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Astronomy Principles and Practice Fourth Edition.pdf

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Geocentric parallax 121<br />

Figure 10.6. The use of parallax on the terrestrial scale.<br />

Table 10.2. Measurement of distance by parallax.<br />

For a base-line one unit long<br />

Distance to be Order of size of Order of accuracy result<br />

measured (in units) parallactic angle 1 part in<br />

1 60 ◦ 200 000<br />

10 6 ◦ 20 000<br />

100 0·6 ◦ ∼ 30 ′ 2000<br />

1000 0·06 ◦ ∼ 3 ′ 200<br />

Figure 10.7. Geocentric <strong>and</strong> horizontal parallax.<br />

increasing distance, the length of the base-line remaining constant. Much of the trouble in the use of<br />

this surveying method to measure distances within the Solar System lies in the smallness of available<br />

base-lines with respect to the distances involved.<br />

Consider an observer at O (figure 10.7) on the surface of the Earth, centre C, the zenith being in

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