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Astronomy Principles and Practice Fourth Edition.pdf

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Telescope resolving power 247<br />

Figure 16.7. Intensity scan through a diffraction pattern.<br />

Figure 16.8. The diffraction pattern in the focal plane of the objective.<br />

For a collector in the form of an objective lens, the resultant diffraction pattern produced from<br />

a point object appears as a spot at the centre of a system of concentric rings (see figure 16.6). The<br />

strength, or energy contained in each ring, decreases according to the number of the ring. However,<br />

after the third ring it is difficult to detect the presence of the outer rings. According to theory, 84% of the<br />

energy is concentrated into the central spot. As this type of diffraction pattern was first investigated by<br />

Airy, the central spot is sometimes referred to as the Airy disc. By making a scan along a line through<br />

the centre of the pattern, an intensity profile such as that illustrated in figure 16.7 can be obtained.<br />

The sizes of the diffraction rings are also predicted by theory. By defining α to be the angle<br />

subtended at the collector by the centre of the Airy disc <strong>and</strong> a point in the diffraction pattern (see<br />

figure 16.8), the positions for minima of intensity are given by<br />

sin α n = m nλ<br />

D<br />

where n is the number or order of the minimum, m is a numerical factor which is obtained by<br />

performing the integration of the interference from points over the telescope aperture, λ is the

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