Scientific American Supplement, No. 633, February 18, 1888Various
Science
Scientific American Supplement, No. 633, February 18, 1888
Various
Science -- Periodicals
The comet's appearance was remarkable. Its tail, long and straight,
extended over an arc of 30 degrees, but there was no appreciable
condensation which could be called the comet's head. The long train of
light, described as nearly equal in brightness to the Magellanic clouds,
seemed to be simply cut off at that end where in most comets a nucleus
and coma are shown.
This comet has helped to throw light on one of the most perplexing
puzzles which those most perplexing of all the heavenly bodies, comets,
have presented to astronomers.
In the year 1668 a comet was seen in the southern skies which attracted
very little notice at the time, and would probably have been little
thought of since had not attention been directed to it by the appearance
and behavior of certain comets seen during the last half century.
Visible for about three weeks, and discovered after it had already
passed the point of its nearest approach to the sun, the comet of 1668
was not observed so satisfactorily that its orbit could be precisely
determined. In fact, two entirely different orbits would satisfy the
observations fairly, though one only could be regarded as satisfying
them well.
This orbit, however, was so remarkable that astronomers were led to
prefer the other, less satisfactory though it was, in explaining the
observed motions of the comet. For the orbit which best explained the
comet's movements carried the comet so close to the sun as actually to
graze his visible surface.
Moreover, there was this remarkable, and, indeed, absolutely unique
peculiarity about the orbit thus assigned: the comet (whose period of
revolution was to be measured by hundreds of years) actually passed
through the whole of that part of its course during which it was north
of our earth's orbit plane in less than two hours and a half! though
this part of its course is a half circuit around the sun, so far as
direction (not distance of travel) is concerned. That comet, when at its
nearest to the sun, was traveling at the rate of about 330 miles per
second. It passed through regions near the sun's surface commonly
supposed to be occupied by atmospheric matter.
Public-domain text, read in full here on John Shaqi.
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