Abstract
Among the small bodies of the Solar System, comets attract perhaps the most attention from amateur observers. In a good year perhaps fifteen to twenty comets may come within range of amateur telescopes, maybe a couple of which might even be sufficiently bright to be seen with the aid of 10 × 50 binoculars. Most are rather faint, and require skill and patience if they are to be observed. Certainly, few come to resemble the popular image, with a long tail streaming away from the head: the objects followed by regular, specialist comet observers are more usually faint, fuzzy patches with little or no obvious tail. Only rarely are we treated to spectacular objects like C/1996 B2 Hyakutake, which appeared in the spring of 1996, or C/1995 O1 Hale-Bopp, which reached naked-eye visibility a year later. The arrival of such bright objects is unpredictable, and they may be easily visible for only a few weeks.
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© 1999 Springer-Verlag London
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Bone, N. (1999). Comets. In: Observing Meteors, Comets, Supernovae and other Transient Phenomena. Practical Astronomy. Springer, London. https://doi.org/10.1007/978-1-4471-0579-4_8
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DOI: https://doi.org/10.1007/978-1-4471-0579-4_8
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