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The observable universe is about 93,000,000,000 light-years across, while a single hydrogen atom spans just 0.000000000106Β meters. Writing out dozens of trailing or leading zeros wastes time and easily leads to counting errors.
To solve this, scientists use scientific notation, a standard format where every number is written as a decimal between 1 and 10 multiplied by a power of 10.
Anatomy of Scientific Notation
In scientific notation, every value is expressed as aΓ10n. The number a is the coefficient (a decimal where 1β€β£aβ£<10), and n is an integer exponent that indicates how many places the decimal moved.
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In the 3rd century BCE, Archimedes first investigated powers of 10 in his treatise The Sand Reckoner to estimate how many grains of sand would fill the cosmos, laying the foundation for our modern exponent system.
How do we take a giant real-world measurement and rewrite it in this compact format without changing its value?
Converting Large Numbers
When a number is greater than 10, shift the decimal point to the left until only one non-zero digit remains in front of it. The number of places you shift becomes your positive exponent.
For example, the average distance from Earth to the Sun is approximately 149,600,000Β km. Moving the decimal point 8 places to the left gives 1.496Γ108Β km.
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Large numbers multiply by factors of 10, but what happens when we zoom into microscopic dimensions where numbers are much smaller than 1?