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Astronomy Principles and Practice Fourth Edition.pdf

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Simple observations 35<br />

Figure 6.1. The h<strong>and</strong> as a means of estimating angles.<br />

the IAU convention, the names of constellations are usually referred to by a st<strong>and</strong>ardized three-letter<br />

abbreviation.<br />

6.2 Simple observations<br />

There are many aids to help provide information about what is available for view in the night sky at any<br />

particular time. Many PC software packages W6.1,W 6.2 offer active demonstrations of the behaviour of<br />

the night sky according to the observer’s location <strong>and</strong> the local time. These can be very informative<br />

as motions which, in reality, may take some months to execute can be simulated on the screen <strong>and</strong><br />

speeded up to take just a few seconds. Thus, for example, the apparent motions of the Moon <strong>and</strong> the<br />

complex planetary paths may be readily appreciated. It is a relatively easy matter to learn which stars<br />

are in the sky at a particular time <strong>and</strong> where the planets are relative to the stellar background. If a<br />

planetarium is available, constellation identification can be learned very quickly, especially if a pattern<br />

projector is attached for highlighting each constellation.<br />

Familiarity with the night sky, however, is best gained by spending a few hours on different nights<br />

observing the ‘real’ panorama. The true feeling of being under a hemispherical rotating dome with<br />

stars attached can only be obtained by outdoor activity. Appreciation of the angular scale associated<br />

with the well-known asterisms <strong>and</strong> identification of the constellation patterns is best gained by direct<br />

experience. On the early occasions, it is useful to be armed with a star atlas (such as Norton’s Star<br />

Atlas) or a simple planisphere. This latter device is a h<strong>and</strong>-held rotatable star map with a masking<br />

visor, allowing the correct part of the sky to be seen according to the season <strong>and</strong> the local time.<br />

In the previous chapters, reference has already been made to angular measure <strong>and</strong>, in the first<br />

place, it is useful to have an appreciation of angular scales as projected on the night sky. For example,<br />

the angular sizes of the Sun <strong>and</strong> Moon are approximately the same being ∼ 1 2 ◦ . If either the Sun or full<br />

Moon is seen close to the horizon it is readily appreciated that their apparent diameters would need to<br />

be extended 720 times to ‘fill’ the 360 ◦ of the full sweep around the horizon. Rough estimates of larger<br />

angles between stars, so providing the impression of just how large an area a particular constellation<br />

covers, can be made by using the ‘rule of thumb’ technique as practised by artists.<br />

If the arm is fully extended, different parts of the h<strong>and</strong> can be used to provide some simple<br />

angular values. Typical values are indicated in figure 6.1 but a system <strong>and</strong> scale should be developed<br />

individually by comparing observations with a star map. In the first place it will be noted that the<br />

angular extent of the thumb at arm’s length is about 1 ◦ . This means that if the Moon is in the sky it<br />

should be easily blocked from view by the use of the thumb. Figure 6.1 indicates that the knuckle-span

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