Here are five myths about the Moon you can easily disprove yourself

Space

This year’s first supermoon potentially graced the sky on February 9. A supermoon is usually defined as the largest full moon possible.

This is a very lose definition and roughly means this happens when the full moon occurs within 10 percent of its closest to Earth.

But in reality, supermoons are never huge at all. There are in fact countless misunderstandings about the Moon and how it appears in the sky. Here are five such examples – and how to disprove them yourself.

The supermoon is huge

From an observer’s point of view, a supermoon is approximately just 14 percent bigger than when it’s smallest. That said, if you were viewing a normal moon and a supermoon side by side, you would be able to spot the difference.

Size comparisons of the Moon for consecutive days and full moons. (Daniel Brown)Size comparisons of the Moon for consecutive days and full moons. (Daniel Brown)

IMAGE: Adjust the size of the image on your screen so the little finger on the right is the size of your little finger. Then hold the image at arms’ length to achieve the size of the Moon as you would see it in the sky.

But our eyes cannot measure the apparent sizes of objects in the sky with high precision without comparing them to something. And herein lies the misconception.

The Moon does not suddenly grow in size, but gradually appears a tiny bit bigger and then smaller during the month. To fully compare how super this moon is, you would need to compare it with a full moon several months ago. And even then, the difference is rather small.

There’s a dark side of the Moon

A classic misconception is that the Moon has a dark side that never sees any light from the Sun. This is because we tend to believe the Moon doesn’t rotate around its own axis – we after all always see the same side facing towards us.

But that’s incorrect. We see the same side because the Moon rotates around itself once while it moves once around the Earth. You can experience this yourself with a simple experiment. Slowly walk around a chair at home so that you always look directly at it.

Note how you might see the chair in front of the window and then later in front of your desk, depending in where are are. If you stop somewhere, you only see one background. To see all the other parts of the room, you will need to turn around or rotate.

The Moon does the same – it moves around the Earth and rotates. Now if the Moon rotates, and the half of the Moon facing the Sun is illuminated, then surely every side of the Moon will see the Sun over a month.

The Earth’s shadow causes moon phases

Over a month, the Moon shows different phases. This is sometimes incorrectly explained by the Earth’s shadow covering parts of the Moon.

But it is rather an issue of how we view the Moon. Given Earth’s location, we see different sides of the Moon that are more or less illuminated.

To discover how, put a ball on a wall to represent the Moon and walk around it. As you have the Sun at your back, you see all of the visible side illuminated. As you move on and the Sun is now to your right as you face the ball, you see half of the visible side illuminated, like a half moon. When the ball and Sun are in the same direction, we see none of the visible side illuminated.

Illustration of three moon phases. (Daniel Brown)Illustration of three moon phases. (Daniel Brown)

IMAGE: As a guide possible objects are included that might cause a shadow to explain the observed shape of the phase.

You can also prove that the Earth’s shadow cannot be responsible for the phases of the Moon by thinking about the shape of the Earth – surely it should always be a sphere.

But note, for example, the different shape of a waxing crescent to gibbous moon. If the Earth’s shadow were causing this then the planet would have to have a rather odd banana shape.

Phases of a lunar eclipse. (Daniel Brown)Phases of a lunar eclipse. (Daniel Brown)

IMAGE: Note how the curvature of the shadow always fits the Earth’s round shadow. 

However, there is one exception. During a lunar eclipse – occurring only at full moon – the Moon actually moves into the Earth’s shadow.

The Moon moves differently in the southern sky

The shape of the crescent reveals whether the Moon is growing or fading. If you are in the northern hemisphere, you can remember the shapes with the mnemonic “DOC”.

When the Moon looks like a D, with the curve on the right, it is a growing or waxing moon. When it looks like an O it is a round full moon. And when it looks like a C, with the curve on the left, it is a fading or waning moon.

However, this sequence has to be inverted to become “COD” in the southern hemisphere. Explaining this difference can cause some confusion, especially because the Moon seemingly moves from right to left in the southern hemisphere, while it clearly moves from left to right in the northern hemisphere.

The explanation is simple and proves that the Earth is a sphere. As you move from the northern hemisphere to the southern (or vice versa), your viewpoint of the Moon turns upside down.

Or, in your frame of reference, the Moon and stars seem to turn upside down. You can do this yourself, by bending down and seeing the Moon and sky upside down through your legs.

(Daniel Brown)(Daniel Brown)

IMAGE: These are three different views of the recent close encounter of Venus and the young moon crescent on January 28 2020. Note it is always the same (enlarged) waxing thin crescent but its orientation is altered nicely marked by Venus.

Since we see the Moon upside down when we move into the opposite hemisphere, the phases will be inverted as well, but they still rise in the eastern part of the sky and set in the western part of the sky. This means their path indeed moves them from right to left.

The Moon’s crescent doesn’t always face the Sun

The Moon’s curved crescent is said to always point towards the location of the Sun. But we don’t always see it like this because of the moon tilt illusion.

The moon tilt illusion. (Daniel Brown)(Daniel Brown)

IMAGE: The (enlarged) half moon in Nottingham, in April 2020. On the right the observer is forcefully leaning back to ensure they directly face the Moon with the Sun to their exact right.

We assume that a line connecting two points – in this case the Moon and the illuminating Sun – should be straight.

But because we look at these points from a fixed location on a spherical planet, the line is really curved. Changing our position so we see a better projection of the two points gives a more realistic view.

You can do this by simply leaning back while looking directly at the Moon until the Sun is exactly to your right or left. The Conversation

Daniel Brown, Lecturer in Astronomy, Nottingham Trent University.

This article is republished from The Conversation under a Creative Commons license. Read the original article.

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