CHAPTER ONE concluded...
Filling the remaining gaps
As the accuracy of astronomical observations improved and fainter stars were
charted, the opportunities grew for innovators to introduce new constellations
even among the area of sky known to the ancient Greeks. Ten more constellations
were introduced later in the 17th century by the Polish astronomer Johannes
Hevelius (1611–87), filling the remaining gaps in the northern sky. They were listed in his
star catalogue dated 1687 and were depicted on his accompanying star atlas
called
span>Firmamentum Sobiescianum, both published posthumously in 1690. Oddly, Hevelius insisted on observing
with the naked eye even though telescopes were by then available; many of his
constellations were deliberately faint as though he was boasting of the power
of his eyesight. Of Hevelius’s inventions, seven are still accepted by astronomers (see Table 3). The rejected three were Cerberus, Mons Maenalus, and Triangulum Minus.
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Table 3: Seven constellations introduced by Johannes Hevelius in his star catalogue of 1687
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Although the northern constellations were now complete, there were still gaps in
the southern sky. These were filled by the French astronomer Nicolas Louis de
Lacaille (1713–62) who sailed to South Africa in 1750. There he set up a small observatory at
the Cape (not yet known as Cape Town) under the famous Table Mountain, which
impressed him so much that he later named a constellation after it, Mensa. At
the Cape from August 1751 to July 1752 Lacaille observed the positions of
nearly 10,000 stars, an astounding total in the short time.
On his return to France in 1754, Lacaille presented a map of the southern skies
to the French Royal Academy of Sciences which included 14 new constellations of
his own invention (see Table 4). An engraved version of the map was published in the Academy’s Mémoires in 1756 and Lacaille’s new constellations were rapidly accepted by other astronomers.
Whereas Keyser and de Houtman had mostly named their constellations after exotic
animals, Lacaille commemorated instruments of science and art, with the
exception of Mensa, named after the Table Mountain under which he had carried
out his observations. His full catalogue, and a revised map with the names of his new constellations in Latin, was published posthumously in 1763 under the
title Coelum Australe Stelliferum. In this catalogue, Lacaille divided up the unwieldy constellation Argo Navis,
the ship, into the subsections Carina, Puppis, and Vela that astronomers still
use as separate constellations. As well as creating 14 new constellations,
Lacaille eliminated a pre-existing one – Robur Carolinum, Charles’s Oak, introduced by the Englishman Edmond Halley in 1678 to honour King Charles
II.
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Table 4: Fourteen constellations introduced by Nicolas Louis de Lacaille in 1754
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All those from Lacaille’s time onwards who gerrymandered with the constellations did so without lasting
success, but there were plenty of astronomers who tried to leave their mark on
the sky. Constellation mania had reached its height by 1801 when the German
astronomer Johann Elert Bode (1747–1826) published his immense star atlas, Uranographia, containing over 100 different constellations; but by then astronomers realized
that things had gone too far, and during the ensuing century this number was
eroded by a process of natural wastage. In 1899 the American historian R. H.
Allen summed up the prevailing situation in his book Star Names and Their Meaning: “From 80 to 90 constellations may be considered as now more or less acknowledged”.
The final 88
One serious deficiency was that there were still no generally agreed boundaries
to the constellations. Since Bode’s time cartographers had drawn dotted lines snaking between constellation
figures, but these were arbitrary lines of demarcation that varied from atlas
to atlas. The matter was settled once and for all by astronomy’s governing body, the International Astronomical Union (IAU).
At its first General Assembly in 1922, the IAU officially adopted the list of 88
constellations, covering the entire sky, that we use today. (For more
information on all 88 constellations and how the final choice came to be made
see here.) On behalf of the IAU a Belgian astronomer, Eugène Delporte (1882–1955), then drew up a definitive list of boundaries for these 88 constellations.
For consistency with the earlier work of the American astronomer Benjamin
Apthorp Gould (1824–96) who in 1877 had published boundaries for the southern constellations in his
atlas called Uranometria Argentina, Delporte drew his boundaries along lines of right ascension and declination
for the year 1875. The boundaries zig-zagged to ensure that all named variable
stars remained within the constellations they were already assigned to.
Delporte also modified some of Gould's boundaries, particularly in places where
he had used diagonal lines.
Delporte’s work, approved by the IAU at its meeting in 1928 and published in 1930 in a
book called Délimitation Scientifique des Constellations, amounts to an international treaty on the demarcation of the sky, to which
astronomers throughout the world have conformed ever since. Constellations are
now regarded not as star patterns but as precisely defined areas of sky, rather
like countries on Earth. Unlike the map of the Earth, though, the map of the
sky is unlikely to change.
Official boundaries to the constellations were fixed in 1930 by a Belgian
astronomer, Eugène Delporte, acting on behalf of the International Astronomical Union. Here is
his chart for part of the northern sky, including Cassiopeia and Andromeda,
from Délimitation Scientifique des Constellations. The constellation boundaries follow
circles of right ascension (the equivalent of longitude in the sky) and
parallels of declination (the celestial equivalent of latitude). In this new
and more scientific depiction of the sky, the old constellation figures have
gone for good. (Author’s collection)