Tag: Universe

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Nature Science Stargazing Universe

The Belt of Venus or the Anti-twilight Arch

Full moon rising underneath the Belt of Venus
Full moon rising underneath the Belt of Venus

You now know why sunsets and sunrises are red (if not, read this article and find out!). But did you know that another beautiful light phenomenon occurs at sunset and sunrise, besides the beautiful reddish skies? It actually occurs opposite of where the Sun is setting or rising, thus opposite of where all the beautiful reddish colors light up the sky! So, next time you have a clear sky, try looking away from the nice sunset, in order to see the anti-twilight arch! But what is this anti-twilight arch?

Let’s explain its name first

The Belt of Venus, which is a stylized name for the anti-twilight arch, is a pink glow above the horizon, right opposite of where the Sun sets/rises. This opposite place of the Sun is actually an imaginary point, which we will call from now on the antisolar point (anti means opposite).

The phenomenon takes place during twilight – thus before sunrise or after sunset respectively. It is represented by a pink glow that surrounds, just like an arch, the horizon opposite of where sunsets and sunrises occur.

So there you have it – the anti-twilight arch!

Concerning the name “Belt of Venus”, contrary of what you might guess, it’s got absolutely nothing to do with the planet Venus, or any of its belts or rings (…which do not exist anyway!). Planet Venus has a smaller orbit around the Sun than Earth does, and this makes Venus visible to our eyes only around sunsets and sunrises, similar to how the antitwilight arch becomes visible at sunset and sunrise. This is the only association that the Belt of Venus might have with the actual planet. The name Belt of Venus is, in fact, inspired from the girdle which was supposedly worn by the goddess Venus and which might resemble the pinkish arch around the antisolar point, at twilight.

So what exactly is this Belt of Venus?

After sunset (or before sunrise), the Sun is below the horizon, relative to an observer on Earth. In the figure below, the observer’s line of sight is represented by the thin grey line and the Sun is below this line of sight, thus below the observer’s horizon. The dotted circle around Earth represents our planet’s atmosphere. Even though the Sun is below the horizon, right after sunset, light rays from the Sun still make way to get to the observer and even further (red arrow), till above the antisolar point, where they get backscattered off Earth’s atmosphere (pink arrow). This region, where the backscattering takes place, has a belt shape, and this belt is nothing else but the antitwilight arch!

In this figure, notice that the backscattering “point”, at the tip of the red arrow, is a little above the line of sight for the observer. The small region between the backscattering point and the line of sight, is represented by a dark belt, which is our planet’s shadow.

What will you, as observer, see? Well, if you look right opposite where the Sun is setting, you will notice, right after sunset, a faint pinkish light, stretching around the antisolar point, like a belt, or arch. As time passes, this pinkish glow will rise. Right underneath it, you will see a darker belt, which is nothing else than Earth’s shadow! As time passes further, the pinkish glow will rise even more, as will our planet’s shadow, until night will take over entirely and it will become pitch black outside.

This effect is sometimes very faint, and in order to get a good view, you will need, first of all, a clear sky. Best is also to have a clear horizon above the antisolar point as well, in order to distinguish this effect as better as possible.

So, now that you know about the antitwilight arch, I dare you to ignore a beautiful sunset and look right opposite! But I promise that if you do, you will get to see another magnificent optical phenomenon, less known, but of equal beauty! Have you already seen the Belt of Venus?

The Belt of Venus. Image credit: Kent Duryee (https://commons.wikimedia.org/wiki/File:Belt-of-venus.jpg), „Belt-of-venus“, https://creativecommons.org/licenses/by/4.0/legalcode
The Belt of Venus.
Image credit: Kent Duryee (https://commons.wikimedia.org/wiki/File:Belt-of-venus.jpg), „Belt-of-venus“, https://creativecommons.org/licenses/by/4.0/legalcode
Categories
Nature Science Universe

Why are sunsets and sunrises red?

