Physics · Ch 9 — Optics
Optical instruments
Optical instruments
Whether an object 'looks big' has nothing to do with its actual size alone -- a huge, distant mountain can appear smaller than a nearby small tree, because APPARENT size depends on the VISUAL ANGLE the object subtends at the eye, and this visual angle shrinks steadily with increasing distance. To make something look bigger, we must either physically bring it closer, or use an optical instrument that increases the visual angle without actually moving the object at all -- this increase is called ANGULAR MAGNIFICATION, or MAGNIFYING POWER. The unaided human eye, however, cannot focus clearly on anything closer than the LEAST DISTANCE OF DISTINCT VISION, cm for a normal eye; trying to bring an object closer than , or trying to resolve something too small even when held at , both fail without optical help -- which is precisely why a microscope (for small nearby objects) or a telescope (for objects too distant to ever be brought closer at all) becomes necessary.
Magnifying power is formally defined as the ratio of the visual angle subtended by the image formed by the optical instrument, to the visual angle that the SAME object would subtend if it were instead placed at the least distance of distinct vision (for telescopes specifically, is instead the angle the object subtends from its own actual position, since a star or planet can never physically be brought any closer).
SIMPLE MICROSCOPE (reading glass): a single convex lens, used with the object placed WITHIN its focal length, so that it forms an erect, virtual, magnified image. Since for small angles the angle itself, (numerically). For MAXIMUM magnifying power the image should be brought as close as the eye can still focus on, i.e. ; substituting this into gives . For MINIMUM magnifying power the image instead forms at infinity (object exactly at the focus, numerically), giving . So a lens of focal length provides angular magnification somewhere between and only; for the standard cm and, say, cm, this gives and -- the image looks only 5 to 6 times bigger, even though the corresponding LINEAR (lateral) magnification can in principle be made arbitrarily large (even effectively infinite, as at ).
Worked illustration: a 10 cm focal length magnifying glass views letters 0.5 mm thick, held 8 cm from the lens. cm; , so the image is mm and the letters appear about 3.125 times bigger. Held instead at only 5 cm (closer than the 10 cm focal length): solving gives cm, which is CLOSER than the eye's least distance of distinct vision (25 cm), so the resulting (magnified) image cannot actually be brought into clear focus by a normal eye -- the letters cannot be comfortably read from 5 cm.
COMPOUND MICROSCOPE: since a simple microscope's power can only be raised by shrinking , and a very small makes the lens thick (worsening both spherical and chromatic aberration), still higher magnifying power instead uses TWO convex lenses mounted in a tube -- a small-aperture OBJECTIVE facing the tiny object, and a somewhat larger EYE LENS the observer actually looks through. The object is placed between and of the objective, which forms a real, inverted, magnified intermediate image positioned just inside the focus of the eye lens; the eye lens then acts on this intermediate image exactly as a simple microscope would, producing a final virtual, further-magnified image (inverted relative to the original object). The overall magnifying power is the PRODUCT , where is the objective's ordinary LINEAR magnification and is the eye lens's own ANGULAR magnifying power (behaving as a simple microscope on the intermediate image); the microscope's overall length is . Raising (by pushing closer to the objective's focus) simultaneously increases , and hence -- so can only be pushed so far before the instrument becomes impractically long. The eye lens's own similarly ranges between (final image at infinity) and (final image at ).
