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The north orbital poles of the Solar System planets all lie within Draco. The central yellow dot represents the Sun's north pole. 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
[a]140°
0.0001°
[a]50°
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 a 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]
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^"HST cycle 26 primer orbital constraints". HST User Documentation. hst-docs.stsci.edu. Retrieved 2022-07-16.
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