What will happen after quadrillion years?

Eventually it will become nothing. In roughly a quadrillion years, a last star will give its last twinkle, and black holes will devour everything before they completely evaporate. And in a googol years (that’s 10 to the hundredth power, which is a lot), the universe will be empty.

How does googol look like?

A googol, officially known as ten-duotrigintillion or ten thousand sexdecillion, is a 1 with one hundred zeros after it. Written out, a googol looks like this: 10,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000.

What will the universe look like in 1 trillion years?

By the year 1 trillion, the accelerating universe will have infinitely stretched the light from all external galaxies – assuming dark energy truly is Einstein’s cosmological constant and not an unstable field that winds up destroying the universe. Their existence will show that the universe cannot be eternal.

How would you visualize a googol year?

I suppose if you want to “visualize” a googol years, the best I can think of uses the fact that the number of atoms on Earth is roughly 10 50, which is the square root of googol. So imagine trying to count every single atom on Earth, at a rate of one per year.

What will the world look like in 5 billion years?

Life will have changed vastly. There could be no death, no disease, no communists and a different coloured gearstick on the Jeep. People will be going round with their iPhone half-of-a-google “s”. Unfortunately the Sun is only expected to last for another 5 billion years.

How long will the universe be empty?

In roughly a quadrillion years, a last star will give its last twinkle, and black holes will devour everything before they completely evaporate. And in a googol years (that’s 10 to the hundredth power, which is a lot), the universe will be empty. Physicists speculate that emptiness will last for an infinite time period.

What happens as time goes on in the universe?

As time goes on, Gravitation weakens, Black Holes go through phase-transitions until they become Neutron Starts… then more time goes by and Neutron Stars surfaces start to evaporate by releasing free neutrons… If you notice, G is epoch-dependent. It depends upon the 4D radius of the Universe.