Mirrors and Ray Diagrams
Why does a spoon show you upside down? Slide the object in front of a concave, convex or plane mirror and watch the rays find the image, just like the ray diagrams in your textbook.
Class 7 Light · Class 10 ReflectionTry this
0 of 5 doneCheck a plane mirror: is the image as far behind it as you are in front?Hint: pick Plane and move the object
Make a real, upside-down image exactly the same size as the object.Hint: concave mirror, object at C
Make a shaving mirror: an upright, magnified image.Hint: concave mirror, object very close (inside F)
Send the image off to infinity.Hint: put the object exactly at F
Use a convex mirror. Can you ever make its image bigger?Hint: pick Convex and try every distance
What's happening
Light bounces like a ball
When light hits a mirror, it bounces off at the same angle it came in: the angle of incidence equals the angle of reflection. In a plane mirror the image is upright, the same size and as far behind the mirror as the object is in front, but left and right are swapped.
Curved mirrors focus or spread light
A concave mirror (curved in, like a spoon's inside) brings parallel rays together at its focus F. Depending on where the object is, it can make a real, inverted image or, very close up, a magnified upright one. A convex mirror (curved out) spreads light, always giving a small, upright image of a wide view.
The mirror formula
With the New Cartesian sign convention (distances measured from the pole; in front of the mirror is negative), the object distance u, image distance v and focal length f are linked by one formula. The magnification tells you the size: negative means inverted.
Who figured this out?
Euclid
About 300 BCE, AlexandriaA book called Catoptrics, credited to Euclid, set out the law of reflection: light bounces off a mirror at the same angle it arrives.
Ibn al-Haytham
About 1021, CairoIn his Book of Optics he showed by experiment that we see because light travels from objects into our eyes, and studied how curved mirrors form images.
Isaac Newton
1668, EnglandBuilt the first practical reflecting telescope, using a concave mirror instead of a lens. Most big telescopes today follow his idea.
Learn more
- Curved mirror · Wikipedia
- Reflecting telescope · Wikipedia
Check yourself
1. Where should an object be placed in front of a concave mirror to get a real image of the same size?
2. Which mirror is used as a rear-view mirror in vehicles?
3. A concave mirror has a focal length of 15 cm. An object is placed 30 cm in front of it. Where is the image?
4. Why do dentists use concave mirrors?
Common questions
How do you draw a ray diagram for a concave mirror?
From the top of the object draw at least two rays. A ray parallel to the principal axis reflects through the focus F. A ray through F reflects parallel to the axis. A ray through the centre of curvature C reflects back along itself, and a ray hitting the pole reflects at an equal angle. Where the reflected rays meet (or appear to meet) is the top of the image.
What is the mirror formula?
1/v + 1/u = 1/f, where u is the object distance, v the image distance and f the focal length, all measured from the pole using the New Cartesian sign convention. Magnification m = −v/u = image height ÷ object height.
What is the difference between a concave and a convex mirror?
A concave mirror curves inward and converges light; it can form real or virtual images and is used in torches, shaving mirrors and solar furnaces. A convex mirror curves outward and diverges light; it always forms virtual, upright, diminished images and is used as rear-view mirrors and on blind corners.
What images does a concave mirror form for different object positions?
Beyond C: real, inverted, diminished, between F and C. At C: real, inverted, same size, at C. Between C and F: real, inverted, magnified, beyond C. At F: image at infinity. Between F and the mirror: virtual, upright, magnified, behind the mirror.
What is the relation between focal length and radius of curvature?
For a spherical mirror the focal length is half the radius of curvature: f = R/2. The focus lies halfway between the pole and the centre of curvature.
What is the sign convention for mirrors?
In the New Cartesian sign convention, all distances are measured from the pole. Distances in the direction of the incoming light (behind the mirror) are positive and against it (in front) are negative. Heights above the principal axis are positive. So a concave mirror has a negative focal length and a convex mirror a positive one.
Paraxial rays (close to the axis), as in the Class 10 textbook. Real curved mirrors blur slightly at the edges (spherical aberration).
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