Lunar standstill

A lunar standstill is a period when the Moon’s monthly north–south range in the sky reaches either a maximum (major standstill) or a minimum (minor standstill). The cycle repeats about every 18.6 years as the orientation of the Moon’s inclined orbital plane changes. During a major standstill, the Moon can rise and set at unusually far-north and far-south points on the horizon; the extreme pattern is observable for roughly two years.

Last updated
7 November 2026
Confidence
Moderate (80%)
Sources
2
Versions
1
This article was researched and drafted with AI assistance and checked by an automated review pass. It is not guaranteed to be accurate — verify important facts against the references below.

What happens during a standstill

The Moon’s rising and setting points shift along the horizon over the course of its monthly cycle. Their northern and southern limits also change from month to month. Near a major lunar standstill, these limits approach their furthest positions; near a minor standstill, the monthly range is more restricted. “Standstill” does not mean that the Moon stops moving. Rather, its extreme limits change so slowly around the peak that the pattern persists over an extended interval.

The 18.6-year cycle

The Moon’s orbit is inclined by about five degrees to the plane of Earth’s orbit around the Sun. The Sun’s gravitational influence causes the orientation of the lunar orbital plane to turn over time. The resulting cycle takes about 18.6 years. When the orbital tilt and the tilt of Earth’s equator relative to the ecliptic combine in the same direction, the Moon reaches its greatest apparent north–south excursions, producing a major standstill. When they partly offset one another, the range is smaller and a minor standstill occurs.

Observing a major standstill

A major standstill can be followed by comparing where the Moon rises or sets on successive dates, especially near its monthly extreme positions. The Moon’s horizon position moves rapidly back and forth through the month, even while the standstill’s overall limits change little. The full Moon can make a striking observation when it rises or sets near those limits, but the exact direction and altitude depend on the observer’s location and the horizon. Unlike an eclipse, a lunar standstill is not confined to a narrow viewing path; the Moon’s extreme horizon positions can be observed from different places on Earth.

Standstills and archaeological interpretation

The long lunar cycle has been proposed as a possible subject of alignments or imagery at some archaeological sites. Such interpretations require care: a structure aligned with a lunar extreme does not by itself prove that its builders intended to track the 18.6-year cycle. The High Altitude Observatory at the National Center for Atmospheric Research describes proposed interpretations at Mesa Verde and other sites as plausible conjectures and notes that alternative explanations exist.

Key facts

Cycle length
About 18.6 years
Major standstill
The Moon’s rising and setting limits reach their widest north–south range
Minor standstill
The Moon’s rising and setting limits reach a comparatively narrow range
Does the Moon stop moving?
No. The term describes the slowly changing extreme limits, not a halt in the Moon’s motion

Ask about this article

Answers use only “Lunar standstill” and its references, with citations.

References

  1. 1.
    Extreme Moon: The Major Lunar Standstill of 2024–2025

    Griffith Observatory, City of Los Angeles · other · reliability: unverified · retrieved 7 November 2026

  2. 2.
    Lunar Astronomy

    High Altitude Observatory, National Center for Atmospheric Research · other · reliability: unverified · retrieved 7 November 2026

References are suggested by the research engine and may be incomplete. Unverified URLs are omitted rather than guessed.

Article history

  1. Version 17 November 2026 · EditorCreated by Zapia