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Reference · Astronomy

What are the lunar nodes, and why do eclipses happen there?

Kevin Blaxton — software builder; astrology student for 40+ years · figures computed by the OrbHeaven engine
Published · Last revised

The lunar nodes are the two points where the Moon’s orbit crosses the ecliptic — the Sun’s apparent path. They are not bodies; nothing is there. They matter in astronomy because eclipses can only happen when a New or Full Moon falls near a node, and in astrology because the tradition reads them as an axis of growth and release.

The “diamond ring” of a total solar eclipse: the Sun almost fully covered by the dark disc of the Moon, with one brilliant point of sunlight blazing at the edge.
The diamond ring of the 2017 total solar eclipse. A solar eclipse can happen only at a New Moon that falls near a lunar node — where the Moon’s tilted orbit crosses the Sun’s path.

Source: NASA/Aubrey Gemignani · natural colour · U.S. public domain (courtesy NASA; no endorsement implied).

How to read this article:Established scienceHistorical scholarshipAstrological traditionOrbHeaven computation
Established science

What are the lunar nodes?

The Moon’s orbit is tilted about 5° to the ecliptic, so for half of each month the Moon is above the Sun’s path and for half below. The two points where it crosses are the nodes: the ascending (North) node, where it crosses going north, and the descending (South) node, directly opposite. They are always exactly 180° apart.

They are points, not objects — there is nothing physically at a node. Because the Moon’s orbit itself slowly rotates, the nodes drift steadily backwards around the zodiac, completing a circuit in about 18.6 years.

the ecliptic (Sun’s path)the Moon’s orbit (tilted ~5°, exaggerated)Earth☊ North (ascending) node☋ South (descending) nodeEclipses can happen only when a New or Full Moon falls near a node — nothing is there; they are points, not bodies
The Moon’s orbit, tilted about 5° to the ecliptic (exaggerated here), crosses it at two opposite points — the North and South nodes. Nothing is there; they are the crossings, not bodies.
OrbHeaven computation

Mean node and true node

The Moon’s orbit wobbles, so the nodes can be given two ways. The true node is the exact, instantaneous crossing point, which drifts backwards but briefly jitters forwards; the mean node is that motion averaged into a smooth, always-backward drift. They differ by up to about 1.5°.

OrbHeaven uses the mean node — the older convention — and says so. Neither is more “correct”; they answer slightly different questions, and the difference is small enough that it rarely changes a sign.

Established science

The nodes and eclipses

Most New Moons pass above or below the Sun, and most Full Moons above or below the Earth’s shadow, because of that 5° tilt. Only when a New Moon or Full Moon happens near a node do the three bodies line up closely enough for an eclipse — a solar eclipse at the New Moon, a lunar eclipse at the Full.

This is why eclipses come in seasons about six months apart, when the Sun is near the node axis. OrbHeaven does not compute or predict eclipses; it locates the nodes and the lunations, and this page explains the geometry rather than forecasting any particular eclipse.

A composite of a total lunar eclipse: the Moon in several phases across the frame, deep coppery red at totality — the “blood moon”.
A total lunar eclipse (a composite of eleven images, March 2025). A lunar eclipse can happen only at a Full Moon near a lunar node, when the Earth’s shadow falls on the Moon.

Source: NASA/GRC/Jordan Cochran · composite · U.S. public domain (courtesy NASA; no endorsement implied).

Historical scholarship

Rahu, Ketu, and the dragon

The nodes are old and were vivid long before their geometry was understood. In Indian astrology they are Rahu (north) and Ketu (south), treated almost as shadow-planets; in the medieval West they were the dragon’s head and tail — caput and cauda draconis — the creature imagined to swallow the Sun at an eclipse.

Predicting where the nodes would be, and so when eclipses could occur, drove some of the oldest exact astronomy: the Babylonian Saros cycle of about 18 years already let eclipses be anticipated thousands of years ago.

Astrological tradition

What the nodes are read as

Interpretation, labelled as such: the tradition reads the North Node as a direction of growth — the unfamiliar thing worth reaching for — and the South Node as what already comes easily and can be leaned on less. They are an axis, always read as a pair.

Where this is disputed

Whether the nodes are a karmic axis, how much weight they carry, and whether to use the mean or true node, all vary by astrologer. The geometry and the eclipse conditions are exact and the same for everyone; the meaning is a tradition, and we keep the two apart.

Common misconceptions

Are the lunar nodes planets or stars?
Neither. They are the two points where the Moon’s orbit crosses the ecliptic — geometry, not objects. Nothing is physically there.
Why isn’t there an eclipse at every New and Full Moon?
Because the Moon’s orbit is tilted ~5°, so most New and Full Moons pass above or below the alignment. An eclipse needs a lunation near a node.
Does OrbHeaven predict eclipses?
No. It locates the nodes and the lunations and explains the geometry; it does not compute or forecast specific eclipses.

References & further reading

  1. [1] NASA — solar and lunar eclipses: geometry, types, and why they occur in seasons.
  2. [2] Meeus, J., Astronomical Algorithms, 2nd ed. (Willmann-Bell, 1998) — the lunar nodes, mean vs true, and eclipse conditions.
  3. [3] Neugebauer, O., A History of Ancient Mathematical Astronomy — the Saros and ancient eclipse prediction.

Suggested citation

Blaxton, K. (2026). What are the lunar nodes, and why do eclipses happen there. OrbHeaven Reference. https://orbheaven.com/reference/the-lunar-nodes

Revision history

  • First build. Original node-geometry diagram (Moon’s orbit crossing the ecliptic); NASA imagery — the 2017 total solar eclipse (NASA/Aubrey Gemignani) and a 2025 total lunar eclipse composite (NASA/GRC/Jordan Cochran), both U.S. public domain. OrbHeaven uses the mean node. No eclipse computation or prediction (decision G6); no interactive.

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