Beautiful sunset over the Dammen Pond on the Vadsøya island
Beautiful sunset over the Dammen Pond on the Vadsøya island

This period in Vadsø, as in much of the Arctic region, nights begin getting longer and longer. It’s not yet the Polar Night, which means that everyday, beautiful sunsets and sunrises mark the beginning and the end of the dark, cold Arctic nights. But what makes sunsets so beautiful? Why does the sky and the Sun turn red?

In order to answer this, we need to review the same concepts we took into account when answering the question “why is the sky blue?“.

Light is an electromagnetic wave, just like radio waves, microwaves, and even the radiation resulted from radioactivity! The only difference between all these different electromagnetic waves is their wavelength.

Even the light that we actually perceive with our own eyes is made up of multiple wavelengths. And to each and all of these wavelengths of light corresponds a different colour! So, the light that comes to us from the Sun and which we see, is made up of multiple colours! Of all colours, to be exact!

Just like an ocean’s waves, light travels the same way: in waves! Blue light travels in shorter waves (with a shorter wavelength) and red light travels in longer waves (longer wavelengths).

When the sunlight, with all its colours, reaches Earth, it meets the planet’s atmosphere! Thus, it starts interacting with various particles in the air, such as tiny ice crystals, dust, water droplets and even gas molecules that make up the air itself! And once the light waves interact with these particles, it gets scattered!

For a wave to interact with a particle, the two must be of the same order of size. Smaller particles scatter short wavelength light (blue) stronger. Small air molecules, which make up the entire atmosphere, scatter the blue component of sunlight the most, and in all directions, because of its short wavelength! And this is why, during a sunny day, everywhere you look, the sky is blue!

At sunrise and sunsets however, the Sun, relative to us, finds itself at low positions in the sky. From these low positions in the sky, sunlight needs to travel longer distances, through thicker amounts of the atmosphere in order to reach our eyes.

At sunset and sunrise, sunlight travels a longer distance (pictured as the thick yellow arrow) through the atmosphere until it reaches our eyes.

Because of this, the light gets scattered more strongly by the atmosphere. Blue light, which gets scattered easiest, is in fact scattered so much, that it is mostly removed before it actually reaches our eyes. Which in turn means that there is more red light (which gets scattered the least) left for our eyes to see.

Me at sunset, on the shore of the beautiful Varanger fjord.
Categories
Nature Stargazing Universe

Comet Neowise

Comet Neowise
Comet Neowise

You have probably heard or read in the news recently about a magnificent sight in the night sky in the Northern hemisphere – the Neowise comet. It’s been discovered since March 2020 with the help of the Neowise space telescope, hence its name, but at the time of discovery it was of a +10 magnitude, thus not visible to the naked eye.

This month, however, its magnitude reduced to around +3 – which means that the comet is not only now visible to the naked eye, but it can also be seen in relatively light polluted areas, such as bigger cities! It is actually so bright that it is the second brightest comet in the night sky after the Hale-Bopp comet of 1997. Remember it?

So, if you live in Earth’s northern hemisphere, and if your sky is clear of clouds (…and, of course, if you don’t live in polar regions, where the Polar Day currently occurs), do take a look at the night sky! Best is to look just after the nautical twilight, or when the stars start being seen in the North-north-west direction, just a little bit above the horizon! More exactly, locate the well known asterism Big Dipper and look just right under it! You will not regret it!

And if you want to take photos of the comet, don’t forget your tripods! I forgot it and the photos look blurry, but still nice! Did you manage to take nice pictures of it? And remember, if you’d like to get to know the night sky better – do visit me in Vadsø next winter, where the perspective of the zenith is completely different and where light pollution almost doesn’t exist, and let’s go on an Arctic Stargazing adventure together!

Photo of Comet Neowise taken with my phone and without a tripod!
Categories
Nature Stargazing Universe

Natural Satellites

Waxing Crescent Moon
Waxing Crescent Moon

Natural satellites are natural celestial bodies that orbit around a planet of the Solar System. But did you know that another commonly used term for denoting a natural satellite is “moon”? You’ve all probably seen the Moon in the night sky! The Moon is Earth’s natural satellite that continuously orbits around our planet. However, other planets of our Solar System do have natural satellites, or moons!

