Getting Started: The Language of Physics

Imagine trying to bake a cake if the recipe just said "add 200 flour" or "bake for 30." You would probably end up with a mess! In Physics, units are the language we use to make sure our measurements make sense. Whether we are measuring the tiny distance across an atom or the massive distance to a star, we need a consistent way to talk about numbers.

In this chapter, we will look at the standard units used in the AQA syllabus, how to use prefixes to handle very large or small numbers, and how to use significant figures to show how precise our measurements really are.


1. SI Units: The Gold Standard

Scientists all over the world use the SI system (International System of Units). This ensures that a measurement taken in a lab in London is understood perfectly by a scientist in Tokyo.

For your GCSE, you need to be comfortable with these core units:

  • Length: measured in metres \( (m) \)
  • Mass: measured in kilograms \( (kg) \)
  • Time: measured in seconds \( (s) \)
  • Current: measured in amperes \( (A) \)
  • Temperature: measured in degrees Celsius \( (^\circ C) \) or Kelvin \( (K) \)

Quick Tip: Always check your units before starting a calculation! Most physics equations (like \( F = m \times a \)) require the numbers to be in these standard units. If your mass is in grams, you must convert it to kilograms first.


2. Prefixes: Handling Huge and Tiny Numbers

Physics deals with everything from the size of the universe to the size of an electron. Writing out all those zeros is exhausting and leads to mistakes. Instead, we use prefixes.

The AQA syllabus requires you to know the prefixes from Tera down to nano. Think of these as "multipliers" for the base unit.

The "Big" Prefixes (Multipliers)
  • Tera \( (T) \): \( \times 10^{12} \) (one trillion times bigger)
  • Giga \( (G) \): \( \times 10^9 \) (one billion times bigger)
  • Mega \( (M) \): \( \times 10^6 \) (one million times bigger)
  • kilo \( (k) \): \( \times 10^3 \) (one thousand times bigger)
The "Small" Prefixes (Dividers)
  • milli \( (m) \): \( \times 10^{-3} \) (one thousandth)
  • micro \( (\mu) \): \( \times 10^{-6} \) (one millionth)
  • nano \( (n) \): \( \times 10^{-9} \) (one billionth)

Example: A distance of \( 5\text{ kilometres} (5\text{ km}) \) is the same as \( 5 \times 10^3\text{ m} \) or \( 5,000\text{ m} \).

Memory Trick: To remember the order of the big ones, think Terrible Giant Monsters kill! (Tera, Giga, Mega, kilo).


3. Standard Form

Standard form is a way of writing very large or very small numbers easily. It always looks like this: \( A \times 10^n \).

  • \( A \) is always a number between 1 and 10.
  • \( n \) tells you how many places to move the decimal point.

Example (Large Number): The speed of light is roughly \( 300,000,000\text{ m/s} \). In standard form, we write this as \( 3 \times 10^8\text{ m/s} \).

Example (Small Number): The radius of an atom is about \( 0.0000000001\text{ m} \). In standard form, this is \( 1 \times 10^{-10}\text{ m} \).


4. Significant Figures (sf)

In your exams, you will often be asked to "give your answer to an appropriate number of significant figures." This is all about precision. Your answer shouldn't look more precise than the data you started with!

The Golden Rule

In a calculation, your final answer should usually be rounded to the same number of significant figures as the piece of data with the fewest significant figures used in the calculation.

How to Count Significant Figures:
  1. All non-zero digits are significant. (\( 435 \) has 3 sf).
  2. Zeros between non-zero digits are significant. (\( 405 \) has 3 sf).
  3. Leading zeros (at the start) are NOT significant. They are just placeholders. (\( 0.0045 \) only has 2 sf).
  4. Trailing zeros AFTER a decimal point are significant. They show exactly how precise the measurement was. (\( 4.50 \) has 3 sf).

Common Mistake: Don't round your numbers too early! Keep all the digits on your calculator during the middle of a multi-step calculation, and only round to the correct significant figures at the very end.


5. Unit Conversions: Step-by-Step

Converting units can be tricky at first, but it follows a simple logic. Don't worry if it takes a moment to click!

Step 1: Identify the prefix. (e.g., \( 5\text{ mA} \) to \( A \)).
Step 2: Recall the multiplier. (milli is \( 10^{-3} \) or divide by \( 1,000 \)).
Step 3: Do the math. \( 5 / 1,000 = 0.005\text{ A} \).

Did you know? Using the wrong units can be disastrous. In 1999, a Mars orbiter was lost in space because one team used imperial units (pounds) and another used metric units (newtons). Always double-check your units!


Quick Review: Key Takeaways

  • SI Units: Stick to metres, kilograms, seconds, and amperes for calculations.
  • Prefixes: Use them to scale units (e.g., \( k = 1,000 \), \( m = 0.001 \)).
  • Standard Form: Use \( A \times 10^n \) to keep large/small numbers tidy.
  • Significant Figures: Match your answer's precision to the data provided in the question.

Note: For more information on how to use these units in experiments, see the "Experimental design, variables and apparatus" chapter.