Power and combinations of lenses · Physics Class 11–12 | StemPy Lab
Course 23.2·Lesson 2 of 3
Power and combinations of lenses
The power of a lens is P=f1
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Try the code and the simulations beside the lesson.
What the optician writes
An optician hands you a card that says −2.50 for the left eye. What does the number mean? It is the power of the lens, in a unit called the dioptre. The minus sign says the lens is concave. A strong lens has a short focal length and a large power. A weak lens has a long focal length and a small power.
The power of a lens is the reciprocal of its focal length in metre:
P=f1
Its unit is the dioptre, symbol D. One dioptre is one reciprocal metre, 1D=1m−1. A convex lens has a positive power and a concave lens has a negative power.
A lens with f=+25cm=+0.25m has P=0.25m1=+4.0D.
A lens with f=−40cm has P=−0.40m1=−2.5D.
A lens of +2.0D has f=2.0D1=0.50m=50cm.
Always change the focal length to metre first. A common slip is to put it in centimetre.
Why the unit is useful
The power of a lens tells how much it bends the light. A lens that bends rays twice as strongly has twice the power. It also tells us how powers combine. We find this out next.
An optician's card has a few more terms. Sphere is the power of the lens as we use it here. A reading addition such as +1.50 is extra convex power for the lower part of a lens, which helps near work. A cylinder value is for an eye that is more curved in one direction than in another. It uses a lens with a different power along two directions, which the course on the eye takes up.
Two lenses in contact
Put two thin lenses against each other. Light from a point object goes through the first lens, which forms an image. That image is the object for the second lens. For a distant object we can follow the rays.
For the first lens, with object distance u and image distance v1:
v11−u1=f11
The lenses touch, so the image at v1 is at the distance v1 from the second lens too. For the second lens it is the object, and its image is at v:
v1−v11=f21
Add the two equations. The term v11 cancels:
v1−u1=f11+f21
The pair behaves like one lens whose focal length f obeys f1=f11+f21. In terms of power:
P=P1+P2
The magnification is the product of the two, m=m1m2, because the second lens enlarges the image made by the first.
Worked example 1: a convex and a concave lens
A convex lens of +5.0D is pressed against a concave lens of −2.0D. Find the power and the focal length of the pair.
The power.P=+5.0D+(−2.0D)=+3.0D.
The focal length. We want f, so f=P1=3.0D1=0.333m=33.3cm.
The pair is converging, because the convex lens is stronger. If the two powers were equal and opposite, the pair would have zero power. Parallel light would pass straight through, like a plain sheet of glass.
Worked example 2: object and image through a pair
A convex lens of f1=+20cm is in contact with a concave lens of f2=−30cm. An object stands 90cm in front. Find the image and the magnification.
The pair.f1=20cm1−30cm1=60cm1, so f=+60cm.
The image.u=−90cm. We want v, so v1=u1+f1=−90cm1+60cm1=180cm1. Then v=+180cm.
The magnification.m=uv=−90cm180cm=−2.0.
Check lens by lens. The first lens gives v1=−90+20(−90)(20)cm=25.7cm with m1=−0.286. The second lens has a virtual object 25.7cm behind it, so u2=+25.7cm and v2=25.7−30(25.7)(−30)cm=180cm, with m2=7.0. Then m1m2=−2.0. It agrees.
Two lenses with a gap
Lenses in a camera or a telescope are not in contact. They are a distance d apart. A ray that goes through both is bent twice, and the second bending happens at a different height. We follow a ray to find out how the powers combine.
Send a ray parallel to the axis at the height h into the first lens L1. After L1 it heads for the focus of L1, so it has the slope −f1h. It reaches the second lens L2 at the height
h2=h−f1hd=h(1−f1d)
A thin lens of focal length f2 adds the slope −f2h2 to a ray at height h2. So after L2 the ray has a slope of size
f1h+f2h2=h[f11+f21(1−f1d)]
The equivalent focal lengthF is the height at which the ray came in, divided by this slope. So
F1=f11+f21−f1f2dthat isP=P1+P2−dP1P2
with d in metre. For d=0 this is the rule for lenses in contact.
