The Mathematical Monthly 1

Cover The Mathematical Monthly 1
The Mathematical Monthly 1
Runkle, John D. (John Daniel), 1822-1902
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17 gives the outlines of the envelope first seen on Oct 15th.
Fig. 18 shows it at a more advanced stage, three days later.
Fig. 17. Fig. la A change, in the relative proportion of light distributed on the two sides of the principal axis of the comet, had been progressing up to about the 6th of October. At this date, although there may still have been a little more light on the right hand side, the difference was not nearly so large as it had been. The diameter of the nucleus was then 800 miles.
... On the 8th, ite diameter was 1100 miles. The envelopes were most distinct on the left hand, or preceding side.
The change was a permanent one, and for the future this became the brightest half of the head of the comet It is curious to observe a corresponding change in the inclination of the envelopes to the axis. They now inclined even more decidedly to the left hand than they had at first done to the opposite side. The two last, those of Oct 15th and 20th, seem in fact in the first instance to have issued as luminous jets or streams from the side, rather than from the — 104 — vertex of the nucleus.


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