JAMB Physics · Section A
Study notes for Light Energy — part of the JAMB UTME Physics syllabus. 12 learning objectives with explanations and exam tips.
When sound waves bounce back and forth inside a pipe, they create standing waves at specific frequencies. An open pipe has both ends free to vibrate, so it resonates when the pipe length equals half a wavelength, or multiples of that. A closed pipe has one end blocked, so it resonates at odd multiples of quarter wavelengths instead.
Think of a Nigerian talking drum or the metal pipes used in our local music. When you blow air through an open bamboo flute, it produces different notes depending on length—longer pipes give lower notes. With closed pipes like some traditional horns, the physics works differently because sound can only exit one end.
The key difference: open pipes vibrate at all harmonics (fundamental and overtones), while closed pipes vibrate only at odd harmonics. This is why organ pipes in churches sound different based on whether they're open or closed.
When sound travels through a closed pipe—like a bottle or a metal tube closed at one end—it creates standing waves. The closed end forces the sound wave to reflect, creating nodes (points of no vibration) at that closed end. This means closed pipes produce specific frequencies based on their length. A pipe that is one-quarter of a sound wave's wavelength will resonate at the fundamental frequency. Think about blowing across a bottle of Fanta; different water levels create different pitches because they change the effective length of the closed air column. The longer the closed pipe, the lower the frequency produced. This relationship helps musicians tune instruments and engineers design acoustic spaces. Understanding this principle means knowing that closed pipes resonate when their lengths equal odd multiples of one-quarter wavelength: L = λ/4, 3λ/4, 5λ/4, and so on.
Natural light comes directly from nature without human intervention. The sun is our primary natural light source, providing energy that powers life on Earth. Other examples include moonlight, lightning, and bioluminescence from fireflies you see in Nigerian villages at night.
Artificial light is produced by humans using energy conversion. Electric bulbs, fluorescent tubes, and LEDs all convert electrical energy into light. When you switch on the generator in your home during darkness, the bulb lighting up is artificial light. The key difference is that natural light originates from natural processes, while artificial light requires human-made devices and energy input.
Both serve important purposes. Natural light is free and essential for health, while artificial light extends our productive hours and enables activities at night. Understanding these sources helps you grasp how light energy transforms and supports human life.
Light energy comes from different sources around you. Natural sources include the sun, which provides daylight and makes life on Earth possible. Fire from burning materials like wood or candles also produces light through heat. Living things like fireflies and certain deep-sea fish create their own light through chemical reactions in their bodies. Artificial sources are human-made and include electric bulbs, fluorescent tubes, and LED lights that power homes and streets in Lagos and other Nigerian cities. When electricity flows through a filament in an incandescent bulb, it heats up and glows, producing both light and heat. Understanding these sources helps you appreciate why light behaves differently depending on where it comes from.
A luminous object is anything that produces its own light. Think of the sun, electric bulbs, or a burning candle—these emit light energy. Non-luminous objects, on the other hand, do not produce light themselves. They only become visible when light from luminous objects shines on them. Your textbook, this phone you're reading, and even the moon are non-luminous because they reflect light from other sources.
Consider a Nigerian example: during evening, a kerosene lamp is luminous and produces its own light. The walls of your room are non-luminous—you see them only because the lamp's light bounces off them. Without that light source, the walls remain invisible in darkness.
This distinction matters because luminous objects are actual light sources, while non-luminous objects are merely reflectors. Understanding this helps explain why we see things and how light travels.
A luminous object is anything that produces its own light energy. Think of it this way: if an object glows or shines because it's actually making light, not just reflecting someone else's light, then it's luminous. The sun is the classic example—it generates light through nuclear reactions inside it. In Nigeria, a kerosene lamp is a perfect everyday example; it produces light by burning fuel, making it luminous. Your phone's screen also produces its own light, so it counts as luminous too.
