Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schoolsServiss, Garrett Putman
Science
Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schools
Serviss, Garrett Putman
Astronomy -- Juvenile literature
touching any island, and it was chosen for this very reason, because if
it ran over inhabited lands, like Europe or America, it would cause
endless confusion. Situated as it is, it causes no trouble except to sea
captains, and very little to them. If a ship crosses the line going
westward the captain jumps his log-book one day forward. If it is, for
instance, Wednesday noon, east of the line he calls it Thursday noon, as
soon as he has passed over. If he is going eastward he drops back a day
on crossing the line, as from Thursday noon to Wednesday noon. The
date-line theoretically follows the 180th meridian, but, in fact, in
order to avoid certain groups of islands, it bends about a little, while
keeping its general direction from north to south.
=9. The Seasons.= We now recall again what was said in Part I, about the
inclination of the ecliptic, or the apparent path of the sun in the
heavens, to the equator. Because of this inclination, the sun appears
half the year above the equator and the other half below it. When it is
above the equator for people living in the northern hemisphere, it is
below the equator for those living in the southern hemisphere, and _vice
versa_. This is because observers on opposite sides of the plane of the
equator look at it from opposite points of view. For the northern
observer the celestial equator appears south of the zenith; for the
southern observer it appears north of the zenith, its distance from the
zenith, in both cases, increasing with the observer's distance from the
equator of the earth. If he is on the earth's equator, the celestial
equator passes directly _through_ the zenith. For convenience we shall
suppose the observer to be somewhere in the northern hemisphere.
[Illustration:
=Head of the Great Comet of 1861=
From a drawing by Warren De La Rue.
]
[Illustration:
=Halley's Comet, May 5, 1910=
Photographed at the Yerkes Observatory by E E. Barnard, with the
ten-inch Bruce telescope.
This was shortly before the passage of the comet between the earth and
the sun, when some think its tail was thrown over us.
]
Public-domain text, read in full here on John Shaqi.
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