Example: The near point of a given eye is N=25cm. Treating the eye as it were a single thin lens a distance 2.5cm from retina. Find the focal length of the lens when it is focused on an object a) At the near point b) At infinity Simple Magnifier A simple magnifier consists of a single converging lens This device is used to increase the apparent size of an object The size of an image formed on the retina depends on the angle subtended by the eye The goal is simply to make the image on the retina larger.We want to put the image at the near point of the eye to make it as large on the retina as the eye can accommodate. The Size of a Magnified Image Image at infinity When an object is placed at the near point, the angle subtended is maximum The near point is about 25 cm When the object is placed just inside the focal point of a converging lens, the lens forms a virtual, upright, and enlarged image Image at near point We use converging lenses with f < N Angular Magnification Angular magnification is defined as Image at infinity Angle with lens h/ f N θ′ M= = = = θ Angle without lens h / N f The angular magnification is a maximum when the image formed by the lens is at the near point of the eye Therefore, . q = - 25 cm Calculated by 1 1 1 = + f d o di 1 1 1 = − do f di N N N = − do f di m N N M = − max f di Image at near point The closer an image is to the eye, the greater the magnification. Since the closest an image can be to the eye and still be in focus is the near point, N N N 25cm = +1 = 1 + M M== N − f − N f f do Magnification by a Lens With a single lens, it is possible to achieve angular magnification up to about 4 without serious aberrations With one or two additional lenses, which correct the aberrations, a magnification of up to about 20 can be achieved Example: A biologist with a near-point distance of N=26cm examines an insect wing through a magnifying glass whose focal length in f=4.3cm. Find angular magnification when the image produced by the magnifier is a) At infinity b) At the near point THE COMPOUND MICROSCOPE A compound microscope uses two lenses in combination – an objective and an eye piece (ocular) – to produce a magnified image The object to be viewed is placed just outside the focal lenght length of the objective lens We must supply light in order to illuminate the sample. Typically the light source must have heat absorbing filters in place so that the energy of the beam does not boil away the liquid-like biological sample. In advanced scopes, on may also use polarized light in order to see details that ordinary white light will not be able to resolve. Compound Microscope The lenses are separated by a distance L The approach to analyze the image formation is the same as for any two lenses in a row L is much greater than either focal length The image formed by the first lens becomes the object for the second lens The image seen by the eye, I2, is virtual, inverted and very much enlarged Compound Microscope A compound microscope consists of two lenses Gives greater magnification than a single lens The objective lens has a short focal length, ƒo<1 cm The ocular lens (eyepiece) has a focal length, ƒe of a few cm Magnifications of the Compound Microscope The lateral magnification of the objective is m =− The di di ≈− do f objectve angular magnification of the eyepiece of the microscope is M eyepiece = N f eyepiece Overall magnification The overall magnification of the microscope is the product of the individual magnifications M total = mobjective M eyepiece = − di N f objectve f eyepiece The magnifications quoted for microscopes assume a near-point distance of 25 cm Other Considerations with a Microscope The ability of an optical microscope to view an object depends on the size of the object relative to the wavelength of the light used to observe it (we will see this in the next chapter interference/diffraction) For example, you could not observe an atom (d ≈ 0.1 nm) with visible light (λ ≈ 500 nm) Telescopes Two fundamental types of telescopes Refracting telescope uses a combination of lenses to form an image (invented Galileo and by Kepler) Reflecting telescope uses a curved mirror and a lens to form an image (invented by Newton) Telescopes can be analyzed by considering them to be two optical elements in a row The image of the first element becomes the object of the second element Refracting Telescope The two lenses are arranged so that the objective forms a real, inverted image of a distance object The image is near the focal point of the eyepiece The two lenses are separated by the distance ƒobj + ƒeye which corresponds to the length of the tube The eyepiece forms an enlarged, inverted image of the first image Note: θ≈h’/fe and θ0 ≈h’/f0 Angular Magnification of a Telescope The angular magnification depends on the focal lengths of the objective and eyepiece θ ' hi / f e ƒo m= = = θ hi / f o ƒe Angular magnification is particularly important for observing “nearby” objects (sun, moon,…) Very distance objects still appear as a small point of light Disadvantages of Refracting Telescopes Large diameters are needed to study distant objects Large lenses are difficult and expensive to manufacture The weight of large lenses leads to sagging, which produces aberrations Reflecting Telescope Helps overcome some of the disadvantages of refracting telescopes Replaces the objective lens with a mirror The mirror is often parabolic to overcome spherical aberrations In addition, the light never passes through glass Except the eyepiece Reduced chromatic aberrations Reflecting Telescope, Newtonian Focus The incoming rays are reflected from the mirror and converge toward point A At A, a photographic plate or other detector could be placed A small flat mirror, M, reflects the light toward an opening in the side and passes into an eyepiece Examples of Telescopes Reflecting Telescopes Largest in the world are 10 m diameter Keck telescopes on Mauna Kea in Hawaii Largest single-mirrored telescope in US is the 5 m diameter instrument on Mount Palomar in California Refracting Telescopes Largest in the world is Yerkes Observatory in Wisconsin Has a 1 m diameter Hubble Telescope