Mixed

How many times would you have to fold paper to reach the sun?

How many times would you have to fold paper to reach the sun?

In fact, if you had a sheet of paper, and folded it in half 50 times, how thick would it be? The answer is about 100 million kilometres, which is about two thirds of the distance between the Sun and the Earth. And so Accepted Wisdom on Paper-Folding ruled, until 2001.

Why can you only fold paper 7 times?

The commonly accepted wisdom is that you can’t fold a single sheet of paper in half more than seven times. The problem with folding paper in half multiple times is that the paper’s surface area decreases by half with each fold. With the assistance of a forklift and steamroller, they get the paper to fold 11 times.

Can you fold paper 42 times and still get the Moon?

Yes, on folding the paper 42 times , it would reach the moon. if the paper is folded 42 times, then there would be 2^42 (=4,398,046,511,104) layers of paper. Standard office paper is 0.1 mm thick. So

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What happens if you fold a piece of paper 103 times?

Problem: If you fold it 103 times (only if you could ) , the thickness of your paper will be larger than the observable Universe: 93 billion light-years. Yes,on folding the paper 42 times ,it would reach the moon. if the paper is folded 42 times, then there would be 2^42 (=4,398,046,511,104) layers of paper.

What is the distance between the Moon and the paper?

Double that twice more and you end up with four trillion. Assuming that 200 sheets of paper makes one inch, Then four trillion layers would be 20 billion inches, or 1,667 million feet, or 315,000 miles. The moon’s distance varies, but it’s generally around 250,000 miles away.

How many kilometers are in 42 folds of paper?

The formula for finding out how many of something you’ll have after doubling it N number of times is as follows where O is the original number (or size in our case). A standard sheet of paper is about 0.1 mm so 42 folds would give us this: That’s 440 billion millimeters, or 439,804 kilometers.