beautiful displays of omnipotence. Despite what its name suggests, The Northern Lights

can be seen almost anywhere in the world, even as far south as the equator. The phenomenon

has been witnessed in Honolulu and Singapore. However, sightings that far south are extremely

rare, it’s most commonly witnessed within the Arctic Circle. The South Pole also has

its own version of the Aurora Borealis, called the Aurora Australis. And Earth isn’t the

only planet with aurora, you would witness a similar phenomenon if you were to stand

on Jupiter or Saturn. Uranus has aurora too, but unlike the other planets with their wave-like

aurora, the aurora on Uranus would look like glowing dots… and yes, I am talking about

the planet. But what exactly causes these mysterious light shows? Let’s find out.

Some Inuit believe that the spirits of their ancestors can be seen dancing within the lights

of the Aurora. The Vikings believed that the Aurora was a bridge of fire to the sky, forged

by the gods. Well, spoiler alert, according to modern science, the northern and southern

lights are not dancing spirits or a bridge of fire. They are actually caused by something

much more tangible, the Sun.

Our Sun is a 4.57 billion-year-old ball of hydrogen and other gasses fusing away in space,

150 million kilometres away from planet Earth. And every once in a while it kicks up a bit

of a storm, a Solar Storm to be precise. The Sun produces energy by smashing hydrogen atoms

together in its core, under such immense temperatures and pressures, to cause the hydrogen atoms

to fuse, to form helium atoms. This process is known as nuclear fusion. When atoms are

under these kinds of pressures they turn into a mushy soup of freely moving particles, which

is a fourth state of matter known as plasma. The Sun is essentially a gigantic ball of

swirling plasma.

Using the process of nuclear fusion, the Sun is able to turn small amounts of matter into

enormous quantities of energy. It’s how the Sun has managed to keep producing energy

for billions of years without running out of fuel. If human-kind were able to consistently

replicate nuclear-fusion here on Earth, we would be able to make almost infinite amounts

of energy, using relatively little resources. In fact, if you could convert the mass of

one bag of sugar into energy it would be enough to drive a car, non-stop, for 100,000 years.

All this plasma swirling around within the Sun generates huge magnetic fields. These

magnetic fields are under such immense pressures within the Sun, that sometimes the lines of

force of theses magnetic fields meet. When this happens, the magnetic field is forced

outwards, towards the surface of the Sun. Once it reaches the Sun’s surface it ejects

outwards into space at great speeds, taking extremely hot gasses and charged particles,

also known as plasma, with it. This is known as a solar flare and they can be witnessed

on the Sun’s surface as a very bright spot followed by a cloud of gas. When a very large

solar flare occurs containing a significantly huge amount of energy, it is referred to as

a Coronal Mass Ejection or CME for short. The gas clouds produced by a CME can sometimes

be larger than the Sun itself.

CME’s and solar flares don’t stop just outside the Sun’s surface. Charged particles

ejected from the Sun continue to travel outwards through space over enormous distances. After

travelling through space for around two days they will reach planet Earth. This is known

as the solar wind and it can be extremely dangerous. If the magnetic field released

from a solar flare or CME were to hit planet Earth it could cause the extinction of the

human race. So why hasn’t it? After all solar flares are taking place regularly on

the Sun’s surface.

Well the solar wind does actually hit Earth, often, but our trusty planet is well-prepared.

We have a defence system to protect us from the huge amounts of energy the Sun bombards

us with on a daily basis. Just like the Sun, the Earth produces its own magnetic field.

At the Earth’s core is a ball of solid iron, the heat of this iron turns the surrounding

outer core into flowing liquid iron. The movement of this outer liquid core produces a magnetic

field, that, luckily for us, encompasses the Earth.

The Earth’s magnetic field protects us from all sorts of harsh destructive forces that

come from far away in space, including solar flares. This protective barrier is called

the Earth’s magnetosphere and it extends thousands of kilometres into space. That sounds

large, but it’s actually rather modest, Jupiter’s magnetosphere extends over seven

million kilometres into space on each side of the planet. In fact, on Jupiter’s nightside,

the side facing away from the Sun, the magnetic field which is emitted is so large, that it

reaches Saturn.

Anyway, back to Earth. Most of the Sun’s solar winds simply bounce off the Earth’s

magnetosphere when it reaches us. However, the magnetosphere has two weak spots, at the

north and south poles. At these two locations the magnetic fields which protect planet Earth

are much less prevalent than nearer the equator.

This means that a very small percentage of the charged particles that come from the Sun

do make their way into the Earth’s atmosphere via the two weak spots at the poles. When

this happens the electrons in the solar wind collide with oxygen and nitrogen atoms in

the Earth’s atmosphere. During this interaction energy is transferred from the atoms in the

solar wind to the Earth’s oxygen and nitrogen atoms. Raising these atom’s energy states

and exciting them. When an atom gets excited its electrons move into an orbit further away

from the nucleus.

These newly excited atoms need to release this new found energy to “calm themselves

down” and return to their baseline energy state. The oxygen and nitrogen atoms release

this energy in the form of particles of light or photons. The light they give out is what

we call the aurora. This process of exciting atoms to cause them to release energy in the

form of light is the exact same way that neon lights work. The aurora are simply mother

nature’s neon lights, executed on a far grander scale. The only difference is that

nature uses this phenomenon in a far subtler way than to advertise strip bars.

The aurora typically appears in vast curtains or waves of light following a distinct line

across the sky. They appear this way because they are following lines of force in the Earth’s

magnetic field. Yep, that’s right, the aurora uses the force.

The different colours of the aurora are caused by different gases in the atmosphere. Each

gas emits a unique colour when it is excited. For example, oxygen gives off a green light

when it’s excited, which is the most common colour seen in the aurora. Nitrogen on the

other hand, gives of blue and red colours when excited.

So to summarise, when charged particles released from the solar flares on the Sun’s surface

hit our planet at either the north or south pole, they interact with atoms in the Earth’s

atmostphere. Causing their electrons to move to a higher energy state. When the electrons

drop back down to a lower energy state they release photons, tiny little particles of

light, which light up the night’s sky in a spectacular display of painted waves, following

the natural magnetic field lines of planet Earth.

Knowing how the aurora are formed may spoil the beauty for you, but I believe there’s

an even greater beauty in understanding the science behind one of nature’s most breathtaking

performances. So if you’re ever lucky enough to experience the aurora for yourself, just

take a moment to contemplate on how truly marvellous and magnificent the universe really

is …and then take selfies.