Magnifiers, Microscopes and Telescopes
An optical instrument can use an objective to form an intermediate image and an eyepiece to enlarge its apparent angle. Microscope magnification combines linear and angular factors. Telescope magnification, field of view, light collection and resolution describe different properties.
What a learner can do afterwards
- Traces an object through a two-lens instrument and computes the overall magnification
- Distinguishes linear from angular magnification and says which matters for a distant object
- Explains why a large aperture helps a telescope in two separate ways
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Linear magnification compares image height with object height. Angular magnification compares viewing angles with and without an instrument. A converging lens with an object inside its focal length gives an upright, enlarged, virtual image. A magnifier lets you view an object closer than your unaided near point while keeping its image in focus. Near points vary; calculations here use the conventional reference distance D = 25 cm.
For a magnifier or eyepiece with its final image at infinity, the small-angle rule is M = D/f. The eye can then view with relaxed focusing. If the lens is close to the eye and the final image is at the near point, use M = 1 + D/f instead. State the viewing condition and use matching distance units. For D = 25 cm and f = 2.5 cm, infinity viewing gives M = 10.
Model a compound microscope with two converging lenses. The specimen sits just beyond the objective's focus. The objective forms a real, enlarged, inverted image well beyond that focus. This intermediate image becomes the eyepiece's object. Place it at the eyepiece's object-side focal plane for a final image at infinity, or inside that focal length for a finite virtual image. The eyepiece preserves the intermediate image's orientation.
The objective's linear factor is m_obj = -di_obj/do_obj. Multiply it by the eyepiece's angular factor: M_total = m_obj × M_eye. For m_obj = -12 and M_eye = 10, the product is -120. Its magnitude is the angular enlargement relative to viewing the specimen unaided at D. Its negative sign means inverted. Objective focal length alone does not determine objective magnification.
A telescope objective receives nearly parallel rays from a distant object and forms a real image at its focal plane. In a two-converging-lens telescope, align this plane with the eyepiece's object-side focal plane for a final image at infinity. Then M = -f_obj/f_eye in the small-angle model. Its magnitude is f_obj/f_eye; the minus sign means inverted. This compares the same distant object's viewing angles with and without the telescope.
For a fixed eyepiece apparent field, increasing magnification reduces the true field on the sky: approximately, true field = apparent field/|M|. A larger-looking image need not reveal finer detail. Magnification and resolution differ. A reflecting telescope uses a curved mirror, rather than a lens, to form the intermediate image. An eyepiece can then enlarge its apparent angle.
A larger clear aperture collects more light and permits finer diffraction-limited detail. For comparable unobstructed telescopes, collected light scales with diameter squared: doubling diameter gives four times the light. At the same wavelength, the diffraction-limited minimum angular separation scales as 1/diameter, so doubling diameter halves it. Atmospheric blur and optical defects can limit the actual gain.
Relative light collection: doubling clear diameter gives four times the collecting area.
Follow the intermediate image and state the viewing condition. Multiply microscope factors. Keep telescope magnification, field of view and resolution separate.
Lesson, questions and flashcards written for this dataset. OpenStax texts were consulted for physics facts; textbook passages are not reproduced.
Readings and flashcards written for this dataset, with OpenStax texts consulted for physics facts. Linked videos are identified as Khan Academy material in the source records; their licenses are unspecified.
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Keeping track of two stages
A microscope uses an intermediate image. Its objective forms a real, enlarged, inverted image of the specimen. The eyepiece then treats that image as its object. In the simplified two-converging-lens arrangement, placing the intermediate image at the eyepiece's object-side focal plane gives a final image at infinity. Suppose the objective's linear magnification is -16 and the eyepiece's angular magnification is 8. The total microscope factor is their product, -128. This is an angular comparison with unaided viewing of the specimen at the chosen reference near point. It is not the height ratio of two finite images. The negative sign records inversion. For a telescope viewing a distant object, the comparison is instead between that object's angles with and without the telescope. In the two-converging-lens infinity arrangement, objective and eyepiece focal lengths of 120 cm and 4 cm give a magnification magnitude of 30. A reflecting telescope replaces the lens objective with a curved mirror. It still forms an intermediate image that an eyepiece can view.
Two settings for one magnifier
Before calculating magnifier angular magnification, choose the comparison distance D and the final image position. D is the reference near-point distance for unaided viewing. Using D = 25 cm is a convention; actual near points differ. For a final image at infinity, place the object at the converging lens's focal plane. Rays leaving from each object point are parallel, and the small-angle formula is M = D/f. For a finite virtual image, place the object inside the focal length. If the lens is close to the eye and the virtual image is at the near point, the formula becomes M = 1 + D/f. For example, a 10 cm focal-length lens gives 2.5x in the infinity arrangement when D = 25 cm. Under the stated near-point conditions, it gives 3.5x. The lens has not changed; its viewing arrangement has. A microscope eyepiece uses these same principles on the objective's intermediate image. State the image position before choosing its magnification formula.
Choosing the unaided comparison
Light entering the eye is focused by the cornea and lens onto the retina. The retinal image is real and inverted. The eye changes its lens shape to focus objects at different distances; this adjustment is called accommodation. The near point is the closest distance at which the eye can focus clearly. It varies between people and can change with age. A stated reference of 25 cm lets an optics calculation compare magnifiers on the same basis without claiming that every eye has that near point. Moving an object closer increases the angle it occupies at the eye, but unaided focusing has a limit. A magnifier allows a closer object while presenting an image the eye can focus on. Its angular magnification is compared with unaided viewing of the object at the reference near point. A telescope uses a different reference: the same distant object viewed without the telescope. Its angular magnification does not require a near-point distance.
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