Resolving and collecting power of telescopes (AQA A-Level Physics): Flashcards

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Resolving and collecting power of telescopes
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Resolving power of telescope

Ability to distinguish between closely spaced objects

Min. angular resolution formula

θ≈λD\theta \approx \frac{\lambda}{D}

DD in formula θ≈λD\theta \approx \frac{\lambda}{D}

Diameter of objective (lens or mirror)

λ\lambda in formula θ≈λD\theta \approx \frac{\lambda}{D}

Wavelength of electromagnetic radiation

Rayleigh criterion for resolving two objects

Angular separation ≥λD\geq \frac{\lambda}{D}

Effect of larger DD on resolving power

Smaller θ\theta, better resolution (finer details)

Collecting power proportional to?

D2D^2 (square of objective diameter)

Doubling diameter effect on collecting power

Quadruples it (increases by factor of 4)

1 arcsecond in degrees

1/3600 of a degree

Airy disc

Diffraction pattern: bright central disc + concentric rings

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