AstronomyThe Big Freeze: How the universe will die

The Big Freeze: How the universe will die

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The cosmos might by no means finish. However for those who had been immortal, you’d most likely want it might. Our cosmos’ ultimate destiny is an extended and frigid affair that astronomers name the Massive Freeze, or Massive Chill.

It’s a becoming description for the day when all warmth and vitality is evenly unfold over incomprehensibly huge distances. At this level, the universe’s ultimate temperature will hover simply above absolute zero. 

The Massive Bang’s accelerating enlargement

Some 13.8 billion years in the past, our universe was born in the Big Bang, and it’s been increasing ever since.

Till a couple of a long time in the past, it seemed like that enlargement would finally finish. Astronomers’ measurements prompt there was sufficient matter within the universe to beat enlargement and reverse the method, triggering a so-called Big Crunch. On this situation, the cosmos would collapse again into an infinitely dense singularity just like the one it emerged from. Maybe this course of might even spark one other Massive Bang, the considering went. 

We’d be gone, however the Massive Bang/Massive Crunch cycle might infinitely repeat. 

Within the years since then, the discovery of dark energy has robbed us of a shot at this everlasting rebirth. In 1998, two separate groups of astronomers introduced that they’d measured particular exploding stars within the distant universe, referred to as a type Ia supernova, which serves as “standard candles” for calculating distances. They discovered that the distant explostions — which ought to all have the identical intrinsic brightness — had been dimmer, and due to this fact farther away, than anticipated. Some mysterious power was pushing the cosmos other than inside.

This darkish vitality is now thought to make up some 69 p.c of the universe’s mass, whereas dark matter accounts for one more roughly 26 p.c. Regular matter — folks, planets, stars, and anything you may see — contains nearly 5 p.c of the cosmos. 

An important affect of darkish vitality is that the universe’s enlargement won’t ever decelerate. It should solely speed up. 

Warmth dying of the universe

Many years of observations have solely confirmed researchers’ findings. All indicators now level to an extended and lonely dying that peters out towards infinity. The scientific time period for this destiny is “warmth dying.”

However issues will likely be quite desolate lengthy earlier than that occurs. 

“Simply” a pair trillion years from now, the universe can have expanded a lot that no distant galaxies will likely be seen from our personal Milky Way, which can have lengthy since merged with its neighbors. Ultimately, 100 trillion years from now, all star formation will stop, ending the Stelliferous Period that’s be operating since not lengthy after our universe first fashioned.


How did we uncover dark matter? What’s dark matter product of? How is dark matter totally different than darkish vitality? Astronomy’s free downloadable eBook, The Science Behind Dark Matter, incorporates all the things it is advisable know in regards to the elusive and invisible substance.


A lot later, within the so-called Degenerate Era, galaxies will likely be gone, too. Stellar remnants will collapse. And all remaining matter will likely be locked up inside black holes.  

In truth, black holes would be the final surviving sentinels of the universe as we all know it. Within the Black Gap Period, they’ll be the one “regular” matter left. However finally, even these titans will disappear, too.

Stephen Hawking predicted that black holes slowly evaporate by releasing their particles into the universe. First, the smaller, solar-mass black holes will vanish. And by a googol years into the longer term (a 1 adopted by 100 zeroes), Hawking radiation can have killed off even the supermassive black holes. 

No regular matter will stay on this ultimate “Darkish Period” of the universe, which can final far longer than all the things that got here earlier than it. And the second legislation of thermodynamics tells us that on this time-frame, all vitality will in the end be evenly distributed. The cosmos will settle at its ultimate resting temperature, simply above absolute zero, the coldest temperature doable.  

If this future appears darkish and miserable, take consolation in realizing that each earthling can have died lengthy earlier than we now have to fret about it. In truth, on this timescale of trillions of years, even the existence of our total species registers as however a quick ray of daylight earlier than an infinite winter of darkness.



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