Orbital pole

An orbital pole is either point at the ends of an imaginary line segment that runs through the center of an orbit (of a revolving body like a planet) and is perpendicular to the orbital plane. Projected onto the celestial sphere, orbital poles are similar in concept to celestial poles, but are based on the body's orbit instead of its equator.

The north orbital poles of the Solar System planets all lie within Draco and Camelopardalis (5 Jupiter, 6 Saturn, 8 Neptune). The Sun's north pole (not shown) also lies within Draco, near the 2-3-4-7 cluster. 1 is Mercury's north orbital pole, 2 is Venus's, and so on. The north orbital pole of the dwarf planet Pluto would lie in Cepheus.

The north orbital pole of a revolving body is defined by the right-hand rule. If the fingers of the right hand are curved along the direction of orbital motion, with the thumb extended and oriented to be parallel to the orbital axis, then the direction the thumb points is defined to be the orbital north.

The poles of Earth's orbit are referred to as the ecliptic poles. For the remaining planets, the orbital pole in ecliptic coordinates is given by the longitude of the ascending node (☊) and inclination (i): l = ☊ - 90°, b = 90° - i.

Object [1]	☊ [2]	i	l	b	RA	Dec [3]	Constellation [4]
Mercury	48.331°	7.005°	318.331°	82.995°	18 h 43 m 57.1 s	+61° 26′ 53″	Draco
Venus	76.680°	3.39458°	346.680°	86.60542°	18 h 32 m 1.8 s	+65° 34′ 2″
Earth[5]	348.73936°	0.00005°	258.73936°	89.99995°	17 h 59 m 59.994 s	+66° 33′ 38.83″
Mars	49.558°	1.850°	319.558°	88.150°	18 h 13 m 29.7 s	+65° 19′ 22″
Jupiter	100.464°	1.303°	10.464°	88.697°	06 h 12 m 59.8 s	+66° 45′ 51″	Camelopardalis
Saturn	113.665°	2.485°	23.665°	87.515°	06 h 23 m 46.5 s	+67° 26′ 59″
Uranus	74.006°	0.773°	344.006°	89.227°	18 h 7 m 24.4 s	+66° 20′ 13″	Draco
Neptune	131.784°	1.768°	41.784°	88.232°	06 h 13 m 54.3 s	+67° 42′ 7″	Camelopardalis

The orbital poles for Jupiter, Saturn and Neptune in the above table and on the image above right are definitely very wrong as they show an almost 45° distance from the ecliptic pole. The orbital poles of all the planets are very close to each other, all within 2.2°of the solar system invariable plane except for Mercury at 6.34°.

Ecliptic pole

The ecliptic is the plane on which Earth orbits the Sun. The ecliptic poles are the two points where the ecliptic axis, the imaginary line perpendicular to the ecliptic, intersects the celestial sphere.

The two ecliptic poles are mapped below.

The north ecliptic pole is in Draco.

The south ecliptic pole is in Dorado.

Due to axial precession, either celestial pole completes a circuit around the nearer ecliptic pole every 25,800 years.

As of 1 January 2000, the positions of the ecliptic poles expressed in equatorial coordinates, as a consequence of Earth's axial tilt, are the following:

• North: right ascension  18^h 0^m 0.0^s (exact), declination +66° 33′ 38.55″
• South: right ascension  6^h 0^m 0.0^s (exact), declination −66° 33′ 38.55″

It is impossible anywhere for either ecliptic pole to be at the zenith in the night sky. By definition, the ecliptic poles are located 90° from the Sun's position. Therefore, whenever and wherever either ecliptic pole is directly overhead, the Sun must be on the horizon. The ecliptic poles can contact the zenith only within the Arctic and Antarctic circles.

The galactic coordinates of the North ecliptic pole can be calculated as l = 96.38°, b = 29.81° (see Celestial coordinate system).

See also

• Celestial pole
• Polar alignment
• Pole star
• Poles of astronomical bodies

References

1. Orbital elements taken from the respective Wikipedia article.
2. Epoch J2000.0
3. Converted from l, b using Les Coleman, Frosty Drew Observatory & Sky Theatre: Tools: Equatorial and Ecliptic Coordinates
4. Moews, David (2008); Finding the constellation which contains given sky coordinates
5. This row comes from the "mean orbital elements" at J2000 given in Williams, David R. (16 March 2017). "Earth Fact Sheet". NASA/Goddard Space Flight Center. Retrieved 26 July 2018. For "orbital parameters" it gives an inclination of zero (corresponding to the definition of the ecliptic).