The Trouvelot astronomical drawings manualTrouvelot, E. L. (Etienne Leopold)
Science
The Trouvelot astronomical drawings manual
Trouvelot, E. L. (Etienne Leopold)
Astronomy -- Pictorial works
the shadow had already crossed about ¾ of the disk, it was still
preceded by the secondary, or mock shadow, as it may be called; the same
relative distance having been kept all the while between the two
objects, which had therefore traveled at the same rate. It is obvious
that this dark spot could not be one of the planet's markings, since the
shadow of the first satellite moves more quickly on the surface of
Jupiter than a spot on the same surface travels by the effect of
rotation, so that in this case the shadow would soon have passed over
this marking, and left it behind, during the time occupied by the
observation. From these observations it seems very probable that Jupiter
has a nucleus, either solid or liquid, which lies several thousand
mites below the surface of its cloudy envelope. It is also probable that
the uniformly shaded dark segment seen in 1876, was a portion of the
surface of this nucleus itself. When the cloudy envelope is
semi-transparent at the place situated on a line with an occulted
satellite and the eye of an observer, this satellite may accordingly
remain visible for a time through the limb, as shown by observation. The
phenomenon of the mock shadow may also be attributed to a similar cause,
where semi-transparent vapors receive the shadow of a satellite at their
surface, while at the same time part of this shadow, passing through the
semi-transparent vapors, may be seen at the surface of the nucleus, or
of a layer of opaque clouds situated at some distance below the surface.
Some astronomers are inclined to think that Jupiter is at a high
temperature, and self-luminous to a certain extent. If this planet is
self-luminous to any degree, we might expect that some light would be
thrown upon the satellites when they are crossing the shadow cast into
space by the planet; but when they cross this shadow they are totally
invisible in the best telescopes, a proof that they do not receive much
light from the non-illuminated side of Jupiter. It would, indeed, seem
probable that some of the intensely white spots occasionally seen on the
equatorial belt of the planet are self-luminous in a degree, yet not
enough to render the satellites visible while they are immersed in
Jupiter's shadow. It does not seem impossible that the planet should
have the high temperature attributed to it, when we remember the
terrific storms observed in its atmosphere, which, owing to the great
distance of Jupiter from the Sun, do not seem to be attributable to this
body, but rather to some local cause within the envelope of the planet.
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