Back قطبا دائرة الكسوف Arabic Pól ekliptiky Czech Polo de la eclíptica Spanish Pôle de l'écliptique French Ekliptisk pol NB Pòl de l'ecliptica Occitan Polo orbital Portuguese Pol ecliptic Romanian Полюс эклиптики Russian Pól ekliptiky Slovak

Orbital pole

The north orbital poles of the Solar System major planets all lie within Draco.[1] The central yellow dot represents the Sun's rotation axis north pole.[citation needed] Jupiter's north orbital pole is colored orange, Mercury's pale blue, Venus's green, Earth's blue, Mars's red, Saturn's magenta, Uranus's grey, and Neptune's lavender. That of the dwarf planet Pluto is shown as the dotless cross off in Cepheus.

An orbital pole is either point at the ends of the orbital normal, an imaginary line segment that runs through a focus of an orbit (of a revolving body like a planet, moon or satellite) and is perpendicular (or normal) 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 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 . In the following table, the planetary orbit poles are given in both celestial coordinates and the ecliptic coordinates for the Earth.

Object ☊[1] i[1] Ecl.Lon. Ecl.Lat. RA (α) Dec (δ)
Mercury 48.331° 7.005° 318.331° 82.995° 18h 43m 57.1s +61° 26′ 52″
Venus 76.678° 3.395° 346.678° 86.605° 18h 32m 01.8s +65° 34′ 01″
Earth 140°[a] 0.0001° 50°[a] 89.9999° 18h 00m 00.0s +66° 33′ 38.84″
Mars 49.562° 1.850° 319.562° 88.150° 18h 13m 29.7s +65° 19′ 22″
Ceres 80.494° 10.583° 350.494° 79.417° 19h 33m 33.1s +62° 50′ 57″
Jupiter 100.492° 1.305° 10.492° 88.695° 18h 13m 00.8s +66° 45′ 53″
Saturn 113.643° 2.485° 23.643° 87.515° 18h 23m 46.8s +67° 26′ 55″
Uranus 73.989° 0.773° 343.989° 89.227° 18h 07m 24.1s +66° 20′ 12″
Neptune 131.794° 1.768° 41.794° 88.232° 18h 13m 54.1s +67° 42′ 08″
Pluto 110.287° 17.151° 20.287° 72.849° 20h 56m 3.7s +66° 32′ 31″

When an artificial satellite orbits close to another large body, it can only maintain continuous observations in areas near its orbital poles. The continuous viewing zone (CVZ) of the Hubble Space Telescope lies inside roughly 24° of Hubble's orbital poles, which precess around the Earth's axis every 56 days.[2]

  1. ^ a b c Cite error: The named reference jpl horizons web was invoked but never defined (see the help page).
  2. ^ Cite error: The named reference STScI-primer was invoked but never defined (see the help page).


Cite error: There are <ref group=lower-alpha> tags or {{efn}} templates on this page, but the references will not show without a {{reflist|group=lower-alpha}} template or {{notelist}} template (see the help page).

Developed by StudentB