The Big Bang

Where does everything come from?
Everything you see around you is made up of atoms. Atoms are made up of particles; protons, neutrons and electrons. These particles are made up of even smaller elements called quarks.

Hydrogen, or hydrogen, is the most abundant element in our universe. It is the simplest element and consists of just a single proton. Hydrogen is important to us as it is used in many chemical compounds. For example, in the water we drink and in the cells of our body.

To find out how the first atoms were formed, we have to turn back time to the beginning of the universe.

Today, we believe that the universe was created over 13 billion years ago in what is known as the Big Bang. But what exactly is it?

The background to the Big Bang theory is relatively simple. In a nutshell, the Big Bang theory explains that everything that has ever existed in the universe came into existence at the exact same moment almost 13.8 billion years ago.

At that time, all the material that exists in the universe came into existence. But also time itself and the space around us came into being at this moment. So the Big Bang created three things: The material we are made of, the space between the material, and time. That's why it's actually not possible to talk about a time before the Big Bang, because time did not exist.

The universe was once much smaller, much denser and much hotter than it is now. Very shortly after the formation of the universe, a massive expansion started and has continued ever since. The driving force behind the expansion of the universe is what we call dark energy. As the universe has expanded, it has also become colder.

When we look out into the universe today, it looks like all of space is expanding around us. But in fact, the universe is expanding at all points and in all directions. In this way, you could also say that the Big Bang didn't happen at a specific point, as all the space we see today originated from the Big Bang.
 

The early universe
We only know a little bit about what happened in the moments after the Big Bang. The theories we have today that describe the laws of physics start to break down when we try to describe the early universe. The laws of physics as we know them seem to have behaved very differently in the first seconds after the Big Bang.

The conditions right after the Big Bang have been so extreme that it's very difficult to replicate here on Earth. We believe that just a few minutes after the formation of the universe, the temperature dropped to around one billion degrees.

About three minutes and 20 seconds after the Big Bang, the first protons and thus the first atomic nuclei are formed. In the following minutes, all other matter in the universe is formed. The first atoms to form are hydrogen, helium and small amounts of lithium.
 

The cosmic microwave background radiation
It's not possible for us to observe the Big Bang directly, but how close can we get? The answer is what is called the cosmic microwave background radiation.

In the first time after the Big Bang, the universe was so hot and so dense that light could not travel freely through space.

It wasn't until 380,000 years after the Big Bang that the universe cooled down enough for electrons to start gathering around the first atomic nuclei to form the first whole atoms. When this happened, light could travel freely for the first time without hitting the free electrons or atomic nuclei. It is also said that the universe became transparent.

The first light was not emitted until 380,000 years after the formation of the universe, and it is this light that we see today as the cosmic microwave background radiation.

The light can be measured in all directions as a kind of faint background noise in the universe. The radiation reaches us as microwaves - a form of light that cannot be seen with the naked eye, but can be measured with special instruments.

By taking a closer look at this background radiation, scientists have learnt more about both the age and composition of the universe.

The cosmic microwave background radiation is one of the strongest pieces of evidence that there was a Big Bang. The radiation was discovered by accident back in the 1960s, but before that several scientists had calculated that there should be an afterglow from the Big Bang and what temperature this afterglow should be. The first measurements of the background radiation agreed well with these calculations and subsequent observations have only strengthened the theory further.

Den kosmiske mikrobølgebaggrundsstråling kan måles i alle retninger som en slags svag baggrundsstøj i universet. Strålingen når frem til os som mikrobølger – en form for lys, som ikke kan ses med det blotte øje, men som kan måles med særlige instrumenter.

Når vi observere universet, er det næsten altid lys, vi observere, så den kosmiske mikrobølgebaggrundsstråling er det tidligste, vi kan observere i universet. Alt hvad der skete før den kosmiske mikrobølgebaggrundsstråling er noget vi har regnet os frem til, og ikke noget vi har set. Men denne baggrundsstråling kan hjælpe forskere til at blive klogere på både universets alder og sammensætning.

Den kosmiske mikrobølgebaggrundsstråling er et af de stærkeste beviser for, at der har været et Big Bang. Strålingen blev opdaget ved et tilfælde tilbage i 1960’erne, men inden da havde flere forskere beregnet, at der burde være en efterglød fra Big Bang, samt hvilken temperatur denne efterglød måtte have. De første målinger af baggrundsstrålingen stemte godt overens med disse beregninger, og efterfølgende observationer har kun styrket teorien yderligere.

Universets udvidelse

Fra da lyset blev sluppet fri og atomerne samlede sig, havde vi alt hvad vi skulle bruge for at opbygge universet som vi kender det i dag.

Efterhånden som universet udvidede sig og kølede ned, samlede atomerne sig i gasskyer, og fra dem skabte vi stjerner (Stjerner). Inde i stjernerne blev de første atomer, brint og helium, omdannet til større atomer, og disse blev frigivet når stjernerne døde (Stjerner og Supernovaer). 

Stjernerne samlede sig i galakser, som skabte strukturer gennem universet (Galakser). Stjernerne fik selskab af mørkt stof der er med til at holde sammen på galakserne, men som vi endnu ikke ved hvad består af (Stof, Mørkt Stof og Mørk Energi).

I det tomme vakuum mellem galakserne er det mørk energi, der hersker, og det er med til at forstærke universets udvidelse, så det går hurtigere og hurtigere (Stof, Mørkt Stof og Mørk Energi).

Omkring 9 milliarder år efter Big Bang var der en gassky med atomer fra både Big Bang og stjernernes død, der kollapsede, og skabte en stjerne, vi i dag kalder Solen, og et planetsystem vi i dag kalder Solsystemet (Solsystemet).

På en af Solsystemets planeter, Jorden, samlede nogle af atomerne sig, og skabte de første celler, og de celler har siden da udviklet sig til millioner af forskellige former for liv (Astrobiologi). 

Og nu, i dag, 13.8 milliarder år efter Big Bang sidder jeg og fortæller dig om alle de fantastiske ting, forskerne har fundet ud af om vores univers! Tænk at vi kan lære så meget ved at kigge op på himlen, og tænk engang at alle de utrolige fænomener vi ser i dag alle sammen opstod fra et enkelt punkt.