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Q.What is the difference in the construction of an astronomical telescope and a compound microscope ? The focal lengths of the objective and eyepiece of a compound microscope are 1⋅251\cdot25 cm and 5⋅05\cdot0 cm, respectively. Find the position of the object relative to the objective in order to obtain an angular magnification of 30 when the final image is formed at the near point.

CBSECBSE Class XII Board 2020Subjective· 3mImportance★★★★★
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A compound microscope is designed to magnify tiny, nearby objects, while an astronomical telescope is built to magnify distant objects. For the given compound microscope, the object must be placed 1.5 cm from the objective lens.

The fundamental difference in the construction of an astronomical telescope and a compound microscope stems from their distinct purposes. Both instruments use two converging lenses: an objective lens and an eyepiece. However, the nature of the objects they view (nearby and tiny vs. distant and large) dictates the specific focal lengths and apertures of these lenses.

A compound microscope is designed to produce a highly magnified image of a very small object placed close to it. The objective lens, having a very short focal length, forms a real, inverted, and magnified intermediate image of the object. This intermediate image then acts as the object for the eyepiece, which functions like a simple magnifier, producing a final, virtual, and highly magnified image.

An astronomical telescope, on the other hand, is designed to view distant objects. Its primary goal is to gather as much light as possible from faint, distant sources and to produce an angularly magnified image. The objective lens, having a very long focal length and a large aperture, forms a real, inverted, and diminished intermediate image of the distant object at its focal plane. This intermediate image is then magnified by the eyepiece, which also has a short focal length.

Here is a summary of their key differences:

FeatureCompound MicroscopeAstronomical Telescope
PurposeTo magnify tiny, nearby objects.To magnify distant objects (e.g., stars, planets).
Objective LensShort focal length (fo≈f_o \approx mm to cm), small aperture.Long focal length (fo≈f_o \approx meters), large aperture.
Eyepiece LensShort focal length (fe≈f_e \approx cm).Short focal length (fe≈f_e \approx cm).
Intermediate ImageReal, inverted, magnified, formed inside the tube.Real, inverted, diminished, formed at the objective's focal plane.
Length of InstrumentRelatively short (L≈vo+ueL \approx v_o + u_e).Relatively long (L≈fo+feL \approx f_o + f_e for normal adjustment).

Now, let's determine the position of the object for the given compound microscope.

  1. Identify the given values and the goal.

    We are given:

    • Focal length of the objective, fo=1.25f_o = 1.25 cm
    • Focal length of the eyepiece, fe=5.0f_e = 5.0 cm
    • Total angular magnification, M=30M = 30
    • The final image is formed at the near point, D=25D = 25 cm (standard value for the least distance of distinct vision). We need to find the position of the object relative to the objective, which is the object distance for the objective, ∣uo∣|u_o|.
  2. Recall the formula for the total angular magnification of a compound microscope.

    The total angular magnification MM of a compound microscope is the product of the linear magnification of the objective (MoM_o) and the angular magnification of the eyepiece (MeM_e).

M=Mo×MeM = M_o \times M_e

When the final image is formed at the near point ($D$), the angular magnification of the eyepiece is given by:

Me=(1+Dfe)M_e = \left(1 + \frac{D}{f_e}\right)

The linear magnification of the objective is given by:

Mo=vo∣uo∣M_o = \frac{v_o}{|u_o|}

where $v_o$ is the image distance for the objective and $|u_o|$ is the object distance for the objective. …

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