Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent AstronomersOlmsted, Denison
Science
Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent Astronomers
Olmsted, Denison
Astronomy
direct motion will therefore continue longer on the one side, and its
retrograde motion longer on the other side, than would be the case, were
it not for the motion of the earth. Mercury, whose greatest angular
distance from the sun is nearly twenty-nine degrees, is stationary at an
elongation of from fifteen to twenty degrees; and Venus, at about
twenty-nine degrees, although her greatest elongation is about
forty-seven degrees.
Mercury and Venus exhibit to the telescope _phases_ similar to those of
the moon. When on the side of their inferior conjunction, as from B to C
through D, Fig. 52, less than half their enlightened disk is turned
towards us, and they appear horned, like the moon in her first and last
quarters; and when on the side of the superior conjunction, as from C to
B through A, more than half the enlightened disk is turned towards us,
and they appear gibbous. At the moment of superior conjunction, the
whole enlightened orb of the planet is turned towards the earth, and the
appearance would be that of the full moon; but the planet is too near
the sun to be commonly visible.
[Illustration Fig. 52.]
We should at first thought expect, that each of these planets would be
largest and brightest near their inferior conjunction, being then so
much nearer to us than at other times; but we must recollect that, when
in this situation, only a small part of the enlightened disk is turned
toward us. Still, the period of greatest brilliancy cannot be when most
of the illuminated side is turned towards us, for then, being at the
superior conjunction, its light will be diminished, both by its great
distance, and by its being so near the sun as to be partially lost in
the twilight. Hence, when Venus is a little within her place of greatest
elongation, about forty degrees from the sun, although less than half
her disk is enlightened, yet, being comparatively near to us, and
shining at a considerable altitude after the evening or before the
morning twilight, she then appears in greatest splendor, and presents an
object admired for its beauty in all ages. Thus Milton,
"Fairest of stars, last in the train of night,
If better thou belong not to the dawn,
Sure pledge of day that crown'st the smiling morn
With thy bright circlet."
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