Jupiter’s Moons

Probably the best known moons (other than our own planet’s Moon) are Jupiter’s: Ganymede, Callisto, Io and Europa. Jupiter has 79 moons in total, but these 4 are the biggest and the most visible from Earth! They’re called Galilean moons, because they were first discovered by Galileo Galilei in 1610 as the first natural satellites that would orbit another planet than Earth! The 4 Galilean moons are visible in the night sky with almost any telescope and are a beautiful sight during a stargazing session.

Animation of the Galilean Moons. Image credit: NASA.

Saturn’s Moons

Saturn has got 82 moons. However, as the planet lies further away from Earth than Jupiter, and because the majority of the ringed planet’s moons are small in diameter, only one – Titan – is rather easily visible through a telescope from Earth.

Saturn moon transit. Image credit: NASA.

Other Moons

Mars, Uranus and Neptune also have their own moons, all varying in sizes from about 10 km diameter to as big as Neptune’s moon Triton, of approximately 2710 km in diameter!

The Moon

But now, coming back to earth’s Moon – did you know that this natural satellite is the brightest celestial body visible in the night sky? Its apparent magnitude varies from -2.50 during the New Moon phase, to -12.90 when it’s a Full Moon.

By the way, apparent magnitude measures the brightness of a celestial body (star, moon, satellite or any other astronomical object) observed from Earth. The lower the magnitude is, the brighter the object appears. As information, the Sun in the daytime sky has the apparent magnitude of -26.74 and the unaided human eye can see in the night sky magnitudes of up to around +3 (in relatively high light-polluted areas) or +5 (under very clear dark sky conditions).

Full Moon

…And did you also know that the Moon’s apparent size in the sky is almost the same as that of the Sun? The Moon’s diameter is, of course much, much smaller than that of the Sun: approximately 3500 km vs. the Sun’s 1.4 million km. But the relatively short distance between our planet and the Moon (384400 km), compared to the distance from Earth to the Sun (150 million km), makes the apparent size of the two celestial bodies approximately the same. Moreover, this relatively similar apparent size makes it possible for the Moon to cover the Sun almost precisely during a total solar eclipse! However, as the Moon’s distance from Earth continually increases, this “perfect” match between the two similar apparent sizes will stop occurring in the far future and total solar eclipses will not be possible anymore.

Oh, and did you know that the Moon is also responsible for the tides? Ocean tides are the continuous rise and fall of sea levels, which occur because of the concurrence between the Moon’s and Sun’s gravities, combined with Earth’s rotation! But more about this subject in another article!

Categories
Nature Science Universe

Why is the sky blue?

Sunny blue sky
Sunny blue sky

Now that the polar day starts to make itself felt more and more in high latitudes, we’ll experience daylight round the clock here in Vadsø in less than 2 weeks! More daylight means more blue skies! But do you know why the sky is blue? Keep on reading to find out!

Light is an electromagnetic wave, just like radio waves, microwaves, and even the radiation resulted from radioactivity! The only difference between all these different electromagnetic waves is their wavelength.

Even the light that we actually perceive with our own eyes is made up of multiple wavelengths. And to each and all of these wavelengths of light corresponds a different colour! So, the light that comes to us from the Sun and which we see, is made up of multiple colours! Of all colours, to be exact!

Just like an ocean’s waves, light travels the same way: in waves! Blue light travels in shorter waves (with a shorter wavelength) and red light travels in longer waves (longer wavelengths).

When the sunlight, with all its colours, reaches Earth, it meets the planet’s atmosphere! Thus, it starts interacting with various particles in the air, such as tiny ice crystals, dust, water droplets and even gas molecules that make up the air itself! And once the light waves interact with these particles, it gets scattered!

For a wave to interact with a particle, the two must be of the same order of size. Smaller particles scatter short wavelength light (blue) stronger. Small air molecules, which make up the entire atmosphere, scatter the blue component of sunlight the most, and in all directions, because of its short wavelength! And this is why, during a sunny day, everywhere you look, the sky is blue!

Do you know why sunsets are reddish? If not, read this article to find out!