Welcome back to Scientific Notation in Real Life! This is our second lesson out of six in the course, so we are off to a strong start. In Lesson 1, we learned how to read scientific notation — picking apart the coefficient and the power of ten, checking for proper form, and expanding expressions back into standard numbers. Now we are going to flip that skill around: given a large standard-form number, we will learn how to write it in proper scientific notation.

By the end of this lesson, you will be able to take a number like $149{,}600{,}000$ (the approximate distance from Earth to the Sun in kilometers) and express it neatly as a coefficient times a power of ten. Let's get to it!

Think about how often you see big numbers in headlines: a country's population, a company's revenue, the distance to another planet. These numbers are packed with zeros that make them hard to read, compare, and use in calculations. Scientific notation strips away that clutter by separating the meaningful digits from the scale.

Converting a large number into scientific notation is really just the reverse of what we did in Lesson 1. Back then, we started with a compact expression like $4.6 \times 10^3$ and expanded it to $4{,}600$ by moving the decimal to the right. Now we start with the long number and compress it back down. The entire task comes down to two questions: where does the decimal point go to create a proper coefficient, and how many places did it move?

Recall that proper scientific notation requires a coefficient $a$ satisfying $1 \leq a < 10$. In practice, that means exactly one nonzero digit sits to the left of the decimal point.

To find the coefficient, locate the leftmost nonzero digit of the number and place the decimal point directly after it. For example, with the number $4{,}500{,}000$:

• The leftmost nonzero digit is 4.
• Place the decimal right after it: 4.500000.
• Drop the trailing zeros: the coefficient is 4.5.

Once we have the coefficient, we need the power of ten. The exponent tells us how many places the decimal point traveled from its new position (right after the first digit) to where it originally sat (at the far right end of the whole number).

Let's continue with $4{,}500{,}000$. In standard form the decimal point lives at the far right: $4500000.$ We moved it to sit right after the 4, which means it shifted 6 places to the left. Each leftward shift corresponds to one power of ten, so the exponent is $6$.

Let's pull the steps together and apply them to a real-world value. The average distance from Earth to the Moon is approximately 384,400 kilometers.

1. Find the first nonzero digit. It is 3.
2. Place the decimal after it to form the coefficient: $3.844$.
3. Count the places the decimal moved. From the original position at the far right of $384400.$ to just after the $3$ is 5 places.
4. Write the result:

Let's try another example. Suppose a country has a population of 67,000,000 — roughly the population of France or the United Kingdom.

1. First nonzero digit: 6.
2. Coefficient: $6.7$.
3. Decimal shifts: from the end of $67000000.$ to after the $6$ is 7 places.
4. Result:

Here is the full process in table form, applied to the Earth-to-Sun distance of $149{,}600{,}000$ km:

Before we wrap up, here are a few pitfalls worth keeping in mind:

• Coefficient out of range. Writing $15 \times 10^7$ instead of $1.5 \times 10^8$. If the coefficient is 10 or greater (or less than 1), the notation is not in proper form. Always verify that .

In this lesson, we learned how to convert large standard-form numbers into proper scientific notation. The process has two core moves: place the decimal after the first nonzero digit to create a coefficient between 1 and 10, then count how many places the decimal shifted to determine the positive exponent. We practiced with real-world values like the Earth-to-Moon distance and national populations, and we reviewed the most common mistakes that can trip you up.

Up next are hands-on exercises where you will convert increasingly large numbers into scientific notation — from guided fill-in-the-blank warm-ups all the way to full conversions of truly massive quantities like light-year distances. Time to put those decimal-shifting skills into action!