Astronomical Curiosities: Facts and FallaciesGore, J. Ellard (John Ellard)
Science
Astronomical Curiosities: Facts and Fallacies
Gore, J. Ellard (John Ellard)
Astronomy -- Miscellanea; Solar system -- Miscellanea
"Among the innumerable stars of all magnitudes, from the ninth
downwards, which at various times were seen through it, and some
extremely near to the nucleus (though not _exactly on it_) there never
appeared the least ground for presuming any extinction of their light
in traversing it. Very minute stars indeed, on entering its brightest
portions, were obliterated, as they would have been by an equal
illumination of the field of view; but stars which before their entry
appeared bright enough to bear that degree of illumination, were in no
case, so far as I could judge, affected to a greater extent than they
would have been by so much lamp-light artificially introduced."[207]
It is computed by Prof. J. Holetschak that, early in October, 1909,
Halley's comet should have the brightness of a star of about 14½
magnitude.[208] It should then--if not detected before--be discoverable
with some of the large telescopes now available.
According to the computations of Messrs. Cowell and Crommelin, the comet
should enter Pisces from Aries in January, 1910. "Travelling westward
towards the star γ Piscium until the beginning of May, and then turning
eastward again, it will travel back through the constellations Cetus,
Orion, Monoceros, Hydra, and Sextans." From this it seems that observers
in the southern hemisphere will have a better view of the comet than those
in northern latitudes. The computed brightness varies from 1 on January 2,
1910, to 1112 on May 10. But the actual brightness of a comet does not
always agree with theory. It is sometimes brighter than calculation would
indicate.
According to Prof. O. C. Wendell, Halley's comet will, on May 12, 1910,
approach the earth's orbit within 4·6 millions of miles; and he thinks
that possibly the earth may "encounter some meteors," which are presumably
connected with the comet. He has computed the "radiant point" of these
meteors (that is, the point from which they appear to come), and finds its
position to be R.A. 22{h} 42{m}·9, Decl. N. 1° 18'. This point lies a
little south-west of the star β Piscium.
Public-domain text, read in full here on John Shaqi.
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