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XV.

Cometary Statistics.

227

It not unfrequently happens that a comet is only discovered after its perihelion passage, when it will be receding from the the Sun, and perhaps also from the Earth. As under such circumstances its brightness will be day by day diminishing, its visibility may only extend to a few days, or a few weeks.

From an examination of a complete catalogue of calculated

Fig. 106.

ECLIPSE OF THE SUN OF MAY 17, 1882, SHOWING AN UNKNOWN COMET. (Ranyard.)

comets[1] we may obtain certain results which will here be analysed.

It appears that 492 comet apparitions have been subjected to mathematical investigation, viz.:—

Known periodical comets30
Subsequent returns108
Elliptic comets not yet verified, and parabolic comets341
Hyberbolic comets13
 492
  1. See the Catalogue in the Appendix (post), read as a continuation of Catalogue I. in my Handbook of Astronomy, 4th ed., vol. i, p. 511.
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