Tai gali paskatinti jūsų mintis apmąstyti, kas iš tikrųjų yra.
Tiesiai virš jūsų yra dangus – arba, kaip mokslininkai vadintų, atmosfera. Jis tęsiasi apie 20 mylių (32 kilometrų) virš Žemės. Aplink atmosferą plūduriuoja a molekulių mišinys – mažytės oro dalelės, tokios mažos, kad kiekvieną kartą kvėpuodami pasiimate jų milijardus.
Virš atmosferos yra erdvė. Jis taip vadinamas, nes turi daug mažiau molekulių, tarp jų yra daug tuščios vietos.
Ar kada susimąstėte, kaip būtų keliauti į kosmosą ir tada tęsti? Ką rastum? Mokslininkai kaip aš gali paaiškinti daug to, ką pamatytumėte. Tačiau yra keletas dalykų, kurių dar nežinome, pavyzdžiui, ar kosmosas tęsiasi amžinai.
Planetos, žvaigždės ir galaktikos
Kelionės erdvėje pradžioje galite atpažinti kai kurias lankytinas vietas. The Žemė yra planetų grupės dalis kad visi skrieja aplink Saulę – kai kurie orbitiniai asteroidai ir kometos taip pat susimaišė.
Pažįstamas rajonas.
Galbūt žinote, kad Saulė iš tikrųjų yra tik vidutinė žvaigždė ir atrodo didesnė ir ryškesnė nei kitos žvaigždės tik todėl, kad yra arčiau. Norėdami patekti į kitą artimiausią žvaigždę, turėtumėte keliauti per trilijonus mylių erdvės. Jei galėtum važiuoti greičiausiu kosminiu zondu[{” attribute=””>NASA has ever made, it would still take you thousands of years to get there.
If stars are like houses, then galaxies are like cities full of houses. Scientists estimate there are 100 billion stars in Earth’s galaxy. If you could zoom out, way beyond Earth’s galaxy, those 100 billion stars would blend together – the way lights of city buildings do when viewed from an airplane.
Recently astronomers have learned that many or even most stars have their own orbiting planets. Some are even like Earth, so it’s possible they might be home to other beings also wondering what’s out there.
This packed image taken with the Hubble Space Telescope showcases the galaxy cluster ACO S 295, as well as a jostling crowd of background galaxies and foreground stars. Credit: ESA/Hubble & NASA, F. Pacaud, D. Coe
You would have to travel through millions of trillions more miles of space just to reach another galaxy. Most of that space is almost completely empty, with only some stray molecules and tiny mysterious invisible particles scientists call “dark matter.”
Using big telescopes, astronomers see millions of galaxies out there – and they just keep going, in every direction.
If you could watch for long enough, over millions of years, it would look like new space is gradually being added between all the galaxies. You can visualize this by imagining tiny dots on a deflated balloon and then thinking about blowing it up. The dots would keep moving farther apart, just like the galaxies are.
Is there an end?
If you could keep going out, as far as you wanted, would you just keep passing by galaxies forever? Are there an infinite number of galaxies in every direction? Or does the whole thing eventually end? And if it does end, what does it end with?
These are questions scientists don’t have definite answers to yet. Many think it’s likely you would just keep passing galaxies in every direction, forever. In that case, the universe would be infinite, with no end.
Some scientists think it’s possible the universe might eventually wrap back around on itself – so if you could just keep going out, you would someday come back around to where you started, from the other direction.
One way to think about this is to picture a globe, and imagine that you are a creature that can move only on the surface. If you start walking any direction, east for example, and just keep going, eventually you would come back to where you began. If this were the case for the universe, it would mean it is not infinitely big – although it would still be bigger than you can imagine.
In either case, you could never get to the end of the universe or space. Scientists now consider it unlikely the universe has an end – a region where the galaxies stop or where there would be a barrier of some kind marking the end of space.
But nobody knows for sure. How to answer this question will need to be figured out by a future scientist.
Written by Jack Singal, Associate Professor of Physics, University of Richmond.
This article was first published in The Conversation.