbous, full moon, waning gibbous, last quarter and waning crescent. Each phase corresponds to a specific position in the Moon’s orbit. A new moon occurs when the Moon is between Earth and the Sun, while a full moon happens when Earth is between the Moon and the Sun. These changes are not caused by Earth’s shadow but by the angle from which we observe the illuminated part of the Moon. The phases reveal the geometry of the Earth‑Moon‑Sun system and have historically been used to measure time and structure calendars.
The Moon shines because it reflects sunlight, just like a mirror reflects the light from a lamp. Its surface is fairly bright and bounces that light back toward us, which is why it looks so luminous in the night sky. It doesn’t emit light on its own—the glow we see is simply sunlight reflected from its surface. Depending on the phase, we see more or less of the illuminated part.
Because the Moon takes the same amount of time to rotate on its axis as it does to orbit Earth. This is called synchronous rotation. Since both motions are perfectly matched, the same side always faces us. The far side exists, of course, but we can’t see it from Earth.
The Moon has no atmosphere, no liquid water and no stable temperatures—three basic conditions needed for life as we know it. Daytime temperatures are extremely hot, while nighttime temperatures are extremely cold. Without an atmosphere, there’s no protection from solar radiation or meteorite impacts. Even though it’s close to Earth, its environment is completely different and far too harsh for life to develop.

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