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Constellations
THE CONSTELLATION NAMES and three-letter abbreviations below are as published by
the International Astronomical Union (IAU) in 1922 at its first-ever General
Assembly. (For a scan of the original published list, plus a discussion of how
the final choice came about, click here.) These names, along with the first official constellation boundaries, were enshrined in two IAU books authored by Eugène Delporte, Délimitation scientifique des constellations and Atlas Céleste, both published in 1930. These books by Delporte remain the definitive
references on the naming and delineation of the constellations.
Unfortunately, the IAU itself upset this happy consensus in 1932 when it agreed
a second list of names with alternative four-letter abbreviations. In this second list,
Corona Australis became “Corona Austrina”. In 1955 the IAU repealed these alternative four-letter abbreviations but
failed to correct the Corona Australis/Corona Austrina confusion. Corona
Austrina continued to appear in the constellation list given by the IAU on its
own website until 2008, as did the long-defunct constellation Argo, although
the rest of the astronomical community followed the Delporte books. These
anomalies have now been rectified (see
http://www.iau.org/public/constellations).
The constellation areas in the table below are those of A. E. Levin (Handbook of the British Astronomical Association, 1935; reprinted 1972). I have rounded
the areas in square degrees to one decimal place, and the percentages of sky
coverage to three decimal places. Levin gave separate areas for Serpens Caput
and Serpens Cauda, but here I have combined them into one.
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Visibility range (partial)*
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* NOTES ON COLUMN HEADINGS:
Visibility range (full) gives the range of latitudes from which each constellation rises fully above the
horizon at some time. Stars close to the horizon will be considerably dimmed by
atmospheric extinction.
Visibility range (partial) gives the latitudes from which the constellation only ever rises partly above
the horizon. Constellations which never rise more than a few degrees above the
horizon from a given latitude will be effectively unobservable.
Number of stars ≤6.5 gives the number of stars within the constellation of magnitude 6.5 and brighter
as listed in the Hipparcos Catalogue.
Origin:
1. Original Greek constellations listed by Ptolemy in the Almagest
2. Considered by the Greeks as part of Leo; made separate by Caspar Vopel in
1536, followed by Gerardus Mercator in 1551.
7. Part of the original Greek constellation Argo Navis, dismantled in the 18th
century by Nicolas Louis de Lacaille.
Who were Ptolemy, Keyser, de Houtman, Plancius, Hevelius and Lacaille? For more
on the origin of the constellations see Chapter One of Ian Ridpath’s Star Tales.
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