IB Maths AA HL Topic 1 β€” Number & Algebra Paper 1 & 2 ~6 min read

Standard Form

Standard form is just a tidy way of writing very big or very small numbers. The IB requires you to write your final answer in this form when asked, so the trick isn’t really the maths β€” it’s spotting when a number isn’t in the correct shape, and fixing it. Your GDC will handle most of the heavy lifting; you just need to read its output properly.

πŸ“˜ What you need to know

What does standard form actually mean?

Some numbers are too big or too small to write out comfortably. The mass of the Earth is roughly 5,972,000,000,000,000,000,000,000 kg. The diameter of a hydrogen atom is about 0.000000000106 m. Counting zeros for either is a recipe for losing marks. Standard form pulls that whole mess into something compact.

Standard form a Γ— 10n,   where   1 ≀ a < 10   and   n ∈ β„€ βœ— not in the formula booklet β€” memorise the form

🌍 Real-world feel

Earth’s mass β‰ˆ 5.97 Γ— 1024 kg. Hydrogen atom β‰ˆ 1.06 Γ— 10βˆ’10 m. Both numbers fit on one line, the powers tell you the scale at a glance, and you don’t have to count zeros twice.

Writing numbers in standard form

The whole game is moving the decimal point until exactly one non-zero digit sits in front of it. Then count how many places you moved.

Where the decimal point lands
Large number: 47 800 4.7800 ↑ decimal moved 4 places left β†’   4.78 Γ— 104 positive power Small number: 0.000356 000 03.56 ↑ decimal moved 4 places right β†’   3.56 Γ— 10βˆ’4 negative power
Quick mental check: if the original number is bigger than 10, the power is positive. If it’s smaller than 1, the power is negative. If it’s between 1 and 10, the power is 0.

Multiplying and dividing

This is the part students like β€” the powers of 10 obey the index laws, and the leading numbers just multiply or divide as normal.

Γ—
Multiply
(a1 Γ— 10m) Γ— (a2 Γ— 10n)
= (a1 Γ— a2) Γ— 10m + n
Γ·
Divide
(a1 Γ— 10m) Γ· (a2 Γ— 10n)
= (a1 Γ· a2) Γ— 10m βˆ’ n
After multiplying or dividing the leading parts, check that the result still satisfies 1 ≀ a < 10. If it doesn’t, shift the decimal and adjust the power. That last shuffle is where almost all the marks get lost.

🧭 Recipe β€” multiply or divide in standard form

  1. Group: separate the leading numbers from the powers of 10.
  2. Operate: multiply (or divide) the leading numbers; add (or subtract) the indices.
  3. Standardise: if the new a isn’t between 1 and 10, write it in standard form, then combine the powers of 10 again.

Adding and subtracting

This is where students slow down. You can’t just add the leading numbers β€” the powers of 10 must match first.

🧭 Recipe β€” add or subtract in standard form

  1. Pick the bigger power of 10 and rewrite the smaller-power term so its 10n matches.
  2. Now add or subtract the leading numbers β€” the powers of 10 are just a common factor.
  3. Standardise the final answer so 1 ≀ a < 10.

πŸ€” Why match powers first?

Because 105 and 104 are different units of size. Adding “3 millions” and “5 thousands” only works if you first convert one of them β€” same idea here. Pull a common power of 10 out as a factor, then add what’s left.

Negative powers β€” same logic: 10βˆ’6 is bigger than 10βˆ’9. The “highest” (least negative) power wins. Match the smaller-power term up to it before combining.

Worked examples

WE 1

Convert to and from standard form

(i) Write 92 400 in standard form.    (ii) Write 6.7 Γ— 10βˆ’5 as an ordinary number.

(i) 92 400 β†’ standard form move decimal 4 places left: 9.2400 9.24 Γ— 104 (ii) 6.7 Γ— 10βˆ’5 β†’ ordinary negative power β†’ small number; move decimal 5 places left 0.000067
WE 2

Multiplication that needs standardising

Calculate (4 Γ— 107) Γ— (3 Γ— 105), giving the answer in standard form.

Step 1: Group leading numbers and powers = (4 Γ— 3) Γ— (107 Γ— 105) = 12 Γ— 1012 Step 2: Standardise β€” 12 is not between 1 and 10 12 = 1.2 Γ— 101 so 12 Γ— 1012 = 1.2 Γ— 101 Γ— 1012 = 1.2 Γ— 1013 forgetting to standardise the leading number is the #1 mark-losing slip
WE 3

Division giving a negative power

Calculate (3 Γ— 102) Γ· (8 Γ— 106), giving the answer in standard form.

Step 1: Group = (3 Γ· 8) Γ— (102 Γ· 106) = 0.375 Γ— 102 βˆ’ 6 = 0.375 Γ— 10βˆ’4 Step 2: Standardise β€” 0.375 is less than 1 0.375 = 3.75 Γ— 10βˆ’1 so 0.375 Γ— 10βˆ’4 = 3.75 Γ— 10βˆ’1 Γ— 10βˆ’4 = 3.75 Γ— 10βˆ’5
WE 4

Addition with different powers

Calculate (6 Γ— 108) + (4 Γ— 107), giving the answer in standard form.

Step 1: Match the powers β€” pick 108 4 Γ— 107 = 0.4 Γ— 108 Step 2: Add the leading numbers (6 Γ— 108) + (0.4 Γ— 108) = 6.4 Γ— 108 = 6.4 Γ— 108 already in standard form β€” no extra adjustment needed
WE 5

Subtraction with negative powers

Calculate (5 Γ— 10βˆ’6) βˆ’ (2 Γ— 10βˆ’7), giving the answer in standard form.

Step 1: Spot the bigger power β€” 10βˆ’6 is bigger than 10βˆ’7 2 Γ— 10βˆ’7 = 0.2 Γ— 10βˆ’6 Step 2: Subtract (5 Γ— 10βˆ’6) βˆ’ (0.2 Γ— 10βˆ’6) = 4.8 Γ— 10βˆ’6 = 4.8 Γ— 10βˆ’6 βˆ’6 is “bigger” than βˆ’7 β€” number-line thinking, not absolute value
WE 6

Application β€” light travel time

Light travels at approximately 3 Γ— 108 m/s. The Sun is approximately 1.5 Γ— 1011 m from Earth. How long, in seconds, does sunlight take to reach Earth? Give your answer in standard form.

Step 1: time = distance Γ· speed t = (1.5 Γ— 1011) Γ· (3 Γ— 108) Step 2: Group and divide = (1.5 Γ· 3) Γ— 1011 βˆ’ 8 = 0.5 Γ— 103 Step 3: Standardise β€” 0.5 is not between 1 and 10 0.5 Γ— 103 = 5 Γ— 102 t = 5 Γ— 102 seconds (β‰ˆ 8.3 min)

πŸ’‘ Top tips

⚠ Common mistakes

Standard form looks small, but it’ll show up in nearly every paper β€” Paper 2 problems with very large or very small physical quantities, and any time IB tells you to give your answer to 3 significant figures. Get fluent on it now and you’ll never lose marks here.

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