Orbital node
An orbital node is one of the two points where an orbit crosses a plane of reference to which it is inclined. An orbit that is contained in the plane of reference (called non-inclined) has no nodes.
Planes of reference
Common planes of reference include:
For a geocentric orbit, the Earth's equatorial plane. In this case, non-inclined orbits are called equatorial.
For a heliocentric orbit, the ecliptic. In this case, non-inclined orbits are called ecliptic.
For an orbit outside the Solar System, the plane through the primary perpendicular to a line through the observer and the primary (called the plane of the sky)., chap. 17.
Node distinction
If a reference direction from one side of the plane of reference to the other is defined, the two nodes can be distinguished. For geocentric and heliocentric orbits, the ascending node (or north node) is where the orbiting object moves north through the plane of reference, and the descending node (or south node) is where it moves south through the plane. In the case of objects outside the Solar System, the ascending node is the node where the orbiting secondary passes away from the observer, and the descending node is the node where it moves towards the observer., p. 137.
