Why is it so hard to see?

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We have always had an incredible ability to see, but the last few years have seen a dramatic decline in that ability.

We are no longer able to see the colours that normally appear when light hits our eyes.

We also cannot see objects that are not visible to us, like people or animals.

We don’t see colours that appear in our peripheral vision because we can’t see them.

As a result, we often see things that we wouldn’t normally recognise.

This is because we are unable to distinguish colour, shape or even size from each other.

When we see a blue object, for example, we think it is a blue sky or a cloud, but if we see something that looks like a pink object, we know it’s a pink cloud.

In this article we’ll look at the basics of how vision works, and how we can learn how to see better.

First we’ll see how light is reflected off the earth.

The earth is made up of a variety of rocks and ice crystals.

The Earth’s surface is very different to the surface of our planet, and the light reflected off of the surface is reflected into space, just as it would be if light was reflected off a water droplet.

The reason that we cannot see through the earth’s surface at night is that there are too many reflections from the earth, and this causes a range of colours to appear on the sky.

The Earth’s atmosphere also contains a range, which we call the blue spectrum, which can be very different from the colours of our eyes and other colours.

We can use this blue spectrum to see objects in the sky, as well as in the world around us.

However, when we look at an object that is moving, the blue is reflected back and the red and green spectrum are reflected.

The difference between the red spectrum and the blue spectra is called the redshift.

The redshift is the amount of light that is shifted to the left or the right of the spectrum.

In the image below we see how the red light of the sun is reflected from the blue sky.

It looks like there are some dark areas in the image, which is due to the reflectance of the red-violet light from the Earth’s sun.

As we look through the red sky, we are able to tell the difference between these different spectra, and can also use it to tell us the distance from the sun.

This helps us to find objects and see things on the ground.

We use this knowledge to navigate on the moon, for instance.

Redshifts in the moon’s colours have been measured for the past 50 years, but there is still a long way to go before we are seeing the reds and oranges of the moon.

We have also noticed that the colours are changing, but we cannot really tell what is causing it.

When the moon was full, the red colour was so intense that the redshifts of all the colours were in a range from 0 to 1.

When the moon has stopped full, however, the sky is now completely blue.

This means that all the red, green and blue are now in the same range as the red wavelength of the Earth.

This also means that we have not been seeing any change in the colours.

The only thing that is really changing is the intensity of the blue, so the colours have not changed.

In addition, when the moon is full, it is also the time when the Earth is at its furthest point from the Sun, and therefore the Moon is getting smaller.

When this happens, the Moon becomes smaller and less massive.

This has caused us to get better and better at seeing the colours in the night sky.

But when the Moon stops full, our night sky is very limited.

The sky is dark and the colours we can see are limited.

So the next time you are outdoors, try not to look directly at the sky but rather at the ground in front of you.

You may be surprised how bright and dark the sky becomes.

This can help you recognise the colours you are seeing.