Two convex lenses L1 and L2, 10 cm apart, with focal lengths 30 cm and 20 cm. Two rays parallel to the principal axis come from the left at heights 2.0 and 1.0 units. They bend a little at L1 and more at L2 and meet on the axis at a red point 10 cm behind L2. Dashed lines extend the final rays backwards until they meet the incoming rays on a purple dashed vertical line, the equivalent lens, which lies 5 cm to the right of L1. A red arrow from this line to the focus is labelled F equal to 15 cm. A scale bar shows 5 cm.
There is one more point to notice. The ray leaves L2 and crosses the axis at a distance slopeh2 behind L2. This is the back focal distance, F(1−f1d). It is not equal to F. The focal length F is measured from a plane of the equivalent lens, which lies inside the pair, as the picture shows.
Worked example 3: the numbers behind the picture
Two convex lenses have f1=30cm and f2=20cm, and they are 10cm apart.
The equivalent focal length.F1=30cm1+20cm1−(30cm)(20cm)10cm=0.0667cm−1. So F=15cm and P=6.7D.
The back focal distance.F(1−f1d)=15cm×(1−3010)=10cm behind L2.
Check without the formula.L1 alone would focus parallel light 30cm behind it. That is 20cm behind L2, so L2 meets a virtual object, u2=+20cm. Then v21=20cm1+20cm1, so v2=10cm. It agrees.
Start with the defaults, +3.0D and +5.0D. What is the power for d=0 and for d=10cm? Now make d larger. At what gap does the power fall to zero? Then give P2 a negative value, and see what a gap does to the pair.
Practise the separated pair
The direct method: one lens at a time
The formulas above give the equivalent lens. Often we want the image and the magnification for a real object. Then the simplest way is the direct method. We do not need any new formula.
Use the thin lens formula for L1. Find v1 and m1.
The image of L1 is the object of L2. Its distance from L2 is u2=v1−d. Keep the sign. If v1 is larger than d, the object of L2 is behind it. Then u2 is positive, and the object is virtual.
Use the thin lens formula for L2. Find v2 and m2.
The total magnification is m=m1m2.
Worked example 4: two convex lenses
An object 2.0cm tall is 30cm in front of L1 with f1=20cm. A second lens L2 with f2=15cm is 30cm behind L1. Find the final image.
Lens 1.u1=−30cm. v1=−30+20(−30)(20)cm=60cm and m1=−3060=−2.0. This image is 4.0cm tall and inverted.
The object of lens 2.u2=v1−d=60cm−30cm=+30cm. It is a virtual object, behind L2.
Lens 2.v2=30+15(30)(15)cm=10cm and m2=3010=+0.333.
Total.m=(−2.0)(+0.333)=−0.667, so h′=−0.667×2.0cm=−1.33cm.
Two convex lenses on one principal axis, L1 at the origin with focal length 20 cm and L2 30 cm to its right with focal length 15 cm, drawn to scale with a 10 cm scale bar and the heights drawn about five times larger. An upright blue object arrow 2.0 cm tall stands 30 cm in front of L1. Two rays leave its tip, one parallel to the axis and one through the centre of L1. After L1 they head for a first image, drawn as a dashed grey inverted arrow 4.0 cm tall at 60 cm behind L1, which lies beyond L2. Lens L2 bends both rays so that they meet at a red inverted final image, 1.33 cm tall, 10 cm behind L2.
The final image is real, 10cm behind L2, inverted and smaller. The picture shows exactly this, drawn to scale.
Try it in Python
The program takes the two convex lenses f1=30cm and f2=20cm and finds the power and the equivalent focal length for six gaps.
Common mistakes
Using centimetre in P=f1. The power is in dioptre only if f is in metre.
Forgetting that a concave lens has a negative power. In contact, a concave lens takes away from a convex one.
Adding powers for lenses that are apart. The simple sum is for lenses in contact. With a gap use P1+P2−dP1P2.
Measuring F from the second lens. The equivalent focal length is measured from the equivalent lens. The distance of the focus behind L2 is the back focal distance.
Dropping the sign of a virtual object. If the image of L1 falls beyond L2, then u2 is positive.