On the Connexion of the Physical SciencesSomerville, Mary
Science
On the Connexion of the Physical Sciences
Somerville, Mary
Physical sciences; Science
Although the apparent diameters
of the satellites are too small to be measured, yet their perturbations
give the values of their masses with considerable accuracy—a striking
proof of the power of analysis.
A singular law obtains among the mean motions and mean longitudes of the
first three satellites. It appears from observation that the mean motion
of the first satellite, plus twice that of the third, is equal to three
times that of the second; and that the mean longitude of the first
satellite, minus three times that of the second, plus twice that of the
third, is always equal to two right angles. It is proved by theory,
that, if these relations had only been approximate when the satellites
were first launched into space, their mutual attractions would have
established and maintained them, notwithstanding the secular
inequalities to which they are liable. They extend to the synodic
motions (N. 92) of the satellites; consequently they affect their
eclipses, and have a very great influence on their whole theory. The
satellites move so nearly in the plane of Jupiter’s equator, which has a
very small inclination to his orbit, that the first three are eclipsed
at each revolution by the shadow of the planet, which is much larger
than the shadow of the moon: the fourth satellite is not eclipsed so
frequently as the others. The eclipses take place close to the disc of
Jupiter when he is near opposition (N. 93); but at times his shadow is
so projected with regard to the earth, that the third and fourth
satellites vanish and reappear on the same side of the disc (N. 94).
These eclipses are in all respects similar to those of the moon: but,
occasionally, the satellites eclipse Jupiter, sometimes passing like
obscure spots across his surface, resembling annular eclipses of the
sun, and sometimes like a bright spot traversing one of his dark belts.
Before opposition, the shadow of the satellite, like a round black spot,
precedes its passage over the disc of the planet; and, after opposition,
the shadow follows the satellite.
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.
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account