The story of the sun, moon, and starsGiberne, Agnes
Science
The story of the sun, moon, and stars
Giberne, Agnes
Astronomy -- Juvenile literature
This dark, transparent ring, described sometimes as dusky, sometimes as
richly purple, rises upwards to a height or breadth of nine thousand
miles. Closely following it is a ring more brilliant than Saturn
himself, over eighteen thousand miles in breadth. When astronomers talk
of the “breadth” of these rings, it must be understood that they mean
the width of the band measured _upwards_, in a direction away from the
planet.
Beyond the broad, bright ring is a gap of about one thousand seven
hundred miles. Then follows the third ring, ten thousand miles in
breadth; its outermost edge being at a height of more than forty-eight
thousand miles from Saturn. The color of the third ring is grayish,
much like the gray markings often seen on Saturn.
What would not be our admiration, our astonishment, our stupor perhaps,
if it were granted us to be transported there alive, and, among all
these extra-terrestrial spectacles, to contemplate the strange aspect
of the rings, which stretch across the sky like a bridge suspended
in the heights of the firmament! Suppose we lived on the Saturnian
equator itself, these rings would appear to us as a thin line drawn
across the sky above our heads, and passing exactly through the zenith,
rising from the east and increasing in width, then descending to the
west and diminishing according to perspective. Only there have we
the rings precisely in the zenith. The traveler who journeys from
the equator towards either pole leaves the plane of the rings, and
these sink imperceptibly, at the same time that the two extremities
cease to appear diametrically opposite, and by degrees approach each
other. What an amazing effect would be produced by this gigantic
arch, which springs from the horizon and spans the sky! The celestial
arch diminishes in height as we approach the pole. When we reach the
sixty-third degree of latitude the summit of the arch has descended to
the level of our horizon and the marvelous system disappears from the
sky; so that the inhabitants of those regions know nothing of it, and
find themselves in a less favorable position to study their own world
than we, who are nearly 800,000,000 miles distant.
During one-half of the Saturnian year the rings afford an admirable
moonlight on one hemisphere of the planet, and during the other half
they illuminate the other hemisphere; but there is always a half-year
without “ringlight,” since the sun illuminates but one face at a time.
Notwithstanding their volume and number, the satellites do not give
as much nocturnal light as might be supposed; for they receive, on an
equal surface, only the ninetieth part of the solar light which our
moon receives. All the Saturnian satellites which can be at the same
time above the horizon and as near as possible to the full phase do not
afford more than the hundredth part of our lunar light. But the result
may be nearly the same, for the optic nerve of the Saturnians may be
ninety times more sensitive than ours.
Public-domain text, read in full here on John Shaqi.
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