| Description |
|---|
|
If the object and the image screen be placed on an optical
bench that the distance (D) between them is greater than four time
the focal length(f) of a given convex lens, then there will be two
different positions of the lens for which an equally sharp image
will be obtained on the image screen. Let the points O and l and
L1 in figure-1 represent respectively the positons of the
object and the imge screen and two different positions of the lens
for which an equally sharp image is formed. Let distance OI = D and
L1 - L2 = x. From the lens equation, we have 1 ⁄ V - 1 ⁄ U = 1 ⁄ f 1 ⁄ D-U - 1 ⁄ U = 1 ⁄ f [using V + U =0] Applying sign convention, u is negative 1 ⁄ D-U + 1 ⁄ U = 1 ⁄ f u2 - ud + df = 0 Solving the above equation which is quadratic, we have two values of corresponding to the two positions of the lens. These are: u2 = D ⁄ 2 - √(D2 - 4Df ⁄ 2), Position L1 of lens u2 = D ⁄ 2 + √(D2 - 4Df ⁄ 2), Position L2 of lens Then x = L1 ~ L2 = u1 ~ u2 = +- √( D2 - 4Df ) or x2 = D2 - 4Df or f = D2- x2 ⁄ 4D -----(1) Where D is the distance between the object adn the image msut be greater than 4f and x is the distance between two different positions of lens. The power of P lens is as usual given by the realtion, P = 100 ⁄ f (in cm) dioptres |
| Length of the index rod in c, (l) | Difference of bench scale reading in cm when the two ends of index rod touch the object and screen (d) | Index correction for D in cm, lambda = (l-d) |
|---|---|---|
| Usually a difference of 0.5 |
| No of obs. |
Position of
|
Displacement of lens x = L1 ~ L2 | Apparent distance between objects and image, D` = O ~ I | Corrected distance between object and image, D = D` + lambda | |||||
|---|---|---|---|---|---|---|---|---|---|
| 1 | |||||||||
| 2 | |||||||||
| 3 |
| No of obs./th> | lens displacement (x) from table-II | Corrected distance (D) from table-II |
Focal length, F = D2-x2 ⁄ 4D |
Mean focal length (f) (cm) | Power, P = 100 ⁄ f dioptres |
|---|
| Point | Explanation |
|---|---|
| 1 | The lens was first used to focus sunlight on paper to get a sharp image; this gave the rough focal length (f). |
| 2 | A distance about four times the focal length (4f) was set between the object (illuminated pin) and the screen. |
| 3 | The lamp, object pin, lens, and screen were adjusted in a straight line at the same height on the optical bench. |
| 4 | The lens was moved to form a clear, inverted image of the pin on the screen — this was the first lens position. |
| 5 | Without shifting the object or screen, the lens was moved to the other side to get another sharp image — the second lens position. |
| 6 | The positions of the object, lens (both positions), and image were carefully measured and noted. |
| 7 | The object was then moved 5 cm backward, and steps 4–6 were repeated for three sets of readings. |
| 8 | All readings were entered in Table-II, and the distance (D) and displacement (d) were calculated for each observation. |
| 9 | The focal length (f) was found using f = (D² - d²) / 4D, and the power (P) was calculated as P = 100 / f(in cm) diopters. |
| 10 | The mean focal length and power were determined from the three observations. |