Side-Lights on Astronomy and Kindred Fields of Popular ScienceNewcomb, Simon
Science
Side-Lights on Astronomy and Kindred Fields of Popular Science
Newcomb, Simon
Astronomy; Compass; Flying-machines; Hyperspace; Learning and scholarship; Rain-making
For the moon, Pierce's tables have been employed up to the year 1882
inclusive. Commencing with the ephemeris for the year 1883, Hansen's
tables are introduced with corrections to the mean longitude founded on
two centuries of observation.
With so great a lack of uniformity, and in the absence of any existing
tables which have any other element of unity than that of being the
work of the same authors, it is extremely desirable that we should be
able to compute astronomical ephemerides from a single uniform and
consistent set of astronomical data. I hope, in the course of years, to
render this possible.
When our ephemeris was first commenced, the corrections applied to
existing tables rendered it more accurate than any other. Since that
time, the introduction into foreign ephemerides of the improved tables
of Le Verrier have rendered them, on the whole, rather more accurate
than our own. In one direction, however, our ephemeris will hereafter
be far ahead of all others. I mean in its positions of the fixed stars.
This portion of it is of particular importance to us, owing to the
extent to which our government is engaged in the determination of
positions on this continent, and especially in our western territories.
Although the places of the stars are determined far more easily than
those of the planets, the discussion of star positions has been in
almost as backward a state as planetary positions. The errors of old
observers have crept in and been continued through two generations of
astronomers. A systematic attempt has been made to correct the places
of the stars for all systematic errors of this kind, and the work of
preparing a catalogue of stars which shall be completely adapted to the
determination of time and longitude, both in the fixed observatory and
in the field, is now approaching completion. The catalogue cannot be
sufficiently complete to give places of the stars for determining the
latitude by the zenith telescope, because for such a purpose a much
greater number of stars is necessary than can be incorporated in the
ephemeris.
Public-domain text, read in full here on John Shaqi.
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