Home » Science »

From Nothing to You in 10 Sentences [Starts With A Bang]

 

“It surprises me how disinterested we are today about things like physics, space, the universe and philosophy of our existence, our purpose, our final destination. It’s a crazy world out there. Be curious.” -Stephen Hawking

One of the most existential questions humanity has ever asked is the question of our origins: where do I come from? Inspired by Ben Kilminster’s writings, here’s the entire history of the Universe — that’s led up to the existence of you — in just 10 sentences*.

Image credit: Amber Stuver of http://www.livingligo.org/.

Image credit: Amber Stuver of http://www.livingligo.org/.

1.) At some point in the distant past**, the Universe consisted of empty spacetime with a large amount of intrinsic energy bound up in itself, and was in a state of exponential expansion known as cosmological inflation.

Image credit: Me.

Image credit: Me.

2.) About 13.7 billion years ago, a region of spacetime that would contain our entire observable Universe saw inflation come to an end; the energy that was bound up in spacetime itself was transferred*** into matter, antimatter and radiation, marking the first time the Universe can be described accurately by the Big Bang model.

Image credit: Retrieved from http://case.ntu.edu.tw/hs/wordpress/?p=41808.

Image credit: Retrieved from http://case.ntu.edu.tw/hs/wordpress/?p=41808.

3.) The energetic, matter-antimatter-and-radiation-filled Universe now cools as it expands, and a fundamental asymmetry**** between matter-and-antimatter leads to a slight, 0.6-parts-in-a-billion dominance of matter over antimatter.

Image credit: Me.

Image credit: Me.

4.) As the Universe continues to expand cool, the excess matter annihilates away with the antimatter, and the radiation shifts to progressively lower energies, allowing the formation of protons and neutrons, stable nuclei, and eventually — after the radiation becomes low enough in energy so that normal-and-dark-matter now dominate the Universe’s expansion rate — neutral, stable atoms form for the first time.

Image credit: Universe Adventure, © 2005 LBNL Physics Division.

Image credit: Universe Adventure, © 2005 LBNL Physics Division.

5.) With the Universe now dominated by dark-and-normal matter, gravitational collapse proceeds, and the great cosmic web begins to form, with the first stars in the Universe igniting after a period of 50-to-75 million years.

Image credit: NASA / JPL-Caltech / Spitzer Space Telescope.

Image credit: NASA / JPL-Caltech / Spitzer Space Telescope.

6.) The light from these stars reionizes the Universe, making it transparent to light, while the Universe hierarchically forms star clusters, galaxies, clusters, and superclusters of galaxies on the largest scales.

Image credit: Jim Misti (Misti Mountain Observatory).

Image credit: Jim Misti (Misti Mountain Observatory).

7.) As time goes on, the most massive first-generation stars run out of fuel and die in supernova explosions, triggering the formation of new stars and enriching the surrounding interstellar media with progressively heavier and heavier elements.

Image credit: X-ray: NASA/CXC/SAO/D.Patnaude, Optical: DSS.

Image credit: X-ray: NASA/CXC/SAO/D.Patnaude, Optical: DSS.

8.) Finally, after generations of stars being born, living, burning through their fuel, and dying, the interstellar medium is sufficiently enriched with enough of the elements for complex chemistry that all new stars and star systems that form will have substantial amounts of the elements and molecules necessary for life.

Image credit: NASA, ESA, CXC, SSC, and STScI.

Image credit: NASA, ESA, CXC, SSC, and STScI.

9.) About 9.2 billion years after the Big Bang, a small region about 1/3 of the distance from the center of our Milky Way — one of a few hundred billion galaxies in our Universe — forms a new population of around a thousand stars, one of which — out of the hundreds of billions in our galaxy — forms with a protoplanetary disk that collapses into eight planets, four rocky inner worlds and four outer gas giants.

Image credit: Avi M. Mandell, NASA.

Image credit: Avi M. Mandell, NASA.

10.) After a few hundred million years, complex chemical life takes off***** on the 3rd world in this solar system, and a vast diversity of lifeforms evolve over billions of years and trillions of generations; a scant few years ago, grown initially from the joining of two cells, a veritable Universe-within-the-Universe of 1028 atoms — left over from the Big Bang and forged in the crucibles of long-dead stars — came together, for a brief while, to exist as you.

Image credit: Ernst Haeckel's Paleontological Tree of Vertebrates (c. 1879).

Image credit: Ernst Haeckel’s Paleontological Tree of Vertebrates (c. 1879).

And that’s how the Universe came from nothing, to create you, in just 10 sentences.******

hline* – Not every aspect of how each of these events happened is fully understood. The asterisks are here to show you the events that are currently still being investigated.

** – It is not clear how the Universe came to be in this state, and whether that state was eternal to the past or whether it came into existence in some fashion.

*** – The particulars of how inflation ended (the “graceful exit” problem) and how the energy was transferred into matter, antimatter and radiation (the “cosmic reheating” problem) do not presently have universally agreed-upon answers.

**** – We don’t know the exact mechanism of what caused the observed asymmetry between matter and antimatter; an illustrative example is here.

***** – We don’t know whether life originated on this world or on another world or in interstellar space; we only know that it took off on this world some 3+ billion years ago.

****** – Fine, ten sentences, two semicolons, and six footnotes.

 

Related Posts

  • No Related Posts
 
 

0 Comments

You can be the first one to leave a comment.

 
 

Leave a Comment

 




 
 

 
 
 
This site is protected by WP-CopyRightPro