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
You may ask, why we do not observe this appearance every time one of the
inferior planets comes into inferior conjunction, for then, of course,
it passes between us and the sun. It must, indeed, at this time, cross
the meridian at the same time with the sun; but, because its orbit is
inclined to that of the sun, it may cross it (and generally does) a
little above or a little below the sun. It is only when the conjunction
takes place at or very near the point where the two orbits cross one
another, that is, near the _node_, that a transit can occur. Thus, if
the orbit of Mercury, N M R, Fig. 50, (page 231,) were in the same plane
with the earth's orbit, (and of course with the sun's apparent orbit,)
then, when the planet was at Q, in its inferior conjunction, the earth
being at E, it would always be projected on the sun's disk at Z, on the
concave sphere of the heavens, and a transit would happen at every
inferior conjunction. But now let us take hold of the point R, and lift
the circle which represents the orbit of Mercury upwards seven degrees,
letting it turn upon the diameter _d b_; then, we may easily see that a
spectator at E would project the planet higher in the heavens than the
sun; and such would always be the case, except when the conjunction
takes place at the node. Then the point of intersection of the two
orbits being in one and the same plane, both bodies would be referred to
the same point on the celestial sphere. As the sun, in his apparent
revolution around the earth every year, passes through every point in
the ecliptic, of course he must every year be at each of the points
where the orbit of Mercury or Venus crosses the ecliptic, that is, at
each of the nodes of one of these planets;[12] and as these nodes are on
opposite sides of the ecliptic, consequently, the sun will pass through
them at opposite seasons of the year, as in January and July, February
and August. Now, should Mercury or Venus happen to come between us and
the sun, just as the sun is passing one of the planet's nodes, a transit
would happen. Hence the transits of Mercury take place in May and
November, and those of Venus, in June and December.
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