The Trouvelot astronomical drawings manualTrouvelot, E. L. (Etienne Leopold)
Science
The Trouvelot astronomical drawings manual
Trouvelot, E. L. (Etienne Leopold)
Astronomy -- Pictorial works
In periods of calm, very few changes are noticeable in the markings of
the planet, except, perhaps, some slight modifications of form in the
cloudy, equatorial belt which, in general, is much more liable to
changes than the other belts. But the Jovian surface is not always so
tranquil, great changes being observed during the terrific storms which
sometimes occur on this mighty planet, when all becomes disorder and
confusion on its usually calm surface; and nothing on the Earth can give
us a conception of the velocity with which some of its clouds and spots
are animated. New belts quickly form, while old ones disappear. The
usual parallelism of the belts no more exists. Huge, white, cumulus-like
masses advance and spread out, the rosy equatorial belt enlarges
sometimes to two or three times its usual size, and occupies two-thirds,
or more, of the disk, the rosy tint spreading out in a very short time.
At times very dark bands extending across the disk are transformed into
knots or dark spots, which encircle the planet with a belt, as it were,
of jet black beads. Sometimes, also, a secondary but narrower rosy belt
forms either in the northern or the southern hemisphere, and remains
visible for a few days or for years at a time.
On May 25, 1876, I witnessed one of the grandest commotions which can be
conceived as taking place in an atmosphere. All the southern hemisphere
of Jupiter, from equator to pole, was in rapid motion, the belts and
spots being transported entirely across the disk, from the eastern to
the western limb, in one hour's time, during which the equatorial belt
swelled to twice its original breadth, towards the south.
Now, when one stops for a moment to think what is signified by that
motion of the dark spots across the little telescopic disk of Jupiter in
an hour's time, he may arrive at some conception of the magnitude of the
Jovian storms, compared with those of our globe. The circumference of
Jupiter's equator, as stated above, is 276,460 miles; half this number,
or 138,230 miles, represents the length of the equatorial line seen from
the Earth. Now, after taking into account the rotation of the planet,
which somewhat diminishes the apparent motion, we arrive at the
astonishing result that the spots and markings were carried along by
this Jovian storm, at the enormous rate of 110,584 miles an hour, or
over 30.7 miles a second. On our globe, a hurricane or tornado, which
blows at the rate of 100 miles an hour, sweeps everything before it.
What, then, must be expected from a velocity over 1,105 times as great?
Enormous as this motion may appear, its occurrence cannot be doubted,
since it is disclosed by direct observation.
The surface of Jupiter, it would seem, has its periods of calm and
activity like that of the Sun, although it is not yet known, as it is
for the latter, that they recur with approximate regularity.
Public-domain text, read in full here on John Shaqi.
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