34-5 Optical Instruments#

Prompts

  • What is the near point of the eye? Why can’t you see clearly when an object is closer than the near point?

  • How does a simple magnifying lens work? Where is the object placed? What is angular magnification \(m_\theta\)?

  • Describe a compound microscope: objective and eyepiece. How does the objective’s image become the eyepiece’s object? What contributes to the overall magnification?

  • Describe a refracting telescope. How does its lens arrangement differ from a microscope? Where do the focal points of the objective and eyepiece coincide?

  • State the formulas for angular magnification of (a) a simple magnifier, (b) a compound microscope, and (c) a refracting telescope.

Lecture Notes#

Overview#

  • Optical instruments extend the eye’s range: simple magnifier, compound microscope, refracting telescope.

  • The near point (~25 cm) is the closest distance at which the eye can focus sharply.

  • Angular magnification \(m_\theta\) compares the angle subtended by the image (with the instrument) to the angle subtended by the object at the near point (without it).

  • All three instruments use converging lenses; the microscope and telescope combine an objective and an eyepiece.


The near point and angular size#

The near point \(P_n\) is the closest distance at which the eye can form a sharp image on the retina. Closer objects appear blurry. A typical reference value is 25 cm.

The apparent size of an object depends on the angle \(\theta\) it subtends at the eye. At the near point, \(\theta \approx h/25\,\text{cm}\) for object height \(h\). Moving the object closer would increase \(\theta\) but blur the image.


The eye and corrective lenses#

  • Farsightedness (hyperopia): near point farther than 25 cm; need converging lenses to bring near objects into focus.

  • Nearsightedness (myopia): far point closer than infinity; need diverging lenses to bring distant objects into focus.

  • Corrective lens principle: Glasses create a virtual image at the person’s actual near/far point when viewing an object at the standard 25 cm / infinity.


Simple magnifying lens#

A converging lens placed between the object and the eye, with the object at or just inside the focal point, produces a virtual image far enough away for the eye to focus. The image subtends a larger angle \(\theta'\) than the object would at the near point.

Angular magnification (object at focal point):

(262)#\[ m_\theta = \frac{\theta'}{\theta} \approx \frac{25\,\text{cm}}{f} \]

where \(f\) is the focal length. Shorter \(f\) gives greater magnification.


Compound microscope#

A compound microscope has two lenses:

  • Objective (focal length \(f_{\text{ob}}\)): Object placed just outside its focal point; produces a real, inverted image \(I\).

  • Eyepiece (focal length \(f_{\text{ey}}\)): Image \(I\) is placed just inside its focal point; acts as a simple magnifier on \(I\), producing a virtual final image.

Tube length \(s\): distance from objective to image \(I\) (typically \(s \gg f_{\text{ob}}\)).

Lateral magnification of objective: \(m \approx -s/f_{\text{ob}}\).

Overall magnification:

(263)#\[ M = m \cdot m_\theta = -\frac{s}{f_{\text{ob}}} \cdot \frac{25\,\text{cm}}{f_{\text{ey}}} \]

The minus sign indicates the final image is inverted.


Refracting telescope#

A refracting telescope views distant objects:

  • Objective (\(f_{\text{ob}}\)): Parallel rays from a distant object form a real image \(I\) at its focal point.

  • Eyepiece (\(f_{\text{ey}}\)): The second focal point of the objective coincides with the first focal point of the eyepiece; image \(I\) lies there and acts as object for the eyepiece, which produces a virtual final image.

Note

Unlike the microscope, the telescope has no tube length between the focal points—they coincide. The telescope is designed for distant objects; the microscope for nearby ones.

Angular magnification:

(264)#\[ m_\theta = -\frac{f_{\text{ob}}}{f_{\text{ey}}} \]

Longer \(f_{\text{ob}}\) and shorter \(f_{\text{ey}}\) increase magnification. The minus sign indicates an inverted image.


Cameras and exposure#

  • Distant objects (\(s \gg f\)): \(s' \approx f\), \(m \approx -f/s\); magnification \(\propto f\).

  • f-number: \(f\)-number \(= f/D\); intensity \(I \propto D^2/f^2 = 1/(f\text{-number})^2\).

  • Exposure \(\propto I \cdot \Delta t_{\text{shutter}}\); zoom changes \(f\) and thus \(I\).


Design considerations#

Real instruments involve more than magnification:

  • Light-gathering power: Larger objective diameter \(\to\) brighter image (important for faint objects).

  • Resolving power: Ability to distinguish closely spaced objects; limited by diffraction.

  • Field of view: Angular extent of the scene.

  • Aberrations: Spherical aberration (non-sharp focus with spherical surfaces); chromatic aberration (different wavelengths focus at different points).


Summary#

  • Near point ~25 cm: closest sharp-focus distance.

  • Simple magnifier: \(m_\theta \approx 25\,\text{cm}/f\); object at focal point.

  • Compound microscope: \(M = -(s/f_{\text{ob}})(25\,\text{cm}/f_{\text{ey}})\); objective forms real image, eyepiece magnifies it.

  • Refracting telescope: \(m_\theta = -f_{\text{ob}}/f_{\text{ey}}\); objective and eyepiece focal points coincide.