Worked illustration: eye lens cm, objective cm, overall microscope length 15 cm, with the final image at its biggest (i.e. at cm, so cm). From cm; then cm; from cm; the overall magnifying power is . …
What this figure shows. Part (a): an object AB (drawn as a short vertical arrow) positioned at the least distance of distinct vision D=25 cm from an unaided eye; two lines are drawn from the top and bottom of the object converging at the eye's position, and the angle between these two lines at the eye is labelled alpha -- captioned as the greatest possible visual angle the object can subtend without any optical aid, since the eye cannot focus on anything brought closer than D. Part (b): the same object AB now placed WITHIN the focal length of a convex lens held in front of the eye; the lens is shown forming an erect, virtual, magnified image A'B' farther away (beyond D) along the same side as the object; two lines are drawn from the top and bottom of this larger image A'B' converging at the eye's position (looking through the lens), and the angle between them at the eye is labelled beta, shown visibly LARGER than alpha in part (a) -- illustrating that although the viewer is now looking at something farth …
Worked out. A magnifying glass of focal length 10 cm is used to view letters of thickness 0.5 mm held 8 cm from the lens. Using 1/f=1/v-1/u with u=-8 cm gives v=-40 cm, and the angular magnification M=D/|u|=25/8=3.125, so the letters appear 3.125 times bigger and the image size is 3.125x0.5=1.5625 mm. If instead the letters are held only 5 cm from the lens (closer than the 10 cm focal length), solving the lens formula gives an image at v=-10 cm -- since this virtual image distance (10 cm) is CLOSER than the eye's least distance of distinct vision (25 cm), a normal unaided eye cannot bring it into clear focus, so the letters CANNOT be read comfortably when held 5 cm from the lens, even though a (blurred) magnified i …
What this figure shows. A compound microscope drawn as two convex lenses mounted coaxially at the two ends of a cylindrical tube: a small-aperture OBJECTIVE lens (focal length fo) nearer the tiny object AB, and a somewhat larger EYE LENS (focal length fe) nearer the observer's eye. The object AB (drawn as a short vertical arrow) is positioned between fo and 2fo of the objective; rays from AB refracted by the objective are traced converging to form a real, inverted, magnified intermediate image A'B' (drawn as a larger, flipped vertical arrow) at distance vo from the objective, positioned so that A'B' falls just WITHIN the focal length of the eye lens. The eye lens then acts on A'B' as a simple magnifier, and rays from A'B' refracted by the eye lens are traced (extended backward as dashed lines on the object side) to form a further virtual, magnified final image A''B'' (drawn even larger, inverted relative to the original AB) at the observer's near point; the overall tube length L (=vo+ue, the distance between the two le …
Worked out. A pocket compound microscope has an eye lens of focal length 6.25 cm and an objective of focal length 2 cm; at a microscope (tube) length of 15 cm, the final image appears biggest (i.e. the final image is at the near point D=25 cm, giving maximum eye-lens magnifying power). Using 1/fe=1/ve-1/ue with ve=-25 cm and fe=6.25 cm gives ue=-5 cm; since L=vo+|ue|, vo=15-5=10 cm; then using 1/fo=1/vo-1/uo with vo=10 cm and fo=2 cm gives uo=-2.5 cm, so the object must be placed 2.5 cm from the objective. The overall magnifying power M=mo x Me = (vo/uo) x (D/ue) = (10/2.5) x (25/5) = …
What this figure shows. An astronomical telescope drawn as two convex lenses mounted coaxially at the two ends of a tube: a large-aperture OBJECTIVE lens of focal length fo at the far (sky-facing) end, and a smaller EYE LENS of focal length fe at the near (eye) end. A bundle of parallel incident rays from a distant object, inclined at a small angle alpha to the principal axis (representing a star/planet too far away to be brought closer), enters the objective and is traced converging to a real, inverted intermediate image AB formed exactly at the objective's focal point, a distance fo from the objective. Since the telescope is under NORMAL adjustment, the eye lens is positioned so this intermediate image AB also falls exactly at ITS OWN focal point (distance fe from the eye lens, on the other side); rays from AB refracted by the eye lens are traced emerging as a second bundle of PARALLEL rays (final image also at infinity), but now inclined at a visibly LARGER angle beta to the principal axis than the origin …
Worked out. An astronomical telescope has an objective of focal length 1 m; under normal adjustment, the total length of the telescope (separation between the two lenses) is 1.05 m. Since for normal adjustment L=fo+fe, solving 1.05=1+fe gives fe=0.05 m=5 cm as the eyepiece's focal length. The magnifying power under normal adjustment is then M=fo/fe=1/0.05=20. …