- Equatorial ring
An Equatorial ring was an astronomical instrument used in the
Hellenistic world to determine the exact moment of the spring andautumn equinoxes . Equatorial rings were placed before the temples inAlexandria , inRhodes , and perhaps in other places, forcalendar purposes.The easiest way to understand the use of an equatorial ring is to imagine a ring placed vertically in the east-west plane at the Earth's
equator . At the time of the equinoxes, theSun will rise precisely in theeast , move across thezenith , and set precisely in thewest . Throughout the day, the bottom half of the ring will be in the shadow cast by the top half of the ring. On other days of the year, the Sun passes to thenorth orsouth of the ring, and will illuminate the bottom half. Forlatitudes away from the equator, the ring merely needs to be placed at the correct angle in the equatorial plane. At the Earth's poles, the ring would behorizontal .The equatorial ring was about one to two
cubits (45cm-90cm) in diameter. Because the Sun is not a point source of light, the width of the shadow on the bottom half of the ring is slightly less than the width of the ring. By waiting until the shadow was centered on the ring, the time of the equinox could be fixed to within an hour or so. If the equinox happened atnight , or if the sky wascloudy , an interpolation could be made between two days' measurements.The main disadvantage with the equatorial ring is that it needed to be aligned very precisely or false measurements could occur.
Ptolemy mentions in the "Almagest " that one of the equatorial rings in use in Alexandria had shifted slightly, which meant that the instrument showed the equinox occurring twice on the same day. False readings can also be produced byatmospheric refraction of the Sun when it is close to thehorizon .Equatorial rings can also be found on armillary spheres and equatorial
sundials .References
*Anton Pannekoek, (1989), "A History of Astronomy", page 124. Courier Dover Publications
*James Evans, (1998), "The History and Practice of Ancient Astronomy", pages 206-7. Oxford University Press.
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