The key difference is between luminous and non-luminous objects. The moon isn't luminous because it doesn't make light; it only reflects sunlight. A white wall in your house works the same way—it reflects light but doesn't produce any. This distinction appears regularly in JAMB questions and it's crucial to get it right.
Light travels as waves, and three things describe how it moves: speed, frequency, and wavelength. Speed is how fast light travels (300,000 km/s in vacuum). Frequency is how many wave peaks pass a point per second, measured in Hertz. Wavelength is the distance between two consecutive peaks. These three connect through one simple equation: speed equals frequency multiplied by wavelength (v = fλ).
Think of it like Lagos traffic: if cars (wave peaks) pass faster and are closer together, they're moving quicker. Red light has longer waves and lower frequency, while blue light has shorter waves and higher frequency. Both travel at the same speed through space, but they behave differently because of their wavelengths and frequencies.
Wavelength is simply the distance between two consecutive peaks (or troughs) of a light wave as it travels. Think of it like the space between one crest and the next crest when you drop a stone in water. Different colours of light have different wavelengths. Red light has the longest wavelength at about 700 nanometres, while violet light has the shortest at around 400 nanometres.
You can actually observe this in Nigeria during harmattan season when dust particles scatter blue light more than red light, making sunsets appear reddish. This happens because blue light's shorter wavelength gets scattered more easily by particles in the air.
The relationship between wavelength, frequency, and speed is important: speed of light equals wavelength multiplied by frequency. These three quantities always work together.
A shadow forms when light travels in straight lines and hits an opaque object, blocking its passage. The light cannot bend around the object, so a dark area appears on the opposite side where light has been blocked. The size and shape of a shadow depend on the position of the light source and the object.
Think of how your shadow appears on the ground during midday when the sun is directly overhead—it's short and directly beneath you. But in the evening when the sun is lower on the horizon, your shadow stretches long across the ground. This happens because the angle between the light source and object changes.
In Nigeria, you see this clearly when trading in markets. A trader's stall creates a shadow on goods beneath it when sunlight hits from above. The shadow's darkness depends on how completely the light is blocked by the stall's material.
Light travels in straight lines in a uniform medium—this is the principle of rectilinear propagation. Imagine shining a torch in a dark room: the beam goes straight until it hits something or changes medium. This happens because light energy moves as rays that don't bend unless they encounter obstacles or different materials.
Think about shadows you see at noon under the hot Nigerian sun. The sharp, clear shadow of a tree occurs because light rays travel straight from the sun, hitting the tree trunk and creating a dark region directly behind it. The shadow's sharp edges prove that light hasn't curved around the tree; it travels in perfectly straight paths.
This principle helps us understand many optical instruments like cameras and telescopes. When light rays are blocked, shadows form exactly where you'd predict using straight-line geometry.
A pin-hole camera is simply a dark box with a tiny hole on one side. Light from an object passes through this small hole and projects an inverted image on the opposite side inside the box. The smaller the hole, the sharper your image becomes. Think of it like this: when you're sitting in a dark cinema and light enters through a small opening, it creates the same effect on the screen.
Imagine standing outside a Lagos cinema on a sunny afternoon. If you make a small hole in black cardboard and hold it up, you'll see an inverted image of the building or vehicles passing by projected inside your box. This happens because light travels in straight lines, and only rays passing through the tiny hole can reach the screen inside.
The pin-hole camera demonstrates that light behaves predictably and follows geometric rules. This principle led to the development of modern photography.
When light hits a mirror or any shiny surface, it bounces back following specific rules called the laws of reflection. The first law states that the angle at which light arrives at a surface equals the angle at which it bounces away. These angles are measured from an imaginary line called the normal, which stands perpendicular to the surface.
The second law says the incident ray, reflected ray, and normal all lie in the same plane. Think of a student looking at their face in a mirror at home—the light from their face hits the mirror at a certain angle and reflects back at exactly the same angle, allowing them to see a clear image.
These laws work the same way for any reflective surface, whether polished or rough. Understanding the angle relationships is crucial because examiners love asking you to calculate reflection angles using geometry.