The Trouvelot astronomical drawings manualTrouvelot, E. L. (Etienne Leopold)
Science
The Trouvelot astronomical drawings manual
Trouvelot, E. L. (Etienne Leopold)
Astronomy -- Pictorial works
Although suspected in 1838, the dusky ring was not recognized before
1850, when G. P. Bond discovered it with the 15-inch refractor of the
Cambridge Observatory. It was also independently discovered the same
year in England by Dawes and Lassell. The dusky ring differs widely in
appearance and in constitution from the other rings, inasmuch as these
last are opaque, and either white or grayish, while the former is very
dark, and yet so transparent that the limb of the planet is plainly seen
through its substance. On particularly favorable occasions, the
appearance of this ring resembles that of the fine particles of dust
floating in a ray of light traversing a dark chamber. Whatever may be
the material of which this ring is composed, it must be quite rarefied,
especially towards its inner border, which appears as if composed of
distinct and minute particles of matter feebly reflecting the solar
light. That the inner part of the dusky ring is composed of separate
particles, is proved by the fact that the part of the ring which is seen
in front of the globe of Saturn has its inner border abruptly deflected
and curved inward on entering upon the disk, causing it to appear
considerably narrower than it must be in reality, a peculiarity which is
shown in the Plate. This phenomenon may be attributed to an effect of
irradiation, due to the strong light reflected by the central parts of
the ball, which so reduces the apparent diameter of the individual
particles that they become invisible to us, especially those near the
inner border, which are more scattered and less numerous than elsewhere.
The dusky ring, which was described by Bond, Lassell and other
astronomers as being equally transparent throughout all its width, has
not been found so by me in later years. The limb of the planet, seen by
these observers through the whole width of the dusky ring in 1850, could
not be traced through its outer half by myself in 1872 and 1874, and
this with the very same instrument used by Bond in his observations of
1848 and 1850. Moreover, I have plainly seen that its transparency was
not everywhere equal, but greatest on the inner border, from which it
gradually decreases, until it becomes opaque, as proved by the gradual
loss of distinctness of the limb, which vanishes at about the middle of
the dusky ring. These facts, which have been well ascertained, prove
that the particles composing this ring are not permanently located, and
are undergoing changes of relative position. It will be shown that the
surface of the other rings is also subject to changes, which are
sometimes very rapid.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account