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Ecliptic is the motion of the Sun across the sky.
The ecliptic is the apparent path the Sun traces out along the sky - independent of Earth's rotation - in the course of the year. More accurately, it is the intersection of the celestial sphere with the ecliptic plane, which is the geometric plane containing the mean orbit of the Earth around the Sun. It should be distinguished from the invariable ecliptic plane, which is the vector sum of the angular momenta of all planetary orbital planes, to which Jupiter is the main contributor. The name ecliptic is derived from being the place where eclipses occur.
Ecliptic and equator.
As the rotation axis of the Earth is not perpendicular to its orbital plane, the equatorial plane is not parallel to the ecliptic plane, but makes an angle of about 23º27' which is known as the obliquity of the ecliptic. The intersections of the equatorial and ecliptic plane with the celestial dome are great circles known as the celestial equator and the ecliptic. The intersection line of the two planes results in two diametrically opposite intersection points, known as the equinoxes. The equinox which the Sun passes from south to north is known as the vernal equinox or first point of Aries. Ecliptic longitude, usually indicated with the letter ?, is measured from this point on 0º to 360º towards the east. Ecliptic latitude, usually indicated with the letter ß is measured +90º to the north or -90º to the south. The same intersection point also defines the origin of the equatorial coordinate system, named Right ascension measured from 0 to 24 hours also to the east and usually indicated with a or R.A., and Declination, usually indicated with d also measured +90º to the north or -90º to the south. Simple rotation formulas allow a conversion from a,d to ?,ß and back (see: ecliptic coordinate system).
Ecliptic and stars.
The ecliptic serves as the center of a region called the Zodiac which constitutes a band of 9º on either side. Traditionally, this region is divided into 12 signs of 30º longitude each. By tradition, these signs are named after 12 of the 13 Constellations straddling the ecliptic. The zodiac signs are very important to many astrologers. Modern Astronomers typically use other coordinate systems today (see below).
The position of the vernal equinox is not fixed among the stars but due to the lunisolar precession slowly shifting westwards over the ecliptic with a speed of 1º per 72 years. A much smaller north/southwards shift can also be discerned, (the planetary precession, along the instantaneous equator, which results in a rotation of the ecliptic plane). Said otherwise the stars shift eastwards (increase their longitude) measured with respect to the equinoxes (in other words, as measured in ecliptic coordinates and (often) also in equatorial coordinates.
Using the current official IAU constellation boundaries - and taking into account the variable precession speed and the rotation of the ecliptic - the equinoxes shift through the constellations in the Astronomical Julian calendar years (in which the year 0 = 1 BC, -1 = 2 BC, etc.) as follows:
Ecliptic and Sun.
Due to perturbations to the Earth's orbit by the other planets, the true Sun is not always exactly on the ecliptic, but may be some arcseconds north or south of it. It is therefore the centre of the mean Sun which outlines its path. As the Earth revolves in one year around the Sun, it appears that the Sun also needs one year to pass the whole ecliptic. With slightly more than 365 days in the year, the Sun moves almost 1º eastwards every day (direction of increasing longitude). This annual motion should not be confused with the daily motion of the Sun (and the stars, the whole celestial sphere for that matter) towards the west in 24 hours and along the equator. In fact where the stars need about 23h56m for one such rotation to complete, the Sidereal day, the Sun, which has shifted 1º eastwards during that time needs 4 minutes extra to complete its circle, making the solar day just 24 hours.
The mean Sun crosses the equator around 21 March in the vernal equinox, its declination, right ascension, and ecliptic longitude are all zero then (the ecliptic latitude is always). The March equinox marks the onset of spring in the northern hemisphere and autumn in the southern. As such the term "spring equinox" should be avoided. The actual date and time varies from year to year because of the occurrence of leap years. It also shifts slowly over the centuries due to imperfections in the Gregorian calendar.
Ecliptic longitude 90º, at right ascension 6 hours and a northern declination equal to the obliquity of the ecliptic (23.44º), is reached around 22 June. This is the June solstice or summer solstice in the northern hemipshere and winter solstice in the southern hemisphere. It is also the first point of Cancer and directly overhead on Earth on the tropic of Cancer so named because the Sun turns around in declination. Ecliptic longitude 180º, right ascension 12 hours is reached around 23 September and marks the second equinox or first point of Libra. Due to perturbations to the Earth orbit, the moment the real Sun passes the equator might be several minutes earlier or later. The southern most declination of the sun is reached at ecliptic longitude 270º, right ascension 18 hours at the first point of the sign of Capricorn around 22 December.
In any case it must be stressed that although these traditional signs (in western tropical astrology) have given their names to the solstices and equinoxes, in reality, (as from the list in the previous chapter) the cardinal points are currently situated in the constellations of Pisces, Taurus, Virgo and Sagittarius respectively.
Ecliptic and planets
Most planets go in orbits around the sun which are almost in the same plane as the Earth's orbital plane, differing by a few degrees at most. As such they always appear close to the ecliptic when seen in the sky. Mercury with an orbital inclination of 7º is an exception. Pluto, at 17º, was previously the exception until it was reclassified a Dwarf planet, but other bodies in the Solar System have even greater orbital incinations (e.g. Eris 44 degrees and Pallas 34 degrees).
The intersection line of the ecliptical plane and another planet's orbital plane is called the nodal line of that planet, and the nodal line's intersection points on the celestial sphere are the ascending node (where the planet crosses the ecliptic from south to north) and the diametrically opposite descending node. Only when an inferior planet passes through one of its nodes can a transit over the Sun take place.
Inclination and nodal lines, as almost all other orbital elements, change slowly over the centuries due to perturbations from the other planets.
Ecliptic and Moon.
The orbit of the Moon is inclined by about 5º on the ecliptic. Its nodal line is not fixed either, but regresses (moves towards the west) over a full circle every 18.6 years. This is the cause of nutation and lunar standstill. The moon crosses the ecliptic about twice per month. If this happens during New Moon a solar eclipse occurs, during full moon a lunar eclipse. This was the way the ancients could trace the ecliptic along the sky; they marked the places where eclipses could occur.
Ecliptic and star coordinates.
Up to the 17th century, starmaps and positions in star catalogues were always given in ecliptical coordinates. It was not until astronomers started to use telescopes to measure star positions that equatorial coordinates came in use, and so exclusively that nowadays ecliptical coordinates are no longer used. This is not always desirable. A planetary conjunction for example would be much more illustratively described by ecliptic coordinates than equatorial.
Also see zodiacal coordinates.
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