The Beauties of Nature, and the Wonders of the World We Live InLubbock, John, Sir
Philosophy
The Beauties of Nature, and the Wonders of the World We Live In
Lubbock, John, Sir
Astronomy; Natural history; Physical geography
The Moon, being so much smaller than the earth, cooled, of course, much
more rapidly, and it is probable that these mountains are millions of
years old--much older than many of our mountain chains. Yet no one can
look at a map of the Moon without being struck with the very rugged
character of its mountain scenery. This is mainly due to the absence of
air and water. To these two mighty agencies, not merely "the
cloud-capped towers, the gorgeous palaces, the solemn temples," but the
very mountains themselves, are inevitable victims. Not merely storms and
hurricanes, but every gentle shower, every fall of snow, tends to soften
our scenery and lower the mountain peaks. These agencies are absent from
the Moon, and the mountains stand to-day just as they were formed
millions of years ago.
But though we find on our own globe (see, for instance, Fig. 21)
volcanic regions closely resembling those of the Moon, there are other
phenomena on the Moon's surface for which our earth presents as yet no
explanation. From Tycho, for instance, a crater 17,000 feet high and 50
miles across, a number of rays or streaks diverge, which for hundreds,
or in some cases two or three thousand, miles pass straight across
plains, craters, and mountains. The true nature of these streaks is not
yet understood.
THE SUN
The Sun is more than 400 times as distant as the Moon; a mighty glowing
globe, infinitely hotter than any earthly fiery furnace, 300,000 times
as heavy, and 1,000,000 times as large as the earth. Its diameter is
865,000 miles, and it revolves on its axis in between 25 and 26 days.
Its distance is 92,500,000 miles. And yet it is only a star, and by no
means one of the first magnitude.
The surface of the Sun is the seat of violent storms and tempests. From
it gigantic flames, consisting mainly of hydrogen, flicker and leap.
Professor Young describes one as being, when first observed, 40,000
miles high. Suddenly it became very brilliant, and in half an hour
sprang up 40,000 more. For another hour it soared higher and higher,
reaching finally an elevation of no less than 350,000 miles, after which
it slowly faded away, and in a couple of hours had entirely disappeared.
This was no doubt an exceptional case, but a height of 100,000 miles is
not unusual, and the velocity frequently reaches 100 miles in a second.
The proverbial spots on the Sun in many respects resemble the
appearances which would be presented if a comparatively dark central
mass was here and there exposed by apertures through the more brilliant
outer gases, but their true nature is still a matter of discussion.
During total eclipses it is seen that the Sun is surrounded by a
"corona," or aureola of light, consisting of radiant filaments, beams,
and sheets of light, which radiate in all directions, and the true
nature of which is still doubtful.
Public-domain text, read in full here on John Shaqi.
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