In geometric optics, the power of a lens is defined as the reciprocal of its: MCQ with Answer and Explanation

In geometric optics, the power of a lens is defined as the reciprocal of its:
A. Refractive index
B. Radius of curvature
C. Focal length in meters
D. Magnification
Answer: Option C
Solution (By JKSSB Mock Tests)
The power (P) of a lens indicates its converging or diverging ability. It is mathematically defined as the reciprocal of the focal length (f), provided the focal length is measured in meters. The formula is P = 1 / f(in meters). The SI unit of power for a lens is the Diopter (D). A focal length of 0.5m gives a power of 2D.

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Practice More Physics Questions

Question #1
A body at 100°C is placed in contact with a body at 0°C. Heat flow stops when
A. Both reach 0°C
B. Thermal equilibrium is reached
C. Both reach 100°C
D. Heat content becomes equal

Correct Answer: Option B


Explanation:
Heat flows until temperatures equal, i.e., thermal equilibrium. Not necessarily 50°C unless heat capacities equal.

This question belongs to: Science Physics
Question #2
Who among the following scientists first experimentally demonstrated the existence of electromagnetic waves, confirming Maxwell's theoretical predictions?
A. Thomas Edison
B. Guglielmo Marconi
C. Nikola Tesla
D. Heinrich Hertz

Correct Answer: Option D


Explanation:
While James Clerk Maxwell predicted electromagnetic waves mathematically, it was the German physicist Heinrich Hertz who successfully built the first spark-gap transmitter in 1887. He physically generated and detected radio waves in his laboratory, proving Maxwell's theories right. The SI unit of frequency, the Hertz (Hz), is named in his absolute honor.

This question belongs to: Science Physics
Question #3
The resolving power of an astronomical telescope can be significantly increased by:
A. Increasing the focal length of the objective lens.
B. Decreasing the focal length of the eyepiece.
C. Increasing the aperture (diameter) of the objective lens.
D. Using light of a longer wavelength.

Correct Answer: Option C


Explanation:
Resolving power is a telescope's ability to distinguish closely spaced objects (like double stars) as separate. It is proportional to D / lambda, where D is the diameter (aperture) of the objective lens and lambda is the wavelength of light. Increasing the aperture D directly and strictly increases the resolving power.

This question belongs to: Science Physics