Geometric Optics
When obstacles are much larger than the wavelength, light can be treated as straight rays. That approximation covers mirrors, lenses, eyes and telescopes — everything optical you use, right up to the point where Unit 9 shows why it must eventually fail.
- Apply the laws of reflection and refraction.
- Compute critical angles and explain total internal reflection.
- Use the mirror and lens equations with correct sign conventions.
- Distinguish real from virtual images.
Tracing rays is far simpler than solving wave equations, and it gives the right answer whenever the wavelength is negligible. Knowing when the approximation holds is as important as the approximation itself.
Spectacles, cameras, microscopes, telescopes. Optical fibre carries essentially all long-distance internet traffic by total internal reflection, trapping light inside a glass thread for thousands of kilometres.
Snell found the refraction law in 1621; Ibn Sahl had described it in Baghdad six centuries earlier. Fermat later showed it follows from light taking the path of least time — a reformulation that turned out to anticipate how modern physics states its laws.
Reflection and refraction
The angle of reflection equals the angle of incidence, both measured from the normal — the perpendicular to the surface, not the surface itself.
The refractive index is $n = c/v$, so a larger $n$ means slower light. Air is about $1.00$, water $1.33$, glass around $1.5$.
Going from slower to faster, the refracted ray bends away from the normal. Beyond a certain incidence angle it would need to exceed $90$ degrees, which is impossible — so none escapes and all the light reflects.
This is the only kind of reflection that is perfectly lossless, which is exactly why optical fibre works over long distances.
Mirrors and lenses
Sign conventions, which is where the marks are:
An object $30$ cm from a lens of focal length $10$ cm.
Now $5$ cm from the same lens.
The commonest arithmetic error is solving for $1/d_i$ and reporting it as $d_i$. Check the sign as well: it tells you real or virtual, which is usually what the question is actually asking.
The eye and corrective lenses
• Measuring angles from the surface rather than the
normal.
• Applying the critical-angle formula going into a denser medium. Total
internal reflection only happens dense to
sparse.
• Forgetting to invert after solving for $1/d_i$.
• Getting the focal-length sign wrong for a diverging
element.
• Treating a negative image distance as a mistake rather than as
"virtual".
Practice
Work each fully before opening the answer. Original exercises written for this guide in the style of the course's problem sets.
Light hits water at $40$ degrees from the normal. Find the refraction angle.
Answer
Find the critical angle for glass of $n = 1.5$ to air.
Answer
Does light bend toward or away from the normal entering glass from air?
Answer
An object $20$ cm from a $15$ cm converging lens. Find the image.
Answer
How do you know an image is virtual from the arithmetic?
Answer
Why does light stay in an optical fibre?
Solution
What does a $+2.0$ D lens do, and which defect does it correct?
Answer
Where is the image in a flat mirror, and is it real?
Answer
Expanded topic checklist
Course coverage. This unit is part of the complete PHY132H1 topic map. It should cover the following items before you move on:
- Reflection and refraction. Angles from the normal, and Snell's law.
- Total internal reflection. The critical angle and its one-way condition.
- Mirrors and lenses. The equation, the sign conventions, and magnification.
- Images. Real versus virtual, and reading the answer off the sign.
The calendar names "optics". Check the syllabus on Quercus for assigned problems; ray diagrams and the sign conventions are standard laboratory and exam material.
Light changes speed between media, which bends it. Curved surfaces bend rays to a focus, and one equation with careful signs handles every mirror and lens. Unit 9 takes over where the ray picture fails.
Deep practice extensions
Use these after the main practice set. They push on definitions and edge cases rather than routine calculation.
From what are optical angles measured?
Guide
When can total internal reflection occur?
Guide
What does a negative image distance mean?
Guide
When does geometric